Collision of light-like shells and mass inflation in rotating black holes

Details Collision of light-like shells and mass inflation in rotating black holes Collision of light-like shells and mass inflation in rotating black holes

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cqgra...7l.273b&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 7, Dec. 1990, p. L273-L278. Research supported by the University of Alberta

Astronomy and Astrophysics

Astrophysics

21

Astrophysics, Black Holes (Astronomy), Cosmology, Shell Stars

Scientific paper

The Dray-'t Hooft-Redmount relation, expressing conservation of energy in the collision of two lightlike thin shells is extended to the case where no symmetries are present. This relation is applied to a schematic model for the internal physics of a rotating black hole. It is shown that Hawking's quasi-local mass increases without limit near the Cauchy horizon. Previous arguments for mass inflation in spherical black holes are thus extended to the generic case.

Affiliated with

Also associated with

No associations

Rating

Collision of light-like shells and mass inflation in rotating black holes 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 Collision of light-like shells and mass inflation in rotating black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collision of light-like shells and mass inflation in rotating black holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1630123