Other
Scientific paper
Sep 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004phrvd..70f4038e&link_type=abstract
Physical Review D, vol. 70, Issue 6, id. 064038
Other
1
Classical Black Holes
Scientific paper
We present two families of solutions (g,Φ) of the Einstein-Klein-Gordon system minimally coupled to gravity, massless scalar field equations possessing a regular R×S2 bifurcating Killing horizon. The solutions may be interpreted as describing the metric g and the field Φ 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 Φ. 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 Φ relaxes into a configuration so that its energy-momentum tensor Tμν on the Killing horizon obeys the property: Tμνlμlν=0 where lμ 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 R×S1×S1 event horizon.
Estevez-Delgado J.
Zannias Thomas
No associations
LandOfFree
Distorted black holes of the Einstein-Klein-Gordon system does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Distorted black holes of the Einstein-Klein-Gordon system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distorted black holes of the Einstein-Klein-Gordon system will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-803047