{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:DR6TOX5O5GN2FDXZSQVULU4I4O","short_pith_number":"pith:DR6TOX5O","schema_version":"1.0","canonical_sha256":"1c7d375faee99ba28ef9942b45d388e3ba7f9e57a9d34f2e6d00a8e723011a17","source":{"kind":"arxiv","id":"hep-th/9602105","version":1},"attestation_state":"computed","paper":{"title":"On One-loop Quantum Corrections to the Thermodynamics of Charged Black Holes","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"S.N.Solodukhin, V.P.Frolov, W. Israel","submitted_at":"1996-02-19T21:12:56Z","abstract_excerpt":"Quantum corrections are studied for a charged black hole in a two-dimensional model obtained by spherisymmetric reduction of the 4D Einstein-Maxwell theory. The classical (tree-level) thermodynamics is re-formulated in the framework of the off-shell approach, considering systems at arbitrary temperature. This implies a conical singularity at the horizon and modifies the gravitational action by terms defined on the horizon. A consistent variational procedure for the action functional is formulated. It is shown that the free energy reaches an extremum on the regular manifold with $T=T_H$. The on"},"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":"hep-th/9602105","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1996-02-19T21:12:56Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"97408f298f4571c35a1c800fe58b03c92d13b57596dce0f8095e282b7a890356","abstract_canon_sha256":"139d66b8306c17b08cbe11e3b2de81410cf56a7d75450e96ada54cf0da100b6e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:35:16.572080Z","signature_b64":"K8H5d3v14ura9QAYnYhTByOTqw5AJvrWxenUprtGylzrCmAdwy24KdmO5YZFRLpOc6yyimLtJthFzP2j93iAAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1c7d375faee99ba28ef9942b45d388e3ba7f9e57a9d34f2e6d00a8e723011a17","last_reissued_at":"2026-05-18T04:35:16.571599Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:35:16.571599Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On One-loop Quantum Corrections to the Thermodynamics of Charged Black Holes","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"S.N.Solodukhin, V.P.Frolov, W. Israel","submitted_at":"1996-02-19T21:12:56Z","abstract_excerpt":"Quantum corrections are studied for a charged black hole in a two-dimensional model obtained by spherisymmetric reduction of the 4D Einstein-Maxwell theory. The classical (tree-level) thermodynamics is re-formulated in the framework of the off-shell approach, considering systems at arbitrary temperature. This implies a conical singularity at the horizon and modifies the gravitational action by terms defined on the horizon. A consistent variational procedure for the action functional is formulated. It is shown that the free energy reaches an extremum on the regular manifold with $T=T_H$. The on"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9602105","kind":"arxiv","version":1},"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":"hep-th/9602105","created_at":"2026-05-18T04:35:16.571668+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9602105v1","created_at":"2026-05-18T04:35:16.571668+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9602105","created_at":"2026-05-18T04:35:16.571668+00:00"},{"alias_kind":"pith_short_12","alias_value":"DR6TOX5O5GN2","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_16","alias_value":"DR6TOX5O5GN2FDXZ","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_8","alias_value":"DR6TOX5O","created_at":"2026-05-18T12:25:47.700082+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.09946","citing_title":"Collapse Scenario and Final State of Evaporation for Schwarzschild Black Hole in Dimensionally-Reduced Model of Dilaton Gravity","ref_index":11,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O","json":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O.json","graph_json":"https://pith.science/api/pith-number/DR6TOX5O5GN2FDXZSQVULU4I4O/graph.json","events_json":"https://pith.science/api/pith-number/DR6TOX5O5GN2FDXZSQVULU4I4O/events.json","paper":"https://pith.science/paper/DR6TOX5O"},"agent_actions":{"view_html":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O","download_json":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O.json","view_paper":"https://pith.science/paper/DR6TOX5O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9602105&json=true","fetch_graph":"https://pith.science/api/pith-number/DR6TOX5O5GN2FDXZSQVULU4I4O/graph.json","fetch_events":"https://pith.science/api/pith-number/DR6TOX5O5GN2FDXZSQVULU4I4O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O/action/storage_attestation","attest_author":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O/action/author_attestation","sign_citation":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O/action/citation_signature","submit_replication":"https://pith.science/pith/DR6TOX5O5GN2FDXZSQVULU4I4O/action/replication_record"}},"created_at":"2026-05-18T04:35:16.571668+00:00","updated_at":"2026-05-18T04:35:16.571668+00:00"}