Quantum-corrected Schwarzschild AdS black hole surrounded by quintessence: Thermodynamics and Shadows

TL;DR

This paper investigates how quintessence matter influences the thermodynamics and shadow properties of quantum-corrected Schwarzschild AdS black holes, revealing parameter-dependent variations in temperature, shadow size, and energy emission.

Contribution

It provides a detailed analysis of the effects of quintessence matter on black hole thermodynamics and shadows, incorporating quantum corrections and exploring parameter impacts.

Findings

Shadow radius decreases with higher quintessence state parameter

Shadow radius increases with higher normalization parameter

Energy emission rate peaks are affected by quintessence parameters

Abstract

In this manuscript, we study the quantum-corrected Schwarzschild AdS black hole surrounded by quintessence matter in two folds: its thermal quantities and shadows. For this purpose, first, we present a detailed analysis of the influences of the quintessence matter field on Hawking temperature, mass, and specific heat functions. Then, we examine the shadows by following Carter's approach. We find that the shadow radius value takes smaller values for greater quintessence state parameter values. On the other hand, we see that the shadow radius takes greater values for greater values of the normalization parameter. Finally, in a brief section, we discuss the energy emission rate and show that the Gaussian-type plots' peak values are also affected by the quintessence matter field parameters.