{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:5YFS66RX2NSFBJNPNBFWCTWBKZ","short_pith_number":"pith:5YFS66RX","schema_version":"1.0","canonical_sha256":"ee0b2f7a37d36450a5af684b614ec1566c5d154167d10152847428c9d0c5c242","source":{"kind":"arxiv","id":"2602.12077","version":2},"attestation_state":"computed","paper":{"title":"Cosmographic Connection Between Cosmological And Planck Scales: The Barrow-Tsallis Entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"D. A. Yerokhin, V.V. Yanovsky, Yu. L. Bolotin","submitted_at":"2026-02-12T15:36:21Z","abstract_excerpt":"One of the fundamental challenges of quantum gravity is to understand how the microscopic degrees of freedom of the cosmological horizon shape the evolution of the Universe. One possible approach to this problem is based on the Barrow--Tsallis entropy. This entropy accounts for both quantum gravitational effects and the nonextensive effects inherent in any long-range interaction. Using a general method we developed for finding the parameters of cosmological models, we discovered a relationship between the parameter describing the microscopic structure of quantum foam and the parameter associat"},"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":"2602.12077","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2026-02-12T15:36:21Z","cross_cats_sorted":["astro-ph.CO","hep-ph","hep-th"],"title_canon_sha256":"27ef419b785cfdb29c874201e1c7f6f468e81fbe38f0f32dd091af4eaa0299a5","abstract_canon_sha256":"9473ec20969e8551fc1c22fc445d22c16ffb406e9cc3a01268303c0b60200985"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-20T00:03:05.684955Z","signature_b64":"FOAIyDj9E9JxCk8gYRqJ2dNRZ54OzePUhEX8pVaU3xqcl92lBo322HmcI10QZbddLHPAyoYQMCtQq2kLZ5vuAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ee0b2f7a37d36450a5af684b614ec1566c5d154167d10152847428c9d0c5c242","last_reissued_at":"2026-05-20T00:03:05.684155Z","signature_status":"signed_v1","first_computed_at":"2026-05-20T00:03:05.684155Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmographic Connection Between Cosmological And Planck Scales: The Barrow-Tsallis Entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"D. A. Yerokhin, V.V. Yanovsky, Yu. L. Bolotin","submitted_at":"2026-02-12T15:36:21Z","abstract_excerpt":"One of the fundamental challenges of quantum gravity is to understand how the microscopic degrees of freedom of the cosmological horizon shape the evolution of the Universe. One possible approach to this problem is based on the Barrow--Tsallis entropy. This entropy accounts for both quantum gravitational effects and the nonextensive effects inherent in any long-range interaction. Using a general method we developed for finding the parameters of cosmological models, we discovered a relationship between the parameter describing the microscopic structure of quantum foam and the parameter associat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2602.12077","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/2602.12077/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":"2602.12077","created_at":"2026-05-20T00:03:05.684295+00:00"},{"alias_kind":"arxiv_version","alias_value":"2602.12077v2","created_at":"2026-05-20T00:03:05.684295+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2602.12077","created_at":"2026-05-20T00:03:05.684295+00:00"},{"alias_kind":"pith_short_12","alias_value":"5YFS66RX2NSF","created_at":"2026-05-20T00:03:05.684295+00:00"},{"alias_kind":"pith_short_16","alias_value":"5YFS66RX2NSFBJNP","created_at":"2026-05-20T00:03:05.684295+00:00"},{"alias_kind":"pith_short_8","alias_value":"5YFS66RX","created_at":"2026-05-20T00:03:05.684295+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2602.12077","citing_title":"Cosmographic Connection Between Cosmological And Planck Scales: The Barrow-Tsallis Entropy","ref_index":1,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ","json":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ.json","graph_json":"https://pith.science/api/pith-number/5YFS66RX2NSFBJNPNBFWCTWBKZ/graph.json","events_json":"https://pith.science/api/pith-number/5YFS66RX2NSFBJNPNBFWCTWBKZ/events.json","paper":"https://pith.science/paper/5YFS66RX"},"agent_actions":{"view_html":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ","download_json":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ.json","view_paper":"https://pith.science/paper/5YFS66RX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2602.12077&json=true","fetch_graph":"https://pith.science/api/pith-number/5YFS66RX2NSFBJNPNBFWCTWBKZ/graph.json","fetch_events":"https://pith.science/api/pith-number/5YFS66RX2NSFBJNPNBFWCTWBKZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ/action/storage_attestation","attest_author":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ/action/author_attestation","sign_citation":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ/action/citation_signature","submit_replication":"https://pith.science/pith/5YFS66RX2NSFBJNPNBFWCTWBKZ/action/replication_record"}},"created_at":"2026-05-20T00:03:05.684295+00:00","updated_at":"2026-05-20T00:03:05.684295+00:00"}