Thermodynamical analysis of acoustic Schwarzschild black hole

被引:4
|
作者
Yasir, Muhammad [1 ,2 ]
Tiecheng, Xia [1 ,2 ]
Ditta, Allah [1 ,2 ]
Ali, Riasat [1 ,2 ]
Atamurotov, Farruh [3 ,4 ,5 ,6 ]
机构
[1] Shanghai Univ, Dept Math, Shanghai 200444, Peoples R China
[2] Shanghai Univ, Newtouch Ctr Math, Shanghai 200444, Peoples R China
[3] New Uzbekistan Univ, Mustaqillik Ave 54, Tashkent 100007, Uzbekistan
[4] Cent Asian Univ, Milliy Bog St 264, Tashkent 111221, Uzbekistan
[5] Inha Univ Tashkent, Ziyolilar 9, Tashkent 100170, Uzbekistan
[6] Natl Univ Uzbekistan, Tashkent 100174, Uzbekistan
关键词
Acoustic black hole; Thermodynamic stability; Thermal fluctuations; Gibbs free energy; Heat capacity; Emission energy; THERMAL FLUCTUATIONS; STABILITY; GRAVITY; FIELD;
D O I
10.1016/j.newast.2023.102106
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we analyze the thermodynamic properties of acoustic Schwarzschild black holes with its parameter. The study is conducted in the extended phase space displaying the phase transition. This phase transition is examined through Gibbs free energy, specific heat, and heat capacity. Later, we discuss the thermal stability of acoustic black holes through Hawking temperature by identifying their stable and unstable regions. We calculate the corrected entropy to examine the thermal fluctuations. Through the corrected entropy we observe that there is no fluctuation in the case of small black holes. We also discuss the energy emission process from acoustic black holes. Moreover, we employ the generalized uncertainty principle to obtain a modified Lagrangian equation. We analyze the tunneling and Hawking temperature of the acoustic Schwarzschild black hole after solving the field equations.
引用
收藏
页数:8
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