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.
Cluster radioactivity of 294118Og176
doi: 10.1103/PhysRevC.99.041304
Ground-state electromagnetic moments of 37Ca
doi: 10.1103/PhysRevC.99.061301
Two-phonon wobbling in 135Pr
doi: 10.1016/j.physletb.2019.03.038
Symmetry energy constraints from GW170817 and laboratory experiments
doi: 10.1016/j.physletb.2019.06.059
Constraining the initial conditions and temperature dependent viscosity with three-particle correlations in Au+Au collisions
doi: 10.1016/j.physletb.2018.10.075
The proton-Ω correlation function in Au + Au collisions at √sNN = 200 GeV
doi: 10.1016/j.physletb.2019.01.055
Laser Spectroscopy of Neutron-Rich Tin Isotopes: A Discontinuity in Charge Radii across the N=82 Shell Closure
doi: 10.1103/PhysRevLett.122.192502
Constraining the Neutron Star Compactness: Extraction of the 23Al(p,γ) Reaction Rate for the rp Process
doi: 10.1103/PhysRevLett.122.232701
Direct Comparison between Bayesian and Frequentist Uncertainty Quantification for Nuclear Reactions
doi: 10.1103/PhysRevLett.122.232502
Is the Structure of 42Si Understood?
doi: 10.1103/PhysRevLett.122.222501
Azimuthal Harmonics in Small and Large Collision Systems at RHIC Top Energies
doi: 10.1103/PhysRevLett.122.172301
Following the Cosmic Evolution of Pristine Gas. III. The Observational Consequences of the Unknown Properties of Population III Stars
doi: 10.3847/1538-4357/aafa1a