Presupernova Evolution and Explosive Nucleosynthesis of Zero Metal Massive Stars

We present a new set of zero metallicity models in the range 13–80 M ☉ together to the associated explosive nucleosynthesis. These models are fully homogeneous with the solar metallicity set we published in Limongi & Chieffi and will be freely available at the Online Repository for the FRANEC Evolutionary Output Web site. 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.