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:
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. 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:
M. G. Bernardini, C. L. Bianco, L. Caito, M. G. Dainotti, R. Guida, R. Ruffini, Yong-Feng Huang, Zi-Gao Dai, Bing Zhang
GRB060607A is a very distant (z = 3.082) and energetic event (Eiso∼1053 erg). Its main peculiarity is that the peak of the near‐infrared afterglow has been observed with the REM robotic telescope, allowing to infer the initial Lorentz gamma facto
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bf1af9c1fb3ed12b326f75546341822
http://hdl.handle.net/11573/199110
http://hdl.handle.net/11573/199110
Autor:
G. de Barros, A. Aksenov, C. L. Bianco, R. Ruffini, G. Vereshchagin, Yong-Feng Huang, Zi-Gao Dai, Bing Zhang
We revisit Cavallo and Rees classification based on the analysis of initial conditions in electron‐positron‐photon plasma which appears suddenly around compact astrophysical objects and gives origin to GRBs. These initial conditions were recently
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fade29019b10b98eb3117bfbf7230d1a
http://hdl.handle.net/11573/198864
http://hdl.handle.net/11573/198864
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