12 Jan

Artificial Intelligence/Machine Learning Applications at SLAC National Accelerator Laboratory

12 January 2024 - 3:00 PM
Online via Zoom
SLAC National Accelerator Laboratory

Daniel Fried Ratner

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Across the DOE, the wealth of data, robust automation, and stringent requirements for control, simulation, and data acquisition, make "Big Science" experiments - telescopes, particle accelerators, etc. - ideal targets for AI/ML. At the same time, the flavor of AI/ML techniques differ from those found in industry. In this talk, I will show some example AI projects at SLAC, including autonomous optimization of an x-ray laser, anomaly detection for a particle accelerator, and single-particle imaging of biomolecules (an example of an inverse problem). I will also highlight how these same methods can find use in other science domains.
19 Jan

Study of Zinc-60 for the Astrophysical Rapid Proton Process

19 January 2024 - 10:00 AM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Gerard Jordan Owens-Fryer

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Committee: Artemis Spyrou (Chairperson), Paul Gueye, Heiko Hergert, Wade Fisher, Wolfgang Kerzendorf
19 Jan

Laboratory for Underground Nuclear Astrophysics: Present and Future of Nuclear Astrophysics at Laboratori Nazionali del Gran Sasso

19 January 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
LNGS

Federico Ferraro

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The LUNA (Laboratory for Underground Nuclear Astrophysics) experiment is located at the LNGS (Laboratori Nazionali del Gran Sasso) in Italy. LUNA is aimed at studying the nuclear reactions that are responsible for the synthesis of the elements and shape the life of stars in the universe. The reduction of the cosmic-rays induced background provided by the 1400 m thick rock overburden at LNGS allows the direct measurement of the cross section in the energy range relevant to astrophysics. The LUNA-400 accelerator is in operation since 2001 and is able to produce H+ and He+ beams using a terminal voltage as high as 400 kV with beam currents up to a few hundreds of microampere. It was mainly focused on reactions relevant to solar physics and hydrogen burning. The new LUNA-MV accelerator has been recently commissioned. It will provide ion beams of H+, He+, C+ and C++ using a terminal voltage as high as 3.5 MV with comparable beam currents. It will allow the study of nuclear reactions involved in more advanced phases of stellar evolution, responsible for the synthesis of heavy elements. This seminar will provide an overview of the LUNA experiment, with a focus on the experimental program at the LUNA-MV accelerator, that is part of the new Bellotti Ion Beam Facility of the LNGS.
21 Jan

Advanced Studies Gateway Event

21 January 2024 - 1:00 PM
Online via Zoom
Massachusetts Institute of Technology, Harvard Medical School, and Massachusetts General Hospital

Emery Brown

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"General anesthesia is a drug-induced, reversible condition comprised of five behavioral states: unconsciousness, amnesia (loss of memory), antinociception (loss of pain sensation), akinesia (immobility), and hemodynamic stability with control of the stress response. Our work shows that a primary mechanism through which anesthetics create these altered states of arousal is by initiating and maintaining highly structured oscillations. These oscillations impair communication among brain regions. We illustrate this effect by presenting findings from our human and non-human primate studies using high-density EEG recordings and intracranial recordings. These studies have allowed us to give a detailed characterization of the neurophysiology of loss and recovery of consciousness due to propofol, and more recently ketamine. We show how these dynamics change systematically with different anesthetic classes and with age. As a consequence, we have developed a principled, neuroscience-based paradigm for using the EEG to monitor the brain states of patients receiving general anesthesia. We demonstrate that the state of general anesthesia can be rapidly reversed by activating specific brain circuits. Finally, we demonstrate that the state of general anesthesia can be controlled using closed-loop feedback control systems. The success of our research has depended critically on tight coupling of experiments, signal processing research and mathematical modeling."
23 Jan

Probing the Heart of Matter with Supercomputers

23 January 2024 - 4:00 PM
1200 FRIB Laboratory and Online via Zoom
Michigan State University

Huey-Wen Lin

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Nucleons are the building blocks of all ordinary matter, and the study of nucleon structure is a critical part of frontier research to unveil the mysteries of the universe and our existence. Gluons and quarks are the underlying degrees of freedom that explain the properties of nucleons, and fully understanding how they contribute to the properties of nucleons (such as mass or spin structure) helps to decode the last part of the Standard Model that rules our physical world. After more than half a century of large-scale experimental efforts, there are still many unknowns concerning the theory quantum chromodynamics (QCD), the branch of the Standard Model describing how gluons strongly interact with themselves and with quarks, binding both nucleons and nuclei. Using supercomputers and a theoretical tool called "lattice QCD", we can simulate the theory that dominates the universe at the femtoscale and unveil its diverse phenomenology, including some properties that are hard to determine in experiments. A few recent lattice-QCD examples and their impacts will be briefly discussed.
26 Jan

Advancing SRF Cryomodules Performance for Modern Particle Accelerators

26 January 2024 - 3:00 PM
Online via Zoom
Fermi National Accelerator Laboratory

Donato Passarelli

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Superconducting Radio Frequency (SRF) technology plays a key role in modern particle accelerators. Starting from an overview on main accelerator types and SRF cryomodule structures, we then delve into the detailed design and development approaches employed for the PIP-II SRF LINAC, an ongoing major upgrade of the Fermilab accelerator complex. Specifically, the presentation focuses on the engineering approaches and innovative solutions that are playing a fundamental role in shaping the future of particle accelerator technology.
02 Feb

The Abundances of the Elements in Stars: 3D Non-Local Thermodynamic Equilibrium Modelling

02 February 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
Uppsala University

Anish Amarsi

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The chemical compositions of stars place key constraints on nuclear astrophysics. The most precise way of determining these compositions is through analyses of the absorption lines in the observed star light (stellar spectroscopy). However, the accuracy of standard analyses of Sun-like stars can be limited by simplifying assumptions: in particular, that the atmosphere of the star is one-dimensional (1D), hydrostatic, and satisfies local thermodynamic equilibrium (LTE). In recent years it has become feasible to relax these assumptions via non-LTE post-processing of three-dimensional (3D) radiation-hydrodynamics simulations. I shall describe this approach, and then present examples where this approach has altered our understanding of the evolution of the elements in the cosmos.
06 Feb

A Review of the Isotopic Dichotomy of the Solar System

06 February 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
Michigan State University

Seth Jacobson

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In the last decade, a startingly discovery has reshaped our understanding of solar system materials. They appear to be sorted into two distinct nucleosynthetic isotopic compositions across a large range of elements (O, Cr, Mo, Ti, Ru, Ni, etc.). One reservoir is associated with inner solar system materials including both primitive ordinary and enstatite chondrites as well as differentiated bodies such as the Moon, Mars, Earth, some iron meteorites and other achondrites. The other reservoir is associated with the carbonaceous chondrites, often believed to originate from the outer solar system (beyond Jupiter). One of the first consequences of the dichotomy was the identification of achondrites including iron meteorites that share the nucleosynthetic anomalies of the carbonaceous chondrites. The nucleosynthetic variations as measured in the Mo system appear to indicate an enrichment of r-process nuclides in the inner solar system materials relative to the outer solar system. The presence of this dichotomy has deep implications for the early history of the Solar System including a possible rapid formation of Jupiter that prevented the inward migration of r-process depleted material (i.e., spatial heterogeneity). Alternatively, thermal processing of pre-solar grains could have created an r-process enriched inner reservoir establishing a temporal heterogeneity between early and late accreting objects. These ideas will be tested using new models of solar system formation that combine astrophysics and geochemistry.
06 Feb

High-Efficiency and Reliable Wide Range Operation of 2 K Helium Cryogenic Systems

06 February 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
Michigan State University

Jonathon Howard

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Operation of helium cryogenic systems below the normal boiling point of helium (approximately 4.2 K) has become a common need for modern high-energy particle accelerators. Cooling near 2 K, ranging from approximately 1.8 to 2.1 K (or a saturation pressure of 16 to 40 mbar), is often required by superconducting radio-frequency (SRF) niobium resonators (also known as SRF cavities) to achieve the performance targets of the particle accelerator. To reach these temperatures, cryogenic systems evacuate, or ‘pump-down’, a liquid helium bath to sub-atmospheric pressures, thereby lowering the boiling temperature below 4.2 K. Multi-stage cryogenic centrifugal compressors (‘cold-compressors’) have been proven to be an efficient, reliable, and cost-effective method to achieve operating conditions of around 2 K for large-scale cryogenic systems. These compressors re-pressurize the sub-atmospheric helium to just above atmospheric conditions before injecting the flow back into the helium refrigerator. Although multi-stage cryogenic centrifugal compressor technology has been implemented in large-scale cryogenic systems since the late 1980’s, published research on their operation (steady-state and transient) is inadequate to provide a general characterization of the compressor performance, efficiency, and stability. The focus of this dissertation is two-fold regarding multi-stage centrifugal compressors as used for sub-atmospheric helium cryogenic systems. First, to develop a reliable performance prediction model for a multi-stage cryogenic centrifugal compressor train and validate with measurements from an actual operating system. Capabilities of the model include estimation of operational envelops that ensure stable and wide range steady-state operation. Second, to develop and validate a process model of the entire sub-atmospheric system (e.g. FRIB) being studied and establish a simple methodology to obtain a reliable thermodynamic path for the transient (‘pump-down’) process of reducing the helium bath pressure from above 1 bar to the operational steady-state conditions near 30 mbar. The effectiveness of the developed methodology is demonstrated by comparing the estimated and measured process parameters from the sub-atmospheric system studied. The developed model and methodology are intended to benefit the design and operation (both steady-state and transient) of multi-stage cryogenic centrifugal compressor used in large-scale cryogenic helium refrigeration systems.
07 Feb

Fundamental Physics in Heavy Nuclei: The Role of Nuclear-Structure Theory

07 February 2024 - 4:10 PM
1300 FRIB Laboratory
University of North Carolina

Jonathan Engel

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Low energy experiments play an increasingly large role in the search for physics beyond the Standard Model. Many experiments in that area involve heavy nuclei, where an understanding of nuclear structure at the level needed to interpret results is both crucial and hard to come by. After describing the fundamental physics we seek to better understand, I examine recent theoretical work on two sets of nuclear matrix elements --- those important for experiments on neutrinoless double-beta and on atomic electric dipole moments --- and discuss projects that may lead to major improvements in the matrix elements in the next few years.
09 Feb

Beam-Beam Effects in Future Electron-Ion Collider

09 February 2024 - 3:00 PM
Online via Zoom
Brookhaven National Laboratory

Yun Luo

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The Electron-Ion Collider (EIC), to be constructed at Brookhaven National Laboratory, will collide polarized high-energy electron beams with hadron beams, achieving luminosities up to 10^34 cm^-2s^-1 in the center-mass energy range of 20-140 GeV. To attain such high luminosity, we adopt high bunch intensities for both beams, employ flat beams at the interaction point, and implement a crossing angle collision with crab cavities in both rings. Beam-beam interaction poses a significant challenge in the design of the EIC. In this talk, the speaker will first introduce the basics of beam-beam interaction in circular colliders and the ongoing Electron-Ion Collider project. The speaker will then present the optimization of beam-beam related design parameters, selected simulation results, optics and machine imperfections, and the impacts of noises on beam-beam performances.
14 Feb

On the Importance of Complementary Observables:
Proton Cross-Shell Excitations in Neutron-Deficient Calcium Isotopes

14 February 2024 - 4:10 PM
1300 FRIB Laboratory
FRIB

Tobias Beck

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The neutron-deficient calcium isotopes have attracted considerable attention recently. Present studies are divided over the amount of proton pf-shell occupancy, ranging from an intact Z=20 shell closure to a considerable weakening already in the vicinity of doubly-magic 40Ca. Coulomb excitation of 36,38Ca and two-neutron removal from 38Ca populating states of 36Ca were performed at the National Superconducting Cyclotron Laboratory. The results yield conclusive evidence for the need of sizable proton cross-shell excitations already for the ground state of 36Ca. These findings furthermore enable a close reproduction of additional observables. Ultimately, the magnitude of proton cross-shell excitations is explored by means of a schematic modification of the sd-pf shell gap.
15 Feb

High-Efficiency and Reliable Wide Range Operation of 2 K Helium Cryogenic Systems

15 February 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
Michigan State University

Jonathon Howard

Show/Hide Abstract
Operation of helium cryogenic systems below the normal boiling point of helium (approximately 4.2 K) has become a common need for modern high-energy particle accelerators. Cooling near 2 K, ranging from approximately 1.8 to 2.1 K (or a saturation pressure of 16 to 40 mbar), is often required by superconducting radio-frequency (SRF) niobium resonators (also known as SRF cavities) to achieve the performance targets of the particle accelerator. To reach these temperatures, cryogenic systems evacuate, or pump-down a liquid helium bath to sub-atmospheric pressures, thereby lowering the boiling temperature below 4.2 K. Multi-stage cryogenic centrifugal compressors (cold-compressor) have been proven to be an efficient, reliable, and cost-effective method to achieve operating conditions of around 2 K for large-scale cryogenic systems. These compressors re-pressurize the sub-atmospheric helium to just above atmospheric conditions before injecting the flow back into the helium refrigerator. Although multi-stage cryogenic centrifugal compressor technology has been implemented in large-scale cryogenic systems since the late 1980s, published research on their operation (steady-state and transient) is inadequate to provide a general characterization of the compressor performance, efficiency, and stability. The focus of this dissertation is two-fold regarding multi-stage centrifugal compressors as used for sub-atmospheric helium cryogenic systems. First, to develop a reliable performance prediction model for a multi-stage cryogenic centrifugal compressor train and validate with measurements from an actual operating system. Capabilities of the model include estimation of operational envelops that ensure stable and wide range steady-state operation. Second, to develop and validate a process model of the entire sub-atmospheric system (e.g. FRIB) being studied and establish a simple methodology to obtain a reliable thermodynamic path for the transient (pump-down) process of reducing the helium bath pressure from above 1 bar to the operational steady-state conditions near 30 mbar. The effectiveness of the developed methodology is demonstrated by comparing the estimated and measured process parameters from the sub-atmospheric system studied. The developed model and methodology are intended to benefit the design and operation (both steady-state and transient) of multi-stage cryogenic centrifugal compressor used in large-scale cryogenic helium refrigeration systems.
20 Feb

Fusion Reaction in Collisions of Weakly Bound Nuclei with Heavy Targets

20 February 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
Facultdade de Tecnologia Universidade do Estado do Rio de Janeiro

Jeannie Rangel

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Collisions of weakly bound projectiles have attracted great interest over the last few decades. The low breakup threshold of the projectile plays an important role in the reaction dynamics, affecting strongly the fusion channel. Besides the ordinary fusion process, where the whole projectile fuses with the target (CF), there is the so-called incomplete fusion (ICF) which one fragment is captured while the other survives the collision. Most experiments can only determine the total fusion cross section (TF), which is the sum of the cross sections for the CF and ICF processes. To make predictions for the CF and ICF cross-sections is also a great challenge to theorists, and several attempts have been made. Many of them are based on classical or semiclassical methods, which cannot properly handle important quantum mechanical effects. This problem is avoided in some quantum mechanical models based on the continuum discretized coupled channel (CDCC) method. However, some of them can only determine the TF cross-section, some can give individual CF and ICF cross-sections but are not valid when the projectile breaks up into fragments of comparable masses. There is also a method that provides the CF cross-section but cannot determine ICF. In this seminar, I will present a new quantum mechanical method to evaluate individual CF and ICF cross-sections. This method can be used for any weakly bound projectile and, in addition, it distinguishes the direct and sequential contributions to the CF cross-section. A few applications will be presented.
22 Feb

Parallel-Plate Avalanche Counters (PPACs) for Heavy-Ion Beam Tracking: History and Mysteries

22 February 2024 - 11:00 AM
1200 FRIB Laboratory
FRIB Michigan State University

Salvatore Di Carlo

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Despite being an old detector concept, position-sensitive Parallel-Plate Avalanche Counters (PPACs) remain widely used today for heavy-ion position and timing measurements. In modern rare isotope beam facilities and large-acceptance fragment separators, PPACs are used to characterize beam properties (diagnostics), facilitate beam delivery (tuning), and provide event-by-event beam tracking for particle identification (PID). Most popular particle localization methods in PPAC detectors are based on strip electrodes electrically connected to resistive-chain circuits or delay-lines. More exotic systems include optical readouts based on recording electroluminescence light with high-granularity photodetector arrays, or high-resolution resistive anode electrodes. PPACs with conventional resistive-chain or delay-line readouts achieve typical position and time resolutions of below 1 mm (σ) and around 150 ps (σ) respectively. In addition, delay-line systems are capable of counting rates above several hundred kHz for beam areas of a few millimeters square, and around 1 MHz for larger beam sizes. Resistive-chain readouts have limited rates of a few tens of kHz. A review of the operation principles and performance of PPAC detectors is presented in this paper. We will discuss decades-long experience building and operating PPACs developed at the National Superconducting Cyclotron Laboratory (NSCL), and then refined at the Facility for Rare Isotope Beams (FRIB), mostly focusing on the delay-line readout technique (DLPPAC). We will also discuss problems that arise due to electric discharges at high rates, and briefly describe ongoing developments at FRIB.
23 Feb

Electron Synchrotron for Electron Ion Collider

23 February 2024 - 3:00 PM
Online via Zoom
Brookhaven National Laboratory

Vahid H. Ranjbar

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"Two new Electron Synchrotron's will be built for the Electron Ion Collider (EIC). These include the Rapid Cycling Synchrotron (RCS) which is used for injection into the Electron Storage Ring (ESR). Both machines will transport and store polarized electrons at energies as high as 18 GeV and be built in the existing RHIC tunnel. We will review the physic requirements and novel design of these machines, focusing on the RCS."
29 Feb

Ion Accelerator Applications, Compact RF Linear Architectures and Machine Learning for Real Time Tuning and Optimization

29 February 2024 - 4:00 PM
1221A and 1221B FRIB Laboratory
FRIB Graduate Research Assistant

Nicholas Anthony Valverde

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Committee: Steven Lund (Chairperson), Yue Hao Dean Lee, Steven Lidia, Chong-Yu Ruan. Thesis is available at https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - select student
01 Mar

Measurement of the Uranium-235(n,f) Cross Section Relative to n-p Scattering Up to 500 MeV at the Neutron Time-of-Flight Facility at CERN

01 March 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
CERN

Alice Manna

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Neutron-induced fission reactions play a key role in the nucleosynthesis of heavy elements. The description of fission recycling during r-process nucleosynthesis, relies on model predictions of fission reactions. To this end, various models are used in literature for calculating the fission rates and the mass distribution of fission fragments for a number of heavy and highly unstable actinides. In order to provide a reliable description of reaction rates for Th, U and heavier actinides, current efforts are underway for refining models with a comprehensive and self-consistent description of the fission process. In this respect, new fission data on a variety of actinides are needed, as the predictive power of current models can only by improved by comparison with a large set of experimental results. The 235U(n,f) cross section is one of the most important neutron cross-section standards, and therefore it is recognized as a convenient reference for other reaction cross-section measurements at thermal energy and between 0.15 MeV and 200 MeV. Outside these energy ranges the cross section is either not so well known or not measured yet, as for example above 200 MeV, where evaluations can only rely on theoretical calculations. With the continuous effort for the improvement of standard cross sections by the International Atomic Energy Agency (IAEA) together with nuclear data evaluators teams, the longstanding quest for accurate and reliable 235U(n,f) cross section data turns out to be still pending, for neutron energies above 20 MeV (only 2 data sets are present in the 20-200 MeV energy region). In particular, fission measurements relative to the neutron-proton elastic scattering, which is considered the primary reference for neutron cross section measurements, are still highly requested. The neutron time-of-flight facility, n_TOF, at CERN, offers the possibility to study neutron-induced reactions thanks to the extremely wide neutron energy spectrum available in its experimental area, from thermal up to 1 GeV. In the recent years, dedicated measurement campaigns were carried out to provide accurate and precise cross section data of the 235U(n,f) reaction, in a low energy region, up to 10 MeV, as well as in the high energy region from 10 MeV to 500 MeV. The experimental apparatus used in the measurements at high neutron energies, which involved the efforts of several research institutions (INFN, PTB and IPN, in addition to CERN), consisted of three flux and two fission detectors, allowing to simultaneously record the number of neutrons impinging on the 235U samples (incident neutron flux), as well as fission events, as a function of the neutron energy. The neutron flux measurement is based on the neutron-proton elastic scattering reaction, and it exploits the detection of the recoil protons from the n-p reaction in a polyethylene target using three Proton Recoil Telescopes. The fission events have been recorded with a fission ionization chamber, as well as by a parallel plates avalanche counters (PPAC) detector, specifically designed for operation at n_TOF. The experimental apparatus and data analysis will be presented, with a focus on the results obtained in the high-energy region, above 200 MeV. A comparison with current model descriptions of the fission process at high neutron energies will be included in the comparison with the experimental results obtained at n_TOF.
07 Mar

Ab Initio Description of Monopole Resonances in Light and Medium Mass Nuclei

07 March 2024 - 2:00 PM
1200 FRIB Laboratory
Technische Universitat Darmstadt

Andrea Porro

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Giant monopole resonances have a long-standing theoretical importance in nuclear structure. The interest resides notably in the so-called breathing mode that has been established as a standard observable to constrain the nuclear incompressibility. The Random Phase Approximation (RPA) within the frame of phenomenological Energy Density Functionals (EDF) has become the standard tool to address giant resonances and extensive studies, have been performed throughout the years. A proper study of collective excitations within the ab initio framework is, however, missing. Additionally, the ab initio many-body methods developed over the past two decades encounter limitations when it comes to dealing with excited-state properties. In this perspective, I will present the first systematic ab initio predictions of (giant) monopole resonances. Ab initio Quasiparticle-RPA (QRPA) and Projected Generator Coordinate Method (PGCM) calculations of monopole resonances are compared in light- and mid-mass closed- and open- shell nuclei. Monopole resonances represent the starting point for exploring higher multipolarities, the goal in the medium term being to establish PGCM and QRPA as complementary tools in the development of a fundamental theory of nuclear excitations.
08 Mar

Strong Hadron Cooling for the Electron-Ion Collider

08 March 2024 - 3:00 PM
Online via Zoom
Brookhaven National Laboratory

Erdong Wang

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The anticipated peak and average luminosity of L = 1034 cm-2s-1 at the Electron Ion Collider (EIC) can be attained with strong cooling of the hadron beam, as the emittance of the highly luminous beams is prone to rapid growth due to Intrabeam Scattering and other diffusion mechanisms. A novel cooling method, coherent electron cooling (CeC), has been considered as the baseline strong hadron cooling approach. CeC involves utilizing an electron beam to detect the positions of protons within the bunch and then applying energy kicks to reduce their longitudinal and transverse actions.

In this presentation, we will first introduce the heating mechanism and provide an overview of the basic principles of hadron cooling. Subsequently, we will delve into the underlying physics of the CeC process. We will then discuss the current progress in design. Finally, we will discuss the challenges encountered and outline mitigation strategies, emphasizing the importance of a high-quality electron beam, high current energy recovery Linac, and the precise sub-micron alignment of electrons and protons.
08 Mar

Three Beethoven Piano Sonatas, Op. 14 and 22

08 March 2024 - 5:30 PM
1300 FRIB Laboratory

Young Hyun Cho

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Young Hyun Cho: Three Beethoven Piano Sonatas, Op. 14 and 22 Young Hyun Cho's concert activities have taken her around the globe. She has performed as a soloist at venues such as the Great Hall (Golden Hall) of the Vienna Musikverein, Berlin Philharmonic Concert Hall, Smetana Hall in Prague, and Solti Hall of the Liszt Academy in Budapest. As a featured soloist, she has performed with the Berlin Symphony Orchestra, Euro Sinfonietta Wien, Filarmonica della Calabria of Italy, North Czech Philharmonic Orchestra Teplice, Korean Broadcasting System Symphony Orchestra, Korean Symphony Orchestra, and numerous other orchestras. She has also performed chamber concerts and solo recitals throughout North America, Asia, and Europe. She released her CD with the Last Three Beethoven Piano Sonatas under the Sony label. She received her Doctoral Arts of Musical degree from the Eastman School of Music, Master's degree and Graduate Performance Diploma from Peabody Conservatory, and Bachelor's degree from Seoul National University. Her primary teachers include Nelita True, Boris Slutsky and Mikyung Kim. Young Hyun Cho is currently an associate professor of piano at the Michigan State University College of Music and previously was a faculty member at the University of Texas at Arlington. Sonata No. 9 in E major, Op. 14, No. 1 Ludwig van Beethoven (1770-1827) Allegro Allegretto Rondo: Allegro comodo Sonata No. 10 in G major, Op. 14, No. 2 Allegro Andante Scherzo: Allegro assai Sonata No. 11 in B-flat major, Op. 22 Allegro con brio Adagio con molta espressione Minuetto Rondo: Allegretto
13 Mar

Measurement of the Isolated Nuclear Two-Photon Decay

13 March 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
IRFU, CEA, Universite Paris-Saclay

Wolfram Korten

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The nuclear two-photon or double-gamma (2y) decay is a second-order electromagnetic decay process whereby a nucleus in an excited state emits two gamma rays simultaneously. Compared to first-order decay pathways, such as single photon emission or internal conversion, the two-photon decay rate is very small. Ideal cases for this search are 0+ → 0+ transitions, where single photon emission is prohibited. However, the only cases where the 2y decay of a was successfully observed using γ-ray spectroscopy are 16O, 40Ca and 90Zr [1, 2], where the high energy of the transitions is favorable for the 2y branch. At lower energies the 2y branch becomes prohibitively small for y-ray spectroscopy (10-6-7). We have therefore combined the isochronous mode of a storage ring with Schottky resonant cavities to perform Schottky + Isochronous Mass Spectrometry (S+IMS) in order to study exotic decays of short-lived states at the Experimental Storage Ring at GSI. This novel technique allowed us to conduct the first measurement of the half-life for the isolated nuclear two-photon decay of the 0+ isomer in 72Ge [3]. The obtained mass resolving power enables future experiments on nuclear isomers with excitation energies down to ~100 keV and half-lives as short as ~10 ms.

15 Mar

The Other Side of Physics: Understanding, Awareness, and Support of Mental Health

15 March 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
Michigan State University

Rachel Younger

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As mental health initiatives are gaining momentum, aspects of mental health remain misunderstood and stigmatized. This presentation aims to provide understanding of the various mental health disorders that commonly impact individuals in STEM fields, their manifestations, factors that impact mental health, and strategies to support mental health wellbeing. Key topics to be discussed will also include intersectionality of mental health with other aspects of identity, and the importance of early intervention and support networks. This presentation aims to empower through knowledge, awareness, and strategies that support mental health wellbeing, encouraging a supportive and understanding community environment.
15 Mar

International Chamber Soloists

15 March 2024 - 6:00 PM
1300 FRIB Laboratory
Michigan State University, College of Music

Dmitri Berlinsky

18 Mar

Measuring the Oxygen-15(a, y) Neon-19 Reaction in Type I X-ray Bursts Using 20Mg B-decay

18 March 2024 - 3:00 PM
1200 FRIB Laboratory
FRIB Graduate Research Assistant

Tyler M. Wheeler

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Committee: Christopher Wrede (Physics Advisor), Saiprasad Ravishanker (CMSE Advisor), Edward Brown Paul Gueye, Darren Grant. Thesis is available at https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - select student
19 Mar

An Adiabatic Hyperspherical Approach to Few-Body Systems in the Nuclear Sector

19 March 2024 - 11:00 AM
1200 FRIB Laboratory
Purdue University

Michael Higgins

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An area of the few-body sector that provides a natural class of systems near the unitarity limit is low-energy nuclear physics. These systems include halo nuclei, which are good candidate systems to study the near-unitarity limit and universality. Two-neutron halos have been extensively studied, such as 6He, 9B, 11Li, 12Be, and 12C. With the large neutron-neutron (nn) 1S0 scattering length (as~-18.5 fm), halo nuclei are good candidates to study universal physics near the unitarity limit and the possible emergence of Efimov physics in Borromean systems or the scattering continuum. In this work, we use the adiabatic hyperspherical representation to study halo nuclei consisting of four neutrons. The adiabatic hyperspherical representation has been extensively applied to few-body systems, in which a description of all possible reaction pathways is treated on an equal footing from treating a collective coordinate, the hyperradius, adiabatically. I will present currently ongoing work that focuses on the 4He+2n , 4He+3n , and 4He+4n systems. In particular, the 4He+4n system has been of recent theoretical interest sparked by the 2022 experiment by Duer et. al. that found a low-energy 4n signal in the missing mass spectrum of the 8He(p,p4He)4n reaction. This work aims to provide theoretical insight into the qualitative and quantitative nature of the five-body scattering continuum and possible universal physics arising in four-neutron halos from the nn interaction. I will further present our previous work on the four-neutron system
20 Mar

The Spin on Angular Momentum in Fission

20 March 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
Lawrence Livermore National Laboratory

Ramona Vogt

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Fission studies have undergone a renaissance in the last decade or so. Much of the new work, both
experimental and theoretical, has focused on correlated observables. To address these types of observables,
fission models that can treat complete fission events are needed. (One cannot look at fission as a black
box generating independent neutron and photon emission.) Simulation codes have been developed to
generate complete fission events. One of these codes is the fission model FREYA which is very well
suited for studying fission because it can quickly and easily generate fission events and reveal observational
consequences. For example, the role of angular momentum in fission has been the subject of intense recent
attention. Data published in Nature suggested that fission fragment spins were largely uncorrelated, while
one might instead expect that the fragment spins are highly correlated. This talk will introduce FREYA
and some of its applications to fission studies, with an emphasis on its treatment of angular momentum.
†This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory
under Contract DE-AC52-07NA27344.

20 Mar

Does Nuclear Arms Control with Russia and China Have a Future?

20 March 2024 - 5:00 PM
1300 FRIB Laboratory
Carnegie Endowment for International Peace

George Perkovich

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Distinguished Nuclear Policy Lecture Series:

Nuclear arms control for the foreseeable future will be hindered by polarized politics that impact compromise with foreign adversaries and internal opponents, and by the emergence of new technologies and multi-party rather than bilateral strategic contests. This presentation will explore how these processes confound military planners, political leaders, and diplomatic negotiators in each country who would have to figure out what sorts of arms control bargains are desirable and acceptable. History suggests ways to overcome these obstacles, but the pathways to be navigated today are more challenging.

22 Mar

Tentative Thesis Title: Investigating Neutron-Rich Pre-Fragment Distributions in Projectile Fragmentation Reactions

22 March 2024 - 1:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Georgia Votta

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Committee: Paul Gueye (Chairperson), Chloe Hebborn Rachel Henderson, Kendall Mahn, Michael Thoennessen
22 Mar

SRF Cavities Resonance Control

22 March 2024 - 3:00 PM
Online via Zoom
Fermilab

Yuriy Pischalnikov

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SRF cavities, that are central elements of the modern accelerator complexes, required accurate frequency control, which is achieved using cavity tuners. Review of the sources of the SRF cavity detuning and brief discussion of the mitigation techniques will be presented. Talk will summarize the result of 20 years of international activities into development of different types of SRF cavity tuners. The solutions of the many technical problems to deliver tuners that could reliably operate for 30+ years (lifetime of the accelerator) will be discussed.
22 Mar

Electronic Music Workshop: Explorations in Improvisation

22 March 2024 - 5:30 PM
1300 FRIB Laboratory
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Electronic Music Workshop (EMW) is an eclectic ensemble that features a rotating instrumentation and combination of acoustic and electronic instruments. EMW is an improvisation-based ensemble, often co-composing pieces as a group based on their collective interests. EMW also interprets poetry or visual art through music and performs non-traditional scores written by contemporary composers. EMW seeks to foster communication, creativity, and confidence through exploring experimental means of music-making.

23 Mar

Artist Talk & Reception

23 March 2024 - 2:00 PM
1300 FRIB Laboratory
Studio Korinsky

Abel Korinsky

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Meet the inaugural MSUFCU Arts Power Up Artist-in-Residence Abel Korinsky, of the Berlin-based Studio Korinsky. Over the next few months, Korinsky will be embedded in the Facility for Rare Isotope Beams (FRIB), one of the world's leading nuclear physics laboratories. From this experience, he will create pieces to be exhibited by the MSU Museum CoLab Studio in Fall 2024. Come hear about Korinsky's artistic philosophy, past work, and his vision for this endeavor. Register here: https://113145.blackbaudhosting.com/113145/Artist-Talk-and-Reception
27 Mar

Past, present and future vision for high-gradient linear accelerators and its applications to future high-energy physics machines, light sources, and medical instruments

27 March 2024 - 4:10 PM
101 Biochemistry Building
Stanford University

Sami Tantawi

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We start with an overview of the history of high-gradient linear accelerator developments that took place over the span of more than three decades to pave the way for a future collider to explore the energy frontier of high-energy physics. We then present an overview of recent advances in high-gradient linear accelerators operating at room temperature and cryogenic temperatures. We will include the advances that enabled us to understand better the underlying fundamental physics that governs the breakdown phenomena in high-field vacuum structures. With this new understanding, recent advances in linac topologies, materials, and operating temperatures started to emerge. We will review these and present a vision for future energy frontier machines and future light sources. The vision for this future research and development will include the core effort on the linacs, RF sources, and other auxiliary components, with the goal of optimizing the overall system performance and cost rather than the optimization of individual components independently. These advances also promise to revolutionize many other applications in the near future, including medical radiotherapy devices. We will explore the ongoing effort on this front, especially the possibilities for realizing the so-called “flash treatment.
28 Mar

Meet and Greet FRIB Artist in Residence Abel Korinsky

28 March 2024 - 11:00 AM
1200 FRIB Laboratory
Studio Korinsky

Abel Korinsky

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Meet the inaugural MSUFCU Arts Power Up Artist-in-Residence Abel Korinsky, of the Berlin-based Studio Korinsky. Over the next few months, Korinsky will be embedded at FRIB. From this experience, he will create pieces to be exhibited by the MSU Museum CoLab Studio in fall 2024. Come hear about Korinsky's artistic philosophy, past work, and his vision for this endeavor. The MSUFCU Arts Power Up Arts Residency at FRIB program is generously supported by an endowed gift from the Michigan State University Federal Credit Union
29 Mar

Nucleosynthesis with Multi-Dimensional Supernova Simulations

29 March 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
LLNL

Andre Sieverding

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Core-collapse supernovae, the extremely energetic explosions of stars 10 times more massive than our sun, are known to be major contributors to the synthesis of the elements in the universe. Most of our understanding of these contributions is based on parameterized, spherically symmetric models. Only recently, multi-dimensional, self-consistent simulations have been carried out. Evaluating the nucleosynthesis of such large-scale simulations poses unique challenges and opens up new questions, that will be presented here. The first studies in this area, however, also show that there is a large potential for such simulations to address some long-standing tensions between theory and observations and due to the large variability of conditions predicted by the recent simulations, accurate predictions of the compositions requires knowledge of the nuclear properties and cross-sections on both sides of beta-stability. Prepared by LLNL under Contract No. DE-AC52-07NA27344. This research was supported by the European Union's Horizon Europe Programme under Marie Sklodowska-Curie grant agreement No.101065891, and by the German Research Foundation through the Collaborative Research Centre “Neutrinos and Dark Matter in Astro-and Particle Physics (NDM)”, grant No. SFB-1258-283604770, and through the Cluster of Excellence ORIGINS (EXC2094-390783311). LLNL-ABS-858843
29 Mar

Harp Performance: Chansons de Paris

29 March 2024 - 5:30 PM
1300 FRIB Laboratory
Show/Hide Abstract

Performer Bios

Richie Diaz is a flutist from Abilene, Texas, where he earned his bachelor’s degree in music performance in flute at Hardin-Simmons University. He is currently studying at MSU to receive his master of music degree in music performance. In 2018, Diaz received the Outstanding Soloist award at the Texas State Solo and Ensemble Contest. During his time at Hardin-Simmons Diaz was a private lesson instructor for the Abilene Independent School District while also holding the co-principal spot of the Civic Orchestra of Abilene. While studying at Hardin-Simmons, Diaz has traveled and performed with the “World Famous” Cowboy Band, marching in the 2020 Mardi Gras parade in New Orleans, Louisiana, as well as the 2022 St. Patrick’s Day Parade in Dublin, Ireland. Diaz has studied under Alex Carpenter (Hardin-Simmons), Richard Sherman (MSU), and Hannah Hammel Maser (Detroit Symphony Orchestra), as well as taken lessons from Melissa Suhr (University of Houston), Kathrine Kemmler (Louisiana State University), and Terri Sundberg (University of North Texas).

Astrophysicist and harpist Katelynn Ehlert is originally from Sturgis, Michigan, and is currently a fifth-year undergraduate student at MSU. She us pursuing her bachelor or art degree in music and bachelor of science degree in astrophysics. Ehlert is currently working as a research assistant at MSU for the IceCube Neutrino Observatory, where she works towards furthering the study of neutrinos. Prior to this, she spent two years working on the ATLAS upgrade for CERN at MSU. Ehlert is also an active advocate for women and minorities in STEM as has served as the president of the MSU chapter of the Society of Women in Space Exploration for the last four years. An experienced orchestral and solo musician, Ehlert has had the opportunity to work with the Symphony of the Lakes, the Lansing Symphony Orchestra, the Livington Symphony Orchestra, and various MSU ensembles. She was also the a finalist for the MASTA Elizabeth E.H. Green Solo Competition in 2023. Ehlert also has experience as a music educator. She is currently an instructor for the Capitol Harp Ensemble, and has been the instructor at the Sturgis High School Orchestra Camp for five years. On top of this, she is currently the vice president of the West Michigan Harp Chapter. Throughout her 12 years as a harpist, Ehlert has studied with many accomplished members of the harp community, includinjg Chen-Yu Huang, Elzbieta Szmyt, Jan Jennings, Molly Grettenberger, and Stephanie Gustafson. Ehlert is currently furthering her studies at MSU with Cheryl-Losey Feder as her primary educator.

Canadian violist Meagan Turner is in demand throughout North America and Australia. Turner has served as principal violist of the New York String Orchestra Seminar, Spoleto Festival Orchestra, Tanglewood Music Centre Orchestra, and Juilliard Orchestras, and regularly performs with the Australian Chamber Orchestra. An active chamber musician, she has attended the Ravinia Steans Music Institute and has been a guest artist at Tippet Rise, the Mackay Chamber Music Festival, and guest principal violist with Sydney’s Omega Ensemble. Turner is the recipient of numerous awards, including the Rachel Elizabeth Barton Pine and Virtu Foundation career grants, and was recently named one of Canada’s “Hottest Musicians Under 30” by the Canadian Broadcasting Corporation (CBC). From 2018-2020, she held a young artists’ residency at Carnegie Hall. Turner completed her undergraduate studies at the University of Toronto and her master’s degree at The Juilliard School as a full scholarship student. She is currently pursuing a doctor of musical arts degree with Eric Nowlin at MSU.

01 Apr

Beyond Rare Connections

01 April 2024 - 11:00 AM
1200 FRIB Laboratory
FRIB/Michigan State University

Agnes Mocsy

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Ágnes Mócsy will give a ten-minute presentation at the beginning, providing her thoughts on projects she is interested in pursuing at FRIB after the completion of the Rare Connections film. After the presentation, there will be an informal discussion where people can share their ideas on how this opportunity can be useful for enhancing diversity, broadening participation, informal science education, student recruitment, highlighting nuclear science to the public, and building bridges between art and science
04 Apr

Studying Fission Properties Near 198Pb with AT-TPC at FRIB

04 April 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
FRIB Michigan State University

Curtis Hunt

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Since the discovery of the fission, fission decays has been measured for actinide nuclei and for compound nuclei formed in collisions of long-lived projectile and target nuclei. Expanding such studies to include collisions of rare isotope beams with stable targets allows fission studies to be extended to new regions of the nuclear chart. Recent measurements with rare isotope beams have revealed an unexpected island of asymmetric fission in the region of the neutron deficient pre-actinides, around 180Hg through 198Pb. The fission properties for isotopes in this region have been calculated, suggesting that asymmetric fission may be more common than expected, but experimental information is sparse. We have developed a new method to study the fission barrier and mass asymmetry using the Active Target Time Projection Chamber (AT-TPC). I will discuss results from an initial study that looked at the rare isotopes along the transition from symmetric to asymmetric fission near 198Pb. These rare isotopes were produced by fusing rare isotopes separated by the A1900 separator at the NSCL with 4He target nuclei in the AT-TPC. The rare isotope beam particles were isotopically identified with the new Heavy Isotope Tagger (HEIST), allowing for the identification of the fissioning nucleus on an event-by-event basis. A combination of traditional and machine learning methods has been utilized to identify fission events and the excitation energy of the compound nucleus has been determined by studying the energy loss of the fission products in the AT-TPC. I will present preliminary cross sections and fission barriers that have been found for some Astatine isotope. Prospects for future fission experiments at FRIB with the AT-TPC will also be discussed.
05 Apr

Solid-phase Isotope Harvesting: Harvesting Radioisotopes from Beam Irradiated Tungsten, Boron and Lutetium

05 April 2024 - 2:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Samridhi Satija

05 Apr

Hadron Storage Ring of Electron-Ion Collider

05 April 2024 - 3:00 PM
Online via Zoom
Brookhaven National Laboratory

Vadim Pittsyn

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The Electron Ion Collider (EIC) is a new collider that will carry out experiments to study in great detail the structure of nucleons and nuclei, as well as the role of gluons in the matter around us. The collider is presently in the design and early construction stages at the Brookhaven National Laboratory. One of the major components of the EIC is the Hadron Storage Ring (HSR), which will provide for collisions in a wide energy range beams of different species, from protons to heavy ions. A large part of the experimental program of the EIC requires polarized beams; thus, the HSR will be capable of providing highly polarized beams of protons and helions. The HSR will reuse most of the existing hardware from the RHIC accelerator ring; however, extensive modifications will have to be performed to prepare for the new accelerator parameters and performance required by the EIC. This includes upgrades of the beam vacuum chamber, beam instrumentation, RF system, and the injection system. A hadron cooler must be constructed to create the hadron beam quality required for high luminosity experiments. We will overview the main design features of the HSR, as well as the most important upgrades required to transform RHIC into the EIC HSR.
09 Apr

Resonance Compensation Studies at the Fermi National Accelerator Laboratory Recycler Ring

09 April 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Cristhian Gonzalez-Ortiz

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Committee: Peter Ostroumov (Chairperson), Paul Gueye, Yue Hao, Steven Lund, Kendall Mahn Thesis is available at https://pa.msu.edu/academics/graduate-program/current-graduate-students/draft-dissertations-for-review/ - Select student name
09 Apr

Beam Diagnostics of the J-PARC Accelerator and Its Applications

09 April 2024 - 4:00 PM
1200 FRIB Laboratory and Online via Zoom
High Energy Accelerator Research Organization (KEK)

Takeshi Toyama

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At first overview of the project status and future plans of J-PARC (Japan Proton Accelerator Research Complex) will be given.

Next beam diagnostic instruments of the J-PARC accelerators will be reviewed.
The talk will focus on measurements of high-intensity H-minus beams and proton beams, discussing our experience of "non-invasive" diagnostics.

Application to the machine protection system (MPS) will be shown how the MPS has been progressing by responding actual incidents caused by increasing beam intensity.

10 Apr

Tentative Thesis Title: Uncertainty Quantification in Few-Body Reaction Theory

10 April 2024 - 9:30 AM
1300 FRIB Laboratory
FRIB Graduate Research Assistant

Manuel Catacora-Rios

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Committee: Filomena Nunes (Chairperson), Chloe Hebborn, Carlo Piermarocchi, Willie WY Wong, Remco Zegers
10 Apr

New Methodology for Probing Halo Structure in Excited States

10 April 2024 - 10:30 AM
1300 FRIB Laboratory
FRIB Graduate Research Assistant

Andrew Douglas

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Committee: Hironori Iwasaki (Chairperson), Sophie Berkman, Alyssa Gaiser, Chloë Hebborn, Artemis Spyrou
10 Apr

New Quantum Algorithms and Analyses for Hamiltonian Simulation

10 April 2024 - 3:00 PM
1400 Biomedical and Physical Sciences Building and Online via Zoom
FRIB Graduate Research Assistant

Jacob Watkins

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Committee: Dean Lee (Chairperson), Morten Hjorth-Jensen, Ryan LaRose, Mohammad Maghrebi, Johannes Pollanen Thesis is available at https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name
10 Apr

Nuclear Data to Quantify Urca Cooling in Accreting Neutron Stars

10 April 2024 - 9:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Rahul Jain

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Committee: Hendrik Schatz (Chairperson), Edward Brown, Michael Murillo, Witold Nazarewicz,Artemis Spyrou Thesis is available at https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name
11 Apr

Scalable Readout System for multiple detector applications

11 April 2024 - 11:00 AM
1200 FRIB Laboratory
CERN

Alexander Rusu

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The SRS developed and introduced in 2009 by RD51 collaboration is a common effort inside the community members. The system was designed to be versatile and to have a multi purpose approach such that one can use multiple Front End ASICs for various detectors. The initial detector application were GEMs and Micromegas and the first ASIC used for the system was the APV25 a multiple channel preamplifier but after some time an upgrade for higher rates was required and the system migrated towards the VMM ASIC developed for the ATLAS New Small Wheel detector. After several iterations and intensive R and D work the final and reliable version of VMM 128 Channel Hybrid V5.2 was ready for the user community. SRS Technology the CERN Spin Off successfully implemented production lines for the SRS hardware and is constantly involved in the support of the research groups and in the new SRS related upgrades. One SRS FEC ( Front End Concentrator ) consists of 1024 channels input from the VMM Hybrids and starting from 2023 new FECs are under development for 256 or 2048 channels extending the flexibility and creating also compactness crate less hardware for easier usage set-up. The new FECs will have possibility for new ASICs integration such as HGCROC and Timepix. The ALICE Collaboration is building for Run 4 at LHC a Forward Calorimeter and the VMM SRS successfully took part in the test beam readout campaign of the Hadronic Calorimeter that is SIPM based of Focal H.
11 Apr

Intersection Conversation: Stellar Connections between Art and Science

11 April 2024 - 5:30 PM
1300 FRIB Laboratory
Studio Korinsky

Abel Korinsky

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Join us for an exciting discussion between Abel Korinsky, the inaugural MSUFCU Arts Power Up Artist-in-Residence, and Hendrik Schatz, MSU University Distinguished Professor of Nuclear Astrophysics and scientist at FRIB. They'll explore the fascinating intersection of artistic expression and scientific discovery. Register for the talk here: https://113145.blackbaudhosting.com/113145/Stellar-Connections-Between-Art-and-Science A hands-on workshop led by artist Abel Korinsky will follow the conversation to continue to explore this topic. This portion take place at Rm 1309. Register for the workshop here: https://113145.blackbaudhosting.com/113145/Stellar-Connections-Hands-On-Workshop
12 Apr

First Light And Reionisation Epoch

12 April 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
University of Sussex

Aswin Vijayan

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In this talk I will walk you through some of the open questions in the galaxy formation and evolution in the first billion years, which can be roughly termed the First Light And Reionisation Epoch. I will discuss how simulations of galaxy formation and evolution are a great avenue to interpret the current observational data. In particular I will focus on a suite of simulations that I work with, termed the First Light And Reionisation Epoch Simulations (FLARES), that have been designed to produce a statistical sample of high-redshift galaxies, that will be accessible to current and next generation telescopes like Euclid, JWST or Roman. I will talk about how we forward model our simulated galaxies into the observed space allowing us to work as close as possible to the observations. I will briefly talk about the successes and drawbacks of the simulation with respect to the latest data from JWST. I will then shift my focus on how the presence of dust complicates the interpretation of emission line spectra that are used to understand the nature of the ISM in these high-redshift systems, now accessible due to JWST.
12 Apr

Voice and Piano Concert

12 April 2024 - 5:30 PM
1300 FRIB Laboratory
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Program

from Mörike-Lieder - Hugo Wolf (1860-1903)
-Er ist's   

from Lieder-Album für die Jugend - Robert Schumann (1810-1856)
-Er ist’s

Die Forelle, Opus 32 - Franz Schubert (1797-1828)

from La Rondine - Giacomo Puccini (1858-1924)
-“Chi il bel sogno”  

from Don Giovanni - Wolfgang Amadeus Mozart (1756-1791)
-“Dalla sua pace”

from Hermit Songs, Opus 29 - Samuel Barber (1910-1981)
-At St. Patrick’s Purgatory
-St. Ita’s Vision
-The Crucifixion
-Promiscuity
-The Monk and His Cat
-The Desire for Hermitage

from 7 Elizabethan Songs, Opus 12 - Roger Quilter (1877-1953)

Weep No More  
My Life’s Delight
Fair House of Joy

Minicabs - William Bolcom (b. 1938)

I Feel Good About Something     
People Change
Those
Food Song #1
Food Song #2
I Will Never Forgive You
Songette
Not Even a Haiku
Maxim #1
Maxim #2
Anyone
Finale: Mystery of the Song?

from Music Box Revue  - Irving Berlin (1888-1989)
What'll I Do?        

from The Fantasticks - Harvey Schmidt (1929-2018)
Soon It’s Gonna Rain

Performer Bios

 

Mira Choi is currently a doctor of musical arts student in collaborative piano at MSU, studying with Zhihua Tang. She holds a master's degree from MSU under Zhihua Tang, a master’s degree from Sungshin Women’s University in Korea under Jinhye Lee and Gyeongju Jang, and a bachelor’s degree from Kyungnam University in Korea, studying with Soohyun Cho. Serving as a collaborative pianist at MSU, Mira plays for the MSU Opera under Professor Helton, showcasing her talent in productions like Mozart's La finta giardiniera, Don Giovanni, Verdi's Falstaff, and Sondheim's A Little Night Music. She also provides accompaniment for the Singing Spartans (the former MSU Men’s Glee Choir), directed by Dr. Reed, and supports vocal students in Professor Fracker's studio. Her participation in numerous master classes, including those led by Helmut Deutsch and Cameron Stowe, highlights her commitment to continual learning and growth. Mira's accompaniment repertoire extends to various music classes, instrumental and vocal recitals, and ensemble performances within MSU. Her previous engagements include facilitating master classes at the Centro Studi Carlo Della Giacoma in Todi, Italy, collaborating with Viridis (the former MSU Women's Glee Choir), and participating at the Interlochen Arts Summer Camp. Currently, she serves as the choir pianist at the First Presbyterian Church in Holt, continuing her dedicated involvement in both educational and community music settings.

 

Cole Harvey is a tenor currently pursuing his master’s degree in vocal performance from MSU. He will return next semester to begin his doctor of musical arts degree at MSU in vocal performance. Cole has sung many roles for MSU Opera Theater, including Albert in Albert. He was also selected as one of 32 emerging artists to participate in this summer’s Seagle Young Artist Festival, featuring young artists from around the country. Cole will cover the role of Don Ottavio in Don Giovanni, as well as play Pireli in Sweeney Todd.

Paige Heidrich, a soprano, is an Ohio native currently pursuing a doctor of musical arts degree in voice performance at MSU. She received a master’s of music degree in voice performance at MSU as well as undergraduate degrees in voice performance and music education from Baldwin Wallace University’s Conservatory of Music. After working mostly in musical theater summer stock, Paige went on to sing the roles of Pamina in The Magic Flute and Constance in Dialogues of the Carmelites with Resonanz Opera after her undergraduate work. She has also been seen on the MSU mainstage as Alice Ford in Falstaff, Lady Billows in Albert Herring, and Geraldine in A Hand of Bridge. As a soloist, Paige has debuted chamber works by composers Lincoln Sandham and Jeremy Makkonen. She has also been a featured soloist with the MSU Chorale, the BW Treble Choir, and the Ashtabula Area Orchestra. As an educator, she frequently collaborates with pianist Dr. Tina Gorter to produce recitals and master classes focusing on chamber music communication. Paige currently maintains two private studios through the MSU Community Music School and the Brighton School for the Arts. This summer, she will appear in the Detroit Opera’s production of The Cunning Little Vixen, and will be working as the assistant director for the Des Moines Metro Opera’s production of The Barber of Seville.

16 Apr

From Chiral Effective Field Theory to Perturbative Quantum Chromodynamics: A Bayesian Model Mixing Approach to Symmetric Nuclear Matter

16 April 2024 - 11:00 AM
1200 FRIB Laboratory
Ohio University

Alexandra Semposki

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Constraining the equation of state (EOS) of strongly interacting, dense matter is the focus of intense experimental, observational, and theoretical effort. Chiral effective field theory (ChEFT) can describe the EOS at densities up to twice nuclear saturation density (n0), while perturbative QCD (pQCD) can be applied to properties of deconfined quark matter. The uncertainty due to truncation of the perturbative series at a finite order can be quantified for both theories using a single methodology, developed by the BUQEYE collaboration, that I will explain in my talk. However, this still leaves uncertainty quantification for the EOS in the intermediate region between 2n0 and (20-40)n0 as an unsolved problem. To bridge this gap between ChEFT and pQCD, we employ Bayesian model mixing (BMM) techniques we are developing for the BAND collaboration’s cyberinfrastructure framework. Specifically, we combine Gaussian random variables that constitute the predictions from each theory for the pressure as a function of the density in symmetric nuclear matter. In this FRIB theory seminar, I will present results from our recent arXiv submission for the pressure and speed of sound squared of symmetric nuclear matter. These results were obtained from the application of two BMM approaches: a pointwise approach, and a correlated approach implemented via a Gaussian process (GP), the latter of which allows for inclusion of full covariance information from both theories to the model mixing. I will also discuss extensions of this work for future improvements and applications to neutron-rich matter.
17 Apr

Probing Neutron-rich Nuclei: from Level Scheme to Nuclear Radii

17 April 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
Facility for Rare Isotope Beams

Paul Gueye

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Starting over two decades ago, the MoNA Collaboration has now established itself as a leader in the understanding of the nuclear structure from the study of neutron unbound nuclei through (primarily) nuclear breakup or particle removal reactions. This Collaboration, comprised of eleven undergraduate institutions working with Michigan State University, started at the then National Superconducting Cyclotron Laboratory and is now entering a new era at the Facility for Rare Isotope Beams. It uses the invariant mass spectroscopy technique to reconstruct the decay energy of these neutron rich nuclei from the experimentally measured four-momenta of the decay (fragments and neutrons) products. This is performed by leveraging the Modular Neutron Array and Large multi-Institutional Scintillator Array (MoNA-LISA) plastic scintillator-based neutron detectors and a large gap Sweeper magnet, the latter preceding a suite of charged detector systems. This talk will highlight two experiments utilizing the MoNA-LISA-Sweeper system: the measurement of the 26O lifetime and search for excited states in 31Ne. In addition to their primary focus, the former lead to extracting further insights into 27O, thus complementing a recent measurement of this isotope at the Japanese RIKEN facility, and the latter is providing new pathways to extract information about nuclear sizes for neutron rich nuclei. These novel analyses are opening new science opportunities for the MoNA Collaboration, including bridging a gap with a recent effort to address the neutron skin puzzle through electron scattering at intermediate energies. The aforementioned also contributed strongly to expanding the reach of FRIB to broaden representation in nuclear science furthering the impact of this facility for the U.S. nuclear science workforce.
19 Apr

High-Field Superconductors and Superconducting Magnets for Electron Cyclotron Resonance Ion Source and Frontier Nuclear Physics

19 April 2024 - 3:00 PM
1221A and 1221B FRIB Laboratory
Lawrence Berkeley National Laboratory

Tengming Shen

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FRIB and LBNL have been collaborating to build high-field superconducting ECR ion source (ECRIS). Out of this collaboration, the first 28 GHz all superconducting Nb-Ti based ECRIS magnet has been in operation at FRIB since 2022 and the designing and prototyping efforts in using a higher-field Nb3Sn conductor are ongoing. This talk will discuss performance, design, design and simulation tools, fabrication methods used for these magnets, and their limits. This talk will also discuss characteristics of practical high field superconductors (Nb-Ti, Nb3Sn, and high-temperature superconductors), a new MARS-ECRIS magnet concept being prototyped at LBNL, the possibility of utilizing high-temperature superconductors for building ECRIS and frontier nuclear physics.

22 Apr

Tentative Thesis Title: Commissioning the Separator for Capture Reactions (SECAR) for Proton Capture Reactions

22 April 2024 - 3:00 PM
1200 FRIB Laboratory
FRIB Graduate Research Assistant

Machenzie Smith

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Committee: Hendrik Schatz (Chairperson) Heiko Hergert, Wolfgang Kerzendorf, Fernando Montes, Artemis Spyrou, Kirsten Tollefson.
23 Apr

Tentative Thesis Title:
Precision Mass Measurement of Proton Halo Candidate Aluminum-22 and the Development of the Single Ion Penning Trap

23 April 2024 - 2:00 PM
1200 FRIB Laboratory
FRIB Graduate Research Assistant

Scott Campbell

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Committee: Ryan Ringle (Chairperson), Kei Minamisono, Scott Pratt, Reinhard Schwienhorst, Hui-Chia Yu.
24 Apr

Exploring the origins of the elements and the limits of existence through nuclear reactions

24 April 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
FRIB

Kyle Brown

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The origin of the chemical elements and the limits of nuclear binding are strongly linked. The heaviest elements on the periodic table are made in explosive astrophysical environments, through reactions on nuclei at the edge of existence. My work focuses on these two separate, but linked problems. I will discuss first the efforts of my group and the broader HiRA collaboration to study the nuclear equation of state (EoS) through collisions of heavy ions. The nuclear EoS underpins our understanding of how nucleons assemble themselves from finite nuclei to neutron stars. With the next generation accelerator facilities coming online, the nuclear science community is poised to further improve our understanding of the nature of neutron-rich nuclear matter with terrestrial measurements. I will discuss our recent results from data taken at NSCL, and discuss our future plans with the new opportunities afforded by the Facility for Rare Isotope beams. I will then discuss my work on two-proton decay. These unbound nuclei allow one to glimpse the underlying nuclear potential and provide a test of our nuclear models.
26 Apr

Towards a Magnetic Centrifuge Decelerator for Polar Molecules for Testing Fundamental Symmetries of the Universe

26 April 2024 - 9:00 AM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Sebastian Miki Silva

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Committee: Wu, Xing [Chairperson], Becker, Jonas Nils, Cocker, Tyler L, Severin, Gregory William, Singh, Jaideep Taggart
26 Apr

Probing Dense Matter in Neutron Stars

26 April 2024 - 10:00 AM
2025 FRIB Laboratory and Online via Zoom
Goethe University Frankfurt

Juergen Schaffner-Bielich

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*Please note that this seminar will take place at 10am Eastern Time Neutron Stars are born in core-collapse supernovae being the endpoint of stellar evolution of massive stars. Their extreme properties allow for the study of dense matter in the sky. In recent years the advancement of astrophysical observations has been so tremendous that the properties of neutron stars can be constrained nowadays to an unprecedented level. I will summarize the basic observations of neutron star masses from pulsar data, the constraints on radii from x-ray measurements, and the first detection of gravitational waves from a neutron star merger. On the other hand, I will discuss the nuclear and particle physics aspects of the equation of state of neutron star matter which is firmly limited at low and high energy densities. Chiral effective field theory puts a stringent constraint up to about saturation density for pure neutron matter. Perturbative QCD calculations narrow the equation of state at ultimately high densities. Finally, I will address the possible existence of new phases in the core of neutron stars which can be revealed from the mass-radius relation of neutron stars. I will argue that it is in principle impossible to rule out phase transitions in neutron stars from observations based on general relativity alone. Speaker Homepage: https://astro.uni-frankfurt.de/schaffner/
29 Apr

Tentative Thesis Title: Evaporative Cooling: Quantum Algorithm for Ground State Preparation of the N-Particle Hamiltonians

29 April 2024 - 3:00 PM
Online via Zoom
FRIB Graduate Research Assistant

Paul-Aymeric McRae

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Committee: Morten Hjorth-Jensen (Chairperson), Alexei Bazavov, Jonas Becker, Alex Brown, Ryan Larose, Dean Lee
30 Apr

Quantum Algorithms for Simulating Nuclear Effective Field Theories

30 April 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
University of Maryland

James Watson

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Quantum computers offer the potential to simulate nuclear processes that are classically intractable. With the goal of understanding the necessary quantum resources, we employ state-of-the-art Hamiltonian-simulation methods, and conduct a thorough algorithmic analysis, to estimate the qubit and gate costs to simulate low-energy effective field theories (EFTs) of nuclear physics. In particular, within the framework of nuclear lattice EFT, we obtain simulation costs for the leading-order pionless and pionful EFTs. We consider both static pions represented by a one-pion-exchange potential between the nucleons, and dynamical pions represented by relativistic bosonic fields coupled to non-relativistic nucleons. We examine the resource costs for the tasks of time evolution and energy estimation for physically relevant scales. We account for model errors associated with truncating either long-range interactions in the one-pion-exchange EFT or the pionic Hilbert space in the dynamical-pion EFT, and for algorithmic errors associated with product-formula approximations and quantum phase estimation. Our results show that the pionless EFT is the least costly to simulate and the dynamical-pion theory is the costliest. We demonstrate how symmetries of the low-energy nuclear Hamiltonians can be utilized to obtain tighter error bounds on the simulation algorithm. By retaining the locality of nucleonic interactions when mapped to qubits, we achieve reduced circuit depth and substantial parallelization. This work highlights the importance of combining physics insights and algorithmic advancement in reducing quantum-simulation costs.
02 May

Tentative Thesis Title: Adiabatic Perturbation Theory

02 May 2024 - 4:00 PM
1221 Conference Room and Online via Zoom
FRIB Graduate Research Assistant

Nicholas Cariello

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Committee: Morten Hjorth-Jensen (Chairperson), Ryan LaRose, Dean Lee, Johannes Pollanen, Yang Yang
05 May

Nobel Prize-winning physicist William Phillips - The Quantum Reform of the Modern Metric System

05 May 2024 - 1:00 PM
Online via Zoom
National Institute of Standards and Technology

William D. Phillips

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“The metric system, now officially known as the International System of Units (SI), was born with the French revolution. It has recently undergone its most revolutionary reform since that birth. Famously, the kilogram is no longer defined as the mass of an artifact, the International Prototype Kilogram, but rather is now a quantum concept, defined by fixing the value of Planck’s constant. In fact, all of the base units of the SI are defined by fixing the values of natural constants, and the SI now has a distinctly quantum flavor. The quantization of charge allows us to fix the charge of the electron, defining the ampere as a certain number of electrons per second. The unit of temperature, the kelvin, is no longer based on the triple point of water, but on the thermal energy of the atomic/molecular components of matter, by fixing the value of Boltzmann’s constant. The unit of time has long been quantum, but its impending re-definition will make it even more so.”

06 May

Tentative Thesis Title: Progress Towards Searching for Time-Reversal Violation Using Pear Shaped Nuclei

06 May 2024 - 1:30 PM
1200 FRIB Laboratory
FRIB Graduate Research Assistant

Aiden Boyer

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Committee: Jaideep Singh (Chairperson), Sophie Berkman, Witek Nazarewicz, Stuart Tessmer, Xing Wu
06 May

Tentative Thesis Title: Progress Towards Searching for Time-Reversal Violation Using Pear Shaped Nuclei

06 May 2024 - 1:30 PM
1200 FRIB Laboratory
FRIB Graduate Research Assistant

Aiden Boyer

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Committee: Jaideep Singh (Chairperson), Sophie Berkman, Witek Nazarewicz, Stuart Tessmer, Xing Wu
07 May

Investigation of Ponderomotive Effects in Narrow Bandwidth, Medium-velocity Elliptical Superconducting Radio-Frequency Cavities

07 May 2024 - 1:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Jacob Brown

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Committee: Ting Xu (Chairperson), Sergey Baryshev Wade Fisher, Peter Ostroumov, Vyacheslav Yakovlev, Remco Zegers
07 May

Tentative Thesis Title: Modeling Transverse Beam Dynamics to Optimize the Luminosity at sPHENIX

07 May 2024 - 2:00 PM
Online via Zoom
FRIB Graduate Research Assistant

William Fung

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Committee: Yue Hao (Chairperson), Wade Fisher Steven Lidia, Stuart Tessmer, Christopher Wrede
08 May

Tentative Thesis Title: Development of the Charge-Exchange Oslo Method and Application Towards Constraining Reaction Rates for Nucleosynthesis of Cosmochronometer Niobium-12

08 May 2024 - 10:30 AM
1300 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Neshad Pathirana

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Committee: Remco Zegers (Chairperson), Sophie Berkman, Laura Chomiuk, Chloe Hebborn, Artemis Spyrou
09 May

STREAMLINE Symposium

09 May 2024 - 8:00 AM
1221A and 1221B FRIB Laboratory
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The STREAMLINE (SmarT Reduction and Emulation Applying Machine Learning In Nuclear Environments) collaboration aims to advance the frontiers of theoretical and computational research on the nuclear many-body problem using ML. The scientific problems we address are among the most challenging in computational nuclear many-body theory and the collaboration is aligned with the U.S. government initiative to build a broad-based, multidisciplinary, multi-agency program for a sustained national AI structure. STREAMLINE will advance large nuclear physics computations to dramatically increase predictive power and improve our understanding of nuclear structure and dynamics, dense nucleonic matter, and emergent many-body phenomena -- this includes the properties of heavy neutron-rich nuclei and related astrophysical environments at the Facility for Rare Isotope Beams (FRIB); structure and reactions of nuclei and nuclear astrophysics at the Argonne Tandem Linac Accelerator System (ATLAS); neutron distributions in nuclei and few-body systems at Thomas Jefferson National Accelerator Facility (TJNAF); properties of fission at Los Alamos Neutron Science Center (LANSCE); and nuclear structure, reactions, and astrophysics at Association for Research at University Nuclear Accelerator facilities (ARUNA).
09 May

Tentative Thesis Title: Exploring the Neutron Drip Line in Elements Around Calcium

09 May 2024 - 11:00 AM
1300 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Isaiah Richardson

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Committee: Bradley Sherrill (Chairperson), Wade Fisher, Dean Lee, Peter Ostroumov, Oleg Tarasov
12 May

Nuclear Science Summer School

12 May 2024 - 5:00 PM
1221A and 1221B FRIB Laboratory
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The Nuclear Science Summer School (NS3) is a summer school that introduces undergraduate student participants to the fields of nuclear science and nuclear astrophysics. NS3 is hosted by FRIB on the campus of Michigan State University (MSU). The school will offer lectures and activities covering selected nuclear science and astrophysics topics.
14 May

Uncertainty Quantification and Development of Optical Potentials for Direct Reactions

14 May 2024 - 2:00 PM
1200 FRIB Laboratory
FRIB Graduate Research Assistant

Andrew Smith

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Committee: Chloe Hebborn (Chairperson), Brian O’Shea, Filomena Nunes, Jay Strader, Remco Zegers
15 May

Design of the Super3Hen Detector for B-Delayed Neutron Emission Studies in the R-Process

15 May 2024 - 2:00 PM
1108 FRIB Laboratory
FRIB Graduate Research Assistant

James Huffman

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Committee: Hendrik Schatz (Chairperson), Alyssa Gaiser, Daniel Hayden, Fernando Montes, Johannes Pollanen
04 Jun

Study of Online Electron Elastic Scattering System for Radioactive Beam

04 June 2024 - 3:00 PM
1200 FRIB Laboratory
FRIB Graduate Research Assistant

Ambar C. Rodriguez Alicea

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Committee: Paul Gueye (Chairperson), Alain Lapierre, Kendall Mahn, Kirsten Tollefson. Thesis is available at https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - choose student
25 Jun

NuclearToolkit.jl and Surrogate Models for In-Medium Similarity Renormalization Group

25 June 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
Utsunomiya University

Sota Yoshida

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In recent years, the development of efficient computational tools and methodologies has become increasingly crucial for advancing our understanding of nuclear structures and reactions. The FRIB/MSU group has been leading these directions: Here is the center of developing nuclear many-body calculations, and many codes (NuShellX, CENS, etc.) have been shared in the community. Starting from the eigenvector continuation method proposed by Prof. Dean Lee’s group, surrogate models have been developed for various nuclear models and models beyond our community. In the first part of this seminar, I will introduce NuclearToolkit.jl, a Julia-based package designed to facilitate complex nuclear physics calculations. This package is for young researchers like old me, struggling with the nuclear many-body calculations. This package covers a wide range of nuclear models, including the shell model, Møller-Plesset (also known as HF-MBPT), the In-Medium Similarity Renormalization Group (IM-SRG) method, surrogate models, and more. In the second part, I will focus on surrogate models especially in the context of the In-Medium Similarity Renormalization Group (IM-SRG) method. The IM-SRG is a powerful ab initio method for nuclear structure calculations and for deriving effective interactions and operators from realistic nuclear forces. I will introduce two surrogate models for further accelerating research workflows using the IM-SRG method. One is using a neural network and the other is based on the so-called dynamic mode decomposition. They are both complementary to each other. I will show the performance of these models and discuss a possible future direction to combine them.
27 Jun

Improved Search for CP-Violation in Ortho-Positronium Decay

27 June 2024 - 10:00 AM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Tom-Erik Haugen

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Committee: Oscar Naviliat-Cuncic (Chairperson), Joey Huston, Kirtimaan Mohan, Gregory Severin, Jaideep Singh. Thesis is available @ https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name
14 Jul

Physicists Inspiring the Next Generation

14 July 2024 - 9:00 AM
1221A and 1221B FRIB Laboratory
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Exploring the Nuclear Matter (PING) is a program that targets both pre-college students and undergraduate students (who serve as mentors). It was launched in 2014 as a collaboration between the National Society of Black Physicists (NSBP) and the National Radio Astronomy Observatory (NRAO) in partnership with Associated Universities, Inc.
16 Jul

Exotic Decays in Open Quantum Systems

16 July 2024 - 10:00 AM
Facility for Rare Isotope Beams
Fudan University

Simin Wang

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The nucleus serves as a distinctive platform for exploring quantum many-body physics, characterized by the interplay between its two fermionic components: protons and neutrons. When nuclei extend beyond the dripline, the delicate balance between these fermionic components is disrupted, leading to spontaneous decay. Under such extreme conditions, the presence of a low-lying continuum can induce exotic phenomena. This presentation will explore two types of exotic decays: 1. Two-Proton (2p) Radioactivity: This decay mode, a unique three-body process, involves the emission of two protons from the ground state of even-Z neutron-deficient nuclei. We will demonstrate how the internal structure influences the decay dynamics and nucleon-nucleon correlations in the asymptotic region. 2. Nonexponential Decay Regimes in Open Quantum Systems: This domain, governed by the continuum, challenges the classical understanding of decay processes. We will introduce new experimental observables designed to probe the post-exponential decay phase, including investigations into decay from threshold resonances, particle correlations in three-body decay scenarios, and the interference patterns arising from closely situated resonances. Through these detailed studies, we aim to provide new insights into the properties of open quantum systems.
21 Jul

Physics of Atomic Nuclei (PAN)

21 July 2024 - 8:00 AM
1221A and 1221B FRIB Laboratory
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PAN introduces participants to the fundamentals of the extremely small domain of atomic nuclei and its connection to the extremely large domain of astrophysics and cosmology.

The PAN @ Michigan State Experience

  • Learn about research in one of the top rare-isotope laboratories in the world.
  • Get introduced to the fascinating fields of astrophysics, precision measurement, and nuclear science.
  • Perform your own nuclear physics experiments.
  • Meet researchers who are exploring a wide array of questions.
  • Discover the surprising array of career opportunities in science.
  • Experience the atmosphere of college life.
  • Participants in the 2024 program get free room and board on campus (if required).
26 Jul

Production of Neutron-Rich Rare Isotopes Near N = 126 Via Medium Energy Fragmentation

26 July 2024 - 12:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Kenneth Taylor Haak

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Committee: Bradley Sherrill (Chairperson), Alexandra Gade, Peter Ostroumov, Carlo Piermarocchi, Oleg Tarasova. Thesis is available @ https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name
12 Aug

FRIB Theory Alliance Summer School - Put the Reaction into Action: A Nuclear Physics Boot Camp on Reaction Methods

12 August 2024 - 8:00 AM
1200 FRIB Laboratory
16 Aug

Eigenstate Preparation on Quantum Computers

16 August 2024 - 12:00 PM
1300 Biomedical and Physical Sciences Building
FRIB Graduate Research Assistant

Joseph Bonitati

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Committee: Dean Lee (Chairperson), Alexei Bazavov Saul Beceiro-Novo, Heiko Hergert, Filomena Nunes Brian O'Shea. Thesis is available @ https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name

04 Sep

Intruder States and Shape Mixing in ab Initio Calculations at the N=8 Shell Closure

04 September 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
University of Notre Dame

Mark Caprio

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While the structure of "normal" states is well described by valence space configurations, in "intruder" states nucleons are excited out of the valence shell, providing access to a much larger configuration space.

This allows intruder states to develop highly collective structure and greater deformation. Intruder states are notoriously challenging to describe in ab initio calculations, appearing too high in the excitation spectrum, if at all. However, with suitably soft interactions and sufficiently large-scale calculations, it becomes possible to reproduce intruders at realistic energies in the low-lying spectrum.  In this seminar, we will explore low-lying intruder structure in nuclei at the neutron N=8 shell closure, through ab initio no-core configuration interaction calculations.  We will see that mixing between normal and intruder configurations, of different deformation (shape), can be described approximately as two-state mixing, permitting extraction of a consistent mixing matrix element from the ab initio calculations.

06 Sep

Optimization Studies of Radiation Shielding for PIP-II Project at Fermilab

06 September 2024 - 3:00 PM
Online via Zoom
FermiLab

Alajos Makovec

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The Proton Improvement Plan-II (PIP-II) at Fermilab represents a significant advancement in the quest to answer some of the most profound questions about our universe using the world's most intense high-energy neutrino beam. The project requires the construction of a new addition to the Fermilab accelerator complex – an 800-MeV high-intensity superconducting linear accelerator. Ensuring the safety and regulatory compliance of this ambitious project is paramount, necessitating thorough dose rate assessments under both normal operational and accidental scenarios to align with the Fermilab Radiological Control Manual (FRCM) standards. Our approach included a comprehensive update of the geometry model to incorporate new magnet and collimator designs, essential for reflecting the current state of PIP-II infrastructure. The implementation of high-resolution detector planes, despite their computational demands, enabled us to gather detailed radiation field data crucial for optimizing shielding configurations. To overcome the significant computational demands, we developed a branching code that drastically reduced simulation runtimes while maintaining statistical integrity. This was achieved through geometry splitting and the application of Russian Roulette techniques, tailored to prioritize regions of interest based on predefined importances and weight limits. To complement these efforts, we are developing a new, more user-friendly graphical user interface (GUI) for the Monte Carlo code MARS. This GUI includes tools like the MTUPLE Grid Visualizer, which simplifies the visualization of simulation results. Together with other features under development, it aims to streamline the input creation and post-processing workflows.
06 Sep

Young Hyun Cho - Beethoven's Piano Sonatas: "Funeral March", "Moonlight", and "Pastoral"

06 September 2024 - 5:30 PM
1300 FRIB Laboratory
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Young Hyun Cho, an associate professor of piano in the MSU College of Music, will play three of Beethoven's piano sonatas. Cho has performed all over the world and released her CD with the Last Three Beethoven Piano Sonatas under the SONY Classical label.
11 Sep

Panning for Gold in the Laboratory: UV/Vis Spectroscopy of Multi-Charged Heavy Ions

11 September 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
Clemson University

Joan Marler

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The astrophysical origin of the heavy elements (masses greater than Rb) remains an open question. A new opportunity to directly probe regions where heavy elements may have formed, specifically as a result of active r-process nucleosynthesis, is provided by recent measurements of spectroscopy of neutron star merger ejecta. Optical and infrared spectra of the recent neutron star merger heralded by the first observation of a gravitational wave were obtained by an array of ground- and space-based telescopes. However, laboratory spectroscopic data on the vast range of heavy elements are so severely limited that emission models are only in qualitative agreement with the observed spectra. Recent experimental results by our group for the electronic structure of singly to triply-charged gold atoms, obtained at the Compact Toroidal Hybrid plasma experiment at Auburn University provide insight into the astrophysically observed spectra. Time permitting I will briefly discuss our current work cataloguing the x-ray spectroscopy resulting from charge exchange between Highly Charged Ions and astrophysically relevant neutral targets. Bio: Joan Marler received her PhD in Physics in 2005 from the University of California San Diego, where she investigated elastic and inelastic cross-sections of positrons with atoms and molecules. Following that, she has done postdocs studying electron plasmas in toroidial traps, CQED with laser cooled ions in rf traps and low temperature chemistry with trapped ions. Currently, she is an associate professor at Clemson University where she and her team investigate single and multi-charged ion physics especially in the context of astrophysically relevant systems.

12 Sep

Art, Words, Science and the Poetry in Between

12 September 2024 - 3:00 PM
1415 Biomedical and Physical Sciences Building
Michigan State University

Violeta Lopez

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The MSUFCU Arts Power Up Arts Residency will host this fall its second artist, Violeta Lopez. Violeta is an interdisciplinary artist who takes a multimedia approach to her practice, merging analog and digital through visuals, sound and words. The resulting work explores language, literature and science from a poetic perspective. For the first colloquium of the year we invite everyone to join us in welcoming Violeta and learning about her experiences and her plans for interacting with physicists at MSU and creating her own unique art work. The MSUFCU Arts Power Up Arts Residency Program is a collaboration between the Facility for Rare Isotope Beams (FRIB), the MSU Museum CoLab Studio, and the STEAMpower Project. It is generously funded by an endowment from the Michigan State University Federal Credit Union (MSUFCU), and administered by University Arts and Collections.
13 Sep

Assessing the Strength of the N=28 Shell Closure through High-Precision Mass Measurements and the Development of the Single Ion Penning Trap

13 September 2024 - 2:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Hannah Erington

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Committee: Ryan Ringle (Chairperson), Paul Gueye, Daniel Hayden, Witold Nazarewicz, Stuart Tessmer
15 Sep

Particle and Heavy Ion Transport code System (PHITS) Advanced Tutorial

15 September 2024 - 8:00 AM
1221A and 1221B FRIB Laboratory
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PHITS (Particle and Heavy Ion Transport code System) is a general-purpose Monte Carlo particle transport simulation code developed under a collaboration between several institutes all over the world. It can simulate the transport of nearly all particles over wide energy ranges, using nuclear reaction models and nuclear data libraries. PHITS can support research in the fields of particle and heavy ion transport phenomena
17 Sep

Towards Nuclear Reactions Essential for A Comprehensive Hindsight of the Universe

17 September 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
CNRS / IJCLab

Guillaume Hupin

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To advance our understanding of the universe, from physics beyond the Standard Model to cosmic events, a unified approach to nuclear structure and reactions is essential. This requires combining few-body techniques with ab initio many-body calculations of nuclear structure, supported by Effective Field Theory and uncertainty quantification. In this talk, I will outline the No-Core Shell Model with Continuum (NC-SMC), its extension, and its application in supporting a CERN program studying exotic nuclei through new experimental methods. The main challenge is developing precise methods that scale with A, while accounting for all relevant reaction channels, including those involving exotic particles.
18 Sep

How do stereotypes about who belongs in STEM relate to STEM belonging and motivation among undergraduates?

18 September 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
University of Wisconsin - Madison

Christy Starr

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Stereotypes may be one reason why there is less diversity in majors and fields related to STEM. This talk explores three kinds of stereotypes about who belongs in STEM: gender stereotypes, race/ethnic stereotypes, and nerd-genius stereotypes. These stereotypes about people who work in STEM may make those who don't fit the stereotypes feel like they don't belong. Research-backed methods of increasing belongingness in STEM classrooms and environments will also be discussed.
20 Sep

SRF technology for Quantum Computing and Dark Matter Searches

20 September 2024 - 3:00 PM
Online via Zoom
Fermilab

David van Zanten

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"Quantum information science is no longer a field of uniquely theoretical endeavors. Current state-of-the-art quantum hardware is capable of processing shallow algorithms and nearly reaches the domain where classical computing will struggle. In addition to the increase in performance, the last decade has shown a broadening of applications well beyond the typical mantra of the programmable quantum processor. A telling example is the use of quantum states for the detection of particles and Dark Matter searches. Despite the advancements of the last decade, there is still ample room for new experiments and a pressing need for improvements. Adopting elements from Superconducting Radiofrequency technologies will help to push the frontier of this field. In this talk I will introduce the concepts of Quantum Information science and discuss why the field would benefit from SRF technologies and how the combination of SRF technologies and Quantum Information science leads to new enabling technologies for example for Dark Matter searches."
24 Sep

Pushing for a Precise Mass Measurement of Tin-100 and the Development of a Next Generation MR-ToF Device for the Facility for Rare Isotope Beams

24 September 2024 - 2:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Christian Ireland

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Committee: Ryan Ringle (Chairperson), Marcos Caballero, Steven Lund, Jaideep Singh, Artemis Spyrou, Christopher Wrede
25 Sep

Exploring the Dynamics of Low-Energy Nuclear Reactions

25 September 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
Vanderbilt

Sait Umar

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Quasifission and multi-nucleon transfer reactions have been of great interest in recent years particularly in connections with the formation of superheavy elements and a source for producing neutron rich nuclei. Such reactions proceed through regions of the periodic table where the dynamical evolution of quantal shell effects influence the formation of final fragments. The time-dependent density functional theory (TDDFT) and its extensions has been found to be an excellent theoretical tool to study these reactions microscopically. TDDFT provides a detailed account of the evolving nuclear density, offering insights into key aspects of quasifission, such as the timescales involved, the mass and charge distribution of fragments, and the impact of shell effects. In this talk, we discuss the results for quasifission reactions obtained using the TDDFT and its extensions. In, particular we focus on the observed shell effects in these calculations and their relevance and/or relationship for shell effects observed in fission.
27 Sep

Aeos Project: Simulating Stellar Chemical Abundances and Galaxy Formation in the Early Universe

27 September 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
Harvard University

Kaley Brauer

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The chemical signatures of the earliest stars hold critical clues to nucleosynthetic processes and galaxy formation in the early Universe. The Aeos project presents a series of high-resolution cosmological simulations that model star-by-star chemical enrichment and galaxy formation within the first ~300 Myr. With 1 pc resolution, these simulations offer insights into the spread of stellar chemical abundances observed in dwarf galaxies, the effects of metal mixing in the interstellar medium, and feedback from Population III stars. Our comparisons with lower-resolution simulations demonstrate the importance of modeling individual stars to capture the formation and evolution of the smallest galaxies, with Aeos resolving galaxies as small as 10-100 solar masses. Additionally, we explore how variations in the Population III initial mass function (IMF) significantly influence ionization history and galaxy formation, with higher Pop III characteristic masses leading to fewer small galaxies. Aeos also reveals the interconnected nature of early galaxies, where metal enrichment from more massive galaxies impacts their neighbors. Future work will extend the simulations to the epoch of reionization, offering deeper insights into the processes shaping ultra-faint dwarf galaxies and their stellar populations.
30 Sep

Exploration of Above-Barrier Coulomb Excitation Using the JANUS Setup

30 September 2024 - 2:30 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Joseph Chung-Jung

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Committee: Alexadra Gade (Chairperson), Heiko Hergert, Mehr Nisa, Carlo Piermarocchi, Remco Zegers
02 Oct

Connecting quarks to the cosmos: the role of quark masses

02 October 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
University of Washington

Sanjay Reddy

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Theorists have wondered how variations in the quark mass would impact nuclear physics and have addressed how Big Bang nucleosynthesis can constrain such variation in the early universe. In my talk, I highlight more recent work inspired by these earlier studies that elucidate the role of the quark mass in low-energy nuclear physics. I show that understanding the quark mass dependence of the nuclear force has implications for three-nucleon forces in nuclei and neutron stars, the interpretation of pionic atoms, and axion condensation at finite baryon density.
04 Oct

High gradient SRF Travelling-Wave Acceleration Structure for Linear Colliders

04 October 2024 - 3:00 PM
1200 FRIB Laboratory and Online via Zoom
FermiLab

Vyacheslav P. Yakovlev

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A niobium-based superconducting standing-wave RF structure has an acceleration gradient limited to about 50 MV/m by the critical RF magnetic field. To overcome this barrier, we investigate a variant of niobium-based traveling-wave (TW) structures. It is shown that the TW structure can have an acceleration gradient above 70 MV/m, which is about 40% higher than that of state-of-the-art standing-wave structures with the same critical magnetic field. The implementation of this work opens the way to upgrade the energy of the International Linear Collider well beyond 1 TeV. The challenges and progress in the development of the TW SRF are presented, as well as the first experimental results for a prototype TW SRF cavity with a feedback waveguide. A traveling wave is demonstrated for the first time in an SRF cavity at 2K.
04 Oct

Sergei Kvitko Performing the Works of Franz Schubert

04 October 2024 - 5:30 PM
1300 FRIB Laboratory
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Performer Bio

Sergei Kvitko’s career is as diverse as it is successful. As a pianist, Mr. Kvitko has captured the attention of music critics with his “polished pianism… glorious Horowitzian three-dimensional perspective” (Gramophone Magazine), “masterful, intuitive playing… arresting artistry…  an iconoclastic sense for rubato rhythm and phrasing”  (Fanfare Magazine), and has been praised for his “luminous touch… warm, round sound… plenty of brilliance” as well as “a natural, appealing musicality and sensual understanding of piano tone” (The Chronicle-Herald).  The American Record Guide placed his recording of Mussorgsky’s Pictures at an Exhibition “among the best ever made” and included it on its coveted Critics’ Choice List. His critically acclaimed 2021 CD “Mozart. Post Scriptum” with Madrid Soloists Chamber Orchestra was praised as “an absolute explosion of creativity for Mr. Kvitko” (EarRelevant, Atlanta). The album has also won The American Prize in Piano Performance (Concerto). His 2023 album “Schubert by Candlelight: Live in Madrid” was released by Reference Recordings label and received such accolades as “beautifully executed and easily joins the best currently available” (American Record Guide) and “outstanding recital… ranked among the best Schubert piano releases in years” (Fanfare Magazine). In 2013, Kvitko made his New York City debut with a solo recital at Carnegie Hall that “was met with rousing applause, bravos, and a standing ovation” (New York Concert Review). He made solo, chamber and orchestral appearances in the United States, Canada, Ireland, Spain, Italy, Austria, Russia, Ukraine, Kazakhstan, and Uzbekistan.

As a composer, he gathered multiple awards for his incidental music for the production of Steven Dietz’s play “Dracula.” Lawrence Cosentino of City Pulse wrote: “Kvitko wove a borderline insane level of care and sophistication into every bar of his score even when you can barely hear it,” and Fanfare Magazine called it “a well-conceived, executed, and imaginative score… entertaining, powerful, witty.” Other compositions include incidental music for Tennessee Williams’ play “The Glass Menagerie” as well as many transcriptions and arrangements. His cadenzas for Mozart’s Concerto in D Minor were called “spectacular, to say the least” (Pizzicato Magazine, Germany)

What makes Kvitko’s career truly unique, is that his artistic accomplishments are balanced by his reputation as an internationally sought-after classical recording engineer and producer of the highest caliber, declared by Fanfare Magazine as “one of the best in the business,” and dubbed a “recording wizard” by New York Concert Review. Gramophone Magazine stated that “as engineer, he makes magic,” while American Record Guide praised his work as a ”consistent stream of exceptionally enjoyable recordings.” He is a Latin Grammy-nominated producer in Best Classical Album category. His recording of Carter Pann’s piece Mechanics was a finalist for Pulitzer Prize in Music. CDs produced and engineered by Sergei Kvitko have been favorably reviewed by national and international publications such as Fanfare Magazine,  BBC Music, Flute World, Clarinet Magazine, Clavier, Percussion and Strings Magazine among many others, earning praises such as “superbly well recorded” (International Record Guide, UK), “vividly detailed, vibrant sonics” (Gramophone, UK), “beautifully balanced and warmly atmospheric” (Gramophone, UK),  “the recording is close to ideal – rich, but clear, truthful and immediate” (American Record Guide), “larger-than-life recording that sounds fabulous at virtually any volume level” (Strings Magazine), “warm and immediate sound” (The Strad).

Sergei Kvitko was born in Russia and began studying music at the age of six. After receiving the highest musical education there, he came to the United States to pursue a Doctor of Musical Arts degree at Michigan State University, where he studied with Ralph Votapek. He is a voting member of the National Academy of Recording Arts and Sciences (GRAMMY).

07 Oct

AI-ML Tools for Heavy-Ion Linac Operations*

07 October 2024 - 3:00 PM
1200 FRIB Laboratory and Online via Zoom
Argonne National Laboratory

Brahim Mustapha

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At a heavy ion linac facility, such as ATLAS at Argonne National Laboratory, a new ion beam is tuned once or twice a week. The use of machine learning can be leveraged to streamline the tuning process, reducing the time needed to tune a given beam and allowing more beam time for the experimental program. After establishing automatic data collection and two-way communication with the control system, we have developed and deployed machine learning models to tune and control the machine. We have successfully trained online different Bayesian Optimization (BO)-based models for different sections of the linac, including the commissioning of a new beamline. We have demonstrated transfer learning from one ion beam to another allowing fast switching between different ion beams. We have also demonstrated transfer learning from a simulation-based model to an online machine model and using Neural Networks as prior-mean for BO optimization. Following a first failed attempt to deploy Reinforcement Learning (RL), we have succeeded in training multiple RL models online. More recently, these models are being generalized to other sections of the ATLAS linac and can, in principle, be adapted to control other ion linacs and accelerators with modern control systems.

 

* This work was supported by the U.S. Department of Energy, under Contract No. DE-AC02-06CH11357. This research used the ATLAS facility, which is a DOE Office of Nuclear Physics User Facility. Project funded through a “Data, Artificial Intelligence, and Machine Learning at DOE Scientific User Facilities” Grant from the DOE’s Office of Nuclear Physics.

11 Oct

CARME@CRYRING - Nuclear reaction measurements using stored ions

11 October 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
University of Edinburgh

Jordan Marsh

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In the last decade, improvements in ring operations and beam intensities at storage ring facilities have opened the door to performing nuclear reaction measurements using stored heavy ion beams. Using this technique, ions are stored in the ring for times ranging from a few seconds to several minutes, depending on the ion species and energy. Nuclear reactions occur by the interaction between the stored ions and an ultra-thin gas-jet target every revolution around the ring. The CRYRING Array for Reaction MEasurements (CARME) is a charged particle detector array recently commissioned at the CRYRING storage ring, designed to study direct nuclear reactions at stellar energies in addition to indirect studies of key nuclear properties with consequences for quiescent and explosive stellar environments. The CRYRING is a low energy storage ring located at GSI (Darmstadt) which is unique worldwide by allowing ion beams produced by a radioactive beam facility (FAIR) to be decelerated, cooled and circulated at energies of astrophysical interest. CARME utilises high resolution (~30 keV FWHM), highly segmented (128x128 strip) Double-Sided Silicon Strip Detectors (DSSSD) installed directly under extreme high vacuum (10-12 mbar) to detect reaction products. I will present recent advances in nuclear reaction measurements using stored ions and in particular, details and technical capabilities of the CARME array. CARME is a significant part of the UK in-kind contribution to FAIR. CARME’s science programme will be supported by the ERC-STG grant ELDAR, PI Dr. C Bruno (U. Edinburgh)
15 Oct

Process Design and Analysis of a Cryogenic Freeze-Out Heat Exchanger for Helium Purification

15 October 2024 - 10:00 AM
3405 Engineering Building and Online via Zoom
FRIB Graduate Research Assistant

Duncan Kroll

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Committee: Abraham Engeda, Nusair Hasan
15 Oct

Shell Model Nuclear Level Densities and their Applications to Astrophysics

15 October 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
Grand Valley State University

Sofia Karampagia

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Attempts to calculate the nuclear level densities are hardly a new field of study in nuclear physics. In his 1936 work, Bethe was already attempting to determine the density of energy levels near neutron separation energies. Over the following decades, various phenomenological models were developed, many of which are still in use today, for predicting level densities. In the last two decades, methods using the Skyrme and Gogny interactions within the Hartree-Fock-Bogoliubov mean-field framework have provided estimates of level densities for thousands of nuclides. Monte Carlo shell model calculations now enable predictions of nuclear level densities for medium and heavy nuclei. The wide array of models developed, and the ongoing advancement of new methods, underscore the importance of accurately predicting nuclear level densities, as this knowledge is critical for modelling nuclear reactions at energies beyond the low-lying discrete levels. Here, we present a statistical approach to estimating nuclear level densities based on the shell model and apply this method to theoretical calculations of neutron capture reaction cross-sections, which are vital for astrophysical applications.
16 Oct

Proton and Neutron Contributions for Cross-Shell Excitations Near Doubly Magic Calcium-40 Studied by Lifetime Measurements of Mirror Transitions

16 October 2024 - 2:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Andrew Sanchez

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Committee: Hironori Iwasaki (Chairperson), Katharina Domnanich, Dean Lee, Sean Liddick, Stuart Tessmer. Thesis is available @ https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name
16 Oct

Threshold effects in stellar reaction processes

16 October 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
Notre Dame

Michel Wiescher

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This talk will discuss a number of pronounced single particle and alpha cluster phenomena that emerge due to quantum coupling effects near the particle threshold and may exhibit substantial influence on low energy proton and alpha capture reactions in stellar hydrogen and helium burning environments. The possible consequences of these threshold features will be discussed for a number of nucleosynthesis environments.
17 Oct

Public Talk Featuring Jan Gordon, Author of "All The Ways You Taught Us"

17 October 2024 - 5:30 PM
1300 FRIB Laboratory
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Abstract

From the speaker:

“A few years ago, I began to write about my parents, Mort and Bernice Gordon, to solve the mystery of their remarkable partnership. My father, a blind physicist, and my mother, his reader, who lived with spina bifida, were bound together by love and necessity decades before recognition of their rights as disabled people. I explored their letters, interviewed Dad’s colleagues, searched for his publications, and listened to audio tapes of their work. As I revisited the scenes we shared, I developed a new understanding of how and what they taught me; my sister, Anne; his students; and their community.

Mort Gordon was a college student during World War II, when he learned that he was going blind from retinitis pigmentosa. Then Mort made two important decisions: he began studying physics, and he courted and married Bernice Rubinstein. These choices enabled him to contribute to the world of accelerator physics and raise a family. Mort, as a new PhD, faced discrimination because of “decreased vision,” then worked on an innovative cyclotron project at Oak Ridge National Laboratory, which led him to take a job at Michigan State University and create something new.  Mort and Bernice Gordon ingeniously found ways for the professor to teach his classes, develop the mathematics and computer models essential for MSU’s innovative cyclotrons, and share knowledge with colleagues around the world. Their story lives at the intersection of disability history and physics history. It illuminates the importance of sustained curiosity and the benefits of persistence, mentoring, and collaboration.”

Bio

Janet Gordon grew up in East Lansing, Michigan, and graduated from the University of Michigan in 1974, with aspirations to make the world better. She received an MA in business administration from George Washington University.  As a federal banking regulator, she developed guidance on the Community Reinvestment Act, which encourages banks to serve low- and moderate-income communities. As Associate Director of Community Affairs at the Federal Deposit Insurance Corporation, Janet improved consumer education to better serve people with disabilities. After retiring in 2018, Janet studied writing at The Writer’s Center in Bethesda, Maryland, and Politics and Prose bookstore in Washington, D.C. In All the Ways You Taught Us, A Memoir of Ability, Disability and the Pursuit of Meaning, she chronicles lessons about inquiry, disability, and meaningful living learned from Mort and Bernice Gordon’s remarkable lives.

Morton M. Gordon and Bernice Gordon

Morton M. Gordon (1924-2012), born in Atlantic City, New Jersey, attended Rutgers University, graduated from the University of Chicago, and received a PhD in physics from Washington University in 1950. Mort was instrumental in the design of a new breed of cyclotrons. By the time he arrived at Michigan State University in his thirties, he was almost completely blind from retinitis pigmentosa. Nonetheless, in 1959 he was the second person hired to design the first particle accelerator at MSU’s Cyclotron Laboratory. Mort was the principal theoretical physicist guiding the mathematics and computer models essential to its development. He continued his contributions at the National Superconducting Cyclotron Laboratory until 1999. He was a professor of physics for 50 years, and his students went on to help build accelerators all over the world. Mort’s principal collaborator in life, Bernice Gordon (1928-2007), also grew up in Atlantic City and graduated from the New Jersey College for Women in 1950. Bernice was born with spina bifida, which slowly reduced her mobility over the course of her life. In addition to a half century of service as Mort’s dedicated (and unpaid) reader, she was a political organizer, a participant in the Lansing area Jewish community, and a lover of literature who influenced the reading of her family and members of her book clubs. Mort and Bernice Gordon raised two daughters and left legacies for the next generations.

18 Oct

Radio-Frequency Superconductivity R&D at Fermilab for Accelerators and Quantum Applications

18 October 2024 - 3:00 PM
Online via Zoom
Fermi National Accelerator Laboratory

Daniel Bafia

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This presentation will highlight recent R&D efforts at Fermilab focused on niobium superconducting radio-frequency (SRF) cavities for both particle accelerator and quantum information science applications. It will present new insights into how various surface processing techniques have enhanced Nb SRF cavity performance, resulting in higher quality factors and accelerating gradients by integrating cryogenic RF measurements with advanced materials science. Additionally, these resonant structures provide a deeper understanding of the mechanisms limiting quantum coherence times in 2D and 3D quantum computing architectures. By simplifying complex multi-layer devices into single-interface systems, Fermilab has identified key sources of loss, such as amorphous native niobium oxide and dielectric substrates. These findings have aided in the development of quantum bits with record-breaking coherence times and thus advancing the field of quantum information science.
24 Oct

The Syntax of Science

24 October 2024 - 5:10 PM
1300 FRIB Laboratory

Violeta Lopez Lopez

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Join us as we search for artistic meaning in the atomic building blocks of the Universe using syntax on October 24 from 5:10-6:30PM at the Facility for Rare Isotope Beams. MSUFCU Arts Power Up Artist-in-Residence Violeta López López will explore the intersection of art, science, and language with Artemis Spyrou, Professor of nuclear astrophysics at the Facility for Rare Isotope Beams (FRIB), and Brian Buccola, Assistant Professor of linguistics and semantics in the Department of Linguistics, Languages, and Cultures. The discussion and audience Q&A will be moderated by Megan Halpern, Associate Professor of science, technology, and society and Director of the Center for Interdisciplinary Research, Collaboration, Learning, and Engagement (CIRCLE).
25 Oct

The Origin of the Heaviest Elements

25 October 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
North Carolina State University

Ian Roederer

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Understanding the origin of the elements remains one of the major challenges of modern astrophysics. I will introduce some of the big, open questions in the field and present several major advances from recent years. These advances include measuring the most complete heavy element chemical inventory beyond the Solar System and the first detection of transuranic fission fragments in stars. These advances can help shape the experiments carried out by future space flagship missions in the 2030s and 2040s, rare isotope facilities, and shape our understanding of our own cosmic origins.
25 Oct

Ab initio lattice Monte Carlo simulations of quantum many-body systems

25 October 2024 - 3:00 PM
1221A and 1221B FRIB Laboratory
University of Bonn

Avik Sarkar

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Nuclear lattice simulations using chiral Effective Field Theory (EFT) and auxiliary-field Monte Carlo have been a powerful and efficient ab initio tool in studying quantum many-body systems. However, these calculations usually suffer from severe sign oscillation problems, where the positive and negative contributions cancel each other, slowing down the Monte Carlo calculations. I will talk about two ways we can deal with the sign oscillation problem. First is the floating-block method, which allows us to use Eigenvector Continuation (EC) to extrapolate from a regime where the sign problem is small to the interaction where direct computation is impossible. Second, is the wavefunction matching method, where we perform a unitary transformation on our high-fidelity Hamiltonian so that the resulting wavefunction matches up to some finite range to a wavefunction corresponding to an easily computable Hamiltonian. We perform our calculations with the easily computable Hamiltonian and then perturbatively calculate the correction. With wavefunction matching, we can calculate up to Next-to-Next-to-Next Leading Order (N3LO) in our chiral EFT framework. Then, I will discuss the Adiabatic Projection Method (APM), which allows us to study scattering problems using lattice quantum Monte Carlo simulations. With wavefunction matching and APM, we study the alpha-alpha scattering at N3LO and find consistent results.
28 Oct

Dense Matter Equation of State from Nuclear Theory and Experiments

28 October 2024 - 8:00 AM
1221A and 1221B FRIB Laboratory
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We are excited to announce the upcoming collaborative workshop organized by IRL NPA (In2p3/FRIB) and taking place from Oct 28 to Nov 1 at FRIB. The meeting will be aimed at gathering researchers from multiple communities interested in the nuclear matter equation of state (EOS): an area that is currently undergoing rapid development due to upcoming unprecedented experimental opportunities, notably at FRIB, and the advent of multi-messenger astronomical observations. The workshop will include discussions of the latest measurements from astrophysics and laboratory experiments, recent developments in ab initio calculations, and new results from dynamical models. A significant portion of the workshop will be used to form working groups devoted to well-defined and closely-connected challenges: 1. Studies of new observables, both from nuclear structure and nuclear dynamics, to obtain tighter constraints on the EOS. 2. Quantification of the theoretical uncertainties and theoretical errors, development of appropriate likelihood models for Bayesian estimation, and using emulators and other machine learning techniques. 3. Optimization of the comparison protocol between transport models and data, notably via a controlled estimation of the unmeasured theoretical parameters and cross-comparison of different experimental data sets. Following the working group sessions, we will reconvene to summarize the discussions, identify near-term research directions, and prioritize the topics for future endeavors. If applicable, emerging collaborative efforts will be formulated and timelines for obtaining and presenting results in a publication will be discussed.
29 Oct

Transport Model Based on Inputs from Chiral Effective Field Theory

29 October 2024 - 11:00 AM
1200 FRIB Laboratory
Texas A&M University

Che-Ming Ko

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Heavy ion collisions make it possible to study the properties of nuclear matter at high density. After briefly describing the history of heavy ion collisions, a short review on the determination of the equation of state of nuclear matter from heavy ion collisions will be given. These studied were based on the use of transport models with mean-filed potentials derived from phenomenological energy density functionals and nucleon-nucleon in-medium scattering cross sections fitted to observables measured in these collisions. Because of the recent advance in chiral effective nucleon-nucleon interactions and its successful applications to nuclear structure studies, where only sub-saturation densities are present, it is of great interest to test their predictions of nuclear matter properties at higher densities. As a first step in this direction, the χBUU model was developed in Ref. [1] by using a Skyre-type energy density functional that was constructed from fitting the nuclear equation of state and nucleon effective masses in asymmetric nuclear matter predicted by the two- and three-body chiral interactions. This energy density functional was shown to describe well the binding energies of finite nuclei and their dipole polarizabilities [2]. Work is in progress to replace the phenomenological nucleon-nucleon scattering cross sections used in χBUU with those calculated from chiral effective field theory for nuclear matter at various densities, isospin asymmetries, and temperatures. With such an extended χBUU model, one can then study heavy ion collisions at intermediate energies available at the FRIB without arbitrary parameters, which would provide the test of chiral nuclear interactions at higher densities as well as allow for more stringent constraints on the nuclear equation of state from the experimental data.
30 Oct

Tentative Thesis Title: Characterization of High Charge Electron Bunches in Radio-Frequency (RF) Systems

30 October 2024 - 2:00 PM
1309 FRIB Laboratory
FRIB Graduate Research Assistant

Timothy Suzuki

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Committee: Steven Lidia (Chairperson), Yue Hao, Chong-Yu Ruan, Hendrik Schatz, Stuart Tessmer, Wootton
01 Nov

Recent Advances in Compact Normal-Conducting Radiofrequency Linacs

01 November 2024 - 3:00 PM
1309 FRIB Laboratory
Northern Illinois University

Xueying Lu

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High-energy particle accelerators continue to play a pivotal role in advancing particle physics. Normal-conducting radiofrequency (NCRF) technology is essential in the development of compact and cost-effective accelerators with increased energy reach and intensity. NCRF linacs have seen remarkable progress in the accelerating gradient and RF-to-beam efficiency, and these advances are driven by new understanding of RF breakdown physics, innovative structure topologies and coupling schemes, advanced materials and fabrication techniques, and new operation regimes including operation at cryogenic temperatures, at various frequencies, and with nanosecond-long RF pulses. In this talk, I will review some recent progress in NCRF linac structures and discuss their synergies with advanced accelerator concepts. These recent advances have directly inspired several current linear collider options and compact light sources, which I will also introduce.
03 Nov

Utility-Scale Quantum Computers

03 November 2024 - 1:00 PM
Online via Zoom
Microsoft

Chetan Nayak

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Chetan Nayak is an American physicist and distinguished professor specializing in condensed matter physics and quantum computing. He is a Fellow of the American Physical Society. He is currently a Technical Fellow at Microsoft and a professor of physics at the University of California, Santa Barbara (UCSB). His research focuses on topological phases of matter, high-temperature superconductivity, the quantum Hall effect, and periodically-driven quantum systems. He leads quantum hardware development at Microsoft.
05 Nov

The Effects of Proto-Neutron Star Convection on the Dynamics and Nucleosynthesis of the Neutrino-Driven Wind

05 November 2024 - 2:00 PM
1300 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Brian Nevins

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Committee: Edward Brown (Chairperson), Sean Couch, Filomena Nunes, Joseph Rodriguez, Man-Yee (Betty) Tsang. Thesis is available @ https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name
06 Nov

Advances in Simulating Fermions on a Quantum Computer

06 November 2024 - 3:00 PM
1221 Conference Room and Online via Zoom
FRIB Graduate Research Assistant

Gabriel Given

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Committee: Dean Lee (Chairperson), Morten Hjorth-Jensen, Mohammad Maghrebi, Kei Minamisono, Daniel Stump. Thesis is available @ https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name
06 Nov

<p>Nucleon Transfer and the Two-Faced Nature of <sup>48</sup>K</p>

06 November 2024 - 4:10 PM
1200 FRIB Laboratory and Online via Zoom
University of Surrey UK

Wilton Catford

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Nucleon transfer reactions allow us to populate nuclear states with very specific structure in a very selective fashion. This makes the selected states relatively easy to identify and they are also the states that the shell model should be most successful in describing - so these experiments allow us to test (and hence improve) the shell model and its extrapolations. This remains true, even if the precise value of the "spectroscopic factors" - that we use in describing the structure -  are a matter of some debate. The introductory part of the talk will examine the meaning of "spectroscopic factor", some of the challenges in deducing experimental values and the reasons for choosing  a pragmatic way forward. Some new experimental results for 48K will be described, recently obtained in an experiment with a reaccelerated beam of radioactive 47K from SPIRAL1 and a silicon array operated with the AGATA gamma-ray array and the VAMOS magnetic spectrometer. These new results greatly extend the knowledge of excited states in 48K, but also show up some interesting challenges due to the coexistence of two different proton configurations at the same excitation energies. Implications for ever-more-neutron rich nuclei will be discussed and finally a few features of the new FAUST array for transfer studies will be described.

07 Nov

25 Years of Technological Advancement in Radiation Oncology

07 November 2024 - 1:30 PM
1300 FRIB Laboratory and Online via Zoom
Mayo Clinic

Jon Kruse

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Jon Kruse got his Ph.D. in nuclear physics at the NSCL, and in February 1999 took a post doc in therapeutic medical physics at the Mayo Clinic in Rochester, MN. He’s been there ever since, and currently leads a group of over 20 physicists in the proton therapy practice. Over that 25-year period there have been several major technological advances in the field of radiation oncology. Jon will describe many of the innovations he’s witnessed and participated in throughout his career. These include image guidance, intensity modulated radiation therapy, the proliferation of particle beams, and treatment of non-malignant conditions such as ventricular tachycardia. This talk will portray the technological landscape of radiation oncology and give some insights into what a career in medical physics may look like.
08 Nov

The Big Bang Nucleosynthesis - How to cook your elements quicker than instant noodles

08 November 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
University of Padova, Italy

Steffen Turkat

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In this seminar we will dive into the first minutes of our universe focusing on a unique period known as Big Bang Nucleosynthesis: After one second, the universe had already cooled down sufficiently to allow protons and neutrons to remain stable particles. However, temperatures were still high enough to allow nuclei to overcome each others Coulomb barrier and therefore enables the formation of the first light elements. Investigating this era, i.e. its relevant nuclear reactions, is providing a main pillar in our understanding of today’s elemental abundance in the universe. We will explore this crucial era in more depth and discuss its impact for the upcoming 13.8 billion years. Furthermore, we will investigate the deuterium bottleneck and the baryon-to-photon ratio, which are also pivotal for multiple other astrophysical fields. Last but not least, we will focus on the current experimental status in order to draw a picture of what we currently have: A rather precise, but not yet perfectly understood picture of the chemical evolution of our early universe.
11 Nov

Tentative Thesis Title: Damage Evolution Due to Heavy Ion Irradiation in Copper Based Alloys

11 November 2024 - 11:00 AM
1300 FRIB Laboratory
FRIB Graduate Research Assistant

Ethan Fletcher

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Committee: Steven Lidia (Chairperson), Carl Boehlert, Patrick Hurh, Hironori Iwasaki, Takuji Kanemura, Remco Zegers
12 Nov

Nuclear many-body structure and dynamics on quantum computers

12 November 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom

WeiJie Du

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Nuclear many-body problems are computationally challenging for classical computers. Quantum computing techniques hold the promise of solving these problems with efficiency. In this talk, we present our efforts to develop quantum algorithms for solving the structure and dynamics of nuclear many-body problems. We begin by discussing our development of Hamiltonian encoding schemes for many-fermion and many-boson systems. We then present our structure and dynamics solutions to nuclear many-body problems based on these Hamiltonian input schemes. We conclude with thoughts on potential future developments.
13 Nov

Isotopes in Motion

13 November 2024 - 11:00 AM
Wharton Center for Performing Arts
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Isotopes in Motion returns to Wharton Center for an exhilarating performance that combines dance, video, and physics. Featuring professional dancers and community members, The contributions of youth, women, and people of color in science will be presented through a diverse cast in age, ethnicity, and cultural backgrounds. This original work at the intersection of science and dance, at turns breathtaking and funny, highlights the wonders of science and illuminates the research at the Facility for Rare Isotope Beams (FRIB). Tickets to this performance will include pre and post-show activities exploring dance and physics along with the chance to tour FRIB.
13 Nov

Informing the Nation’s Leaders: How Physicists Can Inform National Security and Science Policy Decisions

13 November 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
Institute for Defense Analyses

Jaclyn Schmitt

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Federally funded research and development centers (FFRDCs) are a special type of research institution that arose out of the federal government’s efforts to recruit scientific and engineering talent during and after WWII. Today, FFRDCs provide capabilities that the government does not have in-house and that contractors cannot provide. The Institute for Defense Analyses (IDA) is a private, nonprofit corporation that manages three FFRDCs. This talk will generally describe the side of IDA’s work for the Department of Defense that is related to nuclear deterrence, including the study of nuclear policy, nuclear force structure, and nuclear enterprise data management and decision-making. This talk will also cover what working at IDA is like and how physicists’ experience and skills are relevant and important to accomplishing IDA’s mission.
14 Nov

Isotopes in Motion

14 November 2024 - 11:00 AM
Wharton Center for Performing Arts
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Isotopes in Motion returns to Wharton Center for an exhilarating performance that combines dance, video, and physics. Featuring professional dancers and community members, The contributions of youth, women, and people of color in science will be presented through a diverse cast in age, ethnicity, and cultural backgrounds. This original work at the intersection of science and dance, at turns breathtaking and funny, highlights the wonders of science and illuminates the research at the Facility for Rare Isotope Beams (FRIB). Tickets to this performance will include pre and post-show activities exploring dance and physics along with the chance to tour FRIB.
14 Nov

Of Equal Place: Isotopes in Motion

14 November 2024 - 7:30 PM
Wharton Center for Performing Arts
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Wharton Center Original Commission The captivating fusion of science and art, Of Equal Place: Isotopes in Motion, returns to Wharton Center. This dynamic multimedia experience transcends boundaries, intertwining the realms of nuclear physics and dance in partnership with the Facility for Rare Isotope Beams (FRIB) and Dance Exchange. This groundbreaking Dance Exchange work places people of color, women, and youth at the forefront, celebrating their contributions to both science and the arts. With an expanded cast of community partners and performers, Of Equal Place: Isotopes in Motion reshapes perceptions of who can dance and who can be a scientist. Audiences raved about the premiere performance: "The diversity of the dancers was inspiring." "Great way to provide access to the world of science for the non-scientist." "Love the integration of physics, music and dance, and the imagery projected." Don't miss this unforgettable experience that sparks curiosity, ignites the imagination, mixes humor and wonder, and redefines the boundaries of artistic and scientific expression. Sponsored by the Facility for Rare Isotope Beams at Michigan State University.

15 Nov

Paving the Way for Next-Generation Electron Accelerators at Argonne

15 November 2024 - 3:00 PM
Online via Zoom
Argonne National Laboratory

Philippe Regis Guy Piot

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Particle accelerators, especially those based on electron beams, play a vital role in advancing both fundamental research and broader societal applications. In fundamental research, electron beams serve as primary tools to probe quantum materials through, e.g., electron microscopy and explore the fundamental structure of the universe in high-energy particle colliders. Additionally, electron beams are commonly used to generate photon beams over a broad range of energies in storage-ring-based light sources and free-electron lasers, enabling cutting-edge studies across various scientific fields.


At Argonne National Laboratory, several electron-beam facilities provide valuable resources for research and development. These facilities include user-serving centers like the Advanced Photon Source and the Electron Microscopy Center, as well as R&D-focused installations like the Argonne Wakefield Accelerator and the Linac Extension Area, which support the development of next-generation accelerators.


This presentation will offer an overview of ongoing and planned accelerator R&D efforts that will advance research in Basic Energy Sciences, Nuclear Physics, and High-Energy Physics. Additionally, it will highlight research opportunities in Accelerator Science & Engineering for Master's and Doctoral students interested in contributing to this exciting interdisciplinary field.

18 Nov

Jaideep Navigates a Travel Request on Concur!

18 November 2024 - 12:00 PM
1200 FRIB Laboratory and Online via Zoom
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“FRIB 101” is a new informal initiative to help make navigating the FRIB Laboratory a little bit easier. It is comprised of approximately a monthly brown bag lunch talk and a soon-to-be-launched internally-facing wayfinder to useful resources. The intended audience is any new hires as well as anyone curious about the people and processes conducted at the FRIB Laboratory. Please consider joining on your lunch, November 18, in the 1200 Lecture Hall or via Zoom to learn about Concur Travel Requests with a talk brought to you by Jaideep Taggart Singh.
20 Nov

Investigations on Lowering Surface Resistance of Medium-Frequency and -Beta Superconducting Elliptical Cavities

20 November 2024 - 3:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Associate

Sean Moskaitis

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Committee: Peter Ostroumov (Chairperson), Sergey Baryshev, Paul Gueye, Sang-hoon Kim, Chong-Yu Ruan Brad Sherrill.
20 Nov

Gravitational-wave Astrophysics: Taking Advantage of Nature's Hadron Collider

20 November 2024 - 4:10 PM
1300 FRIB Laboratory and Online via Zoom
California Institute of Technology

David Reitze

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Since the first direct detection of gravitational waves in 2015 from a pair of merging black holes, gravitational-wave astrophysics is opening a new window to the high energy universe. In particular, the simultaneous observation of the colliding binary neutron star system GW170817 in the gravitational wave and electromagnetic sectors produced fundamental insights into (among many other things) the nature of the neutron star equation of state and r-process nucleosynthesis. This talk will cover the fundamentals of gravitational-wave detectors and how they work as well as present recent highlights from LIGO-Virgo-KAGRA observing runs with an emphasis on discoveries associated with GW170817. Time permitting, we'll look at the future generation of gravitational-wave observatories being planned for the next decade.
22 Nov

Dvorak String Quintet No. 1 and Bax Oboe Quintet.

22 November 2024 - 5:30 PM
1300 FRIB Laboratory
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String Quintet No. 1 in A minor, Op. 1 (B. 7) Antonin Leopold Dvorak (1841 – 1904) I. Adagio — Allegro ma non troppo II. Lento Lyudmila Gofurova and You-Jung Hsu, violin; Madison Hilborn, viola; Weian Gu, cello; Shaun Rogers, double bass Oboe Quintet, GP 258 (1922) Arnold Bax (1883 – 1953) Movement One: Tempo molto moderato-Allegro moderato Movement Two: Lento espressivo Movement Three: Allegro giocoso John DeBiase, oboe; Yulin Zhou and Chonghua Zuo, violin; Mengyuan Song, viola; Weigen Jiang, cello
24 Nov

Searching for Dark Matter with the Universe's Highest-Energy Light

24 November 2024 - 1:00 PM
Online via Zoom
Massachusetts Institute of Technology

Tracy Slatyer

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Gamma rays, with frequencies billions of times higher than visible light, provide a window on extremely energetic astrophysical processes occurring in our Milky Way Galaxy and beyond. At the same time, the mysterious dark matter of the universe could imprint a range of clues to its existence in the gamma-ray sky. Disentangling the two isn't always easy, but I will discuss how scientists try to distinguish possible dark matter signals from high-energy astrophysics, what we are currently seeing in the data, and what new clues the next generation of gamma-ray telescopes are expected to provide. Prof. Slatyer is a theoretical physicist who works on particle physics, cosmology and astrophysics. Her research is motivated by questions of fundamental particle physics — in particular, the nature and interactions of dark matter — but she seeks answers to these questions by studying possible signatures of new physics in astrophysical and cosmological data. Her particular areas of focus include research into scenarios where the dark matter experiences new forces of nature, precision theoretical predictions for photon signals from heavy colliding dark matter particles, modeling of the possible effects of dark matter interactions on the history of the early cosmos, and hands-on data analysis of high-energy gamma-ray data in search of dark matter signals. She was a co-discoverer of the giant gamma-ray structures known as the “Fermi Bubbles” erupting from the center of the Milky Way. Prof. Slatyer was born in the Solomon Islands and grew up in Australia and Fiji. She completed her undergraduate work with honors in theoretical physics at the Australian National University in 2005 and her doctoral work in physics at Harvard in 2010 under the direction of Prof. Douglas Finkbeiner. Prof. Slatyer was a postdoctoral researcher at the Institute for Advanced Study in Princeton from 2010-2013, and joined the MIT Physics Department as a junior faculty member in July 2013. She was promoted to Associate Professor in 2018 and received tenure in 2019.
25 Nov

Tentative Thesis Title: Study of Shape and Shell Evolution Across N = 20 in Mg Isotopes Using Missing Mass Spectroscopy

25 November 2024 - 1:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Till Schaeffeler

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Committee: Daniel Bazin (Chairperson), Norman Birge, Scott Bogner, Carl Schmidt, Remco Zegers.
03 Dec

Reaction Dynamics In Time-Dependent Density Functional Theory

03 December 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
FRIB / Michigan State University

Kyle Godbey

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Reaction studies between heavy ions at low energies encode an incredible amount of information on the structure and dynamics of atomic nuclei. The relatively slow reaction processes explored at these near-barrier energies give the colliding nuclei time to deform, excite, and transfer particles, making them an excellent probe of self-bound quantum many-body systems. This talk will highlight studies spanning heavy-ion fusion, quasifission, and fission using time-dependent desntiy functional theory -- a time-dependent many-body method that simulates the real-time dynamics of the colliding nuclear system. Various challenges and limitations will be presented, along with potential future directions for more robust models of nuclear dynamics.
06 Dec

Indirect and direct measurements for the s-process

06 December 2024 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
Texas A&M University

Philip Adsley

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Nuclear physics provides vital inputs into understanding the chemical evolution of the universe. Thermonuclear reaction rates strongly depend on nuclear data such as the properties of nuclear states. In this talk, I will discuss how information about important nuclear states can be determined using experiments with stable beams with a focus on the s-process. The s-process depends sensitively on how many neutrons are available for the synthesis of new elements. This means that we must know how many neutrons are made and how many are absorbed by poisons. I will briefly review the state of neutron production in the burning of neon-22 and discuss some interesting recent results on neutron recycling in helium-induced reactions on oxygen-17.
06 Dec

Tentative Thesis Title: A search for Hoyle-like Analogous States in Oxygen-16 and Magnesium-24 with the AT-TPC Data Using Machine Learning Methods

06 December 2024 - 3:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Pranjal Singh

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Committee: Daniel Bazin (Chairperson), Christopher Baldwin, Dean Lee, Carl Schmidt, Remco Zegers.
06 Dec

Quantum microscopes to search for new elementary particles and forces

06 December 2024 - 5:30 PM
1300 FRIB Laboratory
Johns Hopkins University & University of Chicago

David DeMille

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Abstract for the public talk: All elementary particles and forces seen in laboratories are described by a mathematical framework known as the Standard Model. However, some cosmological observations show that there also must be new, additional particles and forces. Traditionally, physicists have searched for these using huge accelerators and giant detectors. However, certain types of new particles and forces can be detected in a very different way: the laws of quantum physics dictate that their existence will modify the properties of ordinary matter in subtle but distinctive ways. These tiny effects can be detected with experiments, small enough to fit in a garage, which use methods of ultra-precise quantum measurements to search for particles that cannot be produced even at the Large Hadron Collider. This talk will describe such experiments and the concepts behind them.
08 Dec

Representing the visual world

08 December 2024 - 1:00 PM
Online via Zoom
University of California Berkeley

Doris Tsao

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How does the brain represent the visual world? Research on how the primate brain represents faces has given us a remarkable window into the processes underlying visual perception. In my talk, I will discuss the organization and feature code used by the brain's system for representing faces, the way the system represents memories, and how the system has provided a model for clarifying how the brain represents objects in general. Registration link https://msu.zoom.us/webinar/register/WN_53mINy2qR5GKxkE2yEJoQA
12 Dec

Extending the In-Medium Similarity Renormalization Group to Nuclear Matter with Novel Insights on Unitary Coupled-Cluster Theory

12 December 2024 - 9:00 AM
1300 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Omokuyani Chibuzor Udiani

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Committee: Scott Bogner (Chairperson), Alexei Bazavov, Edward Brown, Morten Hjorth-Jensen, Dean Lee. Thesis is available @ https://pa.msu.edu/graduate-program/current-graduate-students/draft-dissertations-for-review.aspx - Select student name .
12 Dec

Tentative Thesis Title: Probing the Reduction Factor in 15C Single Nucleon Removal Transfer Reactions Using the AT-TPC

12 December 2024 - 4:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Nathan Turi

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Committee: Daniel Bazin (Chairperson), Norman Birge, Alexandra Gade, Dean Lee, Devin Silvia, Remco Zegers
13 Dec

Distributed Charge Compton Source And Medical Accelerator Technologies

13 December 2024 - 3:00 PM
Online via Zoom
Lumitron Technologies

Mitchell Shneider

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Across the world, accelerators are becoming more a part of the everyday life so there’s a significant effort to shrink the overall footprint of these accelerator system from national laboratory scale machines to a footprint that is reasonable for industrial and medical applications. At Lumitron Technologies we have developed an ultracompact high gradient accelerator. Operating at X-band 11.424 GHz with a distributed charge architecture, this system can produce a high-flux, tunable, mono-energetic x-rays that are ideally suited for range of novel, medical and industrial imaging applications. The underlying electron beam used is also a suitable source of very high energy electrons (VHEE) for FLASH radiotherapy.
13 Dec

J.S. Bach (arr. A. Bartholdy) - Aria with 30 Variations (Goldberg Variations), BWV 988

13 December 2024 - 5:30 PM
1300 FRIB Laboratory
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A hallmark of the High Baroque era, Bach’s iconic keyboard masterwork presents 30 variations on a tuneful Aria, meandering through a mesmerizing mosaic of musical material while exploring a diverse array of styles from all corners of the Baroque aesthetic universe. In this stunning translation for string trio, each part in the three-voice texture finds an avatar in a string instrument, inviting the collaboration of three individuals to create a harmonious whole. Beginning and ending with the same Aria upon which each variation is based, the piece represents a perfect synchronism of vibrant multiplicity and steadfast, unchanging unity. Program: J.S. Bach (arr. A. Bartholdy) - Aria with 30 Variations (Goldberg Variations), BWV 988 Hayne Kim, violin Sophie Choate, viola Cody Byrum, cello The performance will run approximately one hour without intermission.
13 Dec

Bach Goldberg Variations BWV 988
Arranged for string by Annette Bartholdy

13 December 2024 - 5:30 PM
1300 FRIB Laboratory
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A hallmark of the High Baroque era, Bach’s iconic keyboard masterwork presents 30 variations on the bass line of an elegantly elaborated Aria, meandering through a mesmerizing mosaic of musical material while exploring a diverse array of styles from all corners of the Baroque aesthetic universe. In this stunning translation for string trio, each part in the three-voice texture finds an avatar in a string instrument, inviting the collaboration of three individuals to create a harmonious whole. Beginning and ending with the same Aria upon which each variation is based, the piece represents a perfect synchronism of vibrant multiplicity and steadfast, unchanging unity. J.S. Bach (arr. A. Bartholdy) - Aria with 30 variations (Goldberg Variations), BWV 988 Hayne Kim, Violin Sophie Choate, Viola Cody Byrum, Cello The performance will run approximately one hour without intermission
16 Dec

Tentative Thesis Title: Constraining the Neutron Capture Reaction on Zr Isotopes for Astrophysical Processes

16 December 2024 - 2:00 PM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Amal Sebastian

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Committee: Artemis Spyrou (Chairperson), Wade Fisher, Heiko Hergert, Wolfgang Kerzendorf, Sean Liddick.
19 Dec

Production of Vanadium-49, Arsenic-73, Lutetium-173 for Neutron-Induced Cross-Section Measurements

19 December 2024 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
FRIB Graduate Research Assistant

Chloe Kleinfeldt

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There is currently a deficiency in experimental neutron-induced cross-section measurements for many radionuclides, with theoretical predictions often exhibiting high uncertainties or considerable deviations from experimental data [1]. Direct cross-section measurements could improve current nuclear databases. For instance, several radioisotopes of vanadium [2], arsenic [3], and lutetium [4] were produced during underground nuclear tests, and while their transmutation properties are essential for interpreting the archival data, direct measurements of their neutron-reaction cross-sections have not been performed. To conduct these measurements, it is necessary to produce, purify, and fabricate suitable targets. Although production of many of the desired radionuclides is feasible, achieving the required quantity and isotopic purity can be challenging. This work explores the alternative production method of “isotope harvesting” to provide purified vanadium-49 (49V), arsenic-73 (73As), and lutetium-173 (173Lu) for target fabrication, all of which appear in important neutron-reaction networks from underground nuclear tests. Specifically, methods for solid-phase harvesting of 49V from proton- and deuteron-induced reactions for medical isotope production; solid-phase harvesting of 173Lu from a tungsten-alloy beam blocker from the recently decommissioned National Superconducting Cyclotron Laboratory; aqueous harvesting of 73As from a flowing water beam dump at its successor, the Facility for Rare Isotope Beams will be discussed.

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