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10) Nucleosynthesis in Supernovae - ISNAP

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Possible consequences of high<br />

neutr<strong>in</strong>o flux <strong>in</strong> shock-front<br />

Neutr<strong>in</strong>o capture on protons<br />

1<br />

H(ν + ,e + )n, neutron production<br />

which <strong>in</strong>fluence the reaction<br />

path by neutron capture.

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