s-process nucleosynthesis of 142^Nd: crisis of the classical model

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dc.creatorArlandini, C.
dc.creatorKaeppeler, F.
dc.creatorWisshak, K.
dc.creatorGallino, R.
dc.creatorLugaro, M.
dc.creatorBusso, M.
dc.creatorStraniero, O.
dc.date1998-09-17
dc.date.accessioned2026-07-07T02:27:58Z
dc.date.available2026-07-07T02:27:58Z
dc.descriptionThe recently improved information on the stellar neutron capture cross sections of neutron magic nuclei at N = 82, and in particular for 142^Nd, turned out to represent a sensitive test for models of s-process nucleosynthesis. While these data were found to be incompatible with the classical approach, they provide significantly better agreement between the observed abundance distribution and the predictions of models for low mass AGB stars.
dc.description4 pages, 3 figures. To appear in 'Nuclei in the Cosmos 1998' proceedings, (Volos, July 5 - 12, 1998)
dc.identifierhttps://arxiv.org/abs/astro-ph/9809226
dc.identifierhttp://arxiv.org/abs/astro-ph/9809226
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12924
dc.subjectAstrophysics
dc.titles-process nucleosynthesis of 142^Nd: crisis of the classical model
dc.typetext

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