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.
Gamow-Teller Strengths from (t,3He) Charge-Exchange Reactions on Light Nuclei
doi: 10.1016/S0370-2693(97)01393-2
Probing Proton Halos Through Pion Photoproduction
doi: 10.1103/PhysRevLett.80.1614
Beta-Decay of 56Cu
doi: 10.1016/S0370-2693(98)00606-6
Half-Life of 44Ti as a Probe for Supernova Models
doi: 10.1103/PhysRevLett.80.2554
Measurement of E2 Transitions in the Coulomb Dissociation of 8B
doi: 10.1103/PhysRevLett.81.2209
Measurement of the 8Li(n,γ)9Li Cross Section at Astrophysical Energies by Reverse Kinematics
doi: 10.1103/PhysRevC.57.959
Splintering Central Collisions: Systematics of Momentum and Energy Deposition for (17-115)A MeV 40Ar
doi: 10.1103/PhysRevC.57.R1032
Modeling the Breakup Stage of Relativistic Heavy ion Collisions
doi: 10.1103/PhysRevC.57.1907
Sideways-Peaked Angular Distributions in Hadron-Induced Multifragmentation: Shock Waves, Geometry, or Kinematics?
doi: 10.1103/PhysRevC.58.R13
Optimized Discretization of Sources Imaged in Heavy-Ion Reactions
doi: 10.1103/PhysRevC.57.2474
New Skyrme Interaction for Normal and Exotic Nuclei
doi: 10.1103/PhysRevC.58.220
Study of the 56Ni(d,p)57Ni Reaction and the Astrophysical 56Ni(p,γ)57Cu Reaction Rate
doi: 10.1103/PhysRevLett.80.676