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Main Authors: Guo, Guangzhou, Wang, Peng, Wu, Tianshu, Yang, Haitang
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2408.09243
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author Guo, Guangzhou
Wang, Peng
Wu, Tianshu
Yang, Haitang
author_facet Guo, Guangzhou
Wang, Peng
Wu, Tianshu
Yang, Haitang
contents This study investigates scalar clouds around Kerr-Newman black holes within the Einstein-Maxwell-scalar model. Tachyonic instabilities are identified as the driving mechanism for scalar cloud formation. Employing the spectral method, we numerically compute wave functions and parameter space existence domains for both fundamental and excited scalar cloud modes. Our analysis demonstrates that black hole spin imposes an upper limit on the existence of scalar clouds, with excited modes requiring stronger tachyonic instabilities for their formation. These findings lay the groundwork for exploring the nonlinear dynamics and astrophysical implications of scalar clouds.
format Preprint
id arxiv_https___arxiv_org_abs_2408_09243
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Stationary Scalar Clouds around Kerr-Newman Black Holes
Guo, Guangzhou
Wang, Peng
Wu, Tianshu
Yang, Haitang
General Relativity and Quantum Cosmology
This study investigates scalar clouds around Kerr-Newman black holes within the Einstein-Maxwell-scalar model. Tachyonic instabilities are identified as the driving mechanism for scalar cloud formation. Employing the spectral method, we numerically compute wave functions and parameter space existence domains for both fundamental and excited scalar cloud modes. Our analysis demonstrates that black hole spin imposes an upper limit on the existence of scalar clouds, with excited modes requiring stronger tachyonic instabilities for their formation. These findings lay the groundwork for exploring the nonlinear dynamics and astrophysical implications of scalar clouds.
title Stationary Scalar Clouds around Kerr-Newman Black Holes
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2408.09243