{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:WWMCL4JCTUMOKLRJDYUPYQU56T","short_pith_number":"pith:WWMCL4JC","schema_version":"1.0","canonical_sha256":"b59825f1229d18e52e291e28fc429df4ec1d0e449d742e4fe635be0cf050a7ea","source":{"kind":"arxiv","id":"1711.01151","version":2},"attestation_state":"computed","paper":{"title":"Reentrant phase transition of Born-Infeld-AdS black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ahmad Sheykhi, Amin Dehyadegari","submitted_at":"2017-10-30T18:27:40Z","abstract_excerpt":"We investigate thermodynamic phase structure and critical behaviour of Born-Infeld (BI) black holes in an anti-de Sitter (AdS) space, where the charge of the system can vary and the cosmological constant (pressure) is fixed. We find that the BI parameter crucially affects the temperature of the black hole when the horizon radius, $r_{+}$, is small. We observe that depending on the value of the nonlinear parameter, $\\beta $, BI-AdS black hole may be identified as RN black hole for $Q\\geq Q_{m}$, and Schwarzschild-like black hole for $Q<Q_{m}$, where $Q_{m}=1/\\left(8\\pi \\beta \\right) $ is the \\t"},"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":"1711.01151","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2017-10-30T18:27:40Z","cross_cats_sorted":[],"title_canon_sha256":"098ecfaf8ef36f42b46bfd4771d811a6f37d4dbfc8bd0644d38156fd12a4d509","abstract_canon_sha256":"c4dd409cb98fa8acbc3834dbd342ec3b2be869b595c79dea3778c9aa7d86eb6d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:06.827684Z","signature_b64":"dz18Ol4dKVM6pk6rXDjzKllxYS+/sNxthFgh+dw0+B+tEfxtWm2+CG3P3mbbP7gr8j80lKF0g9r0AnsO+wNwDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b59825f1229d18e52e291e28fc429df4ec1d0e449d742e4fe635be0cf050a7ea","last_reissued_at":"2026-05-18T00:11:06.826938Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:06.826938Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reentrant phase transition of Born-Infeld-AdS black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ahmad Sheykhi, Amin Dehyadegari","submitted_at":"2017-10-30T18:27:40Z","abstract_excerpt":"We investigate thermodynamic phase structure and critical behaviour of Born-Infeld (BI) black holes in an anti-de Sitter (AdS) space, where the charge of the system can vary and the cosmological constant (pressure) is fixed. We find that the BI parameter crucially affects the temperature of the black hole when the horizon radius, $r_{+}$, is small. We observe that depending on the value of the nonlinear parameter, $\\beta $, BI-AdS black hole may be identified as RN black hole for $Q\\geq Q_{m}$, and Schwarzschild-like black hole for $Q<Q_{m}$, where $Q_{m}=1/\\left(8\\pi \\beta \\right) $ is the \\t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.01151","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":""},"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":"1711.01151","created_at":"2026-05-18T00:11:06.827057+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.01151v2","created_at":"2026-05-18T00:11:06.827057+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.01151","created_at":"2026-05-18T00:11:06.827057+00:00"},{"alias_kind":"pith_short_12","alias_value":"WWMCL4JCTUMO","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_16","alias_value":"WWMCL4JCTUMOKLRJ","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_8","alias_value":"WWMCL4JC","created_at":"2026-05-18T12:31:53.515858+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.29101","citing_title":"Quasi-normal modes as probes of black hole reentrant phase transitions","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T","json":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T.json","graph_json":"https://pith.science/api/pith-number/WWMCL4JCTUMOKLRJDYUPYQU56T/graph.json","events_json":"https://pith.science/api/pith-number/WWMCL4JCTUMOKLRJDYUPYQU56T/events.json","paper":"https://pith.science/paper/WWMCL4JC"},"agent_actions":{"view_html":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T","download_json":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T.json","view_paper":"https://pith.science/paper/WWMCL4JC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.01151&json=true","fetch_graph":"https://pith.science/api/pith-number/WWMCL4JCTUMOKLRJDYUPYQU56T/graph.json","fetch_events":"https://pith.science/api/pith-number/WWMCL4JCTUMOKLRJDYUPYQU56T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T/action/storage_attestation","attest_author":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T/action/author_attestation","sign_citation":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T/action/citation_signature","submit_replication":"https://pith.science/pith/WWMCL4JCTUMOKLRJDYUPYQU56T/action/replication_record"}},"created_at":"2026-05-18T00:11:06.827057+00:00","updated_at":"2026-05-18T00:11:06.827057+00:00"}