{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:2CSHFACXRSBEVX5P6F3NYH5P3B","short_pith_number":"pith:2CSHFACX","schema_version":"1.0","canonical_sha256":"d0a47280578c824adfaff176dc1fafd863b0a667a7b286f076bf9add4d3b84e2","source":{"kind":"arxiv","id":"1508.01735","version":2},"attestation_state":"computed","paper":{"title":"Holographic Interpretation of Acoustic Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jia-Rui Sun, Xian-Hui Ge, Xiao-Ning Wu, Yun-Long Zhang, Yu Tian","submitted_at":"2015-08-07T15:56:55Z","abstract_excerpt":"With the attempt to find the holographic description of usual acoustic black holes in fluid, we construct an acoustic black hole formed in the $d$-dimensional fluid located at the timelike cutoff surface of a neutral black brane in asymptotically AdS$_{d+1}$ spacetime, the bulk gravitational dual of the acoustic black hole is presented at first order of the hydrodynamic fluctuation. Moreover, the Hawking-like temperature of the acoustic black hole horizon is showed to be connected to the Hawking temperature of the real AdS black brane in the bulk, and the duality between the phonon scattering "},"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":"1508.01735","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2015-08-07T15:56:55Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"db55190b718e019b4ab423bee1926efb56cfd3e143ae4f5b67cbae82b0f1ba06","abstract_canon_sha256":"32d5420867e67942347fe673ee85dd20fb9f5ccbec3c8063faf0604609fb4cfa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:28:03.710297Z","signature_b64":"6ycO3z3FKN7Uc+xucvsKNh5v2Wo/qExyQNd1XvSOvwNqe+zBMlDhWXFwHxqoqiEClNTGuBWNEyYhdh6EgGI0Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0a47280578c824adfaff176dc1fafd863b0a667a7b286f076bf9add4d3b84e2","last_reissued_at":"2026-05-18T01:28:03.709632Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:28:03.709632Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holographic Interpretation of Acoustic Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jia-Rui Sun, Xian-Hui Ge, Xiao-Ning Wu, Yun-Long Zhang, Yu Tian","submitted_at":"2015-08-07T15:56:55Z","abstract_excerpt":"With the attempt to find the holographic description of usual acoustic black holes in fluid, we construct an acoustic black hole formed in the $d$-dimensional fluid located at the timelike cutoff surface of a neutral black brane in asymptotically AdS$_{d+1}$ spacetime, the bulk gravitational dual of the acoustic black hole is presented at first order of the hydrodynamic fluctuation. Moreover, the Hawking-like temperature of the acoustic black hole horizon is showed to be connected to the Hawking temperature of the real AdS black brane in the bulk, and the duality between the phonon scattering "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.01735","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":"1508.01735","created_at":"2026-05-18T01:28:03.709740+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.01735v2","created_at":"2026-05-18T01:28:03.709740+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.01735","created_at":"2026-05-18T01:28:03.709740+00:00"},{"alias_kind":"pith_short_12","alias_value":"2CSHFACXRSBE","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_16","alias_value":"2CSHFACXRSBEVX5P","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_8","alias_value":"2CSHFACX","created_at":"2026-05-18T12:28:59.999130+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"1906.11707","citing_title":"Classical limit for Dirac fermions with modified action in the presence of the black hole","ref_index":34,"is_internal_anchor":true},{"citing_arxiv_id":"2512.23305","citing_title":"Bosonic and Fermionic love number of static acoustic black hole","ref_index":28,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B","json":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B.json","graph_json":"https://pith.science/api/pith-number/2CSHFACXRSBEVX5P6F3NYH5P3B/graph.json","events_json":"https://pith.science/api/pith-number/2CSHFACXRSBEVX5P6F3NYH5P3B/events.json","paper":"https://pith.science/paper/2CSHFACX"},"agent_actions":{"view_html":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B","download_json":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B.json","view_paper":"https://pith.science/paper/2CSHFACX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.01735&json=true","fetch_graph":"https://pith.science/api/pith-number/2CSHFACXRSBEVX5P6F3NYH5P3B/graph.json","fetch_events":"https://pith.science/api/pith-number/2CSHFACXRSBEVX5P6F3NYH5P3B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B/action/storage_attestation","attest_author":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B/action/author_attestation","sign_citation":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B/action/citation_signature","submit_replication":"https://pith.science/pith/2CSHFACXRSBEVX5P6F3NYH5P3B/action/replication_record"}},"created_at":"2026-05-18T01:28:03.709740+00:00","updated_at":"2026-05-18T01:28:03.709740+00:00"}