{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:CDRF4VB6DLWROIBSVUOYFPVG6I","short_pith_number":"pith:CDRF4VB6","schema_version":"1.0","canonical_sha256":"10e25e543e1aed172032ad1d82bea6f216d70ef903c538543daa9f46d06dc4bd","source":{"kind":"arxiv","id":"2004.00479","version":2},"attestation_state":"computed","paper":{"title":"Swampland Implications of GW170817-compatible Einstein-Gauss-Bonnet Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"S.D. Odintsov, V.K. Oikonomou","submitted_at":"2020-04-01T14:50:43Z","abstract_excerpt":"We revisit the Einstein-Gauss-Bonnet theory in view of the GW170817 event, which compels that the gravitational wave speed is equal to $c_T^2=1$ in natural units. We use an alternative approach compared to one previous work of ours, which enables us to express all the slow-roll indices and the observational indices as functions of the scalar field. Using our formalism we investigate if the Swampland criteria are satisfied for the Einstein-Gauss-Bonnet theory and as we demonstrate, the Swampland criteria are satisfied for quite general forms of the potential and the Gauss-Bonnet coupling functi"},"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":"2004.00479","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-04-01T14:50:43Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"97abf0c8150faaec781be7359cebdf6e5f2335636823eecf035028b8fffa6823","abstract_canon_sha256":"0783fa04262bdbd9a1e24ad44c1284f3eed3bfd7a2f3b2aaa994a0e568ec7624"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:57:20.200573Z","signature_b64":"GkDqeXVgu8zb7GVqplYNsOnM/yogfoBfEdnFsEx6faq5n7WcY8e98v98fuob5/Q2ebf2o/4FzSqLwh1dcJllDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"10e25e543e1aed172032ad1d82bea6f216d70ef903c538543daa9f46d06dc4bd","last_reissued_at":"2026-07-05T00:57:20.200115Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:57:20.200115Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Swampland Implications of GW170817-compatible Einstein-Gauss-Bonnet Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"S.D. Odintsov, V.K. Oikonomou","submitted_at":"2020-04-01T14:50:43Z","abstract_excerpt":"We revisit the Einstein-Gauss-Bonnet theory in view of the GW170817 event, which compels that the gravitational wave speed is equal to $c_T^2=1$ in natural units. We use an alternative approach compared to one previous work of ours, which enables us to express all the slow-roll indices and the observational indices as functions of the scalar field. Using our formalism we investigate if the Swampland criteria are satisfied for the Einstein-Gauss-Bonnet theory and as we demonstrate, the Swampland criteria are satisfied for quite general forms of the potential and the Gauss-Bonnet coupling functi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2004.00479","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/2004.00479/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":"2004.00479","created_at":"2026-07-05T00:57:20.200165+00:00"},{"alias_kind":"arxiv_version","alias_value":"2004.00479v2","created_at":"2026-07-05T00:57:20.200165+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2004.00479","created_at":"2026-07-05T00:57:20.200165+00:00"},{"alias_kind":"pith_short_12","alias_value":"CDRF4VB6DLWR","created_at":"2026-07-05T00:57:20.200165+00:00"},{"alias_kind":"pith_short_16","alias_value":"CDRF4VB6DLWROIBS","created_at":"2026-07-05T00:57:20.200165+00:00"},{"alias_kind":"pith_short_8","alias_value":"CDRF4VB6","created_at":"2026-07-05T00:57:20.200165+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.23047","citing_title":"On Thermodynamics of Charged Black Holes, Swampland, and Dark Matter","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2203.06142","citing_title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","ref_index":143,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14659","citing_title":"Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway","ref_index":120,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I","json":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I.json","graph_json":"https://pith.science/api/pith-number/CDRF4VB6DLWROIBSVUOYFPVG6I/graph.json","events_json":"https://pith.science/api/pith-number/CDRF4VB6DLWROIBSVUOYFPVG6I/events.json","paper":"https://pith.science/paper/CDRF4VB6"},"agent_actions":{"view_html":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I","download_json":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I.json","view_paper":"https://pith.science/paper/CDRF4VB6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2004.00479&json=true","fetch_graph":"https://pith.science/api/pith-number/CDRF4VB6DLWROIBSVUOYFPVG6I/graph.json","fetch_events":"https://pith.science/api/pith-number/CDRF4VB6DLWROIBSVUOYFPVG6I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I/action/storage_attestation","attest_author":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I/action/author_attestation","sign_citation":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I/action/citation_signature","submit_replication":"https://pith.science/pith/CDRF4VB6DLWROIBSVUOYFPVG6I/action/replication_record"}},"created_at":"2026-07-05T00:57:20.200165+00:00","updated_at":"2026-07-05T00:57:20.200165+00:00"}