{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:CQV3GBWSHFEBQ77MN2KBU6ODOQ","short_pith_number":"pith:CQV3GBWS","schema_version":"1.0","canonical_sha256":"142bb306d23948187fec6e941a79c37421539d0150337d0824c75166b7aacfd4","source":{"kind":"arxiv","id":"1210.2655","version":2},"attestation_state":"computed","paper":{"title":"Large-scale calculations of supernova neutrino-induced reactions in Z=8-82 target nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","astro-ph.SR","nucl-ex"],"primary_cat":"nucl-th","authors_text":"H. Tutman, N. Paar, T. Fischer, T. Marketin","submitted_at":"2012-10-09T16:10:37Z","abstract_excerpt":"Background: In the environment of high neutrino-fluxes provided in core-collapse supernovae or neutron star mergers, neutrino-induced reactions with nuclei contribute to the nucleosynthesis processes. A number of terrestrial neutrino detectors are based on inelastic neutrino-nucleus scattering and modeling of the respective cross sections allow predictions of the expected detector reaction rates.\n  Purpose: To provide a self-consistent microscopic description of neutrino-nucleus cross sections involving a large pool of Z = 8 - 82 nuclei for the implementation in models of nucleosynthesis and n"},"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":"1210.2655","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2012-10-09T16:10:37Z","cross_cats_sorted":["astro-ph.IM","astro-ph.SR","nucl-ex"],"title_canon_sha256":"c815a69790ee8832639b62f67e29a292c57bb7de44d9443b5cf29000fa9812af","abstract_canon_sha256":"9b0ca2727f1c6c9f11eb471bd0ad219a20c9db4d0c16cdd9327eb5f4997aaf64"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:03.956648Z","signature_b64":"MPt7Tl5gtzxq4r7kXOhj2eMAMxdUzPhmPO6mtb4Y4Z9kXRJRMTQQKR2RvVY/Srimjknq5xyLeWyNNfAbaNozBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"142bb306d23948187fec6e941a79c37421539d0150337d0824c75166b7aacfd4","last_reissued_at":"2026-05-18T01:54:03.955960Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:03.955960Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Large-scale calculations of supernova neutrino-induced reactions in Z=8-82 target nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","astro-ph.SR","nucl-ex"],"primary_cat":"nucl-th","authors_text":"H. Tutman, N. Paar, T. Fischer, T. Marketin","submitted_at":"2012-10-09T16:10:37Z","abstract_excerpt":"Background: In the environment of high neutrino-fluxes provided in core-collapse supernovae or neutron star mergers, neutrino-induced reactions with nuclei contribute to the nucleosynthesis processes. A number of terrestrial neutrino detectors are based on inelastic neutrino-nucleus scattering and modeling of the respective cross sections allow predictions of the expected detector reaction rates.\n  Purpose: To provide a self-consistent microscopic description of neutrino-nucleus cross sections involving a large pool of Z = 8 - 82 nuclei for the implementation in models of nucleosynthesis and n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.2655","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":"1210.2655","created_at":"2026-05-18T01:54:03.956063+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.2655v2","created_at":"2026-05-18T01:54:03.956063+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.2655","created_at":"2026-05-18T01:54:03.956063+00:00"},{"alias_kind":"pith_short_12","alias_value":"CQV3GBWSHFEB","created_at":"2026-05-18T12:27:01.376967+00:00"},{"alias_kind":"pith_short_16","alias_value":"CQV3GBWSHFEBQ77M","created_at":"2026-05-18T12:27:01.376967+00:00"},{"alias_kind":"pith_short_8","alias_value":"CQV3GBWS","created_at":"2026-05-18T12:27:01.376967+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/CQV3GBWSHFEBQ77MN2KBU6ODOQ","json":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ.json","graph_json":"https://pith.science/api/pith-number/CQV3GBWSHFEBQ77MN2KBU6ODOQ/graph.json","events_json":"https://pith.science/api/pith-number/CQV3GBWSHFEBQ77MN2KBU6ODOQ/events.json","paper":"https://pith.science/paper/CQV3GBWS"},"agent_actions":{"view_html":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ","download_json":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ.json","view_paper":"https://pith.science/paper/CQV3GBWS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.2655&json=true","fetch_graph":"https://pith.science/api/pith-number/CQV3GBWSHFEBQ77MN2KBU6ODOQ/graph.json","fetch_events":"https://pith.science/api/pith-number/CQV3GBWSHFEBQ77MN2KBU6ODOQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ/action/storage_attestation","attest_author":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ/action/author_attestation","sign_citation":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ/action/citation_signature","submit_replication":"https://pith.science/pith/CQV3GBWSHFEBQ77MN2KBU6ODOQ/action/replication_record"}},"created_at":"2026-05-18T01:54:03.956063+00:00","updated_at":"2026-05-18T01:54:03.956063+00:00"}