Isometric embeddings of the reduced horizon of a Kerr-Newman black hole into Euclidean 3-space

Details Isometric embeddings of the reduced horizon of a Kerr-Newman black hole into Euclidean 3-space Isometric embeddings of the reduced horizon of a Kerr-Newman black hole into Euclidean 3-space

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cqgra..15.2303s&link_type=abstract

Classical and Quantum Gravity, Volume 15, Issue 8, pp. 2303-2310 (1998).

Computer Science

1

Scientific paper

We prove some results concerning Killing fields, isometric immersions and black hole horizons, and then combine them to arrive at conclusions concerning embeddings of reduced black hole horizons into Euclidean space. We show that not far from the Schwarzschild solution in the class of Kerr-Newman solutions of Einstein equations the reduced horizon of a black hole has a unique isometric embedding in 0264-9381/15/8/013/img1. But certain critical values of parameters describing this class exist, for which it does not take place; when the reduced horizon has negative Gauss curvature areas. We compare these parameters with the thermodynamics of black holes.

Affiliated with

Also associated with

No associations

Rating

Isometric embeddings of the reduced horizon of a Kerr-Newman black hole into Euclidean 3-space 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 Isometric embeddings of the reduced horizon of a Kerr-Newman black hole into Euclidean 3-space, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Isometric embeddings of the reduced horizon of a Kerr-Newman black hole into Euclidean 3-space will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1576434