Stellar equilibrium in Einstein-Chern-Simons gravity
General Relativity and Quantum Cosmology
2016-07-28 v2 High Energy Physics - Theory
Abstract
We consider a spherically symmetric internal solution within the context of Einstein-Chern-Simons gravity and derive a generalized five-dimensional Tolman-Oppenheimer-Volkoff (TOV) equation. It is shown that the generalized TOV equation leads, in a certain limit, to the standard five-dimensional TOV equation
Cite
@article{arxiv.1607.07533,
title = {Stellar equilibrium in Einstein-Chern-Simons gravity},
author = {Cristian Quinzacara and Patricio Salgado},
journal= {arXiv preprint arXiv:1607.07533},
year = {2016}
}
Comments
14 pages