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 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 …
The structure of the ultrarelativistic prompt emission phase and the properties of the black hole in GRB 180720B
In analogy with GRB 190114C, we here analyze the ultrarelativistic prompt emission (UPE)
of GRB 180720B observed in the rest-frame time interval t rf= 4.84–10.89 s by Fermi-GBM …
of GRB 180720B observed in the rest-frame time interval t rf= 4.84–10.89 s by Fermi-GBM …
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 …
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 …
Unveiling the Central Engine of Core-collapse Supernovae in the Local Universe: Neutron Star or Black Hole?
MHPM van Putten, MA Abchouyeh… - The Astrophysical …, 2024 - iopscience.iop.org
The physical trigger powering supernovae following the core collapse of massive stars is
believed to involve a neutron star (NS) or a black hole (BH), depending largely on progenitor …
believed to involve a neutron star (NS) or a black hole (BH), depending largely on progenitor …
Self-similarities and Power Laws in the Time-resolved Spectra of GRB 190114C, GRB 130427A, GRB 160509A, and GRB 160625B
Binary-driven hypernova (BdHN) models have been adopted to explain the observed
properties of long gamma-ray bursts (GRBs). Here, we perform a comprehensive data …
properties of long gamma-ray bursts (GRBs). Here, we perform a comprehensive data …
Unveiling the central engine of core-collapse supernovae in the Local Universe: NS or BH?
MHPM van Putten, MA Abchouyeh… - arXiv preprint arXiv …, 2024 - arxiv.org
The physical trigger powering supernovae following the core collapse of massive stars is
believed to involve a neutron star (NS) or a black hole (BH), depending largely on progenitor …
believed to involve a neutron star (NS) or a black hole (BH), depending largely on progenitor …
From “introducing the black hole”(1971) to the discoveries of an alive black hole in GRB 190114C (2021) a collection of documents prepared in occasion of the 17th …
R Ruffini - AIP Conference Proceedings, 2024 - pubs.aip.org
From “introducing the black hole” (1971) to the discoveries of an alive black hole in GRB
190114C (2021) a collection of documents prepared in occasion of the 17th Italo-Korean …
190114C (2021) a collection of documents prepared in occasion of the 17th Italo-Korean …
On the Origin of the Long Gamma-Ray Burst Afterglow as Synchrotron Radiation from Binary-Driven Hypernovae
JA Rueda - arXiv preprint arXiv:2202.00316, 2022 - arxiv.org
Long gamma-ray bursts show an afterglow emission in the X-rays, optical, and radio
wavelengths with luminosities that fade with time with a nearly identical power-law behavior …
wavelengths with luminosities that fade with time with a nearly identical power-law behavior …