{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:B4MV6TLWTOBW7JJHP4KQS6DCWK","short_pith_number":"pith:B4MV6TLW","schema_version":"1.0","canonical_sha256":"0f195f4d769b836fa5277f15097862b2871186f01d0cde895d36c94c0ab28492","source":{"kind":"arxiv","id":"1012.0519","version":1},"attestation_state":"computed","paper":{"title":"Quantum Statistical Corrections to Astrophysical Photodisintegration Rates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.SR","authors_text":"A. B. Balantekin, G. J. Mathews, Motohiko Kusakabe, Toshitaka Kajino, Yamac Pehlivan","submitted_at":"2010-12-02T17:48:30Z","abstract_excerpt":"Tabulated rates for astrophysical photodisintegration reactions make use of Boltzmann statistics for the photons involved as well as the interacting nuclei. Here we derive analytic corrections for the Planck-spectrum quantum statistics of the photon energy distribution. These corrections can be deduced directly from the detailed-balance condition without the assumption of equilibrium as long as the photons are represented by a Planck spectrum. Moreover we show that these corrections affect not only the photodisintegration rates but also modify the conditions of nuclear statistical equilibrium "},"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":"1012.0519","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-12-02T17:48:30Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"aa57e37038fc5e1e392eb7d0ecb9116b3746b7ab5bdfd5af164086dc317bdb29","abstract_canon_sha256":"6b206b10150ba597d10c603018de02fc11c81313ce00ed4f48307d9ce5eaec6b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:35.888220Z","signature_b64":"LWWnhQxuuQ+bzqO/wJyAvewNjyGFQftRu0Tl+JKW1O4eXfZuciYmjxzMNoAp0X5DK82DNoxt13m/bbzDpuCtAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0f195f4d769b836fa5277f15097862b2871186f01d0cde895d36c94c0ab28492","last_reissued_at":"2026-05-18T02:04:35.887483Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:35.887483Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum Statistical Corrections to Astrophysical Photodisintegration Rates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.SR","authors_text":"A. B. Balantekin, G. J. Mathews, Motohiko Kusakabe, Toshitaka Kajino, Yamac Pehlivan","submitted_at":"2010-12-02T17:48:30Z","abstract_excerpt":"Tabulated rates for astrophysical photodisintegration reactions make use of Boltzmann statistics for the photons involved as well as the interacting nuclei. Here we derive analytic corrections for the Planck-spectrum quantum statistics of the photon energy distribution. These corrections can be deduced directly from the detailed-balance condition without the assumption of equilibrium as long as the photons are represented by a Planck spectrum. Moreover we show that these corrections affect not only the photodisintegration rates but also modify the conditions of nuclear statistical equilibrium "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.0519","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":"1012.0519","created_at":"2026-05-18T02:04:35.887620+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.0519v1","created_at":"2026-05-18T02:04:35.887620+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.0519","created_at":"2026-05-18T02:04:35.887620+00:00"},{"alias_kind":"pith_short_12","alias_value":"B4MV6TLWTOBW","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"B4MV6TLWTOBW7JJH","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"B4MV6TLW","created_at":"2026-05-18T12:26:05.355336+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/B4MV6TLWTOBW7JJHP4KQS6DCWK","json":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK.json","graph_json":"https://pith.science/api/pith-number/B4MV6TLWTOBW7JJHP4KQS6DCWK/graph.json","events_json":"https://pith.science/api/pith-number/B4MV6TLWTOBW7JJHP4KQS6DCWK/events.json","paper":"https://pith.science/paper/B4MV6TLW"},"agent_actions":{"view_html":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK","download_json":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK.json","view_paper":"https://pith.science/paper/B4MV6TLW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.0519&json=true","fetch_graph":"https://pith.science/api/pith-number/B4MV6TLWTOBW7JJHP4KQS6DCWK/graph.json","fetch_events":"https://pith.science/api/pith-number/B4MV6TLWTOBW7JJHP4KQS6DCWK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK/action/storage_attestation","attest_author":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK/action/author_attestation","sign_citation":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK/action/citation_signature","submit_replication":"https://pith.science/pith/B4MV6TLWTOBW7JJHP4KQS6DCWK/action/replication_record"}},"created_at":"2026-05-18T02:04:35.887620+00:00","updated_at":"2026-05-18T02:04:35.887620+00:00"}