{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:PFPJ2WVTZBYDBVFGE5EOZBYOQO","short_pith_number":"pith:PFPJ2WVT","schema_version":"1.0","canonical_sha256":"795e9d5ab3c87030d4a62748ec870e8382105749a5d1ac14cba0a5fb018c6e17","source":{"kind":"arxiv","id":"1710.00921","version":2},"attestation_state":"computed","paper":{"title":"Black hole scrambling from hydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","gr-qc","nlin.CD"],"primary_cat":"hep-th","authors_text":"Koenraad Schalm, Sa\\v{s}o Grozdanov, Vincenzo Scopelliti","submitted_at":"2017-10-02T21:45:47Z","abstract_excerpt":"We argue that the gravitational shock wave computation used to extract the scrambling rate in strongly coupled quantum theories with a holographic dual is directly related to probing the system's hydrodynamic sound modes. The information recovered from the shock wave can be reconstructed in terms of purely diffusion-like, linearized gravitational waves at the horizon of a single-sided black hole with specific regularity-enforced imaginary values of frequency and momentum. In two-derivative bulk theories, this horizon \"diffusion\" can be related to late-time momentum diffusion via a simple relat"},"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":"1710.00921","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-10-02T21:45:47Z","cross_cats_sorted":["cond-mat.str-el","gr-qc","nlin.CD"],"title_canon_sha256":"c712e9361ee11095c8ebae7892c836c2758c8b634837b14032caabe054bb8e58","abstract_canon_sha256":"e4bcc6aee630037263b74c1e1ac086714f944d792f22ce9c3a364126e10b11b9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:59:53.627279Z","signature_b64":"Qn5e0YZe8dWJhKd6dJJFsI+SA10VdSleG1z3ZIezCB3fU72xhQox12bfJBMS7XnPRKnmgoxgw95TbNxWwqMSCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"795e9d5ab3c87030d4a62748ec870e8382105749a5d1ac14cba0a5fb018c6e17","last_reissued_at":"2026-05-17T23:59:53.626647Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:59:53.626647Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black hole scrambling from hydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","gr-qc","nlin.CD"],"primary_cat":"hep-th","authors_text":"Koenraad Schalm, Sa\\v{s}o Grozdanov, Vincenzo Scopelliti","submitted_at":"2017-10-02T21:45:47Z","abstract_excerpt":"We argue that the gravitational shock wave computation used to extract the scrambling rate in strongly coupled quantum theories with a holographic dual is directly related to probing the system's hydrodynamic sound modes. The information recovered from the shock wave can be reconstructed in terms of purely diffusion-like, linearized gravitational waves at the horizon of a single-sided black hole with specific regularity-enforced imaginary values of frequency and momentum. In two-derivative bulk theories, this horizon \"diffusion\" can be related to late-time momentum diffusion via a simple relat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.00921","kind":"arxiv","version":2},"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":"1710.00921","created_at":"2026-05-17T23:59:53.626748+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.00921v2","created_at":"2026-05-17T23:59:53.626748+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.00921","created_at":"2026-05-17T23:59:53.626748+00:00"},{"alias_kind":"pith_short_12","alias_value":"PFPJ2WVTZBYD","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_16","alias_value":"PFPJ2WVTZBYDBVFG","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_8","alias_value":"PFPJ2WVT","created_at":"2026-05-18T12:31:37.085036+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2505.04444","citing_title":"Normal mode analysis within relativistic massive transport","ref_index":65,"is_internal_anchor":true},{"citing_arxiv_id":"2605.17840","citing_title":"Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2605.17840","citing_title":"Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12616","citing_title":"Butterflies in $\\textrm{T}\\overline{\\textrm{T}}$ deformed anomalous CFT$_2$","ref_index":53,"is_internal_anchor":true},{"citing_arxiv_id":"2603.29443","citing_title":"Cosmological brick walls & quantum chaotic dynamics of de Sitter horizons","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14638","citing_title":"Probing bulk geometry via pole skipping: from static to rotating spacetimes","ref_index":9,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO","json":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO.json","graph_json":"https://pith.science/api/pith-number/PFPJ2WVTZBYDBVFGE5EOZBYOQO/graph.json","events_json":"https://pith.science/api/pith-number/PFPJ2WVTZBYDBVFGE5EOZBYOQO/events.json","paper":"https://pith.science/paper/PFPJ2WVT"},"agent_actions":{"view_html":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO","download_json":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO.json","view_paper":"https://pith.science/paper/PFPJ2WVT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.00921&json=true","fetch_graph":"https://pith.science/api/pith-number/PFPJ2WVTZBYDBVFGE5EOZBYOQO/graph.json","fetch_events":"https://pith.science/api/pith-number/PFPJ2WVTZBYDBVFGE5EOZBYOQO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO/action/storage_attestation","attest_author":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO/action/author_attestation","sign_citation":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO/action/citation_signature","submit_replication":"https://pith.science/pith/PFPJ2WVTZBYDBVFGE5EOZBYOQO/action/replication_record"}},"created_at":"2026-05-17T23:59:53.626748+00:00","updated_at":"2026-05-17T23:59:53.626748+00:00"}