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- W4230291205 abstract "In the case of spherical symmetric accretion into a black hole, the matter may be heated up to the temperature KT = 0.1 m p c 2 (Kolykhalov and Sunyaev, 1979). In such a hot plasma inelastic collisions of protons may produce Π° which is the gamma quantum source. In this work we determined γ-rays production spectrum in the comoving plasma reference frame, expected γ-rays spectrum for the case of spherica symmetric accretion of matter into a black hole and the upper limit to the number of black holes in Galaxy is evaluated." @default.
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- W4230291205 date "1981-01-01" @default.
- W4230291205 modified "2023-10-14" @default.
- W4230291205 title "High Energy Gamma Rays from Accretion Disc" @default.
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- W4230291205 doi "https://doi.org/10.1017/s0074180900074842" @default.
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