{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:RFQZM3IKXABARSXRX5K4HTOOPM","short_pith_number":"pith:RFQZM3IK","schema_version":"1.0","canonical_sha256":"8961966d0ab80208caf1bf55c3cdce7b11846a63f125f49831770608b82da856","source":{"kind":"arxiv","id":"2411.19082","version":2},"attestation_state":"computed","paper":{"title":"Nonuniqueness of capped black holes: large and small bubbles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Ryotaku Suzuki, Shinya Tomizawa","submitted_at":"2024-11-28T12:00:36Z","abstract_excerpt":"We present a new non-BPS solution describing an asymptotically flat, stationary, bi-axisymmetric capped black hole in the bosonic sector of five-dimensional minimal supergravity. This solution describes a spherical black hole, while the exterior region of the horizon exhibits a non-trivial topology of $[{\\mathbb R}^4 \\# {\\mathbb C}{\\mathbb P}^2] \\setminus {\\mathbb B}^4$ on a timeslice. This solution extends our previously constructed three-parameter solution to a more general four-parameter solution. To derive this solution, we utilize a combination of the Ehlers and Harrison transformations a"},"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":"2411.19082","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-11-28T12:00:36Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"d3fd9838999d92fbb9ea38a9af0d043f0341cb30f01097c5cf1a8289a33990f4","abstract_canon_sha256":"2c49ce23f4fb4b512089e03d3e8671c4eed3bfe8171daecf3b61a2b9a7ef7e04"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:50:54.571253Z","signature_b64":"Y69GR862JCSiDHpyE8LNjjbf37C4Bm78pgX9ZqEYPKo+nytjbscFonI3VhNIkdgkWGqnBZVoskJ+Y2JlPboFAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8961966d0ab80208caf1bf55c3cdce7b11846a63f125f49831770608b82da856","last_reissued_at":"2026-07-05T09:50:54.570740Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:50:54.570740Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nonuniqueness of capped black holes: large and small bubbles","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Ryotaku Suzuki, Shinya Tomizawa","submitted_at":"2024-11-28T12:00:36Z","abstract_excerpt":"We present a new non-BPS solution describing an asymptotically flat, stationary, bi-axisymmetric capped black hole in the bosonic sector of five-dimensional minimal supergravity. This solution describes a spherical black hole, while the exterior region of the horizon exhibits a non-trivial topology of $[{\\mathbb R}^4 \\# {\\mathbb C}{\\mathbb P}^2] \\setminus {\\mathbb B}^4$ on a timeslice. This solution extends our previously constructed three-parameter solution to a more general four-parameter solution. To derive this solution, we utilize a combination of the Ehlers and Harrison transformations a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.19082","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/2411.19082/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":"2411.19082","created_at":"2026-07-05T09:50:54.570800+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.19082v2","created_at":"2026-07-05T09:50:54.570800+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.19082","created_at":"2026-07-05T09:50:54.570800+00:00"},{"alias_kind":"pith_short_12","alias_value":"RFQZM3IKXABA","created_at":"2026-07-05T09:50:54.570800+00:00"},{"alias_kind":"pith_short_16","alias_value":"RFQZM3IKXABARSXR","created_at":"2026-07-05T09:50:54.570800+00:00"},{"alias_kind":"pith_short_8","alias_value":"RFQZM3IK","created_at":"2026-07-05T09:50:54.570800+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.05696","citing_title":"Monodromy-Matrix Description of Extremal Multi-centered Black Holes","ref_index":58,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM","json":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM.json","graph_json":"https://pith.science/api/pith-number/RFQZM3IKXABARSXRX5K4HTOOPM/graph.json","events_json":"https://pith.science/api/pith-number/RFQZM3IKXABARSXRX5K4HTOOPM/events.json","paper":"https://pith.science/paper/RFQZM3IK"},"agent_actions":{"view_html":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM","download_json":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM.json","view_paper":"https://pith.science/paper/RFQZM3IK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.19082&json=true","fetch_graph":"https://pith.science/api/pith-number/RFQZM3IKXABARSXRX5K4HTOOPM/graph.json","fetch_events":"https://pith.science/api/pith-number/RFQZM3IKXABARSXRX5K4HTOOPM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM/action/storage_attestation","attest_author":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM/action/author_attestation","sign_citation":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM/action/citation_signature","submit_replication":"https://pith.science/pith/RFQZM3IKXABARSXRX5K4HTOOPM/action/replication_record"}},"created_at":"2026-07-05T09:50:54.570800+00:00","updated_at":"2026-07-05T09:50:54.570800+00:00"}