Neutrino Oscillations in Neutrino-Dominated Accretion Around Rotating Black Holes
In the binary-driven hypernova model of long gamma-ray bursts, a carbon–oxygen star explodes as a supernova in the presence of a neutron star binary companion in close orbit. Hypercritical (i.e., highly super-Eddington) accretion of the ejecta matter onto the neutron star sets in, making it reach th...
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| Príomhchruthaitheoirí: | , , |
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| Formáid: | Artigo |
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MDPI AG
2021-01-01
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| Sraith: | Universe |
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| Rochtain ar líne: | https://www.mdpi.com/2218-1997/7/1/7 |
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