Quantum Theory and Thermodynamics of Schwarzschild Black Holes

Details Quantum Theory and Thermodynamics of Schwarzschild Black Holes Quantum Theory and Thermodynamics of Schwarzschild Black Holes

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.1519k&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

Starting from a symplectic reduction of the pure Schwarzschild gravitational system in D ≥ 4 space-time dimensions and an ensuing quantization in terms of the group SU(1,1) yields a universal spectrum AD-2 α n + k, n = 0, 1,...,k ∈ (0, 1] fixed, of the horizon area, and, because AD-2(M) is a function of the mass M, a corresponding spectrum of M. Attributing the Z(2)-valued degree of freedom "orientation" to each basic area quantum yields a degeneracy of the levels which, combined with the mass spectrum, implies the Bekenstein entropy and the Hawking temperature, up to a constant.

Affiliated with

Also associated with

No associations

Rating

Quantum Theory and Thermodynamics of Schwarzschild 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 Quantum Theory and Thermodynamics of Schwarzschild Black Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quantum Theory and Thermodynamics of Schwarzschild Black Holes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1167901