Identifying neutrino mass hierarchy at extremely small theta(13) through Earth matter effects in a supernova signal
| dc.creator | Dasgupta, Basudeb | |
| dc.creator | Dighe, Amol | |
| dc.creator | Mirizzi, Alessandro | |
| dc.date | 2008-02-11 | |
| dc.date | 2008-10-20 | |
| dc.date.accessioned | 2026-07-07T11:55:57Z | |
| dc.date.available | 2026-07-07T11:55:57Z | |
| dc.description | Collective neutrino flavor transformations deep inside a supernova are sensitive to the neutrino mass hierarchy even at extremely small values of theta(13). Exploiting this effect, we show that comparison of the antineutrino signals from a galactic supernova in two megaton class water Cherenkov detectors, one of which is shadowed by the Earth, will enable us to distinguish between the hierarchies if sin^2 theta(13) < 10^{-5}. On the other hand, the observation of Earth effects in the inverted hierarchy for sin^2 theta(13) > 10^{-3} will provide a robust observable signature of collective oscillations occurring deep inside the supernova. | |
| dc.description | Final version: Text clarified, references updated. Matches the version published in Physical Review Letters | |
| dc.identifier | https://arxiv.org/abs/0802.1481 | |
| dc.identifier | http://arxiv.org/abs/0802.1481 | |
| dc.identifier | Phys.Rev.Lett.101:171801,2008 | |
| dc.identifier | doi:10.1103/PhysRevLett.101.171801 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/205420 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Identifying neutrino mass hierarchy at extremely small theta(13) through Earth matter effects in a supernova signal | |
| dc.type | text |