Sensitivity to theta(13) of the CERN to Gran Sasso neutrino beam
| dc.creator | Komatsu, M. | |
| dc.creator | Migliozzi, P. | |
| dc.creator | Terranova, F. | |
| dc.date | 2002-10-02 | |
| dc.date.accessioned | 2026-07-07T10:48:36Z | |
| dc.date.available | 2026-07-07T10:48:36Z | |
| dc.description | The sensitivity of the present CNGS beam to the sub-dominant $ν_μ\leftrightarrow ν_e$ oscillations in the region indicated by the atmospheric neutrino experiments is investigated. In particular, we present a revised analysis of the OPERA detector and discuss the sensitivity to $θ_{13}$ of ICARUS and OPERA combined. We show that the CNGS beam optimised for $ν_τ$ appearance, will improve significantly (about a factor 5) the current limit of CHOOZ and explore most of the region $\sin^22θ_{13}\simeq\mathcal{O}(10^{-2})$. | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0210043 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0210043 | |
| dc.identifier | J.Phys.G29:443,2003 | |
| dc.identifier | doi:10.1088/0954-3899/29/2/318 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183936 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Sensitivity to theta(13) of the CERN to Gran Sasso neutrino beam | |
| dc.type | text |