{"as_of":"2026-08-16T08:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:13e66a511bc787640f25ee8a7552cfd8c4353dd33be588510cab465ded077fde","coverage":[{"denominator":54,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":54,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T14:09:33.366409Z","state":"measured"},{"denominator":55,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":55,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-09T21:02:05.741128Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-11T14:46:55.110464Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"cited_work":{"arxiv_id":"2507.22945","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.22945","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Panotopoulos and F","venue":null,"work_id":"442a89a1-c627-42e7-bff6-7d2200098428","year":2025},"citing_paper":{"arxiv_id":"2605.00037","last_updated":"2026-04-28T09:28:44Z","snapshot_observed_at":"2026-08-10T22:24:35.307799Z","submitted_at":"2026-04-28T09:28:44Z","title":"Topology of black hole thermodynamics: A brief review","version":1},"reference_index":180,"source":"pdf_text","source_observed_at":"2026-05-09T21:02:05.741128Z"},"links":{"cited_paper":"/paper/2507.22945","citing_paper":"/paper/2605.00037"},"observation_digest":"sha256:95ae0572ce0afa8207a3ef76271690a0469cc3fd8dbf4c4901b6a9c06cddd3de","observation_id":"8928f566-25ec-40ba-bd74-1179410fa812","resolution":{"observed_at":"2026-05-11T14:46:55.223270Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.22945/citation-record","integrity":"/paper/2507.22945/integrity","json":"/paper/2507.22945/citation-record.json","paper":"/paper/2507.22945"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.181307Z","title":"Regge, J","venue":null,"work_id":null,"year":1957},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.181307Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:426cc87f0d2adccc34332962ba97aca7df890439e82f853315474016a05b42b8","observation_id":"4b1d5ab6-215c-471f-9a5a-fea8861509e1","resolution":{"observed_at":"2026-08-06T14:09:33.181307Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.184879Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.184879Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:855b063a24e2ba05826f2b70f58cad414c369bbe065bdad5c1ecff640c05729f","observation_id":"063f53bf-e26f-44bf-8d26-6d29cf6ad118","resolution":{"observed_at":"2026-08-06T14:09:33.184879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.188346Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.188346Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:c5fe9965492d25d80f70518ac78cb9eebb19e05adcd77c2e04c201b12edf0a19","observation_id":"3c1cac4e-cddf-490d-8649-04918ccff7c1","resolution":{"observed_at":"2026-08-06T14:09:33.188346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.191687Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.191687Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:d3c12c2fe6fe55dc6e2b593fba17901397fc1e7d72663ae83265ba4e317206b5","observation_id":"d5df3997-e946-4f5d-871b-cda1130a9ab6","resolution":{"observed_at":"2026-08-06T14:09:33.191687Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.195983Z","title":"Moncrief, Gauge-invariant perturbations of Reissner-Nordstrom black holes, Phys","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.195983Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:30f7f0a1d88652ed500f14acd92aa135ee92b9640c9f446e795f69c0d9a88c90","observation_id":"17419207-9fa6-41d7-80cc-ddc1d4cf7cb6","resolution":{"observed_at":"2026-08-06T14:09:33.195983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.199528Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.199528Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:adc495cb8e2114a821cfa0361ad2872fb27421cc75c983b4e79f40edad5aca54","observation_id":"ce413020-4615-4955-9640-09965e19854a","resolution":{"observed_at":"2026-08-06T14:09:33.199528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.980781Z","title":"Chandrasekhar, The mathematical theory of black holes, 1985","venue":null,"work_id":"d56156a5-9af7-470e-945f-40b018f65d2b","year":1985},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.203439Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:32aa8d82984f36181a8941ad3581ac19f1dd87713f5ef7d5a4eba54709bae90b","observation_id":"c1f828c2-4627-4ecd-82ba-f79971ad3e20","resolution":{"observed_at":"2026-08-06T14:09:33.984574Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0905.2975","last_updated":"2009-07-29T07:41:21Z","snapshot_observed_at":"2026-07-06T01:54:40.501878Z","submitted_at":"2009-05-19T05:15:43Z","title":"Quasinormal modes of black holes and black branes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.2975","snapshot_observed_at":"2026-08-06T14:09:33.206412Z","title":"Berti, V","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.206412Z"},"links":{"cited_paper":"/paper/0905.2975","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:5aec829526222d536556247fad0a5766ff683f4898fb1073d728a5449cef061c","observation_id":"b71b24bf-48ac-496a-969e-53e84a3557f8","resolution":{"observed_at":"2026-08-06T14:09:33.206412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.4014","last_updated":"2011-06-15T11:51:40Z","snapshot_observed_at":"2026-08-12T15:25:26.604164Z","submitted_at":"2011-02-19T18:38:22Z","title":"Quasinormal modes of black holes: from astrophysics to string theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.4014","snapshot_observed_at":"2026-08-06T14:09:33.210021Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.210021Z"},"links":{"cited_paper":"/paper/1102.4014","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:4e22e51a876a22a0056e39029414f923aeca1c411209f5236fd4b67a8a88bac9","observation_id":"b36f1c1e-49af-4525-8224-3f688c40b1d1","resolution":{"observed_at":"2026-08-06T14:09:33.210021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.213900Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.213900Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:c6b8b8b0586d3cae205c152bbd93a1c89c9b783982dba9cc4813979739330720","observation_id":"52dda078-f0b8-42b1-a852-1fc653925523","resolution":{"observed_at":"2026-08-06T14:09:33.213900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.216992Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.216992Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:24e04de883d72c4b8802940cf57886d1a5f60ac8c7464c51c795f14764334d75","observation_id":"6f86309e-785f-4c29-a783-80f77be68ca8","resolution":{"observed_at":"2026-08-06T14:09:33.216992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.220052Z","title":null,"venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.220052Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:7400f4603c87fce32e54600405f46a5e1e38b9bcaa31c0e3824450a1bd86ab3b","observation_id":"cc1551af-41eb-4b85-a34d-88946fbb8031","resolution":{"observed_at":"2026-08-06T14:09:33.220052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.223332Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.223332Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:37e15abb03a31bc71cf31adcb8d6b622c4e97458be66354800aa1db95275e6a0","observation_id":"caad9159-29f3-423e-b1ef-fa1c7e61630a","resolution":{"observed_at":"2026-08-06T14:09:33.223332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.226513Z","title":null,"venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.226513Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:92aa22bdc9228a1fa90606311d9ea88541ec67de186b60681bae1044b313d8f6","observation_id":"c127c1cb-7d93-47d9-b8b8-36055e4c24fb","resolution":{"observed_at":"2026-08-06T14:09:33.226513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9504004","last_updated":"1995-06-06T17:47:58Z","snapshot_observed_at":"2026-07-07T03:25:18.614600Z","submitted_at":"1995-04-04T18:54:14Z","title":"Thermodynamics of Spacetime: The Einstein Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9504004","snapshot_observed_at":"2026-08-06T14:09:33.230755Z","title":"Jacobson, Thermodynamics of space-time: The Einstein equation of state, Phys","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.230755Z"},"links":{"cited_paper":"/paper/gr-qc/9504004","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:46bf61f7bd4d88657480839eee73aa232a4a7d4dc0b99b2e86f268ee2e013cd1","observation_id":"7b133746-637a-4f12-97ea-e3a45806a6e2","resolution":{"observed_at":"2026-08-06T14:09:33.230755Z","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":"10.1103/physrevd.38.2434","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields","work_id":"6934dcf8-9361-4f2c-beef-cee144cdeb10","year":1988},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.234536Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:4dc2bbc091e335934775d162874493a1bbbcb6ea4fc18eb95b76b063307b4c3b","observation_id":"66486155-96f3-4ac3-b392-b8ae36eef59e","resolution":{"observed_at":"2026-08-06T14:09:33.423138Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.237707Z","title":"Lovelock, The Einstein tensor and its generalizations, J","venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.237707Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:eb753fea392fae14a4adc132fbd8585050652822b181730def946c364a721d41","observation_id":"53fede09-d9c2-44c9-aae5-a01d470312f7","resolution":{"observed_at":"2026-08-06T14:09:33.237707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.2765","last_updated":"2009-05-11T12:31:33Z","snapshot_observed_at":"2026-08-15T05:50:18.716804Z","submitted_at":"2009-04-17T19:07:41Z","title":"Enthalpy and the Mechanics of AdS Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.2765","snapshot_observed_at":"2026-08-06T14:09:33.241447Z","title":"Kastor, S","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.241447Z"},"links":{"cited_paper":"/paper/0904.2765","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:627fcc0b4e8bb4ce30fe3aaf6f562ad83347920af4e79baa629e289cd72bb20e","observation_id":"ced5a720-ea93-4aa0-ac1d-a98abe42dad4","resolution":{"observed_at":"2026-08-06T14:09:33.241447Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.2586","last_updated":"2014-01-12T02:45:03Z","snapshot_observed_at":"2026-08-14T23:48:47.914588Z","submitted_at":"2014-01-12T02:45:03Z","title":"Thermodynamics of rotating black holes and black rings: phase transitions and thermodynamic volume","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.2586","snapshot_observed_at":"2026-08-06T14:09:33.245098Z","title":"Altamirano, D","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.245098Z"},"links":{"cited_paper":"/paper/1401.2586","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:d224b86c3ff2e075fff3060ad0ba0a5214e4f3a7e14f121e17dc3dd3e223f21d","observation_id":"4b31a877-cf93-4c21-a81e-11e341726124","resolution":{"observed_at":"2026-08-06T14:09:33.245098Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.01706","last_updated":"2022-05-10T08:27:12Z","snapshot_observed_at":"2026-08-13T17:22:42.956890Z","submitted_at":"2021-12-03T04:30:42Z","title":"Topology of black hole thermodynamics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.01706","snapshot_observed_at":"2026-08-06T14:09:33.249152Z","title":"Wei, Y.-X","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.249152Z"},"links":{"cited_paper":"/paper/2112.01706","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:1c610829e346d537740052b18b53172c9975f86fdd93bbb5bc1ef200ee214067","observation_id":"0e103aed-f2c6-420b-acc8-9f215cfcc8fc","resolution":{"observed_at":"2026-08-06T14:09:33.249152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01932","last_updated":"2022-11-01T06:32:08Z","snapshot_observed_at":"2026-08-13T14:51:25.654750Z","submitted_at":"2022-08-03T09:18:58Z","title":"Black Hole Solutions as Topological Thermodynamic Defects","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01932","snapshot_observed_at":"2026-08-06T14:09:33.252621Z","title":"Wei, Y.-X","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.252621Z"},"links":{"cited_paper":"/paper/2208.01932","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:9eb2fb3ef289ed9cc5a034fc5a8b6b02f6b7dff815eb16990000a718b4b638bf","observation_id":"b33e705e-24ea-440c-85dd-9c77514b3a4d","resolution":{"observed_at":"2026-08-06T14:09:33.252621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12747","last_updated":"2024-11-27T12:42:43Z","snapshot_observed_at":"2026-08-12T22:41:44.158011Z","submitted_at":"2024-09-19T13:13:48Z","title":"Universal thermodynamic topological classes of rotating black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.12747","snapshot_observed_at":"2026-08-06T14:09:33.256018Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.256018Z"},"links":{"cited_paper":"/paper/2409.12747","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:3b00410f3b9e2cc432e72cdc3bccc52c52ba21cded5efe7fd01511323c2c1a55","observation_id":"29e38abe-f294-4c4e-9662-413c73327914","resolution":{"observed_at":"2026-08-06T14:09:33.256018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.00579","last_updated":"2024-07-18T11:43:28Z","snapshot_observed_at":"2026-08-14T10:14:18.501035Z","submitted_at":"2024-06-02T00:05:35Z","title":"Kerr-MOG-(A)dS black hole and its shadow in scalar-tensor-vector gravity theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.00579","snapshot_observed_at":"2026-08-06T14:09:33.259758Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.259758Z"},"links":{"cited_paper":"/paper/2406.00579","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:1fd4b5635771dd3c480b23c238f130832f95531e87f64a1654888671f5d3426a","observation_id":"ee23ac5c-4931-4a69-9c9a-dbfd245dffa6","resolution":{"observed_at":"2026-08-06T14:09:33.259758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13461","last_updated":"2024-08-21T11:02:40Z","snapshot_observed_at":"2026-08-12T23:39:17.638363Z","submitted_at":"2024-06-19T11:38:05Z","title":"Static neutral black holes in Kalb-Ramond gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13461","snapshot_observed_at":"2026-08-06T14:09:33.263109Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.263109Z"},"links":{"cited_paper":"/paper/2406.13461","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:f41eb84b5829815229a2f22df3bbe2c309a00d63748202f8e07a282704761db6","observation_id":"da0e49f4-211a-41e6-b44b-ab9731092910","resolution":{"observed_at":"2026-08-06T14:09:33.263109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.05569","last_updated":"2024-10-04T12:10:18Z","snapshot_observed_at":"2026-08-15T21:05:59.680108Z","submitted_at":"2024-08-10T14:44:21Z","title":"Light rings and shadows of static black holes in effective quantum gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.05569","snapshot_observed_at":"2026-08-06T14:09:33.266307Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.266307Z"},"links":{"cited_paper":"/paper/2408.05569","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:30ddbc36faf57d209554ae9d816cacddf3fe4a87d3298ded358da3353f9a10a2","observation_id":"5155572e-cbe9-4e68-a663-a03e771ab8f7","resolution":{"observed_at":"2026-08-06T14:09:33.266307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.20022","last_updated":"2024-11-25T12:16:38Z","snapshot_observed_at":"2026-08-12T23:54:13.346763Z","submitted_at":"2024-05-30T13:05:09Z","title":"Thermodynamic topology of topological black hole in $F(R)$-ModMax gravity's rainbow","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.20022","snapshot_observed_at":"2026-08-06T14:09:33.271166Z","title":"Eslam Panah, B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.271166Z"},"links":{"cited_paper":"/paper/2405.20022","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:b73ae9df28f41a7b3a23ebc64f19bb37a78d5b186a485d97e7d3f6cab1a22525","observation_id":"1d3236a3-2a6b-4adb-a89c-a1e3d8fe63ab","resolution":{"observed_at":"2026-08-06T14:09:33.271166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07522","last_updated":"2024-11-27T10:56:04Z","snapshot_observed_at":"2026-08-13T00:32:54.664949Z","submitted_at":"2024-04-11T07:29:43Z","title":"Thermodynamics of black holes featuring primary scalar hair","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07522","snapshot_observed_at":"2026-08-06T14:09:33.274608Z","title":"Bakopoulos, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.274608Z"},"links":{"cited_paper":"/paper/2404.07522","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:47d904badc8baa31999d254406ca8cee7848a0eddfd54456feecb2322b42bad8","observation_id":"74e30bbc-8083-43c5-a5a1-c0c5bcf3f024","resolution":{"observed_at":"2026-08-06T14:09:33.274608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.18791","last_updated":"2024-05-14T07:48:46Z","snapshot_observed_at":"2026-08-13T04:07:45.732179Z","submitted_at":"2024-02-29T01:39:32Z","title":"Topological interpretation of extremal and Davies-type phase transitions of black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.18791","snapshot_observed_at":"2026-08-06T14:09:33.278923Z","title":"Bhattacharya, K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.278923Z"},"links":{"cited_paper":"/paper/2402.18791","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:63ed539089aa5dadbf4749a468fb585cc676e9fcfa2f0a87338d33274a7737f2","observation_id":"73ceb26c-7163-474c-aa84-eba4e7c7c212","resolution":{"observed_at":"2026-08-06T14:09:33.278923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.02253","last_updated":"2023-02-28T16:55:27Z","snapshot_observed_at":"2026-08-13T14:12:40.586100Z","submitted_at":"2022-10-05T13:31:50Z","title":"Quantum Oppenheimer-Snyder and Swiss Cheese models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.02253","snapshot_observed_at":"2026-08-06T14:09:33.282588Z","title":"Lewandowski, Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.282588Z"},"links":{"cited_paper":"/paper/2210.02253","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:70bcbdb7e78c445d275e9f8673ef3250e8de811c4e63d6c20b5804e032bb48a2","observation_id":"18a5b64a-21c6-433c-9fa4-effedb8cd728","resolution":{"observed_at":"2026-08-06T14:09:33.282588Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04263","last_updated":"2023-07-19T14:25:29Z","snapshot_observed_at":"2026-08-15T21:07:05.883524Z","submitted_at":"2022-11-08T14:14:21Z","title":"Shadow and stability of quantum-corrected black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04263","snapshot_observed_at":"2026-08-06T14:09:33.285642Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.285642Z"},"links":{"cited_paper":"/paper/2211.04263","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:b44ad2bb979c53ae2590833d9786c502c3be85f6b72b0ef91f945173f9598bb1","observation_id":"d6ab7bda-4590-4ac5-acc7-99d553c8f8f9","resolution":{"observed_at":"2026-08-06T14:09:33.285642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04962","last_updated":"2025-03-12T09:10:07Z","snapshot_observed_at":"2026-08-13T10:17:14.214334Z","submitted_at":"2023-09-10T08:32:49Z","title":"Scalar fields around a loop quantum gravity black hole in de Sitter spacetime: Quasinormal modes, late-time tails and strong cosmic censorship","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04962","snapshot_observed_at":"2026-08-06T14:09:33.289171Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.289171Z"},"links":{"cited_paper":"/paper/2309.04962","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:d3899e77d0d3859b9655b96db81832e9d64b745e97ce1ec7fd2109e753db84b9","observation_id":"9865cc05-d5bd-47dd-9b68-55c060b2ce6e","resolution":{"observed_at":"2026-08-06T14:09:33.289171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13638","last_updated":"2024-05-30T03:17:02Z","snapshot_observed_at":"2026-08-13T04:13:53.311399Z","submitted_at":"2024-02-21T09:18:16Z","title":"Effective four-dimensional loop quantum black hole with a cosmological constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.13638","snapshot_observed_at":"2026-08-06T14:09:33.292567Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.292567Z"},"links":{"cited_paper":"/paper/2402.13638","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:572e95eaa2ab0ef394cdde65fcb45113772d4cabec7cd8f0b25c8a4675c86bdc","observation_id":"2a2a12ff-decd-48ed-a0ed-fa65b6a82f92","resolution":{"observed_at":"2026-08-06T14:09:33.292567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06390","last_updated":"2024-05-10T10:58:30Z","snapshot_observed_at":"2026-08-13T00:10:20.139674Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-06T14:09:33.295680Z","title":"Skvortsova, Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer–Snyder Model of Black Holes, Fortsch","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.295680Z"},"links":{"cited_paper":"/paper/2405.06390","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:08a3e6ef490487a98bf76fb58dffac6dc6a186b4fd498876082e057bb3007194","observation_id":"2fd02827-d5bf-4227-b7a7-3f3ff0411be2","resolution":{"observed_at":"2026-08-06T14:09:33.295680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.17639","last_updated":"2024-01-06T13:47:29Z","snapshot_observed_at":"2026-08-13T05:09:21.329499Z","submitted_at":"2023-12-29T15:04:43Z","title":"Quasinormal modes of quantum-corrected black holes","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.17639","snapshot_observed_at":"2026-08-06T14:09:33.299113Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.299113Z"},"links":{"cited_paper":"/paper/2312.17639","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:5860b21bf83899955c1e7e916ef8c0df94c47577f0415aa146bc4d986bd0a934","observation_id":"0d3b9a29-68e2-40e7-8bb9-0382f3819842","resolution":{"observed_at":"2026-08-06T14:09:33.299113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.18606","last_updated":"2024-11-04T08:37:35Z","snapshot_observed_at":"2026-08-13T00:43:48.615803Z","submitted_at":"2024-03-27T14:24:43Z","title":"The Lensing Effect of Quantum-Corrected Black Hole and Parameter Constraints from EHT Observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.18606","snapshot_observed_at":"2026-08-06T14:09:33.302900Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.302900Z"},"links":{"cited_paper":"/paper/2403.18606","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:21bd012e3922a4da68617ed573b82521e652ca5229515d805314f1d19cfc5720","observation_id":"b57412cd-d64c-444e-b4b3-db84bd14ec46","resolution":{"observed_at":"2026-08-06T14:09:33.302900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.992362Z","title":"regularized","venue":null,"work_id":"9ae4545a-7707-4632-8689-673a2b09d551","year":null},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.176464Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:19c88c14fdcb3c5c598f24793fcfeff1d4c688ecca6adf454b0c62834cee5544","observation_id":"af4fc73e-2e83-497d-aee0-ed4b7a0b70e2","resolution":{"observed_at":"2026-08-06T14:09:33.997434Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.17724","last_updated":"2024-01-27T01:45:42Z","snapshot_observed_at":"2026-08-13T04:52:11.864647Z","submitted_at":"2023-12-29T18:23:38Z","title":"Shadows and photon rings of a quantum black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.17724","snapshot_observed_at":"2026-08-06T14:09:33.306708Z","title":"Ye, Z.-Q","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.306708Z"},"links":{"cited_paper":"/paper/2312.17724","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:5c8a83fff00c6e2252c90afe161f78d45241b2bc43fbd864b3dfbffefa570f5d","observation_id":"7e4ce0e5-552d-482d-aa1e-ccfb2b319081","resolution":{"observed_at":"2026-08-06T14:09:33.306708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.08241","last_updated":"2024-11-23T09:21:28Z","snapshot_observed_at":"2026-08-13T20:43:51.184186Z","submitted_at":"2024-05-13T23:51:07Z","title":"Thermodynamics of AdS-Schwarzschild-like black hole in loop quantum gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.08241","snapshot_observed_at":"2026-08-06T14:09:33.310914Z","title":"Wang, S.-J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.310914Z"},"links":{"cited_paper":"/paper/2405.08241","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:076952e08129c963dbe4519757c6089e5a13be5a366896643f7cf822c7e03211","observation_id":"1d969e4e-c0b5-47e1-8ad6-8bbb4da0a07c","resolution":{"observed_at":"2026-08-06T14:09:33.310914Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2024.10153","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.736203Z","title":null,"venue":null,"work_id":"08743e77-1c81-480f-9618-7889485de3a2","year":2024},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.314668Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:9fc524e3f9080e795fa1dad6bda0a09bfe9c0e9b5bf638f9b0b84ab8e4bdba9e","observation_id":"7bd4693e-5b8c-49e4-9776-8303397b694f","resolution":{"observed_at":"2026-08-06T14:09:33.742772Z","resolver_source":"raw_fallback","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.317910Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.317910Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:38750e4fb293796958880a65c81a83c7cc466fffb52bd6ce37fc8d4c5409cb3c","observation_id":"b949565f-06a7-467c-880c-852de11ecde1","resolution":{"observed_at":"2026-08-06T14:09:33.317910Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0407051","last_updated":"2004-08-23T08:08:23Z","snapshot_observed_at":"2026-07-07T03:19:48.839643Z","submitted_at":"2004-07-14T18:52:16Z","title":"Black hole entropy from Quantum Geometry","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0407051","snapshot_observed_at":"2026-08-06T14:09:33.320920Z","title":"Domagala, J","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.320920Z"},"links":{"cited_paper":"/paper/gr-qc/0407051","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:b4e102907aa1da3fe2687b6642c7d48d8b1666c0d83f183cfe2bfd41a1bc7484","observation_id":"f32bfb42-87ad-4126-bdcf-39c9cde65ef7","resolution":{"observed_at":"2026-08-06T14:09:33.320920Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9410014","last_updated":"1994-10-11T21:45:45Z","snapshot_observed_at":"2026-08-15T06:15:45.755613Z","submitted_at":"1994-10-11T21:45:45Z","title":"Real Ashtekar Variables for Lorentzian Signature Space-times","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9410014","snapshot_observed_at":"2026-08-06T14:09:33.324963Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.324963Z"},"links":{"cited_paper":"/paper/gr-qc/9410014","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:ed39cd222432258ac2aaa3cbe28ee4b3b940c0e09e6e4deb8efef9201a294a46","observation_id":"5892cdde-3d50-422c-bba5-352e052ce864","resolution":{"observed_at":"2026-08-06T14:09:33.324963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.328501Z","title":null,"venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.328501Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:716c2b2db8cac2f5d8e9bc9c425e3111328d4976b7da954e282e371331c681e4","observation_id":"b4b86081-224b-4807-a888-9390f039d5e2","resolution":{"observed_at":"2026-08-06T14:09:33.328501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.969528Z","title":null,"venue":null,"work_id":"dae87d63-5723-4cbf-b249-3a7b3740ccae","year":1987},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.331475Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:47d28f69ee9a39acb1d6efd54ad02699de5f46e01d396e9a5e8470697978f445","observation_id":"dd6204ad-cc94-4a88-bcba-6d217d45dcb7","resolution":{"observed_at":"2026-08-06T14:09:33.973617Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0702015","last_updated":"2007-02-02T18:45:37Z","snapshot_observed_at":"2026-07-07T03:23:45.063198Z","submitted_at":"2007-02-02T18:45:37Z","title":"Orbital precession due to central-force perturbations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0702015","snapshot_observed_at":"2026-08-06T14:09:33.334443Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.334443Z"},"links":{"cited_paper":"/paper/gr-qc/0702015","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:c39f458b37dd4c883affe666f58684cc665ebcc69526a3ad5348179e653dafb9","observation_id":"87c172f4-27f9-4365-ab33-89a2f850bedc","resolution":{"observed_at":"2026-08-06T14:09:33.334443Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.05063","last_updated":"2018-08-15T13:12:42Z","snapshot_observed_at":"2026-08-14T18:40:53.974596Z","submitted_at":"2018-08-15T13:12:42Z","title":"Constraints on alternative theories of gravity with observations of the Galactic Center","version":1},"cited_work":{"arxiv_id":"1808.05063","doi":null,"metadata_source":"pith","pith_arxiv_id":"1808.05063","snapshot_observed_at":"2026-08-06T14:09:33.550533Z","title":"Constraints on alternative theories of gravity with observations of the Galactic Center","venue":"gr-qc","work_id":"3a1da595-4218-4288-af49-01e688648b17","year":2018},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.338256Z"},"links":{"cited_paper":"/paper/1808.05063","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:a0e320cb5c9322616ecf8b34405470277943a9896e88a7e0ba86cc6d34066d8d","observation_id":"a762c0a5-1ab7-4764-be41-7d7fd6b4e1ae","resolution":{"observed_at":"2026-08-06T14:09:33.555312Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.15017","last_updated":"2020-10-07T13:57:11Z","snapshot_observed_at":"2026-07-06T09:33:04.388569Z","submitted_at":"2020-06-26T14:39:05Z","title":"Observational Constraints on the Regularized 4D Einstein-Gauss-Bonnet Theory of Gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.15017","snapshot_observed_at":"2026-08-06T14:09:33.341594Z","title":"Clifton, P","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.341594Z"},"links":{"cited_paper":"/paper/2006.15017","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:c67427ce7169799360f9993e5a3a28ce7fbf7c00cc1f77a78cadf476d6c210b2","observation_id":"207ff7db-7301-448d-9df4-dd09542331f6","resolution":{"observed_at":"2026-08-06T14:09:33.341594Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.3043","last_updated":"2013-06-13T07:41:55Z","snapshot_observed_at":"2026-08-15T00:14:13.155007Z","submitted_at":"2013-06-13T07:41:55Z","title":"Relativistic effects and dark matter in the Solar system from observations of planets and spacecraft","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.3043","snapshot_observed_at":"2026-08-06T14:09:33.345588Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.345588Z"},"links":{"cited_paper":"/paper/1306.3043","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:37236c02a8fa8b954e2f98ff6c29a17adbff3cfff6a41ecd98ac283bb4ad5394","observation_id":"e0afe95d-4e04-4627-b73a-ae285c425f44","resolution":{"observed_at":"2026-08-06T14:09:33.345588Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0657","last_updated":"2008-01-11T14:09:17Z","snapshot_observed_at":"2026-08-15T10:32:56.829253Z","submitted_at":"2007-09-05T14:01:37Z","title":"Quasi-Normal Modes and Gravitational Wave Astronomy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.0657","snapshot_observed_at":"2026-08-06T14:09:33.349835Z","title":"Ferrari, L","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.349835Z"},"links":{"cited_paper":"/paper/0709.0657","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:19baa2bf0a34ebfe11266b6f1c91fb8ff665aaeef6a12ada49c03a6b0b73ee81","observation_id":"8e0d0f5a-7d30-4cbd-8003-c85eb7b68a89","resolution":{"observed_at":"2026-08-06T14:09:33.349835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.353106Z","title":null,"venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.353106Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:cbe821dc6b11b3051f9958439cea46a66497701ee4e6dc720d71c1c75631666e","observation_id":"5938a467-574b-4ef2-8cc1-f29fe953a97d","resolution":{"observed_at":"2026-08-06T14:09:33.353106Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.356628Z","title":null,"venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.356628Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:aa7fd9d3be8e07c39186e767f95e12560aef071a0ad5485afc37126eff2a9fb3","observation_id":"5d543050-8fd8-4079-89a1-d0f8826d92e1","resolution":{"observed_at":"2026-08-06T14:09:33.356628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.959839Z","title":"Duan, THE STRUCTURE OF THE TOPOLOGICAL CURRENT (3 1984)","venue":null,"work_id":"19d07128-9a5c-41ea-b9ec-85d148659cad","year":1984},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.359689Z"},"links":{"citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:6792ebc5b6afa9dbea5828ac68502fb6885c2bf17733b0cd37da8e2c65205fda","observation_id":"8adaebbc-faec-4b01-99e4-5bcb71c974dc","resolution":{"observed_at":"2026-08-06T14:09:33.963251Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","snapshot_observed_at":"2026-08-13T16:26:43.626121Z","submitted_at":"2022-03-09T17:21:15Z","title":"Bardeen-Kiselev black hole with cosmological constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.04965","snapshot_observed_at":"2026-08-06T14:09:33.362896Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.362896Z"},"links":{"cited_paper":"/paper/2203.04965","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:b343cb5c5545f1e91aae02a11393dd520667f105f01fae1b426df36d11f7ba2b","observation_id":"e529aa7d-74b9-4111-b9a4-eae855b72964","resolution":{"observed_at":"2026-08-06T14:09:33.362896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.11754","last_updated":"2020-04-03T05:51:01Z","snapshot_observed_at":"2026-08-08T15:56:48.445605Z","submitted_at":"2020-03-26T06:14:04Z","title":"Thermodynamics and P-v criticality of Bardeen-AdS Black Hole in 4-D Einstein-Gauss-Bonnet Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.11754","snapshot_observed_at":"2026-08-06T14:09:33.366409Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T14:09:33.366409Z"},"links":{"cited_paper":"/paper/2003.11754","citing_paper":"/paper/2507.22945"},"observation_digest":"sha256:37377f10e42cc44444ba35399cf5f92c83598f9cd4b0175b7b1c59e611fdd4d5","observation_id":"9c16a49f-f2f9-4f52-b0f8-ded088cfbddb","resolution":{"observed_at":"2026-08-06T14:09:33.366409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.22945","last_updated":"2025-07-26T13:09:50Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T00:41:40.791925Z","submitted_at":"2025-07-26T13:09:50Z","title":"Quantum Black Holes: Perihelion Advance, Quasi Normal Modes and Classical/ Topological Thermodynamics"},"reference_resolution":{"displayed":54,"state_counts":{"malformed_identifier":3,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":45,"verified_exact":2,"verified_fuzzy":3},"total_outbound_references":54},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 1 inbound Pith citation observation for arXiv:2507.22945."}