{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:EZRODWOULNIYNMOMNQCBPBZQ66","short_pith_number":"pith:EZRODWOU","schema_version":"1.0","canonical_sha256":"2662e1d9d45b5186b1cc6c04178730f79aa371809734214693fff265228950a2","source":{"kind":"arxiv","id":"gr-qc/9609056","version":2},"attestation_state":"computed","paper":{"title":"Interacting Spinor and Scalar Fields in Bianchi type-I Universe filled with Perfect Fluid: Exact Self-consistent Solutions","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"B. Saha, G. N. Shikin","submitted_at":"1996-09-24T14:07:16Z","abstract_excerpt":"Self-consistent solutions to interacting spinor and scalar field equations in General Relativity are studied for the case of Bianchi type-I space-time filled with perfect fluid. The initial and the asymptotic behavior of the field functions and the metric one has been thoroughly studied."},"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":"gr-qc/9609056","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1996-09-24T14:07:16Z","cross_cats_sorted":[],"title_canon_sha256":"30791f1b24d2e2aec1c4cdd5a11d0a6458670857b4f34f3f873b59bb38f71078","abstract_canon_sha256":"4ecf570e681d16195da08fa3bacae1c21463ecda7b6aaef632aece033a78692d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:39:19.274877Z","signature_b64":"xWjWd4kugt1uKM/99c/POvMUy3vYiYaOSmh32FyMeQGgGSIJXMLT4FxcmNpqxeMQurHi06um0kGdiA/ihep+Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2662e1d9d45b5186b1cc6c04178730f79aa371809734214693fff265228950a2","last_reissued_at":"2026-05-18T01:39:19.274404Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:39:19.274404Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interacting Spinor and Scalar Fields in Bianchi type-I Universe filled with Perfect Fluid: Exact Self-consistent Solutions","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"B. Saha, G. N. Shikin","submitted_at":"1996-09-24T14:07:16Z","abstract_excerpt":"Self-consistent solutions to interacting spinor and scalar field equations in General Relativity are studied for the case of Bianchi type-I space-time filled with perfect fluid. The initial and the asymptotic behavior of the field functions and the metric one has been thoroughly studied."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9609056","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":"gr-qc/9609056","created_at":"2026-05-18T01:39:19.274470+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9609056v2","created_at":"2026-05-18T01:39:19.274470+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9609056","created_at":"2026-05-18T01:39:19.274470+00:00"},{"alias_kind":"pith_short_12","alias_value":"EZRODWOULNIY","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_16","alias_value":"EZRODWOULNIYNMOM","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_8","alias_value":"EZRODWOU","created_at":"2026-05-18T12:25:47.700082+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/EZRODWOULNIYNMOMNQCBPBZQ66","json":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66.json","graph_json":"https://pith.science/api/pith-number/EZRODWOULNIYNMOMNQCBPBZQ66/graph.json","events_json":"https://pith.science/api/pith-number/EZRODWOULNIYNMOMNQCBPBZQ66/events.json","paper":"https://pith.science/paper/EZRODWOU"},"agent_actions":{"view_html":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66","download_json":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66.json","view_paper":"https://pith.science/paper/EZRODWOU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/9609056&json=true","fetch_graph":"https://pith.science/api/pith-number/EZRODWOULNIYNMOMNQCBPBZQ66/graph.json","fetch_events":"https://pith.science/api/pith-number/EZRODWOULNIYNMOMNQCBPBZQ66/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66/action/storage_attestation","attest_author":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66/action/author_attestation","sign_citation":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66/action/citation_signature","submit_replication":"https://pith.science/pith/EZRODWOULNIYNMOMNQCBPBZQ66/action/replication_record"}},"created_at":"2026-05-18T01:39:19.274470+00:00","updated_at":"2026-05-18T01:39:19.274470+00:00"}