activity
19992024
most citedOn the interpretation of the burst structure of GRBs

103 citations · 1.9k across the 96 of their papers we have counts for

collaborators

101 papers

astro-ph.HE2024

The long-short GRB connection

J. A. Rueda, L. Becerra, C. L. Bianco +4

Long and short gamma-ray bursts (GRBs) are thought to arise from different and unrelated astrophysical progenitors. The association of long GRBs with supernovae (SNe) and the diffe…

astro-ph.HE2024★ 2 cited

Ten Supernova-rise in Binary Driven Gamma-ray Bursts

R. Ruffini, C. L. Bianco, Liang Li +6

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-oxygen…

gr-qc2024★ 1 cited

The role of the irreducible mass in repetitive Penrose energy extraction processes in a Kerr black hole

R. Ruffini, C. L. Bianco, M. Prakapenia +3

The concept of the irreducible mass () has led to the mass-energy () formula of a Kerr black hole (BH), in turn leading to its surface area . Th…

astro-ph.HE2023★ 4 cited

Probing electromagnetic-gravitational wave emission coincidence in type I binary-driven hypernova family of long GRBs at very-high redshift

C. L. Bianco, M. T. Mirtorabi, R. Moradi +7

The repointing time of the XRT instrument on the Neil Gehrels Swift Observatory satellite has posed challenges in observing and studying the early X-ray emissions within $\approx40…

astro-ph.HE2023★ 18 cited

GRB-SN Association within the Binary-Driven Hypernova Model

Y. Aimuratov, L. M. Becerra, C. L. Bianco +11

The 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 where GRBs…

astro-ph.HE2021★ 22 cited

Nature of the ultrarelativistic prompt emission phase of GRB 190114C

R. Moradi, J. A. Rueda, R. Ruffini +7

We address the physical origin of the ultrarelativistic prompt emission (UPE) phase of GRB 190114C observed in the interval 1.9-3.99 s, by the Fermi-GBM in 10 keV-10 MeV . Thanks t…