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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2001, Volume 74, Issue 6, Pages 330–334
(Mi jetpl4210)
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This article is cited in 9 scientific papers (total in 9 papers)
GRAVITY, ASTROPHYSICS
Efficiency of electron-positron pair production by neutrino flux from accretion disk of a Kerr black hole
A. A. Gvozdev, I. S. Ognev P. G. Demidov Yaroslavl State University
Abstract:
Dominant processes of neutrino production and neutrino-induced $e^+e^-$-pair production are examined in the model of a disk hyperaccreting onto a Kerr black hole. The efficiency of plasma production is analytically estimated for both the presence and the absence of a strong magnetic field. It is shown that the efficiency of plasma production by a neutrino flux from the disk in this model is no more than several tenths of percent and, therefore, cannot account for the origin of cosmological gamma-ray bursts.
Received: 18.07.2001 Revised: 21.08.2001
Citation:
A. A. Gvozdev, I. S. Ognev, “Efficiency of electron-positron pair production by neutrino flux from accretion disk of a Kerr black hole”, Pis'ma v Zh. Èksper. Teoret. Fiz., 74:6 (2001), 330–334; JETP Letters, 74:6 (2001), 298–301
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https://www.mathnet.ru/eng/jetpl4210 https://www.mathnet.ru/eng/jetpl/v74/i6/p330
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Abstract page: | 162 | Full-text PDF : | 118 | References: | 1 |
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