{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:R5FW6SUHFRNY67C3377ZOVFXTR","short_pith_number":"pith:R5FW6SUH","schema_version":"1.0","canonical_sha256":"8f4b6f4a872c5b8f7c5bdfff9754b79c6a455483eb48d07851179a7effba6b44","source":{"kind":"arxiv","id":"1203.5123","version":2},"attestation_state":"computed","paper":{"title":"Two binary stars gravitational waves - homotopy perturbation method","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.SR","authors_text":"M. Delshadmanesh, M. Zare, O. Jalili","submitted_at":"2012-03-22T20:51:04Z","abstract_excerpt":"Homotopy perturbation is one of the newest methods for numerical analysis of deferential equations. We have used for solving wave equation around a black hole. Our conclusions have this method far reaching consequences for comparison of theoritical physics and experimental physics."},"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":"1203.5123","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-03-22T20:51:04Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"414a73279d56317ce6693ea7a858304dcee3d07c9446b6e88db2807a6c9e1dc2","abstract_canon_sha256":"07b287a27c80bd7d7d449a7bf66d6cefc69e88e1180362b4813e6d6b67a3b37a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:04.227915Z","signature_b64":"viyh6NJEIZXNdq0c9twFxBEmIBNTjAaQtqC8iM09/ixrv1zY2fS3fJQYMnX0mZ7Int81OgG1/WF3eODJ+7tOAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8f4b6f4a872c5b8f7c5bdfff9754b79c6a455483eb48d07851179a7effba6b44","last_reissued_at":"2026-05-18T01:58:04.227488Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:04.227488Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Two binary stars gravitational waves - homotopy perturbation method","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.SR","authors_text":"M. Delshadmanesh, M. Zare, O. Jalili","submitted_at":"2012-03-22T20:51:04Z","abstract_excerpt":"Homotopy perturbation is one of the newest methods for numerical analysis of deferential equations. We have used for solving wave equation around a black hole. Our conclusions have this method far reaching consequences for comparison of theoritical physics and experimental physics."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.5123","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":"1203.5123","created_at":"2026-05-18T01:58:04.227553+00:00"},{"alias_kind":"arxiv_version","alias_value":"1203.5123v2","created_at":"2026-05-18T01:58:04.227553+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.5123","created_at":"2026-05-18T01:58:04.227553+00:00"},{"alias_kind":"pith_short_12","alias_value":"R5FW6SUHFRNY","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_16","alias_value":"R5FW6SUHFRNY67C3","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_8","alias_value":"R5FW6SUH","created_at":"2026-05-18T12:27:20.899486+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/R5FW6SUHFRNY67C3377ZOVFXTR","json":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR.json","graph_json":"https://pith.science/api/pith-number/R5FW6SUHFRNY67C3377ZOVFXTR/graph.json","events_json":"https://pith.science/api/pith-number/R5FW6SUHFRNY67C3377ZOVFXTR/events.json","paper":"https://pith.science/paper/R5FW6SUH"},"agent_actions":{"view_html":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR","download_json":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR.json","view_paper":"https://pith.science/paper/R5FW6SUH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1203.5123&json=true","fetch_graph":"https://pith.science/api/pith-number/R5FW6SUHFRNY67C3377ZOVFXTR/graph.json","fetch_events":"https://pith.science/api/pith-number/R5FW6SUHFRNY67C3377ZOVFXTR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR/action/storage_attestation","attest_author":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR/action/author_attestation","sign_citation":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR/action/citation_signature","submit_replication":"https://pith.science/pith/R5FW6SUHFRNY67C3377ZOVFXTR/action/replication_record"}},"created_at":"2026-05-18T01:58:04.227553+00:00","updated_at":"2026-05-18T01:58:04.227553+00:00"}