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.
Qcombo: A Python Package for Automated Commutator Calculations of Quantum Many-Body Operators
doi: 10.1016/j.cpc.2026.110444
Beyond constant error: Heteroscedastic Bayesian model combination for modeling unmeasured nuclei
doi: 10.1103/z7g9-7d74
Proton femtoscopy in heavy-ion collisions: From transport theory to source imaging
doi: 10.1103/kfzk-rtnm
QCD phase structure at high baryon density
doi: 10.1016/j.jspc.2026.100590
In Situ X-ray Spectroscopic Identification and Kinetic Control of Highly Hybridized Co(IV) States in Cobalt Oxide Amorphous Catalysts
doi: 10.1021/acscatal.6c04565
Direct transfer to 46,48K as a survey of the 𝜋(𝑠1/2)−𝜈(𝑠𝑑𝑝𝑓) interaction
doi: 10.1103/z145-rfy7
Lowest-radiation environments in the Solar System: New opportunities for underground rare-event searches
doi: 10.1103/7fjv-rz78
High-precision mass measurements of 52Ni and 51Co reveal breakdown of the isobaric multiplet mass equation in the 𝑓𝑝 shell
doi: 10.1103/xrbm-m61q
Square matrix-based six-dimensional convergence map for nonlinear beam dynamics analysis
doi: 10.1103/3x6c-zqpt
Direct nuclear reaction as a tool for nuclear structure and astrophysics
doi: 10.1088/1361-6471/aea4cb
Conformal prediction for uncertainties in the neutron star equation of state
doi: 10.1103/15zm-3bll
Nuclear Beavers
doi: 10.1119/5.0253360
