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Joule-Thomson expansion of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>d</mml:mi></mml:math>-dimensional charged AdS black holes

Jie-Xiong MoInstitute of Theoretical Physics, Lingnan Normal University, Zhanjiang, 524048 Guangdong, ChinaGu-Qiang LiInstitute of Theoretical Physics, Lingnan Normal University, Zhanjiang, 524048 Guangdong, ChinaShan-Quan LanInstitute of Theoretical Physics, Lingnan Normal University, Zhanjiang, 524048 Guangdong, ChinaXiao-Bao XuInstitute of Theoretical Physics, Lingnan Normal University, Zhanjiang, 524048 Guangdong, China
2018lv
ABI

Annotatsiya

Effects of the dimensionality on the Joule-Thomson expansion are discussed in detail by considering the case of $d$-dimensional charged AdS black holes. Specifically, we investigate three important aspects characteristic of the Joule-Thomson expansion. Namely, the Joule-Thomson coefficient, the inversion curves and the isenthalpic curves. To derive the explicit expression of the Joule-Thomson coefficient, we examine two different approaches existed in the pioneering literatures and prove that they are consistent with each other. The divergent point and the zero point of the Joule-Thomson coefficient are discussed. The former is shown to reveal the information of Hawking temperature while the latter is depicted through the so-called inversion curves. Fine structures of the inversion curves are disclosed in the cases $d&gt;4$. At low pressure, the inversion temperature increases with the dimensionality $d$ while at high pressure it decreases with $d$. The ratio between minimum inversion temperature ${T}_{\mathrm{min}}$ and the critical temperature ${T}_{c}$ is discussed with its explicit expression obtained for $d&gt;4$. Surprisingly, it is shown that the ratio is not always equal to $1/2$ but decreases with the dimensionality $d$. Moreover, isenthalpic curves of $d&gt;4$ are shown to expand toward higher pressure when the dimensionality $d$ increases.

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