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.
Floating Block Method for Quantum Monte Carlo Simulations
doi: 10.1103/PhysRevLett.131.242503
Implementing an electronic sideband offset lock for isotope shift spectroscopy in radium
doi: 10.1364/OE.500578
The Standard Model Theory of Neutron Beta Decay
doi: 10.3390/universe9090422
Applications of Machine Learning and Neural Networks for FT-ICR Mass Measurements with SIPT
doi: 10.3390/atoms11100126
Status of CHIP-TRAP: The Central Michigan University High-Precision Penning Trap
doi: 10.3390/atoms11100127
Local Bayesian Dirichlet mixing of imperfect models
doi: 10.1038/s41598-023-46568-0
Elucidating the nature of the proton radioactivity and branching ratio on the first proton emitter discovered 53mCo
doi: 10.1038/s41467-023-39389-2
Colliding heavy nuclei take multiple identities on the path to fusion
doi: 10.1038/s41467-023-43817-8
Dilute neutron star matter from neural-network quantum states
A New Modeling Approach for a Priori Uncertainties of Laser Tracker Angle Measurements
doi: 10.1061/JSUED2.SUENG-1433
Seeking Self-regulating Simulations of Idealized Milky Way–like Galaxies
doi: 10.3847/1538-4357/accbb7
Impact of Pycnonuclear Fusion Uncertainties on the Cooling of Accreting Neutron Star Crusts
doi: 10.3847/1538-4357/acebc4
