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.
Improved precision on the experimental E0 decay branching ratio of the Hoyle state
doi: 10.1103/PhysRevC.102.024320
Many-body correlations in nuclear superfluidity
doi: 10.1103/PhysRevC.102.034310
Properties of a separable representation of optical potentials
doi: 10.1103/PhysRevC.102.024606
Isotopically resolved neutron total cross sections at intermediate energies
doi: 10.1103/PhysRevC.102.034601
First inverse kinematics study of the 22Ne(p,γ)23Na reaction and its role in AGB star and classical nova nucleosynthesis
doi: 10.1103/PhysRevC.102.035801
Collective 2p-2h intruder states in 118Sn studied via β decay of 118In using the GRIFFIN spectrometer at TRIUMF
doi: 10.1103/PhysRevC.102.024323
Benchmark neutrinoless double- β decay matrix elements in a light nucleus
doi: 10.1103/PhysRevC.102.014302
Measurement of D0-meson + hadron two-dimensional angular correlations in Au + Au collisions at √sNN = 200 GeV
doi: 10.1103/PhysRevC.102.014905
Microscopic calculations of nuclear level densities with the Lanczos method
doi: 10.1103/PhysRevC.102.014315
Structure of 33Si and the magicity of the N=20 gap at Z=14
doi: 10.1103/PhysRevC.102.024321
Low-lying level structure of the neutron-unbound N=7 isotones
doi: 10.1103/PhysRevC.102.014325
Shell-model studies of the astrophysical rp-process reactions 34S(p,γ)35Cl and 34g,mCl(p,γ)35Ar
doi: 10.1103/PhysRevC.102.025801