{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:Q6EEZLNIS26WW7HXSOKGH4XGDF","short_pith_number":"pith:Q6EEZLNI","schema_version":"1.0","canonical_sha256":"87884cada896bd6b7cf7939463f2e619731b22246d2986dca7f39493d9db56b5","source":{"kind":"arxiv","id":"2303.15921","version":3},"attestation_state":"computed","paper":{"title":"Pole-skipping of gravitational waves in the backgrounds of four-dimensional massive black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","math-ph","math.MP"],"primary_cat":"hep-th","authors_text":"Mile Vrbica, Sa\\v{s}o Grozdanov","submitted_at":"2023-03-28T12:26:40Z","abstract_excerpt":"Pole-skipping is a property of gravitational waves dictated by their behaviour at horizons of black holes. It stems from the inability to unambiguously impose ingoing boundary conditions at the horizon at an infinite discrete set of Fourier modes. The phenomenon has been best understood, when such a description exists, in terms of dual holographic (AdS/CFT) correlation function that take the value of '0/0' at these special points. In this work, we investigate details of pole-skipping purely from the point of view of classical gravity in 4d massive black hole geometries with flat, spherical and"},"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":"2303.15921","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2023-03-28T12:26:40Z","cross_cats_sorted":["gr-qc","math-ph","math.MP"],"title_canon_sha256":"131a8d555496ffffb0b4f3b2df577577ae815c15715bb29def33705742c2aa00","abstract_canon_sha256":"a292356e4dbcef6c2c9f2dc90bb3711b01bf99945585f5d1f334729fd8ab362f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:41:37.110259Z","signature_b64":"N488LIHVT/gHIxupaQ2qX7L4XEwudVfvhRBsdGGwniYh3C6bYasosxBUZHuIcUDrtwLGp/r3R6VhW63rogKvAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"87884cada896bd6b7cf7939463f2e619731b22246d2986dca7f39493d9db56b5","last_reissued_at":"2026-07-05T08:41:37.109686Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:41:37.109686Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pole-skipping of gravitational waves in the backgrounds of four-dimensional massive black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","math-ph","math.MP"],"primary_cat":"hep-th","authors_text":"Mile Vrbica, Sa\\v{s}o Grozdanov","submitted_at":"2023-03-28T12:26:40Z","abstract_excerpt":"Pole-skipping is a property of gravitational waves dictated by their behaviour at horizons of black holes. It stems from the inability to unambiguously impose ingoing boundary conditions at the horizon at an infinite discrete set of Fourier modes. The phenomenon has been best understood, when such a description exists, in terms of dual holographic (AdS/CFT) correlation function that take the value of '0/0' at these special points. In this work, we investigate details of pole-skipping purely from the point of view of classical gravity in 4d massive black hole geometries with flat, spherical and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.15921","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/2303.15921/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":"2303.15921","created_at":"2026-07-05T08:41:37.109745+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.15921v3","created_at":"2026-07-05T08:41:37.109745+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.15921","created_at":"2026-07-05T08:41:37.109745+00:00"},{"alias_kind":"pith_short_12","alias_value":"Q6EEZLNIS26W","created_at":"2026-07-05T08:41:37.109745+00:00"},{"alias_kind":"pith_short_16","alias_value":"Q6EEZLNIS26WW7HX","created_at":"2026-07-05T08:41:37.109745+00:00"},{"alias_kind":"pith_short_8","alias_value":"Q6EEZLNI","created_at":"2026-07-05T08:41:37.109745+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.11297","citing_title":"Bouncing Geodesics, Singularities, and the Cavity Thermal Product Formula in Asymptotically Flat and de Sitter Black Holes","ref_index":70,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17840","citing_title":"Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17840","citing_title":"Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14638","citing_title":"Probing bulk geometry via pole skipping: from static to rotating spacetimes","ref_index":115,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF","json":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF.json","graph_json":"https://pith.science/api/pith-number/Q6EEZLNIS26WW7HXSOKGH4XGDF/graph.json","events_json":"https://pith.science/api/pith-number/Q6EEZLNIS26WW7HXSOKGH4XGDF/events.json","paper":"https://pith.science/paper/Q6EEZLNI"},"agent_actions":{"view_html":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF","download_json":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF.json","view_paper":"https://pith.science/paper/Q6EEZLNI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.15921&json=true","fetch_graph":"https://pith.science/api/pith-number/Q6EEZLNIS26WW7HXSOKGH4XGDF/graph.json","fetch_events":"https://pith.science/api/pith-number/Q6EEZLNIS26WW7HXSOKGH4XGDF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF/action/storage_attestation","attest_author":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF/action/author_attestation","sign_citation":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF/action/citation_signature","submit_replication":"https://pith.science/pith/Q6EEZLNIS26WW7HXSOKGH4XGDF/action/replication_record"}},"created_at":"2026-07-05T08:41:37.109745+00:00","updated_at":"2026-07-05T08:41:37.109745+00:00"}