The intrinsic character of a black hole

Details The intrinsic character of a black hole The intrinsic character of a black hole

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cqgra...4..619l&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 4, May 1, 1987, p. 619-623.

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Kerr Effects

Scientific paper

The final shape of a Kerr black hole is investigated analytically, applying spin-coefficient notation to a space-time with a horizon assumed to be a null hypersurface of topology S2 x R. An intrinsic coordinate-free characterization is obtained, and it is pointed out that, since the axisymmetric surface of the black hole cannot be embedded in three-dimensional Euclidean space, the hypothesis that the black hole is metrically a spheroid is incorrect.

Affiliated with

Also associated with

No associations

Rating

The intrinsic character of a black hole 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 The intrinsic character of a black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The intrinsic character of a black hole will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-857489