{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1992:2VGILQFMWHC6TA6WBDCHANUTII","short_pith_number":"pith:2VGILQFM","schema_version":"1.0","canonical_sha256":"d54c85c0acb1c5e983d608c47036934208d00a7cb129e70a9bfe534b0995cfd5","source":{"kind":"arxiv","id":"hep-th/9204046","version":1},"attestation_state":"computed","paper":{"title":"Rotating Charged Black Hole Solution in Heterotic String Theory","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Ashoke Sen","submitted_at":"1992-04-15T22:17:00Z","abstract_excerpt":"We construct a solution of the classical equations of motion arising in the low energy effective field theory for heterotic string theory. This solution describes a black hole in four dimensions carrying mass $M$, charge $Q$ and angular momentum $J$. The extremal limit of the solution is discussed."},"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/9204046","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1992-04-15T22:17:00Z","cross_cats_sorted":[],"title_canon_sha256":"5d6b141abdc4d90e1ef820fe40f669e801990257af757c561fbf4f713f47e7f1","abstract_canon_sha256":"79a382f1ce9d32a00f49b455d393a4fd80f8bb8b122428e2dc2e0996dc457920"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:49:41.517353Z","signature_b64":"sFKx8zQWeDCH6oUYenLnUfaY0gKkj3ZuLeWkVMjXHB9GM2ztUmDEO1zrjWoyArWdSpK3/Pyn/+T54/eI0iCTBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d54c85c0acb1c5e983d608c47036934208d00a7cb129e70a9bfe534b0995cfd5","last_reissued_at":"2026-07-04T15:49:41.516970Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:49:41.516970Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rotating Charged Black Hole Solution in Heterotic String Theory","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Ashoke Sen","submitted_at":"1992-04-15T22:17:00Z","abstract_excerpt":"We construct a solution of the classical equations of motion arising in the low energy effective field theory for heterotic string theory. This solution describes a black hole in four dimensions carrying mass $M$, charge $Q$ and angular momentum $J$. The extremal limit of the solution is discussed."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9204046","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/9204046/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/9204046","created_at":"2026-07-04T15:49:41.517035+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9204046v1","created_at":"2026-07-04T15:49:41.517035+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9204046","created_at":"2026-07-04T15:49:41.517035+00:00"},{"alias_kind":"pith_short_12","alias_value":"2VGILQFMWHC6","created_at":"2026-07-04T15:49:41.517035+00:00"},{"alias_kind":"pith_short_16","alias_value":"2VGILQFMWHC6TA6W","created_at":"2026-07-04T15:49:41.517035+00:00"},{"alias_kind":"pith_short_8","alias_value":"2VGILQFM","created_at":"2026-07-04T15:49:41.517035+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":6,"sample":[{"citing_arxiv_id":"2606.24215","citing_title":"Nonlinear Stability of Kerr-Sen Black Holes in Merging Binaries","ref_index":37,"is_internal_anchor":true},{"citing_arxiv_id":"2606.02660","citing_title":"Late-Time Cosmology and Structure Formation in Quadratic $f(Q)$ Gravity","ref_index":89,"is_internal_anchor":true},{"citing_arxiv_id":"2510.07390","citing_title":"Heterotic Footprints in Classical Gravity: PM dynamics from On-Shell soft amplitudes at one loop","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2510.23292","citing_title":"Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity","ref_index":29,"is_internal_anchor":true},{"citing_arxiv_id":"2512.07825","citing_title":"Novel thermodynamic inequality for rotating AdS black holes","ref_index":40,"is_internal_anchor":true},{"citing_arxiv_id":"2603.21459","citing_title":"Symmetries of non-maximal supergravities with higher-derivative corrections","ref_index":21,"is_internal_anchor":true},{"citing_arxiv_id":"2604.08439","citing_title":"Optical images of Kerr-Sen black hole illuminated by thick accretion disks","ref_index":50,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII","json":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII.json","graph_json":"https://pith.science/api/pith-number/2VGILQFMWHC6TA6WBDCHANUTII/graph.json","events_json":"https://pith.science/api/pith-number/2VGILQFMWHC6TA6WBDCHANUTII/events.json","paper":"https://pith.science/paper/2VGILQFM"},"agent_actions":{"view_html":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII","download_json":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII.json","view_paper":"https://pith.science/paper/2VGILQFM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9204046&json=true","fetch_graph":"https://pith.science/api/pith-number/2VGILQFMWHC6TA6WBDCHANUTII/graph.json","fetch_events":"https://pith.science/api/pith-number/2VGILQFMWHC6TA6WBDCHANUTII/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII/action/storage_attestation","attest_author":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII/action/author_attestation","sign_citation":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII/action/citation_signature","submit_replication":"https://pith.science/pith/2VGILQFMWHC6TA6WBDCHANUTII/action/replication_record"}},"created_at":"2026-07-04T15:49:41.517035+00:00","updated_at":"2026-07-04T15:49:41.517035+00:00"}