Turnaround radius in an accelerated universe with quasi-local mass
General Relativity and Quantum Cosmology
2015-10-14 v2
Abstract
We apply the Hawking-Hayward quasi-local energy construct to obtain in a rigorous way the turnaround radius of cosmic structures in General Relativity. A splitting of this quasi-local mass into local and cosmological parts describes the interplay between local attraction and cosmological expansion.
Keywords
Cite
@article{arxiv.1508.01725,
title = {Turnaround radius in an accelerated universe with quasi-local mass},
author = {Valerio Faraoni and Marianne Lapierre-Léonard and Angus Prain},
journal= {arXiv preprint arXiv:1508.01725},
year = {2015}
}
Comments
Updated to accepted JCAP version