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Population Synthesis of High Energy Transients: Relativistic Binary Merging Rates

Published online by Cambridge University Press:  14 August 2015

V.M. Lipunov
V.M. Lipunov*
Affiliation:
Sternberg Astronomical InstituteUniversitetskiy pr.13, Moscow, 119899, Russia

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Binary relativistic stars merging — the most powerful high energy transient in the Universe: Lmerging ˜ Mc2/Rg/c = c5/G ˜ 1058 erg/s. That is equal to Planckian luminosity (Lipunov 1992) Lplanck = EPlanck/tplanck = C5/G.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 779 - 782
Copyright
Copyright © Kluwer 1998

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