Fireballs with a Neutron Component
| dc.creator | Beloborodov, Andrei M. | |
| dc.date | 2003-02-04 | |
| dc.date.accessioned | 2026-07-07T02:07:28Z | |
| dc.date.available | 2026-07-07T02:07:28Z | |
| dc.description | Standard GRB fireballs must carry free neutrons. This crucially changes the mechanism of fireball deceleration by an external medium. As the ion fireball decelerates, the coasting neutrons form a leading front. They gradually decay, leaving behind a relativistic trail of decay products mixed with the ambient medium. The ion fireball sweeps up the trail and drives a shock wave in it. Thus, observed afterglow emission is produced in the neutron trail. The impact of neutrons turns off at 10^{17}cm from the explosion center, and here a spectral transition is expected in GRB afterglows. Absence of neutron signatures would point to absence of baryons and a dominant Poynting flux in the fireballs. | |
| dc.description | talk at "Gamma-Ray Bursts in the Afterglow Era: 3rd Workshop", Rome, September 2002 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0302057 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0302057 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5706 | |
| dc.subject | Astrophysics | |
| dc.title | Fireballs with a Neutron Component | |
| dc.type | text |