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 …

GRB 171205A: Hypernova and Newborn Neutron Star

Y Wang, LM Becerra, CL Fryer, JA Rueda… - The Astrophysical …, 2023 - iopscience.iop.org
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 …

First minutes of a binary-driven hypernova

LM Becerra, R Moradi, JA Rueda, R Ruffini, Y Wang - Physical Review D, 2022 - APS
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 …

Extracting the energy and angular momentum of a Kerr black hole

JA Rueda, R Ruffini - The European Physical Journal C, 2023 - Springer
It has been thought for decades that rotating black holes (BHs) power the energetic gamma-
ray bursts (GRBs) and active galactic nuclei (AGNs), but the mechanism that extracts the BH …

On the x-ray, optical, and radio afterglows of the BdHN I GRB 180720B generated by synchrotron emission

JA Rueda, L Li, R Moradi, R Ruffini… - The Astrophysical …, 2022 - iopscience.iop.org
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 …

Evidence for the transition of a Jacobi ellipsoid into a Maclaurin spheroid in gamma-ray bursts

JA Rueda, R Ruffini, L Li, R Moradi, JF Rodriguez… - Physical Review D, 2022 - APS
In the binary-driven hypernova (BdHN) scenario, long gamma-ray bursts (GRBs) originate in
a cataclysmic event that occurs in a binary system composed of a carbon-oxygen (CO) star …

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 …

Accelerated protons produced by the magnetic Penrose process in Sgr

M Oh, MG Park - Physical Review D, 2024 - APS
Typical mechanisms to extract energies from a rotating black hole are the Blandford-Znajek
process and the Penrose process. The Penrose process requires a special condition that is …

[PDF][PDF] Determining the Mass and Spin of the Black Hole in GRB 220101A Using 0.1-100 GeV Data Observed by Fermi/LAT

S Sheykhi, S Noroozi, F Rastgarnia, R Moradi - indico.icranet.org
GRB 220101A, detected by the Swift satellite with a redshift of (z= 4.618) and an equivalent
isotropic energy of 4× 1054 ergs, is categorized as a Binary Driven Hypernova of type one …

MeV, GeV and TeV neutrinos from binary-driven hypernovae

S Campion, JD Uribe-Suárez, JD Melon Fuksman… - Symmetry, 2023 - mdpi.com
We analyze neutrino emission channels in energetic (≳ 10 52 erg) long gamma-ray bursts
within the binary-driven hypernova model. The binary-driven hypernova progenitor is a …