Oscillation Measurements with Upgraded Conventional Neutrino Beams
| dc.creator | Barger, V. | |
| dc.date | 2001-03-05 | |
| dc.date | 2001-03-06 | |
| dc.date.accessioned | 2026-07-07T03:44:02Z | |
| dc.date.available | 2026-07-07T03:44:02Z | |
| dc.description | We consider the nu_mu to nu_e oscillation measurements that would be possible at upgraded 1 GeV and multi-GeV conventional neutrino sources driven by future megawatt-scale proton drivers. If these neutrino superbeams are used together with detectors that are an order of magnitude larger than those presently foreseen, we find that the sensitivity to nu_mu to nu_e oscillations can be improved by an order of magnitude beyond the next generation of accelerator based experiments. In addition, over a limited region of parameter space, the neutrino mass hierarchy can be determined with a multi-GeV long baseline beam. If the Large Mixing Angle MSW solution correctly describes the solar neutrino deficit, there is a small corner of allowed parameter space in which maximal CP-violation in the lepton sector might be observable at a 1 GeV medium baseline experiment. Superbeams with massive detectors would therefore provide a useful tool en route to a neutrino factory, which would permit a further order of magnitude improvement in sensitivity, together with a more comprehensive check of CP-violation and the oscillation framework. | |
| dc.description | 42 pages, 20 figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0103052 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0103052 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/40450 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Oscillation Measurements with Upgraded Conventional Neutrino Beams | |
| dc.type | text |