Combined potential of future long-baseline and reactor experiments
arXiv:hep-ph/0412133 · doi:10.1016/j.nuclphysbps.2005.04.004
Abstract
We investigate the determination of neutrino oscillation parameters by experiments within the next ten years. The potential of conventional beam experiments (MINOS, ICARUS, OPERA), superbeam experiments (T2K, NOvA), and reactor experiments (D-CHOOZ) to improve the precision on the ``atmospheric'' parameters , , as well as the sensitivity to are discussed. Further, we comment on the possibility to determine the leptonic CP-phase and the neutrino mass hierarchy if turns out to be large.
4 pages, 4 figures, Talk given by T.S. at the NOW2004 workshop, Conca Specchiulla (Otranto, Italy), 11--17 Sept. 2004
References in corpus (4)
Cited by in corpus (10)
- The Absolute Neutrino Mass Scale, Neutrino Mass Spectrum, Majorana CP-Violation and Neutrinoless Double-Beta Decay
- Determining the Neutrino Mass Hierarchy with Atmospheric Neutrinos
- Earth Matter Effects at Very Long Baselines and the Neutrino Mass Hierarchy
- A model realizing the Harrison-Perkins-Scott lepton mixing matrix
- Neutrino Mass Hierarchy Determination Using Reactor Antineutrinos
- Renormalization Group Evolution of Dirac Neutrino Masses
- The 2-3 mixing and mass split: atmospheric neutrinos and magnetized spectrometers
- Measurement of three-family neutrino mixing and search for CP violation
- Sensitivity to neutrino mixing parameters with atmospheric neutrinos
- European facilities for accelerator neutrino physics: perspectives for the decade to come