We study the evolution of a five-dimensional rotating black hole emitting
scalar field radiation via the Hawking process for arbitrary initial values of
the two rotation parameters $a$ and $b$. It is found that any such black hole
whose initial rotation parameters are both nonzero evolves toward an asymptotic
state
$a/M^{1/2}=b/M^{1/2}={\rm const}(\neq 0)$, where this constant is independent
of the initial values of $a$ and $b$.Comment: 6 pages, 6 figure
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 TH 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.
We reexmine some proposals of black hole entropy in loop quantum gravity
(LQG) and consider a new possible choice of the Immirzi parameter which has not
been pointed out so far. We also discuss that a new idea is inevitable if we
regard the relation between the area spectrum in LQG and that in the
quasinormal mode analysis seriously.Comment: 4 pages, 1 figure, error corrected, PRD published versio
We investigate highly damped quasinormal modes of regular black hole coupled to nonlinear electrodynamics. Using the WKB approximation combined with complex-integration technique, we show that the real part of the frequency disappears in the highly damped limit. If we use the Bohr's correspondence principle, the area spectrum of this black hole is continuous. We discuss its implication in the loop quantum gravity.
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