Metric of a Nonrotating Black Hole in a Tidal Environment

Details Metric of a Nonrotating Black Hole in a Tidal Environment Metric of a Nonrotating Black Hole in a Tidal Environment

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aps..aprl10002v&link_type=abstract

American Physical Society, 2008 APS April Meeting and HEDP/HEDLA Meeting, April 11-15, 2008, abstract #L10.002

Physics

Scientific paper

We consider the perturbed field of a Schwarzschild black hole with a mass M much smaller than the local radius of curvature R generated by the external Universe. We discuss light-cone coordinates used to represent the combined metric of the black hole and external matter. The metric of the external Universe is found as an expansion in STF harmonics, then the Einstein equations are solved for the full metric at the first nonlinear order O((M/R)^4). We discuss the gauge freedom and analize the solution.

Affiliated with

Also associated with

No associations

Rating

Metric of a Nonrotating Black Hole in a Tidal Environment 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 Metric of a Nonrotating Black Hole in a Tidal Environment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Metric of a Nonrotating Black Hole in a Tidal Environment will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1424838