{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:2NXDVFYBHONEK6LEZNA3FOY3JQ","short_pith_number":"pith:2NXDVFYB","schema_version":"1.0","canonical_sha256":"d36e3a97013b9a457964cb41b2bb1b4c35c3a213da19f592c880d3ceb4c0b339","source":{"kind":"arxiv","id":"2311.16527","version":1},"attestation_state":"computed","paper":{"title":"Reconstruction of symmteric teleparallel gravity with energy conditions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Allah Ditta, Anil Kumar Yadav, Hira Sohail, Irfan Mahmood, S. H. Shekh","submitted_at":"2023-11-28T05:13:33Z","abstract_excerpt":"This research investigates the impact of modified gravity on cosmic scales, focusing on $f(Q)$ cosmology. By applying energy conditions, the study reconstructs various $f(Q)$ models, considering an accelerating Universe, quintessence, and a cosmological constant $\\Lambda$. Using up-to-date observational data, including the Supernova Pantheon sample and cosmic chronometer data, Hubble constants $H_0$ are estimated as $70.37^{+0.84}_{-0.92}$ km/sec/Mpc (from $H(z)$ data) and $70.02^{+0.44}_{-0.25}$ km/sec/Mpc (from pantheon compilation of SN Ia data). The matter energy density parameter ($\\Omega"},"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":"2311.16527","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-11-28T05:13:33Z","cross_cats_sorted":[],"title_canon_sha256":"eb19c973c85e3dbdeb9924ac1ad0a69dfe16a0c16454598e3ec84afda89f10e5","abstract_canon_sha256":"be4458484e8fe62a4d679ad35125d985874bb4db67fb70503c065c7903f810c0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:47:24.370546Z","signature_b64":"5AmSHbQWc3u0prOywVjjJt3GlGyqJS8bY9pM0IcKNm/1ye5nRHlZz/q3wyC8rgBHrd8zGLBMOsXfZnT/9rgIBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d36e3a97013b9a457964cb41b2bb1b4c35c3a213da19f592c880d3ceb4c0b339","last_reissued_at":"2026-07-05T10:47:24.370054Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:47:24.370054Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reconstruction of symmteric teleparallel gravity with energy conditions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Allah Ditta, Anil Kumar Yadav, Hira Sohail, Irfan Mahmood, S. H. Shekh","submitted_at":"2023-11-28T05:13:33Z","abstract_excerpt":"This research investigates the impact of modified gravity on cosmic scales, focusing on $f(Q)$ cosmology. By applying energy conditions, the study reconstructs various $f(Q)$ models, considering an accelerating Universe, quintessence, and a cosmological constant $\\Lambda$. Using up-to-date observational data, including the Supernova Pantheon sample and cosmic chronometer data, Hubble constants $H_0$ are estimated as $70.37^{+0.84}_{-0.92}$ km/sec/Mpc (from $H(z)$ data) and $70.02^{+0.44}_{-0.25}$ km/sec/Mpc (from pantheon compilation of SN Ia data). The matter energy density parameter ($\\Omega"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.16527","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2311.16527/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":"2311.16527","created_at":"2026-07-05T10:47:24.370112+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.16527v1","created_at":"2026-07-05T10:47:24.370112+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.16527","created_at":"2026-07-05T10:47:24.370112+00:00"},{"alias_kind":"pith_short_12","alias_value":"2NXDVFYBHONE","created_at":"2026-07-05T10:47:24.370112+00:00"},{"alias_kind":"pith_short_16","alias_value":"2NXDVFYBHONEK6LE","created_at":"2026-07-05T10:47:24.370112+00:00"},{"alias_kind":"pith_short_8","alias_value":"2NXDVFYB","created_at":"2026-07-05T10:47:24.370112+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.07976","citing_title":"Dynamical Dark Energy or Modified Gravity? Signatures in Gravitational Wave Propagation","ref_index":43,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ","json":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ.json","graph_json":"https://pith.science/api/pith-number/2NXDVFYBHONEK6LEZNA3FOY3JQ/graph.json","events_json":"https://pith.science/api/pith-number/2NXDVFYBHONEK6LEZNA3FOY3JQ/events.json","paper":"https://pith.science/paper/2NXDVFYB"},"agent_actions":{"view_html":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ","download_json":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ.json","view_paper":"https://pith.science/paper/2NXDVFYB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.16527&json=true","fetch_graph":"https://pith.science/api/pith-number/2NXDVFYBHONEK6LEZNA3FOY3JQ/graph.json","fetch_events":"https://pith.science/api/pith-number/2NXDVFYBHONEK6LEZNA3FOY3JQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ/action/storage_attestation","attest_author":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ/action/author_attestation","sign_citation":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ/action/citation_signature","submit_replication":"https://pith.science/pith/2NXDVFYBHONEK6LEZNA3FOY3JQ/action/replication_record"}},"created_at":"2026-07-05T10:47:24.370112+00:00","updated_at":"2026-07-05T10:47:24.370112+00:00"}