A Brief Review of Binary Driven Hypernova
arXiv:2201.03500 · doi:10.1142/S021827182130007X
Abstract
Binary driven hypernova (BdHN) models long gamma-ray burst (GRBs) as occurring in the binary systems involving a carbon-oxygen core (CO) 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.
arXiv commentReview paper, Published in IJMPD, Volume No. 30, Issue No. 15
References in corpus (29)
- Electron-positron pairs in physics and astrophysics: from heavy nuclei to black holes
- Hypercritical Accretion, Induced Gravitational Collapse, and Binary-Driven Hypernovae
- On the Induced Gravitational Collapse of a Neutron Star to a Black Hole by a Type Ib/c Supernova
- On the classification of GRBs and their occurrence rates
- A double component in GRB 090618: a proto-black hole and a genuinely long GRB
- On the induced gravitational collapse scenario of gamma-ray bursts associated with supernovae
- Angular Momentum Role in the Hypercritical Accretion of Binary-Driven Hypernovae
- Early X-ray Flares in GRBs
- On the Neutron Star-Black Hole Binaries Produced by Binary-driven-Hypernovae
- GRB 090618: The First Example of a Neutron Star Gravitational Collapse to a Black Hole Induced by a Type Ib/c Supernova
- On the GeV emission of the type I BdHN GRB 130427A
- SPH simulations of the induced gravitational collapse scenario of long gamma-ray bursts associated with supernovae
- Two Predictions of supernova: GRB 130427A / SN 2013cq and GRB 180728A / SN 2018fip
- The blackholic quantum
- GRB 130427A and SN 2013cq: A Multi-wavelength Analysis of An Induced Gravitational Collapse Event
- The newborn black hole in GRB 191014C proves that it is alive
- Magnetic Fields and Afterglows of BdHNe: Inferences from GRB 130427A, GRB 160509A, GRB 160625B, GRB 180728A and GRB 190114C
- On a GRB afterglow model consistent with hypernovae observations
- Neutrino Oscillations Within the Induced Gravitational Collapse Paradigm of Long Gamma-Ray Bursts
- GRB 170817A-GW170817-AT 2017gfo and the observations of NS-NS, NS-WD and WD-WD mergers
- On the last stable orbit around rapidly rotating neutron stars
- On the role of a cavity in the hypernova ejecta of GRB 190114C
- The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs
- On the ultra-relativistic Prompt Emission (UPE), the Hard and Soft X-ray Flares, and the extended thermal emission (ETE) in GRB 151027A
- Electromagnetic emission of white dwarf binary mergers
- Magnetic field screening in strong crossed electromagnetic fields
- Self-similarity and power-laws in GRB 190114C
- The inner engine of GeV-radiation-emitting gamma-ray bursts
- X-ray and GeV afterglows and sub-TeV emission of GRB 180720B
Cited by in corpus (6)
- GRB-SN Association within the Binary-Driven Hypernova Model
- The structure of the ultrarelativistic prompt emission phase and the properties of the black hole in GRB 180720B
- GRB 190829A -- A Showcase of Binary Late Evolution
- The first minutes of a binary-driven hypernova
- Self-Similarities and Power-laws in the Time-resolved Spectra of GRB 190114C, GRB 130427A, GRB 160509A, and GRB 160625B
- MeV, GeV and TeV neutrinos from binary-driven hypernovae