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.
Investigation of the triple-α reaction in a full three-body approach
doi: 10.1103/PhysRevC.87.054615
The ratio method: A new tool to study one-neutron halo nuclei
doi: 10.1103/PhysRevC.88.044602
Evidence for the existence of the astrophysically important 6.40-MeV state of 31S
doi: 10.1103/PhysRevC.88.055803
Single-particle and collective excitations in 63Ni
doi: 10.1103/PhysRevC.88.054314
Coupled-cluster studies of infinite nuclear matter
doi: 10.1103/PhysRevC.88.054312
Constraining the initial temperature and shear viscosity in a hybrid hydrodynamic model of √sNN=200 GeV Au+Au collisions using pion spectra, elliptic flow, and femtoscopic radii
doi: 10.1103/PhysRevC.87.044901
Universal properties of infrared oscillator basis extrapolations
doi: 10.1103/PhysRevC.87.044326
Neutron-Hole State in 45Ar from 1H(46Ar, d) 45Ar Reactions
doi: 10.1103/PhysRevC.88.017604
Resonant scattering of 22Na + p studied by the thick-target inverse-kinematic method
doi: 10.1103/PhysRevC.88.035801
β-decay properties for neutron-rich Kr–Tc isotopes from deformed pn-quasiparticle random-phase approximation calculations with realistic forces
doi: 10.1103/PhysRevC.88.024314
Neutrino Pair Emission from Hot Nuclei During Stellar Collapse
doi: 10.1103/PhysRevC.88.015807
Shell-model studies of the astrophysical rp reaction 29P(p,γ)30S
doi: 10.1103/PhysRevC.87.065803