Abstract
Quasistationary states with energies Ω < Μ exist in the vicinity of a Schwarzchild black hole. The process of filling of these states by massive spinor particles is examined. The analysis is conducted in the Pauli approximation for small black holes ΜM≪ 1. In this case, it turns out that the distribution is a thermal distribution.
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Translated from Izvestiya Vysshikh Uchebnykh Zabedenii, Fizika, No. 8, pp. 75–77, August, 1983.
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Gal'tsov, D.V., Pomerantseva, G.V. & Chizhov, G.A. Filling of quasibound states by electrons in a schwarzchild field. Soviet Physics Journal 26, 743–745 (1983). https://doi.org/10.1007/BF00898887
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DOI: https://doi.org/10.1007/BF00898887