Cargando…
The Cannonball Model of Gamma Ray Bursts: high-energy neutrinos and $\gamma$-rays
Recent observations suggest that $\gamma$-ray bursts (GRBs) and their afterglows are produced by jets of highly relativistic cannonballs (CBs), emitted in supernova (SN) explosions. The CBs, reheated by their collision with the shell, emit radiation that is collimated along their direction of motion...
| Autores principales: | , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2001
|
| Materias: | |
| Acceso en línea: | http://cds.cern.ch/record/499043 |