Pith. sign in

REVIEW 1 cited by

Scale invariant elastic stars in General Relativity

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 2306.16584 v2 pith:23RA4N5Q submitted 2023-06-28 gr-qc

Artur Alho , José Natário , Paolo Pani , Guilherme Raposo This is my paper · ORCID
classification gr-qc
keywords compactelasticgeneralradiusrelativityscalestarsabsence
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We present a model of relativistic elastic stars featuring scale invariance. This implies a linear mass-radius relation and the absence of a maximum mass. The most compact spherically symmetric configuration that is radially stable and satisfies all energy and causality conditions has a slightly smaller radius than the Schwarzschild light ring radius. To the best of our knowledge, this is the first material compact object with such remarkable properties in General Relativity, which makes it a unique candidate for a black-hole mimicker.

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