{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:G4LPZW6OWSSY5WVHJJHDREU6DN","short_pith_number":"pith:G4LPZW6O","schema_version":"1.0","canonical_sha256":"3716fcdbceb4a58edaa74a4e38929e1b65fedd4080e18c28dc7cce13ce73ea7b","source":{"kind":"arxiv","id":"1810.00758","version":1},"attestation_state":"computed","paper":{"title":"Action growth rate for a higher curvature gravitational theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Jie Jiang","submitted_at":"2018-10-01T15:27:55Z","abstract_excerpt":"In this paper, we use the \"complexity equals action\" (CA) conjecture to discuss the action growth rate in a black hole with multiple Killing horizons for a higher curvature theory of gravity. Based on the Noether charge formalism of Iyer and Wald, a general formalism can be resorting to finding the action growth rate within the WDW patch at the late time approximation. Moreover, as an application, we apply this formalism to a $U(1)$ invariance matter fields and utilise our results in two specific cases. Our results are universal and can be considered as the extension of the asymptotic AdS to t"},"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":"1810.00758","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2018-10-01T15:27:55Z","cross_cats_sorted":[],"title_canon_sha256":"01149ab884e9ffc5edd7688b290401f69a7208fb1c445d4549407e9c22cd8dde","abstract_canon_sha256":"29d77932f5a6a165d3d3984c80caf7844b7dea1e979942373af4b9ed72e52de0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:02:30.498565Z","signature_b64":"x+tPqSjyAjU1YuxQyC+gM+7TSTV7aszC0fdZZe9RDXzVAv1BIO5dDogepcTtTIWJH45PUweLGmJT7I6BdFhnBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3716fcdbceb4a58edaa74a4e38929e1b65fedd4080e18c28dc7cce13ce73ea7b","last_reissued_at":"2026-05-18T00:02:30.497939Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:02:30.497939Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Action growth rate for a higher curvature gravitational theory","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Jie Jiang","submitted_at":"2018-10-01T15:27:55Z","abstract_excerpt":"In this paper, we use the \"complexity equals action\" (CA) conjecture to discuss the action growth rate in a black hole with multiple Killing horizons for a higher curvature theory of gravity. Based on the Noether charge formalism of Iyer and Wald, a general formalism can be resorting to finding the action growth rate within the WDW patch at the late time approximation. Moreover, as an application, we apply this formalism to a $U(1)$ invariance matter fields and utilise our results in two specific cases. Our results are universal and can be considered as the extension of the asymptotic AdS to t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.00758","kind":"arxiv","version":1},"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":"1810.00758","created_at":"2026-05-18T00:02:30.498026+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.00758v1","created_at":"2026-05-18T00:02:30.498026+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.00758","created_at":"2026-05-18T00:02:30.498026+00:00"},{"alias_kind":"pith_short_12","alias_value":"G4LPZW6OWSSY","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_16","alias_value":"G4LPZW6OWSSY5WVH","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_8","alias_value":"G4LPZW6O","created_at":"2026-05-18T12:32:25.280505+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.09310","citing_title":"Time dependence of complexity for Lovelock black holes","ref_index":26,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN","json":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN.json","graph_json":"https://pith.science/api/pith-number/G4LPZW6OWSSY5WVHJJHDREU6DN/graph.json","events_json":"https://pith.science/api/pith-number/G4LPZW6OWSSY5WVHJJHDREU6DN/events.json","paper":"https://pith.science/paper/G4LPZW6O"},"agent_actions":{"view_html":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN","download_json":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN.json","view_paper":"https://pith.science/paper/G4LPZW6O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.00758&json=true","fetch_graph":"https://pith.science/api/pith-number/G4LPZW6OWSSY5WVHJJHDREU6DN/graph.json","fetch_events":"https://pith.science/api/pith-number/G4LPZW6OWSSY5WVHJJHDREU6DN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN/action/storage_attestation","attest_author":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN/action/author_attestation","sign_citation":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN/action/citation_signature","submit_replication":"https://pith.science/pith/G4LPZW6OWSSY5WVHJJHDREU6DN/action/replication_record"}},"created_at":"2026-05-18T00:02:30.498026+00:00","updated_at":"2026-05-18T00:02:30.498026+00:00"}