Pith. sign in

REVIEW

Scalar perturbations and quasi-normal modes of a non-linear magnetic-charged black hole surrounded by quintessence

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 1811.02847 v2 pith:N2N36FL4 submitted 2018-11-07 gr-qc

classification gr-qc
keywords perturbationsblackholescalarfrequencymagneticmodesnonlinear
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We study scalar perturbations and quasinormal modes of a nonlinear magnetic charged black hole surrounded by quintessence. Time evolution of scalar perturbations is studied for different parameters associated with the black hole solution. We also study the reflection and transmission coefficients along with absorption cross-section for the considered black hole spacetime. It was shown that the real part of quasinormal frequency increases with increase in nonlinear magnetic charge while the module of the imaginary part of the frequency decreases. The analysis of the perturbations with changing quintessential parameter $c$ showed that perturbations with high values of $c$ become unstable.

Discussion (0). Sign in to comment.

Pith tools