paper

Some exact relativistic star solutions in gravity

arXiv:2403.00070 · doi:10.1088/1361-6382/adc8f2

Abstract

We present a covariant description of non-vacuum static spherically symmetric spacetimes in gravity applying the (1+1+2) covariant formalism. The propagation equations are then used to derive a covariant and dimensionless form of the Tolman-Oppenheimer-Volkoff (TOV) equations. We then give a solution strategy to these equations and obtain some new exact solutions for the particular case , which have the correct thermodynamic properties for standard matter.

38 pages, 14 figures, 2 appendices. Class. Quantum Grav (2025)

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