{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:X6Z2GL4S3AKGJCY6TER4ZGX4AA","short_pith_number":"pith:X6Z2GL4S","schema_version":"1.0","canonical_sha256":"bfb3a32f92d814648b1e9923cc9afc0006613c875b461fe117b476edbe877dbc","source":{"kind":"arxiv","id":"1602.02413","version":2},"attestation_state":"computed","paper":{"title":"Black Hole Based Tests of General Relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Kent Yagi, Leo C. Stein","submitted_at":"2016-02-07T19:33:09Z","abstract_excerpt":"General relativity has passed all solar system experiments and neutron star based tests, such as binary pulsar observations, with flying colors. A more exotic arena for testing general relativity is in systems that contain one or more black holes. Black holes are the most compact objects in the universe, providing probes of the strongest-possible gravitational fields. We are motivated to study strong-field gravity since many theories give large deviations from general relativity only at large field strengths, while recovering the weak-field behavior. In this article, we review how one can prob"},"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":"1602.02413","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-02-07T19:33:09Z","cross_cats_sorted":["astro-ph.HE","hep-ph","hep-th"],"title_canon_sha256":"804f16a63e4bb835f5dccfa105de8dcf8910920aead2e8536961e260d38a1211","abstract_canon_sha256":"60332a72cb80e0b7626059eb7a0fca8b7eb86508c08a8c36c5ad826573d40aff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:20:23.888239Z","signature_b64":"/hGyExSaju0fxI8DKpVzVytNmt5nghoJAYrDgx0y/cs3uP8pe79wBOnloEyrikR/rTHPMPWsNeD2oPs8W98bCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bfb3a32f92d814648b1e9923cc9afc0006613c875b461fe117b476edbe877dbc","last_reissued_at":"2026-05-18T01:20:23.887643Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:20:23.887643Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black Hole Based Tests of General Relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Kent Yagi, Leo C. Stein","submitted_at":"2016-02-07T19:33:09Z","abstract_excerpt":"General relativity has passed all solar system experiments and neutron star based tests, such as binary pulsar observations, with flying colors. A more exotic arena for testing general relativity is in systems that contain one or more black holes. Black holes are the most compact objects in the universe, providing probes of the strongest-possible gravitational fields. We are motivated to study strong-field gravity since many theories give large deviations from general relativity only at large field strengths, while recovering the weak-field behavior. In this article, we review how one can prob"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.02413","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":"1602.02413","created_at":"2026-05-18T01:20:23.887730+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.02413v2","created_at":"2026-05-18T01:20:23.887730+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.02413","created_at":"2026-05-18T01:20:23.887730+00:00"},{"alias_kind":"pith_short_12","alias_value":"X6Z2GL4S3AKG","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"X6Z2GL4S3AKGJCY6","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"X6Z2GL4S","created_at":"2026-05-18T12:30:51.357362+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2605.19176","citing_title":"Testing Black Holes with Interstellar Missions: I. Orbiting Probes","ref_index":23,"is_internal_anchor":true},{"citing_arxiv_id":"2512.06051","citing_title":"Investigating the interplay of the braneworld gravity and the plasma environment on the black hole shadow","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"1903.04467","citing_title":"Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1","ref_index":108,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13036","citing_title":"Inspiral gravitational waveforms from charged compact binaries with scalar hair","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2604.18680","citing_title":"Beyond Three Terms: Continued Fractions for Rotating Black Holes in Modified Gravity","ref_index":12,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA","json":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA.json","graph_json":"https://pith.science/api/pith-number/X6Z2GL4S3AKGJCY6TER4ZGX4AA/graph.json","events_json":"https://pith.science/api/pith-number/X6Z2GL4S3AKGJCY6TER4ZGX4AA/events.json","paper":"https://pith.science/paper/X6Z2GL4S"},"agent_actions":{"view_html":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA","download_json":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA.json","view_paper":"https://pith.science/paper/X6Z2GL4S","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.02413&json=true","fetch_graph":"https://pith.science/api/pith-number/X6Z2GL4S3AKGJCY6TER4ZGX4AA/graph.json","fetch_events":"https://pith.science/api/pith-number/X6Z2GL4S3AKGJCY6TER4ZGX4AA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA/action/storage_attestation","attest_author":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA/action/author_attestation","sign_citation":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA/action/citation_signature","submit_replication":"https://pith.science/pith/X6Z2GL4S3AKGJCY6TER4ZGX4AA/action/replication_record"}},"created_at":"2026-05-18T01:20:23.887730+00:00","updated_at":"2026-05-18T01:20:23.887730+00:00"}