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.
Novel evidence for the σ-bond linear-chain molecular structure in 14C
doi: 10.1088/1674-1137/ac04a0
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
Value-Assigned Pulse Shape Discrimination for Neutron Detectors
doi: 10.1109/TNS.2021.3091126
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
Supernova 1987A: 3D Mixing and Light Curves for Explosion Models Based on Binary-merger Progenitors
doi: 10.3847/1538-4357/abf4c5