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.
Azimuthal anisotropy in U+ U and Au+ Au collisions at RHIC
doi: 10.1103/PhysRevLett.115.222301
Observation of Transverse Spin-Dependent Azimuthal Correlations of Charged Pion Pairs in p↑+ p at √s= 200 GeV
doi: 10.1103/PhysRevLett.115.242501
Atomic nucleus as chaotic quantum many-body system
doi: 10.12693/APhysPolA.128.1008
Neutron resonance widths and the Porter-Thomas distribution
doi: 10.1103/PhysRevLett.115.052501
Statistical uncertainties of a chiral interaction at next-to-next-to leading order
doi: 10.1088/0954-3899/42/3/034003
Systematic uncertainties in direct reaction theories
doi: 10.1088/0954-3899/42/3/034014
A comprehensive simulation study of a liquid Xe detector for contraband detection
doi: 10.1088/1748-0221/10/03/P03030
Operation of THGEM-based detector in low-pressure Helium
doi: 10.1088/1748-0221/10/02/P02012
Studies of THGEM-based detector at low-pressure Hydrogen/Deuterium, for AT-TPC applications
doi: 10.1088/1748-0221/10/09/P09020
A Strong Shallow Heat Source in the Accreting Neutron Star Maxi J0556-332
doi: 10.1088/2041-8205/809/2/L31
High intensity targets stations for S3
doi: 10.1007/s10967-015-3936-5
Revalidation of the isobaric multiplet mass equation for the A=20 quintet
doi: 10.1103/PhysRevC.92.042501