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.
Evolution of shell structure in exotic nuclei
doi: 10.1103/RevModPhys.92.015002
Nurse-Reported Bullying and Documented Adverse Patient Events: An Exploratory Study in a US Hospital
doi: 10.1097/NCQ.0000000000000442
Mirror-symmetry violation in bound nuclear ground states
doi: 10.1038/s41586-020-2123-1
Two-neutron knockout as a probe of the composition of states in 22Mg,23Al, and 24Si
doi: 10.1103/PhysRevC.101.031303
As a Matter of State: The Role of Thermodynamics in Magnetohydrodynamic Turbulence
doi: 10.3847/1538-4357/ab5aec
Design of the multi-ion injector linac for the JLAB EIC (JLEIC)
doi: 10.1088/1742-6596/1401/1/012008
On Monolithic Supermassive Stars
doi: 10.1093/mnras/staa763
Calculating n-point charge correlations in evolving systems
doi: 10.1103/PhysRevC.101.014914
Ab initio short-range-correlation scaling factors from light to medium-mass nuclei
doi: 10.1088/1361-6471/ab6af7
3He-rich Solar Energetic Particle Observations at the Parker Solar Probe and near Earth
doi: 10.3847/1538-4365/ab5963
Measurement of the energy distribution of electrons escaping confinement from an electron cyclotron resonance ion source
doi: 10.1063/1.5129656
Bulk properties of the system formed in Au + Au collisions at √sNN=14.5 GeV at the BNL STAR detector
doi: 10.1103/PhysRevC.101.024905