{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:DEDUJCARTN3RZH7X6T4FSJ25Q4","short_pith_number":"pith:DEDUJCAR","schema_version":"1.0","canonical_sha256":"19074488119b771c9ff7f4f859275d870ef9cf69b4e6e4c6e60a2b69529549ec","source":{"kind":"arxiv","id":"hep-th/0110260","version":2},"attestation_state":"computed","paper":{"title":"A rotating black ring in five dimensions","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Harvey S. Reall, Roberto Emparan","submitted_at":"2001-10-29T14:48:14Z","abstract_excerpt":"The vacuum Einstein equations in five dimensions are shown to admit a solution describing an asymptotically flat spacetime regular on and outside an event horizon of topology S^1 x S^2. It describes a rotating ``black ring''. This is the first example of an asymptotically flat vacuum solution with an event horizon of non-spherical topology. There is a range of values for the mass and angular momentum for which there exist two black ring solutions as well as a black hole solution. Therefore the uniqueness theorems valid in four dimensions do not have simple higher dimensional generalizations. I"},"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/0110260","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2001-10-29T14:48:14Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"b94a0a64571b277a5317a9fb8f876213352f84458257e60fe3c7471c4eb017c2","abstract_canon_sha256":"6610fede76c64f59b7cf4763bb3ce2579138300afd4f9e83321c92df313b225a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:45:46.287514Z","signature_b64":"ooA6ZrsLO/k5NspoY1jhQm4w/jVzbVRPpfHUNteQlrFtIpLkeaarsWTQG+3LCA61DN/SsdgHLiSrgthUXEmyBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"19074488119b771c9ff7f4f859275d870ef9cf69b4e6e4c6e60a2b69529549ec","last_reissued_at":"2026-07-04T15:45:46.287125Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:45:46.287125Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A rotating black ring in five dimensions","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Harvey S. Reall, Roberto Emparan","submitted_at":"2001-10-29T14:48:14Z","abstract_excerpt":"The vacuum Einstein equations in five dimensions are shown to admit a solution describing an asymptotically flat spacetime regular on and outside an event horizon of topology S^1 x S^2. It describes a rotating ``black ring''. This is the first example of an asymptotically flat vacuum solution with an event horizon of non-spherical topology. There is a range of values for the mass and angular momentum for which there exist two black ring solutions as well as a black hole solution. Therefore the uniqueness theorems valid in four dimensions do not have simple higher dimensional generalizations. I"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0110260","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/hep-th/0110260/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/0110260","created_at":"2026-07-04T15:45:46.287187+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0110260v2","created_at":"2026-07-04T15:45:46.287187+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0110260","created_at":"2026-07-04T15:45:46.287187+00:00"},{"alias_kind":"pith_short_12","alias_value":"DEDUJCARTN3R","created_at":"2026-07-04T15:45:46.287187+00:00"},{"alias_kind":"pith_short_16","alias_value":"DEDUJCARTN3RZH7X","created_at":"2026-07-04T15:45:46.287187+00:00"},{"alias_kind":"pith_short_8","alias_value":"DEDUJCAR","created_at":"2026-07-04T15:45:46.287187+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":9,"sample":[{"citing_arxiv_id":"2606.13592","citing_title":"Trapped Surface as a Cosmic Censor","ref_index":65,"is_internal_anchor":true},{"citing_arxiv_id":"2606.05319","citing_title":"Non-linear evolution of five-dimensional black strings in effective field theory","ref_index":5,"is_internal_anchor":true},{"citing_arxiv_id":"2606.30507","citing_title":"The Role of the Volume in Black Hole Thermodynamics","ref_index":45,"is_internal_anchor":true},{"citing_arxiv_id":"2605.29831","citing_title":"Five-dimensional Geometry from Spinning Amplitudes","ref_index":88,"is_internal_anchor":true},{"citing_arxiv_id":"2511.15426","citing_title":"Probing decoupled Throats of AdS$_{D}$ Black Holes in $D=6,7$","ref_index":101,"is_internal_anchor":true},{"citing_arxiv_id":"1501.06570","citing_title":"Superradiance -- the 2020 Edition","ref_index":92,"is_internal_anchor":true},{"citing_arxiv_id":"2601.04623","citing_title":"Non-supersymmetric F1-P black rings","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2601.22914","citing_title":"Exact black holes and black branes with bumpy horizons supported by superfluid pions","ref_index":13,"is_internal_anchor":true},{"citing_arxiv_id":"2603.23556","citing_title":"On regular black string spacetimes in nonlinear electrodynamics","ref_index":11,"is_internal_anchor":true},{"citing_arxiv_id":"2605.05067","citing_title":"Gravitational multipoles from scattering amplitudes in higher dimensions","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08951","citing_title":"Weyl-type solutions with multipolar scalar fields","ref_index":45,"is_internal_anchor":false},{"citing_arxiv_id":"2604.05696","citing_title":"Monodromy-Matrix Description of Extremal Multi-centered Black Holes","ref_index":22,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4","json":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4.json","graph_json":"https://pith.science/api/pith-number/DEDUJCARTN3RZH7X6T4FSJ25Q4/graph.json","events_json":"https://pith.science/api/pith-number/DEDUJCARTN3RZH7X6T4FSJ25Q4/events.json","paper":"https://pith.science/paper/DEDUJCAR"},"agent_actions":{"view_html":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4","download_json":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4.json","view_paper":"https://pith.science/paper/DEDUJCAR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0110260&json=true","fetch_graph":"https://pith.science/api/pith-number/DEDUJCARTN3RZH7X6T4FSJ25Q4/graph.json","fetch_events":"https://pith.science/api/pith-number/DEDUJCARTN3RZH7X6T4FSJ25Q4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4/action/storage_attestation","attest_author":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4/action/author_attestation","sign_citation":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4/action/citation_signature","submit_replication":"https://pith.science/pith/DEDUJCARTN3RZH7X6T4FSJ25Q4/action/replication_record"}},"created_at":"2026-07-04T15:45:46.287187+00:00","updated_at":"2026-07-04T15:45:46.287187+00:00"}