{"paper":{"title":"Constraining nova observables: direct measurements of resonance strengths in 33S(p,\\gamma)34Cl","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"astro-ph.SR","authors_text":"A. A. Chen, A. M. Laird, A. Parikh, A. Rojas, B. Davids, B. Guo, B. R. Fulton, C. Herlitzius, C. M. Deibel, C. Ruiz, C. Vockenhuber, C. Wrede, D. A. Hutcheon, D. Ottewell, E. T. Li, G. Christian, G. Lian, J. A. Clark, J. Fallis, J. Jos\\'e, J. M. D'Auria, K. Nelson, K. Setoodehnia, L. Buchmann, L. Martin, P. D. Parker, P. F. Bertone, S. Bishop, S. Reeve, S. Sjue, U. Greife, U. Hager, W. P. Liu, Y. B. Wang, Z. H. Li","submitted_at":"2013-09-13T19:22:21Z","abstract_excerpt":"The 33S(p,\\gamma)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abundance of 33S in oxygen-neon nova ejecta. This overproduction factor may, however, vary by orders of magnitude due to uncertainties in the 33S(p,\\gamma)34Cl reaction rate at nova peak temperatures. Depending on this rate, 33S could potentially be used as a diagnostic tool for classifying certain types of presolar grains. Better knowledge of the 33S(p,\\gamma)34Cl rate would also aid in interpreting nova observati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.3543","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"}