{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:TA62C65INJPOQGX7V2XIR4GN4Q","short_pith_number":"pith:TA62C65I","schema_version":"1.0","canonical_sha256":"983da17ba86a5ee81affaeae88f0cde41cb6e1f7d36e3ec967f9f75b57fdd2b0","source":{"kind":"arxiv","id":"1404.2249","version":3},"attestation_state":"computed","paper":{"title":"Teleparallel equivalent of Gauss-Bonnet gravity and its modifications","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Athens, Catolica), Emmanuel N. Saridakis (Natl. Tech. U., Georgios Kofinas (Aegean U.), Valparaiso U.","submitted_at":"2014-04-08T18:52:21Z","abstract_excerpt":"Inspired by the teleparallel formulation of General Relativity, whose Lagrangian is the torsion invariant T, we have constructed the teleparallel equivalent of Gauss-Bonnet gravity in arbitrary dimensions. Without imposing the Weitzenbock connection, we have extracted the torsion invariant T_G, equivalent (up to boundary terms) to the Gauss-Bonnet term G. T_G is constructed by the vielbein and the connection, it contains quartic powers of the torsion tensor, it is diffeomorphism and Lorentz invariant, and in four dimensions it reduces to a topological invariant as expected. Imposing the Weitze"},"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":"1404.2249","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2014-04-08T18:52:21Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"59684d201b9aed9b992b7410b7abea118132afb74ebb3dba46f8c4b3a20aeee5","abstract_canon_sha256":"545c92fa54802ef9c8eaab816004f2a3730f8f87907104dc77584640d76e41a4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:39:16.448848Z","signature_b64":"sQvGNl8EA2Dm4DDqxYEZ4NPbuHWaeOKHRwww6ZRWoTEmePQSSeomvpMwzuKmkFvNBIbxr9PH66a5UoGj5w7hBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"983da17ba86a5ee81affaeae88f0cde41cb6e1f7d36e3ec967f9f75b57fdd2b0","last_reissued_at":"2026-05-18T02:39:16.448432Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:39:16.448432Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Teleparallel equivalent of Gauss-Bonnet gravity and its modifications","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Athens, Catolica), Emmanuel N. Saridakis (Natl. Tech. U., Georgios Kofinas (Aegean U.), Valparaiso U.","submitted_at":"2014-04-08T18:52:21Z","abstract_excerpt":"Inspired by the teleparallel formulation of General Relativity, whose Lagrangian is the torsion invariant T, we have constructed the teleparallel equivalent of Gauss-Bonnet gravity in arbitrary dimensions. Without imposing the Weitzenbock connection, we have extracted the torsion invariant T_G, equivalent (up to boundary terms) to the Gauss-Bonnet term G. T_G is constructed by the vielbein and the connection, it contains quartic powers of the torsion tensor, it is diffeomorphism and Lorentz invariant, and in four dimensions it reduces to a topological invariant as expected. Imposing the Weitze"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.2249","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":"1404.2249","created_at":"2026-05-18T02:39:16.448490+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.2249v3","created_at":"2026-05-18T02:39:16.448490+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.2249","created_at":"2026-05-18T02:39:16.448490+00:00"},{"alias_kind":"pith_short_12","alias_value":"TA62C65INJPO","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"TA62C65INJPOQGX7","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"TA62C65I","created_at":"2026-05-18T12:28:49.207871+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2603.03568","citing_title":"Observational constraints on Luciano-Saridakis entropic cosmology","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19221","citing_title":"Thick branes and fermion localization in five-dimensional $f(T,T_G)$ gravity","ref_index":80,"is_internal_anchor":true},{"citing_arxiv_id":"2509.02646","citing_title":"Gauge invariant perturbations of $F(T,T_G)$ Cosmology","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2602.16237","citing_title":"Rotating Black Holes with Primary Scalar Hair: Shadow Signatures in Beyond Horndeski Gravity","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2604.13002","citing_title":"Cosmologically viable non-polynomial quasi-topological gravity: explicit models, $\\Lambda$CDM limit and observational constraints","ref_index":21,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q","json":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q.json","graph_json":"https://pith.science/api/pith-number/TA62C65INJPOQGX7V2XIR4GN4Q/graph.json","events_json":"https://pith.science/api/pith-number/TA62C65INJPOQGX7V2XIR4GN4Q/events.json","paper":"https://pith.science/paper/TA62C65I"},"agent_actions":{"view_html":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q","download_json":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q.json","view_paper":"https://pith.science/paper/TA62C65I","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.2249&json=true","fetch_graph":"https://pith.science/api/pith-number/TA62C65INJPOQGX7V2XIR4GN4Q/graph.json","fetch_events":"https://pith.science/api/pith-number/TA62C65INJPOQGX7V2XIR4GN4Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q/action/storage_attestation","attest_author":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q/action/author_attestation","sign_citation":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q/action/citation_signature","submit_replication":"https://pith.science/pith/TA62C65INJPOQGX7V2XIR4GN4Q/action/replication_record"}},"created_at":"2026-05-18T02:39:16.448490+00:00","updated_at":"2026-05-18T02:39:16.448490+00:00"}