{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:PQ76FZID42QPMWPTCMGLCHZBHE","short_pith_number":"pith:PQ76FZID","schema_version":"1.0","canonical_sha256":"7c3fe2e503e6a0f659f3130cb11f21393702bda1b7fd2374ea8c439a65c12316","source":{"kind":"arxiv","id":"1705.03867","version":2},"attestation_state":"computed","paper":{"title":"Cosmological reconstructed solutions in extended teleparallel gravity theories with a teleparallel Gauss-Bonnet term","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Alvaro de la Cruz-Dombriz (Cape Town U.), CSIC/IEEC), Diego Saez-Chillon Gomez (Institute of Space Sciences, Gabriel Farrugia (U. of Malta), Jackson Levi Said (U. of Malta)","submitted_at":"2017-05-10T17:34:37Z","abstract_excerpt":"In the context of extended Teleparallel gravity theories with a 3+1 dimensions Gauss-Bonnet analog term, we address the possibility of these theories reproducing several well-known cosmological solutions. In particular when applied to a Friedmann-Lema\\^itre-Robertson-Walker geometry in four-dimensional spacetime with standard fluids exclusively. We study different types of gravitational Lagrangians and reconstruct solutions provided by analytical expressions for either the cosmological scale factor or the Hubble parameter. We also show that it is possible to find Lagrangians of this type witho"},"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":"1705.03867","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-05-10T17:34:37Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"c70864cc4b5aef8ac9c691ee66324b1b911f13f1e0e27a84d308d5a66365afaa","abstract_canon_sha256":"8fd2f1f39c70b6eb8e25d25066102c4b4f61e1224eefa989ca4a8f856d06f4af"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:46.359233Z","signature_b64":"vIwMK3PQyYHvTZDR8jN9Nk3l3LL7gsLgq6OuL3AQe5SHpaDKxl8j/38r+bNV4Y89iriCTKB4zZywE8M83Co0Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c3fe2e503e6a0f659f3130cb11f21393702bda1b7fd2374ea8c439a65c12316","last_reissued_at":"2026-05-18T00:28:46.358494Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:46.358494Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological reconstructed solutions in extended teleparallel gravity theories with a teleparallel Gauss-Bonnet term","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Alvaro de la Cruz-Dombriz (Cape Town U.), CSIC/IEEC), Diego Saez-Chillon Gomez (Institute of Space Sciences, Gabriel Farrugia (U. of Malta), Jackson Levi Said (U. of Malta)","submitted_at":"2017-05-10T17:34:37Z","abstract_excerpt":"In the context of extended Teleparallel gravity theories with a 3+1 dimensions Gauss-Bonnet analog term, we address the possibility of these theories reproducing several well-known cosmological solutions. In particular when applied to a Friedmann-Lema\\^itre-Robertson-Walker geometry in four-dimensional spacetime with standard fluids exclusively. We study different types of gravitational Lagrangians and reconstruct solutions provided by analytical expressions for either the cosmological scale factor or the Hubble parameter. We also show that it is possible to find Lagrangians of this type witho"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.03867","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":""},"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":"1705.03867","created_at":"2026-05-18T00:28:46.358617+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.03867v2","created_at":"2026-05-18T00:28:46.358617+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.03867","created_at":"2026-05-18T00:28:46.358617+00:00"},{"alias_kind":"pith_short_12","alias_value":"PQ76FZID42QP","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_16","alias_value":"PQ76FZID42QPMWPT","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_8","alias_value":"PQ76FZID","created_at":"2026-05-18T12:31:37.085036+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.19221","citing_title":"Thick branes and fermion localization in five-dimensional $f(T,T_G)$ gravity","ref_index":86,"is_internal_anchor":true},{"citing_arxiv_id":"2509.02646","citing_title":"Gauge invariant perturbations of $F(T,T_G)$ Cosmology","ref_index":60,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE","json":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE.json","graph_json":"https://pith.science/api/pith-number/PQ76FZID42QPMWPTCMGLCHZBHE/graph.json","events_json":"https://pith.science/api/pith-number/PQ76FZID42QPMWPTCMGLCHZBHE/events.json","paper":"https://pith.science/paper/PQ76FZID"},"agent_actions":{"view_html":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE","download_json":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE.json","view_paper":"https://pith.science/paper/PQ76FZID","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.03867&json=true","fetch_graph":"https://pith.science/api/pith-number/PQ76FZID42QPMWPTCMGLCHZBHE/graph.json","fetch_events":"https://pith.science/api/pith-number/PQ76FZID42QPMWPTCMGLCHZBHE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE/action/storage_attestation","attest_author":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE/action/author_attestation","sign_citation":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE/action/citation_signature","submit_replication":"https://pith.science/pith/PQ76FZID42QPMWPTCMGLCHZBHE/action/replication_record"}},"created_at":"2026-05-18T00:28:46.358617+00:00","updated_at":"2026-05-18T00:28:46.358617+00:00"}