Probing CP violation in neutrino oscillations with neutrino telescopes
| dc.creator | Blum, Kfir | |
| dc.creator | Nir, Yosef | |
| dc.creator | Waxman, Eli | |
| dc.date | 2007-06-14 | |
| dc.date | 2007-07-03 | |
| dc.date.accessioned | 2026-07-07T08:13:26Z | |
| dc.date.available | 2026-07-07T08:13:26Z | |
| dc.description | Measurements of flavor ratios of astrophysical neutrino fluxes are sensitive to the two yet unknown mixing parameters $θ_{13}$ and $δ$ through the combination $\sinθ_{13}\cosδ$. We extend previous studies by considering the possibility that neutrino fluxes from more than a single type of sources will be measured. We point out that, if reactor experiments establish a lower bound on $θ_{13}$, then neutrino telescopes might establish an upper bound on $|\cosδ|$ that is smaller than one, and by that prove that CP is violated in neutrino oscillations. Such a measurement requires several favorable ingredients to occur: (i) $θ_{13}$ is not far below the present upper bound; (ii) The uncertainties in $θ_{12}$ and $θ_{23}$ are reduced by a factor of about two; (iii) Neutrino fluxes from muon-damped sources are identified, and their flavor ratios measured with accuracy of order 10% or better. For the last condition to be achieved with the planned km^3 detectors, the neutrino flux should be close to the Waxman-Bahcall bound. It motivates neutrino telescopes that are effectively about 10 times larger than IceCube for energies of O(100 TeV), even at the expense of a higher energy threshold. | |
| dc.description | 22 pages, 6 figures; v2: references added | |
| dc.identifier | https://arxiv.org/abs/0706.2070 | |
| dc.identifier | http://arxiv.org/abs/0706.2070 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/132767 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Probing CP violation in neutrino oscillations with neutrino telescopes | |
| dc.type | text |