{"as_of":"2026-08-20T00:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:741e13f9f2f9ef0deda2d0182a9978c9e7f35a35731a94bebcb82d96dc13ef57","coverage":[{"denominator":50,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":50,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:28:33.393428Z","state":"measured"},{"denominator":51,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":51,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+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":"2026-08-14T05:09:13.359340Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-14T05:09:14.292977Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"cited_work":{"arxiv_id":"1908.09074","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.09074","snapshot_observed_at":"2026-08-14T05:09:14.292977Z","title":"Embedding into flat spacetime and black hole thermodynamics","venue":"gr-qc","work_id":"418811da-84f7-4f5b-a61a-d00b85453464","year":2019},"citing_paper":{"arxiv_id":"1909.02015","last_updated":"2019-09-04T18:00:04Z","snapshot_observed_at":"2026-08-17T13:34:11.968290Z","submitted_at":"2019-09-04T18:00:04Z","title":"Gravity and Quantum Theory: Domains of Conflict and Contact","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T05:09:13.359340Z"},"links":{"cited_paper":"/paper/1908.09074","citing_paper":"/paper/1909.02015"},"observation_digest":"sha256:ea7d1a0557f289300597f983c3363cf0b7feba2f6e983bdd81bf9441fe0ffe7f","observation_id":"87b903be-47e4-47a6-90ee-f39eb2325c06","resolution":{"observed_at":"2026-08-14T05:09:14.296963Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1908.09074/citation-record","integrity":"/paper/1908.09074/integrity","json":"/paper/1908.09074/citation-record.json","paper":"/paper/1908.09074"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-08-14T11:28:32.351694Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.351694Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:cb1aacedf3cc3d6137b5a5de585b561fcc8d029781770d3a9e739e86dc563130","observation_id":"ab4bb1db-714a-4a52-9792-f14509da1987","resolution":{"observed_at":"2026-08-14T11:28:32.351694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03841","last_updated":"2018-10-23T15:08:45Z","snapshot_observed_at":"2026-08-14T22:10:41.610545Z","submitted_at":"2016-02-11T19:26:48Z","title":"Tests of general relativity with GW150914","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03841","snapshot_observed_at":"2026-08-14T11:28:32.446075Z","title":"Tests of general relativity with GW150914,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.446075Z"},"links":{"cited_paper":"/paper/1602.03841","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:428626b70a25d4f7c21600908474f14bb309e4239a35c738c130c8740b16ae9c","observation_id":"503892f2-5ff1-4024-a8f8-ce8e2a045435","resolution":{"observed_at":"2026-08-14T11:28:32.446075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11238","last_updated":"2019-06-26T18:06:46Z","snapshot_observed_at":"2026-08-13T13:53:05.353909Z","submitted_at":"2019-06-26T18:06:46Z","title":"First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11238","snapshot_observed_at":"2026-08-14T11:28:32.505680Z","title":"First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.505680Z"},"links":{"cited_paper":"/paper/1906.11238","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:b6f605cf94a7b8df79b7588f2826d900f5e4754cf9b6a3ccb038df0c054fb6cc","observation_id":"1a4831f9-3988-46b6-92d6-fedf2b08f2a9","resolution":{"observed_at":"2026-08-14T11:28:32.505680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.11243","last_updated":"2019-06-26T18:06:51Z","snapshot_observed_at":"2026-07-06T08:03:03.170900Z","submitted_at":"2019-06-26T18:06:51Z","title":"First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.11243","snapshot_observed_at":"2026-08-14T11:28:32.510861Z","title":"First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.510861Z"},"links":{"cited_paper":"/paper/1906.11243","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:8cfedd62d2c3cf433175c583adaebf7fa6eaa56c255fd0661a6360025c436c0b","observation_id":"43acfc5e-9a75-46c5-b902-cbca2d5cbc30","resolution":{"observed_at":"2026-08-14T11:28:32.510861Z","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":"2026-08-14T11:28:34.697429Z","title":"Black holes and the second law,","venue":null,"work_id":"1ea10bf5-7c0a-4968-870a-7e1e4f3f8f2d","year":1972},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.515940Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:a6bd292d208f34ba3e8455d6c17ecaf518bc4521152a1c877f6a5d88772bce23","observation_id":"03db2853-62ef-486c-a78e-dfae36853204","resolution":{"observed_at":"2026-08-14T11:28:34.702170Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-14T11:28:34.594217Z","title":"Black holes and entropy,","venue":null,"work_id":"42e9d57b-c69e-44e6-9427-477ec53b5d5f","year":1973},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.520857Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:9d49a36b1423f479116cef97fd9366dbffec4bbe76d3ef9152930017090a28a5","observation_id":"f4c61c86-2087-434f-ae98-616331665760","resolution":{"observed_at":"2026-08-14T11:28:34.648072Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-14T11:28:34.540937Z","title":"Particle Creation by Black Holes,","venue":null,"work_id":"abb60dd8-496c-4398-b3de-37f0331a3681","year":1975},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.526170Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:1b793c8c6de663614969ccb6a01f737d139838f10a42d4e5933ad7488146de06","observation_id":"66f9b554-08a4-4a48-8013-c779c0547b8f","resolution":{"observed_at":"2026-08-14T11:28:34.545992Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-14T11:28:34.525469Z","title":"Scalar particle production in Schwarzschild and Rindler metrics,","venue":null,"work_id":"98880631-3851-4fcf-b881-f6f9331252dc","year":1975},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.530685Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:971f0f4eeaa78ad882455db8bd43ec630605317419f4d4e36cc8510980ee4a5e","observation_id":"c3cda9f4-2237-4c49-91ea-2419271b05cb","resolution":{"observed_at":"2026-08-14T11:28:34.530403Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-14T11:28:34.509360Z","title":"Notes on black hole evaporation,","venue":null,"work_id":"194cbc9d-aedd-4a1a-ac71-79c3b8eaaa80","year":1976},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.535269Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:6c4fff59927807d0e692be158df2f1f03cf66ebc0e2b0b52b7a0e856e8f779b6","observation_id":"0f124e60-7593-4b4e-b532-63ded4d93ad2","resolution":{"observed_at":"2026-08-14T11:28:34.514211Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-14T11:28:32.540019Z","title":"On the Quantum Structure of a Black Hole,","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.540019Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:cd955ca34917410525dcf4ee0c50a1990e125fe8670a850b6299c64bf986616a","observation_id":"9927d44c-3889-4e22-a64f-28df8ffa6dea","resolution":{"observed_at":"2026-08-14T11:28:32.540019Z","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":"2026-08-14T11:28:34.484252Z","title":"A Quantum Sour ce of Entropy for Black Holes,","venue":null,"work_id":"d50d5a28-7752-4088-b521-7903e9ffb239","year":1986},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.544730Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:ef860a76d38719ec55396786a8d538f08592b7e5a17320fb5aeb2178e9757522","observation_id":"4e6e7e1e-9541-4b38-a242-0b49d5e062ca","resolution":{"observed_at":"2026-08-14T11:28:34.489898Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9509024","last_updated":"1995-10-20T18:35:46Z","snapshot_observed_at":"2026-08-19T03:12:47.462627Z","submitted_at":"1995-09-13T17:45:20Z","title":"Statistical Mechanics and Black Hole Entropy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9509024","snapshot_observed_at":"2026-08-14T11:28:32.549581Z","title":"Statistical mechanics and black hole entropy,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.549581Z"},"links":{"cited_paper":"/paper/gr-qc/9509024","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:fb8e7fe05dd535400fd01e2b2efd2d43c2a20ef23d7faf165f4aea25113ff0f9","observation_id":"8c547ca9-144e-4234-9e86-1eb3a52b3450","resolution":{"observed_at":"2026-08-14T11:28:32.549581Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0002040","last_updated":"2000-06-14T14:21:37Z","snapshot_observed_at":"2026-08-19T22:57:34.701025Z","submitted_at":"2000-02-10T14:33:39Z","title":"Logarithmic correction to the Bekenstein-Hawking entropy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0002040","snapshot_observed_at":"2026-08-14T11:28:32.554561Z","title":"Logarithmic correction to the Be kenstein-Hawking entropy,","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.554561Z"},"links":{"cited_paper":"/paper/gr-qc/0002040","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:8161273b6713f72bcd3c36fb497624b6f2279a6527c241ed6ee0be4b875006b5","observation_id":"769e9bec-2696-45fd-b106-377acc89b320","resolution":{"observed_at":"2026-08-14T11:28:32.554561Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9307038","last_updated":"1993-07-29T16:37:13Z","snapshot_observed_at":"2026-07-07T03:24:21.295752Z","submitted_at":"1993-07-29T16:37:13Z","title":"Black Hole Entropy is Noether Charge","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9307038","snapshot_observed_at":"2026-08-14T11:28:32.559279Z","title":"Black hole entropy is the Noether charge,","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.559279Z"},"links":{"cited_paper":"/paper/gr-qc/9307038","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:c211ba5da5454f12543d9db9c4ae32bff30ded96df03ed7f17513e4aa0c48db2","observation_id":"f276d9bb-fc64-4f14-9e3a-d0c314e6b73a","resolution":{"observed_at":"2026-08-14T11:28:32.559279Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9403028","last_updated":"1994-03-15T18:18:00Z","snapshot_observed_at":"2026-08-08T08:03:16.411862Z","submitted_at":"1994-03-15T18:18:00Z","title":"Some Properties of Noether Charge and a Proposal for Dynamical Black Hole Entropy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9403028","snapshot_observed_at":"2026-08-14T11:28:32.563379Z","title":"Some properties of Noether charge an d a proposal for dynamical black hole entropy,","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.563379Z"},"links":{"cited_paper":"/paper/gr-qc/9403028","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:3cb9a1af7ef9461343320e784883855e5608e0b124d8fca84bfcad329f4b3416","observation_id":"028bed04-72b3-4671-a727-b84d216ad7a1","resolution":{"observed_at":"2026-08-14T11:28:32.563379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9305016","last_updated":"1993-05-06T01:16:00Z","snapshot_observed_at":"2026-07-07T05:03:04.481102Z","submitted_at":"1993-05-06T01:16:00Z","title":"Entropy of Lovelock Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9305016","snapshot_observed_at":"2026-08-14T11:28:32.567810Z","title":"Black hole entropy and higher cu rvature interactions,","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.567810Z"},"links":{"cited_paper":"/paper/hep-th/9305016","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:89cb3a7939b3b5805a5d40f8f501231bc4caf11917e99f203dd9f5856603724e","observation_id":"37087aa6-1314-4798-a90c-0de4ef4ce88d","resolution":{"observed_at":"2026-08-14T11:28:32.567810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.05840","last_updated":"2018-11-01T03:49:08Z","snapshot_observed_at":"2026-08-16T08:39:34.392557Z","submitted_at":"2018-06-15T07:39:07Z","title":"Noether Current, Black Hole Entropy and Spacetime Torsion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.05840","snapshot_observed_at":"2026-08-14T11:28:32.572296Z","title":"Noether Current, Black Hole Ent ropy and Spacetime Torsion,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.572296Z"},"links":{"cited_paper":"/paper/1806.05840","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:2d8a4b967b361a1e2e601b0e69b7c7a3464f3cdd5297ce2a07b35d209ceb8cda","observation_id":"8a88953a-d0f8-4155-a22c-bf2102713d7c","resolution":{"observed_at":"2026-08-14T11:28:32.572296Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.3253","last_updated":"2014-10-30T15:56:30Z","snapshot_observed_at":"2026-08-16T02:47:44.284897Z","submitted_at":"2013-12-11T17:27:27Z","title":"General Relativity from a Thermodynamic Perspective","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.3253","snapshot_observed_at":"2026-08-14T11:28:32.577110Z","title":"General Relativity from a Thermodynamic Pe rspective,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.577110Z"},"links":{"cited_paper":"/paper/1312.3253","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:c0b8f84614e0e2a41fc0c9937ef204a4c97a299320b93b5554e13b1203fbbcd0","observation_id":"fc8c01b1-f71d-43bd-8cc7-b9dad321b245","resolution":{"observed_at":"2026-08-14T11:28:32.577110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.07272","last_updated":"2015-08-16T09:48:14Z","snapshot_observed_at":"2026-08-19T10:53:45.735060Z","submitted_at":"2015-05-26T04:30:06Z","title":"Lanczos-Lovelock gravity from a thermodynamic perspective","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.07272","snapshot_observed_at":"2026-08-14T11:28:32.581807Z","title":"Lanczos-Lovelock gravity from a thermod ynamic perspective,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.581807Z"},"links":{"cited_paper":"/paper/1505.07272","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:66def257b550c9c9838b4b045c2305af6267cbc17383318fad9b8ecf9bc88437","observation_id":"cdecaba6-e103-4e3c-ba46-bfc28c44e826","resolution":{"observed_at":"2026-08-14T11:28:32.581807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1508.04060","last_updated":"2015-11-06T00:05:57Z","snapshot_observed_at":"2026-08-14T22:36:35.853185Z","submitted_at":"2015-08-13T20:05:43Z","title":"Thermodynamical interpretation of the geometrical variables associated with null surfaces","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.04060","snapshot_observed_at":"2026-08-14T11:28:32.586238Z","title":"Thermodynamical inte rpretation of the geometrical variables associated with null surfaces,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.586238Z"},"links":{"cited_paper":"/paper/1508.04060","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:8b3911fbd9c7b175dbcf457b42ad22589f07ce88d17de3a5e383107914d1eb38","observation_id":"3418ebdd-0ce8-4687-ae49-377d8a7e4581","resolution":{"observed_at":"2026-08-14T11:28:32.586238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05297","last_updated":"2015-10-13T13:03:21Z","snapshot_observed_at":"2026-08-15T16:29:04.776640Z","submitted_at":"2015-05-20T09:30:56Z","title":"Gravitational field equations near an arbitrary null surface expressed as a thermodynamic identity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.05297","snapshot_observed_at":"2026-08-14T11:28:32.615075Z","title":"Gravita tional ﬁeld equations near an arbitrary null surface expressed as a thermodynamic identity,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.615075Z"},"links":{"cited_paper":"/paper/1505.05297","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:99a0b089c77651938a2d66de47d9b7191b4caa0533cb57e9a4044e5964de72cf","observation_id":"4b538d00-7320-4240-a163-3049e43b5100","resolution":{"observed_at":"2026-08-14T11:28:32.615075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.5004","last_updated":"2010-01-19T17:55:15Z","snapshot_observed_at":"2026-08-15T05:32:59.678209Z","submitted_at":"2009-11-26T03:39:55Z","title":"Thermodynamical Aspects of Gravity: New insights","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.5004","snapshot_observed_at":"2026-08-14T11:28:32.650164Z","title":"Thermodynamical Aspects of Gravity: New insights,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.650164Z"},"links":{"cited_paper":"/paper/0911.5004","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:64516b9fde1616c107018dbde378a6aac7f3d512954425423387f6cedbf3ccc1","observation_id":"7021d838-f023-48d9-8d1b-7906b0be5fc1","resolution":{"observed_at":"2026-08-14T11:28:32.650164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.09053","last_updated":"2019-08-31T00:47:25Z","snapshot_observed_at":"2026-08-17T07:01:26.468595Z","submitted_at":"2019-04-19T02:45:49Z","title":"Raychaudhuri equation with zero point length","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.09053","snapshot_observed_at":"2026-08-14T11:28:32.695050Z","title":"Raychaudhuri equation with zero point length,","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.695050Z"},"links":{"cited_paper":"/paper/1904.09053","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:630cb46166618c60e7b6f8f1f2b0839872f758310e0e4267086fb36b74b2f864","observation_id":"9a48a87f-195f-459e-9f70-8a8d5eaeaef1","resolution":{"observed_at":"2026-08-14T11:28:32.695050Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9607022","last_updated":"1996-07-09T12:39:20Z","snapshot_observed_at":"2026-07-07T03:26:35.748537Z","submitted_at":"1996-07-09T12:39:20Z","title":"The scattering matrix approach for the quantum black hole, an overview","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9607022","snapshot_observed_at":"2026-08-14T11:28:32.820847Z","title":"The Scattering matrix approach for the quantum black hole: An Overview,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.820847Z"},"links":{"cited_paper":"/paper/gr-qc/9607022","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:b51c1e3a6ebaf3a43ab8b7c035f6bad50bd575ef2cf4095d70a324fa7d80c3b6","observation_id":"0999aea2-2d8c-4781-b8e9-e2f67956392c","resolution":{"observed_at":"2026-08-14T11:28:32.820847Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9504147","last_updated":"1995-05-06T16:48:59Z","snapshot_observed_at":"2026-07-07T05:08:01.388433Z","submitted_at":"1995-04-28T01:37:23Z","title":"EXTREMAL BLACK HOLES AND ELEMENTARY STRING STATES","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9504147","snapshot_observed_at":"2026-08-14T11:28:32.826304Z","title":"Extremal black holes and elementary string states,","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.826304Z"},"links":{"cited_paper":"/paper/hep-th/9504147","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:9d7bc91663f29e389fc5ab11f1a3b105d24573d27e66955c000fda4ca647bd62","observation_id":"6c382b62-c8f2-4075-a192-18704d52902e","resolution":{"observed_at":"2026-08-14T11:28:32.826304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9601029","last_updated":"1996-02-15T01:40:05Z","snapshot_observed_at":"2026-07-07T05:09:49.618578Z","submitted_at":"1996-01-09T22:20:39Z","title":"Microscopic Origin of the Bekenstein-Hawking Entropy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9601029","snapshot_observed_at":"2026-08-14T11:28:32.831567Z","title":"Microscopic origin of the Bekenste in-Hawking entropy,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.831567Z"},"links":{"cited_paper":"/paper/hep-th/9601029","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:0da3bf41ac72874044968785660a84dfc6a83d7dfa0c3e101d4f3d487976f151","observation_id":"91c87b27-e374-4902-9aa2-e04f812d461f","resolution":{"observed_at":"2026-08-14T11:28:32.831567Z","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":"2026-08-14T11:28:32.836405Z","title":"Black hole entropy from loop quantum gravity,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.836405Z"},"links":{"cited_paper":"/paper/gr-qc/9603063","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:e8a5a0a004c9b2f11e48ddd59fdf23c34a831fcdd4fc5efb46099f052302bf72","observation_id":"e325a70c-0b99-4ac2-8efa-68edb05ab0c6","resolution":{"observed_at":"2026-08-14T11:28:32.836405Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9710007","last_updated":"1997-10-01T20:43:41Z","snapshot_observed_at":"2026-07-07T03:28:00.552426Z","submitted_at":"1997-10-01T20:43:41Z","title":"Quantum Geometry and Black Hole Entropy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9710007","snapshot_observed_at":"2026-08-14T11:28:32.841214Z","title":"Quantum g eometry and black hole entropy,","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.841214Z"},"links":{"cited_paper":"/paper/gr-qc/9710007","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:bf92b5e1e4ece98819d564f4ffc911abbb17a38b3144761c814cb5f83a53ff26","observation_id":"f283446b-d203-4080-bf77-7321a66ee116","resolution":{"observed_at":"2026-08-14T11:28:32.841214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.1300","last_updated":"2013-02-06T04:17:56Z","snapshot_observed_at":"2026-08-16T08:36:46.375044Z","submitted_at":"2013-01-07T18:50:38Z","title":"Algebraic Approach to Entanglement and Entropy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1301.1300","snapshot_observed_at":"2026-08-14T11:28:32.847217Z","title":"Algebraic Approach to Entanglement and Entropy,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.847217Z"},"links":{"cited_paper":"/paper/1301.1300","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:706f25c703695d2bbdfc7fa265a437acf1591c9eb3e5e3e5fc637a615ebb55eb","observation_id":"fca47eeb-a329-4e68-a51e-937a55bc0411","resolution":{"observed_at":"2026-08-14T11:28:32.847217Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.3712","last_updated":"2011-04-19T11:50:46Z","snapshot_observed_at":"2026-08-15T04:48:57.266626Z","submitted_at":"2011-04-19T11:50:46Z","title":"Entanglement entropy of black holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.3712","snapshot_observed_at":"2026-08-14T11:28:32.852201Z","title":"Entanglement entropy of black holes,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.852201Z"},"links":{"cited_paper":"/paper/1104.3712","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:ad4112994ae23df76fb15a86251f6600e8163f0ec0dccb66121d7554f16f7134","observation_id":"cd953ad2-a9ed-49fd-882e-e8df8f467155","resolution":{"observed_at":"2026-08-14T11:28:32.852201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0802.3117","last_updated":"2008-06-25T13:41:45Z","snapshot_observed_at":"2026-08-15T10:21:12.823547Z","submitted_at":"2008-02-21T14:16:43Z","title":"Entanglement entropy, conformal invariance and extrinsic geometry","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0802.3117","snapshot_observed_at":"2026-08-14T11:28:32.857305Z","title":"Entanglement entropy, conformal invarian ce and extrinsic geometry,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.857305Z"},"links":{"cited_paper":"/paper/0802.3117","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:f5e11b402f739bd01d53b080fab0bd230cb5335f7717808cac8360b60fbe6c73","observation_id":"3856f1d7-35a3-433e-beb2-c7d427cd12a2","resolution":{"observed_at":"2026-08-14T11:28:32.857305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1102.4919","last_updated":"2011-06-27T05:21:24Z","snapshot_observed_at":"2026-08-16T01:54:21.171675Z","submitted_at":"2011-02-24T07:38:19Z","title":"Novel black hole bound states and entropy","version":3},"cited_work":{"arxiv_id":"1102.4919","doi":null,"metadata_source":"pith","pith_arxiv_id":"1102.4919","snapshot_observed_at":"2026-08-14T11:28:34.005213Z","title":"Novel black hole bound states and entropy","venue":"gr-qc","work_id":"610f41fd-97b6-4127-8498-fec48d2e75d4","year":2011},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:32.890850Z"},"links":{"cited_paper":"/paper/1102.4919","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:93ae6116e18d535f81dfcf6cf0a3005b3b4b176c9f6a5d12d1558b5ec3c5a663","observation_id":"944b141c-6c8b-4e52-b02c-e069f77dd1bd","resolution":{"observed_at":"2026-08-14T11:28:34.046482Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.05243","last_updated":"2015-08-18T05:57:06Z","snapshot_observed_at":"2026-08-16T08:41:31.383013Z","submitted_at":"2015-06-17T08:45:14Z","title":"Fermionic edge states and new physics","version":2},"cited_work":{"arxiv_id":"1506.05243","doi":null,"metadata_source":"pith","pith_arxiv_id":"1506.05243","snapshot_observed_at":"2026-08-14T11:28:33.981434Z","title":"Fermionic edge states and new physics","venue":"hep-th","work_id":"7263ea79-707e-4d50-9cd3-0ed46af0727a","year":2015},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.001494Z"},"links":{"cited_paper":"/paper/1506.05243","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:f330633fa137806c176d25e6db7929bc9f399ba4e4593e3fb14be4356741391a","observation_id":"a1001b96-05a3-4d6a-8d1f-d7ae8101d252","resolution":{"observed_at":"2026-08-14T11:28:33.987305Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1310.2034","last_updated":"2013-12-19T07:03:50Z","snapshot_observed_at":"2026-08-18T15:15:48.913516Z","submitted_at":"2013-10-08T08:21:11Z","title":"Quantum field theories with boundaries and novel instabilities","version":2},"cited_work":{"arxiv_id":"1310.2034","doi":null,"metadata_source":"pith","pith_arxiv_id":"1310.2034","snapshot_observed_at":"2026-08-14T11:28:33.960060Z","title":"Quantum field theories with boundaries and novel instabilities","venue":"hep-th","work_id":"25a33aec-3824-48b8-a62b-f1b296523903","year":2013},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.007213Z"},"links":{"cited_paper":"/paper/1310.2034","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:f045e206d664ad43f6f8f202b6eb996d3fddd05cbb1281a4f468962bef479aae","observation_id":"d73ad7ac-bc4d-4989-9931-f7107a85827e","resolution":{"observed_at":"2026-08-14T11:28:33.964530Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9706018","last_updated":"1997-06-06T19:45:44Z","snapshot_observed_at":"2026-07-07T03:27:40.597385Z","submitted_at":"1997-06-06T19:45:44Z","title":"Accelerated Detectors and Temperature in (Anti) de Sitter Spaces","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9706018","snapshot_observed_at":"2026-08-14T11:28:33.012830Z","title":"Accelerated detectors and temperat ure in (anti)-de Sitter spaces,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.012830Z"},"links":{"cited_paper":"/paper/gr-qc/9706018","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:591ac3e15e1742d6c596361800921ec48461f7912fa1f27db854bd6541d4850c","observation_id":"63c301cb-82d1-4579-b9f0-3dbe801e34ed","resolution":{"observed_at":"2026-08-14T11:28:33.012830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9709048","last_updated":"1997-09-18T21:43:46Z","snapshot_observed_at":"2026-08-19T03:11:05.578482Z","submitted_at":"1997-09-18T21:43:46Z","title":"Comment on \"Accelerated Detectors and Temperature in (Anti) de Sitter Spaces\"","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9709048","snapshot_observed_at":"2026-08-14T11:28:33.017104Z","title":"Comment on ‘Accelerated detectors and tempe rature in anti-de Sitter spaces’,","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.017104Z"},"links":{"cited_paper":"/paper/gr-qc/9709048","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:657f37f5d6409ab3dd334f0b726572fddd674b75754ba13804d809ea34f42b92","observation_id":"a0abb2f7-1497-4245-9a88-0c84656d84e1","resolution":{"observed_at":"2026-08-14T11:28:33.017104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9809159","last_updated":"1998-09-21T17:41:37Z","snapshot_observed_at":"2026-08-05T03:34:03.273278Z","submitted_at":"1998-09-21T17:41:37Z","title":"Mapping Hawking into Unruh Thermal Properties","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9809159","snapshot_observed_at":"2026-08-14T11:28:33.021680Z","title":"Mapping Hawking into Unruh thermal pro perties,","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.021680Z"},"links":{"cited_paper":"/paper/hep-th/9809159","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:dd96b470cadca2dc24238dce45caf26d6359d335ac8fe93719c02e92b687a2dd","observation_id":"0abc612d-f775-468c-9403-629191ae6e95","resolution":{"observed_at":"2026-08-14T11:28:33.021680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0202078","last_updated":"2002-02-21T16:05:25Z","snapshot_observed_at":"2026-08-19T23:37:08.714699Z","submitted_at":"2002-02-21T16:05:25Z","title":"Thermodynamics and/of Horizons: A Comparison of Schwarzschild,RINDLER and desitter Spacetimes","version":1},"cited_work":{"arxiv_id":"gr-qc/0202078","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0202078","snapshot_observed_at":"2026-08-14T11:28:33.892904Z","title":"Thermodynamics and/of Horizons: A Comparison of Schwarzschild,RINDLER and desitter Spacetimes","venue":"gr-qc","work_id":"a5dd2e25-2c84-43b3-b35d-59bccdce5352","year":2002},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.026906Z"},"links":{"cited_paper":"/paper/gr-qc/0202078","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:cc48c021db96c34ebd832b564bb26b2b2fc6f3b289be6eea19c36f5e40dd4c6d","observation_id":"4afe8c58-542f-4e8a-9051-2446db82324a","resolution":{"observed_at":"2026-08-14T11:28:33.897987Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1002.0985","last_updated":"2010-05-03T09:00:13Z","snapshot_observed_at":"2026-08-15T05:27:23.259426Z","submitted_at":"2010-02-04T12:48:02Z","title":"A New Global Embedding Approach to Study Hawking and Unruh Effects","version":2},"cited_work":{"arxiv_id":"1002.0985","doi":null,"metadata_source":"pith","pith_arxiv_id":"1002.0985","snapshot_observed_at":"2026-08-14T11:28:33.869523Z","title":"A New Global Embedding Approach to Study Hawking and Unruh Effects","venue":"gr-qc","work_id":"5d04dbf2-242b-4452-abe2-e53d4cb5ec4e","year":2010},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.031407Z"},"links":{"cited_paper":"/paper/1002.0985","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:c31c8aecef53a4f4c915f1fc740d1ecacb9cfbed67f2b3f04a9af93f8227daca","observation_id":"eb8f27d2-4886-4d07-809b-1e59778cad40","resolution":{"observed_at":"2026-08-14T11:28:33.874553Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0412076","last_updated":"2004-12-07T19:57:32Z","snapshot_observed_at":"2026-07-07T04:52:36.992545Z","submitted_at":"2004-12-07T19:57:32Z","title":"Global embedding of D-dimensional black holes with a cosmological constant in Minkowskian spacetimes: Matching between Hawking temperature and Unruh temperature","version":1},"cited_work":{"arxiv_id":"hep-th/0412076","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0412076","snapshot_observed_at":"2026-08-14T11:28:33.847464Z","title":"Global embedding of D-dimensional black holes with a cosmological constant in Minkowskian spacetimes: Matching between Hawking temperature and Unruh temperature","venue":"hep-th","work_id":"22106445-f0d0-4183-99fc-ec0960c04a4e","year":2004},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.036350Z"},"links":{"cited_paper":"/paper/hep-th/0412076","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:acb9cec121603caf6fd80ad1955cd9f65fe023edd525907a5f305fb54b21bef5","observation_id":"147b9eb0-eb7a-4381-a32e-fe1524df7a01","resolution":{"observed_at":"2026-08-14T11:28:33.853303Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0001045","last_updated":"2000-08-24T08:34:07Z","snapshot_observed_at":"2026-08-19T22:57:16.539498Z","submitted_at":"2000-01-16T05:20:13Z","title":"Reissner-Nordstr\\\"om-AdS black hole in the GEMS approach","version":2},"cited_work":{"arxiv_id":"gr-qc/0001045","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0001045","snapshot_observed_at":"2026-08-14T11:28:33.805911Z","title":"Reissner-Nordstr\\\"om-AdS black hole in the GEMS approach","venue":"gr-qc","work_id":"d7debe85-cbf1-4023-94ee-726e57d5daf3","year":2000},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.081578Z"},"links":{"cited_paper":"/paper/gr-qc/0001045","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:a75252636b3e5847233b60eff4e3c21ded47798fefc2cacabce217625bfc0212","observation_id":"0447e4e7-c51a-4d17-8374-0d199a5ea8e4","resolution":{"observed_at":"2026-08-14T11:28:33.830738Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0409107","last_updated":"2004-10-27T13:36:13Z","snapshot_observed_at":"2026-08-19T03:13:23.142847Z","submitted_at":"2004-09-28T15:53:10Z","title":"The GEMS Approach to Stationary Motions in the Spherically Symmetric Spacetimes","version":3},"cited_work":{"arxiv_id":"gr-qc/0409107","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0409107","snapshot_observed_at":"2026-08-14T11:28:33.646299Z","title":"The GEMS Approach to Stationary Motions in the Spherically Symmetric Spacetimes","venue":"gr-qc","work_id":"37834850-ac5a-43fe-b8e2-e49af2a8aac4","year":2004},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.191221Z"},"links":{"cited_paper":"/paper/gr-qc/0409107","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:dcb9e2343070aaa5702d4bf5cb0d7c6613d61afaf637b37d8a471821b70bd00a","observation_id":"bb3d99f2-0a88-4d56-ad88-b9bdbad8c64e","resolution":{"observed_at":"2026-08-14T11:28:33.700684Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9204099","last_updated":"2001-03-20T23:56:53Z","snapshot_observed_at":"2026-08-02T06:01:22.609920Z","submitted_at":"1992-04-29T23:16:12Z","title":"The Black Hole in Three Dimensional Space Time","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9204099","snapshot_observed_at":"2026-08-14T11:28:33.253361Z","title":"The Black hole in three- dimensional space-time,","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.253361Z"},"links":{"cited_paper":"/paper/hep-th/9204099","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:5231a34b47a6b7c13aca77b4cefda3792d26e3f14ea9b0e69fa52a040ec66e7a","observation_id":"318a95e7-b188-4bb6-a380-d7c4c15a576f","resolution":{"observed_at":"2026-08-14T11:28:33.253361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.4543","last_updated":"2014-08-07T17:25:37Z","snapshot_observed_at":"2026-08-16T08:36:36.448054Z","submitted_at":"2013-11-18T21:00:03Z","title":"Stability and existence analysis of static black holes in pure Lovelock theories","version":2},"cited_work":{"arxiv_id":"1311.4543","doi":null,"metadata_source":"pith","pith_arxiv_id":"1311.4543","snapshot_observed_at":"2026-08-14T11:28:33.584540Z","title":"Stability and existence analysis of static black holes in pure Lovelock theories","venue":"gr-qc","work_id":"1d173010-bfe6-4474-8cee-dccc1a3f677c","year":2013},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.260044Z"},"links":{"cited_paper":"/paper/1311.4543","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:706fa2ad76ad73f71cb336133c4c05ae4434a654c11e6a5512c2ee888b31247a","observation_id":"bb2bd4e5-2237-476b-82b3-7052e95aadf8","resolution":{"observed_at":"2026-08-14T11:28:33.589217Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1201.4994","last_updated":"2013-05-28T23:33:59Z","snapshot_observed_at":"2026-08-15T04:21:52.120373Z","submitted_at":"2012-01-20T21:06:11Z","title":"On the static Lovelock black holes","version":2},"cited_work":{"arxiv_id":"1201.4994","doi":null,"metadata_source":"pith","pith_arxiv_id":"1201.4994","snapshot_observed_at":"2026-08-14T11:28:33.561786Z","title":"On the static Lovelock black holes","venue":"gr-qc","work_id":"39a2391a-d385-4566-8113-ee3b4d2119ac","year":2012},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.265178Z"},"links":{"cited_paper":"/paper/1201.4994","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:72c12aa494ff7bc620fd51132adf84b9bc07e328bda5b55794cd4028c6670043","observation_id":"3ec2aa7c-32a4-4bc4-8dd1-584b7041ff20","resolution":{"observed_at":"2026-08-14T11:28:33.568878Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-14T11:28:34.469172Z","title":"Cambridge University Press, Cambridge, UK, 2010","venue":null,"work_id":"b24c518a-719c-4a0b-98ae-41d9cafec51f","year":2010},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.269882Z"},"links":{"citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:2a4fb5e2d485131e12d0ceb482a56fab447e5a61ccb6ddcfda1ab6210c75ba6f","observation_id":"94609e22-4765-4c35-b533-b8dd73a12ba4","resolution":{"observed_at":"2026-08-14T11:28:34.474365Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9912119","last_updated":"2000-09-30T17:42:16Z","snapshot_observed_at":"2026-08-07T22:37:16.615451Z","submitted_at":"1999-12-31T00:05:33Z","title":"The Thermodynamics of Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9912119","snapshot_observed_at":"2026-08-14T11:28:33.274974Z","title":"The thermodynamics of black holes,","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.274974Z"},"links":{"cited_paper":"/paper/gr-qc/9912119","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:0c8734896b271cfb26ec9f23bba00607631d26c5d383c8dea5bd51bbaf59dea8","observation_id":"d934d519-1e06-4e29-84b4-fefcc3c60565","resolution":{"observed_at":"2026-08-14T11:28:33.274974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.08263","last_updated":"2019-08-30T06:17:12Z","snapshot_observed_at":"2026-08-15T19:45:55.000474Z","submitted_at":"2019-05-20T18:00:03Z","title":"Thermality of the Rindler horizon: A simple derivation from the structure of the inertial propagator","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.08263","snapshot_observed_at":"2026-08-14T11:28:33.279854Z","title":"Thermality of the Rindler horizon: A simple der ivation from the structure of the inertial propagator,","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.279854Z"},"links":{"cited_paper":"/paper/1905.08263","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:4b2acd89fd2a15358dc21c03e4a922df52bb9e3347a81aef75078152e862973a","observation_id":"e74150e1-82c1-4628-b238-717413a24305","resolution":{"observed_at":"2026-08-14T11:28:33.279854Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.09278","last_updated":"2020-06-15T18:21:08Z","snapshot_observed_at":"2026-08-18T14:26:55.445253Z","submitted_at":"2019-06-21T18:00:29Z","title":"Exploring the Rindler vacuum and the Euclidean Plane","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.09278","snapshot_observed_at":"2026-08-14T11:28:33.284904Z","title":"Exploring the Rindler vacuum a nd the Euclidean Plane,","venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.284904Z"},"links":{"cited_paper":"/paper/1906.09278","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:af71e64b1e2c9e4d5007144fa13e110da59b590cbf2a44bf30970e9a18d3bdb6","observation_id":"8c622281-a42d-4e4d-ac86-cc7d95dcae88","resolution":{"observed_at":"2026-08-14T11:28:33.284904Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.10550","last_updated":"2018-11-29T12:41:36Z","snapshot_observed_at":"2026-08-14T19:21:11.180715Z","submitted_at":"2018-04-27T15:09:45Z","title":"Horizon temperature on the real line","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.10550","snapshot_observed_at":"2026-08-14T11:28:33.393428Z","title":"Horizon temperature on th e real line,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T11:28:33.393428Z"},"links":{"cited_paper":"/paper/1804.10550","citing_paper":"/paper/1908.09074"},"observation_digest":"sha256:ff001683ca78e8fdddd01091138dece273b8f84aa9c8501e100eeafc8928e72c","observation_id":"7f0eeb43-6bda-44a0-8b84-24ccad71958d","resolution":{"observed_at":"2026-08-14T11:28:33.393428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.09074","last_updated":"2019-10-28T08:35:37Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T01:54:23.327835Z","submitted_at":"2019-08-24T02:24:15Z","title":"Embedding into flat spacetime and black hole thermodynamics"},"reference_resolution":{"displayed":50,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":33,"verified_exact":10,"verified_fuzzy":7},"total_outbound_references":50},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 50 of 50 outbound references and 1 inbound Pith citation observation for arXiv:1908.09074."}