On Quantization of Black Holes

Abstract

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} = 8πl_p^2 [\sqrt{N(N+1)} + \sqrt{N(N+1) - j(j+1)} ]. Here both $N$ and $j$ are nonnegative integers or half-integers.

4 pages, latex

References in corpus (2)

• On the Quantum Levels of Isolated Spherically Symmetric Gravitational Systems
• Are There Topological Black Hole Solitons in String Theory?

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