Thermodynamic Phase Transition of Generalized Ayon-Beato Garcia Black Holes

IF 1.5 4区 物理与天体物理 Q3 PHYSICS, PARTICLES & FIELDS
E. Ghasemi, H. Ghaffarnejad
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引用次数: 6

Abstract

In this work, we study thermodynamics of generalized Ayon-Beato and Garcia (ABG) black hole metric which contains three parameters named as mass m , magnetic charge q , and dimensionless coupling constant of nonlinear electrodynamics interacting field γ . We showed that central regions of this black hole behaves as dS (AdS) vacuum space by setting q < 2 m q > 2 m and in the case q = 2 m reaches to a flat Minkowski space. In the large distances, this black hole behaves as a Reissner-Nordstrom BH. However, an important role of the charge q appeared in the production of a formal variable cosmological parameter which will support pressure coordinate in the thermodynamic perspective of this black hole in our setup. We should point that this formal variable cosmological parameter is different with cosmological constant which comes from AdS/CFT correspondence, and it is effective at large distances as AdS space pressure. In our setup, the assumed pressure originated from the internal material of the black hole say q and m here. By calculating the Hawking temperature of this black hole, we obtain equation of state. Then, we plotted isothermal P-V curves and heat capacity at constant pressure. They show that the system participates in the small to large phase transition of the black hole or the Hawking-Page phase transition which is similar to the van der Waals phase transition in the ordinary thermodynamics systems. In fact in the Hawking-Page phase transition disequilibrium, evaporating generalized ABG black hole reaches to a vacuum AdS space finally.
广义Ayon-Beato-Garcia黑洞的热力学相变
本文研究了广义Ayon-Beato和Garcia (ABG)黑洞度量的热力学,该度量包含三个参数:质量m、磁荷q和非线性电动力学相互作用场γ的无量纲耦合常数。我们通过设置q = 2m证明了该黑洞的中心区域表现为dS (AdS)真空空间,在这种情况下q = 2m达到平坦的闵可夫斯基空间。在大的距离内,这个黑洞表现为Reissner-Nordstrom黑洞。然而,电荷q的一个重要作用出现在形式可变宇宙学参数的产生中,该参数将在我们的设置中从黑洞的热力学角度支持压力坐标。需要指出的是,这一形式变量宇宙学参数与AdS/CFT对应的宇宙学常数不同,它作为AdS空间压力在大距离上有效。在我们的设置中,假设压强来自于黑洞的内部物质比如q和m。通过计算该黑洞的霍金温度,得到其状态方程。然后,我们绘制了等温P-V曲线和恒压下的热容。结果表明,该体系参与了黑洞从小到大的相变或类似于普通热力学体系中的范德华相变的霍金-佩奇相变。实际上,在霍金-佩奇相变不平衡中,蒸发广义ABG黑洞最终到达真空的AdS空间。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Advances in High Energy Physics
Advances in High Energy Physics PHYSICS, PARTICLES & FIELDS-
CiteScore
3.40
自引率
5.90%
发文量
55
审稿时长
6-12 weeks
期刊介绍: Advances in High Energy Physics publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter. Considering both original research and focussed review articles, the journal welcomes submissions from small research groups and large consortia alike.
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