{"paper":{"title":"Possible effects of collective neutrino oscillations in the three flavor multi-angle simulations on supernova $\\nu p$ process","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. B. Balantekin, H. Sasaki, T. Hayakawa, T. Kajino, T. Takiwaki, Y. Pehlivan","submitted_at":"2017-07-28T05:55:54Z","abstract_excerpt":"We study the effects of collective neutrino oscillations on $\\nu p$ process nucleosynthesis in proton-rich neutrino-driven winds by including both the multi-angle $3\\times3$ flavor mixing and the nucleosynthesis network calculation. The number flux of energetic electron antineutrinos is raised by collective neutrino oscillations in a $1$D supernova model for $40 M_{\\odot}$ progenitor. When the gas temperature decreases down to $\\sim2-3\\times10^{9}$ K, the increased flux of electron antineutrinos promotes $\\nu p$ process more actively, resulting in the enhancement of $p$-nuclei. In the early ph"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.09111","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"}