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)
As the 50th 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 view, which evidence previous unnoticed connections. They are gaining due prominence in reaching a more complete picture evidencing the main results. We outline the history of GRB observations along with a summary of the contributions made by our group to develop the BdHN interpreting model. We show the seven episodes characterizing the most powerful BdHNe I occurred to date: GRB 190114C and GRB 220101A. New inferences for the explanation of the highest energy radiation in the TeV are presented.
Authors
- F. Rastegarnia
- R. Moradi (ORCID: https://orcid.org/0000-0002-2516-5894)
- Shuang‐Nan Zhang (ORCID: https://orcid.org/0000-0001-5586-1017)
- Y. Aimuratov (ORCID: https://orcid.org/0000-0001-5717-6523)
- Hernando Quevedo (ORCID: https://orcid.org/0000-0003-4433-5550)
- P. Chardonnet (ORCID: https://orcid.org/0000-0002-4049-8582)
- S. S. Xue
- Y. H. Wang
- R. Ruffini
- C. Sigismondi
Institutions
- Altran (France) (FR)
- International Center for Relativistic Astrophysics (IT)
- Sapienza University of Rome (IT)
- National Institute for Astrophysics (IT)
Publication Details
- Journal
- International Journal of Modern Physics D
- Published
- 2026-01-22
- DOI
- https://doi.org/10.1142/s0218271825400206
- Primary Topic
- Gamma-ray bursts and supernovae
- Type
- article
- Field-Weighted Citation Impact
- 0.00