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.
Particle-Number Conservation in Static-Path Approximation for Thermal Superfluid Systems
doi: 10.1103/PhysRevC.76.064306
Neutron Density Distributions from Antiprotonic 208Pb and 209Bi Atoms
doi: 10.1103/PhysRevC.76.014311
One-Particle Excitations Outside the 54Ti Semi-Magic Core: The 55V and 55Ti Yrast Structures
doi: 10.1016/j.physletb.2007.05.014
d-α Correlation Functions and Collective Motion in Xe+Au Collisions at E/A=50 MeV
doi: 10.1016/j.physletb.2007.07.031
Energy Dependence of π±, p and p(bar) Transverse Momentum Spectra for Au+Au Collisions at √sNN = 62.4 and 200 GeV
doi: 10.1016/j.physletb.2007.06.035
α Decay of 109I and Its Implications for the Proton Decay of 105Sb and the Astrophysical Rapid Proton-Capture Process
doi: 10.1103/PhysRevLett.98.212501
Z=50 Shell Gap Near 100Sn from Intermediate-Energy Coulomb Excitations in Even-Mass 106-112Sn Isotopes
doi: 10.1103/PhysRevLett.99.162501
Tidal Effects and the Proximity Decay of Nuclei
doi: 10.1103/PhysRevLett.99.132701
The Laminar Flame Speedup by Neon-22 Enrichment in White Dwarf Supernovae
doi: 10.1086/511856
Heating in the Accreted Neutron Star Ocean: Implications for Superburst Ignition
doi: 10.1086/517869
Pulsations Detected from Accreting High Mass X-ray Binaries at Low Luminosities
doi: 10.1086/510183
Sedimentation and Type I X-ray Bursts at Low Accretion Rates
doi: 10.1086/509628