重力下Reissner-Nordstrom AdS黑洞的焦耳-汤姆逊膨胀

Q2 Physics and Astronomy
M. Chabab, High Energy, H. E. Moumni, S. Iraoui, K. Masmar, S. Zhizeh
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引用次数: 27

摘要

本文研究了\(f(R)\)重力下带电AdS黑洞的焦耳-汤姆逊膨胀。我们得到了反演温度和反演曲线,并研究了在\(f(R)\)重力下范德瓦尔斯流体和带电AdS黑洞的异同。此外,我们还确定了反演点的位置与不同的质量\(M\)、电荷\(Q\)和参数\(b\)值之间的关系。在这一点上,焦耳-汤姆逊系数\(\mu\)消失了,这是我们用来通过仔细检查\(\mu\)量的符号来获得冷却-加热区域的一个重要特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Joule-Thomson Expansion of Reissner-Nordstrom AdS Black Holes in $f(R)$ gravity
In this paper, we study Joule-Thomson expansion for charged AdS black holes in \(f(R)\) gravity. We obtain the inversiontemperatures as well as inversion curves, and investigate similarities and differences between van der Waals fluidsand charged AdS black holes in \(f(R)\) gravity for this expansion.In addition, we determine the position of the inversion point versus different values ofthe mass \(M\), the charge \(Q\) and the parameter \(b\) for such black hole. At this point, the Joule-Thomson coefficient \(\mu\) vanishes, an import feature that we used to obtain the cooling-heating regions by scrutinizing the sign of the \(\mu\) quantity.
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来源期刊
Letters in High Energy Physics
Letters in High Energy Physics Physics and Astronomy-Nuclear and High Energy Physics
CiteScore
1.20
自引率
0.00%
发文量
4
审稿时长
12 weeks
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