{"as_of":"2026-08-20T13:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b0ae359e7fd47fe9225dd229154aa014d18b0e6a025ef110f5db9d3216ea8c58","coverage":[{"denominator":34,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":34,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:34:14.968879Z","state":"measured"},{"denominator":34,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":34,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.00732/citation-record","integrity":"/paper/2505.00732/integrity","json":"/paper/2505.00732/citation-record.json","paper":"/paper/2505.00732"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"physics/9905030","last_updated":"1999-05-12T14:01:36Z","snapshot_observed_at":"2026-07-07T06:59:25.065573Z","submitted_at":"1999-05-12T14:01:36Z","title":"On the gravitational field of a mass point according to Einstein's theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"physics/9905030","snapshot_observed_at":"2026-08-16T05:34:14.720923Z","title":"Schwarzschild, Sitzungsber","venue":null,"work_id":null,"year":1916},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.720923Z"},"links":{"cited_paper":"/paper/physics/9905030","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:664451358f8472a843e89c0a5ba62ef92cc407c72e7277864fe9a7512fbefd32","observation_id":"136991c3-8b06-44d5-aac5-858986ccc734","resolution":{"observed_at":"2026-08-16T05:34:14.720923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"physics/9912033","last_updated":"1999-12-16T18:29:12Z","snapshot_observed_at":"2026-07-07T06:59:50.808861Z","submitted_at":"1999-12-16T18:29:12Z","title":"On the gravitational field of a sphere of incompressible fluid according to Einstein's theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"physics/9912033","snapshot_observed_at":"2026-08-16T05:34:14.731929Z","title":"Schwarzschild, Sitzungsber","venue":null,"work_id":null,"year":1916},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.731929Z"},"links":{"cited_paper":"/paper/physics/9912033","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:32a7c19a5b0d07c18545a108e806c986e155157c95bcfc93985a8f1ca3ae3486","observation_id":"3948292d-b3ab-4f86-96c9-aabd1a8cb8fe","resolution":{"observed_at":"2026-08-16T05:34:14.731929Z","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":"2026-08-16T05:34:14.738883Z","title":"Penrose, Phys","venue":null,"work_id":null,"year":1965},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.738883Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:a1eb2abf7edecbe67f537bf59d7d2235df8f70642fb48365c75a909dd0870ef9","observation_id":"21a02a65-3354-4b9f-890c-34c0a3142770","resolution":{"observed_at":"2026-08-16T05:34:14.738883Z","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":"2026-08-16T05:34:14.746410Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.746410Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:362c99af6103695e7dfa5cc6687d67695ca0c42bc83234012badac90ec1fd32b","observation_id":"0bd5af50-36b8-41d6-93ff-c95132f0594f","resolution":{"observed_at":"2026-08-16T05:34:14.746410Z","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":"2026-08-16T05:34:14.753494Z","title":null,"venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.753494Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:f699913c606977bea71a4ea185925e53a8a725d3ea83476ec0ee98f1d58a9e68","observation_id":"2e07a91e-9015-43bb-bced-25a69cf08615","resolution":{"observed_at":"2026-08-16T05:34:14.753494Z","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":"2026-08-16T05:34:14.760335Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.760335Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:ba4cfb6b48939cd246af273a1b9bc07c0387f8b79c67d44ed52025be6e818c2e","observation_id":"9cb38790-d0d1-46b1-bb26-2c1573825c2a","resolution":{"observed_at":"2026-08-16T05:34:14.760335Z","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":"2026-08-16T05:34:14.767715Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.767715Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:b860ad4f11fabcb3aa67da0f7d5d850ac753bca74d7d5088e2cb0ae5b5a0582f","observation_id":"3b6cf6f6-19e2-402f-878e-1518c0f2feb7","resolution":{"observed_at":"2026-08-16T05:34:14.767715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0405231","last_updated":"2005-03-17T01:44:41Z","snapshot_observed_at":"2026-08-04T23:17:46.226034Z","submitted_at":"2004-05-26T02:04:08Z","title":"Viscosity in Strongly Interacting Quantum Field Theories from Black Hole Physics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0405231","snapshot_observed_at":"2026-08-16T05:34:14.775466Z","title":"Kovtun, D","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.775466Z"},"links":{"cited_paper":"/paper/hep-th/0405231","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:dd7135fc1ed0c8cbb8d5f00ac06c16924da2577fd0be9bb6314753c0589e98bc","observation_id":"230ba1ae-83e9-4ea9-87a1-b4a961463b81","resolution":{"observed_at":"2026-08-16T05:34:14.775466Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0109154","last_updated":"2001-09-20T22:57:38Z","snapshot_observed_at":"2026-07-07T04:41:15.266728Z","submitted_at":"2001-09-20T22:57:38Z","title":"AdS/CFT duality and the black hole information paradox","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0109154","snapshot_observed_at":"2026-08-16T05:34:14.782026Z","title":"Lunin and S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.782026Z"},"links":{"cited_paper":"/paper/hep-th/0109154","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:c4d7cdad6025cf4c459a4614cb9e57658141f921e728ba9c455ba4943add0c09","observation_id":"0d3fd9fc-0a0a-4dd6-a7b1-449749806222","resolution":{"observed_at":"2026-08-16T05:34:14.782026Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0202072","last_updated":"2002-02-12T19:04:48Z","snapshot_observed_at":"2026-08-13T15:38:18.080781Z","submitted_at":"2002-02-11T19:59:12Z","title":"Statistical interpretation of Bekenstein entropy for systems with a stretched horizon","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0202072","snapshot_observed_at":"2026-08-16T05:34:14.788006Z","title":"Lunin and S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.788006Z"},"links":{"cited_paper":"/paper/hep-th/0202072","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:ef90d1ea890869e26b9c8914c104bec1638f42d02cbb250727a5d2af15c4e90d","observation_id":"c30ebb48-0d19-4de8-ba04-dc9407e8de3f","resolution":{"observed_at":"2026-08-16T05:34:14.788006Z","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":"th/0205192","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T05:34:16.176019Z","title":null,"venue":null,"work_id":"94319891-b6e2-4f97-a1aa-7688470b59da","year":2002},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.794534Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:e066afe6dd11f81db0443bb4860af1f1d0594ab72d9797f02313ee141f5a3fae","observation_id":"bad986fb-9342-43a2-8049-247e851236b0","resolution":{"observed_at":"2026-08-16T05:34:16.191511Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0502050","last_updated":"2005-02-03T22:40:11Z","snapshot_observed_at":"2026-07-07T04:53:11.180776Z","submitted_at":"2005-02-03T22:40:11Z","title":"The fuzzball proposal for black holes: an elementary review","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0502050","snapshot_observed_at":"2026-08-16T05:34:14.801288Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.801288Z"},"links":{"cited_paper":"/paper/hep-th/0502050","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:346a750672c31675e714a35147f3cd9fa4e0923525e846c91b81bf07d07cbb06","observation_id":"219327a6-c9d5-4873-a797-905d3b2eb670","resolution":{"observed_at":"2026-08-16T05:34:14.801288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.2030","last_updated":"2008-03-13T18:52:29Z","snapshot_observed_at":"2026-08-15T10:19:36.430593Z","submitted_at":"2008-03-13T18:52:29Z","title":"What Exactly is the Information Paradox?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.2030","snapshot_observed_at":"2026-08-16T05:34:14.809788Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.809788Z"},"links":{"cited_paper":"/paper/0803.2030","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:62a2bba124e46c10d952ca28cc6b9196e1e7a7bf011c910c4139b83a3ece78e7","observation_id":"532e65e5-61e9-434d-9b65-23b1a38b092b","resolution":{"observed_at":"2026-08-16T05:34:14.809788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0810.4525","last_updated":"2008-10-24T18:57:56Z","snapshot_observed_at":"2026-08-15T10:03:34.321424Z","submitted_at":"2008-10-24T18:57:56Z","title":"Fuzzballs and the information paradox: a summary and conjectures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0810.4525","snapshot_observed_at":"2026-08-16T05:34:14.815573Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.815573Z"},"links":{"cited_paper":"/paper/0810.4525","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:0d70b0ed65c2ec259f6ba5ee6adcd3f907a5355d60c7a66fc6ea8097fee3d6b8","observation_id":"f9a80d7f-50d9-48ce-a5ab-da8d58a8bbe1","resolution":{"observed_at":"2026-08-16T05:34:14.815573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.1038","last_updated":"2011-01-25T19:57:37Z","snapshot_observed_at":"2026-08-15T05:39:47.554676Z","submitted_at":"2009-09-05T15:44:54Z","title":"The information paradox: A pedagogical introduction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.1038","snapshot_observed_at":"2026-08-16T05:34:14.822352Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.822352Z"},"links":{"cited_paper":"/paper/0909.1038","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:5a1eded90f395c54153549e5619add3b630b8573912f2320efbee551a7c9968e","observation_id":"71447f79-ce67-446c-80db-0031569940f3","resolution":{"observed_at":"2026-08-16T05:34:14.822352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.0776","last_updated":"2012-05-14T18:58:41Z","snapshot_observed_at":"2026-08-20T08:18:20.120963Z","submitted_at":"2012-05-03T17:47:04Z","title":"Black Holes and Beyond","version":2},"cited_work":{"arxiv_id":"1205.0776","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.0776","snapshot_observed_at":"2026-08-16T05:34:15.908994Z","title":"Black Holes and Beyond","venue":"hep-th","work_id":"12a66078-0dea-4a74-876f-b2affc3c322a","year":2012},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.828970Z"},"links":{"cited_paper":"/paper/1205.0776","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:c12b58bfa8b48bd6a287ac6ef25f7fca79f763d16563278c051ae5357ca7ae7b","observation_id":"37744dd6-b62c-44ad-a740-4e846156e8e7","resolution":{"observed_at":"2026-08-16T05:34:15.921450Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+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":"2026-08-16T05:34:14.834923Z","title":null,"venue":null,"work_id":null,"year":1963},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.834923Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:4289f49fe645b290e59e6ab2b0e32c7724a21de569b727a78847f0855b748457","observation_id":"3fe36de7-82ac-4704-8565-76bf4403e127","resolution":{"observed_at":"2026-08-16T05:34:14.834923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0802.0519","last_updated":"2008-02-04T23:15:27Z","snapshot_observed_at":"2026-08-15T10:22:17.005231Z","submitted_at":"2008-02-04T23:15:27Z","title":"Black Holes in Higher-Dimensional Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0802.0519","snapshot_observed_at":"2026-08-16T05:34:14.841042Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.841042Z"},"links":{"cited_paper":"/paper/0802.0519","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:02cc144a2fe3bf993a2d156440d0cfffe697fc477c3a6c74a5d77fe01d841b37","observation_id":"27bf9aa1-1d66-414e-bcba-e3a66cdf8051","resolution":{"observed_at":"2026-08-16T05:34:14.841042Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.3359","last_updated":"2011-12-14T21:10:39Z","snapshot_observed_at":"2026-08-15T04:25:33.707124Z","submitted_at":"2011-12-14T21:10:39Z","title":"Black Hole's Quantum N-Portrait","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.3359","snapshot_observed_at":"2026-08-16T05:34:14.849456Z","title":"Dvali and C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.849456Z"},"links":{"cited_paper":"/paper/1112.3359","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:460d33f7d9dd016993fa4dd570a49ca4d24e0c655f830f9ca28c8efc0a1d082d","observation_id":"37933b39-27d6-40c1-8188-071d96072e26","resolution":{"observed_at":"2026-08-16T05:34:14.849456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.3372","last_updated":"2012-03-15T14:33:52Z","snapshot_observed_at":"2026-08-15T04:16:12.554210Z","submitted_at":"2012-03-15T14:33:52Z","title":"Landau-Ginzburg Limit of Black Hole's Quantum Portrait: Self Similarity and Critical Exponent","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.3372","snapshot_observed_at":"2026-08-16T05:34:14.856103Z","title":"Dvali and C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.856103Z"},"links":{"cited_paper":"/paper/1203.3372","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:df755baf95e36f8ade6b9fdc22f3f84fa59702e3846113edd95b05489082740b","observation_id":"d1bb3fca-fde3-4620-a5ea-743d5df79d5d","resolution":{"observed_at":"2026-08-16T05:34:14.856103Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.6575","last_updated":"2012-03-29T16:21:43Z","snapshot_observed_at":"2026-08-19T03:07:08.014127Z","submitted_at":"2012-03-29T16:21:43Z","title":"Black Hole's 1/N Hair","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1203.6575","snapshot_observed_at":"2026-08-16T05:34:14.871360Z","title":"Dvali and C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.871360Z"},"links":{"cited_paper":"/paper/1203.6575","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:bdcb5369b8b1dea65c28bff36cc1504832d3deb1d24d1bf21835aa66a0994d8e","observation_id":"ebfddc27-d7da-4108-aa80-fcb7c02e88d8","resolution":{"observed_at":"2026-08-16T05:34:14.871360Z","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":"10.1140/epjc/s10052-014-2752-3","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T05:34:15.118837Z","title":"Dvali and C","venue":null,"work_id":"37916011-3050-4b4f-b47b-22539e3a06ec","year":2014},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.878390Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:94c3b84e87a5d23c2b7837eb6c464c91952203e5328c84c3e1c5d4ddade3e25d","observation_id":"86dd87a9-27f0-462b-ae3b-5236dd1c5eeb","resolution":{"observed_at":"2026-08-16T05:34:15.131534Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.03209","last_updated":"2018-11-08T01:25:27Z","snapshot_observed_at":"2026-08-14T18:02:27.864747Z","submitted_at":"2018-11-08T01:25:27Z","title":"Bosons falling into a black hole: A superfluid analogue","version":1},"cited_work":{"arxiv_id":"1811.03209","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.03209","snapshot_observed_at":"2026-08-16T05:34:15.693872Z","title":"Bosons falling into a black hole: A superfluid analogue","venue":"gr-qc","work_id":"b35a80f5-2dee-42d3-b5cb-28d7fcddca29","year":2018},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.887880Z"},"links":{"cited_paper":"/paper/1811.03209","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:65c1befa1903c48de9b5d873d17b54434f44a128f7da8e3a205566d51c676498","observation_id":"0c37e318-a1ae-48cf-bc87-ac333489d3b8","resolution":{"observed_at":"2026-08-16T05:34:15.705514Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0708.4025","last_updated":"2007-09-21T15:23:15Z","snapshot_observed_at":"2026-08-15T10:33:22.671641Z","submitted_at":"2007-08-29T22:35:15Z","title":"Black holes as mirrors: quantum information in random subsystems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0708.4025","snapshot_observed_at":"2026-08-16T05:34:14.894790Z","title":"Hayden and J","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.894790Z"},"links":{"cited_paper":"/paper/0708.4025","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:17a9fbba74a4bf57628b8324f8ae9785526b61407f6673a3f3d4f04da429ea48","observation_id":"c1ce5afc-fb94-46e5-af27-2eccf3dfb0f7","resolution":{"observed_at":"2026-08-16T05:34:14.894790Z","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":"2026-08-16T05:34:14.901301Z","title":null,"venue":null,"work_id":null,"year":1976},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.901301Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:e2d3768b1412c13101ac90f4324620b143837c2aede2ead7261d4059f0430751","observation_id":"5dfd5f93-71dd-4867-96c0-b7cf05c3027d","resolution":{"observed_at":"2026-08-16T05:34:14.901301Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.18086","last_updated":"2025-03-23T14:34:55Z","snapshot_observed_at":"2026-08-19T15:55:03.996730Z","submitted_at":"2025-03-23T14:34:55Z","title":"The Stochastic Mechanics of Hawking Radiation","version":1},"cited_work":{"arxiv_id":"2503.18086","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.18086","snapshot_observed_at":"2026-08-16T05:34:15.614515Z","title":"The Stochastic Mechanics of Hawking Radiation","venue":"gr-qc","work_id":"e285f63d-c071-4ee0-82e7-1a0cb625dd06","year":2025},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.906536Z"},"links":{"cited_paper":"/paper/2503.18086","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:7ff6a815616e03a8436e7ebd47974f268addf824baebc969a2ac66251104f7f1","observation_id":"ecd40173-767b-4d8d-af5a-5a1ad593f73a","resolution":{"observed_at":"2026-08-16T05:34:15.621927Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+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":"2026-08-16T05:34:14.912567Z","title":null,"venue":null,"work_id":null,"year":1959},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.912567Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:1edd629534227c99f66ce4188788e9214d8c3dc9f2ba3481ad21dc3fd6a1d4e4","observation_id":"74c18ff5-889c-4f11-8d1b-b40b1ab0f2a7","resolution":{"observed_at":"2026-08-16T05:34:14.912567Z","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":"2026-08-16T05:34:16.436231Z","title":null,"venue":null,"work_id":"69e66ec1-bfae-40de-b928-44214dc2fc42","year":null},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.919107Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:e20c29d8528cb080e429bce1a319dc9f790bc4321b13ae2c49276c8be693d745","observation_id":"c00a0765-bc84-4322-b1d2-a0ec01040195","resolution":{"observed_at":"2026-08-16T05:34:16.445346Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.15164","last_updated":"2024-11-12T11:46:41Z","snapshot_observed_at":"2026-08-19T17:18:24.406386Z","submitted_at":"2024-11-12T11:46:41Z","title":"The Modification of Feynman Diagrams in Curved Space-Time","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.15164","snapshot_observed_at":"2026-08-16T05:34:14.928036Z","title":"Li, [arXiv:2411.15164 [physics.gen-ph]]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.928036Z"},"links":{"cited_paper":"/paper/2411.15164","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:92959895c4e73811cddf99ab0eb3e152f177102103e927b14969083077d195e5","observation_id":"08e25f24-192f-4f13-8934-b60e57db131c","resolution":{"observed_at":"2026-08-16T05:34:14.928036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.00433","last_updated":"2020-08-11T07:28:53Z","snapshot_observed_at":"2026-08-20T09:04:03.873766Z","submitted_at":"2020-05-31T04:31:00Z","title":"The nonequilibrium back-reaction of Hawking radiation to a Schwarzschild black hole","version":2},"cited_work":{"arxiv_id":"2006.00433","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.00433","snapshot_observed_at":"2026-08-16T05:34:15.545243Z","title":"The nonequilibrium back-reaction of Hawking radiation to a Schwarzschild black hole","venue":"hep-th","work_id":"f85f5554-d9b0-4d3c-9616-d72e3b50b43e","year":2020},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.939720Z"},"links":{"cited_paper":"/paper/2006.00433","citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:2c922c8f82817c719a277b6180252dccd17948b0ec4b4e3906864520a2599eef","observation_id":"c80c1370-f5f6-49b7-be31-3bad6fd94bbf","resolution":{"observed_at":"2026-08-16T05:34:15.552122Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2502.08816","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T05:34:15.464561Z","title":null,"venue":null,"work_id":"4f8d6338-f6b9-4b91-8988-20641eaefa28","year":null},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.945696Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:97a6422e85d8b0da1915e522c306f9ccb92c437dee2a05d94d4945ea97b5daaf","observation_id":"5a80e5b2-324f-4559-9d6c-6851d7905eab","resolution":{"observed_at":"2026-08-16T05:34:15.484925Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+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":"2026-08-16T05:34:14.954293Z","title":null,"venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.954293Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:938d10d65dd8e3440f8fc972c8d0a1a8088a4fb63cbbc8a30e1f10218c73a47d","observation_id":"174ae986-4e5d-4b07-84eb-7230a0086470","resolution":{"observed_at":"2026-08-16T05:34:14.954293Z","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":"2026-08-16T05:34:16.410510Z","title":"Earthquakes, Starquakes, and Solar Flares","venue":null,"work_id":"3227fef7-04fb-4bcf-9013-03e5b5cf606c","year":null},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.961221Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:4a3500368f341e2efc6f12b35d4bcbb690cd04bb6e3562ea772c320c0983d1eb","observation_id":"ba998bee-540a-4857-be8b-0c21ab4fcdc6","resolution":{"observed_at":"2026-08-16T05:34:16.420445Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/978-1-4757-5426-1_5","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-17T11:03:46.409680Z","title":null,"venue":null,"work_id":"10761c8d-8d03-4960-b2b6-ab90d7271029","year":null},"citing_paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole","version":1},"reference_index":1996,"source":"pdf_text","source_observed_at":"2026-08-16T05:34:14.968879Z"},"links":{"citing_paper":"/paper/2505.00732"},"observation_digest":"sha256:7b7368635ad0707457e8ed582b11341097821ae6befa19be1108323614be4b80","observation_id":"f7df38f0-9961-4091-9b0b-0e698ff90774","resolution":{"observed_at":"2026-08-16T05:34:15.034173Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","latest_version":1,"primary_category":"physics.gen-ph","snapshot_observed_at":"2026-08-19T19:57:10.229702Z","submitted_at":"2025-04-29T08:14:12Z","title":"A Holographic, Hydrodynamic Model of a Schwarzschild Black Hole"},"reference_resolution":{"displayed":34,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":25,"verified_exact":8,"verified_fuzzy":1},"total_outbound_references":34},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 34 of 34 outbound references and 0 inbound Pith citation observations for arXiv:2505.00732."}