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.
Enhanced Electric Dipole Strength for the Weakly Bound States in 27Ne
doi: 10.1103/PhysRevLett.121.262501
Erratum: Observation of D0 Meson Nuclear Modifications in Au+Au Collisions at √sNN=200 GeV [Phys. Rev. Lett. 113, 142301 (2014)]
doi: 10.1103/PhysRevLett.121.229901
Low-pT e+e− Pair Production in Au+Au Collisions at √sNN=200 GeV and U+U Collisions at √sNN=193 GeV at STAR
doi: 10.1103/PhysRevLett.121.132301
From Calcium to Cadmium: Testing the Pairing Functional through Charge Radii Measurements of 100−130Cd
doi: 10.1103/PhysRevLett.121.102501
Extraction of the Landau-Migdal Parameter from the Gamow-Teller Giant Resonance in 132Sn
doi: 10.1103/PhysRevLett.121.132501
Cyberhubs: Virtual Research Environments for Astronomy
doi: 10.3847/1538-4365/aab777
The fast linear accelerator modeling engine for FRIB online model service
doi: 10.1016/j.cpc.2018.07.013
As a Matter of Force—Systematic Biases in Idealized Turbulence Simulations
doi: 10.3847/2041-8213/aac0f5
i-process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-peak Neutron-capture Elements
The Origin of r-process Elements in the Milky Way
doi: 10.3847/1538-4357/aaad67
Nuclear Reactions in the Crusts of Accreting Neutron Stars
doi: 10.3847/1538-4357/aabfe0
Validating Semi-analytic Models of High-redshift Galaxy Formation Using Radiation Hydrodynamical Simulations
doi: 10.3847/1538-4357/aabe8f