Stability of a vacuum non-singular black hole

DOI10.1088/0264-9381/22/12/003zbMATH Open1074.83015arXivgr-qc/0409049OpenAlexW2076033446MaRDI QIDQ5314986

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Publication date: 5 September 2005

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Abstract: This is the first of series of papers in which we investigate stability of the spherically symmetric space-time with de Sitter center. Geometry, asymptotically Schwarzschild for large $r$ and asymptotically de Sitter as $ro0$, describes a vacuum nonsingular black hole for $mgeq{m}_{cr}$ and particle-like self-gravitating structure for $m<m_{cr}$ where a critical value $m_{cr}$ depends on the scale of the symmetry restoration to de Sitter group in the origin. In this paper we address the question of stability of a vacuum non-singular black hole with de Sitter center to external perturbations. We specify first two types of geometries with and without changes of topology. Then we derive the general equations for an arbitrary density profile and show that in the whole range of the mass parameter $m$ objects described by geometries with de Sitter center remain stable under axial perturbations. In the case of the polar perturbations we find criteria of stability and study in detail the case of the density profile $ho(r)=h{o}_0{e}^{-r^3/r_0^2{r}_g}$ where $h{o}_0$ is the density of de Sitter vacuum at the center, $r_0$ is de Sitter radius and $r_g$ is the Schwarzschild radius.

Full work available at URL: https://arxiv.org/abs/gr-qc/0409049

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