Pith. sign in

REVIEW 1 cited by

The covariant Tolman-Oppenheimer-Volkoff equations II: The anisotropic case

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1709.03996 v1 pith:CYNCCNFJ submitted 2017-09-12 gr-qc astro-ph.HE

Sante Carloni , Daniele Vernieri This is my paper · ORCID
classification gr-qcastro-ph.HE
keywords anisotropicequationscasesolutionstolman-oppenheimer-volkoffcovariantdefineinterior
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We generalise the covariant Tolman-Oppenheimer-Volkoff equations proposed in arXiv:1709.02818 [gr-qc] to the case of static and spherically symmetric spacetimes with anisotropic sources. The extended equations allow a detailed analysis of the role of the anisotropic terms in the interior solution of relativistic stars and lead to the generalisation of some well known solutions of this type. We show that, like in the isotropic case, one can define generating theorems for the anisotropic Tolman-Oppenheimer-Volkoff equations. We also find that it is possible to define a reconstruction algorithm able to generate a double infinity of interior solutions. Among these, we derive a class of solutions that can represent "quasi-isotropic" stars.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Locally Rotationally Symmetric Spacetimes in Einstein-Cartan Theory and Their Classification

    gr-qc 2025-07 conditional novelty 6.0 of 10

    A complete covariant system plus a four-class taxonomy for locally rotationally symmetric spacetimes with Weyssenhoff-fluid torsion, with new Gödel-type, silent, and canonical-vacuum solutions.

Pith tools