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

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dc.creatorMartínez-Pinedo, G.
dc.creatorKelic, A.
dc.creatorLanganke, K.
dc.creatorSchmidt, K. -H.
dc.creatorMocelj, D.
dc.creatorFröhlich, C.
dc.creatorThielemann, F. -K.
dc.creatorPanov, I.
dc.creatorRauscher, T.
dc.creatorLiebendörfer, M.
dc.creatorZinner, N. T.
dc.creatorPfeiffer, B.
dc.creatorBuras, R.
dc.creatorJanka, H. -Th.
dc.date2006-08-23
dc.date.accessioned2026-07-07T10:23:28Z
dc.date.available2026-07-07T10:23:28Z
dc.descriptionThis 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.
dc.description10 pages, 3 figures, invited talk at NIC-IX, International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX, CERN, Geneva, Switzerland, 25-30 June, 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0608490
dc.identifierhttp://arxiv.org/abs/astro-ph/0608490
dc.identifierPoSNIC-IX:064,2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175838
dc.subjectAstrophysics
dc.titleNucleosynthesis in neutrino heated matter: The vp-process and the r-process
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