Gravitomagnetic interaction of a Kerr black hole with a magnetic field as the source of the jetted GeV radiation of gamma-ray bursts
We show that the gravitomagnetic interaction of a Kerr black hole (BH) with a surrounding
magnetic field induces an electric field that accelerates charged particles to ultra-relativistic …
magnetic field induces an electric field that accelerates charged particles to ultra-relativistic …
[PDF][PDF] X-ray Swift observations of SN 2018cow
LE Rivera Sandoval, TJ Maccarone… - Monthly Notices of …, 2018 - academic.oup.com
Supernova (SN) 2018cow is an optical transient detected in the galaxy CGCG 137–068. It
has been classified as an SN due to various characteristics in its optical spectra. The …
has been classified as an SN due to various characteristics in its optical spectra. The …
[HTML][HTML] Induced Gravitational Collapse, Binary-Driven Hypernovae, Long Gramma-ray Bursts and Their Connection with Short Gamma-ray Bursts
There is increasing observational evidence that short and long Gamma-ray bursts (GRBs)
originate in different subclasses, each one with specific energy release, spectra, duration …
originate in different subclasses, each one with specific energy release, spectra, duration …
[HTML][HTML] GRB-SN Association within the Binary-driven Hypernova Model
Y Aimuratov, LM Becerra, CL Bianco… - The Astrophysical …, 2023 - iopscience.iop.org
Abstract Observations of supernovae (SNe) Ic occurring after the prompt emission of long
gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model …
gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model …
The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs
We recall evidence that long gamma-ray bursts (GRBs) have binary progenitors and give
new examples. Binary-driven hypernovae (BdHNe) consist of a carbon–oxygen core …
new examples. Binary-driven hypernovae (BdHNe) consist of a carbon–oxygen core …
A brief review of binary-driven hypernova
Binary-driven hypernova (BdHN) models long gamma-ray burst (GRB) as occurring in the
binary systems involving a carbon–oxygen core (CO core) and a companion neutron star …
binary systems involving a carbon–oxygen core (CO core) and a companion neutron star …
SPH simulations of the induced gravitational collapse scenario of long gamma-ray bursts associated with supernovae
We present the first three-dimensional smoothed particle hydrodynamics simulations of the
induced gravitational collapse scenario of long-duration gamma-ray bursts (GRBs) …
induced gravitational collapse scenario of long-duration gamma-ray bursts (GRBs) …
Two predictions of supernova: GRB 130427A/SN 2013cq and GRB 180728A/SN 2018fip
Abstract On 2018 July 28, GRB 180728A triggered Swift satellites and, soon after the
determination of the redshift, we identified this source as a type II binary-driven hypernova …
determination of the redshift, we identified this source as a type II binary-driven hypernova …
GRB 190829A—A Showcase of Binary Late Evolution
GRB 190829A is the fourth-closest gamma-ray burst to date (z= 0.0785). Owing to its wide
range of radio, optical, X-ray, and very-high-energy observations by HESS, it has become an …
range of radio, optical, X-ray, and very-high-energy observations by HESS, it has become an …
Magnetic fields and afterglows of BdHNe: inferences from GRB 130427A, GRB 160509A, GRB 160625B, GRB 180728A, and GRB 190114C
GRB 190114C is the first binary-driven hypernova (BdHN) fully observed from initial
supernova (SN) appearance to the final emergence of the optical SN signal. It offers an …
supernova (SN) appearance to the final emergence of the optical SN signal. It offers an …