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

被引：4

作者：

Hamil, B. ^{[1
]}

Lutfuoglu, B. C. ^{[2
]}

Dahbi, L. ^{[3
]}

机构：

[1] Univ Constantine 1, Fac Sci Exactes, Lab Phys Math & Subatom, Freres Mentouri, Constantine, Algeria

[2] Univ Hradec Kralove, Fac Sci, Dept Phys, Rokitanskeho 62-26, Hradec Kralove 50003, Czech Republic

[3] Teacher Educ Coll Setif, Messaoud Zeghar, Algeria

来源：

MODERN PHYSICS LETTERS A | 2024年 / 39卷 / 33N34期

关键词：

Black hole; quintessence field; quantum correction; thermodynamics; shadows; QUASI-NORMAL MODES; JOULE-THOMSON EXPANSION; TELESCOPE RESULTS. I; COSMOLOGICAL CONSTANT; EVENT HORIZON; GRAVITATIONAL COLLAPSE; PHASE-TRANSITION; SCATTERING; EVOLUTION; SPACETIME;

D O I：

10.1142/S021773232450161X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, 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, Gibbs free energy, 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.

引用

页数：27

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