{"as_of":"2026-08-09T18:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:25a462df87d08011690864e919b5acfbc09b475eceb1cce69a6aeb5a63f44d9d","coverage":[{"denominator":36,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":36,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:30:42.849490Z","state":"measured"},{"denominator":36,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":36,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.00109/citation-record","integrity":"/paper/2507.00109/integrity","json":"/paper/2507.00109/citation-record.json","paper":"/paper/2507.00109"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:46.327222Z","title":"Similar results have been found for the classical Reissner-Nordstr¨ om [5] and Einstein-Yang-Mills [6] black holes","venue":null,"work_id":"e2d8d007-b2c7-4961-bf96-4ff98eb86ba5","year":null},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:40.568562Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:c9ae467b7e9d2ffe0d96885dd1da5bc2a03576b097cf4772c43055ae5254f8af","observation_id":"8414e7fd-b39f-4eda-8678-0f1ee3d36cf6","resolution":{"observed_at":"2026-08-06T21:30:46.419888Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:46.117380Z","title":"In each row, the value of σ(u, vi) is chosen such that the maximal value of σ on the row is equal to zero","venue":null,"work_id":"bc7c6dc8-fd26-422c-a139-d3f25790fe97","year":null},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:40.676755Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:8dcd5f8bdb1b281237f806de0fe30f2e2173d36ddd96b1b2ad8617577a84aaec","observation_id":"d657a63e-59fb-43a5-8324-74517ba98f7b","resolution":{"observed_at":"2026-08-06T21:30:46.215474Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.10390","last_updated":"2018-01-05T08:32:40Z","snapshot_observed_at":"2026-08-04T21:46:43.824799Z","submitted_at":"2017-10-28T05:15:03Z","title":"Static Black Hole and Vacuum Energy: Thin Shell and Incompressible Fluid","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.10390","snapshot_observed_at":"2026-08-06T21:30:40.993055Z","title":"Ho and Y","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:40.993055Z"},"links":{"cited_paper":"/paper/1710.10390","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:7a405afaaff4764182a4da39f984486b9c655cebc8aa3729989640727b94807c","observation_id":"9a9380f1-1873-423d-8163-0fe84e2bfde4","resolution":{"observed_at":"2026-08-06T21:30:40.993055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0512167","last_updated":"2006-05-23T17:49:55Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2005-12-14T18:08:16Z","title":"Semiclassical zero-temperature corrections to Schwarzschild spacetime and holography","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0512167","snapshot_observed_at":"2026-08-06T21:30:40.816637Z","title":"Fabbri, S","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:40.816637Z"},"links":{"cited_paper":"/paper/hep-th/0512167","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:a1e54f950c2570abf65564400fc59ee6d973eb2e7d94b6085979dc9d25919572","observation_id":"f6049c53-c198-47da-ab77-66d2165e37e1","resolution":{"observed_at":"2026-08-06T21:30:40.816637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.08662","last_updated":"2017-12-27T02:10:20Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2017-03-25T08:00:26Z","title":"Static Black Holes With Back Reaction From Vacuum Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.08662","snapshot_observed_at":"2026-08-06T21:30:40.906064Z","title":"Ho and Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:40.906064Z"},"links":{"cited_paper":"/paper/1703.08662","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:7034a828e080a40af88312e7d55e601e2b4464086da3d6cccbdb489a1ffa338c","observation_id":"91ff4994-0006-4bb9-b8a1-4369b36106a9","resolution":{"observed_at":"2026-08-06T21:30:40.906064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.08278","last_updated":"2025-02-12T10:35:35Z","snapshot_observed_at":"2026-08-09T00:40:52.810200Z","submitted_at":"2025-02-12T10:35:35Z","title":"Quantum corrected Einstein-Yang-Mills black holes in semiclassical gravity","version":1},"cited_work":{"arxiv_id":"2502.08278","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.08278","snapshot_observed_at":"2026-08-06T21:30:43.896235Z","title":"Quantum corrected Einstein-Yang-Mills black holes in semiclassical gravity","venue":"gr-qc","work_id":"9addfe5c-fc63-452f-971d-71394e0ee0bc","year":2025},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.143058Z"},"links":{"cited_paper":"/paper/2502.08278","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:f9c48851612cdd6715603f5ce037d5a5788344067249200598060c5edbdf52e4","observation_id":"0323c54e-98fd-437c-b16b-b819e9164776","resolution":{"observed_at":"2026-08-06T21:30:43.978557Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.03213","last_updated":"2020-05-06T23:11:04Z","snapshot_observed_at":"2026-08-04T08:22:52.650499Z","submitted_at":"2019-11-08T12:23:27Z","title":"Schwarzschild geometry counterpart in semiclassical gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.03213","snapshot_observed_at":"2026-08-06T21:30:41.039318Z","title":"Arrechea, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.039318Z"},"links":{"cited_paper":"/paper/1911.03213","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:e29000c47753d00b8ab1581489d241c57913d21abc88b45ad86fbd0bb15a69b6","observation_id":"f6a5eb0a-2166-4f3d-bf2b-33473cc94ddf","resolution":{"observed_at":"2026-08-06T21:30:41.039318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.03544","last_updated":"2021-02-06T09:30:18Z","snapshot_observed_at":"2026-08-09T00:40:58.020210Z","submitted_at":"2021-02-06T09:30:18Z","title":"Reissner-Nordstr\\\"om geometry counterpart in semiclassical gravity","version":1},"cited_work":{"arxiv_id":"2102.03544","doi":null,"metadata_source":"pith","pith_arxiv_id":"2102.03544","snapshot_observed_at":"2026-08-06T21:30:44.047445Z","title":"Reissner-Nordstr\\\"om geometry counterpart in semiclassical gravity","venue":"gr-qc","work_id":"70fc0bff-22d3-4bd5-b1ba-a40fb9ec4936","year":2021},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.101109Z"},"links":{"cited_paper":"/paper/2102.03544","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:0bd1dc1217213e36ff80861b81921ac96bf8697fddfabcdbd8f3bd4155b0f8bf","observation_id":"ca73e3c8-aa30-4363-9687-80827447dfc5","resolution":{"observed_at":"2026-08-06T21:30:44.133890Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:45.571113Z","title":null,"venue":null,"work_id":"7380135d-27b2-421f-a5b4-f6579b75c34b","year":1976},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.314980Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:35cfdefe2b8d2ef9fd9314b37012ca813bf57cd2246ab5d5ffe9de3adf24f736","observation_id":"9627dad8-0034-4011-98f2-eb0831fc024f","resolution":{"observed_at":"2026-08-06T21:30:45.631778Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1712.09914","last_updated":"2018-09-14T07:39:54Z","snapshot_observed_at":"2026-07-06T06:16:23.065777Z","submitted_at":"2017-12-28T16:16:29Z","title":"The quantum fate of black hole horizons","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.09914","snapshot_observed_at":"2026-08-06T21:30:41.194674Z","title":"Berthiere, D","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.194674Z"},"links":{"cited_paper":"/paper/1712.09914","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:2429cff2d5531524836b372a6d6c0c0981285cf9cf4dcb8ecdea0b863b3291e5","observation_id":"72c78086-aa89-4338-b2df-37efe2409805","resolution":{"observed_at":"2026-08-06T21:30:41.194674Z","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":"2026-08-06T21:30:45.714225Z","title":null,"venue":null,"work_id":"41c53dc8-951c-4338-810e-17242190d619","year":1984},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.249280Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:021d79b85fb460f082e254e03e038f1667fa397e1cc357f410e9c8f34d8f6114","observation_id":"1a69a1a6-beb9-4c4f-a58a-14da7c3a62ad","resolution":{"observed_at":"2026-08-06T21:30:45.828178Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9405007","last_updated":"1994-05-05T07:09:08Z","snapshot_observed_at":"2026-07-07T05:05:27.420965Z","submitted_at":"1994-05-02T14:28:01Z","title":"The Internal Geometry of an Evaporating Black Hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9405007","snapshot_observed_at":"2026-08-06T21:30:41.481345Z","title":"Parentani and T","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.481345Z"},"links":{"cited_paper":"/paper/hep-th/9405007","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:1f0cb05e0da10cb3b4b42da4cf89f8488b7345732a05d2b6cc46d0066678d988","observation_id":"b9259ed4-4384-4d16-bd48-0e10dbb69d11","resolution":{"observed_at":"2026-08-06T21:30:41.481345Z","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":"2026-08-06T21:30:45.359994Z","title":"Davies and S","venue":null,"work_id":"abff337e-4dac-4afb-bf5f-b051efd298bd","year":1977},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.351530Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:dc5b09e844c6039ce9ce2284b23c49923086cfdcc6ae04f009eadc6fa4cc2bb8","observation_id":"d4986dcf-d4c9-4ae6-a0c9-57520e1de4ab","resolution":{"observed_at":"2026-08-06T21:30:45.429944Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:45.218821Z","title":null,"venue":null,"work_id":"77b4e1e5-0312-4cb7-9caf-8f378a471d8f","year":1981},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.410795Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:9fe9af6bb2d60c18a56877ee357c440bec2625a0db78690cb04ce84e4f5babf8","observation_id":"bec8da82-6931-4c90-bae9-b6e91686eab9","resolution":{"observed_at":"2026-08-06T21:30:45.282175Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0808.1709","last_updated":"2010-01-30T17:10:05Z","snapshot_observed_at":"2026-07-06T01:41:39.174242Z","submitted_at":"2008-08-12T19:44:17Z","title":"The causal structure of dynamical charged black holes","version":3},"cited_work":{"arxiv_id":"0808.1709","doi":null,"metadata_source":"pith","pith_arxiv_id":"0808.1709","snapshot_observed_at":"2026-08-06T21:30:43.703472Z","title":"The causal structure of dynamical charged black holes","venue":"gr-qc","work_id":"a6707372-6bce-482e-b548-9acbf4870cd4","year":2008},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.658358Z"},"links":{"cited_paper":"/paper/0808.1709","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:f114cff7d35563b3815dc1c2c0f172d000b0f351214cbd8877037d98f22de5dd","observation_id":"2cfec9fc-0e86-408d-bdaa-ecbe0947410f","resolution":{"observed_at":"2026-08-06T21:30:43.783362Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9704027","last_updated":"1997-04-09T07:32:33Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1997-04-09T07:32:33Z","title":"Spherical Collapse of a Mass-Less Scalar Field With Semi-Classical Corrections","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9704027","snapshot_observed_at":"2026-08-06T21:30:41.529851Z","title":"Ayal and T","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.529851Z"},"links":{"cited_paper":"/paper/gr-qc/9704027","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:5e9279d9c35d76e1fd507446afd44a888cd71bf1615a7ab04ae46759a5aa1a50","observation_id":"9a656a13-8b7e-439e-a1b7-cd14819f6204","resolution":{"observed_at":"2026-08-06T21:30:41.529851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0103090","last_updated":"2001-03-25T08:02:15Z","snapshot_observed_at":"2026-08-01T20:09:56.702191Z","submitted_at":"2001-03-25T08:02:15Z","title":"Formation and Evaporation of Charged Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0103090","snapshot_observed_at":"2026-08-06T21:30:41.604423Z","title":"Sorkin and T","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.604423Z"},"links":{"cited_paper":"/paper/gr-qc/0103090","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:1549bcde2dcc138f40faab247b726a1bf82e2bf7622a525c63e717479c7b3e21","observation_id":"4d1b5fd1-cd24-4f35-86ac-b6b8df9c7ba8","resolution":{"observed_at":"2026-08-06T21:30:41.604423Z","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":"2026-08-06T21:30:44.879955Z","title":null,"venue":null,"work_id":"6c83b4f0-77d1-41e5-bd9e-035efd0910ab","year":1973},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.848918Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:4813235e27582110aefded03cc910b2c49bebf8b9a2776ac53a0f74a775e74aa","observation_id":"eb5c66a3-9f39-4e9a-b0f1-def297563ee1","resolution":{"observed_at":"2026-08-06T21:30:44.958073Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1010.2585","last_updated":"2011-10-14T20:00:38Z","snapshot_observed_at":"2026-07-06T02:17:31.240546Z","submitted_at":"2010-10-13T07:23:32Z","title":"Internal structure of charged black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.2585","snapshot_observed_at":"2026-08-06T21:30:41.737155Z","title":"Hwang and D.-h","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.737155Z"},"links":{"cited_paper":"/paper/1010.2585","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:38dc772c717e7d1b76eb2127c76f4ea75b6324c686db4bcc367ec1d873837c40","observation_id":"ab83df98-16a0-4686-88d6-e703613a7b65","resolution":{"observed_at":"2026-08-06T21:30:41.737155Z","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":"2026-08-06T21:30:45.044598Z","title":null,"venue":null,"work_id":"33de5025-dbd9-4fa6-bd60-9dc05caa4f62","year":1973},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.780475Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:2af71b978eb0babcb26508dba6a3b8e660db90c30f6aec2ed990898345886b7a","observation_id":"60229747-d731-445a-b581-b2bf8dfdc647","resolution":{"observed_at":"2026-08-06T21:30:45.103410Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0812.0702","last_updated":"2009-01-23T11:19:35Z","snapshot_observed_at":"2026-07-06T01:48:49.072219Z","submitted_at":"2008-12-03T12:11:21Z","title":"Passage of radiation through wormholes","version":2},"cited_work":{"arxiv_id":"0812.0702","doi":null,"metadata_source":"pith","pith_arxiv_id":"0812.0702","snapshot_observed_at":"2026-08-06T21:30:43.435909Z","title":"Passage of radiation through wormholes","venue":"gr-qc","work_id":"c2eeba17-a0f1-478f-a271-c5ea87e1f182","year":2008},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.019318Z"},"links":{"cited_paper":"/paper/0812.0702","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:9e53938e6bf59a8f1c29b7a4183859464c07d7c337572955fd96c7decf1a74c0","observation_id":"1874e315-05f7-4bda-97d4-ed1e23a921b1","resolution":{"observed_at":"2026-08-06T21:30:43.493418Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:41.893348Z","title":"Shinkai and S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.893348Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:b68477206c9746db439d2a284585f8e9e284d0daec4103db36e79bcb1d9b9553","observation_id":"ea871d62-93f6-4c31-ab58-edf35ed57538","resolution":{"observed_at":"2026-08-06T21:30:41.893348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0806.1370","last_updated":"2008-11-19T05:24:27Z","snapshot_observed_at":"2026-07-06T01:43:37.131093Z","submitted_at":"2008-06-09T04:58:55Z","title":"Instability of wormholes supported by a ghost scalar field. II. Nonlinear evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.1370","snapshot_observed_at":"2026-08-06T21:30:41.934240Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:41.934240Z"},"links":{"cited_paper":"/paper/0806.1370","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:9191e12902777eb790b67d1511a0f7d21d5131907320a7eee89b6d5a0c4fea14","observation_id":"58d40d9f-0fa6-4b85-b6a6-01d3a4ef8ba6","resolution":{"observed_at":"2026-08-06T21:30:41.934240Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.05034","last_updated":"2022-03-04T18:06:08Z","snapshot_observed_at":"2026-07-06T11:17:31.238458Z","submitted_at":"2021-06-09T12:47:20Z","title":"Traversable Wormholes in General Relativity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.05034","snapshot_observed_at":"2026-08-06T21:30:42.171453Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.171453Z"},"links":{"cited_paper":"/paper/2106.05034","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:8ae7c8ca9dedc8565d2fe4f627621e1729517208d9d4946286b6e4c200f28da6","observation_id":"5b8578e3-6952-48dc-87cd-242476c18d30","resolution":{"observed_at":"2026-08-06T21:30:42.171453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.04905","last_updated":"2022-11-29T16:36:29Z","snapshot_observed_at":"2026-07-06T14:03:17.645948Z","submitted_at":"2022-10-10T18:00:00Z","title":"Matter traveling through a wormhole","version":2},"cited_work":{"arxiv_id":"2210.04905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.04905","snapshot_observed_at":"2026-08-06T21:30:43.310202Z","title":"Matter traveling through a wormhole","venue":"gr-qc","work_id":"44b470fe-b44a-4be0-bbe2-b3929e666700","year":2022},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.080735Z"},"links":{"cited_paper":"/paper/2210.04905","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:6bc021c3d16e097719913774b406eb02ead481dfcf3d7608976ea0c4d3285049","observation_id":"379e97a2-b5aa-4dac-b673-d602807297b9","resolution":{"observed_at":"2026-08-06T21:30:43.367054Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.07317","last_updated":"2021-03-12T14:39:56Z","snapshot_observed_at":"2026-08-09T00:40:19.320888Z","submitted_at":"2020-10-14T18:00:09Z","title":"Traversable wormholes in Einstein-Dirac-Maxwell theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.07317","snapshot_observed_at":"2026-08-06T21:30:42.130905Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.130905Z"},"links":{"cited_paper":"/paper/2010.07317","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:b49e8c0020ccb8740d5d4a75cdd50cd81fab9c3ecc6ec4a045fe559272926fc0","observation_id":"dc3fe00d-8c5a-4f06-9818-ec603123d381","resolution":{"observed_at":"2026-08-06T21:30:42.130905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.0489","last_updated":"2012-02-10T21:24:56Z","snapshot_observed_at":"2026-08-07T00:50:08.467097Z","submitted_at":"2011-12-02T15:53:29Z","title":"Two formalisms, one renormalized stress-energy tensor","version":2},"cited_work":{"arxiv_id":"1112.0489","doi":null,"metadata_source":"pith","pith_arxiv_id":"1112.0489","snapshot_observed_at":"2026-08-06T21:30:43.125803Z","title":"Two formalisms, one renormalized stress-energy tensor","venue":"gr-qc","work_id":"8daf15e0-e499-4528-9508-92b4638e39e8","year":2011},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.355327Z"},"links":{"cited_paper":"/paper/1112.0489","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:15fe830a2437899ef19a70989ff4a6e473d626499ebf6ac9b5a2ae651d1589ad","observation_id":"3af2404d-67a1-45f2-b15e-d149e65b1e13","resolution":{"observed_at":"2026-08-06T21:30:43.169991Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.03314","last_updated":"2023-09-06T18:55:21Z","snapshot_observed_at":"2026-08-03T15:12:18.130066Z","submitted_at":"2023-09-06T18:55:21Z","title":"Probing the connection between entangled particles and wormholes in general relativity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.03314","snapshot_observed_at":"2026-08-06T21:30:42.235612Z","title":"Kain, Probing the Connection between Entangled Par- ticles and Wormholes in General Relativity, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.235612Z"},"links":{"cited_paper":"/paper/2309.03314","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:f90f143f78cae3e4975c86a7c3b6eef06784216174dcd7b59bafdcb4380674f2","observation_id":"dc8cb561-df04-4fd6-a476-adfe3151e40d","resolution":{"observed_at":"2026-08-06T21:30:42.235612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.11217","last_updated":"2023-08-08T14:43:16Z","snapshot_observed_at":"2026-07-06T15:29:24.259073Z","submitted_at":"2023-05-18T18:00:01Z","title":"Are Einstein-Dirac-Maxwell wormholes traversable?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.11217","snapshot_observed_at":"2026-08-06T21:30:42.291128Z","title":"Kain, Are Einstein-Dirac-Maxwell wormholes traversable?, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.291128Z"},"links":{"cited_paper":"/paper/2305.11217","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:bd5ac638be41d37a72feb205003fe63009de0e7b67b11324a325fc257c696be5","observation_id":"c26e01cc-5d47-4029-8f7f-f038bc5ad104","resolution":{"observed_at":"2026-08-06T21:30:42.291128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0806.0608","last_updated":"2008-11-19T05:15:23Z","snapshot_observed_at":"2026-07-06T01:42:50.000894Z","submitted_at":"2008-06-03T18:47:37Z","title":"Instability of wormholes supported by a ghost scalar field. I. Linear stability analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.0608","snapshot_observed_at":"2026-08-06T21:30:42.627092Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.627092Z"},"links":{"cited_paper":"/paper/0806.0608","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:09bdc65b8d8f51020baf1701421eb2fed0084c27cc2aca2c6fec672c1325ae61","observation_id":"ff9bc438-7000-4d41-8095-e9bb662d6726","resolution":{"observed_at":"2026-08-06T21:30:42.627092Z","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":"2026-08-06T21:30:44.666339Z","title":"Fabbri and J","venue":null,"work_id":"6882b5aa-1084-4ccd-b699-9b8433c5f167","year":2005},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.449830Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:062f8fc66fb7185fb12896e415e7ecc6fcb8d5d8c78ea98830dbbd4b9fdc611d","observation_id":"daabc747-adf4-4662-b01c-647da2f63137","resolution":{"observed_at":"2026-08-06T21:30:44.775363Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.05273","last_updated":"2015-10-28T12:26:33Z","snapshot_observed_at":"2026-07-06T04:33:28.640674Z","submitted_at":"2015-10-18T16:20:26Z","title":"Adaptive gauge method for long-time double-null simulations of spherical black-hole spacetimes","version":2},"cited_work":{"arxiv_id":"1510.05273","doi":null,"metadata_source":"pith","pith_arxiv_id":"1510.05273","snapshot_observed_at":"2026-08-06T21:30:42.964892Z","title":"Adaptive gauge method for long-time double-null simulations of spherical black-hole spacetimes","venue":"gr-qc","work_id":"0c1120cc-c3e8-49dd-81c8-1d5f83f0336e","year":2015},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.539063Z"},"links":{"cited_paper":"/paper/1510.05273","citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:bba63e86cf8e8737344edfe5a35a26e421448610ccf81fc27ae388c805102fe2","observation_id":"45284b77-f3c6-499d-b045-ca7fa6481ad3","resolution":{"observed_at":"2026-08-06T21:30:43.005319Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:44.285825Z","title":"Alcubierre, Introduction to 3+1 numerical relativity (Oxford University Press, Oxford, UK, 2008)","venue":null,"work_id":"7275e493-f986-401f-a3da-a08e768b8009","year":2008},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.849490Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:b84f9acf342a62920854424375612fb470f7bc822b22bd415e4eeb33df4ab9b1","observation_id":"264bcaf0-7d37-4a86-9813-d25f2a4e3966","resolution":{"observed_at":"2026-08-06T21:30:44.403441Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:42.695255Z","title":null,"venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.695255Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:bf892ac746036e5e523e702243dda60ae50d89a5928a989bb73ad1b42056725a","observation_id":"066c8db5-33d7-4d63-9470-d8e4a2079bc7","resolution":{"observed_at":"2026-08-06T21:30:42.695255Z","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":"2026-08-06T21:30:44.455048Z","title":null,"venue":null,"work_id":"d2158335-fdc1-4140-83fb-408302f45733","year":1975},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:42.766993Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:93e2500740b2e81053a1ea28878ea3981316c49bda6a699fd6c248108f2ee448","observation_id":"f9776dcf-1524-4d1b-9798-7ebbe1dd76d9","resolution":{"observed_at":"2026-08-06T21:30:44.546575Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:30:45.966994Z","title":"That the results are small indicates that the constraint equation is satisfied","venue":null,"work_id":"056205b7-f876-416a-886a-3f6c87b5765e","year":null},"citing_paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity","version":1},"reference_index":200,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:40.745653Z"},"links":{"citing_paper":"/paper/2507.00109"},"observation_digest":"sha256:1a0b056693302138d6c9785f2ca2f80d00c16afa63ddc34f26ec7b44892827be","observation_id":"778558fc-8392-4bfc-8130-1f1a5e5c7395","resolution":{"observed_at":"2026-08-06T21:30:46.033743Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.00109","last_updated":"2025-06-30T18:00:00Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-09T00:40:55.968105Z","submitted_at":"2025-06-30T18:00:00Z","title":"Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity"},"reference_resolution":{"displayed":36,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":23,"verified_exact":7,"verified_fuzzy":6},"total_outbound_references":36},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 36 of 36 outbound references and 0 inbound Pith citation observations for arXiv:2507.00109."}