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1\subsection {$\theta_{13}$ and CP violation in oscillations}
2
3In the recent years, a series of experiments have provided strong evidence
4for oscillations of solar and atmospheric neutrinos, and have started to
5precisely constrain the associated parameters $\Delta m^2_{23}$,
6$\Delta m^2_{12}$, $\theta_{23}$ and $\theta_{12}$. The third mixing angle
7$\theta_{13}$ is still unknown: all we have is an upper bound of
8$\theta_{13} \leq 13^\circ$ coming from the CHOOZ
9experiment \cite{Apollonio:1999ae}. Its
10measurement, as well as the determination of the sign of $\Delta m^2_{23}$
11and therefore of the type of mass hierarchy, is crucial for
12discriminating between different neutrino mass and mixing scenarios.
13Moreover a precise determination of the PMNS matrix (which contrary
14to the CKM matrix is free from hadronic uncertainties) would put very severe
15constraints on models
16of fermion masses, including realistic GUT models, and thus shed some light
17on the underlying flavour theory. A neutrino super-beam from the CERN
18SPL to a megaton water \v{C}erenkov detector located at Fr\'ejus would allow
19to make a significant progress in this programme, reaching in particular
20a sensitivity to $\sin^2(2\theta_{13})$ close to $10^{-3}$ %one degree
21and close to $2\cdot 10^{-4}$ %0.4 degree
22with a Beta-beam (and $1\cdot 10^{-4}$ %0.3 degree
23with both Super-beam and
24Beta-beam), see section~\ref{sec:oscillations}.
25
26Due to its sensitivity to $\theta_{13}$, a megaton water \v{C}erenkov
27detector would also be sensitive to the CP violating phase
28$\delta$ in a large portion of the ($\Delta m^2_{12}$,
29$\theta_{13}$) parameter space. Establishing CP violation in the
30lepton sector would represent a major progress in particle
31physics, since CP violation has only been observed in the quark
32sector so far. Moreover, CP violation is a crucial ingredient of
33leptogenesis, a mechanism for creating the matter-antimatter
34asymmetry of the Universe which relies on the out-of-equilibrium
35decay of heavy Majorana neutrinos. Although the phase involved in
36oscillations is generally distinct from the phase responsible for
37leptogenesis, the measurement of a nonzero $\delta$ would be a
38strong indication that leptogenesis may be at the origin of the
39baryon asymmetry \cite{Fukugita:1986hr}.
40Indeed, standard electroweak baryogenesis would
41require a very light Higgs boson, which is now excluded by LEP,
42and only a small window remains for supersymmetric electroweak
43baryogenesis.
44%After the discovery of neutrino oscillations, leptogenesis
45%therefore appears as one of the most plausible explanations of the
46%baryon asymmetry.
47Another necessary ingredient of leptogenesis is the existence of Majorana
48neutrinos, which could be established by a positive signal in future
49neutrinoless double beta decay experiments.
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