The Blackholic energy and the canonical Gamma-Ray Burst IV: the "long", "genuine short" and "fake - disguised short" GRBs
Remo Ruffini, Alexey G. Aksenov, Maria Grazia Bernardini, Carlo, Luciano Bianco, Letizia Caito, Pascal Chardonnet, Maria Giovanna Dainotti,, Gustavo De Barros, Roberto Guida, Luca Izzo, Barbara Patricelli, Luis Juracy, Rangel Lemos, Michael Rotondo, Jorge Armando Rueda Hernandez

TL;DR
This paper advances the fireshell model to interpret various GRB phenomena, including X-ray flares, short GRBs, and GRB-SN associations, and explores high-energy processes and electrodynamics near black holes and neutron stars.
Contribution
It introduces novel interpretations of GRB subclasses, analyzes specific GRBs with new methods, and discusses high-energy phenomena related to black holes and neutron stars.
Findings
X-ray flares result from fireshell-cloud interactions
Some short GRBs are 'fake-disguised' from binary mergers in low-density environments
Progress on understanding the Amati relation and high-energy processes in GRBs
Abstract
(Shortened) [...] After recalling the basic features of the "fireshell model", we emphasize the following novel results: 1) the interpretation of the X-ray flares in GRB afterglows as due to the interaction of the optically thin fireshell with isolated clouds in the CircumBurst Medium (CBM); 2) an interpretation as "fake - disguised" short GRBs of the GRBs belonging to the class identified by Norris & Bonnell [...] consistent with an origin from the final coalescence of a binary system in the halo of their host galaxies with particularly low CBM density [...]; 3) the first attempt to study a genuine short GRB with the analysis of GRB 050509B, that reveals indeed still an open question; 4) the interpretation of the GRB-SN association in the case of GRB 060218 via the "induced gravitational collapse" process; 5) a first attempt to understand the nature of the "Amati relation", a…
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Taxonomy
TopicsGamma-ray bursts and supernovae
