{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:PTPBTQ77ASWRUWIJJQZWLVX2N5","short_pith_number":"pith:PTPBTQ77","schema_version":"1.0","canonical_sha256":"7cde19c3ff04ad1a59094c3365d6fa6f60d801e0efed6620bde94b8255f8a322","source":{"kind":"arxiv","id":"1301.0537","version":2},"attestation_state":"computed","paper":{"title":"Holography without translational symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el"],"primary_cat":"hep-th","authors_text":"David Vegh","submitted_at":"2013-01-03T20:11:12Z","abstract_excerpt":"We propose massive gravity as a holographic framework for describing a class of strongly interacting quantum field theories with broken translational symmetry. Bulk gravitons are assumed to have a Lorentz-breaking mass term as a substitute for spatial inhomogeneities. This breaks momentum-conservation in the boundary field theory. At finite chemical potential, the gravity duals are charged black holes in asymptotically anti-de Sitter spacetime. The conductivity in these systems generally exhibits a Drude peak that approaches a delta function in the massless gravity limit. Furthermore, the opti"},"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":"1301.0537","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-01-03T20:11:12Z","cross_cats_sorted":["cond-mat.str-el"],"title_canon_sha256":"c78c45cc75c6d87ec31201676aa650ef93de4e3b01df106ccfd29959d45eec73","abstract_canon_sha256":"418e4417f235fe7f4c574032ccacb7dc7ef761095e6c56001ac98108fa88469a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:36:26.515472Z","signature_b64":"rsAIqC+HCL4EawzrVc665SVsit1j1fuTPldIbk25Nx5jds754nQJJdztijAWByFaNMY5oSIYAuuWGIVHeLNoDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7cde19c3ff04ad1a59094c3365d6fa6f60d801e0efed6620bde94b8255f8a322","last_reissued_at":"2026-05-18T03:36:26.514666Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:36:26.514666Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holography without translational symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el"],"primary_cat":"hep-th","authors_text":"David Vegh","submitted_at":"2013-01-03T20:11:12Z","abstract_excerpt":"We propose massive gravity as a holographic framework for describing a class of strongly interacting quantum field theories with broken translational symmetry. Bulk gravitons are assumed to have a Lorentz-breaking mass term as a substitute for spatial inhomogeneities. This breaks momentum-conservation in the boundary field theory. At finite chemical potential, the gravity duals are charged black holes in asymptotically anti-de Sitter spacetime. The conductivity in these systems generally exhibits a Drude peak that approaches a delta function in the massless gravity limit. Furthermore, the opti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.0537","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":"1301.0537","created_at":"2026-05-18T03:36:26.514796+00:00"},{"alias_kind":"arxiv_version","alias_value":"1301.0537v2","created_at":"2026-05-18T03:36:26.514796+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.0537","created_at":"2026-05-18T03:36:26.514796+00:00"},{"alias_kind":"pith_short_12","alias_value":"PTPBTQ77ASWR","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"PTPBTQ77ASWRUWIJ","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"PTPBTQ77","created_at":"2026-05-18T12:27:57.521954+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2509.04261","citing_title":"Topological charge and black hole photon spheres in massive gravity","ref_index":78,"is_internal_anchor":true},{"citing_arxiv_id":"2601.00071","citing_title":"Diagnosing Effective Metal-Insulator and Hawking-Page Transitions: A Mixed-State Entanglement Perspective in Einstein-Born-Infeld-Massive Gravity","ref_index":53,"is_internal_anchor":true},{"citing_arxiv_id":"2604.02402","citing_title":"Thermodynamics and phase transitions of charged-AdS black holes in dRGT massive gravity with nonlinear electrodynamics","ref_index":21,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5","json":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5.json","graph_json":"https://pith.science/api/pith-number/PTPBTQ77ASWRUWIJJQZWLVX2N5/graph.json","events_json":"https://pith.science/api/pith-number/PTPBTQ77ASWRUWIJJQZWLVX2N5/events.json","paper":"https://pith.science/paper/PTPBTQ77"},"agent_actions":{"view_html":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5","download_json":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5.json","view_paper":"https://pith.science/paper/PTPBTQ77","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1301.0537&json=true","fetch_graph":"https://pith.science/api/pith-number/PTPBTQ77ASWRUWIJJQZWLVX2N5/graph.json","fetch_events":"https://pith.science/api/pith-number/PTPBTQ77ASWRUWIJJQZWLVX2N5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5/action/storage_attestation","attest_author":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5/action/author_attestation","sign_citation":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5/action/citation_signature","submit_replication":"https://pith.science/pith/PTPBTQ77ASWRUWIJJQZWLVX2N5/action/replication_record"}},"created_at":"2026-05-18T03:36:26.514796+00:00","updated_at":"2026-05-18T03:36:26.514796+00:00"}