{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:H5KQSVVMG6MHS2MGRUH6QVFAXK","short_pith_number":"pith:H5KQSVVM","schema_version":"1.0","canonical_sha256":"3f550956ac37987969868d0fe854a0baa81032c79d04fd733f1a4348064764e7","source":{"kind":"arxiv","id":"1701.03088","version":3},"attestation_state":"computed","paper":{"title":"First measurement of $^{30}$S+$\\alpha$ resonant elastic scattering for the $^{30}$S($\\alpha$,p) reaction rate","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. A. Chen, A. Parikh, C. C. Yun, D. Kahl, D. N. Binh, H. S. Jung, H. Tokieda, H. Yamaguchi, J. Chen, K. Setoodehnia, L. Y. Zhang, N. Iwasa, N. N. Duy, S. Cherubini, S. Hayakawa, S. Kato, S. Kubono, S. Nishimura, S. Ota, T. Hashimoto, T. Teranishi, T. Yamada, Y. K. Kwon","submitted_at":"2017-01-11T18:27:14Z","abstract_excerpt":"Background: Type I x-ray bursts are the most frequent thermonuclear explosions in the galaxy, resulting from thermonuclear runaway on the surface of an accreting neutron star. The $^{30}$S($\\alpha$,p) reaction plays a critical role in burst models, yet insufficient experimental information is available to calculate a reliable, precise rate for this reaction. Purpose: Our measurement was conducted to search for states in $^{34}$Ar and determine their quantum properties. In particular, natural-parity states with large $\\alpha$-decay partial widths should dominate the stellar reaction rate. Metho"},"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":"1701.03088","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2017-01-11T18:27:14Z","cross_cats_sorted":[],"title_canon_sha256":"1e7b1cdc46ff2b29423c021c4f0464c701f3d5254de3bddc1774ee7414ffb7f5","abstract_canon_sha256":"7a40de996fb7d3ba0a63ab6f5845d29ab50b764ac1442e5801f3ecb16c05d41d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:30.523281Z","signature_b64":"DDn1tX3PRX7OdsyoMz+3UFMR1VFYQYmE3o5uzJVD0PMzOX2Mu7En/jxgJXwto3kk4QVVKXh5+mkq/JdlwomCDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3f550956ac37987969868d0fe854a0baa81032c79d04fd733f1a4348064764e7","last_reissued_at":"2026-05-18T00:26:30.522581Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:30.522581Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"First measurement of $^{30}$S+$\\alpha$ resonant elastic scattering for the $^{30}$S($\\alpha$,p) reaction rate","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. A. Chen, A. Parikh, C. C. Yun, D. Kahl, D. N. Binh, H. S. Jung, H. Tokieda, H. Yamaguchi, J. Chen, K. Setoodehnia, L. Y. Zhang, N. Iwasa, N. N. Duy, S. Cherubini, S. Hayakawa, S. Kato, S. Kubono, S. Nishimura, S. Ota, T. Hashimoto, T. Teranishi, T. Yamada, Y. K. Kwon","submitted_at":"2017-01-11T18:27:14Z","abstract_excerpt":"Background: Type I x-ray bursts are the most frequent thermonuclear explosions in the galaxy, resulting from thermonuclear runaway on the surface of an accreting neutron star. The $^{30}$S($\\alpha$,p) reaction plays a critical role in burst models, yet insufficient experimental information is available to calculate a reliable, precise rate for this reaction. Purpose: Our measurement was conducted to search for states in $^{34}$Ar and determine their quantum properties. In particular, natural-parity states with large $\\alpha$-decay partial widths should dominate the stellar reaction rate. Metho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.03088","kind":"arxiv","version":3},"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":"1701.03088","created_at":"2026-05-18T00:26:30.522711+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.03088v3","created_at":"2026-05-18T00:26:30.522711+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.03088","created_at":"2026-05-18T00:26:30.522711+00:00"},{"alias_kind":"pith_short_12","alias_value":"H5KQSVVMG6MH","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"H5KQSVVMG6MHS2MG","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"H5KQSVVM","created_at":"2026-05-18T12:31:18.294218+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/H5KQSVVMG6MHS2MGRUH6QVFAXK","json":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK.json","graph_json":"https://pith.science/api/pith-number/H5KQSVVMG6MHS2MGRUH6QVFAXK/graph.json","events_json":"https://pith.science/api/pith-number/H5KQSVVMG6MHS2MGRUH6QVFAXK/events.json","paper":"https://pith.science/paper/H5KQSVVM"},"agent_actions":{"view_html":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK","download_json":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK.json","view_paper":"https://pith.science/paper/H5KQSVVM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.03088&json=true","fetch_graph":"https://pith.science/api/pith-number/H5KQSVVMG6MHS2MGRUH6QVFAXK/graph.json","fetch_events":"https://pith.science/api/pith-number/H5KQSVVMG6MHS2MGRUH6QVFAXK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/action/storage_attestation","attest_author":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/action/author_attestation","sign_citation":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/action/citation_signature","submit_replication":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/action/replication_record"}},"created_at":"2026-05-18T00:26:30.522711+00:00","updated_at":"2026-05-18T00:26:30.522711+00:00"}