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[en] In the vicinity of the Schwarzschild black hole there exist quasistationary states for ω < μ energies. The process of filling by massive spinor particles is considered in the Pauli approximation for small black holes, when μM << 1. It turns out that the distribution is thermal
Journal
Izvestiya Vysshikh Uchebnykh Zavedenij, Fizika; ISSN 0021-3411; 
; v. 26(8); p. 75-77
; v. 26(8); p. 75-77