{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:XO5HOXTMIYRLZZAYQJ7XRUKH6D","short_pith_number":"pith:XO5HOXTM","schema_version":"1.0","canonical_sha256":"bbba775e6c4622bce418827f78d147f0d67558fcb70cf5ce7e5cbc27bd0f2a39","source":{"kind":"arxiv","id":"1410.4592","version":2},"attestation_state":"computed","paper":{"title":"Constraining the 6.05 MeV 0$^+$ and 6.13 MeV 3$^-$ cascade transitions in the $^{12}$C($\\alpha$,$\\gamma$)$^{16}$O reaction using the Asymptotic Normalization Coefficients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. M. Mukhamedzhanov, A. N. Kuchera, D. Santiago-Gonzalez, E. Koshchiy, E. Uberseder, G. V. Rogachev, J. Belarge, K. W. Kemper, L. T. Baby, M. L. Avila","submitted_at":"2014-10-16T21:11:59Z","abstract_excerpt":"Background. The $^{12}$C$(\\alpha,\\gamma)^{16}$O reaction plays a fundamental role in astrophysics and needs to be known with accuracy better than 10%. Cascade $\\gamma$ transitions through the excited states of $^{16}$O are contributing to the uncertainty.\n  Purpose. To constrain the contribution of the 0$^+$ (6.05 MeV) and 3$^-$ (6.13 MeV) cascade transitions.\n  Method. The $\\alpha$ Asymptotic Normalization Coefficient for these states were measured using the $\\alpha$-transfer reaction $^{12}$C$(^6$Li,$d)^{16}$O at sub-Coulomb energies.\n  Results. The 0$^+$ and 3$^-$ cascade transitions contri"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1410.4592","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2014-10-16T21:11:59Z","cross_cats_sorted":[],"title_canon_sha256":"1ef0db59327d2effb92183457b3fdad91327862810f52ba99e70de60f1b0cc74","abstract_canon_sha256":"17036d612ed82a15647d67217797d0189298152bce9caf9e90a24be6f2b7429f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:26:52.766108Z","signature_b64":"EQH1sUjazSzzYGlKEk5Jf2C51jmNA8BIs8JsibjKcp1W+Sln1T+dtP4ogqQ16Mad31ZClT65NrbjLA4jxl9WAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bbba775e6c4622bce418827f78d147f0d67558fcb70cf5ce7e5cbc27bd0f2a39","last_reissued_at":"2026-05-18T02:26:52.765692Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:26:52.765692Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining the 6.05 MeV 0$^+$ and 6.13 MeV 3$^-$ cascade transitions in the $^{12}$C($\\alpha$,$\\gamma$)$^{16}$O reaction using the Asymptotic Normalization Coefficients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. M. Mukhamedzhanov, A. N. Kuchera, D. Santiago-Gonzalez, E. Koshchiy, E. Uberseder, G. V. Rogachev, J. Belarge, K. W. Kemper, L. T. Baby, M. L. Avila","submitted_at":"2014-10-16T21:11:59Z","abstract_excerpt":"Background. The $^{12}$C$(\\alpha,\\gamma)^{16}$O reaction plays a fundamental role in astrophysics and needs to be known with accuracy better than 10%. Cascade $\\gamma$ transitions through the excited states of $^{16}$O are contributing to the uncertainty.\n  Purpose. To constrain the contribution of the 0$^+$ (6.05 MeV) and 3$^-$ (6.13 MeV) cascade transitions.\n  Method. The $\\alpha$ Asymptotic Normalization Coefficient for these states were measured using the $\\alpha$-transfer reaction $^{12}$C$(^6$Li,$d)^{16}$O at sub-Coulomb energies.\n  Results. The 0$^+$ and 3$^-$ cascade transitions contri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.4592","kind":"arxiv","version":2},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1410.4592","created_at":"2026-05-18T02:26:52.765754+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.4592v2","created_at":"2026-05-18T02:26:52.765754+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.4592","created_at":"2026-05-18T02:26:52.765754+00:00"},{"alias_kind":"pith_short_12","alias_value":"XO5HOXTMIYRL","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"XO5HOXTMIYRLZZAY","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"XO5HOXTM","created_at":"2026-05-18T12:28:57.508820+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D","json":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D.json","graph_json":"https://pith.science/api/pith-number/XO5HOXTMIYRLZZAYQJ7XRUKH6D/graph.json","events_json":"https://pith.science/api/pith-number/XO5HOXTMIYRLZZAYQJ7XRUKH6D/events.json","paper":"https://pith.science/paper/XO5HOXTM"},"agent_actions":{"view_html":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D","download_json":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D.json","view_paper":"https://pith.science/paper/XO5HOXTM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.4592&json=true","fetch_graph":"https://pith.science/api/pith-number/XO5HOXTMIYRLZZAYQJ7XRUKH6D/graph.json","fetch_events":"https://pith.science/api/pith-number/XO5HOXTMIYRLZZAYQJ7XRUKH6D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D/action/storage_attestation","attest_author":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D/action/author_attestation","sign_citation":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D/action/citation_signature","submit_replication":"https://pith.science/pith/XO5HOXTMIYRLZZAYQJ7XRUKH6D/action/replication_record"}},"created_at":"2026-05-18T02:26:52.765754+00:00","updated_at":"2026-05-18T02:26:52.765754+00:00"}