{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:FX4TOYCS2ZYGYMWQB5NBIT7PPU","short_pith_number":"pith:FX4TOYCS","schema_version":"1.0","canonical_sha256":"2df9376052d6706c32d00f5a144fef7d0e7944f11f4cbff30a0732db14e9df82","source":{"kind":"arxiv","id":"1912.00032","version":1},"attestation_state":"computed","paper":{"title":"Driven black holes: from Kolmogorov scaling to turbulent wakes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","physics.flu-dyn"],"primary_cat":"hep-th","authors_text":"Benjamin Withers, Christiana Pantelidou, Julian Sonner, Tomas Andrade","submitted_at":"2019-11-29T19:00:04Z","abstract_excerpt":"General relativity governs the nonlinear dynamics of spacetime, including black holes and their event horizons. We demonstrate that forced black hole horizons exhibit statistically steady turbulent spacetime dynamics consistent with Kolmogorov's theory of 1941. As a proof of principle we focus on black holes in asymptotically anti-de Sitter spacetimes in a large number of dimensions, where greater analytic control is gained. We also demonstrate that tidal deformations of the horizon induce turbulent dynamics. When set in motion relative to the horizon a deformation develops a turbulent spaceti"},"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":"1912.00032","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-11-29T19:00:04Z","cross_cats_sorted":["gr-qc","physics.flu-dyn"],"title_canon_sha256":"b4c4a8c7740567ce23626efa00eed356a3b70940f4fb5d93282b43d936549a5a","abstract_canon_sha256":"3bb9b76b8f939b0e5baebb6ad3993d276c9339346e5f4abe371eb546920815ae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:22:54.436333Z","signature_b64":"/weRjBA4Y2H8HMAXJHZVdXn1noRFiBPDM7kW2vjBgrQc3W/MwyYEJXBAbrPb5z33069j0IthC6USoT0XS+68DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2df9376052d6706c32d00f5a144fef7d0e7944f11f4cbff30a0732db14e9df82","last_reissued_at":"2026-07-05T00:22:54.435909Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:22:54.435909Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Driven black holes: from Kolmogorov scaling to turbulent wakes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","physics.flu-dyn"],"primary_cat":"hep-th","authors_text":"Benjamin Withers, Christiana Pantelidou, Julian Sonner, Tomas Andrade","submitted_at":"2019-11-29T19:00:04Z","abstract_excerpt":"General relativity governs the nonlinear dynamics of spacetime, including black holes and their event horizons. We demonstrate that forced black hole horizons exhibit statistically steady turbulent spacetime dynamics consistent with Kolmogorov's theory of 1941. As a proof of principle we focus on black holes in asymptotically anti-de Sitter spacetimes in a large number of dimensions, where greater analytic control is gained. We also demonstrate that tidal deformations of the horizon induce turbulent dynamics. When set in motion relative to the horizon a deformation develops a turbulent spaceti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.00032","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1912.00032/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":"1912.00032","created_at":"2026-07-05T00:22:54.435967+00:00"},{"alias_kind":"arxiv_version","alias_value":"1912.00032v1","created_at":"2026-07-05T00:22:54.435967+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1912.00032","created_at":"2026-07-05T00:22:54.435967+00:00"},{"alias_kind":"pith_short_12","alias_value":"FX4TOYCS2ZYG","created_at":"2026-07-05T00:22:54.435967+00:00"},{"alias_kind":"pith_short_16","alias_value":"FX4TOYCS2ZYGYMWQ","created_at":"2026-07-05T00:22:54.435967+00:00"},{"alias_kind":"pith_short_8","alias_value":"FX4TOYCS","created_at":"2026-07-05T00:22:54.435967+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.25329","citing_title":"Quantum field approach to relativistic turbulence","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2510.07467","citing_title":"Weakly turbulent saturation of the nonlinear scalar ergoregion instability","ref_index":39,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU","json":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU.json","graph_json":"https://pith.science/api/pith-number/FX4TOYCS2ZYGYMWQB5NBIT7PPU/graph.json","events_json":"https://pith.science/api/pith-number/FX4TOYCS2ZYGYMWQB5NBIT7PPU/events.json","paper":"https://pith.science/paper/FX4TOYCS"},"agent_actions":{"view_html":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU","download_json":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU.json","view_paper":"https://pith.science/paper/FX4TOYCS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1912.00032&json=true","fetch_graph":"https://pith.science/api/pith-number/FX4TOYCS2ZYGYMWQB5NBIT7PPU/graph.json","fetch_events":"https://pith.science/api/pith-number/FX4TOYCS2ZYGYMWQB5NBIT7PPU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU/action/storage_attestation","attest_author":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU/action/author_attestation","sign_citation":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU/action/citation_signature","submit_replication":"https://pith.science/pith/FX4TOYCS2ZYGYMWQB5NBIT7PPU/action/replication_record"}},"created_at":"2026-07-05T00:22:54.435967+00:00","updated_at":"2026-07-05T00:22:54.435967+00:00"}