The cosmic matrix in the 50th anniversary of relativistic astrophysics - Archive ouverte HAL
Article Dans Une Revue Int.J.Mod.Phys.D Année : 2017

The cosmic matrix in the 50th anniversary of relativistic astrophysics

R. Ruffini
  • Fonction : Auteur
L. Becerra
  • Fonction : Auteur
C.L. Bianco
  • Fonction : Auteur
J.D. Melon Fuksman
  • Fonction : Auteur
R. Moradi
  • Fonction : Auteur
M. Muccino
  • Fonction : Auteur
A.V. Penacchioni
  • Fonction : Auteur
G.B. Pisani
  • Fonction : Auteur
D. Primorac
  • Fonction : Auteur
J.A. Rueda
  • Fonction : Auteur
S. Shakeri
  • Fonction : Auteur
G.V. Vereshchagin
  • Fonction : Auteur
Y. Wang
  • Fonction : Auteur
S.S. Xue
  • Fonction : Auteur

Résumé

Our concept of induced gravitational collapse (IGC paradigm) starting from a supernova occurring with a companion neutron star, has unlocked the understanding of seven different families of gamma ray bursts (GRBs), indicating a path for the formation of black holes in the universe. An authentic laboratory of relativistic astrophysics has been unveiled in which new paradigms have been introduced in order to advance knowledge of the most energetic, distant and complex systems in our universe. A novel cosmic matrix paradigm has been introduced at a relativistic cosmic level, which parallels the concept of an S-matrix introduced by Feynmann, Wheeler and Heisenberg in the quantum world of microphysics. Here the “in” states are represented by a neutron star and a supernova, while the “out” states, generated within less than a second, are a new neutron star and a black hole. This novel field of research needs very powerful technological observations in all wavelengths ranging from radio through optical, X-ray and gamma ray radiation all the way up to ultra-high-energy cosmic rays.
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Dates et versions

hal-01582923 , version 1 (06-09-2017)

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Citer

R. Ruffini, Y. Aimuratov, L. Becerra, C.L. Bianco, M. Karlica, et al.. The cosmic matrix in the 50th anniversary of relativistic astrophysics. Int.J.Mod.Phys.D, 2017, 26 (10), pp.1730019. ⟨10.1142/S0218271817300191⟩. ⟨hal-01582923⟩

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