{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:ENMB5MZV7PIVVIN3ASQQWKNFDC","short_pith_number":"pith:ENMB5MZV","schema_version":"1.0","canonical_sha256":"23581eb335fbd15aa1bb04a10b29a5189458da693c460210ff1484429476bedc","source":{"kind":"arxiv","id":"2605.26129","version":1},"attestation_state":"computed","paper":{"title":"Unified Cosmological Scenario in Holographic $f(Q)$ gravity: From Inflation to Late-Time Acceleration","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"Can Aktas, Moli Ghosh, Surajit Chattopadhyay","submitted_at":"2026-05-20T07:28:03Z","abstract_excerpt":"The present paper reports a study of a unified cosmological scenario in the framework of holographic f(Q) gravity, where, in a single theoretical setup, both the early inflationary epoch and the late-time accelerated epoch are studied. Considering f(Q) = $\\zeta Q^n$, we reconstruct the Hubble parameter in the presence of Barrow holographic fluid and study the inflationary behaviour through the slow-roll parameters, scalar spectral index $n_s$, and tensor-to-scalar ratio r. The obtained inflationary predictions are found to be consistent with the latest Planck 2018 observational constraints, wi"},"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":"2605.26129","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"physics.gen-ph","submitted_at":"2026-05-20T07:28:03Z","cross_cats_sorted":[],"title_canon_sha256":"843e4034ff7b6532d3760b0213d02b22a7315606a369ce8a03d05be05eb2d09a","abstract_canon_sha256":"647bb5c0a5646f18e5fbf827bcfc1aa609fdc0337d5c1ecbb5b05f5297ebaea9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-27T00:04:25.176245Z","signature_b64":"MwwYH9thepMgzHOQAuQ0E6s8Quufq/XHzj8+SDQ/2FpV5dMFulDX59HJd7Bwc/Tbsl3NzsFf2GtCrfbZUvUvAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23581eb335fbd15aa1bb04a10b29a5189458da693c460210ff1484429476bedc","last_reissued_at":"2026-05-27T00:04:25.175518Z","signature_status":"signed_v1","first_computed_at":"2026-05-27T00:04:25.175518Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Unified Cosmological Scenario in Holographic $f(Q)$ gravity: From Inflation to Late-Time Acceleration","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"physics.gen-ph","authors_text":"Can Aktas, Moli Ghosh, Surajit Chattopadhyay","submitted_at":"2026-05-20T07:28:03Z","abstract_excerpt":"The present paper reports a study of a unified cosmological scenario in the framework of holographic f(Q) gravity, where, in a single theoretical setup, both the early inflationary epoch and the late-time accelerated epoch are studied. Considering f(Q) = $\\zeta Q^n$, we reconstruct the Hubble parameter in the presence of Barrow holographic fluid and study the inflationary behaviour through the slow-roll parameters, scalar spectral index $n_s$, and tensor-to-scalar ratio r. The obtained inflationary predictions are found to be consistent with the latest Planck 2018 observational constraints, wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.26129","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/2605.26129/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":"2605.26129","created_at":"2026-05-27T00:04:25.175674+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.26129v1","created_at":"2026-05-27T00:04:25.175674+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.26129","created_at":"2026-05-27T00:04:25.175674+00:00"},{"alias_kind":"pith_short_12","alias_value":"ENMB5MZV7PIV","created_at":"2026-05-27T00:04:25.175674+00:00"},{"alias_kind":"pith_short_16","alias_value":"ENMB5MZV7PIVVIN3","created_at":"2026-05-27T00:04:25.175674+00:00"},{"alias_kind":"pith_short_8","alias_value":"ENMB5MZV","created_at":"2026-05-27T00:04:25.175674+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/ENMB5MZV7PIVVIN3ASQQWKNFDC","json":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC.json","graph_json":"https://pith.science/api/pith-number/ENMB5MZV7PIVVIN3ASQQWKNFDC/graph.json","events_json":"https://pith.science/api/pith-number/ENMB5MZV7PIVVIN3ASQQWKNFDC/events.json","paper":"https://pith.science/paper/ENMB5MZV"},"agent_actions":{"view_html":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC","download_json":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC.json","view_paper":"https://pith.science/paper/ENMB5MZV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.26129&json=true","fetch_graph":"https://pith.science/api/pith-number/ENMB5MZV7PIVVIN3ASQQWKNFDC/graph.json","fetch_events":"https://pith.science/api/pith-number/ENMB5MZV7PIVVIN3ASQQWKNFDC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC/action/storage_attestation","attest_author":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC/action/author_attestation","sign_citation":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC/action/citation_signature","submit_replication":"https://pith.science/pith/ENMB5MZV7PIVVIN3ASQQWKNFDC/action/replication_record"}},"created_at":"2026-05-27T00:04:25.175674+00:00","updated_at":"2026-05-27T00:04:25.175674+00:00"}