{"paper":{"title":"Uncertainties in Supernova Yields I: 1D Explosions","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"2), 3) ((1) Los Alamos National Laboratory (2)Steward Observatory, Chris L. Fryer (1, Patrick A. Young (1, The University of Arizona), the University of Arizona (3) Physics Department","submitted_at":"2006-12-22T19:18:53Z","abstract_excerpt":"Theoretical nucleosynthetic yields from supernovae are sensitive to both the details of the progenitor star and the explosion calculation. We attempt to comprehensively identify the sources of uncertainties in these yields. In this paper we concentrate on the variations in yields from a single progenitor arising from common 1-dimensional methods of approximating a supernova explosion. Subsequent papers will examine 3-dimensional effects in the explosion and the progenitor, and trends in mass and composition. For the 1-dimensional explosions we find that both elemental and isotopic yields for S"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612698","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}