English

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

General Relativity and Quantum Cosmology 2019-08-15 v2 High Energy Physics - Theory

Abstract

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,n=0,1,2,\cdots, where n=0n=0 is called the fundamental black hole and n=1,2,n=1,2,\cdots denote the nn-excited black holes. We show that the n=0n=0 black hole is stable against full perturbations, whereas the n=1,2n=1,2 excited black holes are unstable against the s(l=0)s(l=0)-mode scalar perturbation. This is consistent with the EMS theory with exponential coupling, but it contrasts to the n=0n=0 scalarized black hole in the Einstein-Gauss-Bonnet-Scalar theory with quadratic coupling. This implies that the endpoint of unstable Reissner-Nordstr\"{o}m black holes with α>8.019\alpha>8.019 is the n=0n=0 black hole with the same qq. Furthermore, we study the scalarized charged black holes in the EMS theory with scalar mass mϕ2=α/βm^2_\phi=\alpha/\beta.

Keywords

Cite

@article{arxiv.1904.09864,
  title  = {Stability of scalarized charged black holes in the Einstein-Maxwell-Scalar theory},
  author = {Yun Soo Myung and De-Cheng Zou},
  journal= {arXiv preprint arXiv:1904.09864},
  year   = {2019}
}

Comments

23 pages, 11 figures. arXiv admin note: text overlap with arXiv:1812.03604