{"as_of":"2026-08-09T20:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2fae894fd17f095ecbfefd5f7dcf7ec9347366e95116afc1c0305286d9e63359","coverage":[{"denominator":93,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":93,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T22:00:02.248516Z","state":"measured"},{"denominator":93,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":93,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2603.12919/citation-record","integrity":"/paper/2603.12919/integrity","json":"/paper/2603.12919/citation-record.json","paper":"/paper/2603.12919"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-14T22:00:02.248516Z","title":"The perturbative solution obtained in this work is valid in the regimeϵ≪1, for which the RG corrections represent a small deformation of the Schwarzschild-(A)dS spacetime","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:25fba7ea68f818c1d71a44608bd715d88491b4d7b54207276d16caf3d337aa34","observation_id":"ae3f5270-fb2b-4bde-b266-a05863f90ca4","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:1369d579cfc9f9ad912bae071fe1f1e1a31431545994e545dfd19331aa8d1f41","observation_id":"d724b95e-9696-4873-b4a5-0342f2e7e471","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:7eb09f55e538176b96921e9830ed92907310b6827ed2f689852a14caa66a6b50","observation_id":"06cc7a84-f340-4bf8-807b-e20448753cb2","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:b523709608e698531f1e1e48e78d03e614ae873cda9bab23de4775acdb7e350f","observation_id":"79004b7f-4bce-49b9-91f2-b35c9b7f5ad8","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Abbott et al.,GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c4bf79d889129962244b5854f35d4e8effdbf02dbb38f94864714b1ccc95a881","observation_id":"5893aefb-20f7-4c4a-8602-4102bc4c3ab2","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Abbott et al.,Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences, Astrophys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:84a2d5f61998adea87a7e6fe65d82ebf65196effe139e8da53902e3c87392492","observation_id":"5a8a0f79-24db-4cb7-b496-5d6ec83b1810","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:0fddcd3e92f16a2ac792a1f544206e4562024d838cef543c7ed74bda7da0f2fd","observation_id":"b1c0f00c-6425-4f00-9907-ecfa20ce4a10","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:fb4aa617fc3e8e33c02d4b207c4598aad368cbd86f0982cd0a02ab4737a8c134","observation_id":"41bc4560-985b-48a1-bc6a-ff7acf34e1ef","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:ff7d3f9f47b1e87da8c80ab1deabc6a1781c5cf11bd32a0aa62839c789f8fb29","observation_id":"8a2b604b-aa7b-483f-9ae4-dd5e08035c72","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c032f03a0c9ebf3ba40a073951d3ab3156e63cce3411859e5caed5beeb37708d","observation_id":"7bbedece-b40e-4612-924e-07e8150d6403","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c19c4df64e434121dc06e37eba921709a9dfb13680f2bc01055ae9bf9d4e3b66","observation_id":"aa64544c-8337-4226-a7cd-5c57ae7c1ead","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f913292599f349501a8fad0317389825bd7752b943a5c0bd2c9ced00eb6fcb3c","observation_id":"a938ee4c-433f-48df-b7f1-f3e9f336c4cc","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:734206775448246e630b1ccd7f8374f9098603fa2ad141ab52d1faa1a16f7e0e","observation_id":"b3e46303-5cd3-44aa-8d39-87116cdb80ba","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Perlmutter et al.,Measurements ofΩandΛfrom 42 High Redshift Supernovae, Astrophys","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:6a5eb0808fc7d343f07393bf360ad945b067990ed135d560764287a186a8f310","observation_id":"5cf8c6ee-c26e-47a9-8780-739c025bedab","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"P ´erez de los Heros,Status, Challenges and Directions in Indirect Dark Matter Searches, Symmetry12, 1648 (2020)","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:9c5a23f12cb6499a8545f0040553a2a850c907ea12a779e30157847464bf5e54","observation_id":"60e9b09b-cd5a-42c9-b984-93f91f1f44a4","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:98e085ee542a107aa015b3b82d39efa875ebe6170aec8f3e85cc116f35706165","observation_id":"4ea6a053-4343-4861-99f7-fa545c9f5b51","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Amelino-Camelia,Are we at the dawn of quantum gravity phenomenology?, Lect","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f8326b435404c31df0cddcb91f2a2923a314c4094ec418db58794c0f03910bcc","observation_id":"f9db2089-31e9-4e4c-bd73-55278d4249b4","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Gambini et al.,Fundamental decoherence from quantum gravity: A Pedagogical review, Gen","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:136823d11bb213b700e9f881b6c8cf10d0986ae77f826f79312ac77efcf6814c","observation_id":"ed3abdb9-a9fb-4132-9461-b854de4f8255","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"De et al.,Quantum gravity as an emergent phenomenon, Int","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:a896b4fb7a228fe4efc0ae4bcb16150dde0b38211c90b22ab3d57e202ea58dae","observation_id":"7e31a0fc-44a2-4288-8a58-9e1c36c3ebae","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Van Raamsdonk,Lectures on gravity and entanglement, Theor","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:faabe15c2050c265f94bd31a11cfda2566d82c07f2d8093f16126e2240660232","observation_id":"a3f73637-039d-44ec-8936-3b9c887861d6","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Loll,Quantum Gravity from Causal Dynamical Triangulations: A Review, Class","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:804f93e68cd7e3903368a34f60a723ac878bbc436c1510d3c6759532c3ec7766","observation_id":"515eee1f-ece1-435c-9e84-e5fcf1f6a65d","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Oppenheim,A postquantum theory of classical gravity?, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f420e986972dc7461d8ba4af7cb04bc91f9b64aec3a42395c2b906f3f837f90f","observation_id":"6f18b135-d720-4c39-b9f2-39381d643c9f","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Ashtekar and E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:136c1acbd2f166a071f933bd6af509bc075d9b4dff8bffe89ac7aafcb0a33aba","observation_id":"6b551ba7-a349-447f-a12e-04ce850f5fb5","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Rovelli,Loop quantum gravity, Living Rev","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:2df7a023325c7bd50c4d04daaa161735dbf6355cb45589f6614016df23a5721c","observation_id":"26b883a1-68d8-4206-b4fd-02edceb93b84","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4188","last_updated":"2011-02-01T06:21:25Z","snapshot_observed_at":"2026-07-06T02:05:53.255518Z","submitted_at":"2010-01-23T18:58:32Z","title":"Loop quantum gravity - a short review","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4188","snapshot_observed_at":"2026-07-14T22:00:02.248516Z","title":"Sahlmann,Loop Quantum Gravity - A Short Review, arXiv:1001.4188 [gr-qc]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"cited_paper":"/paper/1001.4188","citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:217c4d095fc2d589c037ca9585e6938553cd8741ca6d6ce327ab76f755af4aec","observation_id":"c61373a7-c852-42f7-a915-7d699b8b42b0","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Girelli, F","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:87652bc1fc2a4a67d8e0ae010a7f6dc3089d0949faaff8c02021a27bcddf3889","observation_id":"ca77d99e-3ae4-4cb1-b000-070087403c50","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:5f390fc5d329a5f89725fc1984aa89e2ef1cfb5f635f168cbe49e2b980a20ff1","observation_id":"76bced58-3b34-4298-a90a-72c64e9dc796","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:b2ed9c84fd702d0c0a7007849e0ae84a5aceacb03c27b641a94768f6e618fad3","observation_id":"3b573949-5576-41db-a4fd-0dcb3ab2f458","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:893bdaf2571083c9d6fea8f7e886bb170c9c61a6983356c513b2307fd3759685","observation_id":"2b63d33b-ace5-4e28-b3b1-aba0662c300d","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Maharana,Quantum gravity and string theory,18th Conference of the Indian Association for General Relativity and Gravitation, 155 (1996)","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:0d1e9019c6b52b4d11045df9456aae4ac34dc944ac46953549c901ec29dde433","observation_id":"30403a20-2875-435e-8d77-17659ce7cc72","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.3967","last_updated":"2012-06-07T17:17:49Z","snapshot_observed_at":"2026-08-04T12:12:21.793606Z","submitted_at":"2011-07-20T13:11:45Z","title":"An Introduction to String Theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.3967","snapshot_observed_at":"2026-07-14T22:00:02.248516Z","title":"Bedford,An Introduction to String Theory, arXiv:1107.3967 [hep-th]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"cited_paper":"/paper/1107.3967","citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:d8e4577e3058041a23e388760651c79bbaac1324122fce8bf2b24ef2a9bf9561","observation_id":"a1416630-0283-4535-9f94-5cdda1d72a37","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:db9231d4bcbd1307d46664e83a5baf1f18bee4c4273062a5c1bfff9206e092ca","observation_id":"48223f01-64c8-466c-ac08-56b319e0da5a","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9512024","last_updated":"1995-12-11T20:28:08Z","snapshot_observed_at":"2026-07-07T03:25:59.458096Z","submitted_at":"1995-12-11T20:28:08Z","title":"Introduction to the Effective Field Theory Description of Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9512024","snapshot_observed_at":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"cited_paper":"/paper/gr-qc/9512024","citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:b58127225a6a878a20d2b47eacb2ea1b829bec5c981565738c0e934e10f699bf","observation_id":"598326da-aef3-4273-85f3-d2444338b4b1","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Faller,Effective field theory of gravity: Leading quantum gravitational corrections to Newton’s and Coulomb’s law, Phys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:b7eec2d65a07352f4e767e1ac8f261dfd98b5b3ef872c518c5a6e5fc4101c07e","observation_id":"28cbf954-5210-4125-84e0-b4e94537385a","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:07dd152e464b57dd7af6e35e4c99bdb8dd684191ab97a83a41aae61d44dec8b0","observation_id":"d6686ec6-16b4-4d5f-97c5-a362a5fc9aef","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.12235","last_updated":"2021-12-22T21:40:57Z","snapshot_observed_at":"2026-07-06T12:21:45.521326Z","submitted_at":"2021-12-22T21:40:57Z","title":"Quantum Gravity at Low Energies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.12235","snapshot_observed_at":"2026-07-14T22:00:02.248516Z","title":"Wallace,Quantum Gravity at Low Energies, arXiv:2112.12235 [gr-qc]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"cited_paper":"/paper/2112.12235","citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:ceaca21bac3e304a277cd64947b3d7ce13006952df8eff2806e53ceebef54bc2","observation_id":"c8a7de0f-77df-43af-8465-3d3082562c65","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:e0d22dfd1906358757e93f9f7855b955456f24144c4a37be4f5239dcd51337f9","observation_id":"1f665306-867c-43c1-a097-6d25c26400b8","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Cardoso et al.,Black holes in an effective field theory extension of general relativity, Phys","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c8e2ae9330d2da81ec7d55e0ac547fa85b77de4d11ca98ed02affde5126c87ab","observation_id":"bc4420f1-ad12-4c37-b898-b2c633096bce","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Hollands, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:05598afa76219f36ffebc2ef0468b67a820d0d8ada5cf5e51d8cc1ac3bf8f98d","observation_id":"68c71443-7903-454f-94eb-3fb9b01a684d","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Bhattacharyya, P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:6e83e50cf07b93a864b2b5662af90d57497c4a549cbb5af7f7d4153a8bc05fa0","observation_id":"f7a8fc52-d724-4a85-932e-b6efecc9ae6e","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Bhattacharyya et al.,An entropy current and the second law in higher derivative theories of gravity, JHEP2021, 169 (2021)","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:81669bace1f9d68af6325e66c708aaaaba37961161751a0faccf1927c224947f","observation_id":"9b4c195a-8a1a-4a60-96c2-b53d1138bfc7","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Davies and H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:71861b9dc80f76120b8afce005bf73f32d85c300147d55b564163d4807e05d99","observation_id":"d8afd682-9d12-487f-b961-d33d3c37b739","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Bhattacharjee, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:1e4a4d48b9eb638fc206ce985fc182c0786ee51893b1c55a5e52b91891334197","observation_id":"4d1b6762-4c6c-4b39-a945-2afa31136a42","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Serra,Black Holes through the Lenses of Effective Field Theory, PhD thesis, Scuola Normale Superiore, Pisa, Italy (2023)","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:7e84d1c4441bb302b82f0215d7263d327967bc3182a8aca284b47b7710506578","observation_id":"fb6efac2-a520-44bd-bfa4-d9748b518987","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:a0c50dcf785e4ba13f359141b4180c1d47e8ddd77fe67c39d755e30be3c7f821","observation_id":"4ef52839-407a-4561-a61d-4b970a12d803","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Davies and H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:6476c8c236f059e82150f4cfd6a92b005a64925f834ba1620bfc46170cc276a5","observation_id":"99c12abf-e6ef-4032-9d43-6e9ecb94e92c","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Eichhorn,Asymptotically safe gravity, inProc","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:a96866b7f35c5618563e063ca0e09e5c7a81e84418e2a7102fdc3199d73377f5","observation_id":"beed6434-f8da-4a64-99e6-ad3cd92ab170","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Lambiase and F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:e64938d4be366f580c206d53ce187f0871f7171baf69d12d0bae7edd00375dc2","observation_id":"3dcf0d9a-f2bd-402c-89d0-29d4579ea76d","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Daas et al.,Asymptotically safe gravity with fermions, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:cea51b42f68de8773f83ab0287ecd26b11abf6cd79e702980df95d89a8c5c563","observation_id":"ab1aa336-b065-48a9-90dc-fbfce133b43c","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Niedermaier and M","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:8620a6a52448c15a9643efb062bdde73545e25d5c112d61b2e57e2ef2e9d5c6a","observation_id":"8d39d74c-45cd-45c6-a401-d176e74a7060","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Eichhorn and A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f52258d65fe504230f9d3e9748d41e032ac8627ee96fd5976ccdc9bf2be87942","observation_id":"85606b3f-540f-436c-a7b6-cdd4bb0fd041","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Cai and D","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:65a5529f9ef075e55d3ccfce703da576ee4f8a327bed033410fa2a8f5ec899d1","observation_id":"2a1756a1-10eb-4715-a9a1-8995f331d208","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Polonyi,Lectures on the functional renormalization group method, Open Phys.1, 1 (2003)","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f6167a4be4fc4c159cfcad7db88c069f4f80ae6c6b95ec00f219bf670705316c","observation_id":"2952ff3d-b5e9-4e83-a045-01db6b654fd9","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f118962f444c7d12b5c392acbe57a9c0024bcb930cd2f17d4a4d64e5e79520a7","observation_id":"edff5075-27dc-49e7-87fb-06cbdf1d105f","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Berges, N","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:03e6a74fe7c606071c8ada94cde7519a1783c80e6407cba402c0ba030747d816","observation_id":"d544e1f4-3068-4c60-87a7-9a918e86b682","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Reuter,Nonperturbative evolution equation for quantum gravity, Phys","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:13d66c4c725bf673894c3f641d0943bd92a4bf6c3ce3f09fd09609e33e32e973","observation_id":"deb7ca09-c3a9-4c85-9642-8e7d09263ac1","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Bonanno, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:eeb14514f870302039afe64758d9aabf98e7a3e73a8253b57110d2fafb0d6eac","observation_id":"0bfe9f59-2727-4826-b909-61846969f5e6","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Bonanno, K","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:10a71c5a92e04cb9a169fc0b6677d5f9536d017bf4608651f9791f63ebe86c2c","observation_id":"84f80a0d-7cac-4386-9489-febefdfc1ff4","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.05689","last_updated":"2025-05-28T21:22:04Z","snapshot_observed_at":"2026-08-09T13:26:42.241334Z","submitted_at":"2025-02-08T20:44:31Z","title":"Transition from Regular Black Holes to Wormholes in Covariant Effective Quantum Gravity: Scattering, Quasinormal Modes, and Hawking Radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.05689","snapshot_observed_at":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"cited_paper":"/paper/2502.05689","citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:ee3cb60ff9701f750939600ecafa8b123f1a19ac4ce235556ae516657151820e","observation_id":"b2a7cbd9-0b5d-49f7-946e-ab586641c4c9","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Guo et al.,Quasinormal modes of black holes with multiple photon spheres, JHEP2022, 60 (2022)","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:2bfea625fb8eadcafd07c52f4672d032dbd632a1be5e00155ed2050c1ed35706","observation_id":"a6004265-9ffc-47b5-8cbc-4f55530efb62","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:57fbe8e9fbbd5ce8427c584efc748aa680e63fd47c90c5e4f0e3bb191bf4c35d","observation_id":"d6b93c1d-4383-4388-9ccc-724214c0f1a3","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Chen and J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:5c6e0585c36f02ccb1c809f3bbd7006f0ed2fcf73f4b05aca25fb63d714e3036","observation_id":"cb51917e-ebba-4620-a8f9-7c7f73115a63","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:1fcf8dda78d3bad1131b9fafec4b6de178ac75dc8e0fb03f6e39f649a5c545a7","observation_id":"523c0689-c246-466b-8733-1ce8cdc54956","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Hazarika and P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c278237635682be4af5b66476ea90cbe7a4bb843177ae5e7abbe4b1ad6364b6e","observation_id":"9460ec21-8da7-4dd1-b90c-8d45f182b607","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:1b50160ae0c93c10b144a9c5a4bcf9d3d9e886155398475cc33ce8cf72506fc1","observation_id":"1a3a094f-5f42-4e50-83e8-beae44d1b0df","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:b74d83107812684a5537c76935e2421a3d534939bce2f1491047d5085b5bfd28","observation_id":"2f78a696-e5ef-4630-ae27-7bd121c819af","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:de21e9bde929262bb1fa5784c282acd24e9a0d205c85033764a52a947addf903","observation_id":"09d68c90-a74a-420f-a2cb-0bf639e130eb","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:75d83505ddf7585d1b2d1bb278bbc76f9af84dd7349e22289e713a17df8c4f3f","observation_id":"0fbe73d5-e635-4cc7-bf9c-79a6dd548ec0","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c8a7937bd3b9008fb0fd1eaa58bd1c1370b970d391a1a34a291d7a269eeb466c","observation_id":"679e7cac-f8e6-4538-905a-f701d9b4805c","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:282052a97bcef1c3c1fe595d94e2589553fc108f22ca5b9c32a9f4ba9832f30a","observation_id":"7d8934e1-3ac0-4594-bedf-432e338b412c","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Hosseinifar et al.,Quasinormal Modes and Topological Characteristics of a Schwarzschild Black Hole Surrounded by the Dehnen Type Dark Matter Halo, arXiv:2503.03260 [gr-qc] (2025)","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:771de239c4d143104d267dffe6af3f26eedf1cff219c474138e08f9de3251812","observation_id":"9cca6242-9d18-4d64-8636-0e625d3eb100","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:eb520824132a9b018b9c9453d5d6d35e7f5ca5c52ac05f523c6c42390f5977f0","observation_id":"594072b0-793c-425e-b01f-1266a833811a","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Karmakar and U","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:7d93fd1f6bc982a27ef168390330cc2864d8e91155c22759822743494f88d815","observation_id":"a7359d67-873c-48fc-b836-ad62758a406a","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Mohan, R","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:359038fae75c4843359ca738f8ee3674ec93727212c2ef7f75409fbf0209bc7e","observation_id":"252ebf13-545c-4cf4-ba17-bd08deb64d62","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:3da14c94567a1fb97c983289dde7497da5596aa6b4bb5f34088278123376620e","observation_id":"fca9fa6a-2228-449b-9405-5932c50dd955","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Franciolini et al.,Effective Field Theory of Black Hole Quasinormal Modes in Scalar-Tensor Theories, JHEP2, 127 (2019)","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:15b8d0a027e766c6f49cb4ae4db72415b567b93f5f00725e5e2e1904eebf3247","observation_id":"7f9ae05b-21fe-40a6-82d0-7f99a1c9c6e4","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:dbd3e48766c0e88764bfe1bd016105ce844c4813ccc28cf013ae6084897a1721","observation_id":"92877e6c-c438-494f-9f1f-57f9fe03a568","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Ishibashi, N","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:58c7a157d810649c6e849274395399e301ab51eb770b35e7ac23d51861b8d357","observation_id":"e91e85b6-aea4-4da5-b15b-ded1f32178a1","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:3fa0105448bf0985ddd66d4efbc602e2eb43bd9fb5e7866acee0554a90918354","observation_id":"11496210-b756-49be-bd52-19b24afaa16b","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:ef4a8227556dcfa10636ed1e4067f278959b887071705f4cffa0ba6a37f0eab2","observation_id":"809f36da-4795-45af-8976-1e4423d3503b","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"de Lima and D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f2c0b821fd9f950388d537dfda99934ac4a7af9f6b86ee142eec7930555d6ab7","observation_id":"45786aea-03a7-48a0-aa47-db2ccc2e0bac","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Podolsky,The structure of the extreme Schwarzschild–de Sitter space-time, Gen","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:0864acb0b88d19cdd8d243fbfa4cb676ab67feabef1cc3977b0e24fdbf8f0061","observation_id":"76fde056-feaa-4b8f-86bf-199248168bf7","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Lin and C","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c243cd90cdfa50f3d9a4c9aa052daa36b99620030106405807602d58dc8855b0","observation_id":"1eab58b1-1a83-4c6a-936f-ce84decc4038","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Berti, V","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:ef30b127775dd6ee97061b8fcc9eeb6b866b270d7374368f1f24d2ec8f0fd3f0","observation_id":"e9870244-da42-4d86-9a0d-824e6485b35d","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:e0dc41a5ae52617edf46ce0e5b7d65ff65600116286744547c34b9f200590d90","observation_id":"773a0047-95fb-4b67-bc89-b36d671c28ce","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:57175f1c7b6b651dc2cb66c11dc58d76f008bcbb0206aec861241c67c78ea28c","observation_id":"481f41dc-cb54-4c43-b740-d04fe9a288e0","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:e3465bbe70f4cff8b244d26b753e2c0ddd302873f1cac04d2a5f471a953d3f65","observation_id":"57d7ad5a-2dd8-4e87-a0ea-b85917dcad1e","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Nollert,Quasinormal modes: the characteristic ‘sound’ of black holes and neutron stars, Class","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:7da3876dbfbe24d73d9090236f31629aa6e88f7e51f061ae8b44c1894bc7b040","observation_id":"fb4ff861-435b-4f81-8b0b-ead0fa4d9d22","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:4d51bce9201500dd8d8b7b918c8609619c26baf9da3df911f054773ff1b91785","observation_id":"76e01dd3-497e-4e44-8e26-e7598af4d57b","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Gundlach, R","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:6476f03ff6c780b387647d29c2fca152ff563d1a6a9bc2900d5e7325ffdbbbd1","observation_id":"9562546c-6fcb-4318-9d87-f2f8c809f81c","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Hua and T","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:c272d04a2341ab9ab0beeb5bc127d83e8b80e685ae07267b5af4fb920f30bc35","observation_id":"099e5b79-65dd-4784-8941-04f2640b8e80","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f033c4bc361adb63ef5e14514eb78eac90fb1a715359417d8ea5228e27ece223","observation_id":"19411326-9dda-48d3-ab16-f54d06dd4647","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","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":"2026-07-14T22:00:02.248516Z","title":"Berti et al.,Mining information from binary black hole mergers: A comparison of estimation methods for complex exponentials in noise, Phys","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-07-14T22:00:02.248516Z"},"links":{"citing_paper":"/paper/2603.12919"},"observation_digest":"sha256:f640f99a78c00746baf3a4865d7e44d1b998f3fe0e964575463610d4dc1e0557","observation_id":"1e3b58ef-4c8f-40a4-86f1-f7b381bec833","resolution":{"observed_at":"2026-07-14T22:00:02.248516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2603.12919","last_updated":"2026-06-28T13:15:59Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-09T13:27:22.233220Z","submitted_at":"2026-03-13T11:48:53Z","title":"Perturbative Renormalisation Group Improved Black Hole Solution and its Quasinormal Modes"},"reference_resolution":{"displayed":93,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":93,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":93},"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 93 of 93 outbound references and 0 inbound Pith citation observations for arXiv:2603.12919."}