Black holes immersed in modified Chaplygin-like dark fluid and cloud of strings: shadows, quasinomal modes and greybody factors

TL;DR

This paper investigates how a modified Chaplygin-like dark fluid and a cloud of strings affect black hole shadows, quasinormal modes, and greybody factors, providing predictions for observational signatures of such exotic environments.

Contribution

It offers a unified analysis of black hole observables in a combined environment of dark fluid and strings, highlighting their distinct impacts on shadows, QNMs, and GBFs.

Findings

CoS intensity primarily influences black hole shadows and QNMs.

MCDF parameters cause complex modifications to observables.

Distinct signatures can probe exotic black hole environments.

Abstract

We present a unified investigation of black hole shadows, quasinormal modes (QNMs), and greybody factors (GBFs) for a static, spherically symmetric black hole within a composite environment of a modified Chaplygin-like dark fluid (MCDF) and a cloud of strings (CoS). We examine the structure of critical photon orbits and the corresponding optical appearance under spherical accretion. Using the Wentzel-Kramers-Brillouin (WKB) approximation, we compute the quasinormal frequencies and greybody spectra, and explore their correspondence with the black hole shadows in the eikonal limit. A systematic parameter study demonstrates that the CoS intensity has the primary influence on the shadows, QNMs and GBFs, while the MCDF parameters introduce more complex but characterizable modifications to each. Our results demonstrate that these environmental components imprint distinct yet interrelated signatures on key observables, offering specific predictions for probing exotic black hole environments.