{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:USHE5UGOYWK6WJF3L4V25246NG","short_pith_number":"pith:USHE5UGO","schema_version":"1.0","canonical_sha256":"a48e4ed0cec595eb24bb5f2baeeb9e698276111d569331af7abd75b9e5803a9d","source":{"kind":"arxiv","id":"1612.03611","version":1},"attestation_state":"computed","paper":{"title":"Neutrino Processes with Hot Nuclei in Supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"A. I. Vdovin, Alan A. Dzhioev","submitted_at":"2016-12-12T10:57:36Z","abstract_excerpt":"In this paper, we calculate cross sections for charged-current neutrino-nucleus processes occuring under presupernova conditions. To treat thermal effects we extend self-consistent Skyrme-QRPA calculations to finite temperature by using the formalism of thermo field dynamics. The numerical results are presented for the sample nuclei, $^{56}$Fe and $^{82}$Ge"},"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":"1612.03611","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2016-12-12T10:57:36Z","cross_cats_sorted":[],"title_canon_sha256":"03c032f0bb9469a604b2f1309331fb57be40d85e05f9eadf907c5f8705bb16bc","abstract_canon_sha256":"c0ad2dd18be6cb44272efcbca16c48e2718a43e2ac84c6812b7eb078904f09fd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:45:44.250290Z","signature_b64":"o96bqpDUdkZLbcTd9QRYzwuqTzgFIla2RzLw1l+Fw7YcIt9jr2IICfIJhDRn+N21hnPX9chC0ry04XTHosBwDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a48e4ed0cec595eb24bb5f2baeeb9e698276111d569331af7abd75b9e5803a9d","last_reissued_at":"2026-05-18T00:45:44.249621Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:45:44.249621Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino Processes with Hot Nuclei in Supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"A. I. Vdovin, Alan A. Dzhioev","submitted_at":"2016-12-12T10:57:36Z","abstract_excerpt":"In this paper, we calculate cross sections for charged-current neutrino-nucleus processes occuring under presupernova conditions. To treat thermal effects we extend self-consistent Skyrme-QRPA calculations to finite temperature by using the formalism of thermo field dynamics. The numerical results are presented for the sample nuclei, $^{56}$Fe and $^{82}$Ge"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.03611","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":"1612.03611","created_at":"2026-05-18T00:45:44.249745+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.03611v1","created_at":"2026-05-18T00:45:44.249745+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.03611","created_at":"2026-05-18T00:45:44.249745+00:00"},{"alias_kind":"pith_short_12","alias_value":"USHE5UGOYWK6","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_16","alias_value":"USHE5UGOYWK6WJF3","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_8","alias_value":"USHE5UGO","created_at":"2026-05-18T12:30:46.583412+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/USHE5UGOYWK6WJF3L4V25246NG","json":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG.json","graph_json":"https://pith.science/api/pith-number/USHE5UGOYWK6WJF3L4V25246NG/graph.json","events_json":"https://pith.science/api/pith-number/USHE5UGOYWK6WJF3L4V25246NG/events.json","paper":"https://pith.science/paper/USHE5UGO"},"agent_actions":{"view_html":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG","download_json":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG.json","view_paper":"https://pith.science/paper/USHE5UGO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.03611&json=true","fetch_graph":"https://pith.science/api/pith-number/USHE5UGOYWK6WJF3L4V25246NG/graph.json","fetch_events":"https://pith.science/api/pith-number/USHE5UGOYWK6WJF3L4V25246NG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG/action/storage_attestation","attest_author":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG/action/author_attestation","sign_citation":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG/action/citation_signature","submit_replication":"https://pith.science/pith/USHE5UGOYWK6WJF3L4V25246NG/action/replication_record"}},"created_at":"2026-05-18T00:45:44.249745+00:00","updated_at":"2026-05-18T00:45:44.249745+00:00"}