Cluster abundance in chameleon f ( R ) gravity I: toward an accurate halo mass function prediction (2016)
Attributed to:
Extragalactic Astronomy at Durham 2011-2016
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/1475-7516/2016/12/024
Publication URI: http://dx.doi.org/10.1088/1475-7516/2016/12/024
Type: Journal Article/Review
Parent Publication: Journal of Cosmology and Astroparticle Physics
Issue: 12