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.
The (6Li,6Li∗[3.56MeV]) reaction at 100 MeV/u as a probe of Gamow-Teller transition strengths in the inelastic scattering channel
doi: 10.1103/PhysRevC.98.015804
Quenching of nuclear matrix elements for 0νββ decay by chiral two-body currents
doi: 10.1103/PhysRevC.98.031301
Non-perturbative collective inertias for fission: A comparative study
doi: 10.1016/j.physletb.2018.10.045
Bogoliubov many-body perturbation theory for open-shell nuclei
doi: 10.1016/j.physletb.2018.09.044
Collision energy dependence of moments of net-kaon multiplicity distributions at RHIC
doi: 10.1016/j.physletb.2018.07.066
From Calcium to Cadmium: Testing the Pairing Functional through Charge Radii Measurements of 100−130Cd
doi: 10.1103/PhysRevLett.121.102501
Finite-Temperature Relativistic Nuclear Field Theory: An Application to the Dipole Response
doi: 10.1103/PhysRevLett.121.082501
Localizing the Shape Transition in Neutron-Deficient Selenium
doi: 10.1103/PhysRevLett.121.082502
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
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