A simple argument is presented in favour of the equidistant spectrum for the horizon area of a black hole in semiclassical limit. The following quantization rules for the mass MN and horizon area ANj are proposed: MN = mp[N(N + 1)]1/4; ANj = 8πl2 p[√N(N + 1) + √N(N + 1) - j(j + 1)]. Here both N and j are nonnegative integers or half-integers.

Original languageEnglish
Pages (from-to)19-21
Number of pages3
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume431
Issue number1-2
DOIs
StatePublished - 9 Jul 1998
Externally publishedYes

    Scopus subject areas

  • Nuclear and High Energy Physics

ID: 36645712