Pith. sign in

REVIEW 1 cited by

Quasi-local studies of the particle surfaces and their stability in general spacetimes

Not yet reviewed by Pith; the record is open.

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 2208.03661 v3 pith:FBDIUYEK submitted 2022-08-07 gr-qc

classification gr-qc
keywords definitioncirculargeneralparticlespacetimesurfacegiveorbits
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

In this paper, enlightened by the definition of the photon surface given by Claudel, Virbhadra and Ellis, we give a quasi-local definition of the particle surface. From this definition, one can study the evolution of the circular orbits in general spacetime. Especially, we pointed out that this definition can be used to get the spherical circular orbits in stationary spacetimes which cannot be got by the definition of Claudel, Virbhadra and Ellis. Further, we give a condition to exclude the particle surface in spacetime without gravity. Simultaneously, we give a quasi-local definition of the stability of the particle surface in general spacetime. From this definition, one can get the evolution equation of the innermost stable circular orbit (ISCO) in general spacetime. To verify the correctness of these definitions, we studied the circular orbits in some special cases and the results are all consistent with the previous results.

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. Gravitational shadow and emission spectrum of thin accretion disks in a plasma medium

    gr-qc 2025-05 conditional novelty 6.0 of 10

    A blackbody accretion disk viewed through transparent, rotating plasma produces frequency-dependent shadows and emission maps, with the frequency of the brightest total flux controlled mainly by viewing angle.

Pith tools