Pith. sign in

REVIEW 1 cited by

Black hole shadow to probe modified gravity

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 2101.08261 v1 pith:RGPY2CFN submitted 2021-01-20 gr-qc astro-ph.CO

classification gr-qcastro-ph.CO
keywords blackholeshadowcosmologicallambdaparametersitteragreement
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We study the black hole's shadow for Schwarzschild - de Sitter and Kerr - de Sitter metrics with the contribution of the cosmological constant \Lambda. Based on the reported parameters of the M87* black hole shadow we obtain constraints for the $\Lambda$ and show the agreement with the cosmological data. It is shown that, the coupling of the \Lambda-term with the spin parameter reveals peculiarities for the photon spheres and hence for the shadows. Within the parametrized post-Newtonian formalism the constraint for the corresponding \Lambda-determined parameter is obtained.

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. Greybody Factor for massive scalar field in charged black hole

    gr-qc 2025-01 unverdicted novelty 3.0 of 10

    For a massive scalar field around a charged black hole, the greybody factor falls as the field mass rises, consistent between WKB and rigorous bound methods.

Pith tools