Thermodynamic product formulae for Finslerian Kiselev black hole

被引：9
|
作者：
Nekouee, Z. [1 ,2 ]
Narasimhamurthy, S. K. [1 ]
机构：
[1] Kuvempu Univ, Dept PG Studies & Res Math, Jnana Sahyadri Shankaraghatta, Shivamogga 577451, Karnataka, India
[2] Univ Mazandaran, Fac Math Sci, Dept Math, POB 47416-95447, Babolsar, Mazandaran, Iran
来源：
EUROPEAN PHYSICAL JOURNAL C | 2023年 / 83卷 / 08期
关键词：
GREYBODY FACTORS; QUINTESSENCE; TRANSITION;
D O I：
10.1140/epjc/s10052-023-11898-w
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
The main goal of this paper is to solve the Finslerian Kiselev black hole and investigate its thermodynamic characteristics surrounded by dust, radiation, quintessence, and the cosmological constant. Since these black holes have multiple horizons, thus we calculate thermodynamic quantities, including area, horizon radius, Bekenstein-Hawking entropy, Hawking temperature, surface gravity, and Komar energy products. In addition, we study all universal relations of these black holes and discuss the role and effect of the Finslerian Ricci scalar (q) on Finslerian Kiselev black holes and their stability.
引用
收藏
页数：12
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