The Universal area spectrum in single-horizon black holes

May, 2004
5 pages
Published in:
  • Phys.Rev.D 70 (2004) 044041
e-Print:
Report number:
  • KUNS-1921

Citations per year

2004200920142019202302468
Abstract:
We investigate highly damped quasinormal mode of single-horizon black holes motivated by its relation to the loop quantum gravity. Using the WKB approximation, we show that the real part of the frequency approaches the value THln3T_{\rm H}\ln 3 for dilatonic black hole as conjectured by Medved et al. and Padmanabhan. It is surprising since the area specrtum of the black hole determined by the Bohr's correspondence principle completely agrees with that of Schwarzschild black hole for any values of the electromagnetic charge or the dilaton coupling. We discuss its generality for single-horizon black holes and the meaning in the loop quantum gravity.
  • 04.60.-m
  • 04.30.-w
  • 04.70.Dy
  • 04.70.-s
  • black hole: oscillation
  • black hole: horizon
  • WKB approximation
  • quantum gravity: loop space