Nonlinear Evolution of unstable Charged de Sitter Black Holes with Hyperboloidal Formalism

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: He, Zhen-Tao, Chen, Qian, Tian, Yu, Zhang, Cheng-Yong, Zhang, Hongbao
Format: Preprint
Published: 2024
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866929715098419200
author He, Zhen-Tao
Chen, Qian
Tian, Yu
Zhang, Cheng-Yong
Zhang, Hongbao
author_facet He, Zhen-Tao
Chen, Qian
Tian, Yu
Zhang, Cheng-Yong
Zhang, Hongbao
contents Based on the hyperboloidal framework, we research the dynamical process of charged de Sitter black holes scattered by a charged scalar field. From the linear perturbation analysis, with the coupling strength within a critical interval, the charged scalar field with a superradiance frequency can induce the instability of the system. To reveal the real-time dynamics of such an instability, the nonlinear numerical simulation is implemented. The results show that the scalar field grows exponentially in the early stages and drastically extracts the charge from the black hole due to the superradiance, analogous to the charged black hole in a closed system. Differently, after saturation, the scalar field can not coexist with the central black hole stably and dissipates beyond the cosmological horizon slowly, leaving behind a bald black hole.
format Preprint
id arxiv_https___arxiv_org_abs_2411_03193
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Nonlinear Evolution of unstable Charged de Sitter Black Holes with Hyperboloidal Formalism
He, Zhen-Tao
Chen, Qian
Tian, Yu
Zhang, Cheng-Yong
Zhang, Hongbao
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Based on the hyperboloidal framework, we research the dynamical process of charged de Sitter black holes scattered by a charged scalar field. From the linear perturbation analysis, with the coupling strength within a critical interval, the charged scalar field with a superradiance frequency can induce the instability of the system. To reveal the real-time dynamics of such an instability, the nonlinear numerical simulation is implemented. The results show that the scalar field grows exponentially in the early stages and drastically extracts the charge from the black hole due to the superradiance, analogous to the charged black hole in a closed system. Differently, after saturation, the scalar field can not coexist with the central black hole stably and dissipates beyond the cosmological horizon slowly, leaving behind a bald black hole.
title Nonlinear Evolution of unstable Charged de Sitter Black Holes with Hyperboloidal Formalism
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2411.03193