{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:IQHQN4VM6I4KODMBE777ZOVLLR","short_pith_number":"pith:IQHQN4VM","schema_version":"1.0","canonical_sha256":"440f06f2acf238a70d8127fffcbaab5c42a63d471eabcf4f02906822d2b57828","source":{"kind":"arxiv","id":"2009.05904","version":3},"attestation_state":"computed","paper":{"title":"Thermodynamics of the Euler-Heisenberg-AdS black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Daniela Magos, Nora Bret\\'on","submitted_at":"2020-09-13T03:15:16Z","abstract_excerpt":"We generalize the solution to the Euler-Heisenberg (EH) theory coupled to gravity that represents a nonlinearly charged static black hole (BH) introducing the cosmological constant; the obtained solution is characterized by four parameters: mass $M$, electric charge $Q$, cosmological constant $\\Lambda$ (positive or negative) and the Euler-Heisenberg theory parameter $a$. Then we briefly analyze some BH features like horizons, electromagnetic field and geodesics. We mainly focus on its thermodynamic properties in the extended space where the anti-de Sitter parameter is interpreted as the pressu"},"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":"2009.05904","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2020-09-13T03:15:16Z","cross_cats_sorted":[],"title_canon_sha256":"f4bf262e9f550866ecbb59229a3f5aa18426857740ece3c3a2f4147c7d315864","abstract_canon_sha256":"193f5412e6c74af7dadf2ccf11c9ce92d9a8b0d13ee886e611ea599c794467a7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:40:44.637753Z","signature_b64":"1PX5r5dPER93adVLcD48D6A4GIu6xgnRYUzw4UL1S/qerMHwIvpMkZIGScA6CKyQtsUGA3g+Di1zAb9zwv58CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"440f06f2acf238a70d8127fffcbaab5c42a63d471eabcf4f02906822d2b57828","last_reissued_at":"2026-07-05T01:40:44.637306Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:40:44.637306Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermodynamics of the Euler-Heisenberg-AdS black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Daniela Magos, Nora Bret\\'on","submitted_at":"2020-09-13T03:15:16Z","abstract_excerpt":"We generalize the solution to the Euler-Heisenberg (EH) theory coupled to gravity that represents a nonlinearly charged static black hole (BH) introducing the cosmological constant; the obtained solution is characterized by four parameters: mass $M$, electric charge $Q$, cosmological constant $\\Lambda$ (positive or negative) and the Euler-Heisenberg theory parameter $a$. Then we briefly analyze some BH features like horizons, electromagnetic field and geodesics. We mainly focus on its thermodynamic properties in the extended space where the anti-de Sitter parameter is interpreted as the pressu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.05904","kind":"arxiv","version":3},"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/2009.05904/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":"2009.05904","created_at":"2026-07-05T01:40:44.637378+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.05904v3","created_at":"2026-07-05T01:40:44.637378+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.05904","created_at":"2026-07-05T01:40:44.637378+00:00"},{"alias_kind":"pith_short_12","alias_value":"IQHQN4VM6I4K","created_at":"2026-07-05T01:40:44.637378+00:00"},{"alias_kind":"pith_short_16","alias_value":"IQHQN4VM6I4KODMB","created_at":"2026-07-05T01:40:44.637378+00:00"},{"alias_kind":"pith_short_8","alias_value":"IQHQN4VM","created_at":"2026-07-05T01:40:44.637378+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.21332","citing_title":"Thermal Stability and QNMs of a Hairy Black Hole in the Presence of a Monopole Field","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2606.03842","citing_title":"Scattering and Hawking Radiation from Einstein--Euler--Heisenberg--de Sitter Black Holes","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11866","citing_title":"Equatorial periodic orbits and gravitational wave signatures in Euler-Heisenberg black holes surrounded by perfect fluid dark matter","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14213","citing_title":"On Computational CUDA Studies of Black Hole Shadows","ref_index":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR","json":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR.json","graph_json":"https://pith.science/api/pith-number/IQHQN4VM6I4KODMBE777ZOVLLR/graph.json","events_json":"https://pith.science/api/pith-number/IQHQN4VM6I4KODMBE777ZOVLLR/events.json","paper":"https://pith.science/paper/IQHQN4VM"},"agent_actions":{"view_html":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR","download_json":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR.json","view_paper":"https://pith.science/paper/IQHQN4VM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.05904&json=true","fetch_graph":"https://pith.science/api/pith-number/IQHQN4VM6I4KODMBE777ZOVLLR/graph.json","fetch_events":"https://pith.science/api/pith-number/IQHQN4VM6I4KODMBE777ZOVLLR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR/action/storage_attestation","attest_author":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR/action/author_attestation","sign_citation":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR/action/citation_signature","submit_replication":"https://pith.science/pith/IQHQN4VM6I4KODMBE777ZOVLLR/action/replication_record"}},"created_at":"2026-07-05T01:40:44.637378+00:00","updated_at":"2026-07-05T01:40:44.637378+00:00"}