{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:4TBTM3YOANLM27AZTQFRI7EIAC","short_pith_number":"pith:4TBTM3YO","schema_version":"1.0","canonical_sha256":"e4c3366f0e0356cd7c199c0b147c88009caa47c386eec99ee3c0c820c7faccaa","source":{"kind":"arxiv","id":"hep-th/0408106","version":2},"attestation_state":"computed","paper":{"title":"One Ring to Rule Them All ... and in the Darkness Bind Them?","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Iosif Bena, Nicholas P. Warner","submitted_at":"2004-08-13T19:44:54Z","abstract_excerpt":"We construct all eleven-dimensional, three-charge BPS solutions that preserve a fixed, standard set of supersymmetries. Our solutions include all BPS three-charge rotating black holes, black rings, supertubes, as well as arbitrary superpositions of these objects. We find very large families of black rings and supertubes with profiles that follow arbitrary closed curves in the spatial R^4 transverse to the branes. The black rings copiously violate black hole uniqueness. The supertube solutions are completely regular, and generically have small curvature. They also have the same asymptotics as t"},"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/0408106","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2004-08-13T19:44:54Z","cross_cats_sorted":[],"title_canon_sha256":"ac139f9b6b54682dcb64976998df764a66f8fcfa1ad09b771e9b58e66108733c","abstract_canon_sha256":"e4f5d79fcfe3711b4d5c7a8e0f5c89fc8b7b065fc3a8fd749971c777abd6ae3c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:49:31.073478Z","signature_b64":"6h9rdlvI6ipsMU9MjQGMRJa87MdP7eA930QdsPfwBhCw46vtbgCU7q2lwFnEwnYADOef5iguVYhiffxI03EJCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e4c3366f0e0356cd7c199c0b147c88009caa47c386eec99ee3c0c820c7faccaa","last_reissued_at":"2026-07-04T14:49:31.073125Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:49:31.073125Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"One Ring to Rule Them All ... and in the Darkness Bind Them?","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Iosif Bena, Nicholas P. Warner","submitted_at":"2004-08-13T19:44:54Z","abstract_excerpt":"We construct all eleven-dimensional, three-charge BPS solutions that preserve a fixed, standard set of supersymmetries. Our solutions include all BPS three-charge rotating black holes, black rings, supertubes, as well as arbitrary superpositions of these objects. We find very large families of black rings and supertubes with profiles that follow arbitrary closed curves in the spatial R^4 transverse to the branes. The black rings copiously violate black hole uniqueness. The supertube solutions are completely regular, and generically have small curvature. They also have the same asymptotics as t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0408106","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/0408106/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/0408106","created_at":"2026-07-04T14:49:31.073183+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0408106v2","created_at":"2026-07-04T14:49:31.073183+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0408106","created_at":"2026-07-04T14:49:31.073183+00:00"},{"alias_kind":"pith_short_12","alias_value":"4TBTM3YOANLM","created_at":"2026-07-04T14:49:31.073183+00:00"},{"alias_kind":"pith_short_16","alias_value":"4TBTM3YOANLM27AZ","created_at":"2026-07-04T14:49:31.073183+00:00"},{"alias_kind":"pith_short_8","alias_value":"4TBTM3YO","created_at":"2026-07-04T14:49:31.073183+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":7,"sample":[{"citing_arxiv_id":"2606.25016","citing_title":"Lost in Translation: Moduli Stabilization from EFT to Eleven Dimensions","ref_index":40,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19552","citing_title":"Large Order Enumerative Geometry, Black Holes and Black Rings","ref_index":78,"is_internal_anchor":true},{"citing_arxiv_id":"2605.28737","citing_title":"Complex BPS Black Holes in AdS$_3\\times S^3$","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2606.27093","citing_title":"Index saddle for the D1-D5-P black string and its decoupling limit","ref_index":35,"is_internal_anchor":true},{"citing_arxiv_id":"2105.11639","citing_title":"Interpolating between multi-center microstate geometries","ref_index":4,"is_internal_anchor":true},{"citing_arxiv_id":"2411.12413","citing_title":"Attractor saddle for 5D black hole index","ref_index":15,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19552","citing_title":"Large Order Enumerative Geometry, Black Holes and Black Rings","ref_index":78,"is_internal_anchor":true},{"citing_arxiv_id":"2604.05696","citing_title":"Monodromy-Matrix Description of Extremal Multi-centered Black Holes","ref_index":39,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC","json":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC.json","graph_json":"https://pith.science/api/pith-number/4TBTM3YOANLM27AZTQFRI7EIAC/graph.json","events_json":"https://pith.science/api/pith-number/4TBTM3YOANLM27AZTQFRI7EIAC/events.json","paper":"https://pith.science/paper/4TBTM3YO"},"agent_actions":{"view_html":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC","download_json":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC.json","view_paper":"https://pith.science/paper/4TBTM3YO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0408106&json=true","fetch_graph":"https://pith.science/api/pith-number/4TBTM3YOANLM27AZTQFRI7EIAC/graph.json","fetch_events":"https://pith.science/api/pith-number/4TBTM3YOANLM27AZTQFRI7EIAC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC/action/storage_attestation","attest_author":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC/action/author_attestation","sign_citation":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC/action/citation_signature","submit_replication":"https://pith.science/pith/4TBTM3YOANLM27AZTQFRI7EIAC/action/replication_record"}},"created_at":"2026-07-04T14:49:31.073183+00:00","updated_at":"2026-07-04T14:49:31.073183+00:00"}