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.
J/Ψ production cross section and its dependence on charged-particle multiplicity in p+p collisions at √s = 200 GeV
doi: 10.1016/j.physletb.2018.09.029
Rapid Neutrino Cooling in the Neutron Star MXB 1659-29
doi: 10.1103/PhysRevLett.120.182701
SYGMA: Stellar Yields for Galactic Modeling Applications
doi: 10.3847/1538-4365/aad691
Cyberhubs: Virtual Research Environments for Astronomy
doi: 10.3847/1538-4365/aab777
The fast linear accelerator modeling engine for FRIB online model service
doi: 10.1016/j.cpc.2018.07.013
Viscous-dynamical Ejecta from Binary Neutron Star Mergers
doi: 10.3847/2041-8213/aaf053
Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts, and Nucleosynthesis
doi: 10.3847/1538-4357/aaf054
New Thermonuclear 10B(α,p)13C Rate and Its Astrophysical Implication in the νp-process
doi: 10.3847/1538-4357/aae479
Metal Mixing and Ejection in Dwarf Galaxies Are Dependent on Nucleosynthetic Source
doi: 10.3847/1538-4357/aaec7d
New Thermonuclear 10B(α,p)13C Rate and Its Astrophysical Implication in the νp-process
doi: 10.3847/1538-4357/aae479
Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
doi: 10.3847/1538-4357/aadcf7
r-process Nucleosynthesis from Three-dimensional Magnetorotational Core-collapse Supernovae
doi: 10.3847/1538-4357/aad6ec