Non-Vacuum Solutions in Cotton Theory

TL;DR

This paper explores non-vacuum solutions in Cotton theory, a higher derivative extension of General Relativity, analyzing their properties and implications for black hole physics and astrophysical phenomena.

Contribution

It introduces and investigates specific non-vacuum solutions in Cotton theory, extending known solutions like Kiselev and Dymnikova to this higher derivative framework.

Findings

Generalizes Kiselev and Dymnikova solutions in CT

Addresses singularities, thermodynamics, and geodesics in generalized solutions

Highlights differences between CT and GR in non-vacuum contexts

Abstract

Cotton theory (CT) introduces a higher derivative extension of General Relativity (GR) characterized by third-rank field equations. Recently, key distinctions between CT and GR concerning wave and vacuum solutions have been highlighted in [1, 2]. In this study, two particular non-vacuum solutions of CT are investigated within its Codazzi formulation. The motivation is to reveal how this theory might account for or adapt to the effects of non-vacuum sources, and whether it can provide new insights into the behavior of both singular and regular black holes in astrophysical contexts. It is shown that CT generalizes the Kiselev and Dymnikova solutions in GR. Some aspects of the generalized solutions, in particular concerning singularities, thermodynamics, and geodesics, are addressed in comparison to GR.