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arXiv 2003.08778gr-qc

4维Gauss-Bonnet AdS黑洞的热力学、相变与Joule-Thomson膨胀

Thermodynamics, Phase Transition and Joule Thomson Expansion of 4-D Gauss-Bonnet AdS Black Hole

Kartheek Hegde, A. Naveena Kumara, C. L. Ahmed Rizwan, Ajith K. M., Md Sabir Ali, Shreyas Punacha

AI总结:

本文研究4维Gauss-Bonnet AdS黑洞的热力学与相变,发现Gauss-Bonnet参数共轭变量的变化可作为临界指数为1/2的序参量,并解析研究其Joule-Thomson膨胀特性。

摘要:

我们探索Einstein-Gauss-Bonnet引力中渐近AdS黑洞的热力学与相变性质,重点关注Joule-Thomson膨胀。热力学在扩展相空间中研究,其中宇宙学常数充当热力学压强。我们观察到该黑洞经历类似于van der Waals系统的相变。我们分别分析带电与中性情形,以区分电荷和Gauss-Bonnet参数对临界行为的影响,并考察相结构。我们发现Gauss-Bonnet耦合参数的行为类似于黑洞电荷或自旋,主导相结构。为了理解由Gauss-Bonnet系数$α$决定的底层相结构,我们引入一个新的序参量。我们发现Gauss-Bonnet参数共轭变量的变化充当序参量,在临界点附近展示出$1/2$的临界指数。由于相结构与van der Waals流体类似,我们研究黑洞的Joule-Thomson膨胀。我们解析地研究Joule-Thomson膨胀,重点关注三个关键特征:Joule-Thomson系数、反转曲线和等焓曲线。我们在$T-P$平面中得到等焓曲线,并展示冷却-加热区域。

英文摘要:

We explore the thermodynamic and phase transition properties of asymptotically AdS black holes within Einstein-Gauss-Bonnet gravity, focusing on Joule Thomson expansion. Thermodynamics is studied in the extended phase space, where the cosmological constant serves as thermodynamic pressure. We observe that the black hole undergoes a phase transition similar to that of a van der Waals system. We analyze charged and neutral cases separately to distinguish the effect of charge and Gauss Bonnet parameter on critical behavior and examine the phase structure. We find that the Gauss-Bonnet coupling parameter behaves similarly to black hole charge or spin, guiding the phase structure. To understand the underlying phase structure determined by the Gauss-Bonnet coefficient $α$, we introduce a new order parameter. We discover that the change in the conjugate variable to the Gauss-Bonnet parameter acts as an order parameter, demonstrating a critical exponent of $1/2$ in the vicinity of the critical point. Since the phase structure is analogous to that of a van der Waals fluid, we investigate the Joule-Thomson expansion of the black hole. We analytically study the Joule-Thomson expansion, focusing on three key characteristics: the Joule-Thomson coefficient, inversion curves, and isenthalpic curves. We obtain isenthalpic curves in the $T-P$ plane and illustrate the cooling-heating regions.

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