{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:32V4XXYL3FFIXS4A4HIO3SQGR3","short_pith_number":"pith:32V4XXYL","schema_version":"1.0","canonical_sha256":"deabcbdf0bd94a8bcb80e1d0edca068ecf00d5e9797cc56457cea8b432abdd45","source":{"kind":"arxiv","id":"2108.12366","version":2},"attestation_state":"computed","paper":{"title":"Modified cosmology through Kaniadakis horizon entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Andreas Lymperis, Emmanuel N. Saridakis, Spyros Basilakos","submitted_at":"2021-08-27T15:58:31Z","abstract_excerpt":"We apply the gravity-thermodynamics conjecture, namely the first law of thermodynamics on the Universe horizon, but using the generalized Kaniadakis entropy instead of the standard Bekenstein-Hawking one. The former is a one-parameter generalization of the classical Boltzmann-Gibbs-Shannon entropy, arising from a coherent and self-consistent relativistic statistical theory. We obtain new modified cosmological scenarios, namely modified Friedmann equations, which contain new extra terms that constitute an effective dark energy sector depending on the single model Kaniadakis parameter $K$. We in"},"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":"2108.12366","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-08-27T15:58:31Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"d3937078e22505a8afdd3af0d460a6d2812810a1612c4695f5656bfeb5463846","abstract_canon_sha256":"52609a8aa2565c4ffd391e0ea493637ea1fb36724b5053a36fee1b6b4838a64a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:37:45.350930Z","signature_b64":"HOt3Uxow5EbXxCjZJefC5NAFvaUVMYXonBrWZzqAwwt75S51Zh9oTxQBnNYlEBcomCbrDU4AlbJKLKs057WeCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"deabcbdf0bd94a8bcb80e1d0edca068ecf00d5e9797cc56457cea8b432abdd45","last_reissued_at":"2026-07-05T03:37:45.350445Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:37:45.350445Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modified cosmology through Kaniadakis horizon entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"gr-qc","authors_text":"Andreas Lymperis, Emmanuel N. Saridakis, Spyros Basilakos","submitted_at":"2021-08-27T15:58:31Z","abstract_excerpt":"We apply the gravity-thermodynamics conjecture, namely the first law of thermodynamics on the Universe horizon, but using the generalized Kaniadakis entropy instead of the standard Bekenstein-Hawking one. The former is a one-parameter generalization of the classical Boltzmann-Gibbs-Shannon entropy, arising from a coherent and self-consistent relativistic statistical theory. We obtain new modified cosmological scenarios, namely modified Friedmann equations, which contain new extra terms that constitute an effective dark energy sector depending on the single model Kaniadakis parameter $K$. We in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2108.12366","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/2108.12366/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":"2108.12366","created_at":"2026-07-05T03:37:45.350503+00:00"},{"alias_kind":"arxiv_version","alias_value":"2108.12366v2","created_at":"2026-07-05T03:37:45.350503+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2108.12366","created_at":"2026-07-05T03:37:45.350503+00:00"},{"alias_kind":"pith_short_12","alias_value":"32V4XXYL3FFI","created_at":"2026-07-05T03:37:45.350503+00:00"},{"alias_kind":"pith_short_16","alias_value":"32V4XXYL3FFIXS4A","created_at":"2026-07-05T03:37:45.350503+00:00"},{"alias_kind":"pith_short_8","alias_value":"32V4XXYL","created_at":"2026-07-05T03:37:45.350503+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.23990","citing_title":"Hamilton-Jacobi Approach to Inflationary Scenarios through Extended Entropies: An Observational Perspective","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2603.03568","citing_title":"Observational constraints on Luciano-Saridakis entropic cosmology","ref_index":51,"is_internal_anchor":false},{"citing_arxiv_id":"2605.21050","citing_title":"Constraints on Kaniadakis Cosmology from Starobinsky Inflation and Primordial Tensor Perturbations","ref_index":22,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18070","citing_title":"Slow-roll inflation in (dual) Kaniadakis cosmology","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3","json":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3.json","graph_json":"https://pith.science/api/pith-number/32V4XXYL3FFIXS4A4HIO3SQGR3/graph.json","events_json":"https://pith.science/api/pith-number/32V4XXYL3FFIXS4A4HIO3SQGR3/events.json","paper":"https://pith.science/paper/32V4XXYL"},"agent_actions":{"view_html":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3","download_json":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3.json","view_paper":"https://pith.science/paper/32V4XXYL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2108.12366&json=true","fetch_graph":"https://pith.science/api/pith-number/32V4XXYL3FFIXS4A4HIO3SQGR3/graph.json","fetch_events":"https://pith.science/api/pith-number/32V4XXYL3FFIXS4A4HIO3SQGR3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3/action/storage_attestation","attest_author":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3/action/author_attestation","sign_citation":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3/action/citation_signature","submit_replication":"https://pith.science/pith/32V4XXYL3FFIXS4A4HIO3SQGR3/action/replication_record"}},"created_at":"2026-07-05T03:37:45.350503+00:00","updated_at":"2026-07-05T03:37:45.350503+00:00"}