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• W2079431983 abstract "We present two families of solutions $(g,ensuremath{Phi})$ of the Einstein-Klein-Gordon system minimally coupled to gravity, massless scalar field equations possessing a regular $mathbb{R}ifmmodetimeselsetexttimesfi{}{S}^{2}$ bifurcating Killing horizon. The solutions may be interpreted as describing the metric $g$ and the field $ensuremath{Phi}$ in an open vicinity containing the event horizon of a Schwarzschild black hole interacting with an exterior, static-axisymmetric distribution of matter carrying scalar charges generating $ensuremath{Phi}$. One family of the solution possesses a spherical bifurcation two sphere and may be interpreted as generated by a distribution of matter carrying scalar charges but of negligible self-gravity. The other family describes an axisymmetric horizon with the distortion caused by the self-gravity of the external matter. For both classes of solutions the scalar field $ensuremath{Phi}$ relaxes into a configuration so that its energy-momentum tensor ${T}^{ensuremath{mu}ensuremath{nu}}$ on the Killing horizon obeys the property: ${T}^{ensuremath{mu}ensuremath{nu}}{l}_{ensuremath{mu}}{l}_{ensuremath{nu}}=0$ where ${l}^{ensuremath{mu}}$ is a null vector normal to the horizon. It is also indicated that the Einstein-Klein-Gordon system ought to admit distorted black holes characterized by an $mathbb{R}ifmmodetimeselsetexttimesfi{}{S}^{1}ifmmodetimeselsetexttimesfi{}{S}^{1}$ event horizon." @default.
• W2079431983 created "2016-06-24" @default.
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• W2079431983 date "2004-09-30" @default.
• W2079431983 modified "2023-10-17" @default.
• W2079431983 title "Distorted black holes of the Einstein-Klein-Gordon system" @default.
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• W2079431983 doi "https://doi.org/10.1103/physrevd.70.064038" @default.
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