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.
Hidden Spin-Isospin Exchange Symmetry
doi: 10.1103/PhysRevLett.127.062501
Rodeo Algorithm for Quantum Computing
doi: 10.1103/PhysRevLett.127.040505
Exascale models of stellar explosions: Quintessential multi-physics simulation
doi: 10.1177/10943420211027937
Improved wavelength meter calibration in near infrared region via Doppler-free spectroscopy of molecular iodine
doi: 10.1007/s00340-021-07650-5
Comprehensive analysis of beta decays within and beyond the Standard Model
doi: 10.1007/JHEP04(2021)126
FMX – the Frontier Microfocusing Macromolecular Crystallography Beamline at the National Synchrotron Light Source II
doi: 10.1107/S1600577520016173
Ne-22 Ion-Beam Radiation Damage to DNA: From Initial Free Radical Formation to Resulting DNA-Base Damage
doi: 10.1021/acsomega.1c01954
The Pair-instability Mass Gap for Black Holes
doi: 10.3847/2041-8213/abf2c4
On the Evolution of Supermassive Primordial Stars in Cosmological Flows
doi: 10.3847/1538-4357/abfaf9
Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
doi: 10.3847/1538-4357/abfb65
Stellar Mass Black Hole Formation and Multimessenger Signals from Three-dimensional Rotating Core-collapse Supernova Simulations
doi: 10.3847/1538-4357/abfb05
Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ~19 M⊙ Progenitor
doi: 10.3847/1538-4357/abf82e