Rotating, radiating black holes, inflation, and cosmic censorship

Details Rotating, radiating black holes, inflation, and cosmic censorship Rotating, radiating black holes, inflation, and cosmic censorship

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvd..51.6783k&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 51, Issue 12, 15 June 1995, pp.6783-6787

Mathematics

Logic

7

Singularities And Cosmic Censorship, Black Holes, Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

The Mallett model of a charged, rotating, evaporating black hole in an inflationary universe is examined. The structure and location of the timelike limit surfaces, apparent horizons, and event horizons are determined. It is noted that a coupling between the cosmological constant and the angular momentum of the black hole produces an axially symmetric deformation of the event horizons which is not seen in noninflationary models. The cosmic censorship conjecture is considered for this model. It is demonstrated that the inflation-rotation coupling can lead to quasinaked primordial singularities in the latter stages of inflation. Such singularities are visible from equatorial regions, but not visible from polar regions.

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