{"as_of":"2026-08-07T21:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:145e63de9af8bcc5ceec7790d3674786ec5589560cdfc7f88ec66f6e473d6701","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":"2026-08-07T06:34:17.273281+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":"2026-08-06T14:09:32.264748Z","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":"2026-08-02T23:35:30.562938Z","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":"sha256:1a055dd65646b90732b9a488625aa554c67b3b8e83f55f614c80a01ef5e6ba62","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/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":"2026-08-06T14:09:32.264748Z","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":"sha256:5eee25e7e0bebed067b14c042ed6e4478795e5afa833f0d2ebc30f02315294bc","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":"2026-08-06T14:09:32.264748Z","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:b08d520606d1968e784dd9bcbf7710a5cc09cb5eda5908ad9191ae24758563c8","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":"2026-08-06T14:09:32.264748Z","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:f445ba2e3ef80f7ebc0078e2c7591e70585a7424c2cfc0deaaf1b65ad593d905","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":"2026-08-06T14:09:32.264748Z","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":"sha256:9fb51c3c417c4e6e8632e54ecbd048b76a613d53483aa7a0df77ff359add9fca","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":"2026-08-06T14:09:32.264748Z","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":"sha256:73b31cf67d24402eddf696158e850d12e5ac545c8aaff7a8f27cfe10fc3a68f0","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":"2026-08-06T14:09:32.264748Z","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":"sha256:66c43fa43d9f09b8962c0ee55d2f2a567bbe5823bf824b8770180026d02f30eb","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":"2026-08-06T14:09:32.264748Z","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:eb0da4f158f4c61967daf102d6ba6095285ed0a9110f26b4877b009a3566b678","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"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":"2026-08-06T14:09:32.264748Z","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:ff3c5552419ea0a604d5e4676ae04074a76105d361eb2d94dd751b5a6ab0d5dc","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":"2026-07-06T02:23:46.264528Z","submitted_at":"2011-02-19T18:38:22Z","title":"Quasinormal modes of black holes: from astrophysics to string theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1102.4014","snapshot_observed_at":"2026-08-06T14:09:33.210021Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:06ad58147d1a42d10ca4f363813dd3407fb0f54aa4a65e2e4e14c9ba137108c2","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":"2026-08-06T14:09:32.264748Z","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":"sha256:5ab7b4a72326828fb411d299041322efde228c3ac5e0ba2c733b5cd9f457dc36","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":"2026-08-06T14:09:32.264748Z","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:a21a803c97857b0d1eecedb889c99cb30f43396de735d9207e34e37af213e9f0","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":"2026-08-06T14:09:32.264748Z","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":"sha256:3f44218766964bdc08cb573a694a361f31b8ee69ad565200a74bd2097686a781","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":"2026-08-06T14:09:32.264748Z","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:db494940b19ed17a3c78201e941459d04b7fd2c142fb56c760fb52bebc89b13a","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":"2026-08-06T14:09:32.264748Z","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":"sha256:56f9cecb213d405cff81dc35bb20774fec743a04276e1a1dc72b589413ba40d0","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":"2026-08-06T14:09:32.264748Z","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":"sha256:3e335d453e08717bb2e1d0dfcb3176509ca964246905a00df7d0b81efc4c7a88","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":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.418710Z","title":null,"venue":null,"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":"2026-08-06T14:09:32.264748Z","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":"sha256:5a10a1dd4609b87af139401d88994a2892a8e624f8272e83b87054e61df4bd8f","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.237707Z","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":"2026-08-06T14:09:32.264748Z","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:ca9300db1e3a75f9b761128ba0991c215578ffa35850524a6142afe44dffa18f","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":"2026-07-06T01:53:52.839980Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:5bc7d4c7b08ddf6ee431e375062c62d1974973c34017b385df1459f3ea89edfd","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":"2026-07-06T03:33:01.594705Z","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":"2026-08-06T14:09:32.264748Z","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:e6dd545a03b87cb7c95904fd4c6a93b2fd7a2e303e884514371f3fecb57bc5d2","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":"2026-07-06T12:14:56.180425Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:13415f064ba692a5b26195c293ce1c28a9363ba4967d5ab72c8139753496d824","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":"2026-07-06T13:38:17.696613Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:9d06180ba23b9d3a92db19a1406832dc07ae689e031efdf8ed0010f8914656b5","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":"2026-08-05T18:40:34.514087Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:0855c1561e58700eb7e8e7f3882655a46e8d690aef1c94b039d8b2057e28fc10","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":"2026-07-06T18:23:52.659446Z","submitted_at":"2024-06-02T00:05:35Z","title":"Kerr-MOG-(A)dS black hole and its shadow in scalar-tensor-vector gravity theory","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.00579","snapshot_observed_at":"2026-08-06T14:09:33.259758Z","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":"2026-08-06T14:09:32.264748Z","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:bd29e75a7bdcc6304cc4e37fc1258df335c4f40c99bf744d0d7e770323a1ca99","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":"2026-08-05T15:24:08.933708Z","submitted_at":"2024-06-19T11:38:05Z","title":"Static neutral black holes in Kalb-Ramond gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13461","snapshot_observed_at":"2026-08-06T14:09:33.263109Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:6d39a7d3babe6002f179a9d4ff32ee4630da1ae51bf8d51311a4ae1f8fbc5486","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":"2026-07-06T18:59:13.491643Z","submitted_at":"2024-08-10T14:44:21Z","title":"Light rings and shadows of static black holes in effective quantum gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.05569","snapshot_observed_at":"2026-08-06T14:09:33.266307Z","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":"2026-08-06T14:09:32.264748Z","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:cec3fed2d14354b8b30cab18fd417629ad6b199e69a21c651f40bfebf49a4073","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":"2026-08-07T04:03:40.186393Z","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":"2026-08-06T14:09:32.264748Z","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:f7a8b73931187fe2ede09ddd5057243b57f1f013a4524ff8feeced366b7d2532","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":"2026-08-02T23:05:23.520450Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:99ff6e417a1bb2480939d848a28ccbc970b9d5761e9f3ee243693dfa42718334","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":"2026-07-06T17:37:09.952632Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:8dd10620a8f5dc832a6ca37e2430d3906d45b7da66f61f2fc58c39f50da0cba3","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":"2026-07-06T13:59:57.800591Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:8e3555cea2dcee6b6baeb15835c2f5be16095f86b115767d9d2a29e013b1d449","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":"2026-07-06T14:15:44.460161Z","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":"2026-08-06T14:09:32.264748Z","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:ca57d1581ee019a065d21707ed8afb51e825a541454126957a5e715b29ded672","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":"2026-07-06T16:16:37.618798Z","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":"2026-08-06T14:09:32.264748Z","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:ff944160d35d15e552d874fa500f2e75ec51c218634c1413e75f49f5d0b71a83","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":"2026-07-06T17:33:17.224327Z","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":"2026-08-06T14:09:32.264748Z","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:d11caf40b18a363c7510f960c4ee6b060fc42d6b9787282d4733caabecc7d2fa","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":"2026-08-04T15:24:05.069161Z","submitted_at":"2024-05-10T10:58:30Z","title":"Quasinormal Frequencies of Fields with Various Spin in the Quantum Oppenheimer-Snyder Model of Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06390","snapshot_observed_at":"2026-08-06T14:09:33.295680Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:55450fdcbd8d8a978730156e311358ef9224fa9ffc40b240142bd22c84f04ab7","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":"2026-07-06T17:09:55.651197Z","submitted_at":"2023-12-29T15:04:43Z","title":"Quasinormal modes of quantum-corrected black holes","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.17639","snapshot_observed_at":"2026-08-06T14:09:33.299113Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:899c2b542f0d9d080d1d6de4bb58df3c7584aae9c262414ff03749ee8aca32df","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":"2026-07-06T17:51:56.621426Z","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":"2026-08-06T14:09:32.264748Z","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:c22580c5214c89e975b8ca654e5e735f97eae15edc8d113549af668787eba794","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":"2026-08-06T14:09:32.264748Z","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":"sha256:0d27a5af96b608d2cd3d04821152c89636b73580a59abdf7bf7fb614ec7315ae","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.17724","last_updated":"2024-01-27T01:45:42Z","snapshot_observed_at":"2026-07-06T17:09:59.848387Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:1aae68510fe27309aae89a5992ada31236b867f40fdc6e04e9c8711e0987df4e","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":"2026-07-06T18:13:55.543513Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:65f000fecd1053f21c3ec3d22825a22214bf09fe45a3df9dff91c419bd41bc61","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":"2026-08-06T14:09:32.264748Z","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":"sha256:45864e04ef2de42f4dba109dcffe20cc25d18e7f6e326e42f804000c25ac2541","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T14:09:33.317910Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:5a5c379a6fcf81ed7a584990fdbfc05c17f7ccc0b60963d37fb20a7ce0ae3e38","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":"2026-08-06T14:09:32.264748Z","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":"sha256:89f45feaa6842bf67cc8e5a1f3e315d78ae992741cfd68d10b48bbc97696c7b8","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":"2026-08-06T11:25:01.573019Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:7ca8164043b5b6ee74cf13cd0543e1aeb1b7796eaaa59a831e3247dd4f064af9","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":"2026-08-06T14:09:32.264748Z","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":"sha256:1cc9d0b9805c214157582725382f20c2e8f260902aa81032b36aac5c9018c46f","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":"2026-08-06T14:09:32.264748Z","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":"sha256:78c658c478deb5a26cc8a93015373963fb74c61d8c1d72315daad6b3121b3f1e","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/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":"2026-08-06T14:09:32.264748Z","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":"sha256:4d7307cc7b5f89989e872715dae7e916576ce206820262b56820f4a5e2c2f72b","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":"2026-08-05T22:57:19.100019Z","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":"2026-08-06T14:09:32.264748Z","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:ec0bcae1fd624bc2e79a0476e1dfa07abd654cb17d810516ec58dfd7516334fb","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"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":"2026-08-06T14:09:32.264748Z","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:e9e46600cbb29ebdb2494de0416c5d787dc3b2d7cd3ca9370e929e0b3da4f369","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":"2026-07-06T03:15:45.494656Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:131af6ec98b981bec825e4b4cfe989bd67ac93c33d3b4398f09e233ae82644d2","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":"2026-07-06T01:29:47.326036Z","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":"2026-08-06T14:09:32.264748Z","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":"sha256:0c0ca800105afd6153c4c1300b1f9c1a76d94e0397e6d6183c9c37761a1d67d2","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":"2026-08-06T14:09:32.264748Z","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":"sha256:2c8a2eecaeedde0c74024cde7ef0f35534ef456040d9000063358518198e18d2","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":"2026-08-06T14:09:32.264748Z","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":"sha256:5b050e18945576bf2f4cae6f111898c410b03f89460b7e15fe643dc058866361","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":"2026-08-06T14:09:32.264748Z","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":"sha256:2ccd09c2112f72d2a719fa50bae41158b74357eccd074d90780727028bd2e775","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 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04965","last_updated":"2022-04-25T22:30:40Z","snapshot_observed_at":"2026-07-06T12:46:08.838773Z","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":"2026-08-06T14:09:32.264748Z","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:dcb81fc7af9995a30f2a077309834bcf75112cb30ab36d1d7e2dc6739120b87e","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":"2026-07-06T09:07:26.866731Z","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":"2026-08-06T14:09:32.264748Z","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:a09ba86d253e66dd1074bf5cdd4be78debe4295077911f98049de1aeb1db0f85","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":"2026-08-06T14:09:32.264748Z","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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 1 inbound Pith citation observation for arXiv:2507.22945."}