Pith. sign in

REVIEW 1 cited by

Maximum bounds on the surface redshift of anisotropic stars

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 gr-qc/0201090 v2 pith:6DPNO6OS submitted 2002-01-29 gr-qc astro-ph

B.V.Ivanov This is my paper · ORCID
classification gr-qcastro-ph
keywords anisotropicredshiftsurfacevaluesboundboundscasecondition
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

It is shown that for realistic anisotropic star models the surface redshift can not exceed the values 3.842 or 5.211 when the tangential pressure satisfies the strong or the dominant energy condition respectively. Both values are higher than 2, the bound in the perfect fluid case.

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. Beyond Buchdahl's limit: bilayered stars and thin-shell configurations

    gr-qc 2024-11 conditional novelty 6.0 of 10

    Explicit bilayered and thin-shell GR models show that relaxing monotonic density or isotropy lets compactness approach Bondi's bound or even the black hole limit.

Pith tools