{"as_of":"2026-08-12T04:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2134bef408ac8454a2887cee00919f28b30ca84ad868ab7924dee29decebae4f","coverage":[{"denominator":83,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":83,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T13:24:44.606464Z","state":"measured"},{"denominator":97,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":97,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-29T23:58:23.049086Z","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":"2026-06-30T00:04:06.159981Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2501.16433","last_updated":"2026-05-13T15:28:20Z","snapshot_observed_at":"2026-08-02T14:23:16.098022Z","submitted_at":"2025-01-27T19:00:06Z","title":"Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects","version":3},"reference_index":124,"source":"pdf_text","source_observed_at":"2026-05-23T04:43:04.006726Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2501.16433"},"observation_digest":"sha256:4326aba866ab7f505bdfb1caa6eee7df535e7841b394405cbc16e7198b22d4bd","observation_id":"682261df-3d1d-4fcf-b1ef-9767bef9be1b","resolution":{"observed_at":"2026-05-23T04:45:25.310964Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2506.16217","last_updated":"2026-04-06T09:35:14Z","snapshot_observed_at":"2026-07-06T21:44:42.748650Z","submitted_at":"2025-06-19T11:09:00Z","title":"Quasinormal modes and grey-body factors of axial gravitational perturbations of regular black holes in asymptotically safe gravity","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-19T09:05:31.241151Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2506.16217"},"observation_digest":"sha256:8d523b848ea96e23a506951e0bce36a35aa51b5fd8018bed63426d7f68e7f394","observation_id":"4ef802c4-ab38-444b-b801-db9cb9c91c5b","resolution":{"observed_at":"2026-05-19T09:07:14.341349Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2512.23510","last_updated":"2026-04-08T06:40:48Z","snapshot_observed_at":"2026-07-06T22:40:17.725041Z","submitted_at":"2025-12-29T14:47:19Z","title":"Quasinormal mode/grey-body factor correspondence for Kerr black holes","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-16T19:26:13.414782Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2512.23510"},"observation_digest":"sha256:fae2ab8435f95f14cc15d2fd891463e9574bdc92a2a5dfb32d09576e41d87560","observation_id":"acba053c-fa22-472b-b78f-4413a2d8dc48","resolution":{"observed_at":"2026-05-16T19:28:20.217780Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-07-06T23:10:24.992210Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":1},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-05-08T02:18:25.796367Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:45dc792b0a49243f0a705166c2bbfa2d723587e7fe3db47258659684e3f1a623","observation_id":"aaa2519c-35f9-4e6d-90c5-abb1c7fe9808","resolution":{"observed_at":"2026-05-11T22:51:23.900983Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2604.24349","last_updated":"2026-05-13T13:55:01Z","snapshot_observed_at":"2026-07-06T23:10:24.992210Z","submitted_at":"2026-04-27T11:44:41Z","title":"Scalar, electromagnetic, and Dirac perturbations of regular black holes constituting primordial dark matter","version":2},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-05-14T22:18:47.797399Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2604.24349"},"observation_digest":"sha256:503186ba454d0dba111219780e48262660f3973a329c4093c7481ec9fa38ca16","observation_id":"a1947853-21da-476e-aa38-5c34b833437b","resolution":{"observed_at":"2026-05-14T22:19:31.201416Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2604.25471","last_updated":"2026-04-28T10:23:30Z","snapshot_observed_at":"2026-08-02T11:44:34.483229Z","submitted_at":"2026-04-28T10:23:30Z","title":"Massive scalar quasinormal modes of an asymptotically flat regular black hole supported by a phantom Dirac--Born--Infeld field","version":1},"reference_index":167,"source":"pdf_text","source_observed_at":"2026-05-07T15:29:43.270538Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2604.25471"},"observation_digest":"sha256:27502ecabfa5304786232f15f89d6e34c4ffe10760bc4b2ffc3c5ac2b1519985","observation_id":"8afc1415-813f-43e6-abfa-30638d21403e","resolution":{"observed_at":"2026-05-12T00:21:20.147368Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2605.03137","last_updated":"2026-05-04T20:22:29Z","snapshot_observed_at":"2026-08-11T04:59:13.445843Z","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":89,"source":"pdf_text","source_observed_at":"2026-05-07T02:21:14.281286Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.03137"},"observation_digest":"sha256:593ba5d54f99f571b88d74c72f02fc78bc2459dd878c046f558e35123a2d851a","observation_id":"c55f990c-4c74-4e12-99a0-ff6aac1030ad","resolution":{"observed_at":"2026-05-12T10:46:30.251921Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2605.03659","last_updated":"2026-05-05T11:41:14Z","snapshot_observed_at":"2026-07-06T23:16:34.988490Z","submitted_at":"2026-05-05T11:41:14Z","title":"Long-lived massive scalar modes, grey-body factors, and absorption cross sections of the Reissner--Nordstr\\\"om-like brane-world black hole","version":1},"reference_index":116,"source":"pdf_text","source_observed_at":"2026-05-07T14:06:56.581854Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.03659"},"observation_digest":"sha256:fb197ef42f42503b61cf2b6798d1248d1201e748d2e825088e6337b0cb6c48e1","observation_id":"c6f48b09-038f-46ad-a848-29995e825420","resolution":{"observed_at":"2026-05-12T00:46:14.189248Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2605.09756","last_updated":"2026-05-10T21:05:04Z","snapshot_observed_at":"2026-07-06T23:21:49.499951Z","submitted_at":"2026-05-10T21:05:04Z","title":"Hawking Radiation and Greybody Factors of Test Scalar and Electromagnetic Fields on Asymptotically Flat Pure Lovelock Black Holes","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-05-12T02:21:03.847822Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.09756"},"observation_digest":"sha256:98b93d75efe87cfc571e0fefedf03d998efd1f3701d69039227caff6e24625f3","observation_id":"3cff55a5-0dbb-4037-8fe9-36546a73de59","resolution":{"observed_at":"2026-05-12T02:21:16.397675Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2605.11013","last_updated":"2026-05-10T12:56:40Z","snapshot_observed_at":"2026-08-11T14:05:06.989302Z","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":164,"source":"pdf_text","source_observed_at":"2026-05-13T01:58:50.185004Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.11013"},"observation_digest":"sha256:884b91e286e527b86bdd21e2632c27ef2ab955725c9b3df808ff35a4a5181ea8","observation_id":"bcca0641-0974-46a8-92da-95d2e843600c","resolution":{"observed_at":"2026-05-13T02:02:06.632485Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2605.11364","last_updated":"2026-05-12T00:34:59Z","snapshot_observed_at":"2026-08-11T14:46:45.677734Z","submitted_at":"2026-05-12T00:34:59Z","title":"Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations","version":1},"reference_index":134,"source":"pdf_text","source_observed_at":"2026-05-13T02:39:27.974688Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.11364"},"observation_digest":"sha256:a5ddfd84cbfff5a835fecb347ddd77b0d1cd71ed9bd767e02c41533e7fd6dba8","observation_id":"8954f314-1027-40ed-8d24-ddd2cb13371a","resolution":{"observed_at":"2026-05-13T02:47:08.387595Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2605.12113","last_updated":"2026-05-12T13:29:10Z","snapshot_observed_at":"2026-08-04T03:37:25.006389Z","submitted_at":"2026-05-12T13:29:10Z","title":"Quasinormal Spectra of Fields of Various Spin in Asymptotically de Sitter Black Holes within Generalized Proca Theory","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-05-13T04:51:34.508568Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.12113"},"observation_digest":"sha256:b4240fcdf43898714be818807d7ff073298af013909dc47c43d1d7e670ec2654","observation_id":"2add7ebf-b068-41a4-920e-37654db7d824","resolution":{"observed_at":"2026-05-13T04:52:16.569720Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"citing_paper":{"arxiv_id":"2605.21533","last_updated":"2026-05-19T22:29:19Z","snapshot_observed_at":"2026-08-02T05:35:23.334080Z","submitted_at":"2026-05-19T22:29:19Z","title":"Long-lived quasinormal modes of Asymptotically de Sitter Black Holes in Generalized Proca Theory","version":1},"reference_index":133,"source":"pdf_text","source_observed_at":"2026-05-22T00:57:40.683341Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.21533"},"observation_digest":"sha256:9f9c7e859d29d3e817eaeddb3b4e64bbef3a439e05578cd291da84172c9c9a70","observation_id":"54d74ba1-8bcf-49ac-80a8-1e091b14e544","resolution":{"observed_at":"2026-05-22T01:00:51.566058Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"cited_work":{"arxiv_id":"2412.13385","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.13385","snapshot_observed_at":"2026-06-30T00:04:06.159981Z","title":"Malik, (2024), arXiv:2412.13385 [gr-qc]","venue":null,"work_id":"959da6f5-c2c0-402f-9f01-8659e6fb3f2c","year":2024},"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":55,"source":"pdf_text","source_observed_at":"2026-06-29T23:58:23.049086Z"},"links":{"cited_paper":"/paper/2412.13385","citing_paper":"/paper/2605.25076"},"observation_digest":"sha256:e232fd704691c16cf1b69044c11d9ab0fa7051c77c7d5e8df3d8bf51d33c5792","observation_id":"2790df97-3d3d-4964-b6a2-2b4ed8a47164","resolution":{"observed_at":"2026-06-30T00:04:06.161411Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2412.13385/citation-record","integrity":"/paper/2412.13385/integrity","json":"/paper/2412.13385/citation-record.json","paper":"/paper/2412.13385"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T13:24:44.085514Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.085514Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:28b7c164ab910ca1b794cea15b03a1d82fa573c239c9768408cc6036b5e4ae6a","observation_id":"824f0bd4-fef6-4b52-9c03-a2b341c5076c","resolution":{"observed_at":"2026-08-11T13:24:44.085514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.08746","last_updated":"2020-08-25T05:01:14Z","snapshot_observed_at":"2026-07-06T08:30:43.834654Z","submitted_at":"2019-10-19T11:04:58Z","title":"Revisiting a family of wormholes: geometry, matter, scalar quasinormal modes and echoes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.08746","snapshot_observed_at":"2026-08-11T13:24:44.093927Z","title":"Dutta Roy, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.093927Z"},"links":{"cited_paper":"/paper/1910.08746","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:35756832de8d7c289866201834d75b4416226d2a8198261947b44d4cf5e52ae8","observation_id":"3ed411aa-9ccb-4a67-884f-7d6831d7666f","resolution":{"observed_at":"2026-08-11T13:24:44.093927Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.12601","last_updated":"2022-12-23T22:23:49Z","snapshot_observed_at":"2026-08-11T15:08:11.123712Z","submitted_at":"2022-12-23T22:23:49Z","title":"Polar modes and isospectrality of Ellis-Bronnikov wormholes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.12601","snapshot_observed_at":"2026-08-11T13:24:44.099823Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.099823Z"},"links":{"cited_paper":"/paper/2212.12601","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ab373908526c7b372cbc8d013fcbb6e0526ca160ce3e2b510e063762fb13caa3","observation_id":"2a63df90-b992-4b72-8621-f640da70a420","resolution":{"observed_at":"2026-08-11T13:24:44.099823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.03282","last_updated":"2018-06-08T17:25:53Z","snapshot_observed_at":"2026-08-01T15:13:43.921212Z","submitted_at":"2018-06-08T17:25:53Z","title":"Scalar and axial quasinormal modes of massive static phantom wormholes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.03282","snapshot_observed_at":"2026-08-11T13:24:44.105643Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.105643Z"},"links":{"cited_paper":"/paper/1806.03282","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:e615216f181d47c274f8630ff07c801ff86bad7d8452e7917280e1b5884557dc","observation_id":"2ea5ebb6-25f4-4cf5-9c1d-983b2b3f4adc","resolution":{"observed_at":"2026-08-11T13:24:44.105643Z","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":"2026-08-09T13:06:37.874006Z","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":"2026-08-11T13:24:44.112658Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.112658Z"},"links":{"cited_paper":"/paper/2102.10679","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:326e1cf2206ab29ed369860a2432ee9d1bbc1f18a6082e10a7ae6cecdd9d1fa2","observation_id":"c72bd346-c96d-4d7b-bb13-b6022d33c524","resolution":{"observed_at":"2026-08-11T13:24:44.112658Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.05977","last_updated":"2021-10-06T21:35:22Z","snapshot_observed_at":"2026-08-04T08:18:08.587544Z","submitted_at":"2021-07-13T10:49:45Z","title":"Wormholes without exotic matter: quasinormal modes, echoes and shadows","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.05977","snapshot_observed_at":"2026-08-11T13:24:44.118929Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.118929Z"},"links":{"cited_paper":"/paper/2107.05977","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:bf7fd4291836e8311296b22d844a1596088eabc094f0dd29a6908f9ba60ae966","observation_id":"a283fff4-8c30-4ef6-922f-a5a542637ca4","resolution":{"observed_at":"2026-08-11T13:24:44.118929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.01798","last_updated":"2018-12-05T03:17:21Z","snapshot_observed_at":"2026-08-06T17:57:25.507123Z","submitted_at":"2018-12-05T03:17:21Z","title":"Quasi-normal modes of bumblebee wormhole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.01798","snapshot_observed_at":"2026-08-11T13:24:44.125471Z","title":"Oliveira, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.125471Z"},"links":{"cited_paper":"/paper/1812.01798","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:835874c6f52ab8de190786e702197f0cc641a6f69369d2ed1ba0202222fdefb9","observation_id":"c4d4e021-12f8-48cd-b700-0501c466d4eb","resolution":{"observed_at":"2026-08-11T13:24:44.125471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05979","last_updated":"2024-10-08T12:25:12Z","snapshot_observed_at":"2026-08-03T03:23:03.782158Z","submitted_at":"2024-10-08T12:25:12Z","title":"A Unified Spectral Approach for Quasinormal Modes of Morris-Thorne Wormholes","version":1},"cited_work":{"arxiv_id":"2410.05979","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.05979","snapshot_observed_at":"2026-08-11T13:24:45.948597Z","title":"A Unified Spectral Approach for Quasinormal Modes of Morris-Thorne Wormholes","venue":"gr-qc","work_id":"4d0d4a97-1f82-4887-889b-b0463dc8b6ea","year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.131557Z"},"links":{"cited_paper":"/paper/2410.05979","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:1adf05c15979acc479a315eee247bf97c7d1dc9bdaaed3668e591055b6afd98d","observation_id":"719f4c0b-bf09-49b6-9b99-6780a04fc006","resolution":{"observed_at":"2026-08-11T13:24:45.955216Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13890","last_updated":"2021-11-27T13:14:15Z","snapshot_observed_at":"2026-08-10T11:36:10.469512Z","submitted_at":"2021-11-27T13:14:15Z","title":"Echoes from Asymmetric Wormholes and Black Bounce","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.13890","snapshot_observed_at":"2026-08-11T13:24:44.137206Z","title":"Ou, M.-Y","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.137206Z"},"links":{"cited_paper":"/paper/2111.13890","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:d9cd53914d9f9ccee9e25dc635c3f1af597ad7aed116440a14f62fda486a3c93","observation_id":"e0d45d1e-60ba-4566-9655-e23625699710","resolution":{"observed_at":"2026-08-11T13:24:44.137206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.05246","last_updated":"2020-01-10T05:28:15Z","snapshot_observed_at":"2026-07-06T08:36:35.767733Z","submitted_at":"2019-11-13T01:57:02Z","title":"Arbitrarily long-lived quasinormal modes in a wormhole background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.05246","snapshot_observed_at":"2026-08-11T13:24:44.143313Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.143313Z"},"links":{"cited_paper":"/paper/1911.05246","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:82dc504fd700429d297ddac8fa4f718e16a9fa28390d2e4c5477c31f55e8dc61","observation_id":"04c3944e-1c24-4f49-9da0-4494b697b1c7","resolution":{"observed_at":"2026-08-11T13:24:44.143313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.08399","last_updated":"2023-06-02T05:54:01Z","snapshot_observed_at":"2026-08-09T22:40:43.799475Z","submitted_at":"2023-03-15T07:03:05Z","title":"Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-\\AE{}ther theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.08399","snapshot_observed_at":"2026-08-11T13:24:44.148985Z","title":"Zhang, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.148985Z"},"links":{"cited_paper":"/paper/2303.08399","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:e1b64eeff36a19b827ebbcafe261886e322bf8490d10143c691dbe545a614710","observation_id":"57aaca0f-5ffc-4e1a-b44b-514edc2903c5","resolution":{"observed_at":"2026-08-11T13:24:44.148985Z","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":"2026-08-11T13:24:44.155017Z","title":"Azad, Lect","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.155017Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:a429cbbed3b409a3ea6c7c676213da9cf924520654819ed3d4d24d81ab1d1f91","observation_id":"e8b6fdbb-c5d5-4f92-ac7d-47cc4a323ce6","resolution":{"observed_at":"2026-08-11T13:24:44.155017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.05019","last_updated":"2022-08-12T12:04:18Z","snapshot_observed_at":"2026-07-06T11:56:24.775449Z","submitted_at":"2021-10-11T06:12:44Z","title":"Novel triple barrier potential for axial gravitational perturbations of a family of Lorentzian wormholes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.05019","snapshot_observed_at":"2026-08-11T13:24:44.159073Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.159073Z"},"links":{"cited_paper":"/paper/2110.05019","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:4372e03fc2e70199a1b3d7652707c1621918fce9d0c91d0a47f20be8397f6684","observation_id":"0b16d89f-1d32-4f13-8824-63abcf751e5b","resolution":{"observed_at":"2026-08-11T13:24:44.159073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.16019","last_updated":"2021-09-20T07:45:13Z","snapshot_observed_at":"2026-08-08T14:13:29.570730Z","submitted_at":"2020-07-30T15:14:20Z","title":"Correspondence between quasinormal modes and the shadow radius in a wormhole spacetime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.16019","snapshot_observed_at":"2026-08-11T13:24:44.163261Z","title":"Jusuﬁ, Gen","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.163261Z"},"links":{"cited_paper":"/paper/2007.16019","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:0694136effeb17a75ca244446bca37705148c9952c0f32ad9674b2536907cd69","observation_id":"447b35a0-ea04-450a-976c-49c7ab82c524","resolution":{"observed_at":"2026-08-11T13:24:44.163261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.17479","last_updated":"2024-02-10T13:27:19Z","snapshot_observed_at":"2026-08-07T01:50:53.486760Z","submitted_at":"2023-10-26T15:31:57Z","title":"Signature quasinormal modes of Ellis-Bronnikov wormhole embedded in warped braneworld background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.17479","snapshot_observed_at":"2026-08-11T13:24:44.168746Z","title":"Mitra and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.168746Z"},"links":{"cited_paper":"/paper/2310.17479","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:61b15d904040d4403f542b6e9c905135ebe10d566a69917db5b0b74458d46e7e","observation_id":"c6371494-5ab0-44c6-b56c-2b8cf162499e","resolution":{"observed_at":"2026-08-11T13:24:44.168746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.07055","last_updated":"2023-02-11T06:19:10Z","snapshot_observed_at":"2026-08-04T05:27:48.419702Z","submitted_at":"2022-08-15T08:03:29Z","title":"Tideless Traversable Wormholes surrounded by cloud of strings in $f(R)$ gravity","version":2},"cited_work":{"arxiv_id":"2208.07055","doi":null,"metadata_source":"pith","pith_arxiv_id":"2208.07055","snapshot_observed_at":"2026-08-11T13:24:45.810645Z","title":"Tideless Traversable Wormholes surrounded by cloud of strings in $f(R)$ gravity","venue":"gr-qc","work_id":"b0b815f4-d95b-4e51-9e89-8f27c13825ab","year":2022},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.173969Z"},"links":{"cited_paper":"/paper/2208.07055","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:54ecaac67a607aaa07d169defd54be0a9b6da8ea81272a2efd3c9bc2f3174550","observation_id":"e67a8704-accd-48be-8825-663503493811","resolution":{"observed_at":"2026-08-11T13:24:45.823248Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.15575","last_updated":"2024-04-10T02:17:32Z","snapshot_observed_at":"2026-07-06T17:34:45.072246Z","submitted_at":"2024-02-23T19:24:01Z","title":"Quasinormal modes and bound states of massive scalar fields in wormhole spacetimes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.15575","snapshot_observed_at":"2026-08-11T13:24:44.179103Z","title":"Alfaro, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.179103Z"},"links":{"cited_paper":"/paper/2402.15575","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:b6ac4d3f93b34cb43e8c44a3fd0f9d52fc356c42ac2d4a78b264bf7c43aa00c6","observation_id":"c000a674-7739-4a3d-868f-065f9403ee7c","resolution":{"observed_at":"2026-08-11T13:24:44.179103Z","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":"2026-08-11T13:24:44.183917Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.183917Z"},"links":{"cited_paper":"/paper/1912.05315","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:c21a364642d5829e390ff1fb6f0fed15a5ee3f3dfd99c931662702bb78cfeebb","observation_id":"054934c3-e102-411f-8d92-d4dee045a451","resolution":{"observed_at":"2026-08-11T13:24:44.183917Z","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":"2026-08-11T13:24:44.189759Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.189759Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:200f07283346e8e921679725e3ed2f2e8618a3ec52ad859470c2d5b3b61ee9f3","observation_id":"285a090e-52c4-4fe7-ad7b-49dc9fbc00c4","resolution":{"observed_at":"2026-08-11T13:24:44.189759Z","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":"2026-08-11T13:24:44.196606Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.196606Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:f7c21ec894625a84a2586a2aa2fe9ecac59ea5364f0832279ede3076c928e965","observation_id":"50417cde-3779-4386-ae11-5b90e78b3bc3","resolution":{"observed_at":"2026-08-11T13:24:44.196606Z","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":"2026-08-11T13:24:44.203065Z","title":"Abbott et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.203065Z"},"links":{"cited_paper":"/paper/2006.12611","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:8d3673a39f042ebb1c7f250b591ef47f60f73d258d379d624844d4e159ae5188","observation_id":"09477e38-160d-42ae-a04b-34740c64ba18","resolution":{"observed_at":"2026-08-11T13:24:44.203065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.05725","last_updated":"2023-10-02T20:20:08Z","snapshot_observed_at":"2026-08-09T09:22:55.971279Z","submitted_at":"2023-09-11T18:00:43Z","title":"Greybody Factors Imprinted on Black Hole Ringdowns: an alternative to superposed quasi-normal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.05725","snapshot_observed_at":"2026-08-11T13:24:44.208623Z","title":"Oshita, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.208623Z"},"links":{"cited_paper":"/paper/2309.05725","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:b2599b04dcba804b1a27e4abce9c79090752fe986d5e040547b6a2b012568701","observation_id":"1c385eae-c5c6-45fa-a9bf-71c411a75db2","resolution":{"observed_at":"2026-08-11T13:24:44.208623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1004.1284","last_updated":"2018-04-01T20:11:54Z","snapshot_observed_at":"2026-08-03T16:16:12.004686Z","submitted_at":"2010-04-08T08:51:53Z","title":"Passage of radiation through wormholes of arbitrary shape","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1004.1284","snapshot_observed_at":"2026-08-11T13:24:44.213924Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.213924Z"},"links":{"cited_paper":"/paper/1004.1284","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:fbfd4384a3f1cbc8c8ac460432b68a6ff9918d8ed64af724582494a7d50b433c","observation_id":"c71545f4-333e-4121-8995-47df58186ccd","resolution":{"observed_at":"2026-08-11T13:24:44.213924Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.01692","last_updated":"2024-11-14T15:12:57Z","snapshot_observed_at":"2026-08-12T00:30:35.861051Z","submitted_at":"2024-06-03T18:00:06Z","title":"Ringdown stability: greybody factors as stable gravitational-wave observables","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.01692","snapshot_observed_at":"2026-08-11T13:24:44.219951Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.219951Z"},"links":{"cited_paper":"/paper/2406.01692","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:56443b0d2c5a42c6b5129a7890b4b2b8333a481a2552af6921a4e7ae97c1760f","observation_id":"dd09ad88-fb46-4bfc-8017-3855c234c7bf","resolution":{"observed_at":"2026-08-11T13:24:44.219951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.11694","last_updated":"2024-09-12T20:32:29Z","snapshot_observed_at":"2026-08-01T01:18:48.841507Z","submitted_at":"2024-06-17T16:11:19Z","title":"Correspondence between grey-body factors and quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.11694","snapshot_observed_at":"2026-08-11T13:24:44.224436Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.224436Z"},"links":{"cited_paper":"/paper/2406.11694","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:f7466ee517d3cf3d1dba0cbf319ef8d4204eda3bf159b65b562ade8bd65fa245","observation_id":"311178b1-8ade-47e2-b1ec-c37f4102570f","resolution":{"observed_at":"2026-08-11T13:24:44.224436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.04525","last_updated":"2024-06-06T21:51:21Z","snapshot_observed_at":"2026-08-10T06:12:47.030897Z","submitted_at":"2024-06-06T21:51:21Z","title":"(In)stability of the black hole greybody factors and ringdowns against a small-bump correction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.04525","snapshot_observed_at":"2026-08-11T13:24:44.229746Z","title":"Oshita, K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.229746Z"},"links":{"cited_paper":"/paper/2406.04525","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:0bead3c0bb0ce5a64d966adf2f310bf847e010598b529ea1b83f59b3e73a0683","observation_id":"61552972-9e92-46e5-b8a0-ab59e174c87b","resolution":{"observed_at":"2026-08-11T13:24:44.229746Z","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":"2026-08-11T13:24:44.235231Z","title":"Dubinsky (2024), 2412.00625","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.235231Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ccca95798884304dffa839e21f4fb6cb9e8bbaa08d3e169aac39234810d7938d","observation_id":"7e217d16-91ab-4d9e-87e6-8258c6166b84","resolution":{"observed_at":"2026-08-11T13:24:44.235231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.06007","last_updated":"2024-11-08T22:59:51Z","snapshot_observed_at":"2026-08-11T15:51:18.946954Z","submitted_at":"2024-11-08T22:59:51Z","title":"Quantum corrected black holes: testing the correspondence between grey-body factors and quasinormal modes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.06007","snapshot_observed_at":"2026-08-11T13:24:44.241078Z","title":"Skvortsova (2024), 2411.06007","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.241078Z"},"links":{"cited_paper":"/paper/2411.06007","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:fe52f74a307ccc45619464f899b024cad4c274c64d11236bdbec5909f2b6736d","observation_id":"012decb6-b391-4c91-9b67-af2cd7a05e81","resolution":{"observed_at":"2026-08-11T13:24:44.241078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.11166","last_updated":"2025-04-13T18:41:28Z","snapshot_observed_at":"2026-08-11T15:12:07.489015Z","submitted_at":"2024-12-15T12:29:32Z","title":"Correspondence between quasinormal modes and grey-body factors of spherically symmetric traversable wormholes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.11166","snapshot_observed_at":"2026-08-11T13:24:44.246722Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.246722Z"},"links":{"cited_paper":"/paper/2412.11166","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:9bd1c828ce2f47d5f80def15d60baf9c7c0261be024e492fade193c877a1d08d","observation_id":"35331e31-3eec-4469-a5e6-56349c931eef","resolution":{"observed_at":"2026-08-11T13:24:44.246722Z","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":"2026-08-11T13:24:44.252392Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.252392Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:fa70e00b9a93d2482d05d014c1dd564676bee6441950908396441335cf0201d9","observation_id":"52c79aaf-fd46-46cb-97c6-4fb0c6197e01","resolution":{"observed_at":"2026-08-11T13:24:44.252392Z","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":"2026-08-11T13:24:44.257972Z","title":"Iyer and C","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.257972Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:482b0c8b294179e8253187a9a3a348f9607a6333613085e0a9fa74d5b9415764","observation_id":"44f692c3-fa01-439f-bb34-5e570b1dc49b","resolution":{"observed_at":"2026-08-11T13:24:44.257972Z","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":"2026-08-11T13:24:44.263898Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.263898Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:c4a35aba7aae952004efed9edb8b63b553028a21a29b6c5fc084bc69db391c71","observation_id":"efd6ef5a-ffa9-41f5-85c9-65c89d9ca3fe","resolution":{"observed_at":"2026-08-11T13:24:44.263898Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.00361","last_updated":"2017-04-02T20:40:48Z","snapshot_observed_at":"2026-08-05T13:08:11.649869Z","submitted_at":"2017-04-02T20:40:48Z","title":"Quasinormal modes of black holes. The improved semianalytic approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.00361","snapshot_observed_at":"2026-08-11T13:24:44.269878Z","title":"Matyjasek and M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.269878Z"},"links":{"cited_paper":"/paper/1704.00361","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:e4999219b3d13e2f4299a7358ec782f362eea043c74edf9f2ac2d21981a709fe","observation_id":"36f2eeff-6899-4149-88b1-8a028b2fb986","resolution":{"observed_at":"2026-08-11T13:24:44.269878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0504139","last_updated":"2005-04-28T14:31:19Z","snapshot_observed_at":"2026-07-07T03:20:53.471754Z","submitted_at":"2005-04-28T14:31:19Z","title":"The ringing wormholes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0504139","snapshot_observed_at":"2026-08-11T13:24:44.275731Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.275731Z"},"links":{"cited_paper":"/paper/gr-qc/0504139","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:826e4bbd48602e5042fa6e1aeb10407c964ff2ff9dfdf2229e9c5d4d6e72d632","observation_id":"2036c169-61c9-4b69-a4e3-880131600c75","resolution":{"observed_at":"2026-08-11T13:24:44.275731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.12664","last_updated":"2019-09-27T13:03:36Z","snapshot_observed_at":"2026-08-10T11:06:21.127746Z","submitted_at":"2019-09-27T13:03:36Z","title":"Quasinormal modes of Dirac field in the Einstein-dilaton-Gauss-Bonnet and Einstein-Weyl gravities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.12664","snapshot_observed_at":"2026-08-11T13:24:44.280573Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.280573Z"},"links":{"cited_paper":"/paper/1909.12664","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:d1a54457cf9040f923cc6f17c7829188f2abdf5a8cad865ec9fba5107712624c","observation_id":"0a71237e-d054-417b-9312-6cd95aaa34e0","resolution":{"observed_at":"2026-08-11T13:24:44.280573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13552","last_updated":"2024-09-12T23:00:23Z","snapshot_observed_at":"2026-08-11T00:47:47.951069Z","submitted_at":"2024-05-22T11:40:05Z","title":"Quantum gravitational corrections to the Schwarzschild spacetime and quasinormal frequencies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.13552","snapshot_observed_at":"2026-08-11T13:24:44.287033Z","title":"Dubinsky (2024), 2405.13552","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.287033Z"},"links":{"cited_paper":"/paper/2405.13552","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:fa38141e4ae158e726a13114d86446930de9adcdef7ea33c3a471b23afc2761f","observation_id":"8e98a947-0c88-48c0-8ff6-f7faad98171b","resolution":{"observed_at":"2026-08-11T13:24:44.287033Z","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":"2026-08-11T13:24:44.292823Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.292823Z"},"links":{"cited_paper":"/paper/hep-th/0503029","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:177c5bd1280f109387a7e203419dfec9a798961321e38412b8878fe6667932a2","observation_id":"4daac5ca-e92f-4948-b59d-892999880b17","resolution":{"observed_at":"2026-08-11T13:24:44.292823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.15807","last_updated":"2024-05-20T14:41:36Z","snapshot_observed_at":"2026-08-08T08:09:49.767174Z","submitted_at":"2024-05-20T14:41:36Z","title":"Ringing of the Extreme Regular Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.15807","snapshot_observed_at":"2026-08-11T13:24:44.300857Z","title":"Skvortsova, Grav","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.300857Z"},"links":{"cited_paper":"/paper/2405.15807","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:578b4442a0a023a287b98e1d920c32f91d6b3ba0293bb4578918d595d8f0983d","observation_id":"bef0aa30-95d8-44c7-b692-d06d44082969","resolution":{"observed_at":"2026-08-11T13:24:44.300857Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.06483","last_updated":"2023-02-02T08:30:33Z","snapshot_observed_at":"2026-08-10T04:15:22.968852Z","submitted_at":"2023-01-16T15:41:56Z","title":"Superradiance Instabilities of Charged Black Holes in Einstein-Maxwell-scalar Theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.06483","snapshot_observed_at":"2026-08-11T13:24:44.305557Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.305557Z"},"links":{"cited_paper":"/paper/2301.06483","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ad8c8ea4f0dbb95f45b8eaeca6c4f6936e01cdcd5412e378bbec1cfc5ceeee6f","observation_id":"036498b2-6255-46c5-b7d3-12356524734e","resolution":{"observed_at":"2026-08-11T13:24:44.305557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.12326","last_updated":"2023-11-01T10:41:37Z","snapshot_observed_at":"2026-08-09T18:50:17.598473Z","submitted_at":"2023-10-08T15:09:21Z","title":"Black holes in Starobinsky-Bel-Robinson Gravity and the breakdown of quasinormal modes/null geodesics correspondence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.12326","snapshot_observed_at":"2026-08-11T13:24:44.311779Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.311779Z"},"links":{"cited_paper":"/paper/2310.12326","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ac310943b64394435e729959dd0be48d447d9f7f25750cecdeffa8c45a7f9cae","observation_id":"2f73347c-e798-46d5-b033-999aeddfc533","resolution":{"observed_at":"2026-08-11T13:24:44.311779Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.16479","last_updated":"2024-03-02T07:30:20Z","snapshot_observed_at":"2026-07-06T17:08:30.524802Z","submitted_at":"2023-12-27T09:05:46Z","title":"Quasinormal modes of Einstein--scalar--Gauss--Bonnet black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.16479","snapshot_observed_at":"2026-08-11T13:24:44.316603Z","title":"Paul, Eur","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.316603Z"},"links":{"cited_paper":"/paper/2312.16479","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:85dfb08dca7574cc8d6bc0e851bc1b956ed3f830e3e353c247041e4641d9ad39","observation_id":"cae7f906-f459-49d0-8f7a-287d9b5a5a5a","resolution":{"observed_at":"2026-08-11T13:24:44.316603Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-11T13:24:44.322024Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.322024Z"},"links":{"cited_paper":"/paper/1604.03604","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:e2d9c845cea28b5c391aaacb104917bc449a6dc5d26c01168503af93240a5742","observation_id":"5f6dfca7-a9cd-4fa6-ac57-cc655ab087ea","resolution":{"observed_at":"2026-08-11T13:24:44.322024Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.1843","last_updated":"2011-01-19T17:55:50Z","snapshot_observed_at":"2026-07-06T02:18:53.260255Z","submitted_at":"2010-11-08T16:35:10Z","title":"Quasinormal modes, scattering and Hawking radiation of Kerr-Newman black holes in a magnetic field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.1843","snapshot_observed_at":"2026-08-11T13:24:44.327631Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.327631Z"},"links":{"cited_paper":"/paper/1011.1843","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:3873eee1ff3583e71386746463cf436fff69be0f5abcea2976662ceed836e9d9","observation_id":"9b803d02-6cc0-486b-8266-3b1839439a85","resolution":{"observed_at":"2026-08-11T13:24:44.327631Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.17639","last_updated":"2024-01-06T13:47:29Z","snapshot_observed_at":"2026-07-06T17:09:55.651197Z","submitted_at":"2023-12-29T15:04:43Z","title":"Quasinormal modes of quantum-corrected black holes","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.17639","snapshot_observed_at":"2026-08-11T13:24:44.333993Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.333993Z"},"links":{"cited_paper":"/paper/2312.17639","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:60e3ec35221d00e589359605f9e1a04077ac8d048d2c90e4b99448f980792ebb","observation_id":"dcca2f46-3028-4a9f-bcb4-db620967e11c","resolution":{"observed_at":"2026-08-11T13:24:44.333993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0802.2262","last_updated":"2008-06-06T18:19:21Z","snapshot_observed_at":"2026-07-06T01:38:40.975193Z","submitted_at":"2008-02-15T18:15:47Z","title":"Evolution of Brane-Localised Standard Model Fields in Gauss-Bonnet theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0802.2262","snapshot_observed_at":"2026-08-11T13:24:44.340560Z","title":"Zhidenko, Phys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.340560Z"},"links":{"cited_paper":"/paper/0802.2262","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ae03a4d9cb59f4410a71f7faec60c60d53539a7449213c3a9dcefb1caf8007e2","observation_id":"a7f6e19c-0e91-401f-8c1b-74aa843c2b19","resolution":{"observed_at":"2026-08-11T13:24:44.340560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.03913","last_updated":"2019-07-23T12:56:54Z","snapshot_observed_at":"2026-07-06T07:00:29.893507Z","submitted_at":"2018-09-11T14:16:59Z","title":"Quasinormal modes of the four-dimensional black hole in Einstein-Weyl gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.03913","snapshot_observed_at":"2026-08-11T13:24:44.346183Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.346183Z"},"links":{"cited_paper":"/paper/1809.03913","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:39be059a3de5f9f077e2336d4cb39db581c63186b2214c2dd3d5b34939dee95f","observation_id":"868cbb2d-4f30-454c-b6d0-0f1edaeb8c4f","resolution":{"observed_at":"2026-08-11T13:24:44.346183Z","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":"2026-08-08T23:56:28.028367Z","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":"2026-08-11T13:24:44.352787Z","title":"Skvortsova, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.352787Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:c4b0e817457133f8ba26cfa17e8655ff4eb203d19f758260f868023712cde026","observation_id":"8fae792b-b243-4a2d-88bb-91282a27f963","resolution":{"observed_at":"2026-08-11T13:24:44.352787Z","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":"2026-08-12T00:09:55.825352Z","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":"2026-08-11T13:24:44.358871Z","title":"Malik, EPL 147, 69001 (2024), 2410.04306","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.358871Z"},"links":{"cited_paper":"/paper/2410.04306","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:91b1dda72450b8e17b3454e8c1cda870950d491731efae35d093752420a421df","observation_id":"90043052-018f-4b92-aa94-63f35de59be5","resolution":{"observed_at":"2026-08-11T13:24:44.358871Z","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":"2026-08-11T13:24:44.365194Z","title":"Malik, Z","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.365194Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:9f0d023273005c597bab9bda431ca03a92de0b4f1477b20b11e6083d6cb798e0","observation_id":"9a9a448a-39e3-43f4-82a7-7fddd5708c38","resolution":{"observed_at":"2026-08-11T13:24:44.365194Z","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":"2026-08-11T13:24:44.370720Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.370720Z"},"links":{"cited_paper":"/paper/2311.05503","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ea9106725a45fec42839ba78b1ac0d1185af4c9fe6af8b245db540126b5c9bca","observation_id":"baa641d4-b654-488b-88f4-fce6c71ba6b2","resolution":{"observed_at":"2026-08-11T13:24:44.370720Z","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":"2026-08-11T13:24:44.375572Z","title":"Dubinsky and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.375572Z"},"links":{"cited_paper":"/paper/2404.01834","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:5fb9d902f0212aa96e7e3215e003a09ade9e18651b3c34ee005bfca788d4ea24","observation_id":"81a17246-f2c3-421e-8d7f-1087cf5dc628","resolution":{"observed_at":"2026-08-11T13:24:44.375572Z","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":"2026-08-11T13:24:44.379531Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.379531Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:3dde23530297a5e0ec5bec00391e410fb54312f403c3a5c0c916c34cad1396ed","observation_id":"a80a79b8-ea57-4141-a4ac-9fdcd4f32b0b","resolution":{"observed_at":"2026-08-11T13:24:44.379531Z","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":"2026-08-11T13:24:44.385718Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.385718Z"},"links":{"cited_paper":"/paper/2307.10801","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:1fac7988bc628d2b841665277a1f0e3718f2243c9705ce3a1173a4959fad53e6","observation_id":"a6015566-4d29-4a35-af71-dc0c2a9f7fd5","resolution":{"observed_at":"2026-08-11T13:24:44.385718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.15232","last_updated":"2024-10-19T22:41:19Z","snapshot_observed_at":"2026-08-06T10:12:21.383909Z","submitted_at":"2024-10-19T22:41:19Z","title":"Analytic expressions for grey-body factors of the general parametrized spherically symmetric black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.15232","snapshot_observed_at":"2026-08-11T13:24:44.392367Z","title":"Dubinsky and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.392367Z"},"links":{"cited_paper":"/paper/2410.15232","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:5a40b3f0476c438fe0f629e3aaede0a10d44c7fc52f5c95010be42cfe1137e21","observation_id":"6d994f65-d29a-4d6c-a420-b8b5c2d31787","resolution":{"observed_at":"2026-08-11T13:24:44.392367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.05737","last_updated":"2015-04-25T00:44:41Z","snapshot_observed_at":"2026-07-06T04:12:30.105429Z","submitted_at":"2015-03-19T12:28:35Z","title":"Quasinormal modes of test fields around regular black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.05737","snapshot_observed_at":"2026-08-11T13:24:44.397229Z","title":"Toshmatov, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.397229Z"},"links":{"cited_paper":"/paper/1503.05737","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:63b3c5698d1c90a6dd570ef5d31f37d360273414fffa436c1ef4881332598bc0","observation_id":"ba599712-8a90-4e86-be02-11abe333282b","resolution":{"observed_at":"2026-08-11T13:24:44.397229Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10419","last_updated":"2024-11-14T17:05:55Z","snapshot_observed_at":"2026-08-09T06:18:56.225990Z","submitted_at":"2024-10-14T12:13:36Z","title":"Circumventing Quantum Gravity: Black Holes Evaporating into Macroscopic Wormholes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10419","snapshot_observed_at":"2026-08-11T13:24:44.402762Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.402762Z"},"links":{"cited_paper":"/paper/2410.10419","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:dd8d52ffaf5b1433a47df6bbe62f619916270513a2eaad83797e59507f75bb78","observation_id":"ceb613d2-d2ed-4e4c-918e-f274b13f0d96","resolution":{"observed_at":"2026-08-11T13:24:44.402762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.10462","last_updated":"2021-09-17T08:46:56Z","snapshot_observed_at":"2026-08-10T14:40:58.264150Z","submitted_at":"2020-06-18T12:16:09Z","title":"Quasinormal modes and Hawking radiation of black holes in cubic gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.10462","snapshot_observed_at":"2026-08-11T13:24:44.408257Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.408257Z"},"links":{"cited_paper":"/paper/2006.10462","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:93ad582447d2c8e54d36b9d52ace949b28f39fd45bfe594d4590c36004cf9bde","observation_id":"16e92669-ec69-4f8c-a1a4-d41cf8c5e47c","resolution":{"observed_at":"2026-08-11T13:24:44.408257Z","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":"2026-08-11T13:24:44.416056Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.416056Z"},"links":{"cited_paper":"/paper/2309.02560","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:548e01a3c4b56412b8fff8f0cdbf51e6b3aae5c1a982b6941bec6ac720c3431d","observation_id":"abf70656-110e-45de-b26b-df47860231ff","resolution":{"observed_at":"2026-08-11T13:24:44.416056Z","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":"2026-08-11T13:24:44.425370Z","title":"Malik, Int","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.425370Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:31223fa14f2826d38b91a742912aeb1b4b9dd20d7b942cfdf12c617af18e63e5","observation_id":"e2ba2a99-8848-4629-a3b4-8258708c1b40","resolution":{"observed_at":"2026-08-11T13:24:44.425370Z","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":"2026-08-11T13:24:44.430654Z","title":"Malik, Int","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.430654Z"},"links":{"cited_paper":"/paper/2409.09872","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:2e235dad11e59e40e03fb2835ede6d5133c0a827d5e260b994092e75e19a2ab2","observation_id":"a60ca117-42e3-4d54-b4b2-540ced9d30e0","resolution":{"observed_at":"2026-08-11T13:24:44.430654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.5041","last_updated":"2011-08-25T08:48:51Z","snapshot_observed_at":"2026-08-05T23:57:18.542530Z","submitted_at":"2011-08-25T08:48:51Z","title":"Pathologies in Lovelock AdS Black Branes and AdS/CFT","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.5041","snapshot_observed_at":"2026-08-11T13:24:44.438249Z","title":"Takahashi and J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.438249Z"},"links":{"cited_paper":"/paper/1108.5041","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ca294a3dec4c7f3292559c3f8ca53f3c29bd1a89af17f87cb4b8a300ed867030","observation_id":"8062dc96-65b2-4836-890f-f56700a90d6f","resolution":{"observed_at":"2026-08-11T13:24:44.438249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1618","last_updated":"2010-08-18T00:03:50Z","snapshot_observed_at":"2026-07-06T02:14:00.875716Z","submitted_at":"2010-08-10T01:54:43Z","title":"Catastrophic Instability of Small Lovelock Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.1618","snapshot_observed_at":"2026-08-11T13:24:44.445140Z","title":"Takahashi and J","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.445140Z"},"links":{"cited_paper":"/paper/1008.1618","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:07b7ff96fd68f11ead24515a01b877d6eab32f7c11b182e0f9ce9f999a616278","observation_id":"08fef7c8-4db7-42b1-9ab3-ddcafdbffc8a","resolution":{"observed_at":"2026-08-11T13:24:44.445140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0510069","last_updated":"2005-10-20T16:57:41Z","snapshot_observed_at":"2026-07-07T03:21:38.235491Z","submitted_at":"2005-10-14T15:07:40Z","title":"Linear stability of Einstein-Gauss-Bonnet static spacetimes. Part II: vector and scalar perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0510069","snapshot_observed_at":"2026-08-11T13:24:44.459290Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.459290Z"},"links":{"cited_paper":"/paper/gr-qc/0510069","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:18074d99f5e042c7dfcd87f99267234f7d20bc8ed89402f70ee5d172c258e412","observation_id":"c149016e-4d62-4606-8f80-5d6aa043ff11","resolution":{"observed_at":"2026-08-11T13:24:44.459290Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0503117","last_updated":"2005-07-28T11:50:48Z","snapshot_observed_at":"2026-07-07T03:20:49.015991Z","submitted_at":"2005-03-30T11:51:35Z","title":"Linear stability of Einstein-Gauss-Bonnet static spacetimes. Part I: tensor perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0503117","snapshot_observed_at":"2026-08-11T13:24:44.467547Z","title":"Dotti and R","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.467547Z"},"links":{"cited_paper":"/paper/gr-qc/0503117","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:6ed39a45a30fffb90eec0c9b8e5b9f0e1538940f057df85200b9bcc41dd516a1","observation_id":"930ce17b-08be-4b37-814a-024ce90849a5","resolution":{"observed_at":"2026-08-11T13:24:44.467547Z","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":"2026-08-11T13:24:44.475571Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.475571Z"},"links":{"cited_paper":"/paper/1701.01652","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:08ad35c4a4d9014e135ceb3853810bbcd8e39b3a452856d3a24c7329c28fd6cf","observation_id":"f24ee920-497e-422a-8dc9-f014968d4988","resolution":{"observed_at":"2026-08-11T13:24:44.475571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.1785","last_updated":"2011-02-28T08:56:52Z","snapshot_observed_at":"2026-07-06T02:23:14.296540Z","submitted_at":"2011-02-09T05:24:17Z","title":"Fatal Effects of Charges on Stability of Black Holes in Lovelock Theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.1785","snapshot_observed_at":"2026-08-11T13:24:44.482721Z","title":"Takahashi, Prog","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.482721Z"},"links":{"cited_paper":"/paper/1102.1785","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:64ece6365b1626e17c61885dce6efee95130212f9fc5ce14dd4a9c0211a9dcfd","observation_id":"d6d7ef9e-3cb6-48b8-9122-3cdb1b67b199","resolution":{"observed_at":"2026-08-11T13:24:44.482721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.01656","last_updated":"2017-05-03T23:51:11Z","snapshot_observed_at":"2026-07-06T05:40:46.652042Z","submitted_at":"2017-05-03T23:51:11Z","title":"The portrait of eikonal instability in Lovelock theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.01656","snapshot_observed_at":"2026-08-11T13:24:44.492496Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.492496Z"},"links":{"cited_paper":"/paper/1705.01656","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:64ff0bf03c68ee88c7176ae5dd8df10749bf7b7b8ec90d12bc422ba0d3bb58b4","observation_id":"3bcce642-94b2-4f02-ab04-c9edbccf5040","resolution":{"observed_at":"2026-08-11T13:24:44.492496Z","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":"2026-08-09T03:20:00.764882Z","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":"2026-08-11T13:24:44.499630Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.499630Z"},"links":{"cited_paper":"/paper/2003.01188","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:6b0cec2bad8bef6facc10f86dd7f70b502276bf750bb4bb14dd7ce0c712a579c","observation_id":"b186ed22-f1f0-4e66-b1b7-66a2fd8c9297","resolution":{"observed_at":"2026-08-11T13:24:44.499630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.00083","last_updated":"2017-04-18T11:57:59Z","snapshot_observed_at":"2026-07-06T05:08:54.821151Z","submitted_at":"2016-09-01T01:39:55Z","title":"Black Hole Ringing, Quasinormal Modes, and Light Rings","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.00083","snapshot_observed_at":"2026-08-11T13:24:44.508133Z","title":"Khanna and R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.508133Z"},"links":{"cited_paper":"/paper/1609.00083","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:44f7e8dfe435c4d8843e6b1c73ee1d6824d916dc65f6c4ea1c0a6bbb20d0cc5a","observation_id":"25d73c61-5e01-494f-a6a5-9276a1e6e04f","resolution":{"observed_at":"2026-08-11T13:24:44.508133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.03483","last_updated":"2019-03-13T11:50:37Z","snapshot_observed_at":"2026-07-06T07:37:59.398044Z","submitted_at":"2019-03-08T15:07:03Z","title":"Quasinormal modes, scattering and Hawking radiation in the vicinity of Einstein-dilaton-Gauss-Bonnet black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.03483","snapshot_observed_at":"2026-08-11T13:24:44.520320Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.520320Z"},"links":{"cited_paper":"/paper/1903.03483","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:2e824df244548c9bf3eb9bd7b9e4447e92a166778c8c791561a4d89dbe2bc1b2","observation_id":"d8de0ebf-e42a-452e-ac4c-91985522511b","resolution":{"observed_at":"2026-08-11T13:24:44.520320Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.04718","last_updated":"2018-07-11T22:30:49Z","snapshot_observed_at":"2026-07-06T06:38:43.563060Z","submitted_at":"2018-05-12T13:13:49Z","title":"How to tell the shape of a wormhole by its quasinormal modes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.04718","snapshot_observed_at":"2026-08-11T13:24:44.527025Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.527025Z"},"links":{"cited_paper":"/paper/1805.04718","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:74b1c3d9e93f4cf64f9ddb08783b7ce24939b035127a2737a308dadf66e975ce","observation_id":"420c37ef-559b-47ac-8f34-e3c4a9f7d807","resolution":{"observed_at":"2026-08-11T13:24:44.527025Z","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":"2026-08-11T13:24:44.532116Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.532116Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:3b7def8a9880b318ddf71a911f43c1dbde5fe9b8dc5e4810125986dce98846f4","observation_id":"2fab3136-c311-4e91-96fe-63e9384128ec","resolution":{"observed_at":"2026-08-11T13:24:44.532116Z","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":"2026-08-11T13:24:44.539984Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.539984Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:828f16f7b15198fba94d12d00b4a6236cba23d02b497b5c4895dbe1decb20d3f","observation_id":"ca32f1f8-165f-4057-b62f-460883f83d95","resolution":{"observed_at":"2026-08-11T13:24:44.539984Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T13:24:46.132511Z","title":null,"venue":null,"work_id":"f87ad2ca-cf98-441e-9e88-dbd2e0c75bfd","year":1971},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.549450Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:35d232811d22d8347b885affa1e171b86f68ad77882c2046e80199ed9b344cba","observation_id":"5f735ba9-069e-495a-9886-d4f548c13a58","resolution":{"observed_at":"2026-08-11T13:24:46.137366Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T13:24:44.558554Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.558554Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:17da8adf95f495ab1c6d4477b064cd483b367af5cfa6a14383b5028a10f51f7c","observation_id":"0c176ccd-973a-42ba-ae3c-3b28da9d1e91","resolution":{"observed_at":"2026-08-11T13:24:44.558554Z","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":"2026-08-11T13:24:44.563576Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.563576Z"},"links":{"citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:a4e474f46cd1d635d4b88600da7b478d54ff3b8a02e92e92825cfa835ff76daa","observation_id":"643df63e-efeb-4002-9d01-5af533bc2bf7","resolution":{"observed_at":"2026-08-11T13:24:44.563576Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9803033","last_updated":"1998-03-10T14:15:53Z","snapshot_observed_at":"2026-07-07T03:28:45.058552Z","submitted_at":"1998-03-10T14:15:53Z","title":"The many faces of superradiance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9803033","snapshot_observed_at":"2026-08-11T13:24:44.568005Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.568005Z"},"links":{"cited_paper":"/paper/gr-qc/9803033","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:c977dd6db92776b4066c4862010e105e03060c1ee8bdbd9d60f6a3fb8cead9c0","observation_id":"aae89bac-5b42-4337-ae33-195040bc2461","resolution":{"observed_at":"2026-08-11T13:24:44.568005Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.04791","last_updated":"2017-06-14T15:29:09Z","snapshot_observed_at":"2026-08-08T10:50:36.127524Z","submitted_at":"2017-04-16T16:04:54Z","title":"Superradiant Instability and Backreaction of Massive Vector Fields around Kerr Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.04791","snapshot_observed_at":"2026-08-11T13:24:44.577084Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.577084Z"},"links":{"cited_paper":"/paper/1704.04791","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:98bd96a10b4156c3e4f4c72a3c99ee41086cd730a4eeb9e01b47602d056ef7dc","observation_id":"b98c209e-bcf3-4979-9e20-ff039279ac60","resolution":{"observed_at":"2026-08-11T13:24:44.577084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.1872","last_updated":"2012-05-09T05:30:55Z","snapshot_observed_at":"2026-08-10T02:29:33.881521Z","submitted_at":"2012-05-09T05:30:55Z","title":"On the instability regime of the rotating Kerr spacetime to massive scalar perturbations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.1872","snapshot_observed_at":"2026-08-11T13:24:44.581958Z","title":"Hod, Phys","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.581958Z"},"links":{"cited_paper":"/paper/1205.1872","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:b67c10a857ac7df7abad88c67cce0307579a51360e08fcec933ead484f687c55","observation_id":"afc375b0-5752-4fca-80b8-64fd9a6e0e3f","resolution":{"observed_at":"2026-08-11T13:24:44.581958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.0846","last_updated":"2008-11-22T07:05:12Z","snapshot_observed_at":"2026-07-31T00:57:25.952874Z","submitted_at":"2008-01-07T06:49:20Z","title":"Superradiant instability for black holes immersed in a magnetic field","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.0846","snapshot_observed_at":"2026-08-11T13:24:44.586340Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.586340Z"},"links":{"cited_paper":"/paper/0801.0846","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:330f81bad8f08aea0af4864d58a44a79453271d885b9ab0549c12925fe7e0ea1","observation_id":"21366b8d-30d7-4722-b327-5d421bac1de5","resolution":{"observed_at":"2026-08-11T13:24:44.586340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.0019","last_updated":"2014-06-11T09:53:01Z","snapshot_observed_at":"2026-07-06T03:45:07.524590Z","submitted_at":"2014-05-30T21:41:35Z","title":"Charged scalar field instability between the event and cosmological horizons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.0019","snapshot_observed_at":"2026-08-11T13:24:44.595173Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.595173Z"},"links":{"cited_paper":"/paper/1406.0019","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:0367c2ea88de5d91e04085d08887751f37142da573330de7856a7560f89709ae","observation_id":"f5e012e9-d290-4148-ae85-4a531670eb43","resolution":{"observed_at":"2026-08-11T13:24:44.595173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.01595","last_updated":"2022-02-26T13:35:01Z","snapshot_observed_at":"2026-07-06T12:04:35.968417Z","submitted_at":"2021-11-02T13:52:28Z","title":"Scattering and absorption of a scalar field impinging on a charged black hole in the Einstein-Maxwell-dilaton theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.01595","snapshot_observed_at":"2026-08-11T13:24:44.600162Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.600162Z"},"links":{"cited_paper":"/paper/2111.01595","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:ea60a4412ab083a16a5db1785642949468dbff891c439a817f2810b923b9a56c","observation_id":"c47fcdde-77d7-46e4-868b-a50337c86f31","resolution":{"observed_at":"2026-08-11T13:24:44.600162Z","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":"2026-08-11T13:24:44.606464Z","title":"Zhu, S.-J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-11T13:24:44.606464Z"},"links":{"cited_paper":"/paper/1405.4931","citing_paper":"/paper/2412.13385"},"observation_digest":"sha256:1f5a4901f5e5d525ec805b8e6b2373358f572f87ed9522942337e3d1a77968aa","observation_id":"cc1590ca-aff2-4f01-8313-c8b665798afe","resolution":{"observed_at":"2026-08-11T13:24:44.606464Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.13385","last_updated":"2024-12-17T23:44:19Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-11T19:20:12.801528Z","submitted_at":"2024-12-17T23:44:19Z","title":"Quasinormal modes and grey-body factors of Morris-Thorne wormholes"},"reference_resolution":{"displayed":83,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":81,"verified_exact":2,"verified_fuzzy":0},"total_outbound_references":83},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 83 of 83 outbound references and 14 inbound Pith citation observations for arXiv:2412.13385."}