[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 …
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 …
First minutes of a binary-driven hypernova
We simulate the first minutes of the evolution of a binary-driven hypernova event, with a
special focus on the associated accretion processes of supernova ejecta onto the newborn …
special focus on the associated accretion processes of supernova ejecta onto the newborn …
On the x-ray, optical, and radio afterglows of the BdHN I GRB 180720B generated by synchrotron emission
Gamma-ray bursts (GRBs) are systems of unprecedented complexity across all the
electromagnetic spectrum, including the radio, optical, X-rays, gamma rays in the MeV and …
electromagnetic spectrum, including the radio, optical, X-rays, gamma rays in the MeV and …
Ten Supernova-rise in Binary Driven Gamma-ray Bursts
R Ruffini, CL Bianco, L Li, MT Mirtorabi… - arXiv preprint arXiv …, 2024 - arxiv.org
The observation of a gamma-ray burst (GRB) associated with a supernova (SN) coincides
remarkably with the energy output from a binary system comprising a very massive carbon …
remarkably with the energy output from a binary system comprising a very massive carbon …
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 …
Occurrence of gravitational collapse in the accreting neutron stars of binary-driven hypernovae
The binary-driven hypernova (BdHN) model proposes long gamma-ray bursts (GRBs)
originate in binaries composed of a carbon-oxygen (CO) star and a neutron star (NS) …
originate in binaries composed of a carbon-oxygen (CO) star and a neutron star (NS) …
On the formation of compact-object binaries from binary-driven hypernovae
We present smoothed-particle-hydrodynamics (SPH) simulations of the binary-driven
hypernova (BdHN) scenario of long gamma-ray bursts (GRBs), focusing on the binary …
hypernova (BdHN) scenario of long gamma-ray bursts (GRBs), focusing on the binary …
Multipolar Electromagnetic Emission of Newborn Magnetar
Y Wang, R Moradi, L Li - arXiv preprint arXiv:2404.09251, 2024 - arxiv.org
It is generally recognized that the electromagnetic multipolar emission from magnetars can
be used to explain radiation from Soft Gamma Repeaters (SGRs) or Anomalous X-ray …
be used to explain radiation from Soft Gamma Repeaters (SGRs) or Anomalous X-ray …
The role of a standard family of Ic supernovae in BDHN I, BDHN II, and BDHN III GRBs
A profound difference has occurred in the analysis of Gamma Ray Bursts (GRBs) initially
analyzed in the domain of gamma‐ray astronomy with the Compton Gamma Ray …
analyzed in the domain of gamma‐ray astronomy with the Compton Gamma Ray …