Cosmic neutron-star merger rate and gravitational waves constrained by the r-process nucleosynthesis

The cosmic evolution of the neutron-star merger (NSM) rate can be deduced from the observed cosmic star formation rate. This allows us to estimate the rate expected in the horizon of the gravitational wave detectors advanced Virgo and advanced LIGO and to compare those rates with independent predict...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-01, Vol.455 (1), p.17-34
Hauptverfasser:	Vangioni, Elisabeth, Goriely, Stéphane, Daigne, Frédéric, François, Patrick, Belczynski, Krzysztof
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Chemistry Coalescence Coalescing Cosmology Detectors Evolution Gravitational waves Horizon Mathematical analysis Metallicity Neutrons Physics Pulsars Supernovae Time series
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