{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:WGKQSPRRIBAAYNH43M5CGH2RWH","short_pith_number":"pith:WGKQSPRR","schema_version":"1.0","canonical_sha256":"b195093e3140400c34fcdb3a231f51b1cca1404881696053672982e4aa90fac1","source":{"kind":"arxiv","id":"2305.18540","version":3},"attestation_state":"computed","paper":{"title":"Gravitational waves from binary black holes in a self-interacting scalar dark matter cloud","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Alexis Boudon, Leong Khim Wong, Patrick Valageas, Philippe Brax","submitted_at":"2023-05-29T18:14:10Z","abstract_excerpt":"We investigate the imprints of accretion and dynamical friction on the gravitational-wave signals emitted by binary black holes embedded in a scalar dark matter cloud. As a key feature in this work, we focus on scalar fields with a repulsive self-interaction that balances against the self-gravity of the cloud. To a first approximation, the phase of the gravitational-wave signal receives extra correction terms at $-3$PN, $-4$PN and $-5.5$PN orders, relative to the prediction of vacuum general relativity, due to cloud gravity, accretion and dynamical friction. Future observations by LISA and B-D"},"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":"2305.18540","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-05-29T18:14:10Z","cross_cats_sorted":["astro-ph.GA","gr-qc","hep-th"],"title_canon_sha256":"39becf1077250b1f70622de21cd5728ef7fb7d55b7027de2d185e95120632d1a","abstract_canon_sha256":"9942d5f1239a6185f9f373aac0bb0d02e90cfd49bca61a440f1ddfe48585f83a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:45:12.695375Z","signature_b64":"w5KwkAweM8m8d1ReyUvoBpvyWqL/FCChrO3tRfo4AZPEWCnFzZP4iaYQQuMAeAWKQkgiwyU0S2ElAsB1uxGBAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b195093e3140400c34fcdb3a231f51b1cca1404881696053672982e4aa90fac1","last_reissued_at":"2026-07-05T11:45:12.694870Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:45:12.694870Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational waves from binary black holes in a self-interacting scalar dark matter cloud","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"Alexis Boudon, Leong Khim Wong, Patrick Valageas, Philippe Brax","submitted_at":"2023-05-29T18:14:10Z","abstract_excerpt":"We investigate the imprints of accretion and dynamical friction on the gravitational-wave signals emitted by binary black holes embedded in a scalar dark matter cloud. As a key feature in this work, we focus on scalar fields with a repulsive self-interaction that balances against the self-gravity of the cloud. To a first approximation, the phase of the gravitational-wave signal receives extra correction terms at $-3$PN, $-4$PN and $-5.5$PN orders, relative to the prediction of vacuum general relativity, due to cloud gravity, accretion and dynamical friction. Future observations by LISA and B-D"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.18540","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2305.18540/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2305.18540","created_at":"2026-07-05T11:45:12.694934+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.18540v3","created_at":"2026-07-05T11:45:12.694934+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.18540","created_at":"2026-07-05T11:45:12.694934+00:00"},{"alias_kind":"pith_short_12","alias_value":"WGKQSPRRIBAA","created_at":"2026-07-05T11:45:12.694934+00:00"},{"alias_kind":"pith_short_16","alias_value":"WGKQSPRRIBAAYNH4","created_at":"2026-07-05T11:45:12.694934+00:00"},{"alias_kind":"pith_short_8","alias_value":"WGKQSPRR","created_at":"2026-07-05T11:45:12.694934+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.27526","citing_title":"Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework","ref_index":177,"is_internal_anchor":false},{"citing_arxiv_id":"2511.03788","citing_title":"Boson Stars Hosting Black Holes","ref_index":34,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH","json":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH.json","graph_json":"https://pith.science/api/pith-number/WGKQSPRRIBAAYNH43M5CGH2RWH/graph.json","events_json":"https://pith.science/api/pith-number/WGKQSPRRIBAAYNH43M5CGH2RWH/events.json","paper":"https://pith.science/paper/WGKQSPRR"},"agent_actions":{"view_html":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH","download_json":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH.json","view_paper":"https://pith.science/paper/WGKQSPRR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.18540&json=true","fetch_graph":"https://pith.science/api/pith-number/WGKQSPRRIBAAYNH43M5CGH2RWH/graph.json","fetch_events":"https://pith.science/api/pith-number/WGKQSPRRIBAAYNH43M5CGH2RWH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH/action/storage_attestation","attest_author":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH/action/author_attestation","sign_citation":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH/action/citation_signature","submit_replication":"https://pith.science/pith/WGKQSPRRIBAAYNH43M5CGH2RWH/action/replication_record"}},"created_at":"2026-07-05T11:45:12.694934+00:00","updated_at":"2026-07-05T11:45:12.694934+00:00"}