pith. machine review for the scientific record. sign in

arxiv: 1709.02818 · v1 · submitted 2017-09-08 · 🌀 gr-qc · astro-ph.HE

Recognition: unknown

The covariant Tolman-Oppenheimer-Volkoff equations I: The isotropic case

Authors on Pith no claims yet
classification 🌀 gr-qc astro-ph.HE
keywords equationssolutionsstellarcasecovariantinteriorisotropicknown
0
0 comments X
read the original abstract

We construct a covariant version of the Tolman-Oppenheimer-Volkoff equations in the case of isotropic sources. The new equations make evident the mathematical problems in the determination of interior solutions of relativistic stellar objects. Using a reconstruction algorithm we find two physically interesting generalisations of previously known stellar interior solutions. The variables that we use also allow an easier formulation of known generating theorems for solutions associated to relativistic stellar objects.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Radial adiabatic perturbations of stellar compact objects

    gr-qc 2026-04 unverdicted novelty 7.0

    A new covariant formulation of radial perturbations for imperfect fluids in GR yields a causality-imposed upper bound on the compactness of stable anisotropic stars.