{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:G5U72SHHUJYGWKXLVIKPL524QY","short_pith_number":"pith:G5U72SHH","schema_version":"1.0","canonical_sha256":"3769fd48e7a2706b2aebaa14f5f75c86112533e982e82e6db5314efa9ff3bccf","source":{"kind":"arxiv","id":"2111.04091","version":2},"attestation_state":"computed","paper":{"title":"Compactified AdS black holes, Chamblin-Reall background, and their dual non-conformal relativistic fluids","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Chao Wu, Yanqi Wang","submitted_at":"2021-11-07T13:50:02Z","abstract_excerpt":"The Chamblin-Reall background is a static solution of Einstein gravity coupled with a background scalar field and a dynamical domain wall, with the potential of the scalar field being of Liouville type. It can be got by dimensionally reducing a higher dimensional background with a constant potential. Compactified AdS black holes are black hole backgrounds constructed by wrapping one or more spatial directions of a higher dimensional AdS black hole on a torus and then integrating them out. The compactified AdS black hole background is asymptotically flat, non-conformal, and of Chamblin-Reall ty"},"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":"2111.04091","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2021-11-07T13:50:02Z","cross_cats_sorted":[],"title_canon_sha256":"3c9f6b26b402b65e26781e608d04bc4e30320cf07b5c6421a9b0c5c9b48c78ef","abstract_canon_sha256":"23a16cb6ed269c92272e3c20e78b4523cdc3f54dfe2ae3d78d964285b8d83cf4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:02:58.709826Z","signature_b64":"uaaw4efimlgpm41p/EVu9f6IVnkbF/3c47sMT0FdyOYQjCxsOLEsmfXUMMGjD67Iwww5t1caPiBEEIMDIu1IDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3769fd48e7a2706b2aebaa14f5f75c86112533e982e82e6db5314efa9ff3bccf","last_reissued_at":"2026-07-05T04:02:58.709227Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:02:58.709227Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Compactified AdS black holes, Chamblin-Reall background, and their dual non-conformal relativistic fluids","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Chao Wu, Yanqi Wang","submitted_at":"2021-11-07T13:50:02Z","abstract_excerpt":"The Chamblin-Reall background is a static solution of Einstein gravity coupled with a background scalar field and a dynamical domain wall, with the potential of the scalar field being of Liouville type. It can be got by dimensionally reducing a higher dimensional background with a constant potential. Compactified AdS black holes are black hole backgrounds constructed by wrapping one or more spatial directions of a higher dimensional AdS black hole on a torus and then integrating them out. The compactified AdS black hole background is asymptotically flat, non-conformal, and of Chamblin-Reall ty"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2111.04091","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2111.04091/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":"2111.04091","created_at":"2026-07-05T04:02:58.709288+00:00"},{"alias_kind":"arxiv_version","alias_value":"2111.04091v2","created_at":"2026-07-05T04:02:58.709288+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2111.04091","created_at":"2026-07-05T04:02:58.709288+00:00"},{"alias_kind":"pith_short_12","alias_value":"G5U72SHHUJYG","created_at":"2026-07-05T04:02:58.709288+00:00"},{"alias_kind":"pith_short_16","alias_value":"G5U72SHHUJYGWKXL","created_at":"2026-07-05T04:02:58.709288+00:00"},{"alias_kind":"pith_short_8","alias_value":"G5U72SHH","created_at":"2026-07-05T04:02:58.709288+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.01146","citing_title":"Forced non-conformal relativistic fluid from the Chamblin-Reall gravity","ref_index":1,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY","json":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY.json","graph_json":"https://pith.science/api/pith-number/G5U72SHHUJYGWKXLVIKPL524QY/graph.json","events_json":"https://pith.science/api/pith-number/G5U72SHHUJYGWKXLVIKPL524QY/events.json","paper":"https://pith.science/paper/G5U72SHH"},"agent_actions":{"view_html":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY","download_json":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY.json","view_paper":"https://pith.science/paper/G5U72SHH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2111.04091&json=true","fetch_graph":"https://pith.science/api/pith-number/G5U72SHHUJYGWKXLVIKPL524QY/graph.json","fetch_events":"https://pith.science/api/pith-number/G5U72SHHUJYGWKXLVIKPL524QY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY/action/storage_attestation","attest_author":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY/action/author_attestation","sign_citation":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY/action/citation_signature","submit_replication":"https://pith.science/pith/G5U72SHHUJYGWKXLVIKPL524QY/action/replication_record"}},"created_at":"2026-07-05T04:02:58.709288+00:00","updated_at":"2026-07-05T04:02:58.709288+00:00"}