Quazinormal modes and greybody factor of black hole surrounded by a quintessence in the S-V-T modified gravity as well as shadow

TL;DR

This paper explores how quintessence and modified gravity parameters influence black hole quasinormal modes, greybody factors, and shadows, revealing that these parameters significantly affect oscillation frequencies, radiation, and shadow size.

Contribution

It provides new analytical and numerical insights into the effects of quintessence and modified gravity on black hole properties, including QNMs, greybody factors, and shadows.

Findings

Increasing quintessence and MOG parameters decrease oscillation frequencies.

Greybody factors increase, allowing more radiation to reach infinity with higher parameters.

Black hole shadow radius slightly shrinks with plasma but increases with parameters, especially quintessence.

Abstract

The purpose of this study is to investigate the quasinormal modes (QNMs), greybody factors (GFs) and shadows in a plasma of a black hole (BH) surrounded by an exotic fluid of quintessence type in a scalar-vector-tensor modified gravity. The effects of a quintessence scalar field and the modified gravity (MOG) field on the QNM, GF, and shadow are examined. Using the sixth-order WKB approach, we investigate the QNMs of massless scalar and electromagnetic perturbations. Our findings show that as the quintessence and the MOG parameter ($\epsilon$ and $\alpha$) increase, the oscillation frequencies decrease significantly. Gravitational wave damping, on the other hand, decreases with increasing $\epsilon$ and $\alpha$. In addition, we obtain an analytical solution for the transmission coefficients (GF) and demonstrate that more thermal radiation reaches the observer at spatial infinity as both the $\epsilon$ and $\alpha$ parameters increase. We also investigate the effect of the plasma background on the BH shadow and show that as the plasma background parameter increases, the shadow radius slightly shrinks. Nevertheless, the shadow radius increases as $\alpha$ and $\epsilon$ increase. Particularly intriguing is the fact that increasing $\epsilon$ has a greater impact on the shadow radius than increasing $\alpha$, indicating that the quintessence parameter has a greater impact than the MOG parameter.