Stellar equilibrium in Einstein-Chern-Simons gravity
Cristian Quinzacara, Patricio Salgado
TL;DR
This paper derives a generalized five-dimensional TOV equation within Einstein-Chern-Simons gravity, extending the understanding of stellar equilibrium in higher-dimensional modified gravity theories.
Contribution
It introduces a new generalized TOV equation specific to Einstein-Chern-Simons gravity and explores its relation to the standard five-dimensional TOV equation.
Findings
Generalized TOV equation derived for Einstein-Chern-Simons gravity
Reduction to standard five-dimensional TOV equation in a specific limit
Provides insights into stellar equilibrium in higher-dimensional modified gravity
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
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