{"as_of":"2026-08-09T14:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:66e0775331ad3dc04cfb530f1775524adfba0393eaab177ce1a4f5b97dd3779b","coverage":[{"denominator":74,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":74,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T21:39:59.889352Z","state":"measured"},{"denominator":75,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":75,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:46:34.363642Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-07T14:46:42.727865Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"cited_work":{"arxiv_id":"2502.04782","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.04782","snapshot_observed_at":"2026-08-07T14:46:42.727865Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","venue":"gr-qc","work_id":"13fc49f6-d2c6-43a5-9ccd-de67cffde2b1","year":2025},"citing_paper":{"arxiv_id":"2505.17947","last_updated":"2025-05-23T14:24:05Z","snapshot_observed_at":"2026-08-08T21:45:31.184340Z","submitted_at":"2025-05-23T14:24:05Z","title":"Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T14:46:34.363642Z"},"links":{"cited_paper":"/paper/2502.04782","citing_paper":"/paper/2505.17947"},"observation_digest":"sha256:ef69c434740dc061c5ee5c0ecd0fc9bd18c24b3a596e419d8581a9866434336f","observation_id":"0498e205-73d7-4d6d-8151-751e6b1615bf","resolution":{"observed_at":"2026-08-07T14:46:42.789531Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2502.04782/citation-record","integrity":"/paper/2502.04782/integrity","json":"/paper/2502.04782/citation-record.json","paper":"/paper/2502.04782"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"hep-th/0112090","last_updated":"2001-12-18T14:38:11Z","snapshot_observed_at":"2026-07-07T04:42:02.517683Z","submitted_at":"2001-12-11T18:01:56Z","title":"Lorentz invariance with an invariant energy scale","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0112090","snapshot_observed_at":"2026-08-08T21:39:59.625297Z","title":"Magueijo and L","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.625297Z"},"links":{"cited_paper":"/paper/hep-th/0112090","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:531a1ad1469f546e0bb871246b49dce8091d2b0c1f9e273264c195491f54cde4","observation_id":"4c44e1b4-64ed-4aee-9c26-87d4287a1499","resolution":{"observed_at":"2026-08-08T21:39:59.625297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.1041","last_updated":"2011-03-24T17:18:30Z","snapshot_observed_at":"2026-07-06T02:16:18.442150Z","submitted_at":"2010-10-06T00:28:09Z","title":"f(T) Gravity and local Lorentz invariance","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.1041","snapshot_observed_at":"2026-08-08T21:39:59.629822Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.629822Z"},"links":{"cited_paper":"/paper/1010.1041","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:4aa92528767e3f377fb51cf57023e60f848a86f4c0566317c99228ba68b7d37c","observation_id":"d2c9f693-7a29-48e9-91b1-a1eb56e9a3f1","resolution":{"observed_at":"2026-08-08T21:39:59.629822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.01725","last_updated":"2018-07-04T18:03:25Z","snapshot_observed_at":"2026-08-01T16:50:51.907456Z","submitted_at":"2018-07-04T18:03:25Z","title":"A systematic approach to generalisations of General Relativity and their cosmological implications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.01725","snapshot_observed_at":"2026-08-08T21:39:59.633608Z","title":"Heisenberg, A systematic approach to generalisations of General Relativity and their cosmological implications, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.633608Z"},"links":{"cited_paper":"/paper/1807.01725","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:15fc90d8d2dc292a87c3c917e2fa3898f17a4f3c0920184a6709502ce937c4ba","observation_id":"c88373d4-fd22-4ae5-a077-2c456803d0f1","resolution":{"observed_at":"2026-08-08T21:39:59.633608Z","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":"2026-08-08T21:40:01.379103Z","title":"Mart ´ınez-Huerta, R","venue":null,"work_id":"c7c555c7-9796-4925-b965-7d445eae37ea","year":2020},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.637663Z"},"links":{"citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:abf8d1b321087131e362314b5cacb61165c3b6459e6065310e8d435208edf528","observation_id":"17379079-3faa-47c0-80ad-988a1736f5bd","resolution":{"observed_at":"2026-08-08T21:40:01.382519Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.04394","last_updated":"2021-04-09T14:32:40Z","snapshot_observed_at":"2026-08-04T02:52:29.777159Z","submitted_at":"2021-04-09T14:32:40Z","title":"A Short Review of Loop Quantum Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.04394","snapshot_observed_at":"2026-08-08T21:39:59.641062Z","title":"Ashtekar and E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.641062Z"},"links":{"cited_paper":"/paper/2104.04394","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:471bbeb68b658691bac3d97afbd3b66fdcb610db9065f1d71da99f0c2d794039","observation_id":"d73e615c-8433-4776-a544-041f01cfd4bf","resolution":{"observed_at":"2026-08-08T21:39:59.641062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.04028","last_updated":"2016-09-13T20:04:32Z","snapshot_observed_at":"2026-08-08T21:45:32.712220Z","submitted_at":"2016-09-13T20:04:32Z","title":"Conformal loop quantum gravity coupled to the Standard Model","version":1},"cited_work":{"arxiv_id":"1609.04028","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.04028","snapshot_observed_at":"2026-08-08T21:40:01.308125Z","title":"Conformal loop quantum gravity coupled to the Standard Model","venue":"gr-qc","work_id":"1cb9aea0-b89e-4032-a3b9-74e8472faea6","year":2016},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.644875Z"},"links":{"cited_paper":"/paper/1609.04028","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:d9bd00d1f279fa90509f7a8c80cc9ae8f2e24d4c0503b1b550d1f56e522c178a","observation_id":"81296e50-18ac-4c59-a98b-aaebc4fab37c","resolution":{"observed_at":"2026-08-08T21:40:01.312022Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9809521","last_updated":"1998-09-24T19:07:01Z","snapshot_observed_at":"2026-08-06T14:55:08.379330Z","submitted_at":"1998-09-24T19:07:01Z","title":"Lorentz-Violating Extension of the Standard Model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9809521","snapshot_observed_at":"2026-08-08T21:39:59.648948Z","title":"Colladay and V","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.648948Z"},"links":{"cited_paper":"/paper/hep-ph/9809521","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:cff96de5d19662263141d2dae8c8887ac2d2a4b356b0f024318b8e3dc105ec19","observation_id":"ca756788-4efe-4aa0-a74f-8b21bc0c0996","resolution":{"observed_at":"2026-08-08T21:39:59.648948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.03378","last_updated":"2018-02-02T20:05:08Z","snapshot_observed_at":"2026-08-08T21:45:32.017355Z","submitted_at":"2017-06-11T16:37:55Z","title":"Testing CPT violation with correlated neutral mesons","version":3},"cited_work":{"arxiv_id":"1706.03378","doi":null,"metadata_source":"pith","pith_arxiv_id":"1706.03378","snapshot_observed_at":"2026-08-08T21:40:01.282861Z","title":"Testing CPT violation with correlated neutral mesons","venue":"hep-ph","work_id":"55f693b5-8268-449b-a44e-bea518efddff","year":2017},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.652671Z"},"links":{"cited_paper":"/paper/1706.03378","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:d597708b7c9122cc35b528f455ba77160fd8817a3c808ba1407681b17feae9aa","observation_id":"c9bfb34b-6d15-4197-b2fe-2b5fc9cf3992","resolution":{"observed_at":"2026-08-08T21:40:01.287248Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.06613","last_updated":"2023-12-06T02:54:06Z","snapshot_observed_at":"2026-07-06T16:05:35.645037Z","submitted_at":"2023-08-12T17:08:28Z","title":"Static and spherically symmetric black holes in gravity with a background Kalb-Ramond field","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.06613","snapshot_observed_at":"2026-08-08T21:39:59.656572Z","title":"Yang, Y .-Z","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.656572Z"},"links":{"cited_paper":"/paper/2308.06613","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:6cfb725a0caf96c32ee2c814078b73544b1a394a0d8caea4af8606be32bc0cbe","observation_id":"80ee3eaa-6e4d-49f1-928f-f8814aa83718","resolution":{"observed_at":"2026-08-08T21:39:59.656572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.13555","last_updated":"2024-09-26T14:24:38Z","snapshot_observed_at":"2026-07-06T16:36:11.682777Z","submitted_at":"2023-10-20T14:57:53Z","title":"Electrically charged black holes in gravity with a background Kalb-Ramond field","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.13555","snapshot_observed_at":"2026-08-08T21:39:59.660043Z","title":"Duan, J.-Y","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.660043Z"},"links":{"cited_paper":"/paper/2310.13555","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:24fba082d81a867cebf2d6cb508104388d294cde2a9b16803d90b60da748e97c","observation_id":"c1799c68-a7c2-46a5-a7b9-4f86ac73d135","resolution":{"observed_at":"2026-08-08T21:39:59.660043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.15778","last_updated":"2024-03-26T17:49:49Z","snapshot_observed_at":"2026-07-06T16:24:26.535120Z","submitted_at":"2023-09-27T16:52:47Z","title":"Exploring antisymmetric tensor effects on black hole shadows and quasinormal frequencies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.15778","snapshot_observed_at":"2026-08-08T21:39:59.663545Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.663545Z"},"links":{"cited_paper":"/paper/2309.15778","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:61d3d55041012f5c2e5824b6324a880412fdfa5f824284445dc6282e75e47496","observation_id":"69afc3e5-8cee-42a8-93d5-bf7da2eddb9a","resolution":{"observed_at":"2026-08-08T21:39:59.663545Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13461","last_updated":"2024-08-21T11:02:40Z","snapshot_observed_at":"2026-08-05T15:24:08.933708Z","submitted_at":"2024-06-19T11:38:05Z","title":"Static neutral black holes in Kalb-Ramond gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13461","snapshot_observed_at":"2026-08-08T21:39:59.667429Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.667429Z"},"links":{"cited_paper":"/paper/2406.13461","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:db3aefb7fb4ea10c77819d50215764038f4dda6d44b28467c26dfab84b354843","observation_id":"56842102-8f44-4711-9c0d-67282e846eff","resolution":{"observed_at":"2026-08-08T21:39:59.667429Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07416","last_updated":"2024-07-14T03:29:36Z","snapshot_observed_at":"2026-07-06T18:44:03.869577Z","submitted_at":"2024-07-10T07:16:50Z","title":"Shadow of slowly rotating Kalb-Ramond black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.07416","snapshot_observed_at":"2026-08-08T21:39:59.671228Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.671228Z"},"links":{"cited_paper":"/paper/2407.07416","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:5ca5ea993c7e92778782e6546bd90c1aac056723948d2a7793a67c2dc294f4db","observation_id":"7260e4ab-808b-4ad0-97e5-0fea131e7ea9","resolution":{"observed_at":"2026-08-08T21:39:59.671228Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.10721","last_updated":"2025-02-24T13:03:15Z","snapshot_observed_at":"2026-08-08T23:13:12.239994Z","submitted_at":"2024-04-16T16:54:00Z","title":"The impact of an antisymmetric tensor on charged black holes: evaporation process, geodesics, deflection angle, scattering effects and quasinormal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.10721","snapshot_observed_at":"2026-08-08T21:39:59.674915Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.674915Z"},"links":{"cited_paper":"/paper/2404.10721","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:4d1651c3877d83e1a2a4e536c23b140adf5e8c312fc8882a5a1c9a6827c19172","observation_id":"35422b08-7963-4a11-bed6-f004b43f0de7","resolution":{"observed_at":"2026-08-08T21:39:59.674915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07017","last_updated":"2024-07-09T16:35:26Z","snapshot_observed_at":"2026-08-06T21:03:47.620078Z","submitted_at":"2024-07-09T16:35:26Z","title":"Shadows, greybody factors, emission rate, topological charge, and phase transitions for a charged black hole with a Kalb-Ramond field background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.07017","snapshot_observed_at":"2026-08-08T21:39:59.678338Z","title":"Hosseinifar, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.678338Z"},"links":{"cited_paper":"/paper/2407.07017","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:81edfeb8d231a2b4c1ba6d964af8f38a0529060f1deac2f687068f157e723592","observation_id":"7edd0c29-beb2-40a4-b166-ce9c41f410e3","resolution":{"observed_at":"2026-08-08T21:39:59.678338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.03090","last_updated":"2024-08-06T10:43:54Z","snapshot_observed_at":"2026-07-06T18:57:22.433852Z","submitted_at":"2024-08-06T10:43:54Z","title":"Thermal, topological, and scattering effects of an AdS charged black hole with an antisymmetric tensor background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.03090","snapshot_observed_at":"2026-08-08T21:39:59.681683Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.681683Z"},"links":{"cited_paper":"/paper/2408.03090","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:75dcef75ef985d4d3f92c1a2233faa69385983a146e312b888c650472d3f7d38","observation_id":"c9aab098-9a2b-471b-91e8-21d97b5792a8","resolution":{"observed_at":"2026-08-08T21:39:59.681683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.4940","last_updated":"2013-02-14T17:48:40Z","snapshot_observed_at":"2026-07-06T02:57:54.811713Z","submitted_at":"2012-10-17T20:03:29Z","title":"Towards thermodynamics of universal horizons in Einstein-{\\ae}ther theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.4940","snapshot_observed_at":"2026-08-08T21:39:59.685327Z","title":"Berglund, J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.685327Z"},"links":{"cited_paper":"/paper/1210.4940","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:f6fb626b15b49cce60f42583f0d05b6a1fbc0ae10d7395bd556b4b20b65cde01","observation_id":"3a6529b4-fd43-46db-8356-8530fb6a71fb","resolution":{"observed_at":"2026-08-08T21:39:59.685327Z","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":"2026-08-08T21:40:01.369233Z","title":null,"venue":null,"work_id":"3cc1749a-9409-4d5b-9840-091384b20933","year":1989},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.688700Z"},"links":{"citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:6a582b65d17e2dc556b26a1e8e156be703aa0baa28f8c6e38926f56889c13bf2","observation_id":"24458283-a7c3-4f76-9ea4-a1b328227ed7","resolution":{"observed_at":"2026-08-08T21:40:01.372545Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02273","last_updated":"2017-11-07T03:46:30Z","snapshot_observed_at":"2026-08-02T03:29:27.920890Z","submitted_at":"2017-11-07T03:46:30Z","title":"An exact Schwarzschild-like solution in a bumblebee gravity model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.02273","snapshot_observed_at":"2026-08-08T21:39:59.692052Z","title":"Casana, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.692052Z"},"links":{"cited_paper":"/paper/1711.02273","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:b30010a05cb29170a3262b0374b7a869ca65e9063cf78a3a264f2d1963e6d58d","observation_id":"39c6fd5e-42f4-406f-8b8f-662e5ce628c1","resolution":{"observed_at":"2026-08-08T21:39:59.692052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.12841","last_updated":"2021-02-01T16:38:29Z","snapshot_observed_at":"2026-08-07T20:03:45.122406Z","submitted_at":"2020-11-25T15:50:55Z","title":"Black holes with a cosmological constant in bumblebee gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.12841","snapshot_observed_at":"2026-08-08T21:39:59.695522Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.695522Z"},"links":{"cited_paper":"/paper/2011.12841","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:ec667a2b21646f4523d710316bfc7de59e65a6ec42f7240199f2d8dc78c64529","observation_id":"be267fe9-c2ed-42c4-9d6f-21d8e96e04ea","resolution":{"observed_at":"2026-08-08T21:39:59.695522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.11821","last_updated":"2023-09-20T15:44:12Z","snapshot_observed_at":"2026-07-06T14:21:26.429460Z","submitted_at":"2022-11-21T19:42:26Z","title":"Vacuum solution within a metric-affine bumblebee gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.11821","snapshot_observed_at":"2026-08-08T21:39:59.699113Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.699113Z"},"links":{"cited_paper":"/paper/2211.11821","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:d1ee0c825529e5d558fdf04190129e2330749b9cc9df1db7e51713cd36346dad","observation_id":"62031e78-987e-4c99-aae5-2faa83f94cd6","resolution":{"observed_at":"2026-08-08T21:39:59.699113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.09911","last_updated":"2019-01-15T00:37:06Z","snapshot_observed_at":"2026-07-06T06:35:33.271817Z","submitted_at":"2018-04-26T06:43:57Z","title":"Exact traversable wormhole solution in bumblebee gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.09911","snapshot_observed_at":"2026-08-08T21:39:59.702677Z","title":"¨Ovg¨un, K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.702677Z"},"links":{"cited_paper":"/paper/1804.09911","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:906f1a3059111be1692c2deef5f156f480545d49845838906908037dcd38494f","observation_id":"0852652b-13ac-4a61-8025-e256f5b9bef8","resolution":{"observed_at":"2026-08-08T21:39:59.702677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.02674","last_updated":"2020-02-13T03:35:27Z","snapshot_observed_at":"2026-08-06T10:31:54.445754Z","submitted_at":"2019-10-07T08:48:57Z","title":"Exact Kerr-like solution and its shadow in a gravity model with spontaneous Lorentz symmetry breaking","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.02674","snapshot_observed_at":"2026-08-08T21:39:59.706152Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.706152Z"},"links":{"cited_paper":"/paper/1910.02674","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:949391120400ab371ff5de3cc2b170197b311df7bc10d79500952e675f2ad33a","observation_id":"05e391c5-7db5-47f4-96a9-dcf6faf7882b","resolution":{"observed_at":"2026-08-08T21:39:59.706152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.01580","last_updated":"2023-06-26T00:49:25Z","snapshot_observed_at":"2026-08-05T19:53:03.291699Z","submitted_at":"2023-02-03T07:18:04Z","title":"Rotating BTZ-like black hole and central charges in Einstein-bumblebee gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.01580","snapshot_observed_at":"2026-08-08T21:39:59.709652Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.709652Z"},"links":{"cited_paper":"/paper/2302.01580","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:7bce160b10aed809e11fd946219a9d45769241fb5a39d68abbb416e5da4dfd0c","observation_id":"04148a90-68d2-47be-a1bb-1829a666ad2c","resolution":{"observed_at":"2026-08-08T21:39:59.709652Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.13335","last_updated":"2022-02-02T02:09:10Z","snapshot_observed_at":"2026-07-06T10:44:50.656480Z","submitted_at":"2021-02-26T07:26:12Z","title":"Einstein-Gauss-Bonnet gravity coupled to bumblebee field in four dimensional spacetime","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.13335","snapshot_observed_at":"2026-08-08T21:39:59.713496Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.713496Z"},"links":{"cited_paper":"/paper/2102.13335","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:f5f4ab6e997ab6129f8a4fba2f077c0870b2aed26a68db4aeea108faff1e2d11","observation_id":"fb627f81-d5e6-4668-a8b6-248312ad0c43","resolution":{"observed_at":"2026-08-08T21:39:59.713496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.07956","last_updated":"2021-05-13T23:14:19Z","snapshot_observed_at":"2026-08-06T12:25:34.693835Z","submitted_at":"2021-05-13T23:14:19Z","title":"Quasinormal frequencies for a black hole in a bumblebee gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.07956","snapshot_observed_at":"2026-08-08T21:39:59.716934Z","title":"Oliveira, D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.716934Z"},"links":{"cited_paper":"/paper/2105.07956","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:a72117aee58a188258a3fa14c026ba125c0fbc9ce04def7ddfc5c865407749da","observation_id":"dd767521-d071-467b-a872-738c6f2a2c07","resolution":{"observed_at":"2026-08-08T21:39:59.716934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.03156","last_updated":"2023-01-30T07:29:45Z","snapshot_observed_at":"2026-07-06T14:14:57.954649Z","submitted_at":"2022-11-06T15:45:31Z","title":"QNMs of slowly rotating Einstein-Bumblebee Black Hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.03156","snapshot_observed_at":"2026-08-08T21:39:59.720400Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.720400Z"},"links":{"cited_paper":"/paper/2211.03156","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:062a7a53dcbd73d2ad18a7128de16bdddb6aa77bbbce9f55b320e8576e151ca4","observation_id":"abe5a618-453b-421f-b349-bd15f666eb14","resolution":{"observed_at":"2026-08-08T21:39:59.720400Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.10412","last_updated":"2024-08-17T12:41:25Z","snapshot_observed_at":"2026-08-08T12:10:49.817383Z","submitted_at":"2023-08-21T01:38:06Z","title":"Quasinormal modes of the bumblebee black holes with a global monopole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.10412","snapshot_observed_at":"2026-08-08T21:39:59.723812Z","title":"Malik, Quasinormal Modes of the Bumblebee Black Holes with a Global Monopole, Int","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.723812Z"},"links":{"cited_paper":"/paper/2308.10412","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:e7df2acfedd95f354bb732a62a4819dcd5881f9dd9d4f8138acd1227356cd7d9","observation_id":"95786294-ec7d-4e28-85ec-a3655778d166","resolution":{"observed_at":"2026-08-08T21:39:59.723812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.07757","last_updated":"2024-04-08T16:11:17Z","snapshot_observed_at":"2026-07-06T17:15:42.343063Z","submitted_at":"2024-01-15T15:10:01Z","title":"Dynamic instability analysis for bumblebee black holes: the odd parity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.07757","snapshot_observed_at":"2026-08-08T21:39:59.727398Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.727398Z"},"links":{"cited_paper":"/paper/2401.07757","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:568f346e14328851f890760224ee32bef4b420ba8cdf5c8091bc62f94aa6a90f","observation_id":"30df1b79-26d1-43bb-b7f7-d3953bf2292d","resolution":{"observed_at":"2026-08-08T21:39:59.727398Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.14916","last_updated":"2020-11-27T12:50:38Z","snapshot_observed_at":"2026-08-07T04:32:12.144165Z","submitted_at":"2020-11-27T12:50:38Z","title":"Bumblebee gravity with a Kerr-Sen-like solution and its Shadow","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.14916","snapshot_observed_at":"2026-08-08T21:39:59.731175Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.731175Z"},"links":{"cited_paper":"/paper/2011.14916","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:4b2cd9f26a122ce70c8973d3892ed9629fd34bcac6b7f3ddb7957659830e9ee8","observation_id":"36db37b9-0359-4030-8401-bc50fc5c9956","resolution":{"observed_at":"2026-08-08T21:39:59.731175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.11003","last_updated":"2022-10-16T08:53:19Z","snapshot_observed_at":"2026-07-06T13:12:39.361042Z","submitted_at":"2022-05-23T02:34:56Z","title":"Strong gravitational lensing and shadow constraint from M87* of slowly rotating Kerr-like black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.11003","snapshot_observed_at":"2026-08-08T21:39:59.734632Z","title":"Kuang and A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.734632Z"},"links":{"cited_paper":"/paper/2205.11003","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:ea856eb6456035e34cfc445e3c5e0a6ee7ae8b828c626f8c21c53253c358a0cc","observation_id":"1dcd978a-5485-4907-833a-6a389e5a98da","resolution":{"observed_at":"2026-08-08T21:39:59.734632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.13661","last_updated":"2025-06-20T15:19:44Z","snapshot_observed_at":"2026-07-06T19:35:21.868885Z","submitted_at":"2024-10-17T15:22:16Z","title":"Testing black holes with cosmological constant in Einstein-bumblebee gravity through the black hole shadow using EHT data and deflection angle","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.13661","snapshot_observed_at":"2026-08-08T21:39:59.741778Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.741778Z"},"links":{"cited_paper":"/paper/2410.13661","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:c7ae67ed2c5719a63220ddf2e6626f0418e2244148c15a80dbca429a839527be","observation_id":"f81c90bf-34fa-4944-8885-c1c0c96855af","resolution":{"observed_at":"2026-08-08T21:39:59.741778Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.08396","last_updated":"2025-03-22T06:31:24Z","snapshot_observed_at":"2026-08-06T18:04:23.309787Z","submitted_at":"2024-07-11T11:02:18Z","title":"Charged spherically symmetric and slowly rotating charged black hole solutions in bumblebee gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.08396","snapshot_observed_at":"2026-08-08T21:39:59.745382Z","title":"Liu, W.-D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.745382Z"},"links":{"cited_paper":"/paper/2407.08396","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:262b5b5e8c79c10e5d36c330e22638fed87e5273dd7d449825d6d2e7a6e3bd24","observation_id":"cc0e283d-58c4-4a1d-ba65-5d2199195715","resolution":{"observed_at":"2026-08-08T21:39:59.745382Z","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":"2026-08-08T21:39:59.748916Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.748916Z"},"links":{"citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:e4ece92ad6b3558a6e8e6519c03266a6344788b68c3c324262e7fc86d097e18e","observation_id":"6b53e67a-34ea-4cb7-b54f-945e464418f8","resolution":{"observed_at":"2026-08-08T21:39:59.748916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.05569","last_updated":"2024-10-04T12:10:18Z","snapshot_observed_at":"2026-07-06T18:59:13.491643Z","submitted_at":"2024-08-10T14:44:21Z","title":"Light rings and shadows of static black holes in effective quantum gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.05569","snapshot_observed_at":"2026-08-08T21:39:59.752169Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.752169Z"},"links":{"cited_paper":"/paper/2408.05569","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:cc9c963b6e9843f5b7d5ceb02614e0b1d8b078062b51cc783dfba41a3ff860de","observation_id":"dfc68844-5f6e-4915-8d95-e79599436145","resolution":{"observed_at":"2026-08-08T21:39:59.752169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.06218","last_updated":"2024-09-10T05:03:17Z","snapshot_observed_at":"2026-08-04T11:25:07.705099Z","submitted_at":"2024-09-10T05:03:17Z","title":"Testing EGB gravity coupled to bumblebee field and black hole parameter estimation with EHT observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.06218","snapshot_observed_at":"2026-08-08T21:39:59.755407Z","title":"Afrin, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.755407Z"},"links":{"cited_paper":"/paper/2409.06218","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:e509dc45641031ef29774f88bd0a7d76b6c688d6bf6964f94fabf237b574f1ba","observation_id":"d1393925-765b-4b3d-a738-a5806ec4a6af","resolution":{"observed_at":"2026-08-08T21:39:59.755407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.21681","last_updated":"2024-12-27T14:01:41Z","snapshot_observed_at":"2026-07-06T19:41:15.267950Z","submitted_at":"2024-10-29T03:05:03Z","title":"Lorentz violation alleviates gravitationally induced entanglement degradation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.21681","snapshot_observed_at":"2026-08-08T21:39:59.762350Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.762350Z"},"links":{"cited_paper":"/paper/2410.21681","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:6b0bee8abb3a0fd0a2e86f7bbab174c09e4b19329ae4a030432fa3ef1e008f62","observation_id":"67bd884f-380c-43be-9bdf-575627a62c39","resolution":{"observed_at":"2026-08-08T21:39:59.762350Z","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":"2026-08-08T21:39:59.765866Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.765866Z"},"links":{"citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:44a1fa0a2d344bf8685363ef42e4ce461aacb0b94bc4fc59f0c2f4e133a0006b","observation_id":"2d15042e-6ecb-469c-99b3-3df2fe26bfad","resolution":{"observed_at":"2026-08-08T21:39:59.765866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.00927","last_updated":"2025-05-08T11:37:21Z","snapshot_observed_at":"2026-07-06T20:15:31.955797Z","submitted_at":"2025-01-01T18:52:50Z","title":"How does non-metricity affect particle creation and evaporation in bumblebee gravity?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.00927","snapshot_observed_at":"2026-08-08T21:39:59.769324Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.769324Z"},"links":{"cited_paper":"/paper/2501.00927","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:4ec3c7255d7fa816c58d34a1165a0655eca336736846df768786ee12dbe37b4c","observation_id":"8748ad47-ed05-4b87-a418-d75f89cb5f5c","resolution":{"observed_at":"2026-08-08T21:39:59.769324Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.18871","last_updated":"2023-12-26T20:46:21Z","snapshot_observed_at":"2026-07-06T15:35:19.167704Z","submitted_at":"2023-05-30T09:05:37Z","title":"Gravitational traces of bumblebee gravity in metric-affine formalism","version":2},"cited_work":{"arxiv_id":"2305.18871","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.18871","snapshot_observed_at":"2026-08-08T21:40:00.612713Z","title":"Gravitational traces of bumblebee gravity in metric-affine formalism","venue":"gr-qc","work_id":"4f7e0049-5ab9-4bed-94b0-64a0a66c60e9","year":2023},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.772809Z"},"links":{"cited_paper":"/paper/2305.18871","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:945638473716c82fd5d21c5bdac348bd64823e3a47c1fc0a0ff291c59dd69009","observation_id":"ff1b272c-daf4-43b7-842f-8c4ab5d88ee1","resolution":{"observed_at":"2026-08-08T21:40:00.616703Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10937","last_updated":"2024-06-12T13:24:58Z","snapshot_observed_at":"2026-08-08T21:44:32.623188Z","submitted_at":"2023-07-20T15:09:15Z","title":"Gravitational waves effects in a Lorentz-violating scenario","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10937","snapshot_observed_at":"2026-08-08T21:39:59.776056Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.776056Z"},"links":{"cited_paper":"/paper/2307.10937","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:542bad3c4ccffa8c605a07e35eac8ae36c18ae6947db09f04a6407e68f7b38a8","observation_id":"2273bfd6-ea32-4809-b844-444faaf6ba20","resolution":{"observed_at":"2026-08-08T21:39:59.776056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.13594","last_updated":"2023-09-24T09:38:27Z","snapshot_observed_at":"2026-07-06T16:22:54.872252Z","submitted_at":"2023-09-24T09:38:27Z","title":"Probing Schwarzschild-like Black Holes in Metric-Affine Bumblebee Gravity with Accretion Disk, Deflection Angle, Greybody Bounds, and Neutrino Propagation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.13594","snapshot_observed_at":"2026-08-08T21:39:59.779459Z","title":"Lambiase, L","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.779459Z"},"links":{"cited_paper":"/paper/2309.13594","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:c035f0270e1d4eb37b452211f7dce51a42dc8b8cd0f761eb41d548df90fb55c6","observation_id":"740a4f17-40a0-42da-9244-0bbd5854a5d8","resolution":{"observed_at":"2026-08-08T21:39:59.779459Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13014","last_updated":"2024-06-10T16:20:40Z","snapshot_observed_at":"2026-08-09T08:20:13.315287Z","submitted_at":"2024-02-20T13:57:23Z","title":"An exact stationary axisymmetric vacuum solution within a metric--affine bumblebee gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.13014","snapshot_observed_at":"2026-08-08T21:39:59.782786Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.782786Z"},"links":{"cited_paper":"/paper/2402.13014","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:4652eb0ea5cc62e164674c6e74b6579c62b1e320834dc5983ac39a6d192369e3","observation_id":"e4e7ed5f-93f9-447b-9906-da9643818d73","resolution":{"observed_at":"2026-08-08T21:39:59.782786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12531","last_updated":"2024-09-19T07:50:17Z","snapshot_observed_at":"2026-07-06T19:18:00.304916Z","submitted_at":"2024-09-19T07:50:17Z","title":"Gravitational lensing and shadow by a Schwarzschild-like black hole in metric-affine bumblebee gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12531","snapshot_observed_at":"2026-08-08T21:39:59.786633Z","title":"Gao, Gravitational lensing and shadow by a Schwarzschild-like black hole in metric-affine bum- blebee gravity, Eur","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.786633Z"},"links":{"cited_paper":"/paper/2409.12531","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:e47e68dc34cc9d5db28d4eb93bb2e01bf79286d951dc42c7e4c131569a9e1c84","observation_id":"875ece3b-dee5-4fe1-bd33-091bc1c6934a","resolution":{"observed_at":"2026-08-08T21:39:59.786633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.05321","last_updated":"2024-07-07T10:17:25Z","snapshot_observed_at":"2026-08-04T12:07:10.016711Z","submitted_at":"2024-07-07T10:17:25Z","title":"Scattering effects of bumblebee gravity in metric affine formalism","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.05321","snapshot_observed_at":"2026-08-08T21:39:59.789600Z","title":"Heidari, C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.789600Z"},"links":{"cited_paper":"/paper/2407.05321","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:29d1b8b7b4d7722b3464ccb9cf58789debafea9e4c7ff993faac93d91dd28be1","observation_id":"5ecff6a1-3f43-4d98-89a0-b9fe65dbd45f","resolution":{"observed_at":"2026-08-08T21:39:59.789600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12909","last_updated":"2024-09-19T17:02:02Z","snapshot_observed_at":"2026-08-07T03:10:02.066485Z","submitted_at":"2024-09-19T17:02:02Z","title":"Constrain from shadows of $M87^*$ and $Sgr A^*$ and quasiperiodic oscillations of galactic microquasars on a black hole arising from metric-affine bumblebee model","version":1},"cited_work":{"arxiv_id":"2409.12909","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.12909","snapshot_observed_at":"2026-08-08T21:40:00.571169Z","title":"Constrain from shadows of $M87^*$ and $Sgr A^*$ and quasiperiodic oscillations of galactic microquasars on a black hole arising from metric-affine bumblebee model","venue":"gr-qc","work_id":"9411f206-be73-46f9-ac71-0bed7d17000e","year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.792979Z"},"links":{"cited_paper":"/paper/2409.12909","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:9c6fc33f1fde36beb81de7d69a8bb9f786e4acfcba5ea8f45284f3fd5a9cb277","observation_id":"b543ff4c-6511-4fdb-9b65-225bfc130187","resolution":{"observed_at":"2026-08-08T21:40:00.575097Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.17351","last_updated":"2025-01-08T19:39:14Z","snapshot_observed_at":"2026-07-06T19:22:23.126605Z","submitted_at":"2024-09-25T20:56:38Z","title":"Modified particle dynamics and thermodynamics in a traversable wormhole in bumblebee gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.17351","snapshot_observed_at":"2026-08-08T21:39:59.796691Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.796691Z"},"links":{"cited_paper":"/paper/2409.17351","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:7f5c3344aa45c443feeebae99d2b8b8683047184388f6b16702f2b1a17d2b1c3","observation_id":"2b9e7f0b-5d74-4802-a3bb-57aa4b749d03","resolution":{"observed_at":"2026-08-08T21:39:59.796691Z","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":"2026-08-08T21:39:59.800279Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.800279Z"},"links":{"citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:e12114e57fc15402065f9cb64ee735f858fafb3457f33de615da342c222d2437","observation_id":"dc4a443a-3408-4b47-b1ef-05a657e3ebca","resolution":{"observed_at":"2026-08-08T21:39:59.800279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.09686","last_updated":"2024-03-07T00:43:37Z","snapshot_observed_at":"2026-08-06T04:31:57.394851Z","submitted_at":"2024-02-15T03:43:20Z","title":"Lorentz violation induces isospectrality breaking in Einstein-Bumblebee gravity theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.09686","snapshot_observed_at":"2026-08-08T21:39:59.803567Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.803567Z"},"links":{"cited_paper":"/paper/2402.09686","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:a59bff5f9afa7e1ca08f2b6174563626a052cb17759969eebed512aa6fc4f247","observation_id":"e215eb26-c0d1-4389-9b55-1b734123f2b3","resolution":{"observed_at":"2026-08-08T21:39:59.803567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04805","last_updated":"2024-11-05T14:50:04Z","snapshot_observed_at":"2026-08-06T08:54:24.145914Z","submitted_at":"2024-09-07T12:08:17Z","title":"Neutron stars in the bumblebee theory of gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.04805","snapshot_observed_at":"2026-08-08T21:39:59.807074Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.807074Z"},"links":{"cited_paper":"/paper/2409.04805","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:9cff9066a9ccbb8820622063060327f7eb624b1677a4d53edeb4d6e4c998c1d9","observation_id":"b2428cfa-428c-45c2-b526-b6dc562fd072","resolution":{"observed_at":"2026-08-08T21:39:59.807074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0702006","last_updated":"2007-11-19T04:47:31Z","snapshot_observed_at":"2026-07-07T03:23:45.063198Z","submitted_at":"2007-02-01T12:12:13Z","title":"No hair theorems for positive \\Lambda","version":2},"cited_work":{"arxiv_id":"gr-qc/0702006","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0702006","snapshot_observed_at":"2026-08-08T21:40:00.302258Z","title":"No hair theorems for positive \\Lambda","venue":"gr-qc","work_id":"a3d35a96-e8bb-4c64-9fa9-b574fd0946d0","year":2007},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.810496Z"},"links":{"cited_paper":"/paper/gr-qc/0702006","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:db7dd17a71d34df7f54ee6eb1e6bfd8209fddd5f7612de5efabef52bcd03544b","observation_id":"13f8bb19-957b-4d22-b2f5-8e1e9174a30e","resolution":{"observed_at":"2026-08-08T21:40:00.305860Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.02687","last_updated":"2016-03-08T21:00:05Z","snapshot_observed_at":"2026-07-06T04:48:48.188054Z","submitted_at":"2016-03-08T21:00:05Z","title":"Kerr black holes with Proca hair","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.02687","snapshot_observed_at":"2026-08-08T21:39:59.813885Z","title":"Herdeiro, E","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.813885Z"},"links":{"cited_paper":"/paper/1603.02687","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:227053cc2c0899cb3fc5c7fc8f9b49a75ca7f9862075f53707bfdbbd1521a4f7","observation_id":"60082d39-ccf3-48ce-aa3d-492926c0ae5d","resolution":{"observed_at":"2026-08-08T21:39:59.813885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.01119","last_updated":"2017-09-19T15:58:38Z","snapshot_observed_at":"2026-08-01T16:27:31.663184Z","submitted_at":"2017-07-04T18:08:49Z","title":"Stability of Schwarzschild singularity in non-local gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.01119","snapshot_observed_at":"2026-08-08T21:39:59.817289Z","title":"Calcagni and L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.817289Z"},"links":{"cited_paper":"/paper/1707.01119","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:7d4a477d581d67bf0b34db1fd9115017bf9c53e4bf2a25b533d1be845002fb08","observation_id":"1236800b-492d-42c6-a721-76d1fe8d0946","resolution":{"observed_at":"2026-08-08T21:39:59.817289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.02943","last_updated":"2022-10-14T15:14:49Z","snapshot_observed_at":"2026-07-06T13:38:59.709514Z","submitted_at":"2022-08-05T00:45:17Z","title":"Generalized Regge-Wheeler Equation from Effective Field Theory of Black Hole Perturbations with a Timelike Scalar Profile","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.02943","snapshot_observed_at":"2026-08-08T21:39:59.820541Z","title":"Mukohyama, K","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.820541Z"},"links":{"cited_paper":"/paper/2208.02943","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:4691a3d7ad84176573aadd6b3150aec95f7078a176fbe859cf7ead77fc9ca618","observation_id":"a216c8d3-ef91-45ba-a518-aa693f1f2d05","resolution":{"observed_at":"2026-08-08T21:39:59.820541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.09160","last_updated":"2021-04-26T20:18:12Z","snapshot_observed_at":"2026-08-05T15:11:46.098201Z","submitted_at":"2021-02-18T05:06:24Z","title":"Gravitational perturbations in the Newman-Penrose formalism: Applications to wormholes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.09160","snapshot_observed_at":"2026-08-08T21:39:59.824098Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.824098Z"},"links":{"cited_paper":"/paper/2102.09160","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:ae2f33dce053ed451b538370204066b465b3b8703814f04c5d601fed12bf2906","observation_id":"e8be8413-5c5c-48bc-a60a-651388c8e27b","resolution":{"observed_at":"2026-08-08T21:39:59.824098Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.03028","last_updated":"2020-08-04T19:13:39Z","snapshot_observed_at":"2026-08-04T22:43:04.125047Z","submitted_at":"2020-05-06T18:00:01Z","title":"Accelerating black holes: quasinormal modes and late-time tails","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.03028","snapshot_observed_at":"2026-08-08T21:39:59.827588Z","title":"Destounis, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.827588Z"},"links":{"cited_paper":"/paper/2005.03028","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:7501c04bb47977b6c6e49eb11b2bece453e346311e2fc23fe6b30563a973f2c7","observation_id":"d321f1cb-149b-4df9-9eb2-87b66dcc8b6a","resolution":{"observed_at":"2026-08-08T21:39:59.827588Z","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":"th/0101160","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T21:40:00.237108Z","title":"Chakrabarti and D","venue":null,"work_id":"01fad826-dc79-4ebf-a80c-ec36550cfd41","year":2002},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.831002Z"},"links":{"citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:2bb79ea4a1ba37a8cf081539f7e40257504eb9e7352de0f41f85fc2496d6ecb2","observation_id":"03adb2f5-881a-4de1-8495-5c5d2ad7babe","resolution":{"observed_at":"2026-08-08T21:40:00.243499Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0307012","last_updated":"2020-03-06T14:37:50Z","snapshot_observed_at":"2026-07-07T03:18:04.960857Z","submitted_at":"2003-07-03T13:03:42Z","title":"Quasi-normal modes of Schwarzschild-de Sitter black holes","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0307012","snapshot_observed_at":"2026-08-08T21:39:59.834430Z","title":"Zhidenko, Quasinormal modes of Schwarzschild de Sitter black holes, Class","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.834430Z"},"links":{"cited_paper":"/paper/gr-qc/0307012","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:51060b4eeb9349a8436b30ca2e49ea0b0e22ccd69b9abb6ffbac86a85b937bdc","observation_id":"91020f1b-180d-4b2f-88b8-690c161d001f","resolution":{"observed_at":"2026-08-08T21:39:59.834430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0303052","last_updated":"2018-04-03T01:45:05Z","snapshot_observed_at":"2026-07-07T03:17:33.021224Z","submitted_at":"2003-03-12T17:16:55Z","title":"Quasinormal behavior of the D-dimensional Schwarzshild black hole and higher order WKB approach","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0303052","snapshot_observed_at":"2026-08-08T21:39:59.837815Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.837815Z"},"links":{"cited_paper":"/paper/gr-qc/0303052","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:a2aa15b96d7dd7c571934bec0f5151ea17002d2ebd46af2e7fb0f194e56ee80b","observation_id":"72731151-c479-4746-8e96-279ab7d1247d","resolution":{"observed_at":"2026-08-08T21:39:59.837815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.06439","last_updated":"2017-07-31T21:07:33Z","snapshot_observed_at":"2026-08-07T17:03:59.730340Z","submitted_at":"2017-03-19T14:05:55Z","title":"A Matrix Method for Quasinormal Modes: Kerr and Kerr-Sen Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.06439","snapshot_observed_at":"2026-08-08T21:39:59.841089Z","title":"Lin, W.-L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.841089Z"},"links":{"cited_paper":"/paper/1703.06439","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:5b5ba8e3dd5edf806abcee36a727b09199f9239c122ede18b6fbf928c6ec4931","observation_id":"d40eb39a-5393-4660-acb1-f932b2038277","resolution":{"observed_at":"2026-08-08T21:39:59.841089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0312079","last_updated":"2003-12-17T15:22:26Z","snapshot_observed_at":"2026-07-07T03:18:39.687978Z","submitted_at":"2003-12-17T15:22:26Z","title":"Dirac quasinormal modes of the Reissner-Nordstr\\\"om de Sitter black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0312079","snapshot_observed_at":"2026-08-08T21:39:59.844522Z","title":"Jing, Dirac quasinormal modes of the Reissner-Nordstrom de Sitter black hole, Phys","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.844522Z"},"links":{"cited_paper":"/paper/gr-qc/0312079","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:c5c7df61ba0c42cbb7fc35e61090187cda81b7743606989800f0644f199e3ded","observation_id":"dba793d4-8dd8-4f86-8e61-978fe4ecb006","resolution":{"observed_at":"2026-08-08T21:39:59.844522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.03599","last_updated":"2023-10-11T02:56:43Z","snapshot_observed_at":"2026-07-06T15:39:10.697564Z","submitted_at":"2023-06-06T11:40:39Z","title":"Gravito-electromagnetic perturbations of MOG black holes with a cosmological constant: Quasinormal modes and Ringdown waveforms","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.03599","snapshot_observed_at":"2026-08-08T21:39:59.847995Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.847995Z"},"links":{"cited_paper":"/paper/2306.03599","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:ec8dd7d06d3d5d8f3a2396697f3a0bd09adfa6ace22d7ab39134bf2bea239e8a","observation_id":"32584f60-8744-4cb6-9fb5-d6e0cff6a07a","resolution":{"observed_at":"2026-08-08T21:39:59.847995Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.00579","last_updated":"2024-07-18T11:43:28Z","snapshot_observed_at":"2026-07-06T18:23:52.659446Z","submitted_at":"2024-06-02T00:05:35Z","title":"Kerr-MOG-(A)dS black hole and its shadow in scalar-tensor-vector gravity theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.00579","snapshot_observed_at":"2026-08-08T21:39:59.851700Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.851700Z"},"links":{"cited_paper":"/paper/2406.00579","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:a1e8aa3b2eb9692572fed535a832b788d0e75b19afbc8b7540e6ecf52bd5a290","observation_id":"f649ac26-72ed-4e5c-81ab-5dfc00831d0c","resolution":{"observed_at":"2026-08-08T21:39:59.851700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06796","last_updated":"2022-07-14T10:21:38Z","snapshot_observed_at":"2026-07-06T13:31:13.285819Z","submitted_at":"2022-07-14T10:21:38Z","title":"Quasinormal modes and the correspondence with shadow in black holes with a deficit solid angle and quintessence-like matter","version":1},"cited_work":{"arxiv_id":"2207.06796","doi":null,"metadata_source":"pith","pith_arxiv_id":"2207.06796","snapshot_observed_at":"2026-08-08T21:40:00.030449Z","title":"Quasinormal modes and the correspondence with shadow in black holes with a deficit solid angle and quintessence-like matter","venue":"gr-qc","work_id":"6e363363-6b2e-4d22-89d2-f63c26c19760","year":2022},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.855062Z"},"links":{"cited_paper":"/paper/2207.06796","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:8ed7e06765de396492315e20b3184005c532eec326dba0b1edaedc6bbad1b75d","observation_id":"8af5f55a-3040-485e-bc2e-5a51d639eaab","resolution":{"observed_at":"2026-08-08T21:40:00.034738Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1610.08135","last_updated":"2017-04-01T18:07:34Z","snapshot_observed_at":"2026-08-05T12:23:07.789464Z","submitted_at":"2016-10-26T01:05:24Z","title":"A Matrix Method for Quasinormal Modes: Schwarzschild Black Holes in Asymptotically Flat and (Anti-) de Sitter Spacetimes","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.08135","snapshot_observed_at":"2026-08-08T21:39:59.858539Z","title":"Lin and W.-L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.858539Z"},"links":{"cited_paper":"/paper/1610.08135","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:be3baa122667f949605faeaf70c1fa8c32d442e134d06c1e34c5e8d250f0b85a","observation_id":"28a81bae-fbee-4f3a-9221-f5f8a16e1f1d","resolution":{"observed_at":"2026-08-08T21:39:59.858539Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.08352","last_updated":"2019-02-27T06:12:48Z","snapshot_observed_at":"2026-07-06T07:34:43.373594Z","submitted_at":"2019-02-22T03:23:30Z","title":"On matrix method for black hole quasinormal modes","version":2},"cited_work":{"arxiv_id":"1902.08352","doi":null,"metadata_source":"pith","pith_arxiv_id":"1902.08352","snapshot_observed_at":"2026-08-08T21:40:00.006106Z","title":"On matrix method for black hole quasinormal modes","venue":"gr-qc","work_id":"445831ce-3de4-47d4-b6cb-fadf0163bace","year":2019},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.861939Z"},"links":{"cited_paper":"/paper/1902.08352","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:5614ed618de667e4597c97b57ca841665cb30aba75bc8e47374c7ec7525f07e6","observation_id":"f07c3367-bbdf-41a5-acf0-43b6c5c3a315","resolution":{"observed_at":"2026-08-08T21:40:00.009992Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T21:40:01.358909Z","title":"Iyer and C","venue":null,"work_id":"a94bb02d-7af7-4f9f-8162-5b79e92fb7b4","year":1987},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.865261Z"},"links":{"citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:4b3ed791fdbd3fabad41d5ad03c143f52dbf1fca2433730a91406a5f603470be","observation_id":"ffcb2870-ba54-43a6-bdf3-75b38adb27d8","resolution":{"observed_at":"2026-08-08T21:40:01.362465Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0705.2880","last_updated":"2007-06-05T09:26:12Z","snapshot_observed_at":"2026-08-03T13:27:51.798429Z","submitted_at":"2007-05-20T17:56:25Z","title":"Instability of the massive Klein-Gordon field on the Kerr spacetime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.2880","snapshot_observed_at":"2026-08-08T21:39:59.868412Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.868412Z"},"links":{"cited_paper":"/paper/0705.2880","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:a1d937bd7092859196a74ebffcb3d3495ea30fe54b6b3b3da1b915b4fd4572d2","observation_id":"067a8fa6-5991-4818-8a52-d4a87d649e26","resolution":{"observed_at":"2026-08-08T21:39:59.868412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.15156","last_updated":"2024-07-02T14:30:17Z","snapshot_observed_at":"2026-07-06T17:21:05.809026Z","submitted_at":"2024-01-26T19:01:20Z","title":"Quasibound state reminiscent in de-Sitter black holes: Quasinormal modes and the decay of massive fields","version":2},"cited_work":{"arxiv_id":"2401.15156","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.15156","snapshot_observed_at":"2026-08-08T21:39:59.982457Z","title":"Quasibound state reminiscent in de-Sitter black holes: Quasinormal modes and the decay of massive fields","venue":"gr-qc","work_id":"c318aab1-0eae-4cf3-8561-4ad1080789bd","year":2024},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.871976Z"},"links":{"cited_paper":"/paper/2401.15156","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:f49a9735e1d559de13c5e987bf51a290b91b092c56a9f5d8cd6d4b7803bc9922","observation_id":"668e8be8-3f12-4913-8691-7793eb9ae20a","resolution":{"observed_at":"2026-08-08T21:39:59.986448Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.04306","last_updated":"2016-04-12T22:59:50Z","snapshot_observed_at":"2026-07-06T04:29:52.837324Z","submitted_at":"2015-09-14T20:30:10Z","title":"Quasinormal frequencies of self-dual black holes","version":2},"cited_work":{"arxiv_id":"1509.04306","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.04306","snapshot_observed_at":"2026-08-08T21:39:59.968267Z","title":"Quasinormal frequencies of self-dual black holes","venue":"gr-qc","work_id":"77fef7da-cced-45e7-9919-fe65ce5e90a0","year":2015},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.875262Z"},"links":{"cited_paper":"/paper/1509.04306","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:cc9ffc827d8959d45ab3826cb9960b993098d55909f8d943fae4dee817c5faa2","observation_id":"59da26c0-ac83-4d30-aa19-376bc73bd7d2","resolution":{"observed_at":"2026-08-08T21:39:59.972085Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.04634","last_updated":"2021-04-09T23:08:02Z","snapshot_observed_at":"2026-07-06T10:58:11.204048Z","submitted_at":"2021-04-09T23:08:02Z","title":"Test of Quantum Gravity in Statistical Mechanics","version":1},"cited_work":{"arxiv_id":"2104.04634","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.04634","snapshot_observed_at":"2026-08-08T21:39:59.954234Z","title":"Test of Quantum Gravity in Statistical Mechanics","venue":"gr-qc","work_id":"5ef340cb-20d4-4a9a-ab1c-2affc5815431","year":2021},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.879015Z"},"links":{"cited_paper":"/paper/2104.04634","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:2ef7fbfb00c843b21b85787475715dbc4dc77d0dd008d513fd00524b517fc44f","observation_id":"6c1c953e-a0ee-4784-aa17-f8ca7a24111a","resolution":{"observed_at":"2026-08-08T21:39:59.958029Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1010.2806","last_updated":"2010-10-21T17:55:50Z","snapshot_observed_at":"2026-07-06T02:17:38.020550Z","submitted_at":"2010-10-14T02:12:04Z","title":"Phase transitions and regions of stability in Reissner-Nordstr\\\"om holographic superconductors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.2806","snapshot_observed_at":"2026-08-08T21:39:59.882453Z","title":"Abdalla, C","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.882453Z"},"links":{"cited_paper":"/paper/1010.2806","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:7142545f1bb86f027be2e778736a7ffff64bf46a2e27e7db7a43d00b78d1d645","observation_id":"a078c7a1-6ace-4d85-95ef-7a175ee67e19","resolution":{"observed_at":"2026-08-08T21:39:59.882453Z","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":"2026-08-08T21:39:59.885821Z","title":"Zhu, S.-J","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.885821Z"},"links":{"cited_paper":"/paper/1405.4931","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:3116e07f346aa8aa2a6bcf6d3802467397d242a4dd4287c526fb8fe09146e934","observation_id":"ba7ccbff-b7ed-47da-b44c-35e9f01a9b19","resolution":{"observed_at":"2026-08-08T21:39:59.885821Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.09531","last_updated":"2023-09-01T14:28:35Z","snapshot_observed_at":"2026-07-06T13:02:06.316286Z","submitted_at":"2022-04-20T15:10:55Z","title":"Echoes of axial gravitational perturbations in stars of uniform density","version":4},"cited_work":{"arxiv_id":"2204.09531","doi":null,"metadata_source":"pith","pith_arxiv_id":"2204.09531","snapshot_observed_at":"2026-08-08T21:39:59.918958Z","title":"Echoes of axial gravitational perturbations in stars of uniform density","venue":"gr-qc","work_id":"1688af21-b388-4a6a-a797-5cbb3755f915","year":2022},"citing_paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-08T21:39:59.889352Z"},"links":{"cited_paper":"/paper/2204.09531","citing_paper":"/paper/2502.04782"},"observation_digest":"sha256:917128d9837e97cf06ee198ebf99d11f956f937b8ccf3613a59b81f25e7d787c","observation_id":"ca496941-c390-43aa-92eb-ee3821477479","resolution":{"observed_at":"2026-08-08T21:39:59.924456Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2502.04782","last_updated":"2025-04-06T03:57:30Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-08T21:45:20.941294Z","submitted_at":"2025-02-07T09:34:29Z","title":"Quasinormal Modes and Dynamical Evolution of Scalar Fields in the Einstein-Bumblebee Theory with a Cosmological Constant"},"reference_resolution":{"displayed":74,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":60,"verified_exact":12,"verified_fuzzy":2},"total_outbound_references":74},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 1 inbound Pith citation observation for arXiv:2502.04782."}