Virial masses of galaxy clusters in the post-Newtonian limit
arXiv:1210.5583
Abstract
We estimate virial masses of galaxy clusters using the parametrized post-Newtonian (PPN) virial theorem. Also, we show explicitly that post-Newtonian corrections can not address the mass discrepancy in the galaxy clusters.
To appear in the proceedings of Conference: C12-07-01.1