{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:R4IWU2P7K7XTICVZITM5IISABU","short_pith_number":"pith:R4IWU2P7","schema_version":"1.0","canonical_sha256":"8f116a69ff57ef340ab944d9d422400d08a358e8ec7b3ff8d3155064d6623961","source":{"kind":"arxiv","id":"2003.07788","version":3},"attestation_state":"computed","paper":{"title":"Black holes in the four-dimensional Einstein-Lovelock gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"A. Zhidenko, R. A. Konoplya","submitted_at":"2020-03-17T16:11:56Z","abstract_excerpt":"A $(3+1)$-dimensional Einstein-Gauss-Bonnet theory of gravity has been recently formulated in [D. Glavan and C. Lin, Phys. Rev. Lett. {\\bf 124}, 081301 (2020)] which is different from the pure Einstein theory, i.e., bypasses the Lovelock's theorem and avoids Ostrogradsky instability. The theory was formulated in $D > 4$ dimensions and its action consists of the Einstein-Hilbert term with a cosmological constant, while the Gauss-Bonnet term multiplied by a factor $1/(D-4)$. Then, the four-dimensional theory is defined as the limit $D \\to 4$. Here we generalize this approach to the four-dimensio"},"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":"2003.07788","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-03-17T16:11:56Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"b1c15e503f35f5de689587da91a54fe4950ba82f6957aa790e61722e536dd8b5","abstract_canon_sha256":"5d1609d2cc2a32c042059d0cc8cb87b443f85700d918196440193efc7b349009"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:36:16.698090Z","signature_b64":"0RNZUTlDelFj7jpy8rG6qmnFX6vePg9N4n/P5cIB3oBrctpv85qWjYFCVrW4z1ao/BqKK/uhGKD4Iq/cWABnDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8f116a69ff57ef340ab944d9d422400d08a358e8ec7b3ff8d3155064d6623961","last_reissued_at":"2026-07-05T01:36:16.697611Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:36:16.697611Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black holes in the four-dimensional Einstein-Lovelock gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"A. Zhidenko, R. A. Konoplya","submitted_at":"2020-03-17T16:11:56Z","abstract_excerpt":"A $(3+1)$-dimensional Einstein-Gauss-Bonnet theory of gravity has been recently formulated in [D. Glavan and C. Lin, Phys. Rev. Lett. {\\bf 124}, 081301 (2020)] which is different from the pure Einstein theory, i.e., bypasses the Lovelock's theorem and avoids Ostrogradsky instability. The theory was formulated in $D > 4$ dimensions and its action consists of the Einstein-Hilbert term with a cosmological constant, while the Gauss-Bonnet term multiplied by a factor $1/(D-4)$. Then, the four-dimensional theory is defined as the limit $D \\to 4$. Here we generalize this approach to the four-dimensio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2003.07788","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/2003.07788/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":"2003.07788","created_at":"2026-07-05T01:36:16.697673+00:00"},{"alias_kind":"arxiv_version","alias_value":"2003.07788v3","created_at":"2026-07-05T01:36:16.697673+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2003.07788","created_at":"2026-07-05T01:36:16.697673+00:00"},{"alias_kind":"pith_short_12","alias_value":"R4IWU2P7K7XT","created_at":"2026-07-05T01:36:16.697673+00:00"},{"alias_kind":"pith_short_16","alias_value":"R4IWU2P7K7XTICVZ","created_at":"2026-07-05T01:36:16.697673+00:00"},{"alias_kind":"pith_short_8","alias_value":"R4IWU2P7","created_at":"2026-07-05T01:36:16.697673+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2205.07787","citing_title":"Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2603.06786","citing_title":"All $2D$ generalised dilaton theories from $d\\geq 4$ gravities","ref_index":85,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU","json":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU.json","graph_json":"https://pith.science/api/pith-number/R4IWU2P7K7XTICVZITM5IISABU/graph.json","events_json":"https://pith.science/api/pith-number/R4IWU2P7K7XTICVZITM5IISABU/events.json","paper":"https://pith.science/paper/R4IWU2P7"},"agent_actions":{"view_html":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU","download_json":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU.json","view_paper":"https://pith.science/paper/R4IWU2P7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2003.07788&json=true","fetch_graph":"https://pith.science/api/pith-number/R4IWU2P7K7XTICVZITM5IISABU/graph.json","fetch_events":"https://pith.science/api/pith-number/R4IWU2P7K7XTICVZITM5IISABU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU/action/storage_attestation","attest_author":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU/action/author_attestation","sign_citation":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU/action/citation_signature","submit_replication":"https://pith.science/pith/R4IWU2P7K7XTICVZITM5IISABU/action/replication_record"}},"created_at":"2026-07-05T01:36:16.697673+00:00","updated_at":"2026-07-05T01:36:16.697673+00:00"}