Neutrinos from Gamma-Ray Bursts in Pulsar Wind Bubbles: \sim 10^{16} eV
| dc.creator | Guetta, Dafne | |
| dc.creator | Granot, Jonathan | |
| dc.date | 2002-12-02 | |
| dc.date | 2003-04-22 | |
| dc.date.accessioned | 2026-07-07T10:31:33Z | |
| dc.date.available | 2026-07-07T10:31:33Z | |
| dc.description | The supranova model for Gamma-Ray Bursts (GRBs) is becoming increasingly more popular. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). Protons accelerated in the internal shocks that emit the GRB may interact with the external PWB photons producing pions which decay into \sim 10^{16} eV neutrinos. A km^2 neutrino detector would observe several events per year correlated with the GRBs. | |
| dc.description | Accepted for publication in PRL. 4 pages, 3 figures, minor changes | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0212045 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0212045 | |
| dc.identifier | Phys.Rev.Lett.90:201103,2003 | |
| dc.identifier | doi:10.1103/PhysRevLett.90.201103 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/178449 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Neutrinos from Gamma-Ray Bursts in Pulsar Wind Bubbles: \sim 10^{16} eV | |
| dc.type | text |