A new mass model for nuclear astrophysics: crossing 200 keV accuracy (2021)
Attributed to:
Nuclear Physics Consolidated Grant
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2102.07497
Publication URI: https://arxiv.org/abs/2102.07497
Type: Preprint