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Etudes des proprietes des neutrinos dans les contextes ...

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

Figure 7.1: The initial, t = 0, density profile used in our SN simulations. The<br />

dense core (A) inside 20 km contains approximately 3M⊙. The slow, outwardmoving<br />

standing accretion shock (B) is located at 200 km. Above that we have<br />

a collapsing, 13.2 M⊙, progenitor (C). Taken from [81]<br />

Figure 7.2: The density as a function of the radius in the 1D SN model used at<br />

t = 1 s (dotted), t = 1.5 s (solid), t = 2 s (long dashed), t = 2.5 s (dash-dot) and<br />

t = 3 s (dash double dot). The horizontal solid lines are (from top to bottom)<br />

the MSW high resonance densities for 20 and 40 MeV <strong>neutrinos</strong>. Taken from [81]<br />

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