Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes

TL;DR

This paper explores how dark energy and dark matter influence the properties of Euler-Heisenberg black holes, focusing on thermodynamics, shadows, and quasinormal modes, revealing their significant effects on these phenomena.

Contribution

It introduces a model incorporating quintessence and perfect fluid dark matter to analyze their impact on black hole characteristics, a novel approach in this context.

Findings

Dark sectors significantly alter black hole thermodynamics

Black hole shadows are affected by dark matter and dark energy

Quasinormal modes vary with dark sector parameters

Abstract

Current observations show that a significant fraction of the Universe is composed of dark energy and dark matter. In this paper, we investigate the simultaneous effects of these dark sectors on the Euler-Heisenberg black hole, using the quintessence matter field and perfect fluid to model them. In particular, we study the black hole's thermodynamics, shadows, and quasinormal modes, and discuss in detail how these properties change with relatively large or small dark sector components.