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The role of neutrinos in core collapse Supernova explosion - LUTh ...

The role of neutrinos in core collapse Supernova explosion - LUTh ...

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Neutr<strong>in</strong>os <strong>in</strong> SN <strong>explosion</strong><br />

Neutr<strong>in</strong>os (<strong>of</strong> all flavours) are fundamental <strong>in</strong>gredients <strong>in</strong><br />

<strong>core</strong> <strong>collapse</strong> SN (Bethe (1990), Burrows (1990), Raffelt (2001));<br />

they . . .<br />

exchange energy with matter (heat<strong>in</strong>g and cool<strong>in</strong>g)<br />

release energy out <strong>of</strong> the system<br />

<strong>in</strong>fluence explosive nucleosynthesis<br />

give us important <strong>in</strong>formations about dense matter<br />

νe and ¯νe differ from νµ,τ and ¯νµ,τ<br />

orig<strong>in</strong> <strong>of</strong> the<br />

difference:<br />

me ≪ mµ ≪ mτ<br />

⇒ at the on-set <strong>of</strong> the <strong>collapse</strong>, Ye = 0<br />

while Yµ = Yτ ≈ 0<br />

Neutr<strong>in</strong>os <strong>in</strong> <strong>core</strong> <strong>collapse</strong> SN <strong>explosion</strong> - Paris, 10 September 2009 – p. 7/48

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