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arXiv · 2201.03500

A Brief Review of Binary Driven Hypernova

Jorge A. Rueda·Remo Ruffini·Rahim Moradi·Yu Wang
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Abstract

Binary driven hypernova (BdHN) models long gamma-ray burst (GRBs) as occurring in the binary systems involving a carbon-oxygen core (CO$_{\rm core}$) and a companion neutron star (NS) or a black hole (BH). This model, first proposed in 2012, succeeds and improves upon the fireshell model and the induced gravitational collapse (IGC) paradigm. After nearly a decade of development, the BdHN model has reached a nearly complete structure, explaining all the observables of long bursts into its theoretical framework, and has given a refined classification of long GRBs according to the original properties of the progenitors. In this article, we present a summary of the BdHN model and the physical processes at work in each of the envisaged Episodes during its occurrence and lifetime, duly contextualized in the framework of GRB observations.

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Jorge A. Rueda, Remo Ruffini, Rahim Moradi, Yu Wang. 2022-01-10. A Brief Review of Binary Driven Hypernova. https://doi.org/10.1142/s021827182130007x

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