Phase structures of holographic screen themodynamics
Wei-Jian Jiang, Yi-Xin Chen, Jian-Long Li

TL;DR
This paper explores the thermodynamic phase structures of holographic screens, demonstrating their phase transitions and analyzing conditions for different types of transitions in various charged spacetime scenarios.
Contribution
It establishes the connection between thermodynamics and gravity for holographic screens and classifies their phase transitions, including second order transitions, in (n+1)D RN-AdS spacetime.
Findings
Holographic screens exhibit phase transitions characterized by heat capacity discontinuities.
Second order phase transitions are confirmed via Ehrenfest equations.
Phase transition conditions depend on charge, electrostatic potential, and a parameter c.
Abstract
Holographic screens are the generalization of the event horizon of a black hole in entropic force scheme, which are defined by setting Newton potential constant, \textit{i. e.} const. By demonstrating that the integrated first law of thermodynamics is equivalent to the () component of Einstein equations, We strengthen the correspondence between thermodynamics and gravity. We show that there are not only the first law of thermodynamics, but also kinds of phase transitions of holographic screens. These phase transitions are characterized by the discontinuity of their heat capacities. In (n+1) dimensional Reissner-Nordstr\"{o}m-anti-de Sitter (RN-AdS) spacetime, we analyze three kinds of phase transitions, which are of the holographic screens with Q=0 (charge), constant (electrostatic potential) and non-zero constant . In the Q=0 case, only the…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Astrophysical Phenomena and Observations
