{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:TML35DEJCHHPGRAL2JBKT4MIWW","short_pith_number":"pith:TML35DEJ","schema_version":"1.0","canonical_sha256":"9b17be8c8911cef3440bd242a9f188b5b2290d398723325ecb4a2a08cb512b2b","source":{"kind":"arxiv","id":"1108.2789","version":1},"attestation_state":"computed","paper":{"title":"Cosmography in f(T)-gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"A. Ravanpak, H. Farajollahi, S. Capozziello, V. F. Cardone","submitted_at":"2011-08-13T13:17:49Z","abstract_excerpt":"Being based on the only assumption that the universe is homogenous and isotropic on large scales, cosmography is an ideal tool to investigate the cosmic expansion history in a almost model-independent way. Fitting the data on the luminosity distance and Baryon Acoustic Oscillations allows to determine the confidence ranges for the cosmographic parameters hence giving some quantitative constraints that a whatever theory has to fulfill. As an application, we consider here the case of teleparallel gravity (TEGR) also referred to as f(T)-gravity. To this end, we first work out analytical expressio"},"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":"1108.2789","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-08-13T13:17:49Z","cross_cats_sorted":["gr-qc","hep-th"],"title_canon_sha256":"c156475db0c8ac5af9c52ad2c9fde6f7b4ad38b5990b263aed8fd1f79cd5e723","abstract_canon_sha256":"35bd606aa90e5162af3c6b5074125731aaa16fcc862bb32d6b82d7f0dbd45fe6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:08:44.487685Z","signature_b64":"GpiD5lZrkVv7Fq4/QI3EEAsgYYDXGOSOkYEm/f1hSDqjUupyrCDZzri2OdSCkeHxmgXcDMSmfo8mMbzvXv5fBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b17be8c8911cef3440bd242a9f188b5b2290d398723325ecb4a2a08cb512b2b","last_reissued_at":"2026-05-18T04:08:44.487287Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:08:44.487287Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmography in f(T)-gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph.CO","authors_text":"A. Ravanpak, H. Farajollahi, S. Capozziello, V. F. Cardone","submitted_at":"2011-08-13T13:17:49Z","abstract_excerpt":"Being based on the only assumption that the universe is homogenous and isotropic on large scales, cosmography is an ideal tool to investigate the cosmic expansion history in a almost model-independent way. Fitting the data on the luminosity distance and Baryon Acoustic Oscillations allows to determine the confidence ranges for the cosmographic parameters hence giving some quantitative constraints that a whatever theory has to fulfill. As an application, we consider here the case of teleparallel gravity (TEGR) also referred to as f(T)-gravity. To this end, we first work out analytical expressio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.2789","kind":"arxiv","version":1},"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":"1108.2789","created_at":"2026-05-18T04:08:44.487356+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.2789v1","created_at":"2026-05-18T04:08:44.487356+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.2789","created_at":"2026-05-18T04:08:44.487356+00:00"},{"alias_kind":"pith_short_12","alias_value":"TML35DEJCHHP","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_16","alias_value":"TML35DEJCHHPGRAL","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_8","alias_value":"TML35DEJ","created_at":"2026-05-18T12:26:42.757692+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW","json":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW.json","graph_json":"https://pith.science/api/pith-number/TML35DEJCHHPGRAL2JBKT4MIWW/graph.json","events_json":"https://pith.science/api/pith-number/TML35DEJCHHPGRAL2JBKT4MIWW/events.json","paper":"https://pith.science/paper/TML35DEJ"},"agent_actions":{"view_html":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW","download_json":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW.json","view_paper":"https://pith.science/paper/TML35DEJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.2789&json=true","fetch_graph":"https://pith.science/api/pith-number/TML35DEJCHHPGRAL2JBKT4MIWW/graph.json","fetch_events":"https://pith.science/api/pith-number/TML35DEJCHHPGRAL2JBKT4MIWW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW/action/storage_attestation","attest_author":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW/action/author_attestation","sign_citation":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW/action/citation_signature","submit_replication":"https://pith.science/pith/TML35DEJCHHPGRAL2JBKT4MIWW/action/replication_record"}},"created_at":"2026-05-18T04:08:44.487356+00:00","updated_at":"2026-05-18T04:08:44.487356+00:00"}