{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:QEUT3ZUTHXMLULTKY5OIKYOE77","short_pith_number":"pith:QEUT3ZUT","schema_version":"1.0","canonical_sha256":"81293de6933dd8ba2e6ac75c8561c4fffd05b31b80d28ae48828fda338421e29","source":{"kind":"arxiv","id":"2302.07799","version":2},"attestation_state":"computed","paper":{"title":"Quantum fractionary cosmology: K-essence theory","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"J. Juan Rosales, J. Socorro","submitted_at":"2023-02-15T17:32:46Z","abstract_excerpt":"Using a particular form of the quantum K-essence scalar field, we show that in the quantum formalism, a fractional differential equation in the scalar field variable, for some epochs in the Friedmann-Lema\\^itre-Robertson-Walker (FLRW) model (radiation and inflation-like epochs, for example), appears naturally. In the classical analysis, the kinetic energy of scalar fields can falsify the standard matter in the sense that we obtain the time behavior for the scale factor in all scenarios of our Universe by using the Hamiltonian formalism, where the results are analogous to those obtained by an a"},"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":"2302.07799","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"gr-qc","submitted_at":"2023-02-15T17:32:46Z","cross_cats_sorted":[],"title_canon_sha256":"7d5ab78d0805d57ea74c8def6da67f303f7de723f268bd6fcc8a8bd780159ee5","abstract_canon_sha256":"d8970bc7699ba2cf894b2ed8813496b12302de8ca45c3e4f6451ae8fb4c9eb83"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:00:36.414827Z","signature_b64":"hkGQ9VUM89lYbLH1nBJNhD++nazIUGk6MoANjwmht4JlnvOqbtf9OuBQlIFQeJgY9I9CDuXIUFFtsxSnEIq2CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"81293de6933dd8ba2e6ac75c8561c4fffd05b31b80d28ae48828fda338421e29","last_reissued_at":"2026-07-05T06:00:36.414384Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:00:36.414384Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum fractionary cosmology: K-essence theory","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"J. Juan Rosales, J. Socorro","submitted_at":"2023-02-15T17:32:46Z","abstract_excerpt":"Using a particular form of the quantum K-essence scalar field, we show that in the quantum formalism, a fractional differential equation in the scalar field variable, for some epochs in the Friedmann-Lema\\^itre-Robertson-Walker (FLRW) model (radiation and inflation-like epochs, for example), appears naturally. In the classical analysis, the kinetic energy of scalar fields can falsify the standard matter in the sense that we obtain the time behavior for the scale factor in all scenarios of our Universe by using the Hamiltonian formalism, where the results are analogous to those obtained by an a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.07799","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/2302.07799/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":"2302.07799","created_at":"2026-07-05T06:00:36.414442+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.07799v2","created_at":"2026-07-05T06:00:36.414442+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.07799","created_at":"2026-07-05T06:00:36.414442+00:00"},{"alias_kind":"pith_short_12","alias_value":"QEUT3ZUTHXML","created_at":"2026-07-05T06:00:36.414442+00:00"},{"alias_kind":"pith_short_16","alias_value":"QEUT3ZUTHXMLULTK","created_at":"2026-07-05T06:00:36.414442+00:00"},{"alias_kind":"pith_short_8","alias_value":"QEUT3ZUT","created_at":"2026-07-05T06:00:36.414442+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.01244","citing_title":"Fractional entropy of the Brown-Kucha\\v{r} dust in fractional anti-de Sitter quantum gravity","ref_index":29,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77","json":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77.json","graph_json":"https://pith.science/api/pith-number/QEUT3ZUTHXMLULTKY5OIKYOE77/graph.json","events_json":"https://pith.science/api/pith-number/QEUT3ZUTHXMLULTKY5OIKYOE77/events.json","paper":"https://pith.science/paper/QEUT3ZUT"},"agent_actions":{"view_html":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77","download_json":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77.json","view_paper":"https://pith.science/paper/QEUT3ZUT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.07799&json=true","fetch_graph":"https://pith.science/api/pith-number/QEUT3ZUTHXMLULTKY5OIKYOE77/graph.json","fetch_events":"https://pith.science/api/pith-number/QEUT3ZUTHXMLULTKY5OIKYOE77/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77/action/storage_attestation","attest_author":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77/action/author_attestation","sign_citation":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77/action/citation_signature","submit_replication":"https://pith.science/pith/QEUT3ZUTHXMLULTKY5OIKYOE77/action/replication_record"}},"created_at":"2026-07-05T06:00:36.414442+00:00","updated_at":"2026-07-05T06:00:36.414442+00:00"}