{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:7GAES3CY7RCAEHKWAXFNSKWNTN","short_pith_number":"pith:7GAES3CY","schema_version":"1.0","canonical_sha256":"f980496c58fc44021d5605cad92acd9b5928efb8f3324c4d886d0c84ec3e765e","source":{"kind":"arxiv","id":"2004.14468","version":2},"attestation_state":"computed","paper":{"title":"Born-Infeld Black Holes in 4D Einstein-Gauss-Bonnet Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bao-Min Gu, Ke Yang, Shao-Wen Wei, Yu-Xiao Liu","submitted_at":"2020-04-29T20:46:56Z","abstract_excerpt":"A novel four-dimensional Einstein-Gauss-Bonnet gravity was formulated by D. Glavan and C. Lin [Phys. Rev. Lett. 124, 081301 (2020)], which is intended to bypass the Lovelock's theorem and to yield a non-trivial contribution to the four-dimensional gravitational dynamics. However, the validity and consistency of this theory has been called into question recently. We study a static and spherically symmetric black hole charged by a Born-Infeld electric field in the novel four-dimensional Einstein-Gauss-Bonnet gravity. It is found that the black hole solution still suffers the singularity problem,"},"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":"2004.14468","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-04-29T20:46:56Z","cross_cats_sorted":[],"title_canon_sha256":"560dfa7a030478eaa726bd35b0498466d40553b92e4badf44b51c2072dffb16a","abstract_canon_sha256":"f98f164dd72ee1d6b508a02f3620a32ff4c842919cf721d0761490b53bdd52e8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:21:48.327067Z","signature_b64":"sbI8hUj4p6dngFgdNZgs0sce1cjSTZXTHEecguMKBKdnMOE6ClQM9SVvuCXFL7io2IIwbkEHNvlyMVlDa3DJCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f980496c58fc44021d5605cad92acd9b5928efb8f3324c4d886d0c84ec3e765e","last_reissued_at":"2026-07-05T01:21:48.326544Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:21:48.326544Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Born-Infeld Black Holes in 4D Einstein-Gauss-Bonnet Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bao-Min Gu, Ke Yang, Shao-Wen Wei, Yu-Xiao Liu","submitted_at":"2020-04-29T20:46:56Z","abstract_excerpt":"A novel four-dimensional Einstein-Gauss-Bonnet gravity was formulated by D. Glavan and C. Lin [Phys. Rev. Lett. 124, 081301 (2020)], which is intended to bypass the Lovelock's theorem and to yield a non-trivial contribution to the four-dimensional gravitational dynamics. However, the validity and consistency of this theory has been called into question recently. We study a static and spherically symmetric black hole charged by a Born-Infeld electric field in the novel four-dimensional Einstein-Gauss-Bonnet gravity. It is found that the black hole solution still suffers the singularity problem,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2004.14468","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2004.14468/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":"2004.14468","created_at":"2026-07-05T01:21:48.326610+00:00"},{"alias_kind":"arxiv_version","alias_value":"2004.14468v2","created_at":"2026-07-05T01:21:48.326610+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2004.14468","created_at":"2026-07-05T01:21:48.326610+00:00"},{"alias_kind":"pith_short_12","alias_value":"7GAES3CY7RCA","created_at":"2026-07-05T01:21:48.326610+00:00"},{"alias_kind":"pith_short_16","alias_value":"7GAES3CY7RCAEHKW","created_at":"2026-07-05T01:21:48.326610+00:00"},{"alias_kind":"pith_short_8","alias_value":"7GAES3CY","created_at":"2026-07-05T01:21:48.326610+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"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":40,"is_internal_anchor":false},{"citing_arxiv_id":"2603.06786","citing_title":"All $2D$ generalised dilaton theories from $d\\geq 4$ gravities","ref_index":94,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25254","citing_title":"The properties and predictions of quasi-periodic oscillations around a black hole in nonlocal gravity","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24860","citing_title":"Bouncing cosmologies from Born-Infeld-type gravity","ref_index":41,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN","json":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN.json","graph_json":"https://pith.science/api/pith-number/7GAES3CY7RCAEHKWAXFNSKWNTN/graph.json","events_json":"https://pith.science/api/pith-number/7GAES3CY7RCAEHKWAXFNSKWNTN/events.json","paper":"https://pith.science/paper/7GAES3CY"},"agent_actions":{"view_html":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN","download_json":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN.json","view_paper":"https://pith.science/paper/7GAES3CY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2004.14468&json=true","fetch_graph":"https://pith.science/api/pith-number/7GAES3CY7RCAEHKWAXFNSKWNTN/graph.json","fetch_events":"https://pith.science/api/pith-number/7GAES3CY7RCAEHKWAXFNSKWNTN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN/action/storage_attestation","attest_author":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN/action/author_attestation","sign_citation":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN/action/citation_signature","submit_replication":"https://pith.science/pith/7GAES3CY7RCAEHKWAXFNSKWNTN/action/replication_record"}},"created_at":"2026-07-05T01:21:48.326610+00:00","updated_at":"2026-07-05T01:21:48.326610+00:00"}