{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:H5KQSVVMG6MHS2MGRUH6QVFAXK","short_pith_number":"pith:H5KQSVVM","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"},"canonical_sha256":"3f550956ac37987969868d0fe854a0baa81032c79d04fd733f1a4348064764e7","source":{"kind":"arxiv","id":"1701.03088","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.03088","created_at":"2026-05-18T00:26:30Z"},{"alias_kind":"arxiv_version","alias_value":"1701.03088v3","created_at":"2026-05-18T00:26:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.03088","created_at":"2026-05-18T00:26:30Z"},{"alias_kind":"pith_short_12","alias_value":"H5KQSVVMG6MH","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"H5KQSVVMG6MHS2MG","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"H5KQSVVM","created_at":"2026-05-18T12:31:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:H5KQSVVMG6MHS2MGRUH6QVFAXK","target":"record","payload":{"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"},"canonical_sha256":"3f550956ac37987969868d0fe854a0baa81032c79d04fd733f1a4348064764e7","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"},"source_kind":"arxiv","source_id":"1701.03088","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:26:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ERi7MdF+BwqokkCyJ0lnhnjm0g7pCgQ/J+jPJ/mZDPMJWKYdRlMobl2O6Ga+BYsqr1/DjbvjtEJnjwSfbx/gBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T00:08:08.350279Z"},"content_sha256":"9369cc2f34376fd2e0098e2e2680dd84052c361821538a108ecfad8b95375ef2","schema_version":"1.0","event_id":"sha256:9369cc2f34376fd2e0098e2e2680dd84052c361821538a108ecfad8b95375ef2"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:H5KQSVVMG6MHS2MGRUH6QVFAXK","target":"graph","payload":{"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:26:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"K1P+pmqLxJ5VFz15qRXK4B91uQwDaQr23aZxY7w+jiwB67Cz+qM5sSp2XqFHMETmtUOZRAMB47G+DU1XCu9HDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T00:08:08.350842Z"},"content_sha256":"59f615a92440d4e3178fe4e66a12d300b5896338448bdd4883ae1b7cb42f6be0","schema_version":"1.0","event_id":"sha256:59f615a92440d4e3178fe4e66a12d300b5896338448bdd4883ae1b7cb42f6be0"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/bundle.json","state_url":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-03T00:08:08Z","links":{"resolver":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK","bundle":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/bundle.json","state":"https://pith.science/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/state.json","well_known_bundle":"https://pith.science/.well-known/pith/H5KQSVVMG6MHS2MGRUH6QVFAXK/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:H5KQSVVMG6MHS2MGRUH6QVFAXK","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"7a40de996fb7d3ba0a63ab6f5845d29ab50b764ac1442e5801f3ecb16c05d41d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2017-01-11T18:27:14Z","title_canon_sha256":"1e7b1cdc46ff2b29423c021c4f0464c701f3d5254de3bddc1774ee7414ffb7f5"},"schema_version":"1.0","source":{"id":"1701.03088","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.03088","created_at":"2026-05-18T00:26:30Z"},{"alias_kind":"arxiv_version","alias_value":"1701.03088v3","created_at":"2026-05-18T00:26:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.03088","created_at":"2026-05-18T00:26:30Z"},{"alias_kind":"pith_short_12","alias_value":"H5KQSVVMG6MH","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"H5KQSVVMG6MHS2MG","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"H5KQSVVM","created_at":"2026-05-18T12:31:18Z"}],"graph_snapshots":[{"event_id":"sha256:59f615a92440d4e3178fe4e66a12d300b5896338448bdd4883ae1b7cb42f6be0","target":"graph","created_at":"2026-05-18T00:26:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"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","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","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2017-01-11T18:27:14Z","title":"First measurement of $^{30}$S+$\\alpha$ resonant elastic scattering for the $^{30}$S($\\alpha$,p) reaction rate"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.03088","kind":"arxiv","version":3},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:9369cc2f34376fd2e0098e2e2680dd84052c361821538a108ecfad8b95375ef2","target":"record","created_at":"2026-05-18T00:26:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"7a40de996fb7d3ba0a63ab6f5845d29ab50b764ac1442e5801f3ecb16c05d41d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2017-01-11T18:27:14Z","title_canon_sha256":"1e7b1cdc46ff2b29423c021c4f0464c701f3d5254de3bddc1774ee7414ffb7f5"},"schema_version":"1.0","source":{"id":"1701.03088","kind":"arxiv","version":3}},"canonical_sha256":"3f550956ac37987969868d0fe854a0baa81032c79d04fd733f1a4348064764e7","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3f550956ac37987969868d0fe854a0baa81032c79d04fd733f1a4348064764e7","first_computed_at":"2026-05-18T00:26:30.522581Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:26:30.522581Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"DDn1tX3PRX7OdsyoMz+3UFMR1VFYQYmE3o5uzJVD0PMzOX2Mu7En/jxgJXwto3kk4QVVKXh5+mkq/JdlwomCDg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:26:30.523281Z","signed_message":"canonical_sha256_bytes"},"source_id":"1701.03088","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:9369cc2f34376fd2e0098e2e2680dd84052c361821538a108ecfad8b95375ef2","sha256:59f615a92440d4e3178fe4e66a12d300b5896338448bdd4883ae1b7cb42f6be0"],"state_sha256":"209f6913c5238cfc0a726a6f889b233bbd2a88877d70739ee2fcdc50a4ca2c3b"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"O5YuR24+kv/d05l51JVziwC+ZzrEFc0fuhqm5FsIvCHVFH0bOCXvYVIaBrPb3XIBHobrOh6+cHEMABCnEQ/GDg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-03T00:08:08.353410Z","bundle_sha256":"0c4de0dbba6e20f7ff10f0497f5dd9062c6a2689ea6ab4ec8a48f9816fd8be7d"}}