Time-integrated supernova neutrino flux from a nearby cluster
| dc.creator | Nguyen, Van. T. | |
| dc.creator | Johnson, Calvin W. | |
| dc.date | 2005-08-11 | |
| dc.date | 2005-08-12 | |
| dc.date.accessioned | 2026-07-07T10:43:17Z | |
| dc.date.available | 2026-07-07T10:43:17Z | |
| dc.description | The rate of gravitational collapse (type II) supernovae in our galaxy is uncertain by a factor of three or more. One way to determine the galactic supernova rate is through a radiogeochemical experiment (for example, the molybdenum-technetium experiment) that would integrate the neutrino flux over several million years. While such a measurement is designed to integrate the flux over the entire galaxy, nearby star-forming regions could skew the results. We model the flux from a recently identified such region, the Scorpius-Centaurus OB association, and compare with the flux from the rest of the galaxy. | |
| dc.description | 8 pages, no figures; corrected typo, added 2 references; now uses elsart.cls | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0508267 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0508267 | |
| dc.identifier | Astropart.Phys.27:233-237,2007 | |
| dc.identifier | doi:10.1016/j.astropartphys.2006.10.002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/182189 | |
| dc.subject | Astrophysics | |
| dc.subject | Nuclear Theory | |
| dc.title | Time-integrated supernova neutrino flux from a nearby cluster | |
| dc.type | text |