{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:NPWXYFZ2SZJO6KKE7655JOLRKM","short_pith_number":"pith:NPWXYFZ2","schema_version":"1.0","canonical_sha256":"6bed7c173a9652ef2944ffbbd4b97153064467e992a582adfbcbff4b90ef5a76","source":{"kind":"arxiv","id":"1610.08019","version":3},"attestation_state":"computed","paper":{"title":"Four-dimensional black holes in Einsteinian cubic gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Pablo A. Cano, Pablo Bueno","submitted_at":"2016-10-25T18:55:20Z","abstract_excerpt":"We construct static and spherically symmetric generalizations of the Schwarzschild- and Reissner-Nordstr\\\"om-(Anti-)de Sitter (RN-(A)dS) black-hole solutions in four-dimensional Einsteinian cubic gravity (ECG). The solutions are determined by a single blackening factor which satisfies a non-linear second-order differential equation. Interestingly, we are able to compute independently the Hawking temperature $T$, the Wald entropy $\\mathsf{S}$ and the Abbott-Deser mass $M$ of the solutions analytically as functions of the horizon radius and the ECG coupling constant $\\lambda$. Using these we sho"},"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":"1610.08019","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2016-10-25T18:55:20Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"b2766d829c13ff14db235b100c79cab321971d5efabe8a445623bc96fbd11bec","abstract_canon_sha256":"94c4f4be6e6f885c8bd36f2f9f45e4ea2df74a8da88105fa18a777bc991219c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:52:22.570417Z","signature_b64":"ohaZBQazRY3SeLPQz4tcrsV1deid6ckkbna5YN7szVbne6+j/DJhW5/EL8g/XJuSQYV27/55iq8IFiaVxc68AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6bed7c173a9652ef2944ffbbd4b97153064467e992a582adfbcbff4b90ef5a76","last_reissued_at":"2026-05-18T00:52:22.569710Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:52:22.569710Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Four-dimensional black holes in Einsteinian cubic gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Pablo A. Cano, Pablo Bueno","submitted_at":"2016-10-25T18:55:20Z","abstract_excerpt":"We construct static and spherically symmetric generalizations of the Schwarzschild- and Reissner-Nordstr\\\"om-(Anti-)de Sitter (RN-(A)dS) black-hole solutions in four-dimensional Einsteinian cubic gravity (ECG). The solutions are determined by a single blackening factor which satisfies a non-linear second-order differential equation. Interestingly, we are able to compute independently the Hawking temperature $T$, the Wald entropy $\\mathsf{S}$ and the Abbott-Deser mass $M$ of the solutions analytically as functions of the horizon radius and the ECG coupling constant $\\lambda$. Using these we sho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.08019","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":""},"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":"1610.08019","created_at":"2026-05-18T00:52:22.569808+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.08019v3","created_at":"2026-05-18T00:52:22.569808+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.08019","created_at":"2026-05-18T00:52:22.569808+00:00"},{"alias_kind":"pith_short_12","alias_value":"NPWXYFZ2SZJO","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"NPWXYFZ2SZJO6KKE","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"NPWXYFZ2","created_at":"2026-05-18T12:30:36.002864+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2311.12104","citing_title":"Cosmological higher-curvature gravities","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2601.01861","citing_title":"Regular Black Holes in Quasitopological Gravity: Null Shells and Mass Inflation","ref_index":21,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM","json":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM.json","graph_json":"https://pith.science/api/pith-number/NPWXYFZ2SZJO6KKE7655JOLRKM/graph.json","events_json":"https://pith.science/api/pith-number/NPWXYFZ2SZJO6KKE7655JOLRKM/events.json","paper":"https://pith.science/paper/NPWXYFZ2"},"agent_actions":{"view_html":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM","download_json":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM.json","view_paper":"https://pith.science/paper/NPWXYFZ2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.08019&json=true","fetch_graph":"https://pith.science/api/pith-number/NPWXYFZ2SZJO6KKE7655JOLRKM/graph.json","fetch_events":"https://pith.science/api/pith-number/NPWXYFZ2SZJO6KKE7655JOLRKM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM/action/storage_attestation","attest_author":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM/action/author_attestation","sign_citation":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM/action/citation_signature","submit_replication":"https://pith.science/pith/NPWXYFZ2SZJO6KKE7655JOLRKM/action/replication_record"}},"created_at":"2026-05-18T00:52:22.569808+00:00","updated_at":"2026-05-18T00:52:22.569808+00:00"}