Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holes

Abstract The black hole scalarization in a special Einstein-scalar–Gauss–Bonnet (EsGB) gravity has been widely investigated in recent years. Especially, the spontaneous scalarization of scalar-free black hole in de-Sitter (dS) spacetime possesses interesting features due to the existence of cosmolog...

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Main Authors: Zhen-Hao Yang, Guoyang Fu, Xiao-Mei Kuang, Jian-Pin Wu
Format: Article
Language:English
Published: SpringerOpen 2022-10-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-022-10834-8
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author Zhen-Hao Yang
Guoyang Fu
Xiao-Mei Kuang
Jian-Pin Wu
author_facet Zhen-Hao Yang
Guoyang Fu
Xiao-Mei Kuang
Jian-Pin Wu
author_sort Zhen-Hao Yang
collection DOAJ
description Abstract The black hole scalarization in a special Einstein-scalar–Gauss–Bonnet (EsGB) gravity has been widely investigated in recent years. Especially, the spontaneous scalarization of scalar-free black hole in de-Sitter (dS) spacetime possesses interesting features due to the existence of cosmological horizon. In this work, firstly, we focus on the massive scalar field perturbation on Schwarzschild dS (SdS) black hole in a special EsGB theory. By analyzing the fundamental QNM frequency and time evolution of the scalar field perturbation, we figure out the unstable/stable regions in $$(\Lambda ,\alpha )$$ ( Λ , α ) -plane as well as in $$(m,\alpha )$$ ( m , α ) -plane for various perturbation modes, where $$\Lambda $$ Λ , $$\alpha $$ α and m denote the cosmological constant, the GB coupling strength and the mass of scalar field, respectively. Then by solving the static perturbation equation, we analyze the bifurcation point at which the SdS black hole supports spherical scalar clouds, and we find that the bifurcation points match well with $$\alpha _c$$ α c on the border of unstable/stable region. Finally, after addressing that the scalarised solutions could only emerge from the scalar could with node $$k\ge 1$$ k ≥ 1 . we explicitly construct the scalarized hairy solutions for different scalar masses and compare the profile of scalar field to the corresponding scalar clouds.
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spelling doaj.art-63c94da39ce64c9aab772a02fa085f6c2022-12-22T04:30:04ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522022-10-01821011410.1140/epjc/s10052-022-10834-8Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holesZhen-Hao Yang0Guoyang Fu1Xiao-Mei Kuang2Jian-Pin Wu3Center for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou UniversityCenter for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou UniversityCenter for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou UniversityCenter for Gravitation and Cosmology, College of Physical Science and Technology, Yangzhou UniversityAbstract The black hole scalarization in a special Einstein-scalar–Gauss–Bonnet (EsGB) gravity has been widely investigated in recent years. Especially, the spontaneous scalarization of scalar-free black hole in de-Sitter (dS) spacetime possesses interesting features due to the existence of cosmological horizon. In this work, firstly, we focus on the massive scalar field perturbation on Schwarzschild dS (SdS) black hole in a special EsGB theory. By analyzing the fundamental QNM frequency and time evolution of the scalar field perturbation, we figure out the unstable/stable regions in $$(\Lambda ,\alpha )$$ ( Λ , α ) -plane as well as in $$(m,\alpha )$$ ( m , α ) -plane for various perturbation modes, where $$\Lambda $$ Λ , $$\alpha $$ α and m denote the cosmological constant, the GB coupling strength and the mass of scalar field, respectively. Then by solving the static perturbation equation, we analyze the bifurcation point at which the SdS black hole supports spherical scalar clouds, and we find that the bifurcation points match well with $$\alpha _c$$ α c on the border of unstable/stable region. Finally, after addressing that the scalarised solutions could only emerge from the scalar could with node $$k\ge 1$$ k ≥ 1 . we explicitly construct the scalarized hairy solutions for different scalar masses and compare the profile of scalar field to the corresponding scalar clouds.https://doi.org/10.1140/epjc/s10052-022-10834-8
spellingShingle Zhen-Hao Yang
Guoyang Fu
Xiao-Mei Kuang
Jian-Pin Wu
Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holes
European Physical Journal C: Particles and Fields
title Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holes
title_full Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holes
title_fullStr Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holes
title_full_unstemmed Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holes
title_short Instability of de-Sitter black hole with massive scalar field coupled to Gauss–Bonnet invariant and the scalarized black holes
title_sort instability of de sitter black hole with massive scalar field coupled to gauss bonnet invariant and the scalarized black holes
url https://doi.org/10.1140/epjc/s10052-022-10834-8
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AT guoyangfu instabilityofdesitterblackholewithmassivescalarfieldcoupledtogaussbonnetinvariantandthescalarizedblackholes
AT xiaomeikuang instabilityofdesitterblackholewithmassivescalarfieldcoupledtogaussbonnetinvariantandthescalarizedblackholes
AT jianpinwu instabilityofdesitterblackholewithmassivescalarfieldcoupledtogaussbonnetinvariantandthescalarizedblackholes