Zobrazeno 1 - 10
of 75
pro vyhledávání: '"L. Caito"'
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1cb950cbf6dd468ba31fa1dfb8adc9db
https://doi.org/10.1063/1.3509327
https://doi.org/10.1063/1.3509327
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6080e3ff92e99fa9aac7ec5878c2dadd
https://doi.org/10.1063/1.2836989
https://doi.org/10.1063/1.2836989
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::313f8eac01184537891447b66acda436
https://doi.org/10.1063/1.2837018
https://doi.org/10.1063/1.2837018
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
Autor:
M. G. Dainotti, M. G. Bernardini, C. L. Bianco, L. Caito, R. Guida, R. Ruffini, Sandip K. Chakrabarti, Archan S. Majumdar
The Swift satellite has given continuous data in the range 0.3–150 keV from 0 s to 106 s for GRB060218 associated with SN2006aj. It has an unusually long duration (T90∼2100 s). We plan to fit the complete γ‐ and X‐ray light curves of this lo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07fb81a1d453fa9c66b8e90104fd8087
http://hdl.handle.net/11573/348630
http://hdl.handle.net/11573/348630
Autor:
M. G. Bernardini, C. L. Bianco, L. Caito, M. G. Dainotti, R. Guida, R. Ruffini, Carlo Luciano Bianco, She-Sheng Xue
On the basis of the recent understanding of GRB050315 and GRB060218, we return to GRB970228, the first Gamma-Ray Burst (GRB) with detected afterglow. We proposed it as the prototype for a new class of GRBs with "an occasional softer extended emission
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b11abc293bff0e51e6c703fb1c9c00bf
http://hdl.handle.net/11573/349592
http://hdl.handle.net/11573/349592
Autor:
M. G. Bernardini, C. L. Bianco, L. Caito, M. G. Dainotti, R. Guida, R. Ruffini, Sandip K. Chakrabarti, Archan S. Majumdar
Publikováno v:
AIP Conference Proceedings.
Within the fireshell model we define a “canonical” GRB light curve with two sharply different components: the Proper‐GRB (P‐GRB), emitted when the optically thick fireshell of electron‐positron plasma originating the phenomenon reaches tran
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa9b5bfbf2154f1eabd03a80a8e240c9
https://doi.org/10.1063/1.3009494
https://doi.org/10.1063/1.3009494
Autor:
G. de Barros, M. G. Bernardini, C. L. Bianco, L. Caito, M. G. Dainotti, R. Guida, R. Ruffini, Yong-Feng Huang, Zi-Gao Dai, Bing Zhang
Publikováno v:
AIP Conference Proceedings.
Within our “flreshell” model we introduced a “canonical” GRB scenario which differentiates physically the “proper GRB” (P‐GRB) emission when photons decouple, and the afterglow emission due to interaction of the accelerated baryons with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d88823fdb7d4c222ff4aeae1f0ef10f
https://doi.org/10.1063/1.3027918
https://doi.org/10.1063/1.3027918