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.
Nuclear Level Densities and γ-ray Strength Functions in 44,45Sc
doi: 10.1103/PhysRevC.76.044303
Fragmentation Cross Sections and Binding Energies of Neutron-Rich Nuclei
doi: 10.1103/PhysRevC.76.041302(R)
Two-Proton Correlations in the Decay of 45Fe
doi: 10.1103/PhysRevLett.99.192501
Heating in the Accreted Neutron Star Ocean: Implications for Superburst Ignition
doi: 10.1086/517869
Selective Population and Neutron Decay of an Excited State of 23O
doi: 10.1103/PhysRevLett.99.112501
Implications of Low-Energy Fusion Hindrance on Stellar Burning and Nucleosynthesis
doi: 10.1103/PhysRevC.76.035802
Comment on “Reduction of the Spin-Orbit Splittings at the N=28 Shell Closure"
doi: 10.1103/PhysRevLett.99.099201
γ-ray Spectroscopy of Neutron-Deficient 110Te. I. Low- and Intermediate-Spin Structures
doi: 10.1103/PhysRevC.76.034322
Backward-Angle Photoproduction of π0 Mesons on the Proton at Eγ=1.5–2.4 GeV
doi: 10.1016/j.physletb.2007.10.032
Has the QCD Critical Point Been Signaled by Observations at the BNL Relativistic Heavy Ion Collider?
doi: 10.1103/PhysRevLett.98.092301
Sedimentation and Type I X-ray Bursts at Low Accretion Rates
doi: 10.1086/509628
The Laminar Flame Speedup by Neon-22 Enrichment in White Dwarf Supernovae
doi: 10.1086/511856