On the Induced Gravitational Collapse
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 und...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
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EDP Sciences
2018-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | https://doi.org/10.1051/epjconf/201816802005 |
| _version_ | 1819131092101234688 |
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| author | M. Becerra Laura Bianco Carlo Fryer Chris Rueda Jorge Ruffini Remo |
| author_facet | M. Becerra Laura Bianco Carlo Fryer Chris Rueda Jorge Ruffini Remo |
| author_sort | M. Becerra Laura |
| collection | DOAJ |
| description | 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 Eiso > 1052 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 Eiso < 1052 erg. We’re going to focus in identify the binary parameters that limits the BdHNe systems with the XRFs systems. |
| first_indexed | 2024-12-22T09:10:00Z |
| format | Article |
| id | doaj.art-9d5aa9db92bd417a8b835462fd5a897a |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-22T09:10:00Z |
| publishDate | 2018-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-9d5aa9db92bd417a8b835462fd5a897a2022-12-21T18:31:27ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011680200510.1051/epjconf/201816802005epjconf_icgaxiii-ik2018_02005On the Induced Gravitational CollapseM. Becerra LauraBianco CarloFryer ChrisRueda JorgeRuffini RemoThe 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 Eiso > 1052 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 Eiso < 1052 erg. We’re going to focus in identify the binary parameters that limits the BdHNe systems with the XRFs systems.https://doi.org/10.1051/epjconf/201816802005 |
| spellingShingle | M. Becerra Laura Bianco Carlo Fryer Chris Rueda Jorge Ruffini Remo On the Induced Gravitational Collapse EPJ Web of Conferences |
| title | On the Induced Gravitational Collapse |
| title_full | On the Induced Gravitational Collapse |
| title_fullStr | On the Induced Gravitational Collapse |
| title_full_unstemmed | On the Induced Gravitational Collapse |
| title_short | On the Induced Gravitational Collapse |
| title_sort | on the induced gravitational collapse |
| url | https://doi.org/10.1051/epjconf/201816802005 |
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