{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:FTEICS22N73XDNDGDONZELTFHZ","short_pith_number":"pith:FTEICS22","schema_version":"1.0","canonical_sha256":"2cc8814b5a6ff771b4661b9b922e653e67c54f750ace1993dfc6575351a40d25","source":{"kind":"arxiv","id":"hep-th/0507275","version":3},"attestation_state":"computed","paper":{"title":"A holographic perspective on Gubser-Mitra conjecture","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Alex Buchel","submitted_at":"2005-07-28T05:04:15Z","abstract_excerpt":"We point out an elementary thermodynamics fact that whenever the specific heat of a system is negative, the speed of sound in such a media is imaginary. The latter observation presents a proof of Gubser-Mitra conjecture on the relation between dynamical and thermodynamic instabilities for gravitational backgrounds with a translationary invariant horizon, provided such geometries can be interpreted as holographic duals to finite temperature gauge theories. It further identifies a tachyonic mode of the Gubser-Mitra instability (the lowest quasinormal mode of the corresponding horizon geometry) a"},"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":"hep-th/0507275","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2005-07-28T05:04:15Z","cross_cats_sorted":[],"title_canon_sha256":"8a975f8e74ffd80fea08e95db829781a28ee746324741e80aabb6010b89469d7","abstract_canon_sha256":"158540b244830b6ebd62690d9ff9e8d9c349ee2831c608b60e2b55346fa576d5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:24:46.678936Z","signature_b64":"A8P1ih09oXK48C7U/6t3Xt0YTZTuod6UpALN83t8Hg9wkYl+NTyK+ScwccDEv8M0uW1LVFF6wNHB+pmhHHRAAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2cc8814b5a6ff771b4661b9b922e653e67c54f750ace1993dfc6575351a40d25","last_reissued_at":"2026-07-04T17:24:46.678527Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:24:46.678527Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A holographic perspective on Gubser-Mitra conjecture","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Alex Buchel","submitted_at":"2005-07-28T05:04:15Z","abstract_excerpt":"We point out an elementary thermodynamics fact that whenever the specific heat of a system is negative, the speed of sound in such a media is imaginary. The latter observation presents a proof of Gubser-Mitra conjecture on the relation between dynamical and thermodynamic instabilities for gravitational backgrounds with a translationary invariant horizon, provided such geometries can be interpreted as holographic duals to finite temperature gauge theories. It further identifies a tachyonic mode of the Gubser-Mitra instability (the lowest quasinormal mode of the corresponding horizon geometry) a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0507275","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/hep-th/0507275/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":"hep-th/0507275","created_at":"2026-07-04T17:24:46.678584+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0507275v3","created_at":"2026-07-04T17:24:46.678584+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0507275","created_at":"2026-07-04T17:24:46.678584+00:00"},{"alias_kind":"pith_short_12","alias_value":"FTEICS22N73X","created_at":"2026-07-04T17:24:46.678584+00:00"},{"alias_kind":"pith_short_16","alias_value":"FTEICS22N73XDNDG","created_at":"2026-07-04T17:24:46.678584+00:00"},{"alias_kind":"pith_short_8","alias_value":"FTEICS22","created_at":"2026-07-04T17:24:46.678584+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2603.27821","citing_title":"Instability in ${\\cal N}=4$ supersymmetric Yang-Mills theory on $S^3$ at finite density","ref_index":8,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ","json":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ.json","graph_json":"https://pith.science/api/pith-number/FTEICS22N73XDNDGDONZELTFHZ/graph.json","events_json":"https://pith.science/api/pith-number/FTEICS22N73XDNDGDONZELTFHZ/events.json","paper":"https://pith.science/paper/FTEICS22"},"agent_actions":{"view_html":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ","download_json":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ.json","view_paper":"https://pith.science/paper/FTEICS22","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0507275&json=true","fetch_graph":"https://pith.science/api/pith-number/FTEICS22N73XDNDGDONZELTFHZ/graph.json","fetch_events":"https://pith.science/api/pith-number/FTEICS22N73XDNDGDONZELTFHZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ/action/storage_attestation","attest_author":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ/action/author_attestation","sign_citation":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ/action/citation_signature","submit_replication":"https://pith.science/pith/FTEICS22N73XDNDGDONZELTFHZ/action/replication_record"}},"created_at":"2026-07-04T17:24:46.678584+00:00","updated_at":"2026-07-04T17:24:46.678584+00:00"}