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.
Direct formation of the C5-radical in the sugar-phosphate backbone of DNA by radiation
First Annular-Ring Coupled Structure Cavity for the Japan Proton Accelerator Research Complex Linac
doi: 10.1103/PhysRevSTAB.15.051005
First High-Power Model of the Annular-Ring Coupled Structure for Use in the Japan Proton Accelerator Research Complex Linac
doi: 10.1103/PhysRevSTAB.15.011001
Design of a New Time-of-flight Small-angle Neutron Scattering Instrument at CPHS
Beta decay of 71,73Co: Probing Single-Particle States Approaching Doubly-Magic 78Ni
doi: 10.1103/PhysRevC.85
Radiation Hardened Superconducting Mixed Multipole Magnet Designs for FRIB
doi: 10.1016/j.phpro.2012.06.045
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
doi: 10.1016/j.nima.2012.06.050
New excited states in the halo nucleus 6He
doi: 10.1016/j.physletb.2012.10.054
Direct Mass Measurements of 19B, 22C, 29F, 31Ne, 34Na and Other Light Exotic Nuclei
doi: 10.1103/PhysRevLett.109.202503
Shell model based Coulomb excitation γ-ray intensity calculations in 107Sn
doi: 10.1088/0031-8949/2012/T150/014012
New Hubble Space Telescope Observations of Heavy Elements in Four Metal-Poor Stars
A high-performance Fortran code to calculate spin- and parity-dependent nuclear level densities
doi: 10.1016/j.cpc.2012.09.006
