{"paper":{"title":"Study of the ^18F(p, alpha)^15O reaction for application to nova gamma-ray emission","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"nucl-ex","authors_text":"A. Coc, A. Lefebvre, A. Ninane, B. Bouzid, C. Angulo, D. Beaumel, D. Labar, F. de Oliveira Santos, F. Hammache, G. Ryckewaert, J. Kiener, J.-P. Thibaud, M. Assuncao, M. Couder, M. Gaelens, M. Loiselet, N. de Sereville, N. Smirnova, P. Demaret, P. Figuera, P. Leleux, S. Cherubini, S. Fortier, S. Ouichaoui, V. Tatischeff","submitted_at":"2002-09-24T08:53:37Z","abstract_excerpt":"The ^18F(p, alpha)^15O reaction is recognized as one of the most important reaction for nova gamma-ray astronomy as it governs the early =< 511 keV emission. However, its rate remains largely uncertain at nova temperatures due to unknown low-energy resonance strengths. In order to better constrain this reaction rate, we have studied the one-nucleon transfer reaction, D(^18F,p alpha)^15N, at the CRC-RIB facility at Louvain La Neuve."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-ex/0209017","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"}