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.
Precise comparison of the Gaussian expansion method and the Gamow shell model
doi: 10.1103/PhysRevC.89.044317
Astrophysical weak-interaction rates for selected A=20 and A=24 nuclei
doi: 10.1103/PhysRevC.89.045806
Baryon annihilation and regeneration in heavy ion collisions
doi: 10.1103/PhysRevC.89.044911
Quasiparticle coupled cluster theory for pairing interactions
doi: 10.1103/PhysRevC.89.054305
Neutrinoless double-β decay of 82Se in the shell model: Beyond the closure approximation
doi: 10.1103/PhysRevC.89.054605
Reexamining surface-integral formulations for one-nucleon transfers to bound and resonance states
doi: 10.1103/PhysRevC.89.054605
Measurement of the 58Ni(α,γ)62Zn reaction and its astrophysical impact
doi: 10.1103/PhysRevC.89.054611
Dipole excitations via isoscalar probes: The splitting of the pygmy dipole resonance in 124Sn
doi: 10.1103/PhysRevC.89.041601
Shell and shape evolution at N=28: The 40Mg ground state
doi: 10.1103/PhysRevC.89.041303
Benchmarking nuclear models for Gamow Teller response
doi: 10.1016/j.physletb.2014.02.001
Constraints on nucleon effective mass splitting with heavy ion collisions
doi: 10.1016/j.physletb.2014.03.030
Pygmy dipole resonance in 124Sn populated by inelastic scattering of 17O
doi: 10.1016/j.physletb.2014.08.029