[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 …
On the GeV emission of the type I BdHN GRB 130427A
We propose that the inner engine of a type I binary-driven hypernova (BdHN) is composed
of Kerr black hole (BH) in a non-stationary state, embedded in a uniform magnetic field B 0 …
of Kerr black hole (BH) in a non-stationary state, embedded in a uniform magnetic field B 0 …
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 …
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 …
GRB 171205A: Hypernova and Newborn Neutron Star
GRB 171205A is a low-luminosity, long-duration gamma-ray burst (GRB) associated with SN
2017iuk, a broad-line type Ic supernova (SN). It is consistent with having been formed in the …
2017iuk, a broad-line type Ic supernova (SN). It is consistent with having been formed in the …
Grb 170817a-gw170817-at 2017gfo and the observations of ns-ns, ns-wd and wd-wd mergers
Abstract The LIGO-Virgo Collaboration has announced the detection of GW170817 and has
associated it with GRB 170817A. These signals have been followed after 11 hours by the …
associated it with GRB 170817A. These signals have been followed after 11 hours by the …
On the Ultra-relativistic Prompt Emission, the Hard and Soft X-Ray Flares, and the Extended Thermal Emission in GRB 151027A
We analyze GRB 151027A within the binary-driven hypernova approach, with a progenitor
of a carbon–oxygen core on the verge of a supernova (SN) explosion and a binary …
of a carbon–oxygen core on the verge of a supernova (SN) explosion and a binary …
Probing Electromagnetic Gravitational-wave Emission Coincidence in a Type I Binary-driven Hypernova Family of Long Gamma-Ray Bursts at Very High Redshift
CL Bianco, MT Mirtorabi, R Moradi… - The Astrophysical …, 2024 - iopscience.iop.org
The repointing time of the X-Ray Telescope (XRT) instrument on the Neil Gehrels Swift
Observatory satellite has posed challenges in observing and studying the early X-ray …
Observatory satellite has posed challenges in observing and studying the early X-ray …
On the universal late X-ray emission of binary-driven hypernovae and its possible collimation
It has previously been discovered that there is a universal power-law behavior exhibited by
the late X-ray emission (LXRE) of a" golden sample" of six long energetic GRBs, when …
the late X-ray emission (LXRE) of a" golden sample" of six long energetic GRBs, when …