{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:BNYPXT4RBUY5TPYSJY4NUMAOIZ","short_pith_number":"pith:BNYPXT4R","schema_version":"1.0","canonical_sha256":"0b70fbcf910d31d9bf124e38da300e4648b48c83cb40866aa977df30bbaf8288","source":{"kind":"arxiv","id":"2405.14799","version":4},"attestation_state":"computed","paper":{"title":"Exploring modified Kaniadakis entropy: MOND-related theory, the Bekenstein bound conjecture, and Hawking evaporation within the Landauer principle","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Cleber N. Costa, Gabriella V. Ambr\\'osio, Jorge Ananias Neto, Michelly S. Andrade, Paulo R. F. Alves, Ronaldo Thibes","submitted_at":"2024-05-23T17:07:20Z","abstract_excerpt":"We investigate the description of black-hole thermodynamics in terms of a recently proposed modified version for Kaniadakis entropy. We discuss the role of that proposal within the Modified Newtonian Dynamics (MOND) theory, a generalization of Newton's second law aimed at explaining galaxy rotation curves without resorting to dark matter. We posit a conjecture that the Kaniadakis entropy precisely describes the Bekenstein-Hawking black-hole entropy. Furthermore, we consider the Bekenstein bound conjecture which imposes an upper limit on the entropy of confined quantum systems. We analyze that "},"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":"2405.14799","kind":"arxiv","version":4},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-05-23T17:07:20Z","cross_cats_sorted":[],"title_canon_sha256":"50ed4f148d00ad20869eef0f5300f2569b9a173e1362d5fc923e9514ba7f3607","abstract_canon_sha256":"6609e75eb284d0a3aef60d6b69b9fe961ccd200ff615eb924c204746153b70a1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:27:49.046522Z","signature_b64":"p3RTARnyM77lSNl4l0zzAW8/BdmedHPIGRSNEqS3G7RkaatQtBauToFmC9gWeKaXQKYmTWWJmWw9OAc2eVSJCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b70fbcf910d31d9bf124e38da300e4648b48c83cb40866aa977df30bbaf8288","last_reissued_at":"2026-07-05T11:27:49.046033Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:27:49.046033Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring modified Kaniadakis entropy: MOND-related theory, the Bekenstein bound conjecture, and Hawking evaporation within the Landauer principle","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Cleber N. Costa, Gabriella V. Ambr\\'osio, Jorge Ananias Neto, Michelly S. Andrade, Paulo R. F. Alves, Ronaldo Thibes","submitted_at":"2024-05-23T17:07:20Z","abstract_excerpt":"We investigate the description of black-hole thermodynamics in terms of a recently proposed modified version for Kaniadakis entropy. We discuss the role of that proposal within the Modified Newtonian Dynamics (MOND) theory, a generalization of Newton's second law aimed at explaining galaxy rotation curves without resorting to dark matter. We posit a conjecture that the Kaniadakis entropy precisely describes the Bekenstein-Hawking black-hole entropy. Furthermore, we consider the Bekenstein bound conjecture which imposes an upper limit on the entropy of confined quantum systems. We analyze that "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.14799","kind":"arxiv","version":4},"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/2405.14799/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":"2405.14799","created_at":"2026-07-05T11:27:49.046086+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.14799v4","created_at":"2026-07-05T11:27:49.046086+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.14799","created_at":"2026-07-05T11:27:49.046086+00:00"},{"alias_kind":"pith_short_12","alias_value":"BNYPXT4RBUY5","created_at":"2026-07-05T11:27:49.046086+00:00"},{"alias_kind":"pith_short_16","alias_value":"BNYPXT4RBUY5TPYS","created_at":"2026-07-05T11:27:49.046086+00:00"},{"alias_kind":"pith_short_8","alias_value":"BNYPXT4R","created_at":"2026-07-05T11:27:49.046086+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.18070","citing_title":"Slow-roll inflation in (dual) Kaniadakis cosmology","ref_index":34,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ","json":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ.json","graph_json":"https://pith.science/api/pith-number/BNYPXT4RBUY5TPYSJY4NUMAOIZ/graph.json","events_json":"https://pith.science/api/pith-number/BNYPXT4RBUY5TPYSJY4NUMAOIZ/events.json","paper":"https://pith.science/paper/BNYPXT4R"},"agent_actions":{"view_html":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ","download_json":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ.json","view_paper":"https://pith.science/paper/BNYPXT4R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.14799&json=true","fetch_graph":"https://pith.science/api/pith-number/BNYPXT4RBUY5TPYSJY4NUMAOIZ/graph.json","fetch_events":"https://pith.science/api/pith-number/BNYPXT4RBUY5TPYSJY4NUMAOIZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ/action/storage_attestation","attest_author":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ/action/author_attestation","sign_citation":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ/action/citation_signature","submit_replication":"https://pith.science/pith/BNYPXT4RBUY5TPYSJY4NUMAOIZ/action/replication_record"}},"created_at":"2026-07-05T11:27:49.046086+00:00","updated_at":"2026-07-05T11:27:49.046086+00:00"}