{"as_of":"2026-08-08T04:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8da02757649b9f788cbde01de27f7de1f05aaf673ba8916ba3ca03d680e30248","coverage":[{"denominator":100,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T04:46:19.408879Z","state":"measured"},{"denominator":108,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":108,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T19:07:34.663480Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-06-30T00:04:06.133212Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-08-05T19:07:34.663480Z","title":"Stuchlík and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.13366","last_updated":"2026-07-22T14:35:30Z","snapshot_observed_at":"2026-08-07T18:18:39.515438Z","submitted_at":"2025-08-18T21:17:11Z","title":"Where Do the Returns to Schooling Come From? Educational Transitions and Labor Market Payoffs","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-05T19:07:34.663480Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2508.13366"},"observation_digest":"sha256:bf7fe0f806500da818a3fcdd55ca81ecd1d00c8da419ca9aff5ad8ed0f5df7cf","observation_id":"2cc218a8-3099-4e76-a1b8-42f7452c87ce","resolution":{"observed_at":"2026-08-05T19:07:34.663480Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-08-04T11:09:54.796896Z","title":"Stuchlík and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.06689","last_updated":"2026-05-28T09:50:09Z","snapshot_observed_at":"2026-08-04T11:09:41.169992Z","submitted_at":"2025-10-08T06:25:32Z","title":"Bonanno-Reuter regular black hole: quasi-resonances, grey-body factors and absorption cross-sections of a massive scalar field","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-04T11:09:54.796896Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2510.06689"},"observation_digest":"sha256:bc2698e20fdc9f0d42b2c9d43298e5dfdecb507d20472d133a0022e1d52c84d6","observation_id":"2547ecd4-17de-453b-b7bb-f3c0f11ec3b9","resolution":{"observed_at":"2026-08-04T11:09:54.796896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":"2506.09829","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-06-30T00:04:06.133212Z","title":"Stuchlík and A","venue":null,"work_id":"c8887ff9-8ccb-4892-aa64-d8252c860625","year":2025},"citing_paper":{"arxiv_id":"2603.10844","last_updated":"2026-04-16T17:09:38Z","snapshot_observed_at":"2026-07-06T22:48:39.649787Z","submitted_at":"2026-03-11T14:52:37Z","title":"Long-lived quasinormal modes, shadows and particle motion in four-dimensional quasi-topological gravity","version":2},"reference_index":210,"source":"pdf_text","source_observed_at":"2026-05-15T13:15:54.975020Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2603.10844"},"observation_digest":"sha256:03926fd9aebf052baf8c26e60281d49a2eac46531104db9fe703226b5b19e3ec","observation_id":"47728c42-698a-4de8-80c0-fc7b1d261f0d","resolution":{"observed_at":"2026-05-15T13:20:02.550383Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-08-04T05:43:13.550028Z","title":"Stuchlík and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.28415","last_updated":"2026-08-03T09:20:37Z","snapshot_observed_at":"2026-08-07T15:27:22.728093Z","submitted_at":"2026-03-30T13:27:04Z","title":"Long-lived quasinormal frequencies for regular black hole supported by the Einasto profile in the presence of the magnetic field","version":2},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-08-04T05:43:13.550028Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2603.28415"},"observation_digest":"sha256:3e18815458dd214bf08322cb788b82c37a61e988c1f95b27ddb6daece8964969","observation_id":"9cf1ac1c-bec8-407d-80f4-b080ed27ecbc","resolution":{"observed_at":"2026-08-04T05:43:13.550028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":"2506.09829","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-06-30T00:04:06.133212Z","title":"Stuchlík and A","venue":null,"work_id":"c8887ff9-8ccb-4892-aa64-d8252c860625","year":2025},"citing_paper":{"arxiv_id":"2605.03137","last_updated":"2026-05-04T20:22:29Z","snapshot_observed_at":"2026-07-06T23:16:05.372336Z","submitted_at":"2026-05-04T20:22:29Z","title":"Scattering of scalar, electromagnetic, and Dirac fields in an asymptotically flat regular black hole supported by primordial dark matter","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-07T02:21:14.281286Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2605.03137"},"observation_digest":"sha256:3add6774e0724987238ba9fb1bb8e4e1c5e68a25ba318c2097092e7b44b6622e","observation_id":"8ccf7693-aa76-4eca-8111-a86c5b003f3d","resolution":{"observed_at":"2026-05-12T10:46:30.473975Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":"2506.09829","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-06-30T00:04:06.133212Z","title":"Stuchlík and A","venue":null,"work_id":"c8887ff9-8ccb-4892-aa64-d8252c860625","year":2025},"citing_paper":{"arxiv_id":"2605.11013","last_updated":"2026-05-10T12:56:40Z","snapshot_observed_at":"2026-07-06T23:22:52.369277Z","submitted_at":"2026-05-10T12:56:40Z","title":"Massive Scalar Quasinormal Modes, Greybody Factors, and Absorption Cross Section of a Parity-Symmetric Beyond-Horndeski Black Hole","version":1},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-05-13T01:58:50.185004Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2605.11013"},"observation_digest":"sha256:5f6c9cc7e6521f83631794c012f00b28a4312da2cdaa459e7d5a63245d4e5f60","observation_id":"3b83e683-c247-494a-a12d-efeff15b1c59","resolution":{"observed_at":"2026-05-13T02:02:06.671445Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":"2506.09829","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-06-30T00:04:06.133212Z","title":"Stuchlík and A","venue":null,"work_id":"c8887ff9-8ccb-4892-aa64-d8252c860625","year":2025},"citing_paper":{"arxiv_id":"2605.25076","last_updated":"2026-05-24T13:39:39Z","snapshot_observed_at":"2026-08-02T03:13:12.097021Z","submitted_at":"2026-05-24T13:39:39Z","title":"Grey-Body Factors and Thermodynamics of Asymptotically de Sitter Black Holes in Generalized Proca Theory","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-06-29T23:58:23.049086Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2605.25076"},"observation_digest":"sha256:d062f96679a59f3393286d994bc207d7152730de3d9689fb52c9602117f971c6","observation_id":"c7f4e725-1352-4d00-b620-7d3770ea8a37","resolution":{"observed_at":"2026-06-30T00:04:06.134630Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"cited_work":{"arxiv_id":"2506.09829","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.09829","snapshot_observed_at":"2026-06-30T00:04:06.133212Z","title":"Stuchlík and A","venue":null,"work_id":"c8887ff9-8ccb-4892-aa64-d8252c860625","year":2025},"citing_paper":{"arxiv_id":"2605.28917","last_updated":"2026-05-27T17:57:30Z","snapshot_observed_at":"2026-07-06T23:38:27.990823Z","submitted_at":"2026-05-27T17:57:30Z","title":"Greybody Factors, Absorption Cross Sections and Hawking Radiation of Holonomy-Corrected Schwarzschild Black Holes","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-06-29T10:32:37.980036Z"},"links":{"cited_paper":"/paper/2506.09829","citing_paper":"/paper/2605.28917"},"observation_digest":"sha256:9e28566d15e369ed2126a3cead2c0f5730719fa7de335ad552c1951bb45bf866","observation_id":"8b9986a1-5a88-4709-bf0a-b3b3cf2faa23","resolution":{"observed_at":"2026-06-29T10:33:18.661041Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2506.09829/citation-record","integrity":"/paper/2506.09829/integrity","json":"/paper/2506.09829/citation-record.json","paper":"/paper/2506.09829"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T04:46:11.765389Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:11.765389Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:121f49cf67aa75e5f9f8926809450502884b592a69df1812b2d40f90cc2102d7","observation_id":"da6519af-767d-4586-975c-d9e73d45dc6c","resolution":{"observed_at":"2026-08-07T04:46:11.765389Z","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":"2026-08-07T04:46:11.889574Z","title":"−” mode becomes one from the black-hole branch, followed by a similar transition for the ℓ = 2 “+","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:11.889574Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3e0c30edc1243e9cfa09caf85bc768b295a0ab6724e7eb399f8a044431c5f88b","observation_id":"b9a8f38f-c0c0-44d7-a97a-15b8410d65b5","resolution":{"observed_at":"2026-08-07T04:46:11.889574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9909058","last_updated":"1999-09-20T14:43:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1999-09-20T14:43:09Z","title":"Quasi-Normal Modes of Stars and Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9909058","snapshot_observed_at":"2026-08-07T04:46:11.962409Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:11.962409Z"},"links":{"cited_paper":"/paper/gr-qc/9909058","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:91524566284c20a4e6af0e8126fa92729dd646e8f4ce78132357e1d4e2efa90c","observation_id":"ff26c98c-f41c-4923-8329-c099622a2dc3","resolution":{"observed_at":"2026-08-07T04:46:11.962409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0905.2975","last_updated":"2009-07-29T07:41:21Z","snapshot_observed_at":"2026-07-06T01:54:40.501878Z","submitted_at":"2009-05-19T05:15:43Z","title":"Quasinormal modes of black holes and black branes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.2975","snapshot_observed_at":"2026-08-07T04:46:12.105995Z","title":"Berti, V","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.105995Z"},"links":{"cited_paper":"/paper/0905.2975","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:27e2527a66c0fe34d375dab87bfdb570a4cb0a669eb32d1665aa2d05d9046c0f","observation_id":"119b5b73-f5b0-4385-bee9-e9d0fb175c6c","resolution":{"observed_at":"2026-08-07T04:46:12.105995Z","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":"2026-08-07T04:46:12.217526Z","title":"Nollert, Class","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.217526Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:d3e54de9aa5c01960fc6f69e68695935ba16b02cb64d67791aa0644ce118cd52","observation_id":"720e5023-f897-4d34-9dde-7036fba4a179","resolution":{"observed_at":"2026-08-07T04:46:12.217526Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.4014","last_updated":"2011-06-15T11:51:40Z","snapshot_observed_at":"2026-07-06T02:23:46.264528Z","submitted_at":"2011-02-19T18:38:22Z","title":"Quasinormal modes of black holes: from astrophysics to string theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.4014","snapshot_observed_at":"2026-08-07T04:46:12.291498Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.291498Z"},"links":{"cited_paper":"/paper/1102.4014","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3d5a449cf3f2356a38804711233ce6153c22654af6d3735bb10c28b0cb81dc37","observation_id":"9808b507-21e7-4a3f-b8da-6974ff6439a1","resolution":{"observed_at":"2026-08-07T04:46:12.291498Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.05014","last_updated":"2025-04-07T12:39:23Z","snapshot_observed_at":"2026-08-07T16:07:59.563710Z","submitted_at":"2025-04-07T12:39:23Z","title":"Review of analytic results on quasinormal modes of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.05014","snapshot_observed_at":"2026-08-07T04:46:12.394638Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.394638Z"},"links":{"cited_paper":"/paper/2504.05014","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:396507c225e2713e80d9bd5f77ad63217ea187eb48c3c27881d8e3607f1bd381","observation_id":"e6af6506-71d5-4d41-bf28-929fd5589865","resolution":{"observed_at":"2026-08-07T04:46:12.394638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-08-07T04:46:12.475566Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.475566Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:fa42758c4327a110a4155f779ba007032fd48ca6c318635697ee67d3b57bcadb","observation_id":"9cf72784-4598-42dd-b39b-1b6a56f4810e","resolution":{"observed_at":"2026-08-07T04:46:12.475566Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-07T04:46:12.584335Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.584335Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:11ce3d317653fce0a14b7c6d1001bb9c8f6e34cefa3557c395c827306ff722ff","observation_id":"3e87e5b6-ebc7-4ca7-b314-c4b59c465f3a","resolution":{"observed_at":"2026-08-07T04:46:12.584335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.12611","last_updated":"2020-06-22T20:56:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-06-22T20:56:34Z","title":"GW190814: Gravitational Waves from the Coalescence of a 23 M$_\\odot$ Black Hole with a 2.6 M$_\\odot$ Compact Object","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.12611","snapshot_observed_at":"2026-08-07T04:46:12.672379Z","title":"Abbott et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.672379Z"},"links":{"cited_paper":"/paper/2006.12611","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:bc46b48d3fa65dd190038d178dbd7396a4e9440e6cf72a6389bd53a88563e503","observation_id":"6ed22b73-a8d4-4cd3-a70b-c1b95fd58bb9","resolution":{"observed_at":"2026-08-07T04:46:12.672379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.01640","last_updated":"2021-10-25T11:24:27Z","snapshot_observed_at":"2026-08-04T11:59:22.240502Z","submitted_at":"2021-09-03T17:36:35Z","title":"Black holes in galactic centers: quasinormal ringing, grey-body factors and Unruh temperature","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.01640","snapshot_observed_at":"2026-08-07T04:46:12.790791Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.790791Z"},"links":{"cited_paper":"/paper/2109.01640","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:732038aa8302bda6d866a74ed2dc03fd735160699b50924ec30d8c0c3d7571b4","observation_id":"ecc43847-5b0f-4952-80a6-e38711360af7","resolution":{"observed_at":"2026-08-07T04:46:12.790791Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0503029","last_updated":"2005-04-01T21:05:30Z","snapshot_observed_at":"2026-07-07T04:53:29.551468Z","submitted_at":"2005-03-03T19:51:31Z","title":"Scalar field perturbations of the Schwarzschild black hole in the G\\\"{o}del Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0503029","snapshot_observed_at":"2026-08-07T04:46:12.861565Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.861565Z"},"links":{"cited_paper":"/paper/hep-th/0503029","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:d761f85f0f0a184824ac8f9084da1e7b30d52755d47339f841ec22d99a623fdc","observation_id":"7fd40545-d8fb-4ef8-9807-d923f6b91d12","resolution":{"observed_at":"2026-08-07T04:46:12.861565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.13320","last_updated":"2020-03-30T12:12:21Z","snapshot_observed_at":"2026-07-06T08:47:47.939800Z","submitted_at":"2019-12-25T13:15:35Z","title":"Quasinormal Modes of Black Holes Surrounded by Dark Matter and Their Connection with the Shadow Radius","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.13320","snapshot_observed_at":"2026-08-07T04:46:12.933144Z","title":"Jusuﬁ, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:12.933144Z"},"links":{"cited_paper":"/paper/1912.13320","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:47ccb36000a422a9f2fcdcbcf3719fb965df3aa5c8df01584de53d6143652afa","observation_id":"3aa8b275-b80b-4760-b302-3ba69db80450","resolution":{"observed_at":"2026-08-07T04:46:12.933144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.04966","last_updated":"2022-02-09T05:20:23Z","snapshot_observed_at":"2026-07-06T12:06:45.710444Z","submitted_at":"2021-11-09T06:44:03Z","title":"Gravitational axial perturbations of Schwarzschild-like black holes in dark matter halos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.04966","snapshot_observed_at":"2026-08-07T04:46:13.002564Z","title":"Zhang, T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.002564Z"},"links":{"cited_paper":"/paper/2111.04966","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:595e465ff2df92e4c12b93c00f24f0ad2eb55ec68a39b27014c96fe8ed49ade3","observation_id":"42f7ca1f-2779-4779-8ede-846c1c08933a","resolution":{"observed_at":"2026-08-07T04:46:13.002564Z","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":"2026-08-07T04:46:13.112446Z","title":"Hamil, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.112446Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:8b10ce24bab8f5c73ff73be64394d955a6a9b497e3ddf629121d762c68679603","observation_id":"d2ba25c6-fc66-4341-8461-09796d03eb1e","resolution":{"observed_at":"2026-08-07T04:46:13.112446Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.16087","last_updated":"2025-03-23T18:57:34Z","snapshot_observed_at":"2026-08-07T16:49:21.209889Z","submitted_at":"2025-03-20T12:29:17Z","title":"Long-lived Quasinormal Modes and Gray-Body Factors of black holes and wormholes in dark matter inspired Weyl Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.16087","snapshot_observed_at":"2026-08-07T04:46:13.186510Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.186510Z"},"links":{"cited_paper":"/paper/2503.16087","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:bc0b2f23e579dee22bb0a36a50d321807b73b6c45c8079675db7a813e968dbc4","observation_id":"b9470899-8521-40c0-ae94-43b62128d128","resolution":{"observed_at":"2026-08-07T04:46:13.186510Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0307012","last_updated":"2020-03-06T14:37:50Z","snapshot_observed_at":"2026-07-07T03:18:04.960857Z","submitted_at":"2003-07-03T13:03:42Z","title":"Quasi-normal modes of Schwarzschild-de Sitter black holes","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0307012","snapshot_observed_at":"2026-08-07T04:46:13.331604Z","title":"Zhidenko, Class","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.331604Z"},"links":{"cited_paper":"/paper/gr-qc/0307012","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:817899eb78cc73e440a0bf9c500b3e6dd88f253277cd93c1f23c3f4a2ff30e34","observation_id":"04f771ef-0d40-451b-bd94-0a927782eaa2","resolution":{"observed_at":"2026-08-07T04:46:13.331604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0308077","last_updated":"2004-01-22T10:34:51Z","snapshot_observed_at":"2026-07-07T03:18:15.032865Z","submitted_at":"2003-08-24T11:14:33Z","title":"Numerical analysis of quasinormal modes in nearly extremal Schwarzschild-de Sitter spacetimes","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0308077","snapshot_observed_at":"2026-08-07T04:46:13.405870Z","title":"Yoshida and T","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.405870Z"},"links":{"cited_paper":"/paper/gr-qc/0308077","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:01da028c006414cc620021d3ed806c987db95f5858c8f6b862172bc4d733f949","observation_id":"85aa97ee-c059-4e5f-a005-6fcfafaa4ace","resolution":{"observed_at":"2026-08-07T04:46:13.405870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0402080","last_updated":"2004-07-04T19:10:01Z","snapshot_observed_at":"2026-07-07T04:49:44.402605Z","submitted_at":"2004-02-10T17:02:39Z","title":"High overtones of Schwarzschild-de-Sitter quasinormal spectrum","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0402080","snapshot_observed_at":"2026-08-07T04:46:13.553681Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.553681Z"},"links":{"cited_paper":"/paper/hep-th/0402080","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:177105bf44f63aa8891b92c42ff54477d26c6aef678ce1e58f0fb768a489d49e","observation_id":"fc51b2bd-a7c2-4ff6-a854-e3fdfe016468","resolution":{"observed_at":"2026-08-07T04:46:13.553681Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0301078","last_updated":"2003-02-18T19:19:14Z","snapshot_observed_at":"2026-08-02T01:46:30.218416Z","submitted_at":"2003-01-21T15:30:28Z","title":"Quasinormal modes of the near extremal Schwarzschild-de Sitter black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0301078","snapshot_observed_at":"2026-08-07T04:46:13.643802Z","title":"Cardoso and J","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.643802Z"},"links":{"cited_paper":"/paper/gr-qc/0301078","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:86dc3ad355f7c6d5f9120f8975bbcfedff70085f484bece498268882d4ee0bbe","observation_id":"c0348dd1-f7e8-410c-80e7-541fcdf3cd12","resolution":{"observed_at":"2026-08-07T04:46:13.643802Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.10758","last_updated":"2018-12-05T17:32:43Z","snapshot_observed_at":"2026-07-06T06:58:33.813486Z","submitted_at":"2018-08-31T14:18:57Z","title":"Kerr-(Anti-)de Sitter Black Holes: Perturbations and quasi-normal modes in the slow rotation limit","version":2},"cited_work":{"arxiv_id":"1808.10758","doi":null,"metadata_source":"pith","pith_arxiv_id":"1808.10758","snapshot_observed_at":"2026-08-07T04:46:22.202705Z","title":"Kerr-(Anti-)de Sitter Black Holes: Perturbations and quasi-normal modes in the slow rotation limit","venue":"gr-qc","work_id":"7746222e-02f1-4887-9ae5-02cbd1ceb15b","year":2018},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.712283Z"},"links":{"cited_paper":"/paper/1808.10758","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:f451919060ce3c5ba9ad4a738bae07cc69d0aee87d744c1ca7bd28e17554ee92","observation_id":"970e7388-8f71-4fc1-ad3f-77d427877d05","resolution":{"observed_at":"2026-08-07T04:46:22.302489Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09386","last_updated":"2020-08-01T20:11:25Z","snapshot_observed_at":"2026-07-06T09:13:44.069836Z","submitted_at":"2020-04-20T15:40:23Z","title":"Anomalous decay rate of quasinormal modes in Schwarzschild-dS and Schwarzschild-AdS black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09386","snapshot_observed_at":"2026-08-07T04:46:13.800905Z","title":"Aragón, P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.800905Z"},"links":{"cited_paper":"/paper/2004.09386","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:7970552fdc9244324ce82ec8f886558ded6603f700e87e1d48c56fa9933d64dc","observation_id":"4f602118-3a68-4f75-9c5a-e8c1d9ee8bce","resolution":{"observed_at":"2026-08-07T04:46:13.800905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.02347","last_updated":"2021-05-05T22:07:10Z","snapshot_observed_at":"2026-08-04T19:54:50.697031Z","submitted_at":"2021-05-05T22:07:10Z","title":"Quasinormal modes of small Schwarzschild-de Sitter black holes","version":1},"cited_work":{"arxiv_id":"2105.02347","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.02347","snapshot_observed_at":"2026-08-07T04:46:22.085341Z","title":"Quasinormal modes of small Schwarzschild-de Sitter black holes","venue":"gr-qc","work_id":"e40aa8fe-7225-4c99-b44b-5e3283373445","year":2021},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.887609Z"},"links":{"cited_paper":"/paper/2105.02347","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:31dd3b7b62671c8a7dcac890e6c8148ccd82d88b9c5282be166084a405d6d0a3","observation_id":"5c1cadf1-c666-4176-925f-d367bb3d440f","resolution":{"observed_at":"2026-08-07T04:46:22.137798Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.04858","last_updated":"2022-04-06T15:34:36Z","snapshot_observed_at":"2026-08-03T17:10:09.524628Z","submitted_at":"2021-08-10T18:18:51Z","title":"Analytic formula for quasinormal modes in the near-extreme Kerr-Newman-de Sitter spacetime governed by a non-P\\\"oschl-Teller potential","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.04858","snapshot_observed_at":"2026-08-07T04:46:13.953155Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:13.953155Z"},"links":{"cited_paper":"/paper/2108.04858","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:7ca629ec8dbc211626738808877fb9e717ec8a5643d34057cbda2c5cd71fdbce","observation_id":"bf51958e-6762-451d-b80e-4274710b9c0c","resolution":{"observed_at":"2026-08-07T04:46:13.953155Z","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":"2026-08-07T04:46:14.040522Z","title":"Roussev, Gen","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.040522Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:a7160037a9eb605b0115a6f1e5cc12ed446cd162b88f588c512e4f1de60382ee","observation_id":"adc5053d-9625-4834-b177-6fa0ab8071c9","resolution":{"observed_at":"2026-08-07T04:46:14.040522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0707.1890","last_updated":"2014-10-09T20:26:49Z","snapshot_observed_at":"2026-07-06T01:31:43.670502Z","submitted_at":"2007-07-12T21:53:57Z","title":"Decay of a charged scalar and Dirac fields in the Kerr-Newman-de Sitter background","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0707.1890","snapshot_observed_at":"2026-08-07T04:46:14.129355Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.129355Z"},"links":{"cited_paper":"/paper/0707.1890","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:88f89e483b6451259defa9d27863bae60f2c1eb1022ae3d94cea3195d39ed3ae","observation_id":"b4d861f4-9cc6-4501-a0fb-9591994a635c","resolution":{"observed_at":"2026-08-07T04:46:14.129355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.1260","last_updated":"2011-12-15T00:08:12Z","snapshot_observed_at":"2026-07-06T02:21:41.310032Z","submitted_at":"2011-01-06T17:16:15Z","title":"Asymptotic distribution of quasi-normal modes for Kerr-de Sitter black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.1260","snapshot_observed_at":"2026-08-07T04:46:14.195802Z","title":"Dyatlov, Annales Henri Poincare 13, 1101 (2012), arXiv:1101.1260 [math.AP]","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.195802Z"},"links":{"cited_paper":"/paper/1101.1260","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:e619ceaaa50f7b8f716369de509af5971a943fc7e19b3fae1c27dac0f66b4890","observation_id":"8aedc1f0-8a09-4ee7-a728-8db7ffba1cc2","resolution":{"observed_at":"2026-08-07T04:46:14.195802Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0309030","last_updated":"2003-12-01T13:10:42Z","snapshot_observed_at":"2026-07-07T04:48:09.418534Z","submitted_at":"2003-09-02T17:28:45Z","title":"Gravitational quasinormal radiation of higher-dimensional black holes","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0309030","snapshot_observed_at":"2026-08-07T04:46:14.278818Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.278818Z"},"links":{"cited_paper":"/paper/hep-th/0309030","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:4732b7b79a596183738f171424d572b3e12c137e3dfd80f49c69ac91f9d471f6","observation_id":"6191a0ad-848f-41b6-93ae-adf76c3b30ae","resolution":{"observed_at":"2026-08-07T04:46:14.278818Z","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":"2026-08-07T04:46:14.351055Z","title":"Molina, Phys","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.351055Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:4441c719efff6986cecb35a9de3b3a583772adf48712352d05379b8afdf6bfce","observation_id":"42646d6c-1d0d-4ebe-a660-305034cba861","resolution":{"observed_at":"2026-08-07T04:46:14.351055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.03581","last_updated":"2015-08-14T17:57:17Z","snapshot_observed_at":"2026-07-06T04:26:44.462977Z","submitted_at":"2015-08-14T17:57:17Z","title":"Regular black holes in de Sitter universe: scalar field perturbations and quasinormal modes","version":1},"cited_work":{"arxiv_id":"1508.03581","doi":null,"metadata_source":"pith","pith_arxiv_id":"1508.03581","snapshot_observed_at":"2026-08-07T04:46:21.900066Z","title":"Regular black holes in de Sitter universe: scalar field perturbations and quasinormal modes","venue":"gr-qc","work_id":"bd9ed363-016f-4b29-9e0e-57e44a18e3d7","year":2015},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.407230Z"},"links":{"cited_paper":"/paper/1508.03581","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3fd2859706c8f3de782bb8b433087ef503b9479f9e349a0795a2a2627d731b4c","observation_id":"c512bafc-6139-4a57-abe9-83260ca0ea93","resolution":{"observed_at":"2026-08-07T04:46:21.959650Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0411267","last_updated":"2005-06-27T15:54:03Z","snapshot_observed_at":"2026-07-07T04:52:31.444752Z","submitted_at":"2004-11-29T21:44:40Z","title":"On the Classification of Asymptotic Quasinormal Frequencies for d-Dimensional Black Holes and Quantum Gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0411267","snapshot_observed_at":"2026-08-07T04:46:14.470112Z","title":"Natario and R","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.470112Z"},"links":{"cited_paper":"/paper/hep-th/0411267","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:4d2ff8696be2395b2a1471daa95268ec33b8215e205c48f4766ee60df500f0fe","observation_id":"15f1fd53-dbf6-4983-8c2e-91c9efd4815b","resolution":{"observed_at":"2026-08-07T04:46:14.470112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.2822","last_updated":"2009-07-03T06:23:33Z","snapshot_observed_at":"2026-07-06T01:45:34.472535Z","submitted_at":"2008-09-16T21:59:38Z","title":"Instability of higher dimensional charged black holes in the de-Sitter world","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.2822","snapshot_observed_at":"2026-08-07T04:46:14.546034Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.546034Z"},"links":{"cited_paper":"/paper/0809.2822","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:b1926a36d18fd697e8d3b0af9939c68595129915210e3299147b29e5d742c74a","observation_id":"37f6c59f-1f07-441f-9a5b-6b96269f5b99","resolution":{"observed_at":"2026-08-07T04:46:14.546034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01652","last_updated":"2017-05-15T21:12:13Z","snapshot_observed_at":"2026-07-06T05:25:18.231190Z","submitted_at":"2017-01-06T15:01:48Z","title":"Eikonal instability of Gauss-Bonnet-(anti-)de Sitter black holes","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.01652","snapshot_observed_at":"2026-08-07T04:46:14.642102Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.642102Z"},"links":{"cited_paper":"/paper/1701.01652","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:280e626749c2cc7ff31565b71cbcff72d343e2fb463ebede22edef2e6173c915","observation_id":"b7cf6429-1ad8-41b2-9fef-97f3e901aa01","resolution":{"observed_at":"2026-08-07T04:46:14.642102Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.07419","last_updated":"2017-07-24T06:47:39Z","snapshot_observed_at":"2026-07-06T05:52:21.844797Z","submitted_at":"2017-07-24T06:47:39Z","title":"Slowly decaying resonances of massive scalar fields around Schwarzschild-de Sitter black holes","version":1},"cited_work":{"arxiv_id":"1707.07419","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.07419","snapshot_observed_at":"2026-08-07T04:46:21.764090Z","title":"Slowly decaying resonances of massive scalar fields around Schwarzschild-de Sitter black holes","venue":"gr-qc","work_id":"f67aa490-4537-4e60-875b-90a5458f67f9","year":2017},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.700117Z"},"links":{"cited_paper":"/paper/1707.07419","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:bc4f57b640aa9bf29c292e90a88e71305d4e2cfc7c1184372f23af2d66367687","observation_id":"f1d65e49-c03a-4328-a7b1-3fe485e85118","resolution":{"observed_at":"2026-08-07T04:46:21.820201Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.03604","last_updated":"2016-05-20T16:24:41Z","snapshot_observed_at":"2026-07-06T04:52:39.631930Z","submitted_at":"2016-04-12T22:11:38Z","title":"Quasinormal modes and a new instability of Einstein-Gauss-Bonnet black holes in the de Sitter world","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.03604","snapshot_observed_at":"2026-08-07T04:46:14.787898Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.787898Z"},"links":{"cited_paper":"/paper/1604.03604","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:a5e1095113d8a2e2a705566ab358978e2b745e0745b25cd7e4b7e0a70f77a9a1","observation_id":"5f48722c-5be7-4feb-8d79-d151d509cd9e","resolution":{"observed_at":"2026-08-07T04:46:14.787898Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.7667","last_updated":"2013-12-25T17:18:29Z","snapshot_observed_at":"2026-07-06T03:24:17.847255Z","submitted_at":"2013-09-29T21:08:54Z","title":"Instability of D-dimensional extremally charged Reissner-Nordstrom(-de Sitter) black holes: Extrapolation to arbitrary D","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.7667","snapshot_observed_at":"2026-08-07T04:46:14.854743Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.854743Z"},"links":{"cited_paper":"/paper/1309.7667","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:e2c28a0dfb3e45d2f9d8698c39001b9ce594c568368bec4d9714b36057eb5922","observation_id":"ac7d4ca4-54c9-41ad-b572-b5d39da08f64","resolution":{"observed_at":"2026-08-07T04:46:14.854743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.16134","last_updated":"2025-04-24T08:48:33Z","snapshot_observed_at":"2026-08-05T23:11:35.542944Z","submitted_at":"2025-01-27T15:24:58Z","title":"Quasinormal Ringing and Shadows of Black Holes and Wormholes in Dark Matter-Inspired Weyl Gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.16134","snapshot_observed_at":"2026-08-07T04:46:14.944973Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:14.944973Z"},"links":{"cited_paper":"/paper/2501.16134","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:0dc4a8a12b53b8ce3e35f4b43b5cc2769e2d3ab38d4538a233774ed6dd5d228d","observation_id":"d3d61802-e83d-4eb2-a88d-83e106a406e2","resolution":{"observed_at":"2026-08-07T04:46:14.944973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.18004","last_updated":"2024-04-27T20:43:12Z","snapshot_observed_at":"2026-07-06T18:06:32.549011Z","submitted_at":"2024-04-27T20:43:12Z","title":"Overtones of black holes via time-domain integration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.18004","snapshot_observed_at":"2026-08-07T04:46:15.033597Z","title":"Dubinsky, Mod","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.033597Z"},"links":{"cited_paper":"/paper/2404.18004","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3ef86107a0869b715e0b621608d8a6ff620147101e08ec05cf86ba977d6ec3af","observation_id":"f471fbd9-dcef-4056-9124-0ddfbcbc7921","resolution":{"observed_at":"2026-08-07T04:46:15.033597Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01834","last_updated":"2024-12-31T14:31:02Z","snapshot_observed_at":"2026-07-06T17:54:27.841979Z","submitted_at":"2024-04-02T10:47:01Z","title":"Asymptotic decay and quasinormal frequencies of scalar and Dirac fields around dilaton-de Sitter black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01834","snapshot_observed_at":"2026-08-07T04:46:15.100154Z","title":"Dubinsky and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.100154Z"},"links":{"cited_paper":"/paper/2404.01834","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:0c8a5bf443a9cda380de81e5f56e817acdce88ac3e0d07a22c4afcff6ecab271","observation_id":"3304a563-936a-4ad2-a635-803e7c8b0b41","resolution":{"observed_at":"2026-08-07T04:46:15.100154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.02560","last_updated":"2023-11-10T05:28:00Z","snapshot_observed_at":"2026-08-05T12:21:10.622895Z","submitted_at":"2023-09-05T20:07:39Z","title":"Analytic expressions for quasinormal modes and grey-body factors in the eikonal limit and beyond","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.02560","snapshot_observed_at":"2026-08-07T04:46:15.165007Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.165007Z"},"links":{"cited_paper":"/paper/2309.02560","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:58d11c12c4789caefbbf506345ef4ec569f8bbfa99803f0fe70b41a37e0fa729","observation_id":"b733bac5-e9ca-416d-8ad2-9cf9fc11072d","resolution":{"observed_at":"2026-08-07T04:46:15.165007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.13020","last_updated":"2021-02-18T23:11:14Z","snapshot_observed_at":"2026-08-05T22:58:44.597007Z","submitted_at":"2020-12-23T23:10:04Z","title":"Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior","version":2},"cited_work":{"arxiv_id":"2012.13020","doi":null,"metadata_source":"pith","pith_arxiv_id":"2012.13020","snapshot_observed_at":"2026-08-07T04:46:21.616089Z","title":"Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior","venue":"gr-qc","work_id":"eb69c4d7-180e-447e-aeb8-913c43cbea36","year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.228831Z"},"links":{"cited_paper":"/paper/2012.13020","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:79caa6cf1eb0c2a751fdb88ccdcace21b00cae83afc192601cdb9f1caf9139b4","observation_id":"72310839-8031-43af-b866-b334b44cf9ec","resolution":{"observed_at":"2026-08-07T04:46:21.669162Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0512257","last_updated":"2006-01-23T16:28:55Z","snapshot_observed_at":"2026-08-05T12:11:03.914820Z","submitted_at":"2005-12-20T18:50:27Z","title":"Quasi-Normal Modes of Brane-Localised Standard Model Fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0512257","snapshot_observed_at":"2026-08-07T04:46:15.310496Z","title":"Kanti and R","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.310496Z"},"links":{"cited_paper":"/paper/hep-th/0512257","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:352112c51f94a5a5c138e9e1f413a8a4bfdcd0bf2ed1cd86a7186f011d8dd016","observation_id":"4bca8a91-c024-46b9-a306-43448d5ff25c","resolution":{"observed_at":"2026-08-07T04:46:15.310496Z","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":"2026-08-07T04:46:15.398894Z","title":"Malik, Z","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.398894Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:7e3eb9970f11594a831e64b9dd67758f7bc6d6a118113fd6158c1eb873c50f2a","observation_id":"f987544e-6fbb-4bbc-bc97-410c705b32bf","resolution":{"observed_at":"2026-08-07T04:46:15.398894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.10502","last_updated":"2018-01-11T21:06:57Z","snapshot_observed_at":"2026-08-06T01:22:02.659761Z","submitted_at":"2017-11-28T19:00:06Z","title":"Quasinormal modes and Strong Cosmic Censorship","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.10502","snapshot_observed_at":"2026-08-07T04:46:15.489500Z","title":"Cardoso, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.489500Z"},"links":{"cited_paper":"/paper/1711.10502","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:afe2271112556413bd956f6f2d57e777e24fe4e616a3d1b32c3bd1fb7c7808d0","observation_id":"f5397fc2-76a5-450e-94cc-0f36771fc2b3","resolution":{"observed_at":"2026-08-07T04:46:15.489500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.09694","last_updated":"2018-01-29T19:00:04Z","snapshot_observed_at":"2026-08-05T13:29:40.862335Z","submitted_at":"2018-01-29T19:00:04Z","title":"Strong cosmic censorship in de Sitter space","version":1},"cited_work":{"arxiv_id":"1801.09694","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.09694","snapshot_observed_at":"2026-08-07T04:46:21.461384Z","title":"Strong cosmic censorship in de Sitter space","venue":"gr-qc","work_id":"d1495790-d7af-499b-9b95-a872864f6005","year":2018},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.567864Z"},"links":{"cited_paper":"/paper/1801.09694","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:b6bdf2f1de6838ddae062428e45d72731972336d3924d938258665a18dfad36b","observation_id":"c54fbd07-75cb-4f72-a2b9-fa0c1bcc437c","resolution":{"observed_at":"2026-08-07T04:46:21.538311Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1808.04832","last_updated":"2018-08-29T18:00:34Z","snapshot_observed_at":"2026-07-06T06:55:39.663720Z","submitted_at":"2018-08-14T18:02:07Z","title":"Strong cosmic censorship for charged de Sitter black holes with a charged scalar field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.04832","snapshot_observed_at":"2026-08-07T04:46:15.658891Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.658891Z"},"links":{"cited_paper":"/paper/1808.04832","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:dd2eabdbc69e131de8f2dfff1d2e5f59e75d0ca99567a9cdd6bc618a8e8c267d","observation_id":"c430d93c-3821-45d5-acee-a3664b559947","resolution":{"observed_at":"2026-08-07T04:46:15.658891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.03635","last_updated":"2018-12-08T04:35:24Z","snapshot_observed_at":"2026-08-05T12:13:55.846114Z","submitted_at":"2018-08-10T17:47:21Z","title":"Strong cosmic censorship for the massless charged scalar field in the Reissner-Nordstrom-de Sitter spacetime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.03635","snapshot_observed_at":"2026-08-07T04:46:15.758501Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.758501Z"},"links":{"cited_paper":"/paper/1808.03635","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:81dfd54d62d69560532ad6d518b7f4c691748548f5f0d12b2c2c929401a1de61","observation_id":"8497d2a0-08e7-4d44-9fd1-42c1116f2f80","resolution":{"observed_at":"2026-08-07T04:46:15.758501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.01865","last_updated":"2019-04-01T13:16:47Z","snapshot_observed_at":"2026-07-06T07:31:19.424498Z","submitted_at":"2019-02-05T19:00:02Z","title":"Strong Cosmic Censorship in higher-dimensional Reissner-Nordstr\\\"{o}m-de Sitter spacetime","version":2},"cited_work":{"arxiv_id":"1902.01865","doi":null,"metadata_source":"pith","pith_arxiv_id":"1902.01865","snapshot_observed_at":"2026-08-07T04:46:21.269562Z","title":"Strong Cosmic Censorship in higher-dimensional Reissner-Nordstr\\\"{o}m-de Sitter spacetime","venue":"gr-qc","work_id":"f40d27ff-52bf-4f40-90fc-1ef7c97eb67c","year":2019},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.823424Z"},"links":{"cited_paper":"/paper/1902.01865","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:afde5369de987b34fa1415101048438c18e2316e00c2c71f19b928a02986af0c","observation_id":"3bb03711-04e8-438e-a3bf-315b8e7a4c9e","resolution":{"observed_at":"2026-08-07T04:46:21.305864Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.01449","last_updated":"2020-12-02T19:00:07Z","snapshot_observed_at":"2026-08-08T04:03:07.118602Z","submitted_at":"2020-12-02T19:00:07Z","title":"A proof of the strong cosmic censorship conjecture","version":1},"cited_work":{"arxiv_id":"2012.01449","doi":null,"metadata_source":"pith","pith_arxiv_id":"2012.01449","snapshot_observed_at":"2026-08-07T04:46:21.119737Z","title":"A proof of the strong cosmic censorship conjecture","venue":"gr-qc","work_id":"a778a9c9-f358-4f71-a452-ef9a908481f6","year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.902090Z"},"links":{"cited_paper":"/paper/2012.01449","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:58d7e7152609b45c2dfc86add51c7333291f117a71a1b076880bf1ed858417c5","observation_id":"cf335d78-b883-42da-a099-3a11de85c22c","resolution":{"observed_at":"2026-08-07T04:46:21.215634Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T04:46:15.966161Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:15.966161Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3a575cf71524bae643ac315ec55f9aa9cd330714a71538f333504b4ddd6907f5","observation_id":"acc69dab-6f86-4948-a8f6-1144aaeeec3c","resolution":{"observed_at":"2026-08-07T04:46:15.966161Z","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":"qc/9611056","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T04:46:20.938020Z","title":null,"venue":null,"work_id":"b0dbfd55-0051-4832-99e7-183c96d54492","year":1997},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.032296Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:167724d988240611acdb2f779e5f6b087bb237a73761294f18ce4506d0529977","observation_id":"ca58c0d4-f0e2-4b0d-97fb-0e009c4f06fd","resolution":{"observed_at":"2026-08-07T04:46:21.009430Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"qc/9902010","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T04:46:20.750667Z","title":null,"venue":null,"work_id":"050c84a2-e59f-411c-9e3d-0684d04e1c53","year":1999},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.079983Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:ef2f37fcbe1c488527a22839f603909c279d7c0f560c0475bb42f2cccab558f0","observation_id":"53de836f-77c0-494f-890e-3183cd827937","resolution":{"observed_at":"2026-08-07T04:46:20.812357Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0309079","last_updated":"2006-04-09T00:24:41Z","snapshot_observed_at":"2026-07-07T03:18:20.366191Z","submitted_at":"2003-09-17T18:11:41Z","title":"Field propagation in de Sitter black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0309079","snapshot_observed_at":"2026-08-07T04:46:16.130312Z","title":"Molina, D","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.130312Z"},"links":{"cited_paper":"/paper/gr-qc/0309079","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:87678f1f181ed41a198adea3411505d5de99292b6462d1a0012bb99f8e32b556","observation_id":"158dfe00-a9b3-4198-bd13-f81c882efacf","resolution":{"observed_at":"2026-08-07T04:46:16.130312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.12058","last_updated":"2022-12-02T15:30:33Z","snapshot_observed_at":"2026-07-06T13:55:52.772660Z","submitted_at":"2022-09-24T17:56:38Z","title":"Nonoscillatory gravitational quasinormal modes and telling tails for Schwarzschild-de Sitter black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.12058","snapshot_observed_at":"2026-08-07T04:46:16.178978Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.178978Z"},"links":{"cited_paper":"/paper/2209.12058","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:2aa6068b0979b86d0be1a2ca3d5881b480f8549e2f35db590d0a717fd452df12","observation_id":"af77fcd1-5174-46c9-8634-76d4d2b6f729","resolution":{"observed_at":"2026-08-07T04:46:16.178978Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.17106","last_updated":"2024-04-15T15:02:15Z","snapshot_observed_at":"2026-07-06T17:22:33.187222Z","submitted_at":"2024-01-30T15:42:17Z","title":"Two Regimes of Asymptotic Fall-off of a Massive Scalar Field in the Schwarzschild-de Sitter Spacetime","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.17106","snapshot_observed_at":"2026-08-07T04:46:16.229167Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.229167Z"},"links":{"cited_paper":"/paper/2401.17106","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:0c431ac1714a0394f6896559db8ed0c882118126b357df0e2f4f422b9bad12e9","observation_id":"ea82f203-5f75-4f0d-b611-7565e3c334c0","resolution":{"observed_at":"2026-08-07T04:46:16.229167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0605022","last_updated":"2006-05-03T08:40:51Z","snapshot_observed_at":"2026-07-07T03:22:29.311647Z","submitted_at":"2006-05-03T08:40:51Z","title":"Absorption and quasinormal modes of classical fields propagating on 3D and 4D de Sitter spacetime","version":1},"cited_work":{"arxiv_id":"gr-qc/0605022","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0605022","snapshot_observed_at":"2026-08-07T04:46:20.477865Z","title":"Absorption and quasinormal modes of classical fields propagating on 3D and 4D de Sitter spacetime","venue":"gr-qc","work_id":"74cdbdec-16b3-434b-a6ed-c1ed4063360c","year":2006},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.293669Z"},"links":{"cited_paper":"/paper/gr-qc/0605022","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:f0bff3f2443568e685f2541c6db527cf54b8c8305938fa7eb4c240b862fe857f","observation_id":"81f25fc9-d429-4a2b-adc9-7ad105b9afbe","resolution":{"observed_at":"2026-08-07T04:46:20.555514Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0605027","last_updated":"2006-11-02T10:03:02Z","snapshot_observed_at":"2026-07-07T03:22:29.311647Z","submitted_at":"2006-05-04T19:24:35Z","title":"Quasinormal modes of D-dimensional de Sitter spacetime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0605027","snapshot_observed_at":"2026-08-07T04:46:16.343447Z","title":"Lopez-Ortega, Gen","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.343447Z"},"links":{"cited_paper":"/paper/gr-qc/0605027","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:a9ab272637d0c1824f93b3fa62ad7d4a3dd3dab29cd5c6d565fc8635ac004a90","observation_id":"80921bb0-be3a-4311-9ac6-5f181b908684","resolution":{"observed_at":"2026-08-07T04:46:16.343447Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.09178","last_updated":"2017-11-17T10:03:11Z","snapshot_observed_at":"2026-07-06T06:01:28.504872Z","submitted_at":"2017-09-26T18:00:04Z","title":"Overdamped modes in Schwarzschild-de Sitter and a Mathematica package for the numerical computation of quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.09178","snapshot_observed_at":"2026-08-07T04:46:16.394424Z","title":"Jansen, Eur","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.394424Z"},"links":{"cited_paper":"/paper/1709.09178","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:c06a789a3c2efea5d9d6dcbcfe6159558354061b9e3bfdc01d649f182fe69e56","observation_id":"2a81beb8-6fb1-4619-9643-f4c374a47253","resolution":{"observed_at":"2026-08-07T04:46:16.394424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.08373","last_updated":"2022-10-20T12:55:34Z","snapshot_observed_at":"2026-08-07T01:38:47.750616Z","submitted_at":"2022-10-15T20:51:21Z","title":"Further clarification on quasinormal modes/circular null geodesics correspondence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.08373","snapshot_observed_at":"2026-08-07T04:46:16.443823Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.443823Z"},"links":{"cited_paper":"/paper/2210.08373","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:dcec4b71288f9af0a029e611e86d18712d505e5d1ab01bae8effaba4cef68d7f","observation_id":"12a19269-5bf1-4315-a616-d25ee57d001b","resolution":{"observed_at":"2026-08-07T04:46:16.443823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0305147","last_updated":"2003-09-30T06:11:26Z","snapshot_observed_at":"2026-07-07T04:47:05.917349Z","submitted_at":"2003-05-16T21:26:36Z","title":"A master equation for gravitational perturbations of maximally symmetric black holes in higher dimensions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0305147","snapshot_observed_at":"2026-08-07T04:46:16.495958Z","title":"Kodama and A","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.495958Z"},"links":{"cited_paper":"/paper/hep-th/0305147","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:09fd2aa1cbe5ccd508363bc4bd7cba9f138ae6e2bc1aa547de5fde87c5e63936","observation_id":"370da43e-d97d-4116-a0e0-2d56c473a08b","resolution":{"observed_at":"2026-08-07T04:46:16.495958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0305185","last_updated":"2003-10-23T15:32:58Z","snapshot_observed_at":"2026-07-07T04:47:11.406820Z","submitted_at":"2003-05-20T20:00:30Z","title":"Stability of Higher-Dimensional Schwarzschild Black Holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0305185","snapshot_observed_at":"2026-08-07T04:46:16.554632Z","title":"Ishibashi and H","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.554632Z"},"links":{"cited_paper":"/paper/hep-th/0305185","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:d5634861037750b3822520573eb6f5687304278cc73d403640783bbcf9efb209","observation_id":"4f6089ff-db70-44f4-94a7-3023baa54b7a","resolution":{"observed_at":"2026-08-07T04:46:16.554632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0308128","last_updated":"2004-03-02T06:22:39Z","snapshot_observed_at":"2026-08-02T19:32:59.820078Z","submitted_at":"2003-08-20T09:22:21Z","title":"Master equations for perturbations of generalised static black holes with charge in higher dimensions","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0308128","snapshot_observed_at":"2026-08-07T04:46:16.604343Z","title":"Kodama and A","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.604343Z"},"links":{"cited_paper":"/paper/hep-th/0308128","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:0fd1dc165fb8d36fd8804c6c2ade3c3b0a425a9697c770a50065bc1d7b43ee24","observation_id":"d915492a-65c2-4a38-a02d-ebc325e98df0","resolution":{"observed_at":"2026-08-07T04:46:16.604343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.2685","last_updated":"2008-03-18T17:45:56Z","snapshot_observed_at":"2026-07-06T01:39:37.535418Z","submitted_at":"2008-03-18T17:45:56Z","title":"Properties of the Reissner-Nordstr\\\"om Spacetimes with a Nonzero Cosmological Constant","version":1},"cited_work":{"arxiv_id":"0803.2685","doi":null,"metadata_source":"pith","pith_arxiv_id":"0803.2685","snapshot_observed_at":"2026-08-07T04:46:20.286947Z","title":"Properties of the Reissner-Nordstr\\\"om Spacetimes with a Nonzero Cosmological Constant","venue":"gr-qc","work_id":"caca354a-e797-408b-98aa-340065cbb372","year":2008},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.658252Z"},"links":{"cited_paper":"/paper/0803.2685","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:32fed5b82dac74bf6ea8feb11dcb583dac69fd79965d780f46d71c0df9979298","observation_id":"d1794f16-4dec-4faf-a4f1-140ce64ab263","resolution":{"observed_at":"2026-08-07T04:46:20.350085Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T04:46:16.712251Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.712251Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:79adb68b32c6da0a66a1a8e9a5942101f977a0ca6de3d3a2e52e647b3b741a86","observation_id":"f490b24a-6da4-49db-85ae-7152d9487f59","resolution":{"observed_at":"2026-08-07T04:46:16.712251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9307009","last_updated":"1993-07-12T16:15:51Z","snapshot_observed_at":"2026-07-07T03:24:16.543366Z","submitted_at":"1993-07-10T17:11:26Z","title":"Late-Time Behavior of Stellar Collapse and Explosions: I. Linearized Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9307009","snapshot_observed_at":"2026-08-07T04:46:16.761811Z","title":"Gundlach, R","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.761811Z"},"links":{"cited_paper":"/paper/gr-qc/9307009","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:10de91110903dc5b845467a7048ec5b0462e899d198a935d2470194bb412695f","observation_id":"d3efcc48-8908-4f7e-b662-9702026787fe","resolution":{"observed_at":"2026-08-07T04:46:16.761811Z","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":"2026-08-07T04:46:16.821140Z","title":"Nollert, Phys","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.821140Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:e463c48273a4396bad629eaa1e2f19e4a0b7e91064571485083bf5c6e41d8efd","observation_id":"573757f6-a93f-4d81-8a0e-86b9a07cbc70","resolution":{"observed_at":"2026-08-07T04:46:16.821140Z","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":"2026-08-07T04:46:16.873729Z","title":"Zhidenko, Phys","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.873729Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:8c1108a91e5073b34e56a8680448887651e9070484e4031713cd4dcda2739b60","observation_id":"f3ff16e4-baeb-4c69-b027-a2eaf04b7437","resolution":{"observed_at":"2026-08-07T04:46:16.873729Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10801","last_updated":"2023-07-20T12:09:19Z","snapshot_observed_at":"2026-07-06T15:56:25.975005Z","submitted_at":"2023-07-20T12:09:19Z","title":"Bardeen spacetime as a quantum corrected Schwarzschild black hole: Quasinormal modes and Hawking radiation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10801","snapshot_observed_at":"2026-08-07T04:46:16.928747Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.928747Z"},"links":{"cited_paper":"/paper/2307.10801","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:7a785617507f25b1588858ecf5452dbedfd6f6a3c46c9ee981a43ccde9816b6b","observation_id":"79cfe8a9-f8f7-4b15-a96c-e133ec5834ef","resolution":{"observed_at":"2026-08-07T04:46:16.928747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.14506","last_updated":"2023-04-13T12:47:03Z","snapshot_observed_at":"2026-07-06T14:10:32.433250Z","submitted_at":"2022-10-26T06:32:52Z","title":"Quasinormal modes in higher derivative gravity: testing the black hole parametrization and sensitivity of overtones","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.14506","snapshot_observed_at":"2026-08-07T04:46:16.994175Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:16.994175Z"},"links":{"cited_paper":"/paper/2210.14506","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:0afac254cc7b2ba8df38c014f920381a433cde6ffd2f5bc77751899d0cab89aa","observation_id":"6dd21b6e-03e5-41f1-aba3-7e92725aba1c","resolution":{"observed_at":"2026-08-07T04:46:16.994175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.06867","last_updated":"2024-03-11T16:21:55Z","snapshot_observed_at":"2026-08-08T00:19:53.063294Z","submitted_at":"2024-03-11T16:21:55Z","title":"Exploring Unique Quasinormal Modes of a Massive Scalar Field in Brane-World Scenarios","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.06867","snapshot_observed_at":"2026-08-07T04:46:17.059422Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.059422Z"},"links":{"cited_paper":"/paper/2403.06867","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:be4047eee80336357f4d5481636e39b7fe5745cf7a5b62a38e76b703b132a172","observation_id":"7beefa3d-e964-470f-b778-36f26337e75a","resolution":{"observed_at":"2026-08-07T04:46:17.059422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.05503","last_updated":"2023-11-01T10:08:36Z","snapshot_observed_at":"2026-07-06T16:45:20.005195Z","submitted_at":"2023-11-01T10:08:36Z","title":"Long-lived quasinormal modes and overtones' behavior of the holonomy corrected black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.05503","snapshot_observed_at":"2026-08-07T04:46:17.125242Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.125242Z"},"links":{"cited_paper":"/paper/2311.05503","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:9380f509d9d6b55d54d37a2422b5b9a4cef9a333208c85fa56fca2aac82bea5d","observation_id":"075bedc9-f7a7-402e-94dc-8aee9b49de0a","resolution":{"observed_at":"2026-08-07T04:46:17.125242Z","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":"2026-08-07T04:46:17.188979Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.188979Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:a1fa96b702a191d36b5a5d8080c11bbcf50b419af4275fe02e864109ae2edf18","observation_id":"3eeab90a-b742-4bb0-ac15-31b517967215","resolution":{"observed_at":"2026-08-07T04:46:17.188979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.02578","last_updated":"2024-11-27T00:11:38Z","snapshot_observed_at":"2026-07-06T18:57:01.474525Z","submitted_at":"2024-08-05T15:55:47Z","title":"Probing the Effective Quantum Gravity via Quasinormal Modes and Shadows of Black Holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.02578","snapshot_observed_at":"2026-08-07T04:46:17.254347Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.254347Z"},"links":{"cited_paper":"/paper/2408.02578","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:1d9b33a77cb747f26168eff13ade7064c773128b6690673b7e750ad178893495","observation_id":"299da09f-ca6f-4bc8-89bf-8e64cb3662a6","resolution":{"observed_at":"2026-08-07T04:46:17.254347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.05689","last_updated":"2025-05-28T21:22:04Z","snapshot_observed_at":"2026-08-02T01:09:26.560822Z","submitted_at":"2025-02-08T20:44:31Z","title":"Transition from Regular Black Holes to Wormholes in Covariant Effective Quantum Gravity: Scattering, Quasinormal Modes, and Hawking Radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.05689","snapshot_observed_at":"2026-08-07T04:46:17.323659Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.323659Z"},"links":{"cited_paper":"/paper/2502.05689","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:0dd7ae63123e43d10dc27a3c34d602e4d71e96d052be3e7ef12b7a6122a0c221","observation_id":"3f2d4b0b-7286-484e-bddc-44984268bd3f","resolution":{"observed_at":"2026-08-07T04:46:17.323659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.08262","last_updated":"2024-05-14T01:40:14Z","snapshot_observed_at":"2026-07-06T18:13:55.543513Z","submitted_at":"2024-05-14T01:40:14Z","title":"Quasinormal modes of charged black holes in Asymptotically Safe Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.08262","snapshot_observed_at":"2026-08-07T04:46:17.387811Z","title":"Dubinsky, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.387811Z"},"links":{"cited_paper":"/paper/2405.08262","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3a7d0973f96a5cb08c31f6fa264d07fdcbf4bf036e61c532ce9b8acb24409225","observation_id":"0e4b3b85-ab01-4795-afa7-c4ed63c56e54","resolution":{"observed_at":"2026-08-07T04:46:17.387811Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04477","last_updated":"2022-10-16T21:35:15Z","snapshot_observed_at":"2026-08-07T18:37:19.365650Z","submitted_at":"2022-03-09T01:37:21Z","title":"On the late-time tails of massive perturbations in spherically symmetric black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.04477","snapshot_observed_at":"2026-08-07T04:46:17.453383Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.453383Z"},"links":{"cited_paper":"/paper/2203.04477","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:ea8eca35c77670f410e25c4c4bd0f802e6235a8e0a5d5aa45351b63e9d72add0","observation_id":"4078b4d7-1fe1-407d-9964-3bdfe92481b5","resolution":{"observed_at":"2026-08-07T04:46:17.453383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.10204","last_updated":"2018-05-29T06:31:51Z","snapshot_observed_at":"2026-07-06T06:30:28.648560Z","submitted_at":"2018-03-27T17:41:04Z","title":"Gravitational waves from quasinormal modes of a class of Lorentzian wormholes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.10204","snapshot_observed_at":"2026-08-07T04:46:17.520334Z","title":"Aneesh, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.520334Z"},"links":{"cited_paper":"/paper/1803.10204","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:f3ec57ce0e853890f8a48856fe1d8fc3eef6b1ad6ccf480d9d75ec4324bbf5b1","observation_id":"68e35209-76b8-45cb-9b24-869c7767bbee","resolution":{"observed_at":"2026-08-07T04:46:17.520334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.09187","last_updated":"2023-06-20T18:52:54Z","snapshot_observed_at":"2026-08-08T04:14:58.938832Z","submitted_at":"2023-05-16T05:50:52Z","title":"Quasinormal modes and grey-body factors of regular black holes with a scalar hair from the Effective Field Theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.09187","snapshot_observed_at":"2026-08-07T04:46:17.604423Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.604423Z"},"links":{"cited_paper":"/paper/2305.09187","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:928199fdd571ca833e5288e4f5170cb9a44f766b664f538cbc56ec26ac39a501","observation_id":"f6731bc2-3a67-4ad6-9f89-6253df7281c4","resolution":{"observed_at":"2026-08-07T04:46:17.604423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.10679","last_updated":"2021-11-19T11:40:30Z","snapshot_observed_at":"2026-07-06T10:43:18.171677Z","submitted_at":"2021-02-21T20:44:41Z","title":"General parametrization of wormhole spacetimes and its application to shadows and quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.10679","snapshot_observed_at":"2026-08-07T04:46:17.691864Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.691864Z"},"links":{"cited_paper":"/paper/2102.10679","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:89787c8151e14dd1a5cdb9aee92bf740a92b21aa7d9f881be7b56e9e82d9950f","observation_id":"1e39afe9-6db9-44cd-932e-38d52663dd1b","resolution":{"observed_at":"2026-08-07T04:46:17.691864Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.11650","last_updated":"2023-11-20T10:34:25Z","snapshot_observed_at":"2026-08-07T16:57:44.818162Z","submitted_at":"2023-11-20T10:34:25Z","title":"Quasinormal spectrum of $(2+1)$-dimensional asymptotically flat, dS and AdS black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.11650","snapshot_observed_at":"2026-08-07T04:46:17.779922Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.779922Z"},"links":{"cited_paper":"/paper/2311.11650","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:99dfd4101929099aa8b798a3fe2438ca1914b65c5ff943633983f16e291195d9","observation_id":"caced46a-a075-490f-9f97-a438771614d0","resolution":{"observed_at":"2026-08-07T04:46:17.779922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-04T15:24:05.069161Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-07T04:46:17.866596Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.866596Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:b49f2c1553196f127a25058f38110542f9ea402ad0d8e68923ba8ce0d8aebdd9","observation_id":"9ed3de29-3a7b-4b13-9265-184bd5f0de49","resolution":{"observed_at":"2026-08-07T04:46:17.866596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05315","last_updated":"2019-12-11T13:56:52Z","snapshot_observed_at":"2026-07-06T08:43:44.231510Z","submitted_at":"2019-12-11T13:56:52Z","title":"Echoes in brane worlds: ringing at a black hole--wormhole transition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05315","snapshot_observed_at":"2026-08-07T04:46:17.932855Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:17.932855Z"},"links":{"cited_paper":"/paper/1912.05315","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:806f2258c5f29d73c9670067f8ed9d39042295095b4ba8549f036e342dcfed90","observation_id":"a910d399-af15-473c-bbbf-3233890eb30a","resolution":{"observed_at":"2026-08-07T04:46:17.932855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.04306","last_updated":"2024-10-05T23:05:07Z","snapshot_observed_at":"2026-07-06T19:28:30.731752Z","submitted_at":"2024-10-05T23:05:07Z","title":"Analytical QNMs of fields of various spin in the Hayward spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.04306","snapshot_observed_at":"2026-08-07T04:46:18.045373Z","title":"Malik, EPL 147, 69001 (2024), arXiv:2410.04306 [gr- qc]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.045373Z"},"links":{"cited_paper":"/paper/2410.04306","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:b636ec82ae7699b37cf206e2f2205dd1895ea710f16f6ec3cdf30b32e029a157","observation_id":"070a27f4-f3c0-414a-991a-03f48dad63f3","resolution":{"observed_at":"2026-08-07T04:46:18.045373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.09872","last_updated":"2024-09-15T21:31:43Z","snapshot_observed_at":"2026-07-06T19:15:43.173430Z","submitted_at":"2024-09-15T21:31:43Z","title":"Quasinormal Modes of Dilaton Black Holes: Analytic approximations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.09872","snapshot_observed_at":"2026-08-07T04:46:18.058409Z","title":"Malik, Int","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.058409Z"},"links":{"cited_paper":"/paper/2409.09872","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3be84927d836d0e8581d66c7275051b694c7f3de6951c6ae50e2675609195479","observation_id":"2bc4fc95-e3fb-4db3-b768-b536cb762112","resolution":{"observed_at":"2026-08-07T04:46:18.058409Z","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":"2026-08-07T04:46:18.127127Z","title":"Malik, Int","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.127127Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:d7c5621ec7caddfaa20c2fd4413ee2a9226c993c449409d0a664ee7e70ec07e6","observation_id":"48335ba6-3702-47eb-bb98-918fd262fe5f","resolution":{"observed_at":"2026-08-07T04:46:18.127127Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03929","last_updated":"2025-01-02T13:43:29Z","snapshot_observed_at":"2026-07-06T18:26:23.994796Z","submitted_at":"2024-06-06T10:12:02Z","title":"Quasinormal ringing of thick braneworlds with a finite extra dimension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03929","snapshot_observed_at":"2026-08-07T04:46:18.207093Z","title":"Jia, W.-D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.207093Z"},"links":{"cited_paper":"/paper/2406.03929","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:8e851f99e9d241a468e49701a0edf6d2b3c14f41881b0c69038868781d86f45a","observation_id":"f5a1cb54-e5ba-4265-9fe2-c33d89710b59","resolution":{"observed_at":"2026-08-07T04:46:18.207093Z","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":"2026-08-07T04:46:18.294992Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.294992Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:bfac19470300ca8216e7f401c60e75f63997f3a24aa482d2e09f74700fe50387","observation_id":"19754012-058a-48be-88e1-5e14a64862ad","resolution":{"observed_at":"2026-08-07T04:46:18.294992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.1806","last_updated":"2009-03-12T00:13:05Z","snapshot_observed_at":"2026-08-01T19:42:55.991469Z","submitted_at":"2008-12-09T21:38:26Z","title":"Geodesic stability, Lyapunov exponents and quasinormal modes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.1806","snapshot_observed_at":"2026-08-07T04:46:18.380123Z","title":"Cardoso, A","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.380123Z"},"links":{"cited_paper":"/paper/0812.1806","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:522350b3ff33d6f73d758b0b87087ef433f0a7de87b30a369259d52cdc2b6a7c","observation_id":"ac7e2a98-0f0c-4c5e-823e-7ee7f65e6e65","resolution":{"observed_at":"2026-08-07T04:46:18.380123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.01128","last_updated":"2025-05-02T09:11:02Z","snapshot_observed_at":"2026-08-07T15:57:07.019051Z","submitted_at":"2025-05-02T09:11:02Z","title":"Time Evolution of Black Hole Perturbations in Quadratic Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.01128","snapshot_observed_at":"2026-08-07T04:46:18.474168Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.474168Z"},"links":{"cited_paper":"/paper/2505.01128","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:ae2a1c045ab24e5511e3c145f2e6f0c120e36336d2929ba89b78d3774c75c723","observation_id":"5342a943-4fc7-4f51-8f43-c3c29a1eb13a","resolution":{"observed_at":"2026-08-07T04:46:18.474168Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.05928","last_updated":"2017-06-01T22:35:22Z","snapshot_observed_at":"2026-07-06T05:42:58.053337Z","submitted_at":"2017-05-16T21:35:48Z","title":"Are eikonal quasinormal modes linked to the unstable circular null geodesics?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.05928","snapshot_observed_at":"2026-08-07T04:46:18.586819Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.586819Z"},"links":{"cited_paper":"/paper/1705.05928","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:6bf5388676e640ff04f4d912cebd97aa442cab70ce71b8885398f3e42473c66e","observation_id":"c799131c-8bd1-446d-9608-1dec0cffc852","resolution":{"observed_at":"2026-08-07T04:46:18.586819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.01188","last_updated":"2020-11-13T06:46:13Z","snapshot_observed_at":"2026-07-31T15:15:49.111443Z","submitted_at":"2020-03-02T21:01:48Z","title":"Quasinormal modes, stability and shadows of a black hole in the 4D Einstein-Gauss-Bonnet gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.01188","snapshot_observed_at":"2026-08-07T04:46:18.646858Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.646858Z"},"links":{"cited_paper":"/paper/2003.01188","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:00a0d4c1eea9fffc2ba138e91a79656072b143f5c764ae0a68245eeb8cb0b712","observation_id":"d96a65c9-7d2f-4c57-8135-6c6d89c76286","resolution":{"observed_at":"2026-08-07T04:46:18.646858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.03778","last_updated":"2019-03-09T10:52:18Z","snapshot_observed_at":"2026-07-06T07:38:10.235807Z","submitted_at":"2019-03-09T10:52:18Z","title":"Relaxations of perturbations of spacetimes in general relativity coupled to nonlinear electrodynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.03778","snapshot_observed_at":"2026-08-07T04:46:18.749297Z","title":"Toshmatov, Z","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.749297Z"},"links":{"cited_paper":"/paper/1903.03778","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:132f8f5fbfea5709e826397847128e0b7a6d002bd4505e7d66d25db99e5e14e7","observation_id":"c5b99938-45f8-4142-8dd0-f92d19b928f7","resolution":{"observed_at":"2026-08-07T04:46:18.749297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.04314","last_updated":"2022-11-16T00:38:11Z","snapshot_observed_at":"2026-07-06T14:02:49.856728Z","submitted_at":"2022-10-09T18:21:50Z","title":"How general is the strong cosmic censorship bound for quasinormal modes?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.04314","snapshot_observed_at":"2026-08-07T04:46:18.803328Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.803328Z"},"links":{"cited_paper":"/paper/2210.04314","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:3c3611c989ef50dc3c67275cd4be58e4e5aa22d32b4e0e022481922a284a571e","observation_id":"6dcdf0c7-0c79-403c-958d-a8bb3a84bf01","resolution":{"observed_at":"2026-08-07T04:46:18.803328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.4931","last_updated":"2014-08-31T15:57:09Z","snapshot_observed_at":"2026-08-07T07:53:03.487332Z","submitted_at":"2014-05-20T01:42:02Z","title":"Stability of Reissner-Nordstr\\\"om black hole in de Sitter background under charged scalar perturbation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.4931","snapshot_observed_at":"2026-08-07T04:46:18.900467Z","title":"Zhu, S.-J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:18.900467Z"},"links":{"cited_paper":"/paper/1405.4931","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:e9b66c2d32adce1b0962adfcc9dc6395ebf00b009855ea162e30f79b44c57957","observation_id":"997fe414-85f2-4cc0-acd8-2c5f76d85883","resolution":{"observed_at":"2026-08-07T04:46:18.900467Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.12722","last_updated":"2020-05-26T13:47:27Z","snapshot_observed_at":"2026-07-06T09:23:23.891393Z","submitted_at":"2020-05-26T13:47:27Z","title":"Relaxation rate of RNdS black hole","version":1},"cited_work":{"arxiv_id":"2005.12722","doi":null,"metadata_source":"pith","pith_arxiv_id":"2005.12722","snapshot_observed_at":"2026-08-07T04:46:19.922108Z","title":"Relaxation rate of RNdS black hole","venue":"gr-qc","work_id":"aa8cbfa2-f4d8-4c98-8a76-a182dd8546a0","year":2020},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:19.006921Z"},"links":{"cited_paper":"/paper/2005.12722","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:6ced1498df4ddac996e0dab5949a56fd3a910f2f020c17f41ff8458f3ec3c3cf","observation_id":"b41ce4ea-d629-4b8c-b08c-04d88451d0e8","resolution":{"observed_at":"2026-08-07T04:46:20.001899Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.10620","last_updated":"2021-02-03T13:23:15Z","snapshot_observed_at":"2026-08-08T04:03:35.094500Z","submitted_at":"2020-11-20T20:24:16Z","title":"Anomalous decay rate of quasinormal modes in Reissner-Nordstr\\\"om black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.10620","snapshot_observed_at":"2026-08-07T04:46:19.099454Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:19.099454Z"},"links":{"cited_paper":"/paper/2011.10620","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:61dfd54dc4c7ef782a6d82a6022357fd4a295f140fbc926d245cd5ea4c1ec8dc","observation_id":"b4d831c4-b68f-4bb8-96ab-49d2730194aa","resolution":{"observed_at":"2026-08-07T04:46:19.099454Z","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":"2026-08-07T04:46:19.159824Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:19.159824Z"},"links":{"citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:a9465d3facce5aedfd3b70f82e41350ba64fa27a0bf37f4aaca9891d90b802c6","observation_id":"d96b547a-e363-477c-994c-0b122c9d531c","resolution":{"observed_at":"2026-08-07T04:46:19.159824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.07311","last_updated":"2023-10-11T08:47:38Z","snapshot_observed_at":"2026-07-06T16:31:08.082416Z","submitted_at":"2023-10-11T08:47:38Z","title":"Reissner-Nordstr\\\"om black holes in de Sitter space-time: bounds with quasinormal frequencies","version":1},"cited_work":{"arxiv_id":"2310.07311","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.07311","snapshot_observed_at":"2026-08-07T04:46:19.735909Z","title":"Reissner-Nordstr\\\"om black holes in de Sitter space-time: bounds with quasinormal frequencies","venue":"gr-qc","work_id":"fcc88ba0-5e85-4a17-9378-08409a49bbfc","year":2023},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:19.271655Z"},"links":{"cited_paper":"/paper/2310.07311","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:f2ff3512f36e5f3ca964e70a6f8ad821ed592ea067b5e7a152d9eff39ca2325d","observation_id":"cf5e9e70-30ad-406c-be9d-5a83913d75ba","resolution":{"observed_at":"2026-08-07T04:46:19.829981Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.14834","last_updated":"2025-01-23T14:58:58Z","snapshot_observed_at":"2026-07-06T20:25:49.871084Z","submitted_at":"2025-01-23T14:58:58Z","title":"Quasinormal frequencies in Reissner-Nordstr\\\"om de Sitter black holes: constraints from space-time and scalar field parameters","version":1},"cited_work":{"arxiv_id":"2501.14834","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.14834","snapshot_observed_at":"2026-08-07T04:46:19.481962Z","title":"Quasinormal frequencies in Reissner-Nordstr\\\"om de Sitter black holes: constraints from space-time and scalar field parameters","venue":"gr-qc","work_id":"a9781aaa-4abf-45f4-aae4-36f3d5c5213c","year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:19.327259Z"},"links":{"cited_paper":"/paper/2501.14834","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:92269c83ddc8c86790dad36d8c9bc735429ff7b6336bccc3d21aec597c2a35aa","observation_id":"3e10bbcd-e43c-41b8-bf5f-17ac4746ab0f","resolution":{"observed_at":"2026-08-07T04:46:19.616875Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.18359","last_updated":"2025-06-06T03:54:35Z","snapshot_observed_at":"2026-08-07T18:31:55.643321Z","submitted_at":"2024-12-24T11:43:08Z","title":"Notes on Quasinormal Modes of charged de Sitter Blackholes from Quiver Gauge Theories","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.18359","snapshot_observed_at":"2026-08-07T04:46:19.408879Z","title":"Liu and R.-D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-07T04:46:19.408879Z"},"links":{"cited_paper":"/paper/2412.18359","citing_paper":"/paper/2506.09829"},"observation_digest":"sha256:9c382e6c0eab71d33142607ac5c6a95c9ca1b90054879ec6a08fbdb0650f4a55","observation_id":"9c383836-656a-41b8-bf2a-5e5c99d7a7bf","resolution":{"observed_at":"2026-08-07T04:46:19.408879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2506.09829","last_updated":"2025-06-11T15:08:21Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-07T16:54:07.609404Z","submitted_at":"2025-06-11T15:08:21Z","title":"Non-oscillatory gravitational quasinormal modes of Reissner-Nordstr\\\"om-de Sitter spacetime"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":85,"verified_exact":15,"verified_fuzzy":0},"total_outbound_references":100},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 100 of 100 outbound references and 8 inbound Pith citation observations for arXiv:2506.09829."}