We also estimate the rate of gravitational wave events received from MBH mergers across all redshifts. At the end of their lives the first stars may explode in supernovae that are associated with gamma ray bursts (GRBs). Provided these are in principle detectable we have estimated the expected rate of events observed
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
Context. Gravitational wave interferometers have proven the existence of a new class of binary black...
The Galactic massive black hole (MBH), with a mass of M•= 3.6 × 106 M⊙, is the closest known MBH, at...
We also estimate the rate of gravitational wave events received from MBH mergers across all redshift...
The first stars forming in minihaloes at redshifts greater than 20 may have been very massive and co...
Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling h...
Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling h...
International audienceGravitational waves (GWs) provide a revolutionary tool to investigate yet unob...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
In this letter we carry out the first systematic investigation of the expected gravitational wave (G...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
We study the gravitational wave emission from the first stars, which are assumed to be very massive ...
Gravitational waves (GWs) provide a revolutionary tool to investigate yet unobserved astrophysical o...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
Context. Gravitational wave interferometers have proven the existence of a new class of binary black...
The Galactic massive black hole (MBH), with a mass of M•= 3.6 × 106 M⊙, is the closest known MBH, at...
We also estimate the rate of gravitational wave events received from MBH mergers across all redshift...
The first stars forming in minihaloes at redshifts greater than 20 may have been very massive and co...
Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling h...
Recent numerical simulations reveal that the isothermal collapse of pristine gas in atomic cooling h...
International audienceGravitational waves (GWs) provide a revolutionary tool to investigate yet unob...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
In this letter we carry out the first systematic investigation of the expected gravitational wave (G...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
We study the gravitational wave emission from the first stars, which are assumed to be very massive ...
Gravitational waves (GWs) provide a revolutionary tool to investigate yet unobserved astrophysical o...
International audienceContext. Gravitational wave interferometers have proven the existence of a new...
Context. Gravitational wave interferometers have proven the existence of a new class of binary black...
The Galactic massive black hole (MBH), with a mass of M•= 3.6 × 106 M⊙, is the closest known MBH, at...