{"as_of":"2026-08-11T07:28:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:22dd8c5d1fcb226b182ecb4588a60d10590da865a9b39ce2895f9d91afad2742","coverage":[{"denominator":46,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":46,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T22:29:48.358920Z","state":"measured"},{"denominator":46,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":46,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2501.02053/citation-record","integrity":"/paper/2501.02053/integrity","json":"/paper/2501.02053/citation-record.json","paper":"/paper/2501.02053"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.230178Z","title":null,"venue":null,"work_id":"0ba21950-efe6-45ee-8906-9f528edb3959","year":1971},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.148576Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:8cf08aca63e39192a5784173ac5b9f5d1fa8b77af58a017e58ac8f26ccfba510","observation_id":"e41b706d-1db9-47bf-93e0-dcf81b702f6e","resolution":{"observed_at":"2026-08-10T22:29:49.257118Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.154352Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.154352Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:87b2de0316d37985e7540ff923a99e30a9f3a44a010698648bb15920949fed8d","observation_id":"db25bcbf-f630-4b3b-a20f-464f4fffb333","resolution":{"observed_at":"2026-08-10T22:29:48.154352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.196871Z","title":null,"venue":null,"work_id":"f73e2d51-0cdc-4511-be06-2e58e4ae6c36","year":1978},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.159161Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:bf4571d41d486f5bcc4429007a8a1b283392e190ca28a395249e999e68a63554","observation_id":"5d13f47c-7830-42d7-a5e1-11f8cd665ba1","resolution":{"observed_at":"2026-08-10T22:29:49.201720Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.181131Z","title":null,"venue":null,"work_id":"8bd7aa57-f298-4f3b-a3af-d306ffe9f0f5","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.164539Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:61d4abf5cb4e4c587c4d22cfa3687292e367fd659b3021e9bbeb0c2e31cdc8cf","observation_id":"692e3edc-c14d-46a9-b194-bbf8cd4947e9","resolution":{"observed_at":"2026-08-10T22:29:49.186051Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1211.3202","last_updated":"2012-11-21T06:23:58Z","snapshot_observed_at":"2026-08-07T03:18:43.603775Z","submitted_at":"2012-11-14T04:32:07Z","title":"Stationary Scalar Clouds Around Rotating Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.3202","snapshot_observed_at":"2026-08-10T22:29:48.169460Z","title":"Hod, Phys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.169460Z"},"links":{"cited_paper":"/paper/1211.3202","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:3f4ae5a8c2771eed9930a8b36a185a063b5d43fe9b64b92648b82ff80d98f7e7","observation_id":"d8a22ef1-0ab8-48ee-a198-2dc4e0999625","resolution":{"observed_at":"2026-08-10T22:29:48.169460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.5298","last_updated":"2013-11-21T02:51:42Z","snapshot_observed_at":"2026-08-10T12:23:14.068288Z","submitted_at":"2013-11-21T02:51:42Z","title":"Stationary resonances of rapidly-rotating Kerr black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.5298","snapshot_observed_at":"2026-08-10T22:29:48.174625Z","title":"Hod, The Euro","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.174625Z"},"links":{"cited_paper":"/paper/1311.5298","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:824f1ff009feb46b8500242bdc3b6fe7cc7e6a412a17565fe660aaa7c6bf9028","observation_id":"863c05d1-16e0-4bb1-9ea3-a69b72f6ac46","resolution":{"observed_at":"2026-08-10T22:29:48.174625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.179796Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.179796Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:2226d9e3e6acf47042444b5eaade35263ae3012bf25231d0f3b51e507b95e594","observation_id":"a7542232-7dbc-4202-b078-72d326e3041a","resolution":{"observed_at":"2026-08-10T22:29:48.179796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.00811","last_updated":"2016-06-02T19:10:32Z","snapshot_observed_at":"2026-08-02T20:47:15.529984Z","submitted_at":"2016-06-02T19:10:32Z","title":"Quantum and classical aspects of scalar and vector fields around black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.00811","snapshot_observed_at":"2026-08-10T22:29:48.184974Z","title":"Brihaye, C","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.184974Z"},"links":{"cited_paper":"/paper/1606.00811","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:f7ef0ab2ca93c21eef9ce03ea2fa51f273932f55df6a03b9cad02dfb5afe2899","observation_id":"dd11c342-2212-4854-a424-a518eeb8194f","resolution":{"observed_at":"2026-08-10T22:29:48.184974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.15888","last_updated":"2023-07-29T05:18:58Z","snapshot_observed_at":"2026-07-06T16:00:04.308757Z","submitted_at":"2023-07-29T05:18:58Z","title":"Regular scalar clouds around a Kerr-Newman black hole: subextremal and extremal scenarios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.15888","snapshot_observed_at":"2026-08-10T22:29:48.189787Z","title":"Garc ´ ıa and M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.189787Z"},"links":{"cited_paper":"/paper/2307.15888","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:2090e02c7bfb369db65f7815d93180a8a683a44d9aa3f0f8e1dcbae064bda958","observation_id":"833313da-daa4-46fb-9e83-03b45abcd41e","resolution":{"observed_at":"2026-08-10T22:29:48.189787Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.194292Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.194292Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:30ec9c0325c1236139c9fe75db1319b659255098e858426b7ff316ac8d510329","observation_id":"7feaefd5-d679-43a7-b36b-532ee7a994ee","resolution":{"observed_at":"2026-08-10T22:29:48.194292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.6474","last_updated":"2013-06-05T04:39:11Z","snapshot_observed_at":"2026-08-03T18:54:57.214773Z","submitted_at":"2013-04-24T03:17:50Z","title":"No-bomb theorem for charged Reissner-Nordstrom black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.6474","snapshot_observed_at":"2026-08-10T22:29:48.198870Z","title":"Hod, Phys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.198870Z"},"links":{"cited_paper":"/paper/1304.6474","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:a1f2b32c779d34da2f23b7d0d994e8db8c9c91a849b4daefb1767ded98315d6f","observation_id":"626c00ec-7722-403f-884c-817143847e16","resolution":{"observed_at":"2026-08-10T22:29:48.198870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.145530Z","title":null,"venue":null,"work_id":"dac8bb9c-35c3-4614-9313-ba410d790f62","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.203349Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:f805996d3a5956e80aeb3fe466e4d6124408d311c92f16e3478411ba7155d30c","observation_id":"0109883a-76e5-47a6-b091-82e010a3836a","resolution":{"observed_at":"2026-08-10T22:29:49.150538Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.129463Z","title":null,"venue":null,"work_id":"62abb9d0-634e-4374-b553-3695daf0f598","year":2013},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.207380Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:9ec3446b222485b8bd20a9ea0f8e4c5efeccf6cccdb2096332385acada3a4967","observation_id":"f4ec1793-26b1-48d1-8e2f-2054a1c00760","resolution":{"observed_at":"2026-08-10T22:29:49.134015Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.114433Z","title":"Sanchis-Gual, J","venue":null,"work_id":"fc6b8c4f-15fb-4e9b-9534-23b0b8055bb4","year":2016},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.211506Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:d1ed9801de17abbbd568d96828ed6ea1360c7ef9df4bdb88c6e6b29e86c482ff","observation_id":"1ae09a40-837d-4241-b69d-9a91fbee032f","resolution":{"observed_at":"2026-08-10T22:29:49.119196Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1310.6101","last_updated":"2013-10-23T03:22:34Z","snapshot_observed_at":"2026-07-06T03:26:17.752972Z","submitted_at":"2013-10-23T03:22:34Z","title":"Analytic treatment of the charged black-hole-mirror bomb in the highly explosive regime","version":1},"cited_work":{"arxiv_id":"1310.6101","doi":null,"metadata_source":"pith","pith_arxiv_id":"1310.6101","snapshot_observed_at":"2026-08-10T22:29:48.593017Z","title":"Analytic treatment of the charged black-hole-mirror bomb in the highly explosive regime","venue":"gr-qc","work_id":"a234ed31-a1d7-48ce-9de6-899bf1f97c24","year":2013},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.215661Z"},"links":{"cited_paper":"/paper/1310.6101","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:1663a2409e0a7ea4e544b1c164e49a0e883d4aad423ca40a86cf8c9b2599871d","observation_id":"9846a05e-ddf5-4f28-bd4b-dccc903472fa","resolution":{"observed_at":"2026-08-10T22:29:48.598633Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.4567","last_updated":"2014-10-16T20:00:11Z","snapshot_observed_at":"2026-07-06T03:57:37.685269Z","submitted_at":"2014-10-16T20:00:11Z","title":"Resonance spectra of caged black holes","version":1},"cited_work":{"arxiv_id":"1410.4567","doi":null,"metadata_source":"pith","pith_arxiv_id":"1410.4567","snapshot_observed_at":"2026-08-10T22:29:48.568665Z","title":"Resonance spectra of caged black holes","venue":"gr-qc","work_id":"21dea7fb-4201-4f6c-93eb-f9e0133e79bf","year":2014},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.220033Z"},"links":{"cited_paper":"/paper/1410.4567","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:1754ee8a3a5cb43828a649899da69055520a59c532466b710b5a07e2827c8bcf","observation_id":"a0de5f38-b522-4d68-8055-e4fba35f8117","resolution":{"observed_at":"2026-08-10T22:29:48.574907Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.01767","last_updated":"2024-01-03T14:39:38Z","snapshot_observed_at":"2026-08-09T17:47:27.727759Z","submitted_at":"2024-01-03T14:39:38Z","title":"Absorption and (unbounded) superradiance in a static regular black hole spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.01767","snapshot_observed_at":"2026-08-10T22:29:48.224092Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.224092Z"},"links":{"cited_paper":"/paper/2401.01767","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:161b6725918f6b0a03fc5bff9c59e9e07fbc4de31bb7868202224568033fbbd4","observation_id":"fde5092a-0859-4c36-bc7f-498471a00f7a","resolution":{"observed_at":"2026-08-10T22:29:48.224092Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.14967","last_updated":"2024-05-31T14:19:39Z","snapshot_observed_at":"2026-07-06T17:20:57.937385Z","submitted_at":"2024-01-26T16:01:06Z","title":"Superradiant instability of a charged regular black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.14967","snapshot_observed_at":"2026-08-10T22:29:48.228536Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.228536Z"},"links":{"cited_paper":"/paper/2401.14967","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:9cee7666bf57f0c3f60568c446b780338f2bc6a6475618dadb6457df7433a200","observation_id":"52681862-f364-4700-91b1-dfd31fcbc668","resolution":{"observed_at":"2026-08-10T22:29:48.228536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.07907","last_updated":"2024-01-15T19:00:02Z","snapshot_observed_at":"2026-07-06T17:15:50.649358Z","submitted_at":"2024-01-15T19:00:02Z","title":"Spatially regular charged black holes supporting charged massive scalar clouds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.07907","snapshot_observed_at":"2026-08-10T22:29:48.233509Z","title":"Hod, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.233509Z"},"links":{"cited_paper":"/paper/2401.07907","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:0bf9e7cd2a3f3ae19be1b4681c73f7137f7742d76b24edcb6ab09b0235063c0e","observation_id":"b38d9611-fecf-450e-a43a-d5f007c46cb7","resolution":{"observed_at":"2026-08-10T22:29:48.233509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.098817Z","title":"Ay´ on-Beato and A","venue":null,"work_id":"2e37ea96-7d70-424d-b5fe-1fb15c013363","year":1998},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.238619Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:c99e5497dd47b58b3eb398e5a905fc44efc6e88d9d51e6b40083b97e836c1559","observation_id":"af1b5e26-7990-426b-8ec8-11e7838c0e0d","resolution":{"observed_at":"2026-08-10T22:29:49.103547Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.082489Z","title":"Hence, these ﬁeld parameters have the dimensions of length − 1","venue":null,"work_id":"1e6d982a-1332-4036-bf2b-b9ea04870d1d","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.243145Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:457b3c77939def213f9aab37494f791afe2cfb32df746f66379523769e4ec4da","observation_id":"f398c873-74b9-4231-9382-dc583b6ad71a","resolution":{"observed_at":"2026-08-10T22:29:49.087562Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:49.058801Z","title":null,"venue":null,"work_id":"2bf5cfe7-37c9-48b4-86cd-646d81c2a8ad","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.247778Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:22ddc51e61f761b78ee5008bf0747f560729afa18a968cb73ef04ae594354d25","observation_id":"651add42-6f0f-443a-b302-ef46d0cc1db3","resolution":{"observed_at":"2026-08-10T22:29:49.071232Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.252084Z","title":"Chandrasekhar, The Mathematical Theory of Black Holes , (Oxford University Press, New York, 1983)","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.252084Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:5964fb5c02d6ac4baef601a0388b558516332eba071c61d51d2ccd17fa3ea38d","observation_id":"b747dee8-cb2b-4252-b36b-898e9c988911","resolution":{"observed_at":"2026-08-10T22:29:48.252084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.967587Z","title":null,"venue":null,"work_id":"cb391351-2c8d-496f-b07f-13d75ad93623","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.256193Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:e269365f725126d4cdaf829fb9fc35edeb4a5e80895a1351392e31706d39aa3d","observation_id":"95a91c4a-a7d0-42e5-b78e-6dfa7898da97","resolution":{"observed_at":"2026-08-10T22:29:49.007458Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.905491Z","title":null,"venue":null,"work_id":"0b6e17b9-d003-4839-9ba2-db29220d8215","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.261231Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:fa7c45182abfcf24b01cbe8722e0575c04c3e644f27631d09e3f9c1ab859fb27","observation_id":"6a686679-5121-4c64-b62e-091ac7e813cd","resolution":{"observed_at":"2026-08-10T22:29:48.926251Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.890748Z","title":"Dymnikova, Class","venue":null,"work_id":"d46b85c9-5081-447f-aafb-a57cc7fae59e","year":2004},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.265539Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:038ba9c20c699ec95d88ce86cd4ee7af5bacd7d08e21d289aad598fc800c8567","observation_id":"28b5d151-4863-49b4-87a3-d23bcc9494f1","resolution":{"observed_at":"2026-08-10T22:29:48.895448Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9712041","last_updated":"1997-12-09T10:32:44Z","snapshot_observed_at":"2026-07-07T03:28:23.418344Z","submitted_at":"1997-12-09T10:32:44Z","title":"Late-Time Evolution of Charged Gravitational Collapse and Decay of Charged Scalar Hair - I","version":1},"cited_work":{"arxiv_id":"gr-qc/9712041","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9712041","snapshot_observed_at":"2026-08-10T22:29:48.501188Z","title":"Late-Time Evolution of Charged Gravitational Collapse and Decay of Charged Scalar Hair - I","venue":"gr-qc","work_id":"9ed32479-85cb-45d5-adea-cf7f835ae6e8","year":1997},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.269893Z"},"links":{"cited_paper":"/paper/gr-qc/9712041","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:9a371dbc52c0ca44511de6231cb53c8892e9673c4382ff4bf1d63c2120dbfc3c","observation_id":"a80d75d1-92c7-4373-8b01-864933828844","resolution":{"observed_at":"2026-08-10T22:29:48.506752Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.875862Z","title":"Hartman, W","venue":null,"work_id":"c29fc77c-d622-4b53-949f-d0db08323010","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.274863Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:302fd0d29d792d17a9956fda28705302371ba6a2f263da6b95a956b1510aa099","observation_id":"74cad23f-6b4b-4a2e-aceb-86fba7017ca5","resolution":{"observed_at":"2026-08-10T22:29:48.880264Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0511047","last_updated":"2005-11-09T19:38:31Z","snapshot_observed_at":"2026-07-07T03:21:43.331487Z","submitted_at":"2005-11-09T19:38:31Z","title":"Quasinormal Spectrum and Quantization of Charged Black Holes","version":1},"cited_work":{"arxiv_id":"gr-qc/0511047","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0511047","snapshot_observed_at":"2026-08-10T22:29:48.476759Z","title":"Quasinormal Spectrum and Quantization of Charged Black Holes","venue":"gr-qc","work_id":"5aad41de-cf61-45bd-9f37-5adcc86fae17","year":2005},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.279465Z"},"links":{"cited_paper":"/paper/gr-qc/0511047","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:6f66f6a23dfc7919f94f0f07967cc879f01afa55fad694443221e4dd7d607717","observation_id":"a89ddaca-12b7-4a3d-8e22-2c5d25f2a1ca","resolution":{"observed_at":"2026-08-10T22:29:48.482562Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.860100Z","title":null,"venue":null,"work_id":"2276b66f-abde-4db0-bcd0-38df988f7dc2","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.284062Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:872b72d57fed048f6686751f56d04378a3793e5c49c0688733b483d689db3638","observation_id":"f0adcd51-9109-4d97-b91e-fac2aa44a073","resolution":{"observed_at":"2026-08-10T22:29:48.865542Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.845153Z","title":null,"venue":null,"work_id":"17c200f0-fe0b-402b-8e13-022cad9abd99","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.288345Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:538d89b9611cbdf9816ba6d45397271f279951e336de404d762d3b71416c691d","observation_id":"75b23107-aa83-4075-8517-40d1645bc480","resolution":{"observed_at":"2026-08-10T22:29:48.849619Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.828663Z","title":null,"venue":null,"work_id":"beb7a368-70bc-4cd8-a738-a64a1efc105d","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.293031Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:bbfbc75c072140fb76bc452f47084eba67275c6f1be9b8f007a8d628c71a28ca","observation_id":"0e4449de-e6aa-47f9-8788-7250f757c79f","resolution":{"observed_at":"2026-08-10T22:29:48.834349Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.812278Z","title":"(13)] with ℑω = 0, mark the boundary between stable (exponentially decaying) and unstable (exponentially growing) resonant modes of the massive bosonic ﬁelds [5–9]","venue":null,"work_id":"0e4e0d28-417d-4815-a893-4e64b406a065","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.297540Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:485aac04d34c011492c94319727db20a64982dd5c4c20a6d6fa7bced92bdc1f5","observation_id":"c38fe5d6-535d-42df-9612-2a3728be011d","resolution":{"observed_at":"2026-08-10T22:29:48.817169Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.797271Z","title":null,"venue":null,"work_id":"c1c4c8a8-6d47-4ccb-918b-20dcd78c02f4","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.302447Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:77ca119d67a7f8bff39f2f026f95bafe53a7f5729d6a744a3a88f133e133e42d","observation_id":"5ca5ea11-de8c-45bc-b15d-0f42ea3335fd","resolution":{"observed_at":"2026-08-10T22:29:48.802053Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.782647Z","title":null,"venue":null,"work_id":"ab00ff5a-e7e3-4a2d-86c7-c3bd9c4522b7","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.308080Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:28e3ada331815a46384708676fad644a68620d73af484bf2befff841b7483c17","observation_id":"295d1da1-a971-4eba-b8b5-cd3ceb3df011","resolution":{"observed_at":"2026-08-10T22:29:48.787661Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.767713Z","title":null,"venue":null,"work_id":"d68e3d32-d61b-4d77-91bb-f7bf456ac9c1","year":2019},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.313066Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:7265445dc7f85cb3739a91736dce998ea524bc9e5efe02b4e34bc130b0048c1e","observation_id":"01f3b185-adaa-45ae-906c-3001294508d3","resolution":{"observed_at":"2026-08-10T22:29:48.772442Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.09399","last_updated":"2020-08-04T05:04:34Z","snapshot_observed_at":"2026-07-06T09:29:45.475911Z","submitted_at":"2020-06-16T18:00:05Z","title":"Onset of spontaneous scalarization in spinning Gauss-Bonnet black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.09399","snapshot_observed_at":"2026-08-10T22:29:48.317557Z","title":"Hod, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.317557Z"},"links":{"cited_paper":"/paper/2006.09399","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:af180ac635c030a138ab844467fc3c2dda5d4a31f7303f5e7f6a3a0e98e0cab8","observation_id":"c65910a5-eb08-4683-ad44-99e4f2f3c7d2","resolution":{"observed_at":"2026-08-10T22:29:48.317557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.06442","last_updated":"2021-11-11T19:58:20Z","snapshot_observed_at":"2026-07-06T12:07:45.652474Z","submitted_at":"2021-11-11T19:58:20Z","title":"Aspects of Gauss-Bonnet scalarisation of charged black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.06442","snapshot_observed_at":"2026-08-10T22:29:48.322766Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.322766Z"},"links":{"cited_paper":"/paper/2111.06442","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:4f24fd81304c10008b2577efff892c971055a81fdff67b7c0f1757c7ecaba7b8","observation_id":"d5dd579d-847c-4a87-896c-6aca04c60011","resolution":{"observed_at":"2026-08-10T22:29:48.322766Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.03503","last_updated":"2022-02-07T16:24:19Z","snapshot_observed_at":"2026-07-06T12:26:09.094759Z","submitted_at":"2022-01-10T18:00:29Z","title":"Infinitesimally thin static scalar shells surrounding charged Gauss-Bonnet black holes","version":2},"cited_work":{"arxiv_id":"2201.03503","doi":null,"metadata_source":"pith","pith_arxiv_id":"2201.03503","snapshot_observed_at":"2026-08-10T22:29:48.421026Z","title":"Infinitesimally thin static scalar shells surrounding charged Gauss-Bonnet black holes","venue":"hep-th","work_id":"ce8d6577-1d0e-4229-8f74-3c3e063c0dae","year":2022},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.327470Z"},"links":{"cited_paper":"/paper/2201.03503","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:616e449be75a128793655de5720601486a6f138e2a63f28235864ed54cf194c4","observation_id":"f63b4eb8-dd19-4026-9122-922f6dd604e4","resolution":{"observed_at":"2026-08-10T22:29:48.426136Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.12990","last_updated":"2023-08-24T18:00:02Z","snapshot_observed_at":"2026-07-06T16:10:07.931347Z","submitted_at":"2023-08-24T18:00:02Z","title":"Analytic study of the Maxwell electromagnetic invariant in spinning and charged Kerr-Newman black-hole spacetimes","version":1},"cited_work":{"arxiv_id":"2308.12990","doi":null,"metadata_source":"pith","pith_arxiv_id":"2308.12990","snapshot_observed_at":"2026-08-10T22:29:48.396208Z","title":"Analytic study of the Maxwell electromagnetic invariant in spinning and charged Kerr-Newman black-hole spacetimes","venue":"gr-qc","work_id":"711e14ee-c92a-4f37-acdc-10c86dd3ae97","year":2023},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.332560Z"},"links":{"cited_paper":"/paper/2308.12990","citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:358058993b0e6d683b99d83bf9af4525f6748cd8fb8690b32352e7391cec9683","observation_id":"dcda2c17-6e2b-4eae-a5a2-b969085a820a","resolution":{"observed_at":"2026-08-10T22:29:48.404205Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.752946Z","title":null,"venue":null,"work_id":"81c85bb0-a5e4-4f96-9ff7-4d346eab9542","year":1977},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.337271Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:f85f3b797f262313fb1a62a7497ed0ad13ce20e7226d5d3c79076b37c009caa0","observation_id":"ca33a8be-955b-41b6-a410-6518af6b913a","resolution":{"observed_at":"2026-08-10T22:29:48.757568Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.341543Z","title":"Heading, An Introduction to Phase Integral Methods (Wiley, New York, 1962)","venue":null,"work_id":null,"year":1962},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.341543Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:4ad59b2f86c97ea4e1f42cc5b92c8cf856515b7e94dcd8adf9c3401d118fbcdc","observation_id":"d1525ad7-4edb-4cdd-af30-73bf65001f90","resolution":{"observed_at":"2026-08-10T22:29:48.341543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.345933Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.345933Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:2009e7ae53ba681ee77e34146925e67e74b7c62ac6c004fa3d345d72af6927e0","observation_id":"bbdbaaad-a3f0-485d-8211-5b965e60eae0","resolution":{"observed_at":"2026-08-10T22:29:48.345933Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.718856Z","title":null,"venue":null,"work_id":"b21a1b20-61a9-41ee-aa6f-1e79fb129f9e","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.350491Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:f4255ba9b2b38022a62eedbe349adca7abc7bb7ce12be4c85ea26c0f758e2665","observation_id":"8539107c-6dc1-4b05-9b9f-bbe673d448b2","resolution":{"observed_at":"2026-08-10T22:29:48.723424Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.704326Z","title":null,"venue":null,"work_id":"aa5b52bf-de34-4e57-9491-2df1114747d4","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.354486Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:08f499c61f6b84af2e4593d310ba4835dda6c1526689677aa0473c8d664c0ac1","observation_id":"978d7f6e-0e18-4fe7-a5f6-faa5bb6bf332","resolution":{"observed_at":"2026-08-10T22:29:48.708813Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T22:29:48.689060Z","title":null,"venue":null,"work_id":"15844dd4-db3b-4a1b-b1aa-deaa9b6fd584","year":null},"citing_paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-10T22:29:48.358920Z"},"links":{"citing_paper":"/paper/2501.02053"},"observation_digest":"sha256:f4581b50627b986b95639bd444c5b97a6976abd266988244029ca3e6a68c3bcd","observation_id":"5cf0d524-0237-4df2-8f2b-e1ac91c69bc7","resolution":{"observed_at":"2026-08-10T22:29:48.693742Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2501.02053","last_updated":"2025-01-03T19:00:01Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-11T03:37:50.291603Z","submitted_at":"2025-01-03T19:00:01Z","title":"A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes"},"reference_resolution":{"displayed":46,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":34,"verified_exact":6,"verified_fuzzy":6},"total_outbound_references":46},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 46 of 46 outbound references and 0 inbound Pith citation observations for arXiv:2501.02053."}