activity
20022026
most citedOn the GeV emission of the type I BdHN GRB 130427A

47 citations · 152 across the 10 of their papers we have counts for

collaborators

11 papers

hep-ph2026

Particle-antiparticle perturbation superhorizon crossing: baryogenesis, leptogenesis, magnetogenesis and darkogenesis

She-Sheng Xue

During the reheating epoch, gravitationally produced superheavy particle-antiparticle pairs undergo quantum oscillations. Perturbations in their relative densities cross out the ho…

astro-ph.HE2025

Selected topics on: 1) proposal of interpreting the Crab supernova with a GRB 2) progress in identifying the seven GRBs episodes 3) the role of Sagittarius A in identifying the dark matter component (the X fermion)

R. Ruffini, C. Sigismondi, Y. Wang +10

As the fiftieth anniversary of our common effort in the field of relativistic astrophysics is approaching, we offer a new look to some of our acquired knowledge in a more complete…

astro-ph.HE2025

Trapped fireshell (halo) of photons and pairs around black-hole horizon: source for ultra-high-energy particles

She-Sheng Xue

We study the Compton-rocket effect of strong radiation force accelerating electrons in an opaque fireshell (or fire spot) of dense photons and electron-positron pairs, whose temper…

astro-ph.HE2020★ 6 cited

Magnetic field screening in strong crossed electromagnetic fields

S. Campion, J. A. Rueda, R. Ruffini +1

We consider crossed electric and a magnetic fields , with , in presence of some initial number of pairs. We do…

astro-ph.HE2019★ 4 cited

Self-Similarities and Power-laws in the Time-resolved Spectra of GRB 190114C, GRB 130427A, GRB 160509A, and GRB 160625B

L. Liang, R. Ruffini, J. A. Rueda +3

[Shortened] CONTEXT: [...] AIMS: To identify and verify the BdHNe I properties in the additional sources GRB160509A, GRB160625B and GRB1340427A, and compare and contrast the result…

astro-ph.HE2018★ 47 cited

On the GeV emission of the type I BdHN GRB 130427A

R. Ruffini, R. Moradi, J. A. Rueda +9

We propose that the "inner engine" of a type I binary-driven hypernova (BdHN) is composed of a Kerr black hole (BH) in a non-stationary state, embedded in a uniform magnetic field…