Near Extremal Schwarzschild-de Sitter Black Hole Area Spectrum from Quasi-normal Modes

Details Near Extremal Schwarzschild-de Sitter Black Hole Area Spectrum from Quasi-normal Modes Near Extremal Schwarzschild-de Sitter Black Hole Area Spectrum from Quasi-normal Modes

2004-01-11

arxiv.org/abs/hep-th/0401063v1

Gen.Rel.Grav. 37 (2005) 1411-1417

Physics

High Energy Physics

High Energy Physics - Theory

7 pages, no figure

Scientific paper

10.1007/s10714-005-0125-9

Using the quasi-normal modes frequency of near extremal Schwarzschild-de Sitter black holes, we obtain area and entropy spectrum for black hole horizon. By using Boher-Sommerfeld quantization for an adiabatic invariant $I=\int {dE\over \omega(E)}$, which $E$ is the energy of system and $\omega(E)$ is vibrational frequency, we leads to an equally spaced mass spectrum. In the other term we extend directly the Kunstatter's approach [7] to determine mass and entropy spectrum of near extremal Schwarzschild-de Sitter black holes which is asymptotically de Sitter rather than asymptotically flat.

Affiliated with

Also associated with

No associations

Rating

Near Extremal Schwarzschild-de Sitter Black Hole Area Spectrum from Quasi-normal Modes 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 Near Extremal Schwarzschild-de Sitter Black Hole Area Spectrum from Quasi-normal Modes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Near Extremal Schwarzschild-de Sitter Black Hole Area Spectrum from Quasi-normal Modes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-166743