{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:IWGRN67CSJR7YXGZAN4LPTO4UW","short_pith_number":"pith:IWGRN67C","schema_version":"1.0","canonical_sha256":"458d16fbe29263fc5cd90378b7cddca5b22a8ce9dc79a9a8a3dd79c51d5461b7","source":{"kind":"arxiv","id":"2410.00968","version":3},"attestation_state":"computed","paper":{"title":"Tidal Love numbers of gravitational atoms","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Gon\\c{c}alo Castro, Ricardo Arana, Richard Brito","submitted_at":"2024-10-01T18:00:05Z","abstract_excerpt":"Ultralight bosonic fields can form condensates, or clouds, around spinning black holes. When this system is under the influence of a secondary massive body, its tidal response can be quantified in the tidal Love numbers (TLNs). Although TLNs vanish for black holes in vacuum, it has been shown that the same is not true for black holes immersed in matter environments. In this work, we compute the gravitational TLNs of black holes surrounded by scalar clouds, in the Newtonian limit. We show that they are non-vanishing, have a strong power-law dependence on the boson's mass, and are proportional t"},"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":"2410.00968","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-10-01T18:00:05Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"3bb456a61d5ea5bf98c982be8be66e030668ce21f13df34b1ce1514d40470950","abstract_canon_sha256":"0a62f6d0288dfe53192e6db76c633e4a8a16c08360bd21dfa09a8afa499f67bb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:12:20.692070Z","signature_b64":"EoZ05lQ2FVQH19Ytc+SxbAjV+yizyzsQRbdENmWoZNCAcjUwE8Se8HQc1E7p3jdgPvav9ennNvRF1cWXSfYSCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"458d16fbe29263fc5cd90378b7cddca5b22a8ce9dc79a9a8a3dd79c51d5461b7","last_reissued_at":"2026-07-05T10:12:20.691556Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:12:20.691556Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tidal Love numbers of gravitational atoms","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"gr-qc","authors_text":"Gon\\c{c}alo Castro, Ricardo Arana, Richard Brito","submitted_at":"2024-10-01T18:00:05Z","abstract_excerpt":"Ultralight bosonic fields can form condensates, or clouds, around spinning black holes. When this system is under the influence of a secondary massive body, its tidal response can be quantified in the tidal Love numbers (TLNs). Although TLNs vanish for black holes in vacuum, it has been shown that the same is not true for black holes immersed in matter environments. In this work, we compute the gravitational TLNs of black holes surrounded by scalar clouds, in the Newtonian limit. We show that they are non-vanishing, have a strong power-law dependence on the boson's mass, and are proportional t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.00968","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/2410.00968/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":"2410.00968","created_at":"2026-07-05T10:12:20.691617+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.00968v3","created_at":"2026-07-05T10:12:20.691617+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.00968","created_at":"2026-07-05T10:12:20.691617+00:00"},{"alias_kind":"pith_short_12","alias_value":"IWGRN67CSJR7","created_at":"2026-07-05T10:12:20.691617+00:00"},{"alias_kind":"pith_short_16","alias_value":"IWGRN67CSJR7YXGZ","created_at":"2026-07-05T10:12:20.691617+00:00"},{"alias_kind":"pith_short_8","alias_value":"IWGRN67C","created_at":"2026-07-05T10:12:20.691617+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.21439","citing_title":"Relativistic effects in extreme-mass-ratio inspirals within scalar clouds: Eccentric and inclined orbits","ref_index":99,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW","json":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW.json","graph_json":"https://pith.science/api/pith-number/IWGRN67CSJR7YXGZAN4LPTO4UW/graph.json","events_json":"https://pith.science/api/pith-number/IWGRN67CSJR7YXGZAN4LPTO4UW/events.json","paper":"https://pith.science/paper/IWGRN67C"},"agent_actions":{"view_html":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW","download_json":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW.json","view_paper":"https://pith.science/paper/IWGRN67C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.00968&json=true","fetch_graph":"https://pith.science/api/pith-number/IWGRN67CSJR7YXGZAN4LPTO4UW/graph.json","fetch_events":"https://pith.science/api/pith-number/IWGRN67CSJR7YXGZAN4LPTO4UW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW/action/storage_attestation","attest_author":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW/action/author_attestation","sign_citation":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW/action/citation_signature","submit_replication":"https://pith.science/pith/IWGRN67CSJR7YXGZAN4LPTO4UW/action/replication_record"}},"created_at":"2026-07-05T10:12:20.691617+00:00","updated_at":"2026-07-05T10:12:20.691617+00:00"}