{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:KQJZ7FAMUWOTDEJSLTOSOJ27XL","short_pith_number":"pith:KQJZ7FAM","schema_version":"1.0","canonical_sha256":"54139f940ca59d3191325cdd27275fbac25f362c5faf87890973bb65e080db0e","source":{"kind":"arxiv","id":"2601.18967","version":2},"attestation_state":"computed","paper":{"title":"Classical emergence of the quantum-backreacted BTZ black hole from exponential electrodynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Efra\\'in Rojas, Jos\\'e Joaqu\\'in Su\\'arez-Garibay, Julio A. M\\'endez-Zavaleta","submitted_at":"2026-01-26T21:09:45Z","abstract_excerpt":"In this work, we revisit a recently reported generalization of the Ba\\~nados-Teitelboim-Zanelli black hole arising in New Massive Gravity sourced by the quantum fluctuations of scalar matter, now examined through the lens of a purely classical framework. We show that the same geometry, distinguished by its logarithmic asymptotic structure, emerges as the unique static solution of Einstein gravity coupled to an exponential nonlinear electrodynamics. We trace the origin of this correspondence and prove that this geometry belongs to a unique class of metrics constituting the intersection of the m"},"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":"2601.18967","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2026-01-26T21:09:45Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"a57dd151e90ef9d301802f8d349942e89819496f04adbcacd38d56adb49d7599","abstract_canon_sha256":"bcb074749ce79a5af0d42621c305eaad6c9375980d3866f8f93e193fdc242fcc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-08-19T00:26:21.319437Z","signature_b64":"Dlp4b72lEiPWmOAykVWmD8km+/bZxxJp/bempjSn/L7YZdGo/9DraoCK7PWCGZoqiVGGPfDKlKQn1r5cUTR4Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"54139f940ca59d3191325cdd27275fbac25f362c5faf87890973bb65e080db0e","last_reissued_at":"2026-08-19T00:26:21.316761Z","signature_status":"signed_v1","first_computed_at":"2026-08-19T00:26:21.316761Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Classical emergence of the quantum-backreacted BTZ black hole from exponential electrodynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Efra\\'in Rojas, Jos\\'e Joaqu\\'in Su\\'arez-Garibay, Julio A. M\\'endez-Zavaleta","submitted_at":"2026-01-26T21:09:45Z","abstract_excerpt":"In this work, we revisit a recently reported generalization of the Ba\\~nados-Teitelboim-Zanelli black hole arising in New Massive Gravity sourced by the quantum fluctuations of scalar matter, now examined through the lens of a purely classical framework. We show that the same geometry, distinguished by its logarithmic asymptotic structure, emerges as the unique static solution of Einstein gravity coupled to an exponential nonlinear electrodynamics. We trace the origin of this correspondence and prove that this geometry belongs to a unique class of metrics constituting the intersection of the m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2601.18967","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/2601.18967/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":"2601.18967","created_at":"2026-08-19T00:26:21.317620+00:00"},{"alias_kind":"arxiv_version","alias_value":"2601.18967v2","created_at":"2026-08-19T00:26:21.317620+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2601.18967","created_at":"2026-08-19T00:26:21.317620+00:00"},{"alias_kind":"pith_short_12","alias_value":"KQJZ7FAMUWOT","created_at":"2026-08-19T00:26:21.317620+00:00"},{"alias_kind":"pith_short_16","alias_value":"KQJZ7FAMUWOTDEJS","created_at":"2026-08-19T00:26:21.317620+00:00"},{"alias_kind":"pith_short_8","alias_value":"KQJZ7FAM","created_at":"2026-08-19T00:26:21.317620+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2603.08971","citing_title":"New Construction of Black Hole Solution in Non-Commutative Geometry and Their Thermodynamic Properties","ref_index":96,"is_internal_anchor":true},{"citing_arxiv_id":"2604.16545","citing_title":"Energy conditions in static, spherically symmetric spacetimes and effective geometries","ref_index":95,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL","json":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL.json","graph_json":"https://pith.science/api/pith-number/KQJZ7FAMUWOTDEJSLTOSOJ27XL/graph.json","events_json":"https://pith.science/api/pith-number/KQJZ7FAMUWOTDEJSLTOSOJ27XL/events.json","paper":"https://pith.science/paper/KQJZ7FAM"},"agent_actions":{"view_html":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL","download_json":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL.json","view_paper":"https://pith.science/paper/KQJZ7FAM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2601.18967&json=true","fetch_graph":"https://pith.science/api/pith-number/KQJZ7FAMUWOTDEJSLTOSOJ27XL/graph.json","fetch_events":"https://pith.science/api/pith-number/KQJZ7FAMUWOTDEJSLTOSOJ27XL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL/action/storage_attestation","attest_author":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL/action/author_attestation","sign_citation":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL/action/citation_signature","submit_replication":"https://pith.science/pith/KQJZ7FAMUWOTDEJSLTOSOJ27XL/action/replication_record"}},"created_at":"2026-08-19T00:26:21.317620+00:00","updated_at":"2026-08-19T00:26:21.317620+00:00"}