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.
Triggering and Delivery Algorithms for AGN Feedback
doi: 10.3847/1538-4357/aa6fb1
Viewpoint: Doubly Magic Nickel
Spartak Timofeevich Belyaev
doi: 10.1063/PT.3.3602
Direct injection of fully stripped carbon ions into a fast-cycling induction synchrotron and their capture by the barrier bucket
doi: 10.1103/PhysRevAccelBeams.20.080101
Time-dependent potential functions to stretch the time distributions of ion pulses ejected from EBIST
doi: 10.1139/cjp-2016-0716
Measurement of the cross section and longitudinal double-spin asymmetry for dijet production in polarized <i>pp</i> collisions at <i>√s<sub>NN</sub></i>= 200 GeV
doi: 10.1103/PhysRevD.95.071103
Neodymium-140 DOTA-LM3: Evaluation of an In Vivo Generator for PET with a Non-Internalizing Vector
doi: 10.3389/fmed.2017.00098
Charge-state distribution of Li ions from the β decay of laser-trapped 6He atoms
doi: 10.1103/PhysRevA.96.053411
Dynamics, nucleosynthesis, and kilonova signature of black hole—neutron star merger ejecta
doi: 10.1088/1361-6382/aa7a77
Nuclear Data Sheets for A=138
doi: 10.1016/j.nds.2017.11.001
SRF acceleration for heavy ions: ATLAS decadal operation and evolution
doi: 10.1088/1748-0221/12/04/T04001
Neutrino-heated winds from millisecond protomagnetars as sources of the weak r-process
doi: 10.1093/mnras/stx478