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Nucleosynthesis in neutrino heated matter: The vp-process and the r-process

G. Martínez-Pinedo·A. Kelic·K. Langanke·K. -H. Schmidt·D. Mocelj·C. Fröhlich·F. -K. Thielemann·I. Panov·T. Rauscher·M. Liebendörfer·N. T. Zinner·B. Pfeiffer·R. Buras·H. -Th. Janka
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Abstract

This manuscript reviews recent progress in our understanding of the nucleosynthesis of medium and heavy elements in supernovae. Recent hydrodynamical models of core-collapse supernovae show that a large amount of proton rich matter is ejected under strong neutrino fluxes. This matter constitutes the site of the vp-process where antineutrino absorption reactions catalyze the nucleosynthesis of nuclei with A > 64. Supernovae are also associated with the r-process responsible for the synthesis of the heaviest elements in nature. Fission during the r-process can play a major role in determining the final abundance patter and in explaining the almost universal features seen in metal-poor r-process-rich stars.

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G. Martínez-Pinedo, A. Kelic, K. Langanke, K. -H. Schmidt, D. Mocelj, C. Fröhlich, F. -K. Thielemann, I. Panov, T. Rauscher, M. Liebendörfer, N. T. Zinner, B. Pfeiffer, R. Buras, H. -Th. Janka. 2006-08-23. Nucleosynthesis in neutrino heated matter: The vp-process and the r-process. https://arxiv.org/abs/astro-ph/0608490

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