Expected neutrino signal from supernova remnant RX J1713.7-3946 and flavor oscillations
| dc.creator | Costantini, Maria Laura | |
| dc.creator | Vissani, Francesco | |
| dc.date | 2004-11-29 | |
| dc.date | 2005-06-01 | |
| dc.date.accessioned | 2026-07-07T02:16:04Z | |
| dc.date.available | 2026-07-07T02:16:04Z | |
| dc.description | We consider the impact of oscillations on 1-200 TeV neutrinos expected from RX J1713.7-3946. After a description of the nature of the source, we obtain a prediction for the neutrino fluxes, based on the intense gamma ray flux first seen by CANGAROO and recently measured by H.E.S.S. experiment. We study the effect of 3 flavor oscillations in detail and consider the impact on the muon flux induced by these high energy neutrinos, potentially observable by a neutrino telescope located in the Northern hemisphere. A detector in the Mediterranean with an effective area of 1 km^2 and unit detection efficiency should be able to see a signal of about 10 muons per year. | |
| dc.description | LaTeX. 8 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0411761 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0411761 | |
| dc.identifier | Astropart.Phys. 23 (2005) 477-485 | |
| dc.identifier | doi:10.1016/j.astropartphys.2005.03.003 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8651 | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Expected neutrino signal from supernova remnant RX J1713.7-3946 and flavor oscillations | |
| dc.type | text |