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.
RIB studies for explosive scenarios and future opportunities at FRIB
doi: 10.1088/1742-6596/1643/1/012068
Global R-matrix analysis of the 11B(α,n)14N reaction
doi: 10.1088/1742-6596/1668/1/012011
Indirect, experimental constraints of (n,γ) reaction rates for the i- and r-process
doi: 10.1088/1742-6596/1668/1/012024
Spectroscopic Study of 39Ca for Endpoint Nucleosynthesis in Classical Novae
doi: 10.1088/1742-6596/1668/1/012025
Extracting capture from transfer reactions
doi: 10.1088/1742-6596/1668/1/012030
Nucleosynthesis of "Light" Heavy Nuclei in Neutrino-driven Winds. Role of (α,n) reactions
doi: 10.1088/1742-6596/1668/1/012033
Heavy ion beam physics at Facility for Rare Isotope Beams
doi: 10.1088/1748-0221/15/12/P12034
Nucleosynthesis imprints from different Type Ia supernova explosion scenarios and implications for galactic chemical evolution
doi: 10.1051/0004-6361/202038721
Nuclear Data Sheets for A=190
doi: 10.1016/j.nds.2020.10.001
The impact of (n,γ) reaction rate uncertainties on the predicted abundances of i-process elements with 32 ≤ Z ≤ 48 in the metal-poor star HD94028
doi: 10.1093/mnras/stz3322
Cool-core cycles and Phoenix
doi: 10.1093/mnras/staa1247
The efficiency of nuclear burning during thermonuclear (Type I) bursts as a function of accretion rate
doi: 10.1093/mnras/staa2858
