{"paper":{"title":"Light Curves and Spectra from a Unimodal Core-Collapse SuperNova","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Aimee L. Hungerford, Allan B. Wollaber, Chris L. Fryer, Daniel R. van Rossum, Ryan T. Wollaeger, Wesley Even","submitted_at":"2017-08-03T18:23:52Z","abstract_excerpt":"To assess the effectiveness of optical emission as a probe of spatial asymmetry in core-collapse supernovae (CCSNe), we apply the radiative transfer software, \\supernu, to a unimodal CCSN model. The \\snsph\\ radiation-hydrodynamics software was used to simulate an asymmetric explosion of a 16 M$_{\\odot}$ ZAMS binary star. The ejecta has 3.36 M$_{\\odot}$ with 0.024 M$_{\\odot}$ of radioactive $^{56}$Ni, with unipolar asymmetry along the z-axis. For 96 discrete angular views, we find the ratio between maximum and minimum peak total luminosities is $\\sim$1.36. The brightest light curves emerge from"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.01271","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"}