Cargando…
Towards a complete theory of Gamma Ray Bursts
Gamma Ray Bursts (GRBs) are notorious for their diversity. Yet, they have a series of common features. The typical energy of their $\gamma$ rays is a fraction of an MeV. The energy distributions are well described by a ``Band spectrum'', with ``peak energies'' spanning a surprisi...
Autores principales: | Dar, Arnon, De Rujula, A. |
---|---|
Lenguaje: | eng |
Publicado: |
2003
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.physrep.2004.09.008 http://cds.cern.ch/record/636942 |
Ejemplares similares
-
The Cannonball Model of Gamma Ray Bursts: high-energy neutrinos and $\gamma$-rays
por: Dar, Arnon, et al.
Publicado: (2001) -
The Cannonball Model of Gamma Ray Bursts: Spectral and Temporal Properties of the Gamma Rays
por: Dar, Arnon, et al.
Publicado: (2000) -
On the radio afterglow of gamma ray bursts
por: Dado, Shlomo, et al.
Publicado: (2002) -
On the optical and X-ray afterglows of gamma ray bursts
por: Dado, Shlomo, et al.
Publicado: (2001) -
The Cannonball Model of Gamma Ray Bursts: Lines in the X-Ray Afterglow
por: Dar, Arnon, et al.
Publicado: (2001)