Presupernova evolution and explosive nucleosynthesis of zero metal massive stars

Abstract

We present a new set of zero metallicity models in the range 13-80 ${\mathrm{M}}_{\odot }$ together to the associated explosive nucleosynthesis. These models are fully homogeneous with the solar metallicity set we published in Limongi & Chieffi (2006) and will be freely available at the web site http://www.iasf-roma.inaf.it./orfeo/public{\_}html. A comparison between these yields and an average star that represents the average behavior of most of the very metal poor stars in the range $-5.0<[Fe/H]<-2.5$ confirms previous findings that only a fraction of the elemental [X/Fe] may be fitted by the ejecta of $standard$ core collapse supernovae.

39 pages, 8 figures, 2 tables, accepted for publication in ApJS

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