{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:BQPKROGJWKCENIMYNMZUMGRNBS","short_pith_number":"pith:BQPKROGJ","schema_version":"1.0","canonical_sha256":"0c1ea8b8c9b28446a1986b33461a2d0ca82b14d67df8deb0abcf215b0dbc6b0b","source":{"kind":"arxiv","id":"1804.03947","version":1},"attestation_state":"computed","paper":{"title":"Production of Mo and Ru isotopes in neutrino-driven winds: implications for solar abundances and presolar grains","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Almudena Arcones, Julia Bliss, Yong-Zhong Qian","submitted_at":"2018-04-11T11:50:26Z","abstract_excerpt":"The origin of the so-called $p$-isotopes $^{92,94}\\mathrm{Mo}$ and $^{96,98}\\mathrm{Ru}$ in the solar system remains a mystery as several astrophysical scenarios fail to account for them. In addition, data on presolar silicon carbide grains of type X (SiC X) exhibit peculiar Mo patterns, especially for $^{95,97}\\mathrm{Mo}$. We examine production of Mo and Ru isotopes in neutrino-driven winds associated with core-collapse supernovae (CCSNe) over a wide range of conditions. We find that proton-rich winds can make dominant contributions to the solar abundance of $^{98}\\mathrm{Ru}$, significant c"},"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":"1804.03947","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-04-11T11:50:26Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"5fea245fcc430eb225267d7c727d1d703a111cd96382128c96f773329b923aef","abstract_canon_sha256":"1f8bd0513b7b0e26d1f5f65d94c9f2a7664c8bad26b628d61580a6a67d694f30"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:02:35.247087Z","signature_b64":"nnqC3rdG4oZhpxrGoiO7Uddhu6IlWdbmgQ2HFcgn+Ehtq5r9DW7QnTCmE1Erqk+uitEe8dirDp637TRR/OxfBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c1ea8b8c9b28446a1986b33461a2d0ca82b14d67df8deb0abcf215b0dbc6b0b","last_reissued_at":"2026-05-18T00:02:35.246460Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:02:35.246460Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Production of Mo and Ru isotopes in neutrino-driven winds: implications for solar abundances and presolar grains","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Almudena Arcones, Julia Bliss, Yong-Zhong Qian","submitted_at":"2018-04-11T11:50:26Z","abstract_excerpt":"The origin of the so-called $p$-isotopes $^{92,94}\\mathrm{Mo}$ and $^{96,98}\\mathrm{Ru}$ in the solar system remains a mystery as several astrophysical scenarios fail to account for them. In addition, data on presolar silicon carbide grains of type X (SiC X) exhibit peculiar Mo patterns, especially for $^{95,97}\\mathrm{Mo}$. We examine production of Mo and Ru isotopes in neutrino-driven winds associated with core-collapse supernovae (CCSNe) over a wide range of conditions. We find that proton-rich winds can make dominant contributions to the solar abundance of $^{98}\\mathrm{Ru}$, significant c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.03947","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":"1804.03947","created_at":"2026-05-18T00:02:35.246569+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.03947v1","created_at":"2026-05-18T00:02:35.246569+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.03947","created_at":"2026-05-18T00:02:35.246569+00:00"},{"alias_kind":"pith_short_12","alias_value":"BQPKROGJWKCE","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_16","alias_value":"BQPKROGJWKCENIMY","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_8","alias_value":"BQPKROGJ","created_at":"2026-05-18T12:32:16.446611+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/BQPKROGJWKCENIMYNMZUMGRNBS","json":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS.json","graph_json":"https://pith.science/api/pith-number/BQPKROGJWKCENIMYNMZUMGRNBS/graph.json","events_json":"https://pith.science/api/pith-number/BQPKROGJWKCENIMYNMZUMGRNBS/events.json","paper":"https://pith.science/paper/BQPKROGJ"},"agent_actions":{"view_html":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS","download_json":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS.json","view_paper":"https://pith.science/paper/BQPKROGJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.03947&json=true","fetch_graph":"https://pith.science/api/pith-number/BQPKROGJWKCENIMYNMZUMGRNBS/graph.json","fetch_events":"https://pith.science/api/pith-number/BQPKROGJWKCENIMYNMZUMGRNBS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS/action/storage_attestation","attest_author":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS/action/author_attestation","sign_citation":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS/action/citation_signature","submit_replication":"https://pith.science/pith/BQPKROGJWKCENIMYNMZUMGRNBS/action/replication_record"}},"created_at":"2026-05-18T00:02:35.246569+00:00","updated_at":"2026-05-18T00:02:35.246569+00:00"}