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.
Spectroscopy of proton-rich 79Zr: Mirror energy differences in the highly-deformed fpg shell
doi: 10.1016/j.physletb.2020.135873
Harvesting 62Zn from an aqueous cocktail at the NSCL
doi: 10.1039/D0NJ04411C
RF deflecting cavity for fast radioactive ion beams
doi: 10.1140/epjti/s40485-020-00056-1
Predicting time to graduation at a large enrollment American university
doi: 10.1371/journal.pone.0242334
θ-dependence of light nuclei and nucleosynthesis
doi: 10.1103/PhysRevResearch.2.033392
Production, Collection, and Purification of 47Ca for the Generation of 47Sc through Isotope Harvesting at the National Superconducting Cyclotron Laboratory
doi: 10.1021/acsomega.0c03020
Figuring Out Gas & Galaxies in Enzo (FOGGIE). IV. The Stochasticity of Ram Pressure Stripping in Galactic Halos
doi: 10.3847/1538-4357/abc5b8
Environmental Dependence of Self-regulating Black Hole Feedback in Massive Galaxies
doi: 10.3847/1538-4357/abc33c
On the development of multidimensional progenitor models for core-collapse supernovae
doi: 10.3847/1538-4357/abada7
Process of equilibration in many-body isolated systems: diagonal versus thermodynamic entropy
doi: 10.1088/1367-2630/aba652
Reaction Rate Sensitivity of the Production of γ-Ray Emitting Isotopes in Core-collapse Supernovae
doi: 10.3847/1538-4357/abafb5
Tests of AGN Feedback Kernels in Simulated Galaxy Clusters
doi: 10.3847/1538-4357/abb08c