{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:OOAZF2FHY7QTHOLCSSQMO27UIB","short_pith_number":"pith:OOAZF2FH","schema_version":"1.0","canonical_sha256":"738192e8a7c7e133b96294a0c76bf4405d78d9322eba63037a994a65f4cbc02e","source":{"kind":"arxiv","id":"1408.2589","version":1},"attestation_state":"computed","paper":{"title":"Wiggly tails: a gravitational wave signature of massive fields around black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Carlos A. R. Herdeiro, Juan Carlos Degollado","submitted_at":"2014-08-12T00:29:43Z","abstract_excerpt":"Massive fields can exist in long-lived configurations around black holes. We examine how the gravitational wave signal of a perturbed black hole is affected by such `dirtiness' within linear theory. As a concrete example, we consider the gravitational radiation emitted by the infall of a massive scalar field into a Schwarzschild black hole. Whereas part of the scalar field is absorbed/scattered by the black hole and triggers gravitational wave emission, another part lingers in long-lived quasi-bound states. Solving numerically the Teukolsky master equation for gravitational perturbations coupl"},"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":"1408.2589","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-08-12T00:29:43Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"65cc98c387a34f4e47fb60f782f669b180a1323405bb988396917c61a4a39276","abstract_canon_sha256":"f77e908c59a97e93cfba94b6c7c37586dfaaa4a4141d2e3b4db21589fcff7f9f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:42:07.513876Z","signature_b64":"GFD7YvVRpQHubcjZ3ZktRCxU7je0hUKljtko1b9cE18NhFQw3vg+XKxf42MYapQBLIW/j7k5SHLP118O7LZcCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"738192e8a7c7e133b96294a0c76bf4405d78d9322eba63037a994a65f4cbc02e","last_reissued_at":"2026-05-18T02:42:07.513429Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:42:07.513429Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wiggly tails: a gravitational wave signature of massive fields around black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Carlos A. R. Herdeiro, Juan Carlos Degollado","submitted_at":"2014-08-12T00:29:43Z","abstract_excerpt":"Massive fields can exist in long-lived configurations around black holes. We examine how the gravitational wave signal of a perturbed black hole is affected by such `dirtiness' within linear theory. As a concrete example, we consider the gravitational radiation emitted by the infall of a massive scalar field into a Schwarzschild black hole. Whereas part of the scalar field is absorbed/scattered by the black hole and triggers gravitational wave emission, another part lingers in long-lived quasi-bound states. Solving numerically the Teukolsky master equation for gravitational perturbations coupl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.2589","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":"1408.2589","created_at":"2026-05-18T02:42:07.513490+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.2589v1","created_at":"2026-05-18T02:42:07.513490+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.2589","created_at":"2026-05-18T02:42:07.513490+00:00"},{"alias_kind":"pith_short_12","alias_value":"OOAZF2FHY7QT","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"OOAZF2FHY7QTHOLC","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"OOAZF2FH","created_at":"2026-05-18T12:28:41.024544+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB","json":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB.json","graph_json":"https://pith.science/api/pith-number/OOAZF2FHY7QTHOLCSSQMO27UIB/graph.json","events_json":"https://pith.science/api/pith-number/OOAZF2FHY7QTHOLCSSQMO27UIB/events.json","paper":"https://pith.science/paper/OOAZF2FH"},"agent_actions":{"view_html":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB","download_json":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB.json","view_paper":"https://pith.science/paper/OOAZF2FH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.2589&json=true","fetch_graph":"https://pith.science/api/pith-number/OOAZF2FHY7QTHOLCSSQMO27UIB/graph.json","fetch_events":"https://pith.science/api/pith-number/OOAZF2FHY7QTHOLCSSQMO27UIB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB/action/storage_attestation","attest_author":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB/action/author_attestation","sign_citation":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB/action/citation_signature","submit_replication":"https://pith.science/pith/OOAZF2FHY7QTHOLCSSQMO27UIB/action/replication_record"}},"created_at":"2026-05-18T02:42:07.513490+00:00","updated_at":"2026-05-18T02:42:07.513490+00:00"}