Facility acknowledgment for publications
All users are asked to submit information about their resulting publications to the FRIB Manager for User Relations (useroffice@frib.msu.edu). In the future, publication information will be entered on the FRIB Scientific User Portal.
To the extent possible, an acknowledgment of Federal support must appear in the publication of any material, whether copyrighted or not, based on or developed using FRIB resources, as follows:
- Acknowledgment: "This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics and used resources of the Facility for Rare Isotope Beams (FRIB) Operations, which is a DOE Office of Science User Facility under Award Number DE-SC0023633.”
Users must submit their publication information to the DOE Energy Link (E-Link) System.
Comparing proton momentum distributions in A = 2 and 3 nuclei via 2H 3H and 3He (e,e′p) measurements
doi: 10.1016/j.physletb.2019.134890
Constraining the Neutron Star Compactness: Extraction of the 23Al(p,γ) Reaction Rate for the rp Process
doi: 10.1103/PhysRevLett.122.232701
Direct Comparison between Bayesian and Frequentist Uncertainty Quantification for Nuclear Reactions
doi: 10.1103/PhysRevLett.122.232502
Azimuthal Harmonics in Small and Large Collision Systems at RHIC Top Energies
doi: 10.1103/PhysRevLett.122.172301
Direct Observation of Proton Emission in 11Be
doi: 10.1103/PhysRevLett.123.082501
Evidence for Rigid Triaxial Deformation in 76Ge from a Model-Independent Analysis
doi: 10.1103/PhysRevLett.123.102501
New Limit on the Permanent Electric Dipole Moment of 129Xe Using 3He Comagnetometry and SQUID Detection
doi: 10.1103/PhysRevLett.123.143003
Following the Cosmic Evolution of Pristine Gas. III. The Observational Consequences of the Unknown Properties of Population III Stars
doi: 10.3847/1538-4357/aafa1a
Neutron Star Mergers Might Not Be the Only Source of r-process Elements in the Milky Way
doi: 10.3847/1538-4357/ab10db
Figuring Out Gas & Galaxies in Enzo (FOGGIE). I. Resolving Simulated Circumgalactic Absorption at 2 ≤ z ≤ 2.5
doi: 10.3847/1538-4357/ab0654
Complex energies of open one-dimensional disordered wires
doi: 10.1016/j.physe.2019.02.015
New physics searches in nuclear and neutron decay
doi: 10.1016/j.ppnp.2018.08.002