Welcome to FRIB

The Facility for Rare Isotope Beams (FRIB) at Michigan State University (MSU) is a world-class research, teaching and training center, hosting the most powerful rare isotope accelerator. MSU operates FRIB as a user facility for the U.S. Department of Energy Office of Science (DOE-SC), with financial support from and furthering the mission of the DOE-SC Office of Nuclear Physics. FRIB allows MSU graduate students to engage in groundbreaking research in tandem with their coursework. Open the doors to discovery with the newest and most advanced rare isotope research facility and the world's most powerful rare isotope accelerator. Apply and inquire through FRIB’s graduate studies page at frib.msu.edu/grad.

29 Jan

From Tensor Current Limits to Solar Neutrinos: 8Li and 8B Studies with the Beta-decay Paul Trap

29 January 2025 - 3:30 PM
1300 FRIB Laboratory
Lawrence Livermore National Laboratory

Brenden Longfellow

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The vector – axial vector form of the electroweak interaction was established through pioneering beta-decay experiments in the 1960s and incorporated into the standard model of particle physics. However, there is no a priori reason that the other currents, scalar and tensor, could not be present. The Gamow-Teller beta decays of 8Li and 8B have extremely large Q values and the daughter nucleus in both cases, 8Be, is alpha unbound making these systems exemplary probes of the presence of any tensor contribution affecting the beta-neutrino angular correlation. The improvements from over a decade of high-statistics experiments on 8Li and 8B performed at Argonne National Laboratory using the Beta-decay Paul Trap (BPT) will be presented. In these measurements, the energies of the alpha and beta particles were determined using four 32x32 double-sided silicon strip detectors surrounding the BPT to precisely reconstruct the decay kinematics. The latest iteration of experiments has set the two world-leading limits on tensor currents from single beta-decay measurements. The combined BPT limits from 8Li and 8B for tensor coupling to right-handed neutrinos are comparable to a recent global evaluation of all other precision beta decay studies and are consistent with the standard model, relieving some existing tension. In addition, the high-energy neutrinos observed in solar neutrino astrophysics experiments on Earth predominately originate from 8B beta decay in the Sun. Results on determining the 8B neutrino energy spectrum, an important input for the astrophysics community, from the same data set will be discussed.

31 Jan

Pulsating massive stars as finely tuned instruments in the stellar symphony

31 January 2025 - 2:00 PM
2025 FRIB Laboratory and Online via Zoom
Newcastle University, UK

Dominic Bowman

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Massive stars are important metal factories in the Universe because through their winds and explosive deaths as supernovae they provide radiative, kinematic, and chemical feedback to their surroundings. However, stellar evolution models currently contain large theoretical uncertainties for physical mechanisms at work in the deep interiors of massive stars. The uncertainties associated with rotation, chemical mixing, magnetic fields, and angular momentum transport propagate throughout stellar evolution making it difficult to accurately determine stellar masses and ages. The analysis of pulsation frequencies in massive stars allows one to break model degeneracies, uniquely probe stellar interiors, and constrain uncalibrated physical processes within our models. In this seminar, I discuss the recent advances in our understanding of massive stars by means of asteroseismology – the study of stellar pulsations. Modern space telescopes have revealed diverse variability mechanisms in massive stars across different evolutionary stages, which includes the main sequence through to blue supergiant stars. This provides us with the opportunity to perform a data-driven calibration of evolution models for some of the most massive and short-lived stars in the Universe.
04 Feb

Scaling law of quantum entanglement in nuclear shell model

04 February 2025 - 11:00 AM
1200 FRIB Laboratory and Online via Zoom
Hohai University

Dong Bai

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Quantum entanglement represents a classically forbidden form of correlation shared between separate local subsystems. The atomic nucleus serves as an ideal platform for exploring quantum entanglement at subatomic scales. A key characteristic of quantum entanglement is its scaling behavior with respect to subsystem size. Motivated by a recent study [Gu et al., Phys. Rev. C 108, 054309 (2023)], I investigate the scaling behavior of orbital entanglement in nuclear shell model. The results show that the average orbital entanglement entropy follows a Page-like curve, consistent with volume law scaling, for both ground and excited states. This finding suggests the absence of an entanglement crossover from area law to volume law in the nuclear shell model, distinguishing it from typical condensed matter systems. Additionally, the influence of angular momentum conservation on orbital entanglement is examined.
07 Feb

TBD

07 February 2025 - 3:00 PM
Online via Zoom
Lawrence Berkeley National Laboratory

Damon Todd

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TBD
09 Feb

What can theoretical physics tell us about the origin and evolution of early life?

09 February 2025 - 3:00 PM
Online via Zoom
University of California San Diego

Nigel Goldenfeld

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Life on Earth is wonderfully diverse, with a multitude of life forms, structures and evolutionary mechanisms. However, there are two aspects of life that are universal - shared by all known organisms. These are the genetic code, which governs how DNA is converted into the proteins making up your body, and the unexpected left-handedness of the amino acids in your body. One would expect that your amino acids were a mixture of left and right-handed molecules, but none are right handed! In this talk, I describe how these universal aspects of biology can be understood as arising from evolution, but generalized to an era where genes, species and individuality had not yet emerged. I will also discuss to what extent one can find general principles of biology that can apply to all life in the universe, and what this would mean for the nascent field of astrobiology. Prof. Nigel Goldenfeld holds the Chancellor's Distinguished Professorship in Physics and joined UCSD in Fall 2021 after 36 years at the University of Illinois at Urbana-Champaign (UIUC). His research spans condensed matter theory, the theory of living systems, hydrodynamics and non-equilibrium statistical physics. He received his Ph.D in theoretical physics from the University of Cambridge (UK) in 1982, and for the years 1982-1985 was a postdoctoral fellow at the Institute for Theoretical Physics, University of California at Santa Barbara, where his work on the dynamics of snowflake growth helped launch the modern theory of pattern formation in nature. He joined the condensed matter theory group at the Department of Physics, UIUC in 1985, where his work was instrumental to the discovery of d-wave pairing in high temperature superconductors. In 1996, he co-founded NumeriX, a company that develops high-performance software for pricing and risk managing derivative securities. His interests in biology include microbial ecology, evolution and systems biology. He was a founding member of the Institute for Genomic Biology at UIUC, where he led the Biocomplexity Group and directed the NASA Astrobiology Institute for Universal Biology. During the COVID-19 pandemic, he pivoted from his experience in mathematical modeling of bacteria and viruses to computational epidemiology, advising the Governor of Illinois, and helping devise, set up and run the COVID saliva testing system at UIUC, which provided ~12 hour turnaround of PCR tests to the 50,000 people in the campus community and eventually to over 1700 schools and other institutions in Illinois and beyond. He has served on the editorial boards of several journals, including The Philosophical Transactions of the Royal Society, Physical Biology and the International Journal of Theoretical and Applied Finance. Selected honours include: Alfred P. Sloan Foundation Fellow, University Scholar of the University of Illinois, the Xerox Award for research, the A. Nordsieck award for excellence in graduate teaching and the American Physical Society's Leo P. Kadanoff Prize 2020. He is a Fellow of the American Physical Society, a Fellow of the American Academy of Arts and Sciences, a Fellow of the Royal Society (UK) and a Member of the US National Academy of Sciences.