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article · 1998

Population Synthesis of High Energy Transients: Relativistic Binary Merging Rates

Binary relativistic stars merging — the most powerful high energy transient in the Universe: L merging ˜ Mc 2 /R g /c = c 5 /G ˜ 10 58 erg/s . That is equal ...

0 citationsDOI: https://doi.org/10.1017/s1539299600018761Open accessPDF reported by metadataFull text reported by metadata
Population Synthesis of High Energy Transients: Relativistic Binary Merging Rates