论文标题
Ruppeiner几何形状,重新进入相变和微观结构的生产广告Black Hole
Ruppeiner Geometry, Reentrant Phase transition and Microstructure of Born-Infeld AdS Black Hole
论文作者
论文摘要
Born-Infeld Ads Black Hole展示了出生式参数$ b $的某些值的重入相过渡。与范德华(Van der Waals)相比,这种行为是一个附加特征,例如在带电广告中观察到的相变。因此,值得观察该返回相变的基本微观起源。根据参数$ b $的值,黑洞系统具有四种不同的情况:没有相变,带有两种情况的重入相变或类似于范德华的(标准)相变。在本文中,通过在温度和体积的参数空间中采用新颖的鲁皮剂几何学方法,我们通过相变研究研究了出生的侵权广告黑洞的微观结构,该研究包括标准和重新进入相变。我们发现,黑洞的微观结构导致标准和重入相变的本质是不同的。标准相变的特征是典型的RN-ADS微结构。在这种情况下,小黑洞相对于低温情况具有主要的排斥相互作用。有趣的是,在系统的重新进入相转换期间,系统在特定$ b $值的一系列压力下显示,微观结构中相互作用的主要吸引力。我们的结果表明,在重入相过渡案例中,中间黑洞的行为像玻色子气体,而在标准相过渡案例中,小黑色孔的表现像量子,任何气体。在这两种情况下,大黑孔相都显示出类似于骨气气体的相互作用。从曲率标量中观察到临界现象,包括重进入相变的特征。
Born-Infeld AdS black hole exhibits a reentrant phase transition for certain values of the Born-Infeld parameter $b$. This behaviour is an additional feature compared to the van der Waals like phase transition observed in charged AdS black holes. Therefore, it is worth observing the underlying microscopic origin of this reentrant phase transition. Depending on the value of the parameter $b$, the black hole system has four different cases: no phase transition, a reentrant phase transition with two scenarios, or a van der Waals-like (standard) phase transition. In this article, by employing a novel Ruppeiner geometry method in the parameter space of temperature and volume, we investigate the microstructure of Born-Infeld AdS black hole via the phase transition study, which includes standard and reentrant phase transition. We find that the microstructures of the black hole that lead to standard and reentrant phase transitions are distinct in nature. The standard phase transition is characterised by the typical RN-AdS microstructure. In this case, the small black hole phase has a dominant repulsive interaction for the low temperature case. Interestingly, during the reentrant phase transition, displayed by the system in a range of pressures for specific $b$ values, the dominant attractive nature of interaction in the microstructure is preserved. Our results suggest that in the reentrant phase transition case, the intermediate black holes behave like a bosonic gas, and in the standard phase transition case the small black holes behave like a quantum anyon gas. In both cases, the large black hole phase displays an interaction similar to the bosonic gas. The critical phenomenon is observed from the curvature scalar, including the signature of the reentrant phase transition.