On the mechanism of prompt emission of gamma-ray bursts
| dc.creator | Neronov, Andrey | |
| dc.date | 2003-11-05 | |
| dc.date.accessioned | 2026-07-07T02:11:04Z | |
| dc.date.available | 2026-07-07T02:11:04Z | |
| dc.description | We propose a model in which prompt gamma emission of gamma-ray bursts is the synchrotron radiation of electron-positron plasma in the ordered magnetic field in the direct vicinity of horizon of a young black hole formed in the core collapse of a massive star. This mechanism can naturally explain high degree of polarization of the gamma-ray flux and hard low energy photon spectral index. Interaction of gamma-quanta with ambient matter provides a mechanism of formation of relativistic ejecta which are responsible for the gamma-ray burst afterglows. | |
| dc.description | 4 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0311111 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0311111 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6950 | |
| dc.subject | Astrophysics | |
| dc.title | On the mechanism of prompt emission of gamma-ray bursts | |
| dc.type | text |