Non-Rotating BTZ Black Hole Area Spectrum from Quasi-normal Modes

Details Non-Rotating BTZ Black Hole Area Spectrum from Quasi-normal Modes Non-Rotating BTZ Black Hole Area Spectrum from Quasi-normal Modes

2003-11-23

arxiv.org/abs/hep-th/0311221v2

Class.Quant.Grav. 21 (2004) 1453-1458

Physics

High Energy Physics

High Energy Physics - Theory

7 pages, no figure, some refs added, clarifying comments added, no physics changed, version to appear in Class. Quant. Grav

Scientific paper

10.1088/0264-9381/21/6/012

In this paper, by using the quasi-normal frequencies for non-rotating BTZ black hole derived by Cardos and Lemos, also via Bohr-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. The result for the area of event horizon is $A_{n}=2\pi \sqrt{\frac{nm \hbar}{\Lambda}}$ which is not equally spaced, in contrast with area spectrum of black hole in higher dimension.

Affiliated with

Also associated with

No associations

Rating

Non-Rotating BTZ 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 Non-Rotating BTZ 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 Non-Rotating BTZ Black Hole Area Spectrum from Quasi-normal Modes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-495558