Pith. sign in

REVIEW 1 cited by

Circular geodesics and accretion disks in Janis-Newman-Winicour and Gamma metric

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 1112.2522 v2 pith:AJCEDM7R submitted 2011-12-12 gr-qc astro-ph.HE

classification gr-qcastro-ph.HE
keywords circulardifferentdisksgeodesicsmetricnakedaccretionaround
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We study here circular timelike geodesics in the Janis-Newman-Winicour and Gamma metric spacetimes which contain a strong curvature naked singularity and reduce to the Schwarzschild metric for a specific value of one of the parameters. We show that for both the metrics the range of allowed parameters can be divided into three regimes where structure of the circular geodesics is qualitatively different. It follows that the properties of the accretion disks around such naked singularities can be significantly different from those of disks around black holes. This adds to previous studies showing that if naked singularities exist in nature, their observational signature would be significantly different from that of the black hole.

Discussion (0). Sign in 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. Constraining quadrupole deformations with relativistic effects

    gr-qc 2025-06 reject novelty 6.0 of 10

    In the Zipoy-Voorhees spacetime, the Shapiro time delay and the Shirokov oscillation frequencies acquire corrections from the quadrupole deformation parameter q, with the delay correction appearing at first order in q.

Pith tools