{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:WTLQYXJ225NUNNK3EVIONHJ54J","short_pith_number":"pith:WTLQYXJ2","schema_version":"1.0","canonical_sha256":"b4d70c5d3ad75b46b55b2550e69d3de27808f4e1c419a4547763a422009e1749","source":{"kind":"arxiv","id":"1005.1287","version":1},"attestation_state":"computed","paper":{"title":"Small Hairy Black Holes in $AdS_5 \\times S^5$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Kyriakos Papadodimas, Sayantani Bhattacharyya, Shiraz Minwalla","submitted_at":"2010-05-07T20:00:03Z","abstract_excerpt":"We study small hairy black holes in a consistent truncation of ${\\cal N}=8$ gauged supergravity that consists of a single charged scalar field interacting with the metric and a U(1) gauge field. Small very near extremal RNAdS black holes in this system are unstable to decay by superradiant emission. The end point of this instability is a small hairy black hole that we construct analytically in a perturbative expansion in its charge. Unlike their RNAdS counterparts, hairy black hole solutions exist all the way down to the BPS bound, demonstrating that ${\\cal N}=4$ Yang Mills theory has an ${\\ca"},"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":"1005.1287","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2010-05-07T20:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"397da5856d7e9955844323d61e348f193d85de8b8f75fd44d2399cb612379c60","abstract_canon_sha256":"86527f44b5a7468f433d454e58c2b8f68363f69f14307da61e36377c7a6f36b4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:35.190534Z","signature_b64":"QNU+vbPwUxViiJl3HxumkLULG+Yo7o99RcgXTn9eocJ0TkXD5vs0/MmXnbGbLsAD2YsKxy5c91Z+GjjvGSyLDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b4d70c5d3ad75b46b55b2550e69d3de27808f4e1c419a4547763a422009e1749","last_reissued_at":"2026-05-18T02:07:35.189843Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:35.189843Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Small Hairy Black Holes in $AdS_5 \\times S^5$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Kyriakos Papadodimas, Sayantani Bhattacharyya, Shiraz Minwalla","submitted_at":"2010-05-07T20:00:03Z","abstract_excerpt":"We study small hairy black holes in a consistent truncation of ${\\cal N}=8$ gauged supergravity that consists of a single charged scalar field interacting with the metric and a U(1) gauge field. Small very near extremal RNAdS black holes in this system are unstable to decay by superradiant emission. The end point of this instability is a small hairy black hole that we construct analytically in a perturbative expansion in its charge. Unlike their RNAdS counterparts, hairy black hole solutions exist all the way down to the BPS bound, demonstrating that ${\\cal N}=4$ Yang Mills theory has an ${\\ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.1287","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":""},"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":"1005.1287","created_at":"2026-05-18T02:07:35.189954+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.1287v1","created_at":"2026-05-18T02:07:35.189954+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.1287","created_at":"2026-05-18T02:07:35.189954+00:00"},{"alias_kind":"pith_short_12","alias_value":"WTLQYXJ225NU","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_16","alias_value":"WTLQYXJ225NUNNK3","created_at":"2026-05-18T12:26:17.028572+00:00"},{"alias_kind":"pith_short_8","alias_value":"WTLQYXJ2","created_at":"2026-05-18T12:26:17.028572+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.00095","citing_title":"Instanton condensation and a new phase of BPS black holes","ref_index":49,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J","json":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J.json","graph_json":"https://pith.science/api/pith-number/WTLQYXJ225NUNNK3EVIONHJ54J/graph.json","events_json":"https://pith.science/api/pith-number/WTLQYXJ225NUNNK3EVIONHJ54J/events.json","paper":"https://pith.science/paper/WTLQYXJ2"},"agent_actions":{"view_html":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J","download_json":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J.json","view_paper":"https://pith.science/paper/WTLQYXJ2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.1287&json=true","fetch_graph":"https://pith.science/api/pith-number/WTLQYXJ225NUNNK3EVIONHJ54J/graph.json","fetch_events":"https://pith.science/api/pith-number/WTLQYXJ225NUNNK3EVIONHJ54J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J/action/storage_attestation","attest_author":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J/action/author_attestation","sign_citation":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J/action/citation_signature","submit_replication":"https://pith.science/pith/WTLQYXJ225NUNNK3EVIONHJ54J/action/replication_record"}},"created_at":"2026-05-18T02:07:35.189954+00:00","updated_at":"2026-05-18T02:07:35.189954+00:00"}