Nucleosynthesis in early supernova winds III: No significant contribution from neutron-rich pockets
R. D. Hoffman, J. Pruet, J. L. Fisker, H.-T. Janka, R. Burras, and S., E. Woosley

TL;DR
This study investigates the nucleosynthesis contribution of neutron-rich pockets in early supernova winds and finds they are not significant compared to the overall ejecta.
Contribution
It provides a detailed calculation showing neutron-rich pockets in supernova winds have minimal impact on total nucleosynthesis.
Findings
Neutron-rich pockets contribute insignificantly to nucleosynthesis.
Early neutrino winds are predominantly proton-rich.
Neutron-rich pockets are present but have limited nucleosynthesis impact.
Abstract
Recent nucleosynthesis calculations of Type II supernovae using advanced neutrino transport determine that the early neutrino winds are proton-rich. However, a fraction of the ejecta emitted at the same time is composed of neutron-rich pockets. In this paper we calculate the nucleosynthesis contribution from the neutron-rich pockets in the hot convective bubbles of a core-collapse supernova and show that they do not contribute significantly to the total nucleosynthesis.
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Taxonomy
TopicsNeutrino Physics Research · Gamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena
