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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 />

1.03<br />

1.02<br />

1.01<br />

1<br />

0.99<br />

0.98<br />

0.97<br />

0.96<br />

20 40 60 80 100<br />

Neutrino Energy (MeV)<br />

Flux Ratio<br />

1.04<br />

1.03<br />

1.02<br />

1.01<br />

1<br />

0.99<br />

0.98<br />

0.97<br />

20 40 60 80 100<br />

Neutrino Energy (MeV)<br />

Figure 4.2: Same as Fig.4.1 for νµ (left) and ντ (right) fluxes.<br />

curves show results for the two hierarchies and the two values of θ13. Similarly to<br />

the case where Tνµ = Tντ, while for the N-L case the first resonance is adiabatic<br />

and the electron <strong>neutrinos</strong> get a hotter spectrum, for all other cases the spectra<br />

keep very close to the Fermi-Dirac distributions (Figure 3.3). The situation is<br />

obviously reversed for the muon neutrino flux. Figures 4.5, 4.6 and 4.7 show the<br />

ratios of the νe and νµ fluxes for a non-zero over a zero delta phase, as a function<br />

of neutrino energy, at different distances from the neutron star surface. One can<br />

see that effects up to a factor of 2-4 on the νe and up to 10 % on νµ are present.<br />

A similar behavior is found for the ¯νe and ντ fluxes.<br />

The behavior of the flux ratios shown in Figure 4.6 is easy to understand.<br />

From Eqs. (4.26) and (4.27) one can write<br />

φνe(δ) = φνe(δ = 0) + sin 2θ23 sin δ<br />

2 (Lντ − Lνµ) (4.39)<br />

<br />

× sin 2θ23 sin δ<br />

2 (|Bµe| 2 − |Bτe| 2 <br />

) + cos 2θ23 sin δ<br />

<br />

δ<br />

− i cos (BµeB<br />

2 2<br />

∗ <br />

τe ) + h.c.<br />

Clearly the ratios calculated in these figures would be identity at the value of the<br />

energy where νµ and ντ spectra would cross (i.e., Lντ = Lνµ). Away from this<br />

energy one expects an oscillatory behavior due to the additional terms in Eq.<br />

(4.39) as the figure indicates. Note that even for δ = 0 the neutrino fluxes could<br />

also exhibit an oscillatory behavior. Concerning Fig. 4.7, one can see that the<br />

effects due to δ = 0 and induced by taking different temperatures or luminosities<br />

are small, compared to the case with δ = 0 only (Figure 4.3).<br />

Effects on the electron fraction Ye<br />

Figure 4.8 shows results on the electron fraction Ye. As previously discussed,<br />

if δ = 0 there are no CP violation effects on Ye since this quantity depends on<br />

76

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