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

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µ and τ <strong>neutr<strong>in</strong>os</strong> reactions<br />

Reaction Current Important for . . .<br />

ν + N → ν ′ + N ′ NC opacity<br />

ν + A → ν ′ + A ′ NC opacity<br />

ν + e ± → ν ′ + e ±′<br />

NC energy exchange<br />

e + + e − ↔ νx + ¯νx NC ν production<br />

N + N ↔ N ′ + N ′ + νx + ¯νx NC ν production and energy exchange<br />

N + N + ν → N ′ + N ′ + ν ′ NC energy exchange<br />

νe + ¯νe ↔ νx + ¯νx NC ν production<br />

νe + ν → ν ′ e + ν ′ NC secondary importance<br />

¯νe + ν → ¯ν ′ e + ν ′ NC secondary importance<br />

νx stands for both νµ and ντ<br />

ν stands for both νx and ¯νx<br />

Bruenn 1985, Hannestad & Raffelt 1998, Buras et al. 2002, Marek et al. 2005, Buras et al.<br />

2006<br />

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

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