On Gamma-Ray Bursts
Remo Ruffini, Maria Grazia Bernardini, Carlo Luciano Bianco, Letizia, Caito, Pascal Chardonnet, Christian Cherubini, Maria Giovanna Dainotti,, Federico Fraschetti, Andrea Geralico, Roberto Guida, Barbara Patricelli,, Michael Rotondo, Jorge Armando Rueda Hernandez

TL;DR
This paper explores the physics of gamma-ray bursts (GRBs) through theoretical models involving vacuum polarization, black holes, and nuclear matter configurations, proposing a new framework for understanding GRB energetics and classifications.
Contribution
It introduces a novel theoretical approach linking neutron star physics and heavy nuclei to GRB phenomena, emphasizing the role of electric fields and plasma creation in GRB models.
Findings
Configurations of nuclear matter with near-critical electric fields can exist on macroscopic scales.
The model explains the energetics and high Lorentz factors observed in GRBs.
The approach offers new insights into short and long GRB classifications and their relation to supernovae.
Abstract
(Shortened) We show by example how the uncoding of Gamma-Ray Bursts (GRBs) offers unprecedented possibilities to foster new knowledge in fundamental physics and in astrophysics. After recalling some of the classic work on vacuum polarization in uniform electric fields by Klein, Sauter, Heisenberg, Euler and Schwinger, we summarize some of the efforts to observe these effects in heavy ions and high energy ion collisions. We then turn to the theory of vacuum polarization around a Kerr-Newman black hole, leading to the extraction of the blackholic energy, to the concept of dyadosphere and dyadotorus, and to the creation of an electron-positron-photon plasma. We then present a new theoretical approach encompassing the physics of neutron stars and heavy nuclei. It is shown that configurations of nuclear matter in bulk with global charge neutrality can exist on macroscopic scales and with…
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