Self-gravitating collapsing star and black hole spin-up in long gamma ray bursts
Self-gravitating collapsing star and black hole spin-up in long gamma ray bursts
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Long Gamma Ray Bursts (GRBs) originate from the collapse of massive, rotating stars. We aim to model the process of stellar collapse in the scenario of a self-gravitating collapsing star. We account for the changes in Kerr metric induced by the growth of the black hole, accretion of angular momentum, as well as the self-gravity effect due to a larg...
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Full title
Self-gravitating collapsing star and black hole spin-up in long gamma ray bursts
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TN_cdi_proquest_journals_2795864170
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2795864170
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2304.01342
