{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:F4MIIXOZNPJ4JKMKRDBUTTUKFN","short_pith_number":"pith:F4MIIXOZ","schema_version":"1.0","canonical_sha256":"2f18845dd96bd3c4a98a88c349ce8a2b495e4b2cb9935a03147b239bcb8e40e6","source":{"kind":"arxiv","id":"2312.17277","version":2},"attestation_state":"computed","paper":{"title":"Observational Constraints and Cosmographic Analysis of $f({T},{T}_{{G}})$ Gravity and Cosmology","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Emmanuel N. Saridakis, Harshna Balhara, J. K. Singh, Shaily","submitted_at":"2023-12-27T19:28:25Z","abstract_excerpt":"We perform observational confrontation and cosmographic analysis of $f(T,T_G)$ gravity and cosmology. This higher-order torsional gravity is based on both the torsion scalar, as well as on the teleparallel equivalent of the Gauss--Bonnet combination, and gives rise to an effective dark-energy sector which depends on the extra torsion contributions. We employ observational data from the Hubble function and supernova Type Ia Pantheon datasets, applying a Markov chain Monte Carlo sampling technique, and we provide the iso-likelihood contours, as well as the best-fit values for the parameters of t"},"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":"2312.17277","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-12-27T19:28:25Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"fe8b4c8f68fefe9bb9737ac3b12ca217b4076ee8b1dd456c16c6252b3727de2e","abstract_canon_sha256":"70f0d09d45793dcb2d39d157638d7c5269199e54f1ba174af8f8dbc251c187da"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:19:25.687324Z","signature_b64":"UPoU5m3bMcq3G2+aE7t0hfeckqwcGnllJpFGMI8bCXohnptjID/vsJ/9XgG4WVTFGti0C4qLvZCh918Xs0mEBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2f18845dd96bd3c4a98a88c349ce8a2b495e4b2cb9935a03147b239bcb8e40e6","last_reissued_at":"2026-07-05T09:19:25.686882Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:19:25.686882Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Observational Constraints and Cosmographic Analysis of $f({T},{T}_{{G}})$ Gravity and Cosmology","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Emmanuel N. Saridakis, Harshna Balhara, J. K. Singh, Shaily","submitted_at":"2023-12-27T19:28:25Z","abstract_excerpt":"We perform observational confrontation and cosmographic analysis of $f(T,T_G)$ gravity and cosmology. This higher-order torsional gravity is based on both the torsion scalar, as well as on the teleparallel equivalent of the Gauss--Bonnet combination, and gives rise to an effective dark-energy sector which depends on the extra torsion contributions. We employ observational data from the Hubble function and supernova Type Ia Pantheon datasets, applying a Markov chain Monte Carlo sampling technique, and we provide the iso-likelihood contours, as well as the best-fit values for the parameters of t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.17277","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/2312.17277/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":"2312.17277","created_at":"2026-07-05T09:19:25.686933+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.17277v2","created_at":"2026-07-05T09:19:25.686933+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.17277","created_at":"2026-07-05T09:19:25.686933+00:00"},{"alias_kind":"pith_short_12","alias_value":"F4MIIXOZNPJ4","created_at":"2026-07-05T09:19:25.686933+00:00"},{"alias_kind":"pith_short_16","alias_value":"F4MIIXOZNPJ4JKMK","created_at":"2026-07-05T09:19:25.686933+00:00"},{"alias_kind":"pith_short_8","alias_value":"F4MIIXOZ","created_at":"2026-07-05T09:19:25.686933+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.18285","citing_title":"Einstein-Gauss-Bonnet-Myrzakulov Gravity from $R + F(T, G)$: Numerical Insights and Torsion-Gauss-Bonnet Dynamics in Weitzenb\\\"ock Spacetime","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN","json":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN.json","graph_json":"https://pith.science/api/pith-number/F4MIIXOZNPJ4JKMKRDBUTTUKFN/graph.json","events_json":"https://pith.science/api/pith-number/F4MIIXOZNPJ4JKMKRDBUTTUKFN/events.json","paper":"https://pith.science/paper/F4MIIXOZ"},"agent_actions":{"view_html":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN","download_json":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN.json","view_paper":"https://pith.science/paper/F4MIIXOZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.17277&json=true","fetch_graph":"https://pith.science/api/pith-number/F4MIIXOZNPJ4JKMKRDBUTTUKFN/graph.json","fetch_events":"https://pith.science/api/pith-number/F4MIIXOZNPJ4JKMKRDBUTTUKFN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN/action/storage_attestation","attest_author":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN/action/author_attestation","sign_citation":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN/action/citation_signature","submit_replication":"https://pith.science/pith/F4MIIXOZNPJ4JKMKRDBUTTUKFN/action/replication_record"}},"created_at":"2026-07-05T09:19:25.686933+00:00","updated_at":"2026-07-05T09:19:25.686933+00:00"}