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arxiv: astro-ph/0308350 · v1 · submitted 2003-08-20 · 🌌 astro-ph

Neutrino-induced fission of neutron-rich nuclei

classification 🌌 astro-ph
keywords fissionneutrinoneutrino-inducedenergiesnucleir-processalterationaverage
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We calculate neutrino-induced fission cross sections for selected nuclei with Z=84-92. We show that these reactions populate the daughter nucleus at excitation energies where shell effects are significantly washed out, effectively reducing the fission barrier. If the r-process occurs in the presence of a strong neutrino fluence, and electron neutrino average energies are sufficiently high, perhaps as a result of matter-enhanced neutrino flavor transformation, then neutrino-induced fission could lead to significant alteration in the r-process flow in slow outflow scenarios.

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