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Etudes des proprietes des neutrinos dans les contextes ...

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

be seen in [81].<br />

Our predictions for the positron time signal associated to inverse beta-decay<br />

in a detector are shown in Figure 7.5. Let us consider the case of inverted hierarchy<br />

and large third neutrino mixing angle. At early times, the conversion is<br />

adiabatic and <strong>neutrinos</strong> with <strong>les</strong>s than 20 MeV will produce a number of positrons<br />

determined by the “cold” spectrum. This number will decrease when the shock<br />

wave renders the resonance conversion non-adiabatic and the <strong>neutrinos</strong> reach the<br />

Earth with a “hot” spectrum. This will show up in the positron time signal as a<br />

dip. One can see it going from point A1 to point A2 on Fig.(7.4) and (7.5) when<br />

one considers the 10 MeV positron energy. Its depth is energy dependent. (Note<br />

that if the neutrino-neutrino interaction is absent, the time signal would show a<br />

bump instead, as discussed in [81].) For energies larger than 20 MeV, since the<br />

relative number flux of “hot” and “cold” spectra interchange, the dip turns into<br />

a bump. One can see it going from point B1 to point B2 on Fig.(7.4) and (7.5)<br />

when one considers the 29 MeV positron energy. One can also notice that the<br />

global intensity of the 29 MeV signal is much <strong>les</strong>s than the 10 MeV signal for<br />

instance since the fluxes are smaller in intensity at that energy (see Fig.7.4)<br />

Figure 7.5: Positron time signal in a detector, for a galactic explosion at 10 kpc.<br />

The case of inverted hierarchy and large θ13 is considered. Upper figure: positron<br />

spectrum as a function of time and positron energy per unit tonne of the detector.<br />

The contours are separated by 10 −4 (MeV s t) −1 with the outermost contours at<br />

10 −4 (MeV s t) −1 . Lower figure: results obtained for 10 (solid), 15 (dashed), 19<br />

(dash-dotted) and 29 (dot-dot-dashed line) MeV positron energies.<br />

Finally let us discuss the sensitivity to the hierarchy and upon the third neutrino<br />

mixing angle (Figure 7.6). If the hierarchy is inverted and θ13 is large the<br />

positron signal as a function of time presents a dip as discussed above. If θ13 is<br />

small, no flavor conversion occurs in the high density resonance region and the<br />

130

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