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Supernova Neutrinos - Department of Theoretical Physics

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NEUTRONIZATION BURST<br />

WC<br />

Lar TPC<br />

I.H.<br />

N.H.<br />

N=182<br />

70 kton<br />

N=110<br />

sin 2 q 13 =<br />

1 Mton<br />

n e,x e - n e,x e -<br />

[M.Kachelriess & R. Tomas, hep-ph/0412082]<br />

[I.Gil-Botella & A.Rubbia, hep-ph/0307244]<br />

• Robust feature <strong>of</strong> SN simulations<br />

• Possibility to probe oscillation physics during early stages <strong>of</strong> a SN<br />

• SN distance measurement (with a precision <strong>of</strong> ~5 %): N~ 1/d 2 . Useful in<br />

case <strong>of</strong> dust oscuration.

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