Quantum black hole. II.

Details Quantum black hole. II. Quantum black hole. II.

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pthph..97..873c&link_type=abstract

Prog. Theor. Phys., Vol. 97, No. 6, p. 873 - 880

Mathematics

Logic

3

Black Holes: Quantum Gravity, Black Holes: Cosmology

Scientific paper

It is believed that the spacetime of the Planckian era of the universe can be described by the de Sitter metric. Primordial black holes should originate from ordinary or generalized gravitational instantons. The probability of black hole creation in the de Sitter space background is the exponential of the negative of its Euclidean action. The author shows that the probability for the creation of a spherically symmetric, charged or neutral black hole is the exponential of the total entropy of the universe. The entropy is one quarter of the sum of the black hole and cosmological horizon areas.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1481421