{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:VO3LRF566O5AQYSARX5B3CAMZM","short_pith_number":"pith:VO3LRF56","schema_version":"1.0","canonical_sha256":"abb6b897bef3ba0862408dfa1d880ccb2127e54e4ee6da2115f5c8e7b196d006","source":{"kind":"arxiv","id":"1605.07810","version":1},"attestation_state":"computed","paper":{"title":"Recent results in nuclear astrophysics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"nucl-ex","authors_text":"Alain Coc, Fairouz Hammache, Juergen Kiener","submitted_at":"2016-05-25T10:21:55Z","abstract_excerpt":"In this review, we emphasize the interplay between astrophysical observations, modeling, and nuclear physics laboratory experiments. Several important nuclear cross sections for astrophysics have long been identified e.g. 12C(alpha,gamma)16O for stellar evolution, or 13C(alpha,n)16O and 22Ne(alpha,n)25Mg as neutron sources for the s-process. More recently, observations of lithium abundances in the oldest stars, or of nuclear gamma-ray lines from space, have required new laboratory experiments. New evaluation of thermonuclear reaction rates now includes the associated rate uncertainties that ar"},"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":"1605.07810","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-ex","submitted_at":"2016-05-25T10:21:55Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"ba5bb14dda13dc66c63d4144b1d05fbff5c11912d7ef08442d4f0fc793ee41e9","abstract_canon_sha256":"6be3eb08dea651ab170f5338917709db7caf6bb85c74fc55027c7a6a252177c6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:39.037618Z","signature_b64":"cfOEU/Hm0m5ZRb4ZTrn2n0e+lm5UANm4IDM+UsLmQKxQlleyLfRN0WHivaLMJx4SNrT6drKcJ5zVPYTwXP1RBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"abb6b897bef3ba0862408dfa1d880ccb2127e54e4ee6da2115f5c8e7b196d006","last_reissued_at":"2026-05-18T01:13:39.036548Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:39.036548Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Recent results in nuclear astrophysics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"nucl-ex","authors_text":"Alain Coc, Fairouz Hammache, Juergen Kiener","submitted_at":"2016-05-25T10:21:55Z","abstract_excerpt":"In this review, we emphasize the interplay between astrophysical observations, modeling, and nuclear physics laboratory experiments. Several important nuclear cross sections for astrophysics have long been identified e.g. 12C(alpha,gamma)16O for stellar evolution, or 13C(alpha,n)16O and 22Ne(alpha,n)25Mg as neutron sources for the s-process. More recently, observations of lithium abundances in the oldest stars, or of nuclear gamma-ray lines from space, have required new laboratory experiments. New evaluation of thermonuclear reaction rates now includes the associated rate uncertainties that ar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.07810","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1605.07810","created_at":"2026-05-18T01:13:39.036763+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.07810v1","created_at":"2026-05-18T01:13:39.036763+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.07810","created_at":"2026-05-18T01:13:39.036763+00:00"},{"alias_kind":"pith_short_12","alias_value":"VO3LRF566O5A","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_16","alias_value":"VO3LRF566O5AQYSA","created_at":"2026-05-18T12:30:48.956258+00:00"},{"alias_kind":"pith_short_8","alias_value":"VO3LRF56","created_at":"2026-05-18T12:30:48.956258+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/VO3LRF566O5AQYSARX5B3CAMZM","json":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM.json","graph_json":"https://pith.science/api/pith-number/VO3LRF566O5AQYSARX5B3CAMZM/graph.json","events_json":"https://pith.science/api/pith-number/VO3LRF566O5AQYSARX5B3CAMZM/events.json","paper":"https://pith.science/paper/VO3LRF56"},"agent_actions":{"view_html":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM","download_json":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM.json","view_paper":"https://pith.science/paper/VO3LRF56","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.07810&json=true","fetch_graph":"https://pith.science/api/pith-number/VO3LRF566O5AQYSARX5B3CAMZM/graph.json","fetch_events":"https://pith.science/api/pith-number/VO3LRF566O5AQYSARX5B3CAMZM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM/action/storage_attestation","attest_author":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM/action/author_attestation","sign_citation":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM/action/citation_signature","submit_replication":"https://pith.science/pith/VO3LRF566O5AQYSARX5B3CAMZM/action/replication_record"}},"created_at":"2026-05-18T01:13:39.036763+00:00","updated_at":"2026-05-18T01:13:39.036763+00:00"}