Time dependent models for Li, Be and B production in the early Galaxy
| dc.creator | Parizot, Etienne | |
| dc.creator | Drury, Luke | |
| dc.date | 1999-03-24 | |
| dc.date.accessioned | 2026-07-07T02:30:57Z | |
| dc.date.available | 2026-07-07T02:30:57Z | |
| dc.description | We calculate the light element production induced by the explosion of an isolated supernova in the ISM. We use a time-dependent model and consider energetic particles accelerated at the forward (process~1) and reverse (process~2) shocks. Both processes are primary, but are shown to underproduce Be and B. The reasons for this failure are analyzed and used to propose a possible alternative, based on the acceleration of particles inside superbubbles. | |
| dc.description | 8 pages, 8 figures, proc. of "LiBeB, cosmic rays and gamma-ray line astronomy" (Paris, dec. 1998) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9903369 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9903369 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14001 | |
| dc.subject | Astrophysics | |
| dc.title | Time dependent models for Li, Be and B production in the early Galaxy | |
| dc.type | text |