{"as_of":"2026-08-14T09:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:90fb8377c28aa59ea3bfb9b4f4f95b68d2195612c76ae66c9029e1fb5b55ef4b","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":37,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":37,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":37,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":37,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T04:31:45.631882Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T15:59:56.952554Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-12T20:39:03.150948Z","title":"The black hole in- terior from non-isometric codes and complexity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09616","last_updated":"2024-11-14T17:36:01Z","snapshot_observed_at":"2026-08-13T10:27:32.433553Z","submitted_at":"2024-11-14T17:36:01Z","title":"Non-Locality induces Isometry and Factorisation in Holography","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T20:39:03.150948Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2411.09616"},"observation_digest":"sha256:f46b0ce5388de57597a7bab01850a30f7228426425be5956ecb35df6759e62ec","observation_id":"dac57a27-e62f-48cd-a957-338312037799","resolution":{"observed_at":"2026-08-12T20:39:03.150948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-12T15:24:06.789503Z","title":"The black hole interior from non-isometric codes and complexity.arXiv preprint arXiv:2207.06536, 2022","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14389","last_updated":"2024-11-21T18:24:03Z","snapshot_observed_at":"2026-08-13T06:36:40.980683Z","submitted_at":"2024-11-21T18:24:03Z","title":"Unified and Generalized Approach to Entanglement-Assisted Quantum Error Correction","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T15:24:06.789503Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2411.14389"},"observation_digest":"sha256:d5264fc279dace0ca592c01baa6c0fc2ee32a305769b18e3323d682d3f8b71db","observation_id":"1238c413-be17-49d0-8275-9599940e6296","resolution":{"observed_at":"2026-08-12T15:24:06.789503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-11T05:58:26.902495Z","title":"The black hole interior from non-isometric codes and complexity,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.17059","last_updated":"2024-12-22T15:13:38Z","snapshot_observed_at":"2026-08-12T03:17:26.736416Z","submitted_at":"2024-12-22T15:13:38Z","title":"Projections and teleportation of operator quenches in CFT","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T05:58:26.902495Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2412.17059"},"observation_digest":"sha256:316233cc80bdaf7f37d03d79f5e68c5d0e1ba5f1572e1f6cb882b09cc7cedcda","observation_id":"badc5a96-2084-483f-aa53-e95f84f7eefe","resolution":{"observed_at":"2026-08-11T05:58:26.902495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-10T22:25:00.580073Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.02359","last_updated":"2025-01-17T02:12:04Z","snapshot_observed_at":"2026-08-12T15:25:03.115706Z","submitted_at":"2025-01-04T18:59:41Z","title":"Quantum mechanics and observers for gravity in a closed universe","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T22:25:00.580073Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2501.02359"},"observation_digest":"sha256:0f26ca4779d8bd274cb8836bc61a65543cfde00650959f0ed4aa8a177341619e","observation_id":"7a68fa7d-aba7-4ce0-89c5-fa9662fb2bff","resolution":{"observed_at":"2026-08-10T22:25:00.580073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-08T21:04:41.304192Z","title":"The black hole interior from non-isometric codes and complexity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04924","last_updated":"2025-02-07T13:42:27Z","snapshot_observed_at":"2026-08-14T04:11:03.301769Z","submitted_at":"2025-02-07T13:42:27Z","title":"Hilbert Bundles and Holographic Space-time: the Hydrodynamic Approach to Gravity","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-08T21:04:41.304192Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2502.04924"},"observation_digest":"sha256:0669dc441def46b14ddb02fefd2cfdfaebf99eb9c828746b5436aeb3837e05c4","observation_id":"aa26ec26-9d3f-428f-ab30-25e16f083530","resolution":{"observed_at":"2026-08-08T21:04:41.304192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-08T00:04:13.142069Z","title":"Akers, N","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.08724","last_updated":"2025-02-12T19:00:43Z","snapshot_observed_at":"2026-08-09T22:58:33.289834Z","submitted_at":"2025-02-12T19:00:43Z","title":"Firewalls From General Covariance","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-08T00:04:13.142069Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2502.08724"},"observation_digest":"sha256:de5c4eb5a5105a7db54a0da2906a1655e5eae09dd411cf291707e63bb71cbeb0","observation_id":"23a03e84-3d1f-4ffe-9b7a-6c77dc951e3d","resolution":{"observed_at":"2026-08-08T00:04:13.142069Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-07T12:47:20.125182Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.23664","last_updated":"2025-06-02T15:41:02Z","snapshot_observed_at":"2026-08-14T01:31:06.315933Z","submitted_at":"2025-05-29T17:10:57Z","title":"Measurements $\\mathit{with}$ probabilities in the final state proposal","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T12:47:20.125182Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2505.23664"},"observation_digest":"sha256:b8fac6912e0ec9a7d84fdfa5db5d5134e1e201db2f3bfcd54a72ad6f605dbaa8","observation_id":"fd569b42-38ac-4770-ac57-701e7b10e10a","resolution":{"observed_at":"2026-08-07T12:47:20.125182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-07T10:52:56.549162Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.04311","last_updated":"2025-06-04T18:00:00Z","snapshot_observed_at":"2026-08-13T06:27:13.402167Z","submitted_at":"2025-06-04T18:00:00Z","title":"An apologia for islands","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:56.549162Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2506.04311"},"observation_digest":"sha256:19e33ba51cbc2fa1175c03e630713fadc7875c5203571a3f128ba816ac140f09","observation_id":"3e85c9a7-c39b-4363-bba5-0f81c87bf022","resolution":{"observed_at":"2026-08-07T10:52:56.549162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-06T22:34:14.792537Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.21489","last_updated":"2025-06-26T17:18:50Z","snapshot_observed_at":"2026-08-09T23:51:30.836829Z","submitted_at":"2025-06-26T17:18:50Z","title":"Observers and Timekeepers: From the Page-Wootters Mechanism to the Gravitational Path Integral","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T22:34:14.792537Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2506.21489"},"observation_digest":"sha256:6add367bdbcda5639c1a9c496079e94e3e251235e7adc60ee51c309f3b02d819","observation_id":"727ad595-62ce-4172-be97-8e74f8665c65","resolution":{"observed_at":"2026-08-06T22:34:14.792537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-06T19:17:49.958488Z","title":"The black hole in- terior from non-isometric codes and complexity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.06046","last_updated":"2025-07-08T14:47:30Z","snapshot_observed_at":"2026-08-12T15:25:24.547925Z","submitted_at":"2025-07-08T14:47:30Z","title":"Observer complementarity for black holes and holography","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T19:17:49.958488Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2507.06046"},"observation_digest":"sha256:fe6bf04e762cd355d95f414f6c9c05867416c0a8ce6f28c4c9253dec0cc782fc","observation_id":"af6e5261-cc00-4ebd-abd7-bfd9b2693048","resolution":{"observed_at":"2026-08-06T19:17:49.958488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-06T17:35:47.970603Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.10649","last_updated":"2025-08-08T13:29:08Z","snapshot_observed_at":"2026-08-10T07:07:14.201118Z","submitted_at":"2025-07-14T18:00:00Z","title":"The Baby Universe is Fine and the CFT Knows It: On Holography for Closed Universes","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T17:35:47.970603Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2507.10649"},"observation_digest":"sha256:a87f6e71016eafbe245f69d92865fe3191f1925fe3cadf951e6950c45a44813a","observation_id":"df29982f-ebc2-4871-9a65-1d5fcb995dbc","resolution":{"observed_at":"2026-08-06T17:35:47.970603Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-06T15:08:06.948918Z","title":"The black hole interior from non-isometric codes and complexity,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.17031","last_updated":"2025-07-22T21:39:34Z","snapshot_observed_at":"2026-08-09T06:10:38.562995Z","submitted_at":"2025-07-22T21:39:34Z","title":"A Quantum Superposition of Black Hole Evaporation Histories: Recovering Unitarity","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T15:08:06.948918Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2507.17031"},"observation_digest":"sha256:e63a17a1ed1b1cf71bd994c69b50da76f4abc5df0db0e965036093ffbeec0f47","observation_id":"9516fc17-c013-4873-a96f-1b0312562c9d","resolution":{"observed_at":"2026-08-06T15:08:06.948918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2507.23667","last_updated":"2026-04-20T14:35:05Z","snapshot_observed_at":"2026-08-11T14:29:58.011217Z","submitted_at":"2025-07-31T15:47:34Z","title":"Universal Time Evolution of Holographic and Quantum Complexity","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-19T02:18:35.187658Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2507.23667"},"observation_digest":"sha256:e571034edc5fb0b67bead20e839b88362c359e150bfde1e8c4a6390f5327851b","observation_id":"dad99a80-8e41-4418-86ea-f83cbe69ffda","resolution":{"observed_at":"2026-05-19T02:21:59.391395Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2509.15295","last_updated":"2026-05-01T00:45:22Z","snapshot_observed_at":"2026-08-12T20:52:26.079041Z","submitted_at":"2025-09-18T18:00:00Z","title":"Living on the edge: a non-perturbative resolution to the negativity of bulk entropies","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-18T15:48:04.841164Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2509.15295"},"observation_digest":"sha256:be4c297a82976afc880ad959d1fdbd7564188dd932333c2ce49eef2a68f3c8b6","observation_id":"9a857e9b-c10f-4767-8a24-ccabf84ffc0e","resolution":{"observed_at":"2026-05-18T15:51:34.347819Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-04T08:51:12.792912Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.18967","last_updated":"2026-08-01T23:27:01Z","snapshot_observed_at":"2026-08-08T13:02:25.710942Z","submitted_at":"2025-10-21T18:00:04Z","title":"On the stabilizer complexity of Hawking radiation","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-04T08:51:12.792912Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2510.18967"},"observation_digest":"sha256:0cff50d89c9ed42c91f15b704bb0e88b6c5d43d20639ea2b31224c515adf4f9d","observation_id":"e861b29e-1f98-4b02-9074-f7a767399121","resolution":{"observed_at":"2026-08-04T08:51:12.792912Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2511.02903","last_updated":"2026-04-26T23:59:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-11-04T19:00:00Z","title":"Entanglement inequalities, black holes and the architecture of typical states","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-18T00:55:34.734413Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2511.02903"},"observation_digest":"sha256:aca86398c948ab1d25f35fd1f3e81e4ca0f89cb8d4a4590fa5516b82ef34881f","observation_id":"01d88fce-867e-4032-8b6e-9ad4b674b49f","resolution":{"observed_at":"2026-05-18T01:00:35.132400Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-03T19:58:35.464040Z","title":"The black hole interior from non-isometric codes and complexity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.22168","last_updated":"2025-11-27T07:13:02Z","snapshot_observed_at":"2026-08-13T07:34:31.422812Z","submitted_at":"2025-11-27T07:13:02Z","title":"Composite AdS geodesics for CFT correlators and timelike entanglement entropy","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T19:58:35.464040Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2511.22168"},"observation_digest":"sha256:6866fe12a14befacccef9c1155792d89c16e3cb2d1990310ae1b2f3ef360c7c1","observation_id":"f110df34-e570-4f32-b078-115532be9d91","resolution":{"observed_at":"2026-08-03T19:58:35.464040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2512.04318","last_updated":"2026-04-30T11:15:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-12-03T23:08:07Z","title":"Probing Evaporating Black Holes with Modular Flow in SYK","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-17T01:42:22.001560Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2512.04318"},"observation_digest":"sha256:64a1cd7d9735eaa7f4025e09746a44f8f7294193aea5557549483d38acce8f0e","observation_id":"79a14167-e44e-4a7f-8ac6-a05c3a1be4ab","resolution":{"observed_at":"2026-05-17T01:43:50.011350Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-03T14:25:10.671028Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.21037","last_updated":"2026-03-11T04:29:39Z","snapshot_observed_at":"2026-08-13T10:36:08.646573Z","submitted_at":"2025-12-24T08:03:55Z","title":"Black hole as a multipartite entangler: multi-entropy in AdS${}_3$/CFT${}_2$","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T14:25:10.671028Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2512.21037"},"observation_digest":"sha256:c0bdab7bbc3d8e98d736f47bc1be9b089c178f3a9d8eb7fbad920687338ae28d","observation_id":"c2553615-3647-4608-9039-61f32f2f67ed","resolution":{"observed_at":"2026-08-03T14:25:10.671028Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2602.09100","last_updated":"2026-04-08T19:39:17Z","snapshot_observed_at":"2026-07-06T22:45:11.110274Z","submitted_at":"2026-02-09T19:00:03Z","title":"Area Scaling of Dynamical Degrees of Freedom in Regularised Scalar Field Theory","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-05-16T05:13:33.143479Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2602.09100"},"observation_digest":"sha256:5612f84293750a28460546100a1e9f4669f49d6d55c6363b1564f230c1d9682a","observation_id":"da579905-d731-42bc-9938-5bfdc81be47f","resolution":{"observed_at":"2026-05-16T05:17:22.600687Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2604.20170","last_updated":"2026-07-28T10:32:56Z","snapshot_observed_at":"2026-08-07T11:33:16.916430Z","submitted_at":"2026-04-17T16:54:49Z","title":"Computational Cosmic Censorship","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-10T07:21:14.393923Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2604.20170"},"observation_digest":"sha256:8733082a8b197e2ebd5d72541c353ad29aeb7ee530e7a1e40983083c82eb6374","observation_id":"60424209-9098-4146-9874-ec8af7ec9d1c","resolution":{"observed_at":"2026-05-10T07:21:55.142015Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2605.06780","last_updated":"2026-05-07T18:00:02Z","snapshot_observed_at":"2026-08-13T04:22:27.181451Z","submitted_at":"2026-05-07T18:00:02Z","title":"A Semiclassical Diagnostic for Spacetime Emergence","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-11T00:58:15.656261Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2605.06780"},"observation_digest":"sha256:9af975be134779701159fff56f7975d55f03b0d19ef35ecb6be8eb3cfc8348f5","observation_id":"9c118b25-eafc-4857-bae8-3da3e86bfda6","resolution":{"observed_at":"2026-05-11T04:55:59.580981Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2605.23670","last_updated":"2026-06-03T14:10:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-22T14:18:32Z","title":"Twirled Perfect Tensor Networks: Computationally covariant holographic tensor networks","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-25T04:16:53.859656Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2605.23670"},"observation_digest":"sha256:a8ca419a8c5d830589d2dbb3289ccbe8b9552e29b52befd4cad39bb13bdc6f39","observation_id":"ae73f23e-7940-42eb-ae01-0f4c0e1bcef9","resolution":{"observed_at":"2026-05-25T04:20:19.668238Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2605.23670","last_updated":"2026-06-03T14:10:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-22T14:18:32Z","title":"Twirled Perfect Tensor Networks: Computationally covariant holographic tensor networks","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-06-30T15:35:54.995405Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2605.23670"},"observation_digest":"sha256:24bd7dbdca102e850bda9afc3b5b982a155578dba83e7b8dc32574a6df0887f0","observation_id":"72f23b95-66c6-4823-859f-d37b841532e6","resolution":{"observed_at":"2026-06-30T15:44:48.770573Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2606.06404","last_updated":"2026-06-04T17:09:30Z","snapshot_observed_at":"2026-08-12T22:30:42.676155Z","submitted_at":"2026-06-04T17:09:30Z","title":"Smooth horizons from topology change in canonical quantum gravity","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-06-28T00:05:23.070933Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.06404"},"observation_digest":"sha256:b7938aece8e04de41a11ff603bb880dbefc2e5f91f0e22e9d4cd7b3cbe77a2cc","observation_id":"0ea1a21f-4ef5-4129-ac71-2812a78c00a1","resolution":{"observed_at":"2026-07-02T15:07:04.905673Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2606.10924","last_updated":"2026-06-18T14:26:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-09T14:31:02Z","title":"Spacetime from Operator Algebras","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-06-27T12:18:11.543469Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.10924"},"observation_digest":"sha256:4cb31acb69c8309aa0deb02e48946df9ed4588629746e82b5464c0aae3e01eb3","observation_id":"66f5453e-5490-4baf-835f-1669fdbe2f7f","resolution":{"observed_at":"2026-07-03T07:07:44.596621Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2606.22598","last_updated":"2026-07-13T19:23:28Z","snapshot_observed_at":"2026-08-14T02:10:14.853567Z","submitted_at":"2026-06-21T17:16:10Z","title":"When does a state-dependent proto-area define a bulk geometry?","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-26T09:47:08.257614Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.22598"},"observation_digest":"sha256:020aeeba160309582a7ae1e9e87c4c8f9a586f457a0f7e3da1a89d362877fed1","observation_id":"95993ae4-3c20-4809-b75b-d5db0b9ba056","resolution":{"observed_at":"2026-07-04T09:39:46.043449Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-15T10:38:36.221072Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.22598","last_updated":"2026-07-13T19:23:28Z","snapshot_observed_at":"2026-08-14T02:10:14.853567Z","submitted_at":"2026-06-21T17:16:10Z","title":"When does a state-dependent proto-area define a bulk geometry?","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-07-15T10:38:36.221072Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.22598"},"observation_digest":"sha256:b37d8af150121460eb75268117331be3768f3703f9c1bdddf6b60450a2242e5b","observation_id":"27e86840-36a5-4b25-9666-2e755355104b","resolution":{"observed_at":"2026-07-15T10:38:36.221072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2606.26357","last_updated":"2026-07-12T13:33:14Z","snapshot_observed_at":"2026-08-04T22:48:05.446553Z","submitted_at":"2026-06-24T20:10:22Z","title":"Deformed BTZ Radiance and Single Trace $T\\bar{T}$ Holography","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-06-26T01:09:18.016335Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.26357"},"observation_digest":"sha256:4c30171227450fe23c8d9db85b8ad2021a0827ae181f41e2489fcc71faccfb5d","observation_id":"9b50c12e-6988-4923-8285-54657d76377a","resolution":{"observed_at":"2026-07-04T15:59:56.953704Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-14T17:17:49.685428Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.26357","last_updated":"2026-07-12T13:33:14Z","snapshot_observed_at":"2026-08-04T22:48:05.446553Z","submitted_at":"2026-06-24T20:10:22Z","title":"Deformed BTZ Radiance and Single Trace $T\\bar{T}$ Holography","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-14T17:17:49.685428Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.26357"},"observation_digest":"sha256:5d23c286b46d137d8b835bc23f78fe21999a9ba53d041662cb51cacfc2c3751d","observation_id":"24eacfda-2caf-4d34-b6dd-6c8417092500","resolution":{"observed_at":"2026-07-14T17:17:49.685428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2606.28484","last_updated":"2026-06-26T18:00:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-26T18:00:01Z","title":"Subregion observer rules from generalized entanglement wedges","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-30T01:12:01.372649Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.28484"},"observation_digest":"sha256:2daedb62bf850923ecd58027f65dd12032e730cfd2decba66ebfa4e73d456376","observation_id":"5d0812b8-5cef-4c0b-91f0-42034bf881d9","resolution":{"observed_at":"2026-07-01T15:45:48.044601Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2606.30853","last_updated":"2026-06-29T19:34:06Z","snapshot_observed_at":"2026-08-12T15:24:36.939257Z","submitted_at":"2026-06-29T19:34:06Z","title":"Rethinking quantum information in gravity and fields","version":1},"reference_index":158,"source":"pdf_text","source_observed_at":"2026-07-01T01:14:50.851412Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2606.30853"},"observation_digest":"sha256:fdecffb64bb0c8721c19043526f633dfc0ffcffc62927d76bd6c9448888dd9b7","observation_id":"3ab19606-bb31-4b97-8244-88f4c9d3410a","resolution":{"observed_at":"2026-07-01T01:15:12.894058Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2607.01322","last_updated":"2026-07-01T18:00:01Z","snapshot_observed_at":"2026-07-12T23:17:37.547262Z","submitted_at":"2026-07-01T18:00:01Z","title":"Wormholes as red herrings: reflection positivity and the reconstruction of unitary quantum field theories","version":1},"reference_index":198,"source":"pdf_text","source_observed_at":"2026-07-03T19:39:35.189207Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2607.01322"},"observation_digest":"sha256:d16455b3c903646a2b0bf2ae155f66fc3135bceb2a0de1634f414dc2bfb13750","observation_id":"de0bad77-0d56-48ac-9aac-8b2055674629","resolution":{"observed_at":"2026-07-03T19:58:54.292283Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":"2207.06536","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-04T15:59:56.952554Z","title":"The black hole interior from non-isometric codes and complexity","venue":null,"work_id":"b46a09fd-b568-45a3-810d-08cd1678e99d","year":2024},"citing_paper":{"arxiv_id":"2607.01351","last_updated":"2026-07-01T18:09:10Z","snapshot_observed_at":"2026-08-07T18:37:34.362404Z","submitted_at":"2026-07-01T18:09:10Z","title":"Wigner negativity in Krylov space and emergent semiclassicality","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-03T19:27:01.063141Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2607.01351"},"observation_digest":"sha256:633046e2ee166343792476543a95865002fed020e2015fa6c76c950aabf8b5d3","observation_id":"53124ae4-c0eb-4cc1-b465-47a910633d1e","resolution":{"observed_at":"2026-07-03T19:28:51.808847Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-07-14T10:08:11.925513Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.10663","last_updated":"2026-07-12T09:16:46Z","snapshot_observed_at":"2026-08-10T17:14:16.270599Z","submitted_at":"2026-07-12T09:16:46Z","title":"Certified boundary-magic witness for state-dependent proto-area in a holographic code","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-14T10:08:11.925513Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2607.10663"},"observation_digest":"sha256:371e3f575cc00ab689a421d26de04356a0c02874aeee7a561dfeb6d04f04960e","observation_id":"3e36559f-7a83-4394-b7bc-8f02aec6dd8d","resolution":{"observed_at":"2026-07-14T10:08:11.925513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-14T04:31:45.631882Z","title":"The black hole interior from non-isometric codes and complexity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.08972","last_updated":"2026-08-11T05:16:32Z","snapshot_observed_at":"2026-08-14T09:09:41.092246Z","submitted_at":"2026-08-10T00:35:11Z","title":"Matrix Multiverses Meet Multiple Mythologies","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T04:31:45.631882Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2608.08972"},"observation_digest":"sha256:ec2a055078a7c79c6491e3370c2cf909ab40413e44d4a372b6b62a77812659d4","observation_id":"a08b79f1-724e-4d99-b24f-7504fb57e46f","resolution":{"observed_at":"2026-08-14T04:31:45.631882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.06536","snapshot_observed_at":"2026-08-14T04:28:23.501584Z","title":"Akers, N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.10085","last_updated":"2026-08-10T18:01:01Z","snapshot_observed_at":"2026-08-14T09:09:57.064054Z","submitted_at":"2026-08-10T18:01:01Z","title":"Approximate locality, black hole complementarity and overlapping qubits","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T04:28:23.501584Z"},"links":{"cited_paper":"/paper/2207.06536","citing_paper":"/paper/2608.10085"},"observation_digest":"sha256:20d43750782ef9235d7d263d49aabcbea90036f3274f218c553d058ebf99acec","observation_id":"df490cd3-b455-4a6a-9b2c-3b6ab5881f3b","resolution":{"observed_at":"2026-08-14T04:28:23.501584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2207.06536/citation-record","integrity":"/paper/2207.06536/integrity","json":"/paper/2207.06536/citation-record.json","paper":"/paper/2207.06536"},"outbound":[],"paper":{"arxiv_id":"2207.06536","last_updated":"2022-10-04T21:43:24Z","latest_version":2,"primary_category":"hep-th","snapshot_observed_at":"2026-08-13T15:04:35.966877Z","submitted_at":"2022-07-13T22:47:45Z","title":"The black hole interior from non-isometric codes and complexity"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 37 inbound Pith citation observations for arXiv:2207.06536."}