{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:6FJKIXEK2TOWMGZJVKJ2XOX72O","short_pith_number":"pith:6FJKIXEK","schema_version":"1.0","canonical_sha256":"f152a45c8ad4dd661b29aa93abbaffd38442c1ab1a63f0a417145c3c4e191c77","source":{"kind":"arxiv","id":"2411.13123","version":1},"attestation_state":"computed","paper":{"title":"Validity of Brink Axel Hypothesis for calculations of allowed stellar weak rates of heavy nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"nucl-th","authors_text":"Fakeha Farooq, Jameel-Un Nabi, Ramoona Shehzadi","submitted_at":"2024-11-20T08:34:42Z","abstract_excerpt":"The knowledge of beta decay transitional probabilities and GamowTeller (GT) strength functions from highly excited states of nuclides is of particular importance for applications to astrophysical network calculations of nucleosynthesis in explosive stellar events. These quantities are challenging to achieve from measurements or computations using various nuclear models. Due to unavailability of feasible alternatives, many theoretical studies often rely on the Brink Axel (BA) hypothesis, that is, the response of strength functions depends merely on the transition energy of the parent nuclear gr"},"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":"2411.13123","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2024-11-20T08:34:42Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"801bdb883c7fe5a9fdc8f8df77b6c8beb9ec9203a6638f4a141398a0b1f00d47","abstract_canon_sha256":"b94891c8567b48c7e50fa7266a6608746f368e70172b357aeab0af1473a6d00e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:38:05.445455Z","signature_b64":"UEYV/Pp+kB7gd3myODT25jDEIp5Ks4pGtIic2VRVtQIxtYGDmtEq+zSv2yVvLUkwo9XEi4ZLIhVdzTsDCw4EAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f152a45c8ad4dd661b29aa93abbaffd38442c1ab1a63f0a417145c3c4e191c77","last_reissued_at":"2026-07-05T09:38:05.444979Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:38:05.444979Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Validity of Brink Axel Hypothesis for calculations of allowed stellar weak rates of heavy nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"nucl-th","authors_text":"Fakeha Farooq, Jameel-Un Nabi, Ramoona Shehzadi","submitted_at":"2024-11-20T08:34:42Z","abstract_excerpt":"The knowledge of beta decay transitional probabilities and GamowTeller (GT) strength functions from highly excited states of nuclides is of particular importance for applications to astrophysical network calculations of nucleosynthesis in explosive stellar events. These quantities are challenging to achieve from measurements or computations using various nuclear models. Due to unavailability of feasible alternatives, many theoretical studies often rely on the Brink Axel (BA) hypothesis, that is, the response of strength functions depends merely on the transition energy of the parent nuclear gr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.13123","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.13123/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2411.13123","created_at":"2026-07-05T09:38:05.445041+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.13123v1","created_at":"2026-07-05T09:38:05.445041+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.13123","created_at":"2026-07-05T09:38:05.445041+00:00"},{"alias_kind":"pith_short_12","alias_value":"6FJKIXEK2TOW","created_at":"2026-07-05T09:38:05.445041+00:00"},{"alias_kind":"pith_short_16","alias_value":"6FJKIXEK2TOWMGZJ","created_at":"2026-07-05T09:38:05.445041+00:00"},{"alias_kind":"pith_short_8","alias_value":"6FJKIXEK","created_at":"2026-07-05T09:38:05.445041+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/6FJKIXEK2TOWMGZJVKJ2XOX72O","json":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O.json","graph_json":"https://pith.science/api/pith-number/6FJKIXEK2TOWMGZJVKJ2XOX72O/graph.json","events_json":"https://pith.science/api/pith-number/6FJKIXEK2TOWMGZJVKJ2XOX72O/events.json","paper":"https://pith.science/paper/6FJKIXEK"},"agent_actions":{"view_html":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O","download_json":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O.json","view_paper":"https://pith.science/paper/6FJKIXEK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.13123&json=true","fetch_graph":"https://pith.science/api/pith-number/6FJKIXEK2TOWMGZJVKJ2XOX72O/graph.json","fetch_events":"https://pith.science/api/pith-number/6FJKIXEK2TOWMGZJVKJ2XOX72O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O/action/storage_attestation","attest_author":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O/action/author_attestation","sign_citation":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O/action/citation_signature","submit_replication":"https://pith.science/pith/6FJKIXEK2TOWMGZJVKJ2XOX72O/action/replication_record"}},"created_at":"2026-07-05T09:38:05.445041+00:00","updated_at":"2026-07-05T09:38:05.445041+00:00"}