{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:I4ZWE75IRVNANKGLN7HNQTTS7J","short_pith_number":"pith:I4ZWE75I","schema_version":"1.0","canonical_sha256":"4733627fa88d5a06a8cb6fced84e72fa61c5521e3e036724a648d22a375f05d6","source":{"kind":"arxiv","id":"1711.09098","version":2},"attestation_state":"computed","paper":{"title":"Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex","nucl-th"],"primary_cat":"astro-ph.SR","authors_text":"A. St. J. Murphy, C. Travaglio, G. Cescutti, N. Nishimura, R. Hirschi, T. Rauscher","submitted_at":"2017-11-24T19:00:01Z","abstract_excerpt":"Thermonuclear supernovae originating from the explosion of a white dwarf accreting mass from a companion star have been suggested as a site for the production of $p$ nuclides. Such nuclei are produced during the explosion, in layers enriched with seed nuclei coming from prior strong $s$ processing. These seeds are transformed to proton-richer isotopes mainly by photodisintegration reactions. Several thousand trajectories from a 2D explosion model were used in a Monte Carlo approach. Temperature-dependent uncertainties were assigned individually to thousands of rates varied simultaneously in po"},"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":"1711.09098","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-11-24T19:00:01Z","cross_cats_sorted":["nucl-ex","nucl-th"],"title_canon_sha256":"b2f32c14490f2c6dbd5058cbb470326cab20441aeb13b36f50480b6d216a0154","abstract_canon_sha256":"ae7607002dfed56e7e511331d41e348b367a72424a6c4b72b57b825beab1245b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:59.987302Z","signature_b64":"OwL5SzZv9vl1EOv/xydYOZRg6w5hwyqajl4NPK8r2S45RIDbjlJPvs9JFo/tP6RyogW9MPtMpWkgwhvb3utFCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4733627fa88d5a06a8cb6fced84e72fa61c5521e3e036724a648d22a375f05d6","last_reissued_at":"2026-05-18T00:26:59.986649Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:59.986649Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex","nucl-th"],"primary_cat":"astro-ph.SR","authors_text":"A. St. J. Murphy, C. Travaglio, G. Cescutti, N. Nishimura, R. Hirschi, T. Rauscher","submitted_at":"2017-11-24T19:00:01Z","abstract_excerpt":"Thermonuclear supernovae originating from the explosion of a white dwarf accreting mass from a companion star have been suggested as a site for the production of $p$ nuclides. Such nuclei are produced during the explosion, in layers enriched with seed nuclei coming from prior strong $s$ processing. These seeds are transformed to proton-richer isotopes mainly by photodisintegration reactions. Several thousand trajectories from a 2D explosion model were used in a Monte Carlo approach. Temperature-dependent uncertainties were assigned individually to thousands of rates varied simultaneously in po"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.09098","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":"1711.09098","created_at":"2026-05-18T00:26:59.986745+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.09098v2","created_at":"2026-05-18T00:26:59.986745+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.09098","created_at":"2026-05-18T00:26:59.986745+00:00"},{"alias_kind":"pith_short_12","alias_value":"I4ZWE75IRVNA","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_16","alias_value":"I4ZWE75IRVNANKGL","created_at":"2026-05-18T12:31:21.493067+00:00"},{"alias_kind":"pith_short_8","alias_value":"I4ZWE75I","created_at":"2026-05-18T12:31:21.493067+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/I4ZWE75IRVNANKGLN7HNQTTS7J","json":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J.json","graph_json":"https://pith.science/api/pith-number/I4ZWE75IRVNANKGLN7HNQTTS7J/graph.json","events_json":"https://pith.science/api/pith-number/I4ZWE75IRVNANKGLN7HNQTTS7J/events.json","paper":"https://pith.science/paper/I4ZWE75I"},"agent_actions":{"view_html":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J","download_json":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J.json","view_paper":"https://pith.science/paper/I4ZWE75I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.09098&json=true","fetch_graph":"https://pith.science/api/pith-number/I4ZWE75IRVNANKGLN7HNQTTS7J/graph.json","fetch_events":"https://pith.science/api/pith-number/I4ZWE75IRVNANKGLN7HNQTTS7J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J/action/storage_attestation","attest_author":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J/action/author_attestation","sign_citation":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J/action/citation_signature","submit_replication":"https://pith.science/pith/I4ZWE75IRVNANKGLN7HNQTTS7J/action/replication_record"}},"created_at":"2026-05-18T00:26:59.986745+00:00","updated_at":"2026-05-18T00:26:59.986745+00:00"}