{"as_of":"2026-08-17T04:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:654ae37b5c43b541a74a8a209ce837717afb97adc7b5f052cd87d2b22807185b","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":"2026-08-16T06:30:59.297886+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":"2026-08-16T05:23:57.741491Z","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":"sha256:7df98b1d14095a784d576d43967a29cf7e21944b91f2adb0f9722c7bad2ab237","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":"2026-08-16T05:23:57.741491Z","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":"sha256:3bcff513466c2d4d730adfd126148bb7a255149265c7cb9e8a890ec1976a79fd","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":"2026-08-16T05:23:57.741491Z","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":"sha256:0e5fa17a808d1121cbfe1e87b7905b0f1c09b9c5ef2528db7396a37108040b62","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":"2026-08-16T05:23:57.741491Z","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:fd8a0b10b47caa059471f454ab7b188e13fbbb7848d648d6b072afa3c166a8c7","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":"2026-08-16T05:23:57.741491Z","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":"sha256:7acf136eddd97aee232b6b17493ef80cc644ae7e683709886c4294e95fec0072","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":"2026-08-16T05:23:57.741491Z","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:dbbae9d4ed8f9e846ca8d4310307a6d1907948a011cb55d106c8795b018ad9c7","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":"2026-08-16T05:23:57.741491Z","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":"sha256:56ffa5b29f40a940892b541cc087a490a655d14be82929f28f1db6bcb08d1155","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":"2026-08-16T05:23:57.741491Z","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:c1cd20bb319e1aba814e1585840e87d6cf05055aa1d86ab016e2d94de0dd7604","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":"2026-08-16T05:23:57.741491Z","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":"sha256:8cd277405d3ccc89037020cefc3d4a3959fb7dac898cca715ec11a25a523162c","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":"2026-08-16T05:23:57.741491Z","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":"sha256:64970e890a4fdbf6fd35e941418afd6c7dc51d2d9af5ca2b335025bf6115d42d","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":"2026-08-16T05:23:57.741491Z","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":"sha256:53f1a772c05fd8c947e568daed1eb068c477baa440bac80afff6b4fd41614e08","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"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":"2026-08-16T05:23:57.741491Z","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:cc05c431a9d2bb6c15918d847fe212e4911e9a797a7f1507fd7c73b28365a6d0","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":"2026-08-16T05:23:57.741491Z","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":"sha256:5861ff44b98822c2652a44462916e4dcaf3e24c57fea2051592d0a38982e7962","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":"2026-08-16T05:23:57.741491Z","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":"sha256:325de73f257284754ca6529b9f60c0156040da8bc59e5657e8d0b2f0133008e3","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":"2026-08-16T05:23:57.741491Z","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":"sha256:30a3801359984a9409e3f719a2b25fa347a2200817ff5c70a2a108b50013e0ac","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":"2026-08-15T04:11:08.258092Z","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":"2026-08-16T05:23:57.741491Z","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:cc3e278b92e746d32664424abb499f55a07e06e1fd8e73d5ed13859885b6985f","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T05:34:14.834923Z","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":"2026-08-16T05:23:57.741491Z","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:d567dfcda100285fe83a22968c258d99354db04b21eb37fb07836606045c476c","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":"2026-08-16T05:23:57.741491Z","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":"sha256:15960d456e5f12ada090cafffae7a64510b16988d396653ea0f49eeb1002bf3d","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":"2026-08-16T05:23:57.741491Z","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":"sha256:3f1d05847f1ca340ee9b6d5726d88aefeb4978fa6c99d6c7a303eb8c70d79eb6","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":"2026-08-16T05:23:57.741491Z","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":"sha256:82e014294fb31b96d9426da55927bc3a26cf06f48ba9c51a313e4cf4026c4787","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":"2026-08-16T17:16:29.604970Z","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":"2026-08-16T05:23:57.741491Z","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":"sha256:91288832cbff70fe11d6721d9ea60b69b227721b7c2f0d96a261f2f4bc97c1e7","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":"2026-08-16T05:23:57.741491Z","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":"sha256:2409fb5763e1f8d8914150f14c427225123ef4dd635b91cf5a7f2c29aa009ecd","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"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":"2026-08-16T05:23:57.741491Z","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:e3eb161aa357803b6a6428762727713b958fb2cace36011740bf22b7582bcaa8","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"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":"2026-08-16T05:23:57.741491Z","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":"sha256:51316385d2c459fc6057fcecc0f7c9b1da125b47bf63f903a1fc359c9fdea260","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":"2026-08-16T05:23:57.741491Z","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":"sha256:2b4bfd448f1cacd1a8f39686253aef098932c481f86fc502d1b52a78491e0f7e","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":"2026-08-16T17:18:33.454982Z","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":"2026-08-16T05:23:57.741491Z","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":"sha256:6b5cffebabdd06fe8f38cfcbbd1b07bac50770c318bcce115fc452998a53ed51","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T05:34:14.912567Z","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":"2026-08-16T05:23:57.741491Z","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":"sha256:7fe534403f516ab49741bd5ea10118a7951c1262a31463bf7ba60c3917dd0895","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":"2026-08-16T05:23:57.741491Z","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":"sha256:8fb8041b49353bd4cce326418eb65be6221e0c555368c09e07c924adfbc83559","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.15164","last_updated":"2024-11-12T11:46:41Z","snapshot_observed_at":"2026-08-16T13:00:50.849820Z","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":"2026-08-16T05:23:57.741491Z","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":"sha256:56d6277065f8ada7156c644666df2dd6a8ece90a597dc2ef31f31691574a4c17","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":"2026-07-06T09:24:45.369211Z","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":"2026-08-16T05:23:57.741491Z","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":"sha256:122bd5821237d64550d29529e786c81251d3b3d5ef5df3fb50ab94339590bdc1","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"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":"2026-08-16T05:23:57.741491Z","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":"sha256:96ed41b61fd95d05d6eab59b36f015dfe72181a24e0077c15fad786c4cd8dc05","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T05:34:14.954293Z","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":"2026-08-16T05:23:57.741491Z","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:cbbb2dae354995259757215c57dff30b4c02710113d98532c2dc14c3d4330517","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":"2026-08-16T05:23:57.741491Z","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":"sha256:4e8b4642de546aac70ad31062b20f8d4bd637f90dc34c67e70bfbf88815f4e71","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/978-1-4757-5426-1_5","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T05:34:15.025262Z","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":"2026-08-16T05:23:57.741491Z","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:f10118560b715d37b2e97b475b059570191b94c90d0b9b3067b54ad3a5bcd1cd","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 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2505.00732","last_updated":"2025-04-29T08:14:12Z","latest_version":1,"primary_category":"physics.gen-ph","snapshot_observed_at":"2026-08-16T05:23:57.741491Z","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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 34 of 34 outbound references and 0 inbound Pith citation observations for arXiv:2505.00732."}