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.
Many-body correlations in nuclear superfluidity
doi: 10.1103/PhysRevC.102.034310
Process of equilibration in many-body isolated systems: diagonal versus thermodynamic entropy
doi: 10.1088/1367-2630/aba652
Spectroscopic Study of 39Ca for Endpoint Nucleosynthesis in Classical Novae
doi: 10.1088/1742-6596/1668/1/012025
Nucleon localization function in rotating nuclei
doi: 10.1103/PhysRevC.102.044305
Global description of β− decay with the axially deformed Skyrme finite-amplitude method: Extension to odd-mass and odd-odd nuclei
doi: 10.1103/PhysRevC.102.034326
Commissioning Status of the Linac for the Facility for Rare Isotope Beams
doi: 10.3938/jkps.77.344
Accessing the Single-Particle Structure of the Pygmy Dipole Resonance in 208Pb
doi: 10.1103/PhysRevLett.125.102503
A Black Hole Feedback Valve in Massive Galaxies
doi: 10.3847/1538-4357/aba42e
Isotopically resolved neutron total cross sections at intermediate energies
doi: 10.1103/PhysRevC.102.034601
Tests of AGN Feedback Kernels in Simulated Galaxy Clusters
doi: 10.3847/1538-4357/abb08c
Improved precision on the experimental E0 decay branching ratio of the Hoyle state
doi: 10.1103/PhysRevC.102.024320
On the development of multidimensional progenitor models for core-collapse supernovae
doi: 10.3847/1538-4357/abada7