{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QK6I4R52TIDLW2XP3H7MZIJBTA","short_pith_number":"pith:QK6I4R52","schema_version":"1.0","canonical_sha256":"82bc8e47ba9a06bb6aefd9fecca12198101a5816923268b64c0cf9d55200c318","source":{"kind":"arxiv","id":"1610.05752","version":2},"attestation_state":"computed","paper":{"title":"Impact of New Gamow-Teller Strengths on Explosive Type Ia Supernova Nucleosynthesis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jun Hidaka, Kanji Mori, Ken'ichi Nomoto, Koichi Iwamoto, Michael A. Famiano, Michio Honma, Takaharu Otsuka, Toshio Suzuki, Toshitaka Kajino","submitted_at":"2016-10-18T19:34:58Z","abstract_excerpt":"Recent experimental results have confirmed a possible reduction in the GT$_+$ strengths of pf-shell nuclei. These proton-rich nuclei are of relevance in the deflagration and explosive burning phases of Type Ia supernovae. While prior GT strengths result in nucleosynthesis predictions with a lower-than-expected electron fraction, a reduction in the GT$_+$ strength can result in an slightly increased electron fraction compared to previous shell model predictions, though the enhancement is not as large as previous enhancements in going from rates computed by Fuller, Fowler, and Newman based on an"},"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":"1610.05752","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-10-18T19:34:58Z","cross_cats_sorted":[],"title_canon_sha256":"a005eb4a82eebe25d2e67f05f80ff1dedef5dc3c258b3a93da0891b15b893aac","abstract_canon_sha256":"dbd22c289bb8495d5f034e68cae42688e52c2e5eb801f5af17c61e165b0defd0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:54:28.400972Z","signature_b64":"glIiBVxZKAjxWncIJq2l/ygDUz/hMpHKsVzy2TNX5GFJ4fdl8WuukzEw7a/ze01fKqRRab7iuzuXmLphlMjRBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"82bc8e47ba9a06bb6aefd9fecca12198101a5816923268b64c0cf9d55200c318","last_reissued_at":"2026-05-18T00:54:28.400250Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:54:28.400250Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Impact of New Gamow-Teller Strengths on Explosive Type Ia Supernova Nucleosynthesis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jun Hidaka, Kanji Mori, Ken'ichi Nomoto, Koichi Iwamoto, Michael A. Famiano, Michio Honma, Takaharu Otsuka, Toshio Suzuki, Toshitaka Kajino","submitted_at":"2016-10-18T19:34:58Z","abstract_excerpt":"Recent experimental results have confirmed a possible reduction in the GT$_+$ strengths of pf-shell nuclei. These proton-rich nuclei are of relevance in the deflagration and explosive burning phases of Type Ia supernovae. While prior GT strengths result in nucleosynthesis predictions with a lower-than-expected electron fraction, a reduction in the GT$_+$ strength can result in an slightly increased electron fraction compared to previous shell model predictions, though the enhancement is not as large as previous enhancements in going from rates computed by Fuller, Fowler, and Newman based on an"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.05752","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":"1610.05752","created_at":"2026-05-18T00:54:28.400379+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.05752v2","created_at":"2026-05-18T00:54:28.400379+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.05752","created_at":"2026-05-18T00:54:28.400379+00:00"},{"alias_kind":"pith_short_12","alias_value":"QK6I4R52TIDL","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"QK6I4R52TIDLW2XP","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"QK6I4R52","created_at":"2026-05-18T12:30:39.010887+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/QK6I4R52TIDLW2XP3H7MZIJBTA","json":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA.json","graph_json":"https://pith.science/api/pith-number/QK6I4R52TIDLW2XP3H7MZIJBTA/graph.json","events_json":"https://pith.science/api/pith-number/QK6I4R52TIDLW2XP3H7MZIJBTA/events.json","paper":"https://pith.science/paper/QK6I4R52"},"agent_actions":{"view_html":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA","download_json":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA.json","view_paper":"https://pith.science/paper/QK6I4R52","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.05752&json=true","fetch_graph":"https://pith.science/api/pith-number/QK6I4R52TIDLW2XP3H7MZIJBTA/graph.json","fetch_events":"https://pith.science/api/pith-number/QK6I4R52TIDLW2XP3H7MZIJBTA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA/action/storage_attestation","attest_author":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA/action/author_attestation","sign_citation":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA/action/citation_signature","submit_replication":"https://pith.science/pith/QK6I4R52TIDLW2XP3H7MZIJBTA/action/replication_record"}},"created_at":"2026-05-18T00:54:28.400379+00:00","updated_at":"2026-05-18T00:54:28.400379+00:00"}