On the energy and baseline optimization to study effects related to the δ-phase (CP-/T-violation) in neutrino oscillations at a neutrino factory

被引:37
作者
Bueno, A [1 ]
Campanelli, M [1 ]
Navas-Concha, S [1 ]
Rubbia, A [1 ]
机构
[1] Swiss Fed Inst Technol, Inst Teilchenphys, CH-8093 Zurich, Switzerland
关键词
D O I
10.1016/S0550-3213(02)00211-0
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this paper we discuss the detection of CP- and T-violation effects in the framework of a neutrino factory. We introduce three quantities, which are good discriminants for a non-vanishing complex phase (delta) in the 3 x 3 neutrino mixing matrix: Delta(CP) and AT. We find that these three discriminants (in vacuum) all scale with L/E-nu, where L is the baseline and E-nu the neutrino energy. Matter effects modify the scaling, but these effects are large enough to spoil the sensitivity only for baselines larger than 5000 kin. So, in the hypothesis of constant neutrino factory power (i.e., number of muons inversely proportional to muon energy), the sensitivity on the delta-phase is independent of the baseline chosen. Specially interesting is the direct measurement of T-violation from the "wrong-sign" electron channel (i.e., the AT discriminant), which involves a comparison of the nu(e) --> nu(mu) and nu(mu) --> nu(e) oscillation rates. However, the nu(mu) --> nu(e) measurement requires magnetic discrimination of the electron charge, experimentally very challenging in a neutrino detector. Since the direction of the electron curvature has to be estimated before the start of the electromagnetic shower, low-energy neutrino beams and hence short baselines, are preferred. In this paper we show, as an example, the exclusion regions in the Deltam(12)(2)-delta plane using the Delta(CP) and Delta(T) discriminants for two concrete cases keeping the same L/E-nu ratio (730 km/7.5 GeV and 2900 km/30 GeV). We obtain a similar excluded region provided that the electron detection efficiency is similar to20% and the charge confusion 0.1%. The Deltam(12)(2), compatible with the LMA solar data can be tested with a flux of 5 x 10(21) muons. We compare these results with the fit of the visible energy distributions. (C) 2002 Elsevier Science B.V. All rights reserved.
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页码:239 / 284
页数:46
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