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- W2783306251 abstract "The induced gravitational collapse (IGC) paradigm has been applied to explain the long gamma ray burst (GRB) associated with type Ic supernova, and recently the Xray flashes (XRFs). The progenitor is a binary systems of a carbon-oxygen core (CO) and a neutron star (NS). The CO core collapses and undergoes a supernova explosion which triggers the hypercritical accretion onto the NS companion (up to 10 -2 M ⊙ s -1 ). For the binary driven hypernova (BdHNe), the binary system is enough bound, the NS reach its critical mass, and collapse to a black hole (BH) with a GRB emission characterized by an isotropic energy E iso > 10 52 erg. Otherwise, for binary systems with larger binary separations, the hypercritical accretion onto the NS is not sufficient to induced its gravitational collapse, a X-ray flash is produced with E iso < 10 52 erg. We’re going to focus in identify the binary parameters that limits the BdHNe systems with the XRFs systems." @default.
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- W2783306251 date "2018-01-01" @default.
- W2783306251 modified "2023-09-25" @default.
- W2783306251 title "On the Induced Gravitational Collapse" @default.
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- W2783306251 doi "https://doi.org/10.1051/epjconf/201816802005" @default.
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