{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:R7NISQCUZOW56AY2G5TDV73IRD","short_pith_number":"pith:R7NISQCU","schema_version":"1.0","canonical_sha256":"8fda894054cbaddf031a37663aff6888eb8d903a0330e3be7b86552f4fd0d1fd","source":{"kind":"arxiv","id":"1210.3860","version":2},"attestation_state":"computed","paper":{"title":"Linearized Gravitational Waves in Nonlocal General Relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"B. Mashhoon, C. Chicone","submitted_at":"2012-10-15T00:04:53Z","abstract_excerpt":"We investigate gravitational radiation in the linear approximation within the framework of the recent nonlocal generalization of Einstein's theory of gravitation. In this theory, nonlocality can simulate dark matter; in fact, in the Newtonian regime, we recover the phenomenological Tohline-Kuhn approach to modified gravity. To account for the observational data regarding the rotation curves of spiral galaxies, nonlocality is associated with a characteristic length scale of order \\lambda_0 = 10 kpc. It follows that in nonlocal gravity, the treatment of extremely low-frequency (~ 10^{-12} Hz) 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":"1210.3860","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-10-15T00:04:53Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"802a1eba4f5eae6ed25b998014436d51d6e254801711f1b735eadd1ade347359","abstract_canon_sha256":"2b7931b1f96b9f0426fea8b4478a6241e305898b59100c870456419db79b0557"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:55.518053Z","signature_b64":"wgpi+AVLNcmQsBcjBACS+K9L1KSrSgaql/LeLokBA+hfvbrkkJY+iPgGLpNITaO2y8JJBvy6Lq5LR8o49qibAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8fda894054cbaddf031a37663aff6888eb8d903a0330e3be7b86552f4fd0d1fd","last_reissued_at":"2026-05-18T01:53:55.517349Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:55.517349Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Linearized Gravitational Waves in Nonlocal General Relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"B. Mashhoon, C. Chicone","submitted_at":"2012-10-15T00:04:53Z","abstract_excerpt":"We investigate gravitational radiation in the linear approximation within the framework of the recent nonlocal generalization of Einstein's theory of gravitation. In this theory, nonlocality can simulate dark matter; in fact, in the Newtonian regime, we recover the phenomenological Tohline-Kuhn approach to modified gravity. To account for the observational data regarding the rotation curves of spiral galaxies, nonlocality is associated with a characteristic length scale of order \\lambda_0 = 10 kpc. It follows that in nonlocal gravity, the treatment of extremely low-frequency (~ 10^{-12} Hz) gr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.3860","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":"1210.3860","created_at":"2026-05-18T01:53:55.517466+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.3860v2","created_at":"2026-05-18T01:53:55.517466+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.3860","created_at":"2026-05-18T01:53:55.517466+00:00"},{"alias_kind":"pith_short_12","alias_value":"R7NISQCUZOW5","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_16","alias_value":"R7NISQCUZOW56AY2","created_at":"2026-05-18T12:27:20.899486+00:00"},{"alias_kind":"pith_short_8","alias_value":"R7NISQCU","created_at":"2026-05-18T12:27:20.899486+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.25254","citing_title":"The properties and predictions of quasi-periodic oscillations around a black hole in nonlocal gravity","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD","json":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD.json","graph_json":"https://pith.science/api/pith-number/R7NISQCUZOW56AY2G5TDV73IRD/graph.json","events_json":"https://pith.science/api/pith-number/R7NISQCUZOW56AY2G5TDV73IRD/events.json","paper":"https://pith.science/paper/R7NISQCU"},"agent_actions":{"view_html":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD","download_json":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD.json","view_paper":"https://pith.science/paper/R7NISQCU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.3860&json=true","fetch_graph":"https://pith.science/api/pith-number/R7NISQCUZOW56AY2G5TDV73IRD/graph.json","fetch_events":"https://pith.science/api/pith-number/R7NISQCUZOW56AY2G5TDV73IRD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD/action/storage_attestation","attest_author":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD/action/author_attestation","sign_citation":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD/action/citation_signature","submit_replication":"https://pith.science/pith/R7NISQCUZOW56AY2G5TDV73IRD/action/replication_record"}},"created_at":"2026-05-18T01:53:55.517466+00:00","updated_at":"2026-05-18T01:53:55.517466+00:00"}