On the Induced Gravitational Collapse of a Neutron Star to a Black Hole by a Type Ib/c Supernova
arXiv:1206.1684 · doi:10.1088/2041-8205/758/1/L7
Abstract
It is understood that the Supernovae (SNe) associated to Gamma Ray Bursts (GRBs) are of type Ib/c. The temporal coincidence of the GRB and the SN represents still a major enigma of Relativistic Astrophysics. We elaborate here, from the earlier paradigm, that the concept of induced gravitational collapse is essential to explain the GRB-SN connection. The specific case of a close (orbital period <1 h) binary system composed of an evolved star with a Neutron Star (NS) companion is considered. We evaluate the accretion rate onto the NS of the material expelled from the explosion of the core progenitor as a type Ib/c SN, and give the explicit expression of the accreted mass as a function of the nature of the components and binary parameters. We show that the NS can reach, in a few seconds, the critical mass and consequently gravitationally collapses to a Black Hole. This gravitational collapse process leads to the emission of the GRB.
ApJ Letters; in press
References in corpus (7)
- The Supernova -- Gamma-Ray Burst Connection
- Constraints on neutron star radii based on chiral effective field theory interactions
- The nuclear symmetry energy and stability of matter in neutron star
- Neutron star equilibrium configurations within a fully relativistic theory with strong, weak, electromagnetic, and gravitational interactions
- Equation of state of the neutron star matter, and the nuclear symmetry energy
- GRB060614: a "fake" short GRB from a merging binary system
- GRB 090227B: the missing link between the genuine short and long GRBs
Cited by in corpus (54)
- Fast Rotating Neutron Stars with Realistic Nuclear Matter Equation of State
- Hypercritical Accretion, Induced Gravitational Collapse, and Binary-Driven Hypernovae
- On the classification of GRBs and their occurrence rates
- 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
- SPH simulations of the induced gravitational collapse scenario of long gamma-ray bursts associated with supernovae
- On Binary Driven Hypernovae and their nested late X-ray emission
- The blackholic quantum
- Two Predictions of supernova: GRB 130427A / SN 2013cq and GRB 180728A / SN 2018fip
- GRB 130427A and SN 2013cq: A Multi-wavelength Analysis of An Induced Gravitational Collapse Event
- GRB 090227B: the missing link between the genuine short and long GRBs
- Magnetic Fields and Afterglows of BdHNe: Inferences from GRB 130427A, GRB 160509A, GRB 160625B, GRB 180728A and GRB 190114C
- The newborn black hole in GRB 191014C proves that it is alive
- A white dwarf merger as progenitor of the anomalous X-ray pulsar 4U 0142+61?
- Fast ejecta as a potential way to distinguish black holes from neutron stars in high-mass gravitational-wave events
- Novel distance indicator for gamma-ray bursts associated with supernovae
- GRB 110709B in the Induced Gravitational Collapse paradigm
- On a GRB afterglow model consistent with hypernovae observations
- Neutrino Oscillations Within the Induced Gravitational Collapse Paradigm of Long Gamma-Ray Bursts
- GRB 140619B: a short GRB from a binary neutron star merger leading to black hole formation
- On the last stable orbit around rapidly rotating neutron stars
- The quest for new correlations in the realm of the Gamma-Ray Burst -- Supernova connection
- The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs
- GRB 090510: a genuine short-GRB from a binary neutron star coalescing into a Kerr-Newman black hole
- Globally visible singularity in an astrophysical setup
- On the ultra-relativistic Prompt Emission (UPE), the Hard and Soft X-ray Flares, and the extended thermal emission (ETE) in GRB 151027A
- On the rate and on the gravitational wave emission of short and long GRBs
- GRB-SN Association within the Binary-Driven Hypernova Model
- Induced Gravitational Collapse, Binary-Driven Hypernovae, Long Gramma-ray Bursts and Their Connection with Short Gamma-ray Bursts
- Induced gravitational collapse at extreme cosmological distances: the case of GRB 090423
- The structure of the ultrarelativistic prompt emission phase and the properties of the black hole in GRB 180720B
- GRB 081024B and GRB 140402A: two additional short GRBs from binary neutron star mergers
- GRB 190829A -- A Showcase of Binary Late Evolution
- On the X-ray, optical and radio afterglows of the BdHN I GRB 180720B generated by the synchrotron emission
- The first minutes of a binary-driven hypernova
- GRB 171205A: Hypernova and Newborn Neutron Star
- Evidence for the transition of a Jacobi ellipsoid into a Maclaurin spheroid in gamma-ray bursts
- A Brief Review of Binary Driven Hypernova
- On the universal late X-ray emission of binary-driven hypernovae and its possible collimation
- Magnetized black holes: interplay between charge and rotation
- Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH
- Induced Gravitational Collapse in the BATSE era: the case of GRB 970828
- Long gamma-ray burst light curves as the result of a common stochastic pulse-avalanche process
- Neutron star binaries produced by binary-driven hypernovae, their mergers, and the link between long and short GRBs
- Probing electromagnetic-gravitational wave emission coincidence in type I binary-driven hypernova family of long GRBs at very-high redshift
- The Quantum Emission of an Alive Black Hole
- A common behavior in the late X-ray afterglow of energetic GRB-SN systems
- An advanced pulse-avalanche stochastic model of long gamma-ray burst light curves
- Some Recent Results on Neutrino Oscillations in Hypercritical Accretion
- MeV, GeV and TeV neutrinos from binary-driven hypernovae
- Luminous Fast Blue Optical Transients and Type Ibn/Icn SNe from Wolf-Rayet/Black Hole Mergers