Zobrazeno 1 - 10
of 40
pro vyhledávání: '"C. L. Bianco"'
Autor:
C. L. Bianco, M. T. Mirtorabi, R. Moradi, F. Rastegarnia, J. A. Rueda, R. Ruffini, Y. Wang, M. Della Valle, Liang Li, S. R. Zhang
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 2, p 219 (2024)
The repointing time of the X-Ray Telescope (XRT) instrument on the Neil Gehrels Swift Observatory satellite has posed challenges in observing and studying the early X-ray emissions within ≈40 s after a gamma-ray burst (GRB) trigger. To address this
Externí odkaz:
https://doaj.org/article/55a309c1217d468b92f1310668196bcc
Autor:
Y. Aimuratov, L. M. Becerra, C. L. Bianco, C. Cherubini, M. Della Valle, S. Filippi, Liang Li, R. Moradi, F. Rastegarnia, J. A. Rueda, R. Ruffini, N. Sahakyan, Y. Wang, S. R. Zhang
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 2, p 93 (2023)
Observations of supernovae (SNe) Ic occurring after the prompt emission of long gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model where GRBs originate from a binary composed of a ∼10 M _⊙ carbon–oxygen (CO) s
Externí odkaz:
https://doaj.org/article/873d883b5cc84d209bdcd41c997eb075
Autor:
L. Izzo, G. B. Pisani, M. Muccino, J. A. Rueda, Y. Wang, C. L. Bianco, A. V. Penacchioni, R. Ruffini
Publikováno v:
Gamma-ray Bursts: 15 Years of GRB Afterglows ISBN: 9782759810024
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8015a506abf2cb5a2630c394a21d64ce
https://doi.org/10.1051/978-2-7598-1002-4.c097
https://doi.org/10.1051/978-2-7598-1002-4.c097
Publikováno v:
Scopus-Elsevier
Autor:
L. Izzo, M. G. Bernardini, C. L. Bianco, L. Caito, B. Patricelli, L. J. Rangel Lemos, R. Ruffini, Nobuyuki Kawai, Shigehiro Nagataki
We propose a possible explanation, in the context of the Fireshell scenario, for the high‐energy emission observed in GRB 080916C and GRB 090902B. The physical process underlying this emission consists mainly in the interaction of the baryon in the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d313128ef78440d77c4921e0bde10b2
http://hdl.handle.net/11573/199184
http://hdl.handle.net/11573/199184
Autor:
B. Patricelli, M. G. Bernardini, C. L. Bianco, L. Caito, G. de Barros, L. Izzo, R. Ruffini, Nobuyuki Kawai, Shigehiro Nagataki
Publikováno v:
AIP Conference Proceedings.
Within the fireshell model, Gamma Ray Bursts (GRBs) originate from an optically thick e± plasma created by vacuum polarization process during the formation of a Black Hole (BH). Here we briefly recall the basic features of this model, then we show h
Autor:
L. Caito, M. G. Bernardini, C. L. Bianco, M. G. Dainotti, R. Guida, R. Ruffini, Carlo Luciano Bianco, She-Sheng Xue
Publikováno v:
AIP Conference Proceedings.
The explosion of GRB 060614, detected by the Swift satellite, produced a deep break in the GRB scenario opening new horizons of investigation, because it can't be traced back to any traditional scheme of classification. In fact, it manifests peculiar
Autor:
R. Guida, M. G. Bernardini, C. L. Bianco, L. Caito, M. G. Dainotti, R. Ruffini, Carlo Luciano Bianco, She-Sheng Xue
Publikováno v:
AIP Conference Proceedings.
In this work we show the existence of a spectral‐energy correlation within our “fireshell” model for GRBs. The free parameters of the model are the total energy E tot e± of the e ± plasma and its baryon loading B≡M B c 2 /E tot e± , charac
Autor:
R. Guida, M. G. Bernardini, C. L. Bianco, L. Caito, M. G. Dainotti, R. Ruffini, M. Galassi, David Palmer, Ed Fenimore
We discuss within our theoretical “fireshell” model for Gamma‐Ray Bursts (GRBs) the theoretical interpretation of the phenomenological correlation between the isotropic‐equivalent radiated energy of the prompt emission Eiso and the cosmologic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::668ecda46de5d827677cea430c7bc52c
http://hdl.handle.net/11573/348626
http://hdl.handle.net/11573/348626
Autor:
L. Caito, M. G. Bernardini, C. L. Bianco, M. G. Dainotti, R. Guida, R. Ruffini, M. Galassi, David Palmer, Ed Fenimore
The explosion of GRB 060614 produced a deep break in the GRB scenario and opened new horizons of investigation because it can't be traced back to any traditional scheme of classification. In fact, it has features both of long bursts and of short burs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::426878d140b8d13004eede02a6fa167b
http://hdl.handle.net/11573/348625
http://hdl.handle.net/11573/348625