{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1991:4ILKPS272LH5RVLWQ4DFXRJWUS","short_pith_number":"pith:4ILKPS27","schema_version":"1.0","canonical_sha256":"e216a7cb5fd2cfd8d57687065bc536a485aec5e5284c18b2081949907c13cc2b","source":{"kind":"arxiv","id":"hep-th/9108001","version":1},"attestation_state":"computed","paper":{"title":"Exact Black String Solutions in Three Dimensions","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gary T. Horowitz, James H. Horne","submitted_at":"1991-08-14T22:25:19Z","abstract_excerpt":"A family of exact conformal field theories is constructed which describe charged black strings in three dimensions. Unlike previous charged black hole or extended black hole solutions in string theory, the low energy spacetime metric has a regular inner horizon (in addition to the event horizon) and a timelike singularity. As the charge to mass ratio approaches unity, the event horizon remains but the singularity disappears."},"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/9108001","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1991-08-14T22:25:19Z","cross_cats_sorted":[],"title_canon_sha256":"ada066190fe2d84cb1df033ca1baf5832ca7606e8af8c538c60ee79433e2bfdb","abstract_canon_sha256":"50f6ca7b85e382c283e703a42d23bce7e378309dc4fa4bc6b4327346c772b8f1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:54:58.569598Z","signature_b64":"fZuKPmvFzY99v++qg+KurN9HnPzkZISwVfyFe4d9TBQVj370KZCjwf171svcvqFvg1g9cqc/xOBFzdb+mbjrCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e216a7cb5fd2cfd8d57687065bc536a485aec5e5284c18b2081949907c13cc2b","last_reissued_at":"2026-07-04T15:54:58.569253Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:54:58.569253Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exact Black String Solutions in Three Dimensions","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Gary T. Horowitz, James H. Horne","submitted_at":"1991-08-14T22:25:19Z","abstract_excerpt":"A family of exact conformal field theories is constructed which describe charged black strings in three dimensions. Unlike previous charged black hole or extended black hole solutions in string theory, the low energy spacetime metric has a regular inner horizon (in addition to the event horizon) and a timelike singularity. As the charge to mass ratio approaches unity, the event horizon remains but the singularity disappears."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9108001","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-th/9108001/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":"hep-th/9108001","created_at":"2026-07-04T15:54:58.569309+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9108001v1","created_at":"2026-07-04T15:54:58.569309+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9108001","created_at":"2026-07-04T15:54:58.569309+00:00"},{"alias_kind":"pith_short_12","alias_value":"4ILKPS272LH5","created_at":"2026-07-04T15:54:58.569309+00:00"},{"alias_kind":"pith_short_16","alias_value":"4ILKPS272LH5RVLW","created_at":"2026-07-04T15:54:58.569309+00:00"},{"alias_kind":"pith_short_8","alias_value":"4ILKPS27","created_at":"2026-07-04T15:54:58.569309+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.14127","citing_title":"New analytic solutions of non-SUSY black branes in $10$-D heterotic supergravity and the phase transition","ref_index":50,"is_internal_anchor":true},{"citing_arxiv_id":"2604.15566","citing_title":"One-loop effect in the charged 2D black hole near extremality","ref_index":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS","json":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS.json","graph_json":"https://pith.science/api/pith-number/4ILKPS272LH5RVLWQ4DFXRJWUS/graph.json","events_json":"https://pith.science/api/pith-number/4ILKPS272LH5RVLWQ4DFXRJWUS/events.json","paper":"https://pith.science/paper/4ILKPS27"},"agent_actions":{"view_html":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS","download_json":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS.json","view_paper":"https://pith.science/paper/4ILKPS27","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9108001&json=true","fetch_graph":"https://pith.science/api/pith-number/4ILKPS272LH5RVLWQ4DFXRJWUS/graph.json","fetch_events":"https://pith.science/api/pith-number/4ILKPS272LH5RVLWQ4DFXRJWUS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS/action/storage_attestation","attest_author":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS/action/author_attestation","sign_citation":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS/action/citation_signature","submit_replication":"https://pith.science/pith/4ILKPS272LH5RVLWQ4DFXRJWUS/action/replication_record"}},"created_at":"2026-07-04T15:54:58.569309+00:00","updated_at":"2026-07-04T15:54:58.569309+00:00"}