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Etudes des proprietes des neutrinos dans les contextes ...

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tel-00450051, version 1 - 25 Jan 2010<br />

Flux Ratio<br />

2<br />

1.5<br />

1<br />

0.5<br />

Flux Ratio<br />

0 10 20 30 40 50 60 70 80 90 100<br />

Neutrino Energy (MeV)<br />

8<br />

6<br />

4<br />

2<br />

Flux Ratio<br />

1.1<br />

1.05<br />

1<br />

0.95<br />

Figure 4.6: Same as Fig.4.5 but at 1000 km.<br />

0<br />

0 20 40 60 80 100<br />

Neutrino Energy (MeV)<br />

Flux Ratio<br />

0.9<br />

0 20 40 60 80 100<br />

Neutrino Energy (MeV)<br />

8<br />

6<br />

4<br />

2<br />

0 20 40 60 80 100<br />

Neutrino Energy (MeV)<br />

Figure 4.7: Same as Fig.4.6 but for the νµ flux ratios.<br />

where the upper (lower) sign refers to <strong>neutrinos</strong> (anti<strong>neutrinos</strong>), E = (p 2 + m 2 ν) 1<br />

2<br />

is the neutrino energy,<br />

K(p, mν) ≡ 1<br />

<br />

(E + mν) 1 +<br />

4E<br />

p<br />

E + mν<br />

2<br />

(4.42)<br />

and CV νlf and CA νlf are the vector and axial-vector couplings in the expression of<br />

the neutrino scattering amplitude matrix:<br />

M(νlf → νlf) = −i GF<br />

√2νlγ α (1 − γ 5 )νlfγα(C V νlf + γ5C A νlf )f (4.43)<br />

where f is a generic fermion. This relation is valid for homogeneous, isotropic<br />

media and for scattering amplitu<strong>des</strong> sufficiently small, i.e n − 1 ≪ 1. For an<br />

80

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