Nonlinear evolution of unstable charged de Sitter black holes with hyperboloidal formalism

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 cannot coexist with the central black hole stably and dissipates beyond the cosmological horizon slowly, leaving behind a bald black hole.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-01-09
DOI
https://doi.org/10.1103/physrevd.111.024025
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

Nonlinear evolution of unstable charged de Sitter black holes with hyperboloidal formalism

Hongbao Zhang, Cheng-Yong Zhang, Yu Tian, Qian Chen et al.
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
article

Nonlinear evolution of unstable charged de Sitter black holes with hyperboloidal formalism

Hongbao Zhang, Cheng-Yong Zhang, Yu Tian, Qian Chen, Zhiqi He
article en

Abstract

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 cannot coexist with the central black hole stably and dissipates beyond the cosmological horizon slowly, leaving behind a bald black hole.

Physical review. D/Physical review. D.Vol. 111(2)
Beijing Normal University (CN), Institute of Theoretical Physics (CN), University of Chinese Academy of Sciences (CN)
National Natural Science Foundation of China, China Postdoctoral Science Foundation, National Key Research and Development Program of China
Openalex Percentile: Top 100%
Black Holes and Theoretical Physics
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