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.
Analyzing Correlation Functions with Tesseral and Cartesian Spherical Harmonics
doi: 10.1103/PhysRevC.75.034907
In-Medium NN Cross Sections Determined from the Nuclear Stopping and Collective Flow in Heavy-Ion Collisions at Intermediate Energies
doi: 10.1103/PhysRevC.75.034615
Shell-Model Calculations of Two-Neutrino Double-Beta Decay Rates of 48Ca with the GXPF1A Interaction
doi: 10.1103/PhysRevC.75.034303
Structure of 23F via β-decay of 23O
doi: 10.1103/PhysRevC.75.024305
Proton Single-Particle Energies in 23F
doi: 10.1103/PhysRevC.75.024303
Are Spectroscopic Factors from Transfer Reactions Consistent with Asymptotic Normalization Coefficients?
doi: 10.1103/PhysRevC.75.024601
Scaling Properties of Hyperon Production in Au+Au Collisions at √sNN=200 GeV
doi: 10.1103/PhysRevLett.98.062301
Coupled-Cluster and Configuration-Interaction Calculations for Heavy Nuclei
doi: 10.1103/PhysRevLett.98.112501
Sensitivity of p-process Nucleosynthesis to Nuclear Reaction Rates in a 25 M(solar) Supernova Model
doi: 10.1086/508402
Physics of a Rare Isotope Accelerator
A Laser Ablation Ion Source for Gas Cell Studies
doi: 10.1016/j.nima.2006.09.055
Excited States and Signature Inversion in 116Cs
doi: 10.1103/PhysRevC.74.034310