Exact Physical Black Hole States in Generic 2-D Dilaton Gravity

Details Exact Physical Black Hole States in Generic 2-D Dilaton Gravity Exact Physical Black Hole States in Generic 2-D Dilaton Gravity

1996-06-20

arxiv.org/abs/hep-th/9606134v1

Phys.Lett. B389 (1996) 231-237

Physics

High Energy Physics

High Energy Physics - Theory

11 pages, Revtex

Scientific paper

10.1016/S0370-2693(96)01261-0

The quantum mechanics of black holes in generic 2-D dilaton gravity is considered. The Hamiltonian surface terms are derived for boundary conditions corresponding to an eternal black hole with slices on the interior ending on the horizon bifurcation point. The quantum Dirac constraints are solved exactly for these boundary conditions to yield physical eigenstates of the energy operator. The solutions are obtained in terms of geometrical phase space variables that were originally used by Cangemi, Jackiw and Zwiebach in the context of string inspired dilaton gravity. The spectrum is continuous in the Lorentzian sector, but in the Euclidean sector the thermodynamic entropy must be $2\pi n/G$ where $n$ is an integer. The general class of models considered contains as special cases string inspired dilaton gravity, Jackiw-Teitelboim gravity and spherically symmetry gravity.

Affiliated with

Also associated with

No associations

Rating

Exact Physical Black Hole States in Generic 2-D Dilaton Gravity 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 Exact Physical Black Hole States in Generic 2-D Dilaton Gravity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Exact Physical Black Hole States in Generic 2-D Dilaton Gravity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-66879