Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction (2016)
Attributed to:
Durham DiRAC-2 petascale facility
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1607.08788
Publication URI: https://arxiv.org/abs/1607.08788
Type: Other