On Quantization of Black Holes

Details On Quantization of Black Holes On Quantization of Black Holes

1998-04-02

arxiv.org/abs/gr-qc/9804004v1

Heavy Ion Phys. 8 (1998) 301-305; Phys.Lett. B431 (1998) 19-21

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, latex

Scientific paper

10.1016/S0370-2693(98)00580-2

A simple argument is presented in favour of the equidistant spectrum in
semiclassical limit for the horizon area of a black hole. The following
quantization rules for the mass $M_N$ and horizon area $A_{Nj}$ are proposed:
M_N = m_p [N(N+1)]^{1/4}; A_{Nj} = 8\pi l_p^2 [\sqrt{N(N+1)} + \sqrt{N(N+1) -
j(j+1)} ]. Here both $N$ and $j$ are nonnegative integers or half-integers.

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