The canonical Gamma-Ray Bursts: long, "fake"-"disguised" and "genuine" short bursts
Remo Ruffini, Alexey Aksenov, Maria Grazia Bernardini, Carlo Luciano, Bianco, Letizia Caito, Maria Giovanna Dainotti, Gustavo De Barros, Roberto, Guida, Gregory Vereshchagin, She-Sheng Xue

TL;DR
This paper discusses the structure and classification of Gamma-Ray Bursts (GRBs), introducing the fireshell model which differentiates between various types of GRBs and offers a new perspective on their origins and observed features.
Contribution
The paper presents the fireshell model as an alternative to the traditional fireball model, providing a new framework for understanding GRB structure and classification.
Findings
Fireshell model explains GRB structure as composed of a proper-GRB and an extended afterglow.
Differentiates between long, short, and disguised short GRBs based on the fireshell paradigm.
Provides a unified interpretation of diverse GRB phenomena through relativistic plasma dynamics.
Abstract
The Gamma-Ray Bursts (GRBs) offer the unprecedented opportunity to observe for the first time the blackholic energy extracted by the vacuum polarization during the process of gravitational collapse to a black hole leading to the formation of an electron-positron plasma. The uniqueness of the Kerr-Newman black hole implies that very different processes originating from the gravitational collapse a) of a single star in a binary system induced by the companion, or b) of two neutron stars, or c) of a neutron star and a white dwarf, do lead to the same structure for the observed GRB. The recent progress of the numerical integration of the relativistic Boltzmann equations with collision integrals including 2-body and 3-body interactions between the particles offer a powerful conceptual tool in order to differentiate the traditional "fireball" picture, an expanding hot cavity considered by…
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