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Stability of scalarized charged black holes in the Einstein–Maxwell–Scalar theory

Yun Soo MyungInstitute of Basic Sciences and Department of Computer Simulation, Inje University Gimhae, 50834, Gimhae, South KoreaDe-Cheng ZouCenter for Gravitation and Cosmology and College of Physical Science and Technology, Yangzhou University, Yangzhou, 225009, China
2019en
ABI

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We analyze the stability of scalarized charged black holes in the Einstein–Maxwell–Scalar (EMS) theory with quadratic coupling. These black holes are labelled by the number of $$n=0,1,2,\ldots $$ , where $$n=0$$ is called the fundamental black hole and $$n=1,2,\ldots $$ denote the n-excited black holes. We show that the $$n=0$$ black hole is stable against full perturbations, whereas the $$n=1,2$$ excited black holes are unstable against the $$s(l=0)$$ -mode scalar perturbation. This is consistent with the EMS theory with exponential coupling, but it contrasts to the $$n=0$$ scalarized black hole in the Einstein–Gauss–Bonnet–Scalar theory with quadratic coupling. This implies that the endpoint of unstable Reissner-Nordström black holes with $$\alpha >8.019$$ is the $$n=0$$ black hole with the same q. Furthermore, we study the scalarized charged black holes in the EMS theory with scalar mass $$m^2_\phi =\alpha /\beta $$ .

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