{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:2GE3HFQCWD5FFQADQDFPTOQQEM","short_pith_number":"pith:2GE3HFQC","schema_version":"1.0","canonical_sha256":"d189b39602b0fa52c00380caf9ba10230c80d188909bfbc0b61e395b2db07d07","source":{"kind":"arxiv","id":"1404.6825","version":1},"attestation_state":"computed","paper":{"title":"Imaginary mass lune determinants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"J.S.Dowker","submitted_at":"2014-04-27T20:40:14Z","abstract_excerpt":"Functional determinants for a scalar field with negative mass squared are numerically evaluated on an orbifolded three-sphere, in particular on a lune and on a regular 4--polytope fundamental domain. Graphs are provided of the logdets and some Hartle-Hawking probabilities, on the basis of the dS/CFT correspondence."},"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":"1404.6825","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2014-04-27T20:40:14Z","cross_cats_sorted":[],"title_canon_sha256":"ac33bc8c7cac4dcb0024da1a5cfcb2f955d48e3ac6ca67a93b616c916e5d8969","abstract_canon_sha256":"3acd3626baf299a5cd3324f02eb359fbcc790d1388ea342cea31a28bb5020cd8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:53:05.826922Z","signature_b64":"W2FQcxVagkvlxmV9piDkc/2Syt4ee/DOb7k/8xTY7sKYGLnMMBevx2RMeqWi9Osq2uie8FQACmFnTBiF4y3FDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d189b39602b0fa52c00380caf9ba10230c80d188909bfbc0b61e395b2db07d07","last_reissued_at":"2026-05-18T02:53:05.826486Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:53:05.826486Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Imaginary mass lune determinants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"J.S.Dowker","submitted_at":"2014-04-27T20:40:14Z","abstract_excerpt":"Functional determinants for a scalar field with negative mass squared are numerically evaluated on an orbifolded three-sphere, in particular on a lune and on a regular 4--polytope fundamental domain. Graphs are provided of the logdets and some Hartle-Hawking probabilities, on the basis of the dS/CFT correspondence."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.6825","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":"1404.6825","created_at":"2026-05-18T02:53:05.826561+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.6825v1","created_at":"2026-05-18T02:53:05.826561+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.6825","created_at":"2026-05-18T02:53:05.826561+00:00"},{"alias_kind":"pith_short_12","alias_value":"2GE3HFQCWD5F","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_16","alias_value":"2GE3HFQCWD5FFQAD","created_at":"2026-05-18T12:28:11.866339+00:00"},{"alias_kind":"pith_short_8","alias_value":"2GE3HFQC","created_at":"2026-05-18T12:28:11.866339+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/2GE3HFQCWD5FFQADQDFPTOQQEM","json":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM.json","graph_json":"https://pith.science/api/pith-number/2GE3HFQCWD5FFQADQDFPTOQQEM/graph.json","events_json":"https://pith.science/api/pith-number/2GE3HFQCWD5FFQADQDFPTOQQEM/events.json","paper":"https://pith.science/paper/2GE3HFQC"},"agent_actions":{"view_html":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM","download_json":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM.json","view_paper":"https://pith.science/paper/2GE3HFQC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.6825&json=true","fetch_graph":"https://pith.science/api/pith-number/2GE3HFQCWD5FFQADQDFPTOQQEM/graph.json","fetch_events":"https://pith.science/api/pith-number/2GE3HFQCWD5FFQADQDFPTOQQEM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM/action/storage_attestation","attest_author":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM/action/author_attestation","sign_citation":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM/action/citation_signature","submit_replication":"https://pith.science/pith/2GE3HFQCWD5FFQADQDFPTOQQEM/action/replication_record"}},"created_at":"2026-05-18T02:53:05.826561+00:00","updated_at":"2026-05-18T02:53:05.826561+00:00"}