{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:VMQLGWBRYUAXA2GI4WSCEVISGH","short_pith_number":"pith:VMQLGWBR","schema_version":"1.0","canonical_sha256":"ab20b35831c5017068c8e5a422551231f43db5692332d71a7b73d21b95600c7f","source":{"kind":"arxiv","id":"1701.06318","version":2},"attestation_state":"computed","paper":{"title":"Testing the binary black hole nature of a compact binary coalescence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Chandra Kant Mishra, K. G. Arun, N. V. Krishnendu","submitted_at":"2017-01-23T10:20:30Z","abstract_excerpt":"We propose a novel method to test the binary black hole (BBH) nature of compact binaries detectable by gravitational wave (GW) interferometers and hence constrain the parameter space of other exotic compact objects. The spirit of the test lies in the \"no-hair\" conjecture for black holes where all properties of a black hole are characterised by the mass and the spin of the black hole. The method relies on observationally measuring the quadrupole moments of the compact binary constituents induced due to their spins. If the compact object is a Kerr black hole (BH), its quadrupole moment is expres"},"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":"1701.06318","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-01-23T10:20:30Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"c793b4ac1d7c807d9367ea2c1ab0594ca79362792fde1945357911a5f0ee3052","abstract_canon_sha256":"07ef3e2ad4dd17e67d5cd678d530ee307cb29af9873bcc9e5066b644bbd2f538"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:23.852069Z","signature_b64":"F3Kfg5XfSDhErpxLx7iv98dgX1Q9U4+Q0ejMD9XmFMtjfuOFFYy+vJIR+6iK/6rCYF3scgq36FmecdzdX8ziBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ab20b35831c5017068c8e5a422551231f43db5692332d71a7b73d21b95600c7f","last_reissued_at":"2026-05-18T00:35:23.851478Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:23.851478Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing the binary black hole nature of a compact binary coalescence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Chandra Kant Mishra, K. G. Arun, N. V. Krishnendu","submitted_at":"2017-01-23T10:20:30Z","abstract_excerpt":"We propose a novel method to test the binary black hole (BBH) nature of compact binaries detectable by gravitational wave (GW) interferometers and hence constrain the parameter space of other exotic compact objects. The spirit of the test lies in the \"no-hair\" conjecture for black holes where all properties of a black hole are characterised by the mass and the spin of the black hole. The method relies on observationally measuring the quadrupole moments of the compact binary constituents induced due to their spins. If the compact object is a Kerr black hole (BH), its quadrupole moment is expres"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.06318","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":"1701.06318","created_at":"2026-05-18T00:35:23.851571+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.06318v2","created_at":"2026-05-18T00:35:23.851571+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.06318","created_at":"2026-05-18T00:35:23.851571+00:00"},{"alias_kind":"pith_short_12","alias_value":"VMQLGWBRYUAX","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_16","alias_value":"VMQLGWBRYUAXA2GI","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_8","alias_value":"VMQLGWBR","created_at":"2026-05-18T12:31:49.984773+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":10,"internal_anchor_count":6,"sample":[{"citing_arxiv_id":"2504.07862","citing_title":"Resummation of Universal Tails in Gravitational Waveforms","ref_index":49,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19731","citing_title":"Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability","ref_index":64,"is_internal_anchor":true},{"citing_arxiv_id":"2510.22137","citing_title":"Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework","ref_index":23,"is_internal_anchor":true},{"citing_arxiv_id":"2303.15923","citing_title":"Science with the Einstein Telescope: a comparison of different designs","ref_index":203,"is_internal_anchor":true},{"citing_arxiv_id":"1912.02622","citing_title":"Science Case for the Einstein Telescope","ref_index":163,"is_internal_anchor":true},{"citing_arxiv_id":"2010.14529","citing_title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","ref_index":165,"is_internal_anchor":true},{"citing_arxiv_id":"2112.06861","citing_title":"Tests of General Relativity with GWTC-3","ref_index":222,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25582","citing_title":"Lessons from binary dynamics of inspiralling equal-mass boson-star mergers","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09828","citing_title":"Testing the Kerr hypothesis beyond the quadrupole with GW241011","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15965","citing_title":"Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH","json":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH.json","graph_json":"https://pith.science/api/pith-number/VMQLGWBRYUAXA2GI4WSCEVISGH/graph.json","events_json":"https://pith.science/api/pith-number/VMQLGWBRYUAXA2GI4WSCEVISGH/events.json","paper":"https://pith.science/paper/VMQLGWBR"},"agent_actions":{"view_html":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH","download_json":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH.json","view_paper":"https://pith.science/paper/VMQLGWBR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.06318&json=true","fetch_graph":"https://pith.science/api/pith-number/VMQLGWBRYUAXA2GI4WSCEVISGH/graph.json","fetch_events":"https://pith.science/api/pith-number/VMQLGWBRYUAXA2GI4WSCEVISGH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH/action/storage_attestation","attest_author":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH/action/author_attestation","sign_citation":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH/action/citation_signature","submit_replication":"https://pith.science/pith/VMQLGWBRYUAXA2GI4WSCEVISGH/action/replication_record"}},"created_at":"2026-05-18T00:35:23.851571+00:00","updated_at":"2026-05-18T00:35:23.851571+00:00"}