{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:M7ULSN3GIVFFECL7DU46NMKMHL","short_pith_number":"pith:M7ULSN3G","schema_version":"1.0","canonical_sha256":"67e8b93766454a52097f1d39e6b14c3af292a8040729e6951a6e4db142881d93","source":{"kind":"arxiv","id":"1411.0686","version":1},"attestation_state":"computed","paper":{"title":"Black holes as particle detectors: evolution of superradiant instabilities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Paolo Pani, Richard Brito, Vitor Cardoso","submitted_at":"2014-11-03T21:00:29Z","abstract_excerpt":"Superradiant instabilities of spinning black holes can be used to impose strong constraints on ultralight bosons, thus turning black holes into effective particle detectors. However, very little is known about the development of the instability and whether its nonlinear time evolution accords to the linear intuition. For the first time, we attack this problem by studying the impact of gravitational-wave emission and gas accretion on the evolution of the instability. Our quasi-adiabatic, fully-relativistic analysis shows that: (i) gravitational-wave emission does not have a significant effect o"},"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":"1411.0686","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-11-03T21:00:29Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"0c650150ee87bdb8d5c187ccdb6c8a0256b72b0b05d940ec3335792dd4917406","abstract_canon_sha256":"313f17832fce861a56dd8af689a204bde07a2db14b371af6f395d8dbba692c5e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:22.261181Z","signature_b64":"1Ixv+s883M/dSVJFqJM4taH3Zyq3qdllRiFQa199zmp/moviSYpwvuSgeodlb809bnUXvjwONacxr+KZDydADA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"67e8b93766454a52097f1d39e6b14c3af292a8040729e6951a6e4db142881d93","last_reissued_at":"2026-05-18T01:46:22.260640Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:22.260640Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black holes as particle detectors: evolution of superradiant instabilities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Paolo Pani, Richard Brito, Vitor Cardoso","submitted_at":"2014-11-03T21:00:29Z","abstract_excerpt":"Superradiant instabilities of spinning black holes can be used to impose strong constraints on ultralight bosons, thus turning black holes into effective particle detectors. However, very little is known about the development of the instability and whether its nonlinear time evolution accords to the linear intuition. For the first time, we attack this problem by studying the impact of gravitational-wave emission and gas accretion on the evolution of the instability. Our quasi-adiabatic, fully-relativistic analysis shows that: (i) gravitational-wave emission does not have a significant effect o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.0686","kind":"arxiv","version":1},"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":"1411.0686","created_at":"2026-05-18T01:46:22.260721+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.0686v1","created_at":"2026-05-18T01:46:22.260721+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.0686","created_at":"2026-05-18T01:46:22.260721+00:00"},{"alias_kind":"pith_short_12","alias_value":"M7ULSN3GIVFF","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_16","alias_value":"M7ULSN3GIVFFECL7","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_8","alias_value":"M7ULSN3G","created_at":"2026-05-18T12:28:38.356838+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":9,"sample":[{"citing_arxiv_id":"2606.24642","citing_title":"When Black Holes Can Wear Pants","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2606.21439","citing_title":"Relativistic effects in extreme-mass-ratio inspirals within scalar clouds: Eccentric and inclined orbits","ref_index":41,"is_internal_anchor":true},{"citing_arxiv_id":"2606.20524","citing_title":"String Axiverse Enhancement of Superradiant Dark Matter Production","ref_index":45,"is_internal_anchor":true},{"citing_arxiv_id":"2605.14797","citing_title":"How Much Can Gravitons Be Squeezed?","ref_index":33,"is_internal_anchor":true},{"citing_arxiv_id":"2508.09965","citing_title":"GW231123: A Possible Primordial Black Hole Origin","ref_index":80,"is_internal_anchor":true},{"citing_arxiv_id":"2509.03568","citing_title":"Probing dense environments around Sgr A* with S-stars dynamics","ref_index":30,"is_internal_anchor":true},{"citing_arxiv_id":"2511.10307","citing_title":"Gravitational Atoms from Topological Stars","ref_index":67,"is_internal_anchor":true},{"citing_arxiv_id":"1501.06570","citing_title":"Superradiance -- the 2020 Edition","ref_index":114,"is_internal_anchor":true},{"citing_arxiv_id":"1912.02622","citing_title":"Science Case for the Einstein Telescope","ref_index":182,"is_internal_anchor":true},{"citing_arxiv_id":"2604.21239","citing_title":"Relativistic frequency shifts in gravitational waves from axion clouds","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11893","citing_title":"Relativistic signatures of scalar dark matter in extreme-mass-ratio inspirals","ref_index":72,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08053","citing_title":"Constraining Ultralight Scalar Dark Matter in the Galactic Center with the S2 Orbit","ref_index":46,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL","json":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL.json","graph_json":"https://pith.science/api/pith-number/M7ULSN3GIVFFECL7DU46NMKMHL/graph.json","events_json":"https://pith.science/api/pith-number/M7ULSN3GIVFFECL7DU46NMKMHL/events.json","paper":"https://pith.science/paper/M7ULSN3G"},"agent_actions":{"view_html":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL","download_json":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL.json","view_paper":"https://pith.science/paper/M7ULSN3G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.0686&json=true","fetch_graph":"https://pith.science/api/pith-number/M7ULSN3GIVFFECL7DU46NMKMHL/graph.json","fetch_events":"https://pith.science/api/pith-number/M7ULSN3GIVFFECL7DU46NMKMHL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL/action/storage_attestation","attest_author":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL/action/author_attestation","sign_citation":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL/action/citation_signature","submit_replication":"https://pith.science/pith/M7ULSN3GIVFFECL7DU46NMKMHL/action/replication_record"}},"created_at":"2026-05-18T01:46:22.260721+00:00","updated_at":"2026-05-18T01:46:22.260721+00:00"}