{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:LTKP2EODYIMQNI4VBGFAXVRGKH","short_pith_number":"pith:LTKP2EOD","schema_version":"1.0","canonical_sha256":"5cd4fd11c3c21906a395098a0bd62651eafc1f93ca4da0c8e41fa3a5702ee845","source":{"kind":"arxiv","id":"2408.08349","version":3},"attestation_state":"computed","paper":{"title":"Self-interacting axion clouds around rotating black holes in binary systems","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"Hidetoshi Omiya, Takahiro Tanaka, Takuya Takahashi","submitted_at":"2024-08-15T18:00:01Z","abstract_excerpt":"Superradiant instability can form clouds around rotating black holes (BHs) composed of ultralight bosonic fields, such as axions. A BH with such a cloud in a binary system exhibits rich phenomena, and gravitational waves (GWs) from the BH merger provide a means to probe axions. For the first time, we study the evolution of axion clouds in a binary system during the inspiral phase, including axion self-interaction effects. When the self-interaction is significant, unlike in the negligible case, two types of clouds coexist through mode coupling. We examine the evolution of the system considering"},"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":"2408.08349","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-08-15T18:00:01Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"46e41e5adc1924c3a70593d743b3cc915f0186b0f0b48d034329bb1bc29d292c","abstract_canon_sha256":"7715db6dd021a66a46c657d39f427dbfe6bfd8de84d66ad323bbb592d1c77176"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:45:52.640933Z","signature_b64":"yG478/WGBwTmbHTjx+kGh8/v4LZtfCsBKp/DiIWHCNdCHd3uN8DBcHIu09fKXGpbJJTmxar2YJ24EpiU+95xDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5cd4fd11c3c21906a395098a0bd62651eafc1f93ca4da0c8e41fa3a5702ee845","last_reissued_at":"2026-07-05T09:45:52.640522Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:45:52.640522Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Self-interacting axion clouds around rotating black holes in binary systems","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"Hidetoshi Omiya, Takahiro Tanaka, Takuya Takahashi","submitted_at":"2024-08-15T18:00:01Z","abstract_excerpt":"Superradiant instability can form clouds around rotating black holes (BHs) composed of ultralight bosonic fields, such as axions. A BH with such a cloud in a binary system exhibits rich phenomena, and gravitational waves (GWs) from the BH merger provide a means to probe axions. For the first time, we study the evolution of axion clouds in a binary system during the inspiral phase, including axion self-interaction effects. When the self-interaction is significant, unlike in the negligible case, two types of clouds coexist through mode coupling. We examine the evolution of the system considering"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.08349","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/2408.08349/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":"2408.08349","created_at":"2026-07-05T09:45:52.640577+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.08349v3","created_at":"2026-07-05T09:45:52.640577+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.08349","created_at":"2026-07-05T09:45:52.640577+00:00"},{"alias_kind":"pith_short_12","alias_value":"LTKP2EODYIMQ","created_at":"2026-07-05T09:45:52.640577+00:00"},{"alias_kind":"pith_short_16","alias_value":"LTKP2EODYIMQNI4V","created_at":"2026-07-05T09:45:52.640577+00:00"},{"alias_kind":"pith_short_8","alias_value":"LTKP2EOD","created_at":"2026-07-05T09:45:52.640577+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.10776","citing_title":"Gravitational superfluorescence from superradiant axion clouds","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"2409.14946","citing_title":"Black Hole Solutions with Electric and Magnetic Charges in Nonlinear Electrodynamic","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2509.03568","citing_title":"Probing dense environments around Sgr A* with S-stars dynamics","ref_index":63,"is_internal_anchor":false},{"citing_arxiv_id":"2511.03788","citing_title":"Boson Stars Hosting Black Holes","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2511.16244","citing_title":"Constraining interacting dark energy models with black hole superradiance","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2512.13816","citing_title":"Stellar Superradiance and Low-Energy Absorption in Dense Nuclear Media","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2604.21239","citing_title":"Relativistic frequency shifts in gravitational waves from axion clouds","ref_index":42,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH","json":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH.json","graph_json":"https://pith.science/api/pith-number/LTKP2EODYIMQNI4VBGFAXVRGKH/graph.json","events_json":"https://pith.science/api/pith-number/LTKP2EODYIMQNI4VBGFAXVRGKH/events.json","paper":"https://pith.science/paper/LTKP2EOD"},"agent_actions":{"view_html":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH","download_json":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH.json","view_paper":"https://pith.science/paper/LTKP2EOD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.08349&json=true","fetch_graph":"https://pith.science/api/pith-number/LTKP2EODYIMQNI4VBGFAXVRGKH/graph.json","fetch_events":"https://pith.science/api/pith-number/LTKP2EODYIMQNI4VBGFAXVRGKH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH/action/storage_attestation","attest_author":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH/action/author_attestation","sign_citation":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH/action/citation_signature","submit_replication":"https://pith.science/pith/LTKP2EODYIMQNI4VBGFAXVRGKH/action/replication_record"}},"created_at":"2026-07-05T09:45:52.640577+00:00","updated_at":"2026-07-05T09:45:52.640577+00:00"}