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.
Quantifying uncertainty in physics-based predictions of rare-isotope production cross sections via Bayesian-inspired model averaging across nuclear mass tables
doi: 10.1103/rd5c-4m5w
Nuclear level density and 𝛾-ray strength function of 97Zr
doi: 10.1103/bmw2-h889
Isotopic discrepancy in microscopic fusion of 16O + 40,48Ca
doi: 10.1103/v7jd-l94j
34Ar(𝛼,𝑝)37K reaction rate from proton scattering on 37K and its impact on properties of modeled x-ray bursts
doi: 10.1103/x8xt-y8dr
Total absorption spectroscopy study of the 71Fe →71Co 𝛽 decay
doi: 10.1103/ms66-lg13
𝑙-forbidden 𝑀1 strengths near 100Sn from knockout reactions in Cd and Sn
doi: 10.1103/jd5v-hg3c
Optimization of the FRIB beam dump: a hybrid genetic algorithm and reinforcement learning approach
doi: 10.1007/s41365-026-02020-2
Physical thickness characterization of the FRIB production targets
doi: 10.1088/1748-0221/21/07/T07005
Three-dimensional printing as a rapid prototyping approach for novel radio frequency cavity designs
doi: 10.1063/5.0315255
Suppression of high-intensity stripped heavy-ion beam losses
doi: 10.1016/j.nima.2026.171871
The role of ab initio beta-decay calculations in light nuclei for probes of physics beyond the standard model
doi: 10.1016/j.ppnp.2026.104260
𝛽-decay measurements near the 𝑁=40 island of inversion to quantify cooling of accreted neutron star crusts
doi: 10.1103/vmfw-c2kb
