{"as_of":"2026-08-07T17:39:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:df5d7f92c386944140bd5fe983d43993ccf6e836fbe03847b4bf6a3e2623d663","coverage":[{"denominator":58,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":58,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:04:17.561732Z","state":"measured"},{"denominator":67,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":67,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T22:34:11.702526Z","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":"2026-07-02T09:56:51.651537Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-08-06T22:34:11.702526Z","title":"Nomura and T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.21489","last_updated":"2025-06-26T17:18:50Z","snapshot_observed_at":"2026-08-06T22:21:23.231984Z","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":25,"source":"pdf_text","source_observed_at":"2026-08-06T22:34:11.702526Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2506.21489"},"observation_digest":"sha256:6e686e8fd6dc9a39fca09a5a422e81a27806293ed2e1b5c74a1d99a10f783fcd","observation_id":"0aa060dc-8de5-4528-9d07-523859ee3e20","resolution":{"observed_at":"2026-08-06T22:34:11.702526Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-08-06T17:35:47.423768Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.10649","last_updated":"2025-08-08T13:29:08Z","snapshot_observed_at":"2026-08-07T12:54:44.591001Z","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":56,"source":"pdf_text","source_observed_at":"2026-08-06T17:35:47.423768Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2507.10649"},"observation_digest":"sha256:613db77da480fb01d240984c972784c27f76b0cd66fccadaaf987b429841b3fa","observation_id":"1b036193-e114-44a6-8183-1170399a3e61","resolution":{"observed_at":"2026-08-06T17:35:47.423768Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-08-04T09:03:22.219987Z","title":"Nomura and T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2510.17953","last_updated":"2026-06-01T22:42:45Z","snapshot_observed_at":"2026-08-07T11:09:22.218148Z","submitted_at":"2025-10-20T18:00:00Z","title":"Junctions, strings, clocks and gravitational memory in three dimensional dS space","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-04T09:03:22.219987Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2510.17953"},"observation_digest":"sha256:b7d3cde2f0b962cb398ae5a7086c7845e54b168e356afe0e9f9d82eeae375a41","observation_id":"c55e958b-33d7-499e-b8df-5393e0004f44","resolution":{"observed_at":"2026-08-04T09:03:22.219987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":"2505.20390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-07-02T09:56:51.651537Z","title":"Nomura and T","venue":null,"work_id":"e1b77ea0-80f0-46d1-87ab-2c47dda07b35","year":2025},"citing_paper":{"arxiv_id":"2512.00704","last_updated":"2026-05-07T09:49:20Z","snapshot_observed_at":"2026-08-02T16:01:55.757696Z","submitted_at":"2025-11-30T02:51:17Z","title":"No boundary density matrix in elliptic de Sitter dS/$\\mathbb{Z}_2$","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-17T03:53:14.977749Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2512.00704"},"observation_digest":"sha256:298bf2d7b1bba49d391477e436bcddb1058e1fdf9eae27a371250e870aac975f","observation_id":"7e96e599-222a-4c0a-b2c6-271d189eb20f","resolution":{"observed_at":"2026-05-17T03:53:59.310988Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":"2505.20390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-07-02T09:56:51.651537Z","title":"Nomura and T","venue":null,"work_id":"e1b77ea0-80f0-46d1-87ab-2c47dda07b35","year":2025},"citing_paper":{"arxiv_id":"2604.14387","last_updated":"2026-04-27T17:58:39Z","snapshot_observed_at":"2026-07-06T23:02:09.426599Z","submitted_at":"2026-04-15T20:01:32Z","title":"Emergent States and Algebras from the Double-Scaling limit of Pure States in SYK","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-10T12:16:49.217769Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2604.14387"},"observation_digest":"sha256:5477a73effdbca399f5f3a4e9465980c1dfdac618eaf452e4cf3626a3d68969e","observation_id":"4527e478-19c5-4670-8a15-2b4ce2310f2d","resolution":{"observed_at":"2026-05-10T12:20:22.868441Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":"2505.20390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-07-02T09:56:51.651537Z","title":"Nomura and T","venue":null,"work_id":"e1b77ea0-80f0-46d1-87ab-2c47dda07b35","year":2025},"citing_paper":{"arxiv_id":"2605.13970","last_updated":"2026-05-13T18:00:07Z","snapshot_observed_at":"2026-08-02T14:33:20.915591Z","submitted_at":"2026-05-13T18:00:07Z","title":"A Tale of Two Hartle-Hawking Wave Functions: Fully Gravitational vs Partially Frozen","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-05-15T02:34:34.514607Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2605.13970"},"observation_digest":"sha256:5553b8445ddcb05366bb6a60b5f59850c7766a89d609ebb3119367cd4a3986db","observation_id":"167a65ed-e6a8-4d92-9042-ac261e4a7a28","resolution":{"observed_at":"2026-05-15T02:39:41.659233Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":"2505.20390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-07-02T09:56:51.651537Z","title":"Nomura and T","venue":null,"work_id":"e1b77ea0-80f0-46d1-87ab-2c47dda07b35","year":2025},"citing_paper":{"arxiv_id":"2606.04575","last_updated":"2026-06-03T08:11:07Z","snapshot_observed_at":"2026-07-29T13:50:45.063356Z","submitted_at":"2026-06-03T08:11:07Z","title":"Emergent Closed Universes in Symmetric Orbifold CFTs","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-28T05:21:57.878503Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2606.04575"},"observation_digest":"sha256:8b4016c1fbdf14529f1107cfcff8185d2d1c98437711b9ed0974d6851124f5eb","observation_id":"fed51c8a-2599-41eb-a0c7-5f38cd2ce465","resolution":{"observed_at":"2026-07-02T09:56:51.652836Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":"2505.20390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-07-02T09:56:51.651537Z","title":"Nomura and T","venue":null,"work_id":"e1b77ea0-80f0-46d1-87ab-2c47dda07b35","year":2025},"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":39,"source":"pdf_text","source_observed_at":"2026-06-30T01:12:01.372649Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2606.28484"},"observation_digest":"sha256:48550c91f231ce3d3c5f3e9a37b364db3cf623f690803c9413ff980e1fd2b015","observation_id":"4e5ee148-849c-47b6-9e99-1bb9d856ab76","resolution":{"observed_at":"2026-07-01T15:45:48.167063Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"cited_work":{"arxiv_id":"2505.20390","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.20390","snapshot_observed_at":"2026-07-02T09:56:51.651537Z","title":"Nomura and T","venue":null,"work_id":"e1b77ea0-80f0-46d1-87ab-2c47dda07b35","year":2025},"citing_paper":{"arxiv_id":"2606.30853","last_updated":"2026-06-29T19:34:06Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-29T19:34:06Z","title":"Rethinking quantum information in gravity and fields","version":1},"reference_index":162,"source":"pdf_text","source_observed_at":"2026-07-01T01:14:50.851412Z"},"links":{"cited_paper":"/paper/2505.20390","citing_paper":"/paper/2606.30853"},"observation_digest":"sha256:130faa922bbe469399a0f06b25d25cca33154fcbd54f0507be2409ca134fb4b5","observation_id":"9bc2932e-cfa9-4900-a86b-7c1e82123d62","resolution":{"observed_at":"2026-07-01T01:15:12.601021Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2505.20390/citation-record","integrity":"/paper/2505.20390/integrity","json":"/paper/2505.20390/citation-record.json","paper":"/paper/2505.20390"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"hep-th/9711200","last_updated":"1998-01-22T15:42:41Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"1997-11-27T23:53:13Z","title":"The Large N Limit of Superconformal Field Theories and Supergravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9711200","snapshot_observed_at":"2026-08-07T14:04:12.520880Z","title":"The large N limit of superconformal field theories and supergravity,","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:12.520880Z"},"links":{"cited_paper":"/paper/hep-th/9711200","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:cf821504b72b434bd9ae317876f70faa487741e5fe0fd4a11f0ed4a7c8e74941","observation_id":"7a270103-1ea4-4ffa-8b9c-0cdbc691d87a","resolution":{"observed_at":"2026-08-07T14:04:12.520880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0603001","last_updated":"2006-03-07T19:21:09Z","snapshot_observed_at":"2026-07-07T04:56:49.142200Z","submitted_at":"2006-02-28T21:29:24Z","title":"Holographic Derivation of Entanglement Entropy from AdS/CFT","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0603001","snapshot_observed_at":"2026-08-07T14:04:12.609708Z","title":"Holographic derivation of entanglement entropy from AdS/CFT,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:12.609708Z"},"links":{"cited_paper":"/paper/hep-th/0603001","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:506cc09191607926f6e55bf9e1d3d51b848b43165cec818c662585cd2d570ea0","observation_id":"0f06f533-3f82-49a9-b2d8-e8087fa28fa8","resolution":{"observed_at":"2026-08-07T14:04:12.609708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.0016","last_updated":"2012-06-14T13:23:35Z","snapshot_observed_at":"2026-07-06T01:26:58.535235Z","submitted_at":"2007-05-01T15:54:13Z","title":"A Covariant Holographic Entanglement Entropy Proposal","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.0016","snapshot_observed_at":"2026-08-07T14:04:12.714370Z","title":"A covariant holographic entanglement entropy proposal,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:12.714370Z"},"links":{"cited_paper":"/paper/0705.0016","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:b1d03cf884dcaa606579473afbab232a9cecb9ad59c96d2a4981754e0252f747","observation_id":"400bbefe-6169-4e5f-986c-e865677f0e81","resolution":{"observed_at":"2026-08-07T14:04:12.714370Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.2892","last_updated":"2013-07-11T22:55:50Z","snapshot_observed_at":"2026-08-05T13:26:52.849030Z","submitted_at":"2013-07-10T19:51:51Z","title":"Quantum corrections to holographic entanglement entropy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.2892","snapshot_observed_at":"2026-08-07T14:04:12.796632Z","title":"Quantum corrections to holographic entanglement entropy,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:12.796632Z"},"links":{"cited_paper":"/paper/1307.2892","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:8d53edbecde6592bf078a4efbb522be3681da9f79270a949245941f9e9fc89d5","observation_id":"8f573e25-17a7-4747-ab4e-dfb673554a96","resolution":{"observed_at":"2026-08-07T14:04:12.796632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3203","last_updated":"2015-01-14T22:05:02Z","snapshot_observed_at":"2026-08-05T09:41:45.470493Z","submitted_at":"2014-08-14T06:57:49Z","title":"Quantum Extremal Surfaces: Holographic Entanglement Entropy beyond the Classical Regime","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3203","snapshot_observed_at":"2026-08-07T14:04:12.884218Z","title":"Quantum extremal surfaces: holographic entanglement entropy beyond the classical regime,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:12.884218Z"},"links":{"cited_paper":"/paper/1408.3203","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:186ef46a42f084a27c2d67b0bbff90134c3efa12f182d226c7d4ceea1b6a80a9","observation_id":"a56a65cf-e981-4b5d-836d-7fcec490965d","resolution":{"observed_at":"2026-08-07T14:04:12.884218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.08255","last_updated":"2020-08-29T01:47:10Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2019-05-20T18:00:01Z","title":"Entanglement Wedge Reconstruction and the Information Paradox","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.08255","snapshot_observed_at":"2026-08-07T14:04:12.973772Z","title":"Entanglement wedge reconstruction and the information paradox,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:12.973772Z"},"links":{"cited_paper":"/paper/1905.08255","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:809ec6ebb189db27c1348404a9afd0f2a6520f91300dd39d9dc1e419574c0791","observation_id":"45de28fb-1ab2-4b6a-9e68-128f49a1f9d4","resolution":{"observed_at":"2026-08-07T14:04:12.973772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.10996","last_updated":"2019-11-04T16:40:19Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2019-08-29T00:37:46Z","title":"The Page curve of Hawking radiation from semiclassical geometry","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.10996","snapshot_observed_at":"2026-08-07T14:04:13.024061Z","title":"The Page curve of Hawking radiation from semiclassical geometry,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.024061Z"},"links":{"cited_paper":"/paper/1908.10996","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:05e94b00a4a62956bb562f224434663627ffb7ff572e7c683d06fea1ae03b4b0","observation_id":"303c10bd-e982-4e88-899e-9bde040738ca","resolution":{"observed_at":"2026-08-07T14:04:13.024061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.00098","last_updated":"2024-08-14T19:20:49Z","snapshot_observed_at":"2026-07-06T17:23:18.724263Z","submitted_at":"2024-01-31T19:00:00Z","title":"Closed universes in two dimensional gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.00098","snapshot_observed_at":"2026-08-07T14:04:13.096865Z","title":"Closed universes in two dimensional gravity,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.096865Z"},"links":{"cited_paper":"/paper/2402.00098","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:fd4115c10add2599cf88b4b315c9dfa2cbff6d779d20e34ab16ed49fa27690c4","observation_id":"e74c0e1f-050c-41f8-b74a-fa9a257f56bc","resolution":{"observed_at":"2026-08-07T14:04:13.096865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.13047","last_updated":"2025-02-14T16:12:41Z","snapshot_observed_at":"2026-08-07T00:56:49.736724Z","submitted_at":"2024-03-19T18:00:00Z","title":"Closed universes, factorization, and ensemble averaging","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.13047","snapshot_observed_at":"2026-08-07T14:04:13.154689Z","title":"Closed universes, factorization, and ensemble averaging,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.154689Z"},"links":{"cited_paper":"/paper/2403.13047","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:07e0ca8ae94e8f899cfbf44d801b62f959929d895c09f79067d82cff99b6d406","observation_id":"45b2de3c-6c1d-4038-8447-8f1578f683cd","resolution":{"observed_at":"2026-08-07T14:04:13.154689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.09978","last_updated":"2025-04-24T14:33:59Z","snapshot_observed_at":"2026-07-06T16:48:41.065654Z","submitted_at":"2023-11-16T15:51:11Z","title":"Gauging spacetime inversions in quantum gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.09978","snapshot_observed_at":"2026-08-07T14:04:13.221206Z","title":"Gauging spacetime inversions in quantum gravity,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.221206Z"},"links":{"cited_paper":"/paper/2311.09978","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:5bf4476fdb55580e13c6c0f98a1fbb24cd0ca8a4d3eb0c1da27f55fc7077c892","observation_id":"5b88ab96-0354-4284-9a69-c3a7576ba2a7","resolution":{"observed_at":"2026-08-07T14:04:13.221206Z","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":"2026-08-07T14:04:24.752927Z","title":"Black holes as red herrings: topological fluctuations and the loss of quantum coherence,","venue":null,"work_id":"917bce47-ae23-4289-8f49-c263b234ad69","year":1988},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.292823Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:c66b74b9bcf7574862d82b07641d9cd15356dd6c3f77979d71dba92b44014c26","observation_id":"1480dc2b-4ad3-4aba-bd0a-77a010aab81f","resolution":{"observed_at":"2026-08-07T14:04:24.851266Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:24.531915Z","title":"Loss of incoherence and determination of coupling constants in quantum gravity,","venue":null,"work_id":"dcda4ac7-6709-4cb8-ae56-0c6920b16568","year":1988},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.368189Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:18c2df2f52c771586a53ff51f030a2838c135e5c4d2dba92c074218801b2b4ec","observation_id":"e93d53f0-4d04-414f-8af5-1482899f1e21","resolution":{"observed_at":"2026-08-07T14:04:24.608838Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.08950","last_updated":"2020-02-20T18:58:54Z","snapshot_observed_at":"2026-08-06T19:58:26.008396Z","submitted_at":"2020-02-20T18:58:54Z","title":"Transcending the ensemble: baby universes, spacetime wormholes, and the order and disorder of black hole information","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.08950","snapshot_observed_at":"2026-08-07T14:04:13.424223Z","title":"Transcending the ensemble: baby universes, spacetime wormholes, and the order and disorder of black hole information,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.424223Z"},"links":{"cited_paper":"/paper/2002.08950","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:d3b2b90582538edfaaaffa245546794e5833f08fb78413973b1274377fc0edd1","observation_id":"79d9710a-7269-4190-95ef-347457403e2d","resolution":{"observed_at":"2026-08-07T14:04:13.424223Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.10780","last_updated":"2023-07-03T14:54:23Z","snapshot_observed_at":"2026-07-06T13:23:21.926490Z","submitted_at":"2022-06-22T00:22:20Z","title":"An Algebra of Observables for de Sitter Space","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.10780","snapshot_observed_at":"2026-08-07T14:04:13.488412Z","title":"An algebra of observables for de Sitter space,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.488412Z"},"links":{"cited_paper":"/paper/2206.10780","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:5fed359f0550e0af1c62d41d512117044df6c88b99e77a7c234cb10e5dd512f1","observation_id":"7c2aec3e-eacf-4617-b8b4-8f0cdf39926c","resolution":{"observed_at":"2026-08-07T14:04:13.488412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.09748","last_updated":"2023-08-18T18:00:03Z","snapshot_observed_at":"2026-07-06T16:07:49.197575Z","submitted_at":"2023-08-18T18:00:03Z","title":"de Sitter space is sometimes not empty","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.09748","snapshot_observed_at":"2026-08-07T14:04:13.557307Z","title":"de Sitter space is sometimes not empty,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.557307Z"},"links":{"cited_paper":"/paper/2308.09748","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:fa1f2622c29bfc2c60e7cf6566816bb11aefcd5f9f089c1f00dc1fd352ea4e90","observation_id":"dc57d17a-48b8-4a02-bd13-81b699e57f01","resolution":{"observed_at":"2026-08-07T14:04:13.557307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.02359","last_updated":"2025-01-17T02:12:04Z","snapshot_observed_at":"2026-07-06T20:16:35.984578Z","submitted_at":"2025-01-04T18:59:41Z","title":"Quantum mechanics and observers for gravity in a closed universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.02359","snapshot_observed_at":"2026-08-07T14:04:13.620008Z","title":"Quantum mechanics and observers for gravity in a closed universe,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.620008Z"},"links":{"cited_paper":"/paper/2501.02359","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:d0994d39ab698f7e9c437583c7f71649e39b6fd5c68e0c69085b7ef4bd34f831","observation_id":"81f4daef-2845-4920-b0d5-8f95e27b66f0","resolution":{"observed_at":"2026-08-07T14:04:13.620008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.02632","last_updated":"2025-03-07T00:22:23Z","snapshot_observed_at":"2026-07-06T20:16:48.980017Z","submitted_at":"2025-01-05T19:27:03Z","title":"The gravitational path integral from an observer's point of view","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.02632","snapshot_observed_at":"2026-08-07T14:04:13.679312Z","title":"The gravitational path integral from an observer’s point of view,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.679312Z"},"links":{"cited_paper":"/paper/2501.02632","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:a7bc8ccd9d65453a703431898c3aa427ea50ab31087478c79594dfcd263928d8","observation_id":"e1454ebd-ce4b-4584-8256-3bed93ed08a1","resolution":{"observed_at":"2026-08-07T14:04:13.679312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.09681","last_updated":"2025-03-12T18:00:00Z","snapshot_observed_at":"2026-08-07T17:09:22.503477Z","submitted_at":"2025-03-12T18:00:00Z","title":"On observers in holographic maps","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.09681","snapshot_observed_at":"2026-08-07T14:04:13.731247Z","title":"On observers in holographic maps,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.731247Z"},"links":{"cited_paper":"/paper/2503.09681","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:20c93955baff5bdc4895955b394af8a635fda8e7e50c71f2a48a85eac8c68fde","observation_id":"f65edb61-28f8-426e-9c61-87d81f95c478","resolution":{"observed_at":"2026-08-07T14:04:13.731247Z","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":"2026-08-07T14:04:24.383022Z","title":"Quantum theory of gravity. I. The canonical theory,","venue":null,"work_id":"867a50fc-eda0-43f8-ad8a-58bf364de8ce","year":1967},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.788975Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:dfb43aaad4a7f08488b5efa5e079a6182e7bf508bf8d4494a1e37b4147523736","observation_id":"64356203-63ca-4c44-8d40-42cf931ac061","resolution":{"observed_at":"2026-08-07T14:04:24.441794Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:24.246676Z","title":"Dynamical structure and definition of energy in general relativity,","venue":null,"work_id":"6741829a-8d35-46c5-9cc4-4ae6fd08f52b","year":1959},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.848260Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:bc4a0326c39fb24d0069ef9799ac856cc29f419a207aabf4b4c76ea5afb93d0e","observation_id":"e0119b58-d001-4bfd-8957-f037e2e9295e","resolution":{"observed_at":"2026-08-07T14:04:24.297638Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:24.043178Z","title":"Quantum mechanics of the gravitational field,","venue":null,"work_id":"926906ba-37dc-4095-bf33-3c987c68b8b8","year":1982},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.903842Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:76012dd9c28e22917b2cc0e0873c955a472830b33f94efb4691072f4c121cb0c","observation_id":"6dcfe1ab-8e87-4089-91e3-56a629cd5b9a","resolution":{"observed_at":"2026-08-07T14:04:24.119615Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:23.757541Z","title":"Derivation of the Wheeler-DeWitt equation from a path integral for minisuperspace models,","venue":null,"work_id":"0082ed0f-34b5-48e8-9f6b-2bdade5ddc88","year":1988},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:13.977888Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:65f329e5048e817cedd9804ac384da526d45de357a5025f62469870464e63061","observation_id":"6d11a776-c9d2-44a2-bf01-34659c73b6b2","resolution":{"observed_at":"2026-08-07T14:04:23.864776Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:23.531953Z","title":"Wave functions constructed from an invariant sum over histories satisfy constraints,","venue":null,"work_id":"008a8664-f89d-4523-ba38-52da3dd9a67e","year":1991},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.045676Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:bc1255564046f2d9f5ec93d580c6f55ab91ef224b88f70636ef600a6341a9eb4","observation_id":"15ee2cef-81ca-4d10-a621-6bc3178357b9","resolution":{"observed_at":"2026-08-07T14:04:23.667177Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:23.346059Z","title":"Quantization of relativistic systems with constraints,","venue":null,"work_id":"5991a89e-90e1-482b-810e-ba36cab822d1","year":1975},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.110482Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:c8da42130e03ae86016dac319007ac9f5358267a5e9bc820205c9d2464307b10","observation_id":"fa261d1f-137a-4c9b-aa34-3a595645944c","resolution":{"observed_at":"2026-08-07T14:04:23.387951Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:23.161974Z","title":"Operator quantization of relativistic dynamical systems subject to first class constraints,","venue":null,"work_id":"5dffd465-aa98-45af-96f8-265117111c5a","year":1983},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.183871Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:965fbe3e00f923785224a1c7826f1593cf17e28dcca73a1ec5072bd038d16e96","observation_id":"09b21c56-dda3-49c9-8f6e-13388dde2ceb","resolution":{"observed_at":"2026-08-07T14:04:23.245200Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:22.954420Z","title":"Quantum linearization instabilities of de Sitter space-time. II,","venue":null,"work_id":"da21f847-d06f-4d29-b8ea-089058ddfe10","year":1991},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.191788Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:6f7dbffb3bc7cee5c6115cc2db76ddc03cb0c33c65728bad165249d1fefeee68","observation_id":"ac826ee0-af8f-4056-b0c9-c07fb0e0474a","resolution":{"observed_at":"2026-08-07T14:04:23.046738Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9504018","last_updated":"1995-06-05T16:35:53Z","snapshot_observed_at":"2026-07-07T03:25:18.614600Z","submitted_at":"1995-04-12T21:06:50Z","title":"Quantization of diffeomorphism invariant theories of connections with local degrees of freedom","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9504018","snapshot_observed_at":"2026-08-07T14:04:14.274389Z","title":"Quantization of diffeomorphism invariant theories of connections with local degrees of freedom,","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.274389Z"},"links":{"cited_paper":"/paper/gr-qc/9504018","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:68044712d7e33bee34c745e14fee9da5bb18c847d66d58d5793e3f38e57f765c","observation_id":"07668319-be23-4405-8d0e-49450e9e4242","resolution":{"observed_at":"2026-08-07T14:04:14.274389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9508015","last_updated":"1999-02-10T18:20:42Z","snapshot_observed_at":"2026-07-07T03:25:38.343394Z","submitted_at":"1995-08-07T19:00:50Z","title":"Refined Algebraic Quantization: Systems with a single constraint","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9508015","snapshot_observed_at":"2026-08-07T14:04:14.411092Z","title":"Refined algebraic quantization: systems with a single constraint,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.411092Z"},"links":{"cited_paper":"/paper/gr-qc/9508015","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:4caf2ce7173af6bbc93beb45fd201ca8a171c87e581c74f1f7b26e17e252ab15","observation_id":"30939a53-95dc-4fbc-812c-5b0ce2f73522","resolution":{"observed_at":"2026-08-07T14:04:14.411092Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0011112","last_updated":"2000-11-30T00:02:33Z","snapshot_observed_at":"2026-07-07T03:13:21.978001Z","submitted_at":"2000-11-30T00:02:33Z","title":"Group Averaging and Refined Algebraic Quantization: Where are we now?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0011112","snapshot_observed_at":"2026-08-07T14:04:14.508038Z","title":"Group averaging and refined algebraic quantization: Where are we now?,","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.508038Z"},"links":{"cited_paper":"/paper/gr-qc/0011112","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:dff902d9166ceba460745e3c1d62090e9792b14d2c8153192036e5d2df70d663","observation_id":"afc195e3-708f-4f39-bd21-b1e2d27afbd8","resolution":{"observed_at":"2026-08-07T14:04:14.508038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T14:04:14.620090Z","title":"The Hilbert space of de Sitter JT: a case study for canonical methods in quantum gravity,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.620090Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:335be58c619e19c4a0fdb262f8b9c88357c732cc3ff0bcd342b8f409826c6d2e","observation_id":"0814e507-40e5-4aaa-bdd7-8031395d8d6b","resolution":{"observed_at":"2026-08-07T14:04:14.620090Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9511023","last_updated":"1997-01-07T16:39:14Z","snapshot_observed_at":"2026-07-07T03:25:52.314780Z","submitted_at":"1995-11-06T23:30:22Z","title":"Complex actions in two-dimensional topology change","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9511023","snapshot_observed_at":"2026-08-07T14:04:14.702131Z","title":"Complex actions in two-dimensional topology change,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.702131Z"},"links":{"cited_paper":"/paper/gr-qc/9511023","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:ad528842ba7789b3d14d5b2df17c0a444d65d7cbe3423c608f56c1d35db89ee6","observation_id":"9772c1b3-433a-4517-8852-3bf4c7e5466e","resolution":{"observed_at":"2026-08-07T14:04:14.702131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0004134","last_updated":"2000-06-26T19:17:09Z","snapshot_observed_at":"2026-07-07T04:36:26.761021Z","submitted_at":"2000-04-18T22:56:09Z","title":"Quantization of Four-form Fluxes and Dynamical Neutralization of the Cosmological Constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0004134","snapshot_observed_at":"2026-08-07T14:04:14.822265Z","title":"Quantization of four form fluxes and dynamical neutralization of the cosmological constant,","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.822265Z"},"links":{"cited_paper":"/paper/hep-th/0004134","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:325908adfd09a7f6211870af3be52a961a673df19dd3aaf80d5e14a2d16cc9c5","observation_id":"efd849b6-af99-4bb2-a4f0-5411bdebe9f3","resolution":{"observed_at":"2026-08-07T14:04:14.822265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0302219","last_updated":"2003-02-27T18:57:45Z","snapshot_observed_at":"2026-07-07T04:46:24.743002Z","submitted_at":"2003-02-27T18:57:45Z","title":"The Anthropic Landscape of String Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0302219","snapshot_observed_at":"2026-08-07T14:04:14.915082Z","title":"The Anthropic landscape of string theory,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:14.915082Z"},"links":{"cited_paper":"/paper/hep-th/0302219","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:bd1e2477a4a833b9c88f0ab246cc102d7630c031e35b76099a735c1c91a4a58c","observation_id":"d6f4a1af-ebc7-48a9-bd34-cf8190944230","resolution":{"observed_at":"2026-08-07T14:04:14.915082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0303194","last_updated":"2003-04-24T16:20:28Z","snapshot_observed_at":"2026-07-07T04:46:36.493963Z","submitted_at":"2003-03-21T19:36:16Z","title":"The statistics of string/M theory vacua","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0303194","snapshot_observed_at":"2026-08-07T14:04:15.013068Z","title":"The statistics of string/M theory vacua,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.013068Z"},"links":{"cited_paper":"/paper/hep-th/0303194","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:285f0a491bd324f75aced7e6c67048cc068c84d965d3239b5f34a1f8e97a5069","observation_id":"7d901b7c-1193-4ffe-9659-68bb6298d324","resolution":{"observed_at":"2026-08-07T14:04:15.013068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.09453","last_updated":"2019-04-02T17:08:22Z","snapshot_observed_at":"2026-07-06T07:09:51.109116Z","submitted_at":"2018-10-22T18:00:00Z","title":"Reanalyzing an Evaporating Black Hole","version":4},"cited_work":{"arxiv_id":"1810.09453","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.09453","snapshot_observed_at":"2026-08-07T14:04:20.743033Z","title":"Reanalyzing an Evaporating Black Hole","venue":"hep-th","work_id":"59649181-5325-4b49-b740-b66fbd609dff","year":2018},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.127772Z"},"links":{"cited_paper":"/paper/1810.09453","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:658b553a12d76cd7f7ad6b3e132167e3d5592c41d1a8cf859a86142d916f278c","observation_id":"fefa910a-e8f6-4c20-9a85-8edf30e1b0da","resolution":{"observed_at":"2026-08-07T14:04:20.829561Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.11977","last_updated":"2020-04-15T16:07:46Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2019-11-27T06:30:56Z","title":"Replica wormholes and the black hole interior","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.11977","snapshot_observed_at":"2026-08-07T14:04:15.216645Z","title":"Replica wormholes and the black hole interior,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.216645Z"},"links":{"cited_paper":"/paper/1911.11977","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:8951c048cf5568635c435a0f489e88350645926a55a5f509febd1e4957d1640b","observation_id":"9fa78bd2-9cb7-472e-9281-db8a9172c024","resolution":{"observed_at":"2026-08-07T14:04:15.216645Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.12333","last_updated":"2020-04-24T11:14:44Z","snapshot_observed_at":"2026-08-06T23:22:13.290780Z","submitted_at":"2019-11-27T18:23:34Z","title":"Replica Wormholes and the Entropy of Hawking Radiation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.12333","snapshot_observed_at":"2026-08-07T14:04:15.291080Z","title":"Replica wormholes and the entropy of Hawking radiation,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.291080Z"},"links":{"cited_paper":"/paper/1911.12333","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:23061928117f0f857c541034e2b51ed3625830c2e7c259cda9fce203279e1b63","observation_id":"1b2bae9c-57b1-432a-ac96-b2e64f7f0064","resolution":{"observed_at":"2026-08-07T14:04:15.291080Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.16986","last_updated":"2026-07-07T13:03:36Z","snapshot_observed_at":"2026-08-07T15:59:47.356123Z","submitted_at":"2025-04-23T18:00:00Z","title":"A Nonperturbative Toolkit for Quantum Gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.16986","snapshot_observed_at":"2026-08-07T14:04:15.398322Z","title":"A nonperturbative toolkit for quantum gravity,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.398322Z"},"links":{"cited_paper":"/paper/2504.16986","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:0df45e9366a032e3ecad9c15d23a77272ab85eaab56af79f33187f4b226c146a","observation_id":"62e6f5a0-60fe-4497-9b48-f6bd57dce632","resolution":{"observed_at":"2026-08-07T14:04:15.398322Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2324","last_updated":"2011-04-27T20:54:59Z","snapshot_observed_at":"2026-07-06T02:26:13.600248Z","submitted_at":"2011-04-12T20:00:01Z","title":"Physical Theories, Eternal Inflation, and Quantum Universe","version":2},"cited_work":{"arxiv_id":"1104.2324","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2324","snapshot_observed_at":"2026-08-07T14:04:20.428104Z","title":"Physical Theories, Eternal Inflation, and Quantum Universe","venue":"hep-th","work_id":"21a6c59e-e165-4f46-8698-f5e2b9ea8a54","year":2011},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.515443Z"},"links":{"cited_paper":"/paper/1104.2324","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:adef983618e40157921d245eb48591a8b7032583efbfb18e6f4aa7a8739c52c2","observation_id":"832449fe-abf2-4dea-b985-34581b4820e4","resolution":{"observed_at":"2026-08-07T14:04:20.496108Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06738","last_updated":"2020-08-19T16:34:28Z","snapshot_observed_at":"2026-08-06T09:32:58.264223Z","submitted_at":"2020-04-14T18:01:02Z","title":"Baby Universes, Holography, and the Swampland","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.06738","snapshot_observed_at":"2026-08-07T14:04:15.602849Z","title":"Baby universes, holography, and the swampland,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.602849Z"},"links":{"cited_paper":"/paper/2004.06738","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:d7a1b36b3b9c8855657f203afe91f777f6482bf74679b6b91e8cd170c9055fc5","observation_id":"a1457e93-fc39-4a71-be4d-ed0e3a6cb378","resolution":{"observed_at":"2026-08-07T14:04:15.602849Z","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":"2026-08-07T14:04:22.711530Z","title":"Anthropic bound on the cosmological constant,","venue":null,"work_id":"d90df946-b73b-4428-b2d6-2be966362e4e","year":1987},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.724749Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:aaf6da9d2d25c74da3b1ae0a6813e677b27463ad6e397f195939062291277bcf","observation_id":"0b404abf-66de-468f-a047-819ddb75789c","resolution":{"observed_at":"2026-08-07T14:04:22.846764Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9406010","last_updated":"1994-10-27T22:06:00Z","snapshot_observed_at":"2026-07-07T03:24:45.763672Z","submitted_at":"1994-06-06T10:35:27Z","title":"Predictions from Quantum Cosmology","version":2},"cited_work":{"arxiv_id":"gr-qc/9406010","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9406010","snapshot_observed_at":"2026-08-07T14:04:20.148827Z","title":"Predictions from Quantum Cosmology","venue":"gr-qc","work_id":"a95bd9b0-cf52-4832-92ca-26811ce08497","year":1994},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.841488Z"},"links":{"cited_paper":"/paper/gr-qc/9406010","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:a53db8750217f6ab2cc39c055d6de9b8a153d9c1f2f591bd08b377950148a023","observation_id":"02c43828-bd1a-4d37-a18f-5a79d5fcf3a5","resolution":{"observed_at":"2026-08-07T14:04:20.227951Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0712.2454","last_updated":"2007-12-17T14:43:08Z","snapshot_observed_at":"2026-07-06T01:36:36.760739Z","submitted_at":"2007-12-17T14:43:08Z","title":"Evidence for the Multiverse in the Standard Model and Beyond","version":1},"cited_work":{"arxiv_id":"0712.2454","doi":null,"metadata_source":"pith","pith_arxiv_id":"0712.2454","snapshot_observed_at":"2026-08-07T14:04:19.966161Z","title":"Evidence for the Multiverse in the Standard Model and Beyond","venue":"hep-ph","work_id":"6aaffaac-27aa-4f4c-a0e5-9bc89e4ff754","year":2007},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:15.943392Z"},"links":{"cited_paper":"/paper/0712.2454","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:6e7f2913016f26574521dbaf525aefc320a9f9060f25a2aa9058b813d4ff71e0","observation_id":"d0a4360f-e131-4a5e-87e8-26980450ee07","resolution":{"observed_at":"2026-08-07T14:04:20.031881Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.03580","last_updated":"2016-04-12T20:50:31Z","snapshot_observed_at":"2026-07-06T04:52:39.631930Z","submitted_at":"2016-04-12T20:50:31Z","title":"One Bubble to Rule Them All","version":1},"cited_work":{"arxiv_id":"1604.03580","doi":null,"metadata_source":"pith","pith_arxiv_id":"1604.03580","snapshot_observed_at":"2026-08-07T14:04:19.664947Z","title":"One Bubble to Rule Them All","venue":"hep-th","work_id":"872c7fe0-f462-49ac-8597-d47b9e8d9abd","year":2016},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.056516Z"},"links":{"cited_paper":"/paper/1604.03580","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:7c8bbf79c6844771d2c02a79338917ffbf209d40bf9ab39d394d88900d8af337","observation_id":"401a5554-d946-4071-84ed-fe875eb5c36a","resolution":{"observed_at":"2026-08-07T14:04:19.778653Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.14218","last_updated":"2024-10-02T00:44:35Z","snapshot_observed_at":"2026-08-03T05:31:13.365957Z","submitted_at":"2024-09-21T18:41:16Z","title":"The no boundary density matrix","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.14218","snapshot_observed_at":"2026-08-07T14:04:16.169986Z","title":"The no boundary density matrix,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.169986Z"},"links":{"cited_paper":"/paper/2409.14218","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:80c1c1ad1f1641b74ad4a88810a7b1d3ee7522cfd17528fc370de61496ce85fe","observation_id":"11f5b6d1-ef7e-435b-abce-82f4d6211566","resolution":{"observed_at":"2026-08-07T14:04:16.169986Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.05340","last_updated":"2017-06-13T22:51:50Z","snapshot_observed_at":"2026-07-06T05:42:42.520454Z","submitted_at":"2017-05-15T17:15:09Z","title":"The Real No-Boundary Wave Function in Lorentzian Quantum Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.05340","snapshot_observed_at":"2026-08-07T14:04:16.294139Z","title":"Real no-boundary wave function in Lorentzian quantum cosmology,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.294139Z"},"links":{"cited_paper":"/paper/1705.05340","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:2d5263111a7133e47cf4bbec0587c07a071e88ae39cf230174b7ba9a2d6e97b1","observation_id":"962d13b7-42ba-4f87-9ba0-40b4b4457e12","resolution":{"observed_at":"2026-08-07T14:04:16.294139Z","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":"2026-08-07T14:04:22.524840Z","title":"Pointer basis of quantum apparatus: Into what mixture does the wave packet collapse?,","venue":null,"work_id":"fb4cf91c-3576-47aa-bedf-6518f49caf09","year":1981},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.411307Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:f050364e42d1e8744edabf5520200adfad4b8a9607769faae2a164c057575575","observation_id":"da269a63-7665-4602-91cf-c4ade8f31370","resolution":{"observed_at":"2026-08-07T14:04:22.601199Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"quant-ph/0105127","last_updated":"2003-06-19T18:28:36Z","snapshot_observed_at":"2026-07-07T07:06:00.302233Z","submitted_at":"2001-05-24T21:20:33Z","title":"Decoherence, einselection, and the quantum origins of the classical","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"quant-ph/0105127","snapshot_observed_at":"2026-08-07T14:04:16.525913Z","title":"Decoherence, einselection, and the quantum origins of the classical,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.525913Z"},"links":{"cited_paper":"/paper/quant-ph/0105127","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:d35effe36652e944325c835e3be204c2d97b229e59d31651dea78c91a8362b0f","observation_id":"c6de9f1f-8739-47b4-8345-288e6364f69a","resolution":{"observed_at":"2026-08-07T14:04:16.525913Z","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":"2026-08-07T14:04:22.303653Z","title":"Evolution without evolution: dynamics described by stationary observables,","venue":null,"work_id":"27d3854a-ed67-4eab-ac8c-d9eb2272ffbb","year":1983},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.641990Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:138cd5b824402c8d1785ee6285374c4934b7f7b06044652c919fab5407310877","observation_id":"734a3636-0f0b-4a31-aaea-243500c04acc","resolution":{"observed_at":"2026-08-07T14:04:22.407783Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.4630","last_updated":"2012-05-08T20:32:03Z","snapshot_observed_at":"2026-07-06T02:36:10.003031Z","submitted_at":"2011-10-20T20:00:01Z","title":"Quantum Mechanics, Spacetime Locality, and Gravity","version":3},"cited_work":{"arxiv_id":"1110.4630","doi":null,"metadata_source":"pith","pith_arxiv_id":"1110.4630","snapshot_observed_at":"2026-08-07T14:04:19.223386Z","title":"Quantum Mechanics, Spacetime Locality, and Gravity","venue":"hep-th","work_id":"e14aa1f0-9453-4873-941f-00f1beb747a8","year":2011},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.744786Z"},"links":{"cited_paper":"/paper/1110.4630","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:51fec4b11732784239450a29b5face9a6988c9c8ebc3842483d149d6cbb62d90","observation_id":"75725514-4bf1-4ddb-9659-5b4ea9af6ef8","resolution":{"observed_at":"2026-08-07T14:04:19.293305Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3770","last_updated":"2009-01-14T19:25:00Z","snapshot_observed_at":"2026-07-06T01:43:45.088115Z","submitted_at":"2008-08-27T20:00:57Z","title":"Properties of the scale factor measure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3770","snapshot_observed_at":"2026-08-07T14:04:16.823378Z","title":"Properties of the scale factor measure,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.823378Z"},"links":{"cited_paper":"/paper/0808.3770","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:6bc101efd24a8b7d758c4272205a527dff44b78f2a32c77aa87c974d749c60ca","observation_id":"432abd0d-36f4-4d79-83f2-357dd0203847","resolution":{"observed_at":"2026-08-07T14:04:16.823378Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.7540","last_updated":"2013-04-24T16:31:57Z","snapshot_observed_at":"2026-07-06T02:58:38.977337Z","submitted_at":"2012-10-29T01:28:26Z","title":"Watchers of the multiverse","version":3},"cited_work":{"arxiv_id":"1210.7540","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.7540","snapshot_observed_at":"2026-08-07T14:04:18.987263Z","title":"Watchers of the multiverse","venue":"hep-th","work_id":"5374fb3c-0943-4f58-a33b-af61ba09f942","year":2012},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:16.932190Z"},"links":{"cited_paper":"/paper/1210.7540","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:91052599ea4aa4beeb58daf41feb5f0f565311fbb20afef11f47433f7630a693","observation_id":"62738bed-2fb2-4f81-bc6c-c956f2597857","resolution":{"observed_at":"2026-08-07T14:04:19.069179Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:17.008475Z","title":"A local Wheeler-DeWitt measure for the string landscape,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:17.008475Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:3a2602a8009295a1915d69034fc25d04f1df6a0e2a7e82af915cd8260257e30f","observation_id":"ea2d2876-691d-4a12-b19a-37b1eefbcf44","resolution":{"observed_at":"2026-08-07T14:04:17.008475Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.5550","last_updated":"2012-05-26T09:10:18Z","snapshot_observed_at":"2026-08-06T09:14:04.016411Z","submitted_at":"2012-05-24T19:59:41Z","title":"The Static Quantum Multiverse","version":2},"cited_work":{"arxiv_id":"1205.5550","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.5550","snapshot_observed_at":"2026-08-07T14:04:18.542140Z","title":"The Static Quantum Multiverse","venue":"hep-th","work_id":"bed4f600-ff53-4189-8632-b9b6bf3da045","year":2012},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:17.078993Z"},"links":{"cited_paper":"/paper/1205.5550","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:4a19a9fa4a48995bb3dc690954d187cddaa37cc728a9e47cdf2d4406038b34c4","observation_id":"8ee733bd-77ad-4ff1-8fbb-a763b8f6ac04","resolution":{"observed_at":"2026-08-07T14:04:18.653038Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1202.5037","last_updated":"2012-02-22T21:00:05Z","snapshot_observed_at":"2026-08-04T05:24:27.898430Z","submitted_at":"2012-02-22T21:00:05Z","title":"Spatial Curvature Falsifies Eternal Inflation","version":1},"cited_work":{"arxiv_id":"1202.5037","doi":null,"metadata_source":"pith","pith_arxiv_id":"1202.5037","snapshot_observed_at":"2026-08-07T14:04:18.336128Z","title":"Spatial Curvature Falsifies Eternal Inflation","venue":"astro-ph.CO","work_id":"a6768b50-1bf6-4430-bc2d-be46555b3ee1","year":2012},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:17.164003Z"},"links":{"cited_paper":"/paper/1202.5037","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:83975e7a362bb1c34a74cd419d139e39753f14d047ddb036346c601c45fb9603","observation_id":"49f6d79e-13f5-4482-9d7b-6c23ba4b4567","resolution":{"observed_at":"2026-08-07T14:04:18.410361Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1203.6876","last_updated":"2012-07-24T15:12:21Z","snapshot_observed_at":"2026-07-06T02:45:30.916199Z","submitted_at":"2012-03-30T18:01:23Z","title":"What can the observation of nonzero curvature tell us?","version":2},"cited_work":{"arxiv_id":"1203.6876","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.6876","snapshot_observed_at":"2026-08-07T14:04:18.091221Z","title":"What can the observation of nonzero curvature tell us?","venue":"hep-th","work_id":"9f79c902-0ae0-4b85-b8ee-1dbb03cfeb4b","year":2012},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:17.281984Z"},"links":{"cited_paper":"/paper/1203.6876","citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:48bd89b7b3f1d390d8251f8232ec167e723f199f08166bafa4576d10d055c710","observation_id":"afe99c40-cd9a-4c66-b6be-dac09cb65683","resolution":{"observed_at":"2026-08-07T14:04:18.191236Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-07T14:04:17.435922Z","title":"Absolute entropy and the observer’s no-boundary state,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:17.435922Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:21dc063290969442b11e606fae047df88483aefc61944fec56d7fe1e789a4e8b","observation_id":"03913c8b-ffce-4450-b778-ff34e251d196","resolution":{"observed_at":"2026-08-07T14:04:17.435922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T14:04:17.561732Z","title":"Observers seeing gravitational Hilbert spaces: abstract sources for an abstract path integral,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-07T14:04:17.561732Z"},"links":{"citing_paper":"/paper/2505.20390"},"observation_digest":"sha256:9602976510da05242d7381b36bed2e58e0b913e14d9eb6ce397962cfb2cfba26","observation_id":"32b15af3-1e7b-488a-8d16-8a85948d720f","resolution":{"observed_at":"2026-08-07T14:04:17.561732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.20390","last_updated":"2025-06-16T06:07:08Z","latest_version":2,"primary_category":"hep-th","snapshot_observed_at":"2026-08-07T13:53:12.083770Z","submitted_at":"2025-05-26T18:00:00Z","title":"Nonperturbative Quantum Gravity in a Closed Lorentzian Universe"},"reference_resolution":{"displayed":58,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":35,"verified_exact":10,"verified_fuzzy":13},"total_outbound_references":58},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 58 of 58 outbound references and 9 inbound Pith citation observations for arXiv:2505.20390."}