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Population Synthesis of High Energy Transients: Relativistic Binary Merging Rates
Published online by Cambridge University Press: 14 August 2015
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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.
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- II. Joint Discussions
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- Copyright © Kluwer 1998