{"as_of":"2026-08-17T16:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3c7cb798321cb2f63500949f025feee5db86ef29001f80b3342b8b6fafccbefa","coverage":[{"denominator":83,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":83,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:24:51.661934Z","state":"measured"},{"denominator":84,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":84,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T03:36:03.444833Z","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":[{"citation":{"cited_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.13050","snapshot_observed_at":"2026-08-02T03:36:03.444833Z","title":"Alonso-Bardaji, D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.13857","last_updated":"2026-07-15T14:02:52Z","snapshot_observed_at":"2026-08-12T18:06:39.936614Z","submitted_at":"2026-07-15T14:02:52Z","title":"Evaporating cosmologically coupled black holes","version":1},"reference_index":185,"source":"pdf_text","source_observed_at":"2026-08-02T03:36:03.444833Z"},"links":{"cited_paper":"/paper/2504.13050","citing_paper":"/paper/2607.13857"},"observation_digest":"sha256:6e1291c45da1ae9e6f4237300be192b8b9033954bf7610c9941c33bcbd8956ee","observation_id":"6c2d29c1-ef01-4f12-95fb-f2dfd83667f3","resolution":{"observed_at":"2026-08-02T03:36:03.444833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2504.13050/citation-record","integrity":"/paper/2504.13050/integrity","json":"/paper/2504.13050/citation-record.json","paper":"/paper/2504.13050"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:24:51.366879Z","title":"These turning points are given by the roots r =ρrg that solve ¯Ωl(r(r∗);ω)|r=ρrg = 0","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.366879Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:e31ca2530d63e01ef3ff18991c49cfa39be88361b524f0dd12dfccf18e02b9e3","observation_id":"dd8f2ca5-cc62-4eb3-bf9e-dd547ba1cd47","resolution":{"observed_at":"2026-08-16T12:24:51.366879Z","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":"2026-08-16T12:24:51.371772Z","title":"[71] and first determine the gray-body factor for large angular mode numberl","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.371772Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:99a1fa18bbc2d597b9dd2a413bcdfdfc6a7a39ea50a597913e57a47b0174fcb6","observation_id":"daabc16c-688f-49ee-9778-0fc1d9c40d4e","resolution":{"observed_at":"2026-08-16T12:24:51.371772Z","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":"2026-08-16T12:24:51.375774Z","title":"This waves are ignorant of the centrifugal barrier and experience the reduced potential v0(x) = 1− 1 x 2 +λ 2x3 − 3λ 2x4","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.375774Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:598c389315009a5ff3366e140a30ae40f92a5c33d98f39cef294a29ed32f22d9","observation_id":"015a9a8a-2443-401a-b197-94ec002e9dcb","resolution":{"observed_at":"2026-08-16T12:24:51.375774Z","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":"2026-08-16T12:24:52.471266Z","title":null,"venue":null,"work_id":"09c175b1-4c9a-4c07-86c0-4246b108fdd5","year":null},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.379497Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:59cf6ce6f6d9c625e01c148c1d30fcb3322743102169484b82d573b848da45fe","observation_id":"b40a278d-5c99-42fa-939e-caea98f4ef07","resolution":{"observed_at":"2026-08-16T12:24:52.475156Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:51.383016Z","title":"classical","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.383016Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:87e8317eaeaaa806015f4911355d778e79f23da023591eb12bbd69e1eb2c9498","observation_id":"256f5de8-2bfc-4859-93d0-fce781213085","resolution":{"observed_at":"2026-08-16T12:24:51.383016Z","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":"2026-08-16T12:24:51.408528Z","title":"Thiemann, Modern Canonical Quantum General Relativity , Cambridge Monographs on Mathematical Physics (Cam- bridge University Press, 2007)","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.408528Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:79fada51f6f166b37e91217898038d1dc33f974c838453d886e07b11a4f3ddbc","observation_id":"1f1d5e18-4887-49a5-b2c0-e25382922759","resolution":{"observed_at":"2026-08-16T12:24:51.408528Z","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":"2026-08-16T12:24:52.443394Z","title":"Penrose, Gravitational collapse and space-time singularities, Phys","venue":null,"work_id":"445f6e60-d4c1-4f45-bbf4-7b7f09a17892","year":1965},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.390721Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:8482f63ce3f8bd8d28f2c1825f664f93de2aa70132fe9a445fb8fdc5b6b3506b","observation_id":"cda249f4-c002-4b78-8380-5b9196882637","resolution":{"observed_at":"2026-08-16T12:24:52.446957Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.432913Z","title":null,"venue":null,"work_id":"1f16534d-28d7-449a-935c-12deec3b68c8","year":1970},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.394095Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:457efa0f500e93ea2acd1cdf661c7d19b17e4e0f9091d5b96fbb21c0b08bd1ff","observation_id":"f19f1102-af64-4ee3-90c8-fd6608e5dc47","resolution":{"observed_at":"2026-08-16T12:24:52.436524Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.07296","last_updated":"2021-08-16T18:03:02Z","snapshot_observed_at":"2026-08-17T01:59:59.749994Z","submitted_at":"2021-08-16T18:03:02Z","title":"A critical appraisal of the singularity theorems","version":1},"cited_work":{"arxiv_id":"2108.07296","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.07296","snapshot_observed_at":"2026-08-16T12:24:52.158888Z","title":"A critical appraisal of the singularity theorems","venue":"gr-qc","work_id":"49496253-98a9-4dc9-b1c7-62915230892b","year":2021},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.397387Z"},"links":{"cited_paper":"/paper/2108.07296","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:2d6b15734298a6676089bb8481fff2dc5757309a38f5de09198a95590298733e","observation_id":"12b2d91a-354e-4a12-811f-8d5ffe4a53c3","resolution":{"observed_at":"2026-08-16T12:24:52.162671Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:51.401360Z","title":"Rovelli, Quantum gravity , Cambridge Monographs on Mathematical Physics (Univ","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.401360Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:6b25880121140d9ab8211f269db808c43613cbeddecddd557e6b0282252bf582","observation_id":"06046614-fe42-4e40-8fd8-5fe49bae15f3","resolution":{"observed_at":"2026-08-16T12:24:51.401360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0404018","last_updated":"2004-09-03T23:18:29Z","snapshot_observed_at":"2026-07-07T03:19:04.182335Z","submitted_at":"2004-04-05T13:34:11Z","title":"Background Independent Quantum Gravity: A Status Report","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0404018","snapshot_observed_at":"2026-08-16T12:24:51.404517Z","title":"Ashtekar and J","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.404517Z"},"links":{"cited_paper":"/paper/gr-qc/0404018","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:f7dff7faf5a1a26a9974eb6043be39c96d2289585866b47143f7cb067b178956","observation_id":"6a29bced-8304-47a6-bf4a-36f45daf6e1d","resolution":{"observed_at":"2026-08-16T12:24:51.404517Z","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":"2026-08-16T12:24:52.391591Z","title":"Agull´ o, J","venue":null,"work_id":"19dfc69d-b0ec-44fb-a23d-77e14c8cc0a8","year":2012},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.429216Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:d36ae6a1ec51a155809bef4109f2f495aa933b14ab731ddd423d1edc79b69dd9","observation_id":"fdea6263-b2f5-4427-83c4-6cd5f2a6588f","resolution":{"observed_at":"2026-08-16T12:24:52.394951Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.410783Z","title":"Ashtekar and E","venue":null,"work_id":"6a160300-9b8e-4e6b-8fde-b68b16a22385","year":2021},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.412101Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:fb78c3ac3cd6e2376631df110c6a1a52323fded062917db9fdff429aeaf93ea0","observation_id":"0e1bb66d-82cb-459e-bd26-26d467b24a3e","resolution":{"observed_at":"2026-08-16T12:24:52.414065Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9411005","last_updated":"1994-11-02T04:51:54Z","snapshot_observed_at":"2026-08-05T14:37:53.324208Z","submitted_at":"1994-11-02T04:51:54Z","title":"Discreteness of area and volume in quantum gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9411005","snapshot_observed_at":"2026-08-16T12:24:51.415210Z","title":"Rovelli and L","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.415210Z"},"links":{"cited_paper":"/paper/gr-qc/9411005","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:9080753d32b1268e2e4d6554cfcc10dc8bc62a51f8ddc46cda0aadc4c5597d73","observation_id":"65bcc32d-0f1f-4750-a9ab-cb298e88e360","resolution":{"observed_at":"2026-08-16T12:24:51.415210Z","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":"2026-08-16T12:24:52.401052Z","title":"Ashtekar and J","venue":null,"work_id":"b98cf385-2275-4f64-87f8-700b881d0825","year":1997},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.418830Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:ba60d41baca4bff48a607171b87db9a6d2144c4ddec0025f4a2a00ab6f5a8c68","observation_id":"8898e838-fd28-4248-a7f2-73c5b96796db","resolution":{"observed_at":"2026-08-16T12:24:52.404506Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0407052","last_updated":"2004-07-14T19:36:34Z","snapshot_observed_at":"2026-08-16T19:04:18.348770Z","submitted_at":"2004-07-14T19:36:34Z","title":"Black hole entropy in Loop Quantum Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0407052","snapshot_observed_at":"2026-08-16T12:24:51.422034Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.422034Z"},"links":{"cited_paper":"/paper/gr-qc/0407052","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:02640dfca307b8574a7ff6cff9845ac4bd91ff3034bae2e7bcbb4dbbdb76b88d","observation_id":"7d636253-49ed-4834-9c23-de19751f9ec4","resolution":{"observed_at":"2026-08-16T12:24:51.422034Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9603063","last_updated":"1996-03-30T19:45:20Z","snapshot_observed_at":"2026-08-15T20:46:41.114137Z","submitted_at":"1996-03-30T19:45:20Z","title":"Black Hole Entropy from Loop Quantum Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9603063","snapshot_observed_at":"2026-08-16T12:24:51.425584Z","title":"Rovelli, Black hole entropy from loop quantum gravity, Phys","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.425584Z"},"links":{"cited_paper":"/paper/gr-qc/9603063","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:4d360abb5bb8e92fbfb1f909e9067375b4838459aa94125a51612ce6979ef292","observation_id":"789518d2-076c-4841-9976-fe22c27f9b9f","resolution":{"observed_at":"2026-08-16T12:24:51.425584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.01236","last_updated":"2016-12-05T03:26:24Z","snapshot_observed_at":"2026-08-15T08:16:32.473111Z","submitted_at":"2016-12-05T03:26:24Z","title":"Loop Quantum Cosmology: A brief review","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.01236","snapshot_observed_at":"2026-08-16T12:24:51.448996Z","title":"Agullo and P","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.448996Z"},"links":{"cited_paper":"/paper/1612.01236","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:87e6ac1c03f9a2b3c5d0b73edc3b9cebf864ca7393c6e9fdd4aead2a46f06a93","observation_id":"da13b562-4dc2-4774-8dbb-8da2ba1c13d8","resolution":{"observed_at":"2026-08-16T12:24:51.448996Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.13469","last_updated":"2022-12-27T12:38:39Z","snapshot_observed_at":"2026-08-16T16:05:50.526233Z","submitted_at":"2022-12-27T12:38:39Z","title":"Black Hole Entropy in Loop Quantum Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.13469","snapshot_observed_at":"2026-08-16T12:24:51.432162Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.432162Z"},"links":{"cited_paper":"/paper/2212.13469","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:6e2218bef7ee91f9b4d623608573ce8c2836dc93cb5a1f750ab1fab04caae34c","observation_id":"d0578e89-0f13-4b3d-a976-df864282b1e7","resolution":{"observed_at":"2026-08-16T12:24:51.432162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09149","last_updated":"2017-09-08T13:12:36Z","snapshot_observed_at":"2026-08-14T21:09:49.837237Z","submitted_at":"2017-03-27T15:38:15Z","title":"Black Holes in Loop Quantum Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.09149","snapshot_observed_at":"2026-08-16T12:24:51.435495Z","title":"Perez, Black Holes in Loop Quantum Gravity, Rept","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.435495Z"},"links":{"cited_paper":"/paper/1703.09149","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:2670217f7aeb3e3437e7150331a4407db489dbc927842112248603049c08915f","observation_id":"3977958b-8bfd-4ef9-a97b-3711385acd34","resolution":{"observed_at":"2026-08-16T12:24:51.435495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0304074","last_updated":"2003-12-24T16:11:20Z","snapshot_observed_at":"2026-08-14T08:16:00.233644Z","submitted_at":"2003-04-21T18:13:53Z","title":"Mathematical structure of loop quantum cosmology","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0304074","snapshot_observed_at":"2026-08-16T12:24:51.439021Z","title":"Ashtekar, M","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.439021Z"},"links":{"cited_paper":"/paper/gr-qc/0304074","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:62e543204b6bced34e9c077a0f185eea9b19fa97eb3b3e7d51e743cd714acf3d","observation_id":"3f40f00b-68cf-436c-b416-1e2974a6257d","resolution":{"observed_at":"2026-08-16T12:24:51.439021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0601085","last_updated":"2006-01-20T15:54:24Z","snapshot_observed_at":"2026-08-10T12:00:35.372763Z","submitted_at":"2006-01-20T15:54:24Z","title":"Loop Quantum Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0601085","snapshot_observed_at":"2026-08-16T12:24:51.442356Z","title":"Bojowald, Loop quantum cosmology, Living Rev","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.442356Z"},"links":{"cited_paper":"/paper/gr-qc/0601085","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:ee9aac00247f4bd34b7c90835a014fd547246f8c88e481074f3c8a5e49491b42","observation_id":"350befda-5f0b-43e3-a756-b47b4bd7291c","resolution":{"observed_at":"2026-08-16T12:24:51.442356Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0893","last_updated":"2011-08-22T03:57:38Z","snapshot_observed_at":"2026-08-15T04:39:08.444874Z","submitted_at":"2011-08-03T17:04:35Z","title":"Loop Quantum Cosmology: A Status Report","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.0893","snapshot_observed_at":"2026-08-16T12:24:51.445580Z","title":"Ashtekar and P","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.445580Z"},"links":{"cited_paper":"/paper/1108.0893","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:5a9f78f16dcdb5a7d2ab436aef3dc2fab6351889a6f509176e3cc197ae6cc42b","observation_id":"3c37f982-c88a-48d2-8a80-1000a2b8b3fb","resolution":{"observed_at":"2026-08-16T12:24:51.445580Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.12646","last_updated":"2021-06-29T20:08:57Z","snapshot_observed_at":"2026-08-16T12:40:44.542560Z","submitted_at":"2019-11-28T11:08:55Z","title":"(b,v)-type variables for black to white hole transitions in effective loop quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.12646","snapshot_observed_at":"2026-08-16T12:24:51.470062Z","title":"Bodendorfer, F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.470062Z"},"links":{"cited_paper":"/paper/1911.12646","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:c88df3b48278f29712b76108b0bcb107e543b556605254b266448e695f04b1e9","observation_id":"6bfc4723-bfb7-4c66-a952-a82c02f5b7bf","resolution":{"observed_at":"2026-08-16T12:24:51.470062Z","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.90.023538","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:24:51.732600Z","title":"Rovelli and E","venue":null,"work_id":"41ff2c98-68c8-4f32-ada5-925c176fcbfa","year":2014},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.452464Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:1c663dc73f4dd22e2dd1ad63b959e4f77d4ef998f41c4905b80b77bd88bd890b","observation_id":"5fdc2d32-82b9-4a7a-afc5-a3c7a14e2272","resolution":{"observed_at":"2026-08-16T12:24:51.736513Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.09302","last_updated":"2022-06-13T20:35:29Z","snapshot_observed_at":"2026-08-15T21:06:17.460381Z","submitted_at":"2020-06-16T16:46:03Z","title":"Effective loop quantum gravity framework for vacuum spherically symmetric space-times","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.09302","snapshot_observed_at":"2026-08-16T12:24:51.456072Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.456072Z"},"links":{"cited_paper":"/paper/2006.09302","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:194329657d0924d7c7ea2bce3a228f6d84b3f914267cf6a80ab4f70965a0fdeb","observation_id":"3561439f-bdd0-4e93-9cc4-a63d6bc15b05","resolution":{"observed_at":"2026-08-16T12:24:51.456072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.02406","last_updated":"2019-02-14T18:52:53Z","snapshot_observed_at":"2026-08-14T19:06:43.296891Z","submitted_at":"2018-06-06T19:57:27Z","title":"Quantum Extension of the Kruskal Space-time","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.02406","snapshot_observed_at":"2026-08-16T12:24:51.459376Z","title":"Ashtekar, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.459376Z"},"links":{"cited_paper":"/paper/1806.02406","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:c50525ba4465bb2896f7ee64f11d994108efa1480e129ab5febde1986bdd564f","observation_id":"96107c4c-8f51-448f-81c2-98b676da7184","resolution":{"observed_at":"2026-08-16T12:24:51.459376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.00648","last_updated":"2018-11-09T20:17:33Z","snapshot_observed_at":"2026-08-15T21:07:10.032466Z","submitted_at":"2018-06-02T15:01:34Z","title":"Quantum Transfiguration of Kruskal Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.00648","snapshot_observed_at":"2026-08-16T12:24:51.463054Z","title":"Ashtekar, J","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.463054Z"},"links":{"cited_paper":"/paper/1806.00648","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:48e52c8cf2b2f86eb4eaf8fd331c35267f0272c6f43adf07915535cd71fbacaa","observation_id":"2fd01c60-5937-4218-b7ae-5795386738b6","resolution":{"observed_at":"2026-08-16T12:24:51.463054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04542","last_updated":"2019-11-05T13:29:05Z","snapshot_observed_at":"2026-08-15T21:01:01.392925Z","submitted_at":"2019-02-12T18:42:03Z","title":"Effective Quantum Extended Spacetime of Polymer Schwarzschild Black Hole","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04542","snapshot_observed_at":"2026-08-16T12:24:51.466493Z","title":"Bodendorfer, F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.466493Z"},"links":{"cited_paper":"/paper/1902.04542","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:12b85298d1d35cb50787f2eb0e750ba409b32039292f72adb1c9d6a78d80ac6a","observation_id":"41624bea-0fd8-4bc8-9788-310ac86b7f47","resolution":{"observed_at":"2026-08-16T12:24:51.466493Z","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":"2026-08-16T12:24:52.454195Z","title":"In contrast to what we analyzed in the main text (Sec","venue":null,"work_id":"7d4f3ef5-e3ae-42d9-9181-5fac27bdc85e","year":null},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.386909Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:9fc0ab37304bc2a4911a2fc3d5af542cfd7fc3a2d80249154d5351618246e122","observation_id":"ec3d1579-67c9-4542-a322-27997739256e","resolution":{"observed_at":"2026-08-16T12:24:52.457848Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.01152","last_updated":"2019-01-31T10:16:49Z","snapshot_observed_at":"2026-08-16T12:40:44.012570Z","submitted_at":"2018-03-03T12:36:12Z","title":"Polymer Schwarzschild black hole: An effective metric","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.01152","snapshot_observed_at":"2026-08-16T12:24:51.473673Z","title":"Ben Achour, F","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.473673Z"},"links":{"cited_paper":"/paper/1803.01152","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:6380773f487be0d5004ed17352ed44ed8b56dd327e68dd475305fb88d9ce0840","observation_id":"2f0130c5-f9b9-4287-954d-906bcd7ddfa4","resolution":{"observed_at":"2026-08-16T12:24:51.473673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.01513","last_updated":"2020-06-02T10:45:15Z","snapshot_observed_at":"2026-08-05T05:07:02.446074Z","submitted_at":"2020-06-02T10:45:15Z","title":"Spherically symmetric loop quantum gravity: analysis of improved dynamics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.01513","snapshot_observed_at":"2026-08-16T12:24:51.477297Z","title":"Gambini, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.477297Z"},"links":{"cited_paper":"/paper/2006.01513","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:dec8270294ea36bebe3de5aa61fccef29361f22b3ed002e92eb1369702c64bd9","observation_id":"06961434-881e-4678-9359-4161b34de69f","resolution":{"observed_at":"2026-08-16T12:24:51.477297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.14212","last_updated":"2021-06-15T12:21:49Z","snapshot_observed_at":"2026-08-16T18:55:42.005374Z","submitted_at":"2020-12-28T12:28:02Z","title":"Loop quantum black hole extensions within the improved dynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.14212","snapshot_observed_at":"2026-08-16T12:24:51.480931Z","title":"Gambini, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.480931Z"},"links":{"cited_paper":"/paper/2012.14212","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:8273913a146bf4528b56320a2f5a51a2255ccf9f461170b42aa3e6176c089792","observation_id":"a16b4eb6-4848-452a-a0f3-bf90f507a657","resolution":{"observed_at":"2026-08-16T12:24:51.480931Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.07595","last_updated":"2022-08-11T14:24:25Z","snapshot_observed_at":"2026-08-16T18:17:15.272842Z","submitted_at":"2021-06-14T16:55:45Z","title":"Anomaly-free deformations of spherical general relativity coupled to matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.07595","snapshot_observed_at":"2026-08-16T12:24:51.484853Z","title":"Alonso-Bardaji and D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.484853Z"},"links":{"cited_paper":"/paper/2106.07595","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:ecc3d86e85fecd80fc15d6fa4010ce8c87528289cb1dc9d5c657009983e3c65e","observation_id":"3fdd1fd7-3a4c-4240-aa13-ce430a90bee3","resolution":{"observed_at":"2026-08-16T12:24:51.484853Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.12110","last_updated":"2023-04-17T12:55:11Z","snapshot_observed_at":"2026-08-16T17:32:35.315668Z","submitted_at":"2021-12-22T18:20:11Z","title":"An effective model for the quantum Schwarzschild black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.12110","snapshot_observed_at":"2026-08-16T12:24:51.488570Z","title":"Alonso-Bardaji, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.488570Z"},"links":{"cited_paper":"/paper/2112.12110","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:3d0736b0030c1ff9f0a7e4706a4ae8df527de80c0c618c0dd05157b80c39fc4d","observation_id":"48e9d1d8-38e5-40cb-ad32-cf09341653f5","resolution":{"observed_at":"2026-08-16T12:24:51.488570Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.02098","last_updated":"2022-08-08T17:14:34Z","snapshot_observed_at":"2026-08-16T17:02:38.443850Z","submitted_at":"2022-05-04T14:51:31Z","title":"Nonsingular spherically symmetric black-hole model with holonomy corrections","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.02098","snapshot_observed_at":"2026-08-16T12:24:51.492169Z","title":"Alonso-Bardaji, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.492169Z"},"links":{"cited_paper":"/paper/2205.02098","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:7c6fbadd287c3030e74ccd7fca0f8746314c98473164bcf8d7c09b102b3de617","observation_id":"2fc04734-5eb4-429e-8c03-83565f3003b4","resolution":{"observed_at":"2026-08-16T12:24:51.492169Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.10619","last_updated":"2023-03-29T09:01:48Z","snapshot_observed_at":"2026-08-16T15:56:28.231241Z","submitted_at":"2023-02-21T12:02:20Z","title":"Singularity resolution by holonomy corrections: Spherical charged black holes in cosmological backgrounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.10619","snapshot_observed_at":"2026-08-16T12:24:51.495800Z","title":"Alonso-Bardaji, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.495800Z"},"links":{"cited_paper":"/paper/2302.10619","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:29d3515a4582cfa7dc804000547a12a8563d7a1543bb375c1872b041f9ed369c","observation_id":"285939c4-af5c-4370-8303-27377142493f","resolution":{"observed_at":"2026-08-16T12:24:51.495800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.01616","last_updated":"2022-01-05T13:52:40Z","snapshot_observed_at":"2026-08-16T18:07:26.150426Z","submitted_at":"2022-01-05T13:52:40Z","title":"Towards a quantum notion of covariance in spherically symmetric loop quantum gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.01616","snapshot_observed_at":"2026-08-16T12:24:51.499525Z","title":"Gambini, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.499525Z"},"links":{"cited_paper":"/paper/2201.01616","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:8f60925bdd56a99d0a90df8bb767287e5bfca6d1ce3d3d2d875563f9a0592176","observation_id":"4ad93e00-a127-4ae6-a290-58d7a7c58607","resolution":{"observed_at":"2026-08-16T12:24:51.499525Z","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":"2026-08-16T12:24:51.503876Z","title":"Ben´ ıtez, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.503876Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:f73df4a8ba1bebca1f0be3efb03fe87f21db908477b3185c5b940dd5cdad6f2b","observation_id":"9cc6a1b3-eadd-48a8-8481-e520f0ba1dec","resolution":{"observed_at":"2026-08-16T12:24:51.503876Z","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":"2026-08-16T12:24:51.508316Z","title":"Giesel, B.-F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.508316Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:18b06377dca0ca0dc6c3ad10719138084f765dcd5efa9682441230c6182d8fa4","observation_id":"bb37edcd-16ad-4714-9bda-ba0e312503be","resolution":{"observed_at":"2026-08-16T12:24:51.508316Z","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":"2026-08-16T12:24:52.381872Z","title":"Gambini, F","venue":null,"work_id":"a34a9b37-0c47-494e-9b32-f2170294a3ef","year":2022},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.511792Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:6ec8f234e8924f31bbf8ee0a9b19107b940d6ae1cac09aadb419b80d573e12b6","observation_id":"da818794-419a-4928-85b0-0cfc4819d347","resolution":{"observed_at":"2026-08-16T12:24:52.385062Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:51.515389Z","title":"Husain, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.515389Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:cd01cd5a3df1becaeed287868b3261a342f570bebaf9b772fb5d814a7dc5ba79","observation_id":"13287a88-dd85-4635-a768-1d8c6bfc261e","resolution":{"observed_at":"2026-08-16T12:24:51.515389Z","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":"2026-08-16T12:24:51.518748Z","title":"Giesel, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.518748Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:d22aa4bdfe426669e01376aada44d8b7200e797a5e6dd2fd354ddba2869c7da9","observation_id":"606e6a4f-e04f-4be0-a84a-f32d284d05d4","resolution":{"observed_at":"2026-08-16T12:24:51.518748Z","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.110.066004","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T12:24:51.689591Z","title":"Cipriani, F","venue":null,"work_id":"ae03a93e-0731-4916-9952-bc96b7deab9e","year":2024},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.522500Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:45f643939b50be28f6fe836e78cd59adbba5aba2dbd6d4010200ab7faa231f9d","observation_id":"215969fb-6572-449c-b71d-f33079cf9e84","resolution":{"observed_at":"2026-08-16T12:24:51.694884Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.15505","last_updated":"2024-03-06T16:48:22Z","snapshot_observed_at":"2026-08-16T14:31:52.246906Z","submitted_at":"2023-12-24T15:14:01Z","title":"Nonsingular collapse of a spherical dust cloud","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.15505","snapshot_observed_at":"2026-08-16T12:24:51.525871Z","title":"Alonso-Bardaji and D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.525871Z"},"links":{"cited_paper":"/paper/2312.15505","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:26169330cf25515ff4d6f03b735d94a578ee5ff2b09994d0c25f5b29f72ef89b","observation_id":"1d83b0d5-656c-4ae7-a932-3c7c68c8bde2","resolution":{"observed_at":"2026-08-16T12:24:51.525871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.20529","last_updated":"2025-06-04T07:59:02Z","snapshot_observed_at":"2026-08-16T13:05:36.654534Z","submitted_at":"2024-10-27T17:47:20Z","title":"Formation of nonsingular spherical black holes with holonomy corrections","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.20529","snapshot_observed_at":"2026-08-16T12:24:51.529453Z","title":"Alonso-Bardaji, Formation of nonsingular spherical black holes with holonomy corrections, Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.529453Z"},"links":{"cited_paper":"/paper/2410.20529","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:9662f18f2dfafb7074033525ac55239b89855be276b2e95e5c48f550d5cc982c","observation_id":"d35c3db7-f468-45e8-bbac-9f733d86f1e8","resolution":{"observed_at":"2026-08-16T12:24:51.529453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.12951","last_updated":"2024-10-03T15:20:56Z","snapshot_observed_at":"2026-08-16T14:50:37.228312Z","submitted_at":"2023-10-19T17:51:54Z","title":"Spacetime geometry from canonical spherical gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.12951","snapshot_observed_at":"2026-08-16T12:24:51.532902Z","title":"Alonso-Bardaji and D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.532902Z"},"links":{"cited_paper":"/paper/2310.12951","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:4ade70e640d271d7d6bd5f69d5e6c85e30d966850005d11c534bdff4e1bca976","observation_id":"d22e4475-2045-45c6-a77d-35d4df80661a","resolution":{"observed_at":"2026-08-16T12:24:51.532902Z","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":"2026-08-16T12:24:52.371697Z","title":"Bojowald and E","venue":null,"work_id":"2040d023-3b9f-4ab1-8873-0f27319b8767","year":2023},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.536296Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:449207b9096b6b31143b2b1309d1a827317edb714316468768a806e040c33ae2","observation_id":"10e70199-1571-48cc-a055-a476a5edb7d2","resolution":{"observed_at":"2026-08-16T12:24:52.375007Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:51.539753Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.539753Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:a6c2a3f05a022bff7cb84c8dc3a49ea71155306498459f910f62c1cebe775476","observation_id":"925d1c33-3f87-4d70-b7f1-3305d33c6690","resolution":{"observed_at":"2026-08-16T12:24:51.539753Z","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":"2026-08-16T12:24:51.543276Z","title":null,"venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.543276Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:23d01b68e7cb8109db765b7522f928fa3ba3a8740a0d6c7706425065df0ffba1","observation_id":"d7b137b8-662a-40bc-b21d-368ef39268e5","resolution":{"observed_at":"2026-08-16T12:24:51.543276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.09584","last_updated":"2024-09-09T17:02:58Z","snapshot_observed_at":"2026-08-16T13:34:47.730682Z","submitted_at":"2024-07-12T11:44:43Z","title":"Planck stars, White Holes, Remnants and Planck-mass quasi-particles. The quantum gravity phase in black holes' evolution and its manifestations","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.09584","snapshot_observed_at":"2026-08-16T12:24:51.546549Z","title":"Rovelli and F","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.546549Z"},"links":{"cited_paper":"/paper/2407.09584","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:cb0af9afc4b4b880be470551cc85a18870f9a64fb364022d135b2baa9719f933","observation_id":"a3b39dcb-3dbd-48e6-b92b-4029e5e07315","resolution":{"observed_at":"2026-08-16T12:24:51.546549Z","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":"2026-08-16T12:24:52.351002Z","title":null,"venue":null,"work_id":"d429fea0-eb82-45b3-b518-29c6ec20022f","year":2024},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.550104Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:eb54a928459673a039372e5e87fa9680481028a71b9182883a811d311c56557f","observation_id":"8e728b65-0760-4a93-957b-f52d56c3169e","resolution":{"observed_at":"2026-08-16T12:24:52.354136Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.341369Z","title":"Calz` a, Grayhawk: A public code for calculating the gray body factors of massless fields around spherically symmetric black holes, Physics of the Dark Universe , 101900 (2025)","venue":null,"work_id":"af7a95b7-421f-4a31-92f8-258cb8a461aa","year":2025},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.553779Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:190b46047065ed80467713a09ff8f74ee1cf542079f8bbe40f6d4be804da5e2f","observation_id":"5f6ae478-b53e-4101-8a2a-0cc7ab5d2866","resolution":{"observed_at":"2026-08-16T12:24:52.344864Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.331222Z","title":"Calz` a, D","venue":null,"work_id":"ae54e7db-4b40-4d97-8375-ab82046b13e0","year":2025},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.557133Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:77eb99bc38765d9cfa4a250663b10a7cf877399101d6ab680bd1f976f320c9e2","observation_id":"f3eb02a8-7dc4-4d96-a228-a250096ce945","resolution":{"observed_at":"2026-08-16T12:24:52.334970Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.321243Z","title":"Calz` a, D","venue":null,"work_id":"ff025391-b14d-42d5-ba2b-9f5a1af5b050","year":2025},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.560852Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:9304ebacc56742ac42c1ae9922321ccce304d88e7d21e64edaca063e1ea52963","observation_id":"52668670-5f72-440a-91e0-f99c0df885eb","resolution":{"observed_at":"2026-08-16T12:24:52.324933Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.06964","last_updated":"2025-04-09T15:19:03Z","snapshot_observed_at":"2026-08-16T12:42:39.983528Z","submitted_at":"2025-04-09T15:19:03Z","title":"Thermodynamics of effective loop quantum black holes","version":1},"cited_work":{"arxiv_id":"2504.06964","doi":null,"metadata_source":"pith","pith_arxiv_id":"2504.06964","snapshot_observed_at":"2026-08-16T12:24:51.876169Z","title":"Thermodynamics of effective loop quantum black holes","venue":"gr-qc","work_id":"9f3c2387-0bfe-418b-af29-462e9831a43e","year":2025},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.564476Z"},"links":{"cited_paper":"/paper/2504.06964","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:3a717ec2f6dd1bdff54fa1f1f6b1ed14667e23109593f0821dc14f7764549d99","observation_id":"6828b21a-8142-408e-a678-3548ffec5f15","resolution":{"observed_at":"2026-08-16T12:24:51.880734Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.311203Z","title":"Szekeres, The gravitational compass, Journal of Mathematical Physics 6, 1387 (1965)","venue":null,"work_id":"bb4a5b4f-fe5d-4e63-8532-c1217406eae8","year":1965},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.567953Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:455fed1e89a711db9ee5997346863a322576ea92534784df1c8712a4ec4d5e18","observation_id":"ec35a716-ae59-41d6-a993-eb804366b9e9","resolution":{"observed_at":"2026-08-16T12:24:52.314614Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.300711Z","title":null,"venue":null,"work_id":"827da58f-741e-4801-a7f0-d4ef2f5105c4","year":1976},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.571616Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:abbbeb775f8038d08af542af097cc3c38b1b38d17a2efb012345e21182df5ae5","observation_id":"febb43cb-32be-48fc-b2c9-266d2f67d1e0","resolution":{"observed_at":"2026-08-16T12:24:52.304221Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.290852Z","title":null,"venue":null,"work_id":"968dee55-bca9-481c-9197-7eba261d7add","year":2024},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.575164Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:dffdf26f76fc67244bc032af8738aa42503c2c2904611c665ee04c7aa496d333","observation_id":"8844127a-e134-42e6-aad2-ede229d6a129","resolution":{"observed_at":"2026-08-16T12:24:52.294194Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.280956Z","title":null,"venue":null,"work_id":"efa5b024-08e4-4a87-b1c7-b77c76379485","year":1975},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.578484Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:12429c05739fd756096663d4b8fd71e079ad503de23e2e443afed39ea4438c31","observation_id":"2f0912c1-ef36-4bc3-9264-e07d9c880758","resolution":{"observed_at":"2026-08-16T12:24:52.284340Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9907001","last_updated":"2001-03-02T13:52:00Z","snapshot_observed_at":"2026-07-07T05:20:17.184705Z","submitted_at":"1999-07-01T23:24:32Z","title":"Hawking Radiation as Tunneling","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9907001","snapshot_observed_at":"2026-08-16T12:24:51.582009Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.582009Z"},"links":{"cited_paper":"/paper/hep-th/9907001","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:72d9f897927dabbdc6afbbd41871b9de5f62086fa6b2aa089b1a90165ba01830","observation_id":"4691752a-13fe-445e-990f-8e628d814fb1","resolution":{"observed_at":"2026-08-16T12:24:51.582009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0007022","last_updated":"2001-03-24T15:22:57Z","snapshot_observed_at":"2026-08-17T14:05:03.671470Z","submitted_at":"2000-07-11T17:30:47Z","title":"Method of complex paths and general covariance of Hawking radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0007022","snapshot_observed_at":"2026-08-16T12:24:51.585514Z","title":"Shankaranarayanan, K","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.585514Z"},"links":{"cited_paper":"/paper/gr-qc/0007022","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:f823bf361d56525efb7ed9cee4f5147f7ed033e5a746e4a238c0236b3d25b9d6","observation_id":"bf45780b-ae06-4ebb-aaa8-d458ffdf85ef","resolution":{"observed_at":"2026-08-16T12:24:51.585514Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9903027","last_updated":"2000-01-26T10:15:28Z","snapshot_observed_at":"2026-07-07T03:30:12.663121Z","submitted_at":"1999-03-08T09:26:38Z","title":"How the Change in Horizon Area Drives Black Hole Evaporation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9903027","snapshot_observed_at":"2026-08-16T12:24:51.589066Z","title":"Massar and R","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.589066Z"},"links":{"cited_paper":"/paper/gr-qc/9903027","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:25c46efd2e7f04178e0aaf86af8c00f0c171e1c55f330b183535995e829223e8","observation_id":"01ac6fbd-0727-41db-94c6-8eea0898877e","resolution":{"observed_at":"2026-08-16T12:24:51.589066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.4153","last_updated":"2011-06-21T09:50:22Z","snapshot_observed_at":"2026-08-15T04:43:20.460572Z","submitted_at":"2011-06-21T09:50:22Z","title":"Tunnelling Methods and Hawking's radiation: achievements and prospects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.4153","snapshot_observed_at":"2026-08-16T12:24:51.592632Z","title":"Vanzo, G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.592632Z"},"links":{"cited_paper":"/paper/1106.4153","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:edd0a00768f76a4afa82491ffaa6c95cbc022cce9e882d5aec13f611fe09f04a","observation_id":"f09dd7cc-632f-47be-bc0c-43355fdfc089","resolution":{"observed_at":"2026-08-16T12:24:51.592632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.1569","last_updated":"2011-04-19T09:47:20Z","snapshot_observed_at":"2026-08-16T12:40:40.750946Z","submitted_at":"2011-04-08T13:19:00Z","title":"On tunneling across horizons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.1569","snapshot_observed_at":"2026-08-16T12:24:51.596303Z","title":"Vanzo, On tunneling across horizons, EPL 95, 20001 (2011), arXiv:1104.1569 [gr-qc]","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.596303Z"},"links":{"cited_paper":"/paper/1104.1569","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:7001b8d23f06cdadcc0c3e9d9e2b63e45816b2ffe8416a2ec99931060514ff37","observation_id":"b595dfe3-ba45-4550-8a80-11d83625b38a","resolution":{"observed_at":"2026-08-16T12:24:51.596303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0707.4425","last_updated":"2007-10-03T13:11:08Z","snapshot_observed_at":"2026-08-15T10:35:09.805100Z","submitted_at":"2007-07-30T14:37:35Z","title":"On the Hawking radiation as tunneling for a class of dynamical black holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0707.4425","snapshot_observed_at":"2026-08-16T12:24:51.600204Z","title":"Di Criscienzo, M","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.600204Z"},"links":{"cited_paper":"/paper/0707.4425","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:51aa3d590460ba0e546b742172cad28db4c6cc2a6c7533d656bf3fb70381d6fd","observation_id":"957bf338-f300-4900-860a-ae35d798b5d8","resolution":{"observed_at":"2026-08-16T12:24:51.600204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.0797","last_updated":"2010-10-05T08:35:35Z","snapshot_observed_at":"2026-08-15T05:06:58.542338Z","submitted_at":"2010-10-05T08:35:35Z","title":"Hamilton-Jacobi Method and Gravitation","version":1},"cited_work":{"arxiv_id":"1010.0797","doi":null,"metadata_source":"pith","pith_arxiv_id":"1010.0797","snapshot_observed_at":"2026-08-16T12:24:51.792908Z","title":"Hamilton-Jacobi Method and Gravitation","venue":"gr-qc","work_id":"84e9fdc5-257d-4240-8d6f-a1c12a03f7ca","year":2010},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.603908Z"},"links":{"cited_paper":"/paper/1010.0797","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:66c5782faf68f0a7cf3051a3e1615558ebb542d20a74b32455cc3620b8154f30","observation_id":"4f31a9f3-521f-411a-865f-47857ab2af6e","resolution":{"observed_at":"2026-08-16T12:24:51.797811Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0806.0014","last_updated":"2009-02-11T11:48:23Z","snapshot_observed_at":"2026-08-15T10:14:17.334651Z","submitted_at":"2008-05-30T20:42:47Z","title":"Local Hawking temperature for dynamical black holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.0014","snapshot_observed_at":"2026-08-16T12:24:51.607696Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.607696Z"},"links":{"cited_paper":"/paper/0806.0014","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:df7569e902c5a778eedf521d23aa06b8886bd01c944998957afaf4f3676e3047","observation_id":"138e2600-097a-4f61-be3c-81cba3cccd15","resolution":{"observed_at":"2026-08-16T12:24:51.607696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.11095","last_updated":"2020-10-16T10:24:27Z","snapshot_observed_at":"2026-08-17T01:57:15.777158Z","submitted_at":"2020-03-24T20:00:01Z","title":"Quantum effects across dynamical horizons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.11095","snapshot_observed_at":"2026-08-16T12:24:51.611276Z","title":"Giavoni and M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.611276Z"},"links":{"cited_paper":"/paper/2003.11095","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:eee55f9808aa7450dcb6e230caf1d69367389a17278d0a2953daa1c559d157db","observation_id":"c593d548-c600-4746-8793-cb16231854dd","resolution":{"observed_at":"2026-08-16T12:24:51.611276Z","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":"2026-08-16T12:24:52.271096Z","title":null,"venue":null,"work_id":"c3971cc8-a6ec-45bf-95c8-d0778b28e343","year":2015},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.615211Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:e2adec44afbc50ca2d908289f5f7d15fac1a6d9dbcea541c583615be17ff7fea","observation_id":"97683eb7-df1e-4dc4-8e8c-bb84a96a9e0f","resolution":{"observed_at":"2026-08-16T12:24:52.274276Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.14603","last_updated":"2025-02-28T18:00:01Z","snapshot_observed_at":"2026-08-17T13:53:30.269826Z","submitted_at":"2024-06-20T18:00:00Z","title":"Tunneling method for Hawking quanta in analogue gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.14603","snapshot_observed_at":"2026-08-16T12:24:51.618471Z","title":"Del Porro, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.618471Z"},"links":{"cited_paper":"/paper/2406.14603","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:633a8558be2e7540aec539955f1a404903bb4bae2978c2daa56c8d89af4d5351","observation_id":"cb356984-f7dd-4472-98fe-e15f8d08c73c","resolution":{"observed_at":"2026-08-16T12:24:51.618471Z","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":"2026-08-16T12:24:51.622806Z","title":null,"venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.622806Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:e32124e2555a142ce8b7a92b4689881ebe14484c7d3f4b45b7ed61536c5802bc","observation_id":"cf105082-0072-492c-ae82-c92f808c975e","resolution":{"observed_at":"2026-08-16T12:24:51.622806Z","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":"2026-08-16T12:24:52.254644Z","title":"Israel, Thermo-field dynamics of black holes, Physics Letters A 57, 107 (1976)","venue":null,"work_id":"372476f8-19d0-4e73-8add-5b8211cff16e","year":1976},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.626199Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:817ce9065ff8703d239006b5fca78e766df71b274c2d626bd82224de73b3bf0c","observation_id":"7abfb437-4e40-4627-aff5-9dffd306ee24","resolution":{"observed_at":"2026-08-16T12:24:52.258668Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.245130Z","title":"Moretti and N","venue":null,"work_id":"72ac54db-4786-4684-ad71-bf44cf2c7928","year":2012},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.630208Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:748c9dbb747e48e3003cd82a8884c0e554e2918809e185e0eb2b1ff4265e16a3","observation_id":"9ac87f35-2c1c-4635-8a37-dfe630c801fd","resolution":{"observed_at":"2026-08-16T12:24:52.248476Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.234928Z","title":"H¨ ormander,The analysis of linear partial differential operators I: Distribution Theory and Fourier Analysis (Springer Science & Business Media, 2002)","venue":null,"work_id":"7a99acd6-c0cf-4a40-90a4-9a8a43853f4b","year":2002},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.633538Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:34ffbe27ec31be1fb4401570cf6bea03996066634cd095141f6f5ed6808357e0","observation_id":"e4c374ab-a86e-4490-aca3-fe45bd99a23f","resolution":{"observed_at":"2026-08-16T12:24:52.238604Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.224472Z","title":"Cropp, S","venue":null,"work_id":"ab94e31e-603e-4f89-b5d9-db86b55aa7f7","year":2013},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.636808Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:ec63a60360ae7610f8357b1083b2e5ee28a5347732d126fb185262da2942fdb4","observation_id":"be04d586-3ce5-4c83-83bb-802d3edec34b","resolution":{"observed_at":"2026-08-16T12:24:52.227788Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.214348Z","title":"Fabbri, Scattering and absorption of electromagnetic waves by a Schwarzschild black hole, Phys","venue":null,"work_id":"01fabcd1-94b0-4b64-93b2-2030dd7fc2d5","year":1975},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.640090Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:eaa88ba460903141e3198da399c320a194c0680c7f0a0d33eaa30ce996b08d45","observation_id":"cb5f862e-929a-488c-a3c2-104582a5c5a1","resolution":{"observed_at":"2026-08-16T12:24:52.217877Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.10333","last_updated":"2019-07-12T15:48:14Z","snapshot_observed_at":"2026-08-14T16:42:40.866420Z","submitted_at":"2019-04-23T13:55:18Z","title":"Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.10333","snapshot_observed_at":"2026-08-16T12:24:51.643627Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.643627Z"},"links":{"cited_paper":"/paper/1904.10333","citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:a5e795f1615ded3a0a6efeebf9225a71c2734e9668bd8b6d319aef1ce4f530cd","observation_id":"8685cf15-35ff-41a4-a126-868afdec277e","resolution":{"observed_at":"2026-08-16T12:24:51.643627Z","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":"2026-08-16T12:24:52.204156Z","title":null,"venue":null,"work_id":"7efd163e-dc96-429f-9865-a3b918fd485c","year":1991},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.647306Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:b340dd9c5f426c486a4e227146665f490c3438526331a03d760b35c35ad97063","observation_id":"2d3f5c3a-2bf8-4b5e-af21-53d0ff5f8789","resolution":{"observed_at":"2026-08-16T12:24:52.208007Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.194467Z","title":"Lazard, Solving quintics by radicals, The Legacy of Niels Henrik Abel: The Abel Bicentennial, Oslo, 2002 , 207 (2004)","venue":null,"work_id":"83b533c7-6d33-40c4-a6dd-f1ad81857400","year":2004},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.650960Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:c11cdfda47c0f7d045e76bc11287a536f296c1c352037b88d3f91a0f6402b15b","observation_id":"c116c3aa-06cd-43ef-b458-a4651b5e5f46","resolution":{"observed_at":"2026-08-16T12:24:52.197933Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:52.184500Z","title":null,"venue":null,"work_id":"0bef7233-87cf-4041-8397-c0e3e11fcb7c","year":1985},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.654474Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:85763856f5ad6b1e7d67f689e42b9171a9e739b45a77a660cadcadcec2b63b2a","observation_id":"5dac5634-2207-4131-b5ea-64d043f909c8","resolution":{"observed_at":"2026-08-16T12:24:52.187959Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+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":"2026-08-16T12:24:51.658323Z","title":"Iyer and C","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.658323Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:443d28160cb1c25dd7869e8a9ad0af859587c0e6910fad848f092e067d3a0607","observation_id":"da352ff0-e1de-4f13-9355-af72777b7462","resolution":{"observed_at":"2026-08-16T12:24:51.658323Z","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":"2026-08-16T12:24:52.169448Z","title":"Carballo-Rubio, F","venue":null,"work_id":"0792c233-66b1-46c7-a5ce-f50a7ee30382","year":2020},"citing_paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-16T12:24:51.661934Z"},"links":{"citing_paper":"/paper/2504.13050"},"observation_digest":"sha256:a856c0558abcdd738b80463e1bb5bf5437b4da9d54ce9931113237a3f9afd25c","observation_id":"d8d701cf-67c5-40cf-8397-26c302e638b3","resolution":{"observed_at":"2026-08-16T12:24:52.172653Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2504.13050","last_updated":"2025-07-22T15:16:28Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T12:27:45.453570Z","submitted_at":"2025-04-17T16:07:11Z","title":"Radiative properties of a nonsingular black hole: Hawking radiation and gray-body factor"},"reference_resolution":{"displayed":83,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":60,"verified_exact":5,"verified_fuzzy":18},"total_outbound_references":83},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 83 of 83 outbound references and 1 inbound Pith citation observation for arXiv:2504.13050."}