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10) Nucleosynthesis in Supernovae - ISNAP

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νp-process <strong>in</strong> hydrogen rich, high<br />

neutron flux environments<br />

On-site neutron production<br />

through neutr<strong>in</strong>o <strong>in</strong>duced<br />

<strong>in</strong>teraction: 1 H(ν + ,e + )n!<br />

By-pass<strong>in</strong>g wait<strong>in</strong>g<br />

po<strong>in</strong>t nuclei 64 Ge,<br />

68<br />

Se by n-capture<br />

reactions.

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