Holographic Complexity and Phase Transition for AdS Black Holes

Fuente: arXiv
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Autores principales: Jiang, Hong-Yue, Wang, Meng-Ting, Liu, Yu-Xiao
Formato: Preprint
Publicado: 2023
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author Jiang, Hong-Yue
Wang, Meng-Ting
Liu, Yu-Xiao
author_facet Jiang, Hong-Yue
Wang, Meng-Ting
Liu, Yu-Xiao
contents Recently, the complexity equals any gravitational observable conjecture has been proposed in [Phys. Rev. Lett. 128, 081602 (2022)], which is an extension of the complexity equals volume proposal. These gravitational observables are referred to as generalized volumes. In this paper, we investigate the generalized volume-complexity for black holes with one or two horizons respectively. We verify that the turning time is universal and independent of the Cauchy horizon. Not only does this phase transition occur once, but it may also occur two or more times depending on the number and height of the effective potential peaks. On the other hand, we confirm that the generalized volume-complexity can be divided based on the shape of the effective potential. We then discuss the non-smooth transition from the Reissner-Nordström-AdS black hole to the Schwarzschild-AdS black hole.
format Preprint
id arxiv_https___arxiv_org_abs_2307_09223
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Holographic Complexity and Phase Transition for AdS Black Holes
Jiang, Hong-Yue
Wang, Meng-Ting
Liu, Yu-Xiao
High Energy Physics - Theory
General Relativity and Quantum Cosmology
Recently, the complexity equals any gravitational observable conjecture has been proposed in [Phys. Rev. Lett. 128, 081602 (2022)], which is an extension of the complexity equals volume proposal. These gravitational observables are referred to as generalized volumes. In this paper, we investigate the generalized volume-complexity for black holes with one or two horizons respectively. We verify that the turning time is universal and independent of the Cauchy horizon. Not only does this phase transition occur once, but it may also occur two or more times depending on the number and height of the effective potential peaks. On the other hand, we confirm that the generalized volume-complexity can be divided based on the shape of the effective potential. We then discuss the non-smooth transition from the Reissner-Nordström-AdS black hole to the Schwarzschild-AdS black hole.
title Holographic Complexity and Phase Transition for AdS Black Holes
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2307.09223