{"as_of":"2026-08-09T17:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f77c258df35982ffcff2394dbdb73ad3a199785ea9dfb48a3c4fb732ade951d0","coverage":[{"denominator":298,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T12:50:17.418018Z","state":"measured"},{"denominator":105,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":105,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T06:32:00.677563Z","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":"2026-07-04T12:09:49.180374Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"cited_work":{"arxiv_id":"2502.07437","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.07437","snapshot_observed_at":"2026-07-04T12:09:49.180374Z","title":"Mandal and S","venue":null,"work_id":"82f066e5-a547-45d1-ba5a-8efe2a566566","year":2025},"citing_paper":{"arxiv_id":"2511.14047","last_updated":"2026-04-16T11:45:43Z","snapshot_observed_at":"2026-08-02T23:25:19.429899Z","submitted_at":"2025-11-18T01:52:43Z","title":"Exact, non-singular black holes from a phantom DBI Field as primordial dark matter","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-17T21:33:04.666578Z"},"links":{"cited_paper":"/paper/2502.07437","citing_paper":"/paper/2511.14047"},"observation_digest":"sha256:eed7a86db11a4a7716b2f2b386764998dab4cc48dccd82c9ba45f88b52a0e68b","observation_id":"f3337fd0-4726-4b99-97a1-868f93b6dc7f","resolution":{"observed_at":"2026-05-17T21:35:17.827846Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"cited_work":{"arxiv_id":"2502.07437","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.07437","snapshot_observed_at":"2026-07-04T12:09:49.180374Z","title":"Mandal and S","venue":null,"work_id":"82f066e5-a547-45d1-ba5a-8efe2a566566","year":2025},"citing_paper":{"arxiv_id":"2602.04593","last_updated":"2026-04-14T10:02:17Z","snapshot_observed_at":"2026-07-06T22:44:33.166340Z","submitted_at":"2026-02-04T14:19:10Z","title":"Emergent Hawking Radiation and Quantum Sensing in a Quenched Chiral Spin Chain","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-16T07:18:20.594827Z"},"links":{"cited_paper":"/paper/2502.07437","citing_paper":"/paper/2602.04593"},"observation_digest":"sha256:b64c4cb4a3a61bf7bdeb505b3716ef731caace6dd5bdc18ccdc7556832da53c6","observation_id":"adedf8cd-a69d-4e46-b17a-4a310b1e06d9","resolution":{"observed_at":"2026-05-16T07:20:43.856564Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"cited_work":{"arxiv_id":"2502.07437","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.07437","snapshot_observed_at":"2026-07-04T12:09:49.180374Z","title":"Mandal and S","venue":null,"work_id":"82f066e5-a547-45d1-ba5a-8efe2a566566","year":2025},"citing_paper":{"arxiv_id":"2605.13042","last_updated":"2026-05-13T05:54:23Z","snapshot_observed_at":"2026-07-06T23:24:37.915639Z","submitted_at":"2026-05-13T05:54:23Z","title":"The Gravitational Spectral Radio Forest: A Signature of Primordial Black Holes","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-14T19:08:52.224510Z"},"links":{"cited_paper":"/paper/2502.07437","citing_paper":"/paper/2605.13042"},"observation_digest":"sha256:8da5836ecc69e2ccbc3ea108a71161d45bf2358da1e6d869cfb9bb502be129cb","observation_id":"84872894-8c62-4200-9358-109abfd20991","resolution":{"observed_at":"2026-05-14T19:09:23.029011Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"cited_work":{"arxiv_id":"2502.07437","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.07437","snapshot_observed_at":"2026-07-04T12:09:49.180374Z","title":"Mandal and S","venue":null,"work_id":"82f066e5-a547-45d1-ba5a-8efe2a566566","year":2025},"citing_paper":{"arxiv_id":"2606.23846","last_updated":"2026-08-04T11:29:48Z","snapshot_observed_at":"2026-08-07T23:11:39.653838Z","submitted_at":"2026-06-22T18:29:10Z","title":"Primordial Black Holes: A Review of Formation and Evolution","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-06-26T07:13:12.429183Z"},"links":{"cited_paper":"/paper/2502.07437","citing_paper":"/paper/2606.23846"},"observation_digest":"sha256:1870d50305f796fddb162800ce59d04caf3043701ff2161347c371e09ee42711","observation_id":"3bf6497f-9029-4207-9d8c-8595a06c9d31","resolution":{"observed_at":"2026-07-04T12:09:49.181573Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.07437","snapshot_observed_at":"2026-08-02T06:32:00.677563Z","title":"Mandal and S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.13109","last_updated":"2026-07-14T10:27:17Z","snapshot_observed_at":"2026-08-09T09:21:37.874054Z","submitted_at":"2026-07-14T10:27:17Z","title":"Reconstruction of f(G) Gravity from an Interacting Viscous Generalized QCD Ghost Dark Energy Model: Cosmology and Thermodynamics: Cosmology and Thermodynamics","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-02T06:32:00.677563Z"},"links":{"cited_paper":"/paper/2502.07437","citing_paper":"/paper/2607.13109"},"observation_digest":"sha256:a1f68fe16329d4bcfec729e7411300834f3233c2477058df7e075cef7b45ccb6","observation_id":"8afbb6d5-86c7-4d53-a51c-31a9edea164b","resolution":{"observed_at":"2026-08-02T06:32:00.677563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2502.07437/citation-record","integrity":"/paper/2502.07437/integrity","json":"/paper/2502.07437/citation-record.json","paper":"/paper/2502.07437"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T12:50:16.913981Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.913981Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:f077a01d9cca25f1ec319622b0770ec84aa18e9815c1b7dcccc2d8389ebd7f01","observation_id":"9216aa45-063c-4865-9919-611076285052","resolution":{"observed_at":"2026-08-08T12:50:16.913981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.04248","last_updated":"2024-07-26T22:16:00Z","snapshot_observed_at":"2026-08-06T07:57:05.327375Z","submitted_at":"2024-04-05T17:54:11Z","title":"Observation of Gravitational Waves from the Coalescence of a $2.5\\text{-}4.5~M_\\odot$ Compact Object and a Neutron Star","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.04248","snapshot_observed_at":"2026-08-08T12:50:16.920701Z","title":"( collaboration LIGO Scientific, Virgo,, KAGRA, VIRGO ) ( year 2024 )","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.920701Z"},"links":{"cited_paper":"/paper/2404.04248","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:1b6ef0d3a21fa437ab7d599765dee88754809f0e2e2c891da552129f7654675a","observation_id":"b77693b3-4d7f-4e0b-a15e-5a7afbc4afaf","resolution":{"observed_at":"2026-08-08T12:50:16.920701Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-08-08T12:50:16.926365Z","title":"( collaboration LIGO Scientific, Virgo ) ( year 2016 )","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.926365Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ee2e4ddbcb0f134a37f0a49902f60060eca17936e5b0b0ea3639685f7d3c14df","observation_id":"6e7061c0-e11a-4f15-ae84-01c4c2d3ef8f","resolution":{"observed_at":"2026-08-08T12:50:16.926365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-08T12:50:16.932410Z","title":"( collaboration LIGO Scientific, Virgo ) ( year 2017 a )","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.932410Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ef9e1257a9f2f3215e50ee272e40063293321b3d2abf7988eb54a206decdb1b1","observation_id":"5db69a13-6717-42b1-90c2-a131e79238e2","resolution":{"observed_at":"2026-08-08T12:50:16.932410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01940","last_updated":"2017-02-24T18:18:21Z","snapshot_observed_at":"2026-07-06T05:06:08.294944Z","submitted_at":"2016-08-05T17:06:57Z","title":"The basic physics of the binary black hole merger GW150914","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01940","snapshot_observed_at":"2026-08-08T12:50:16.938278Z","title":"( collaboration LIGO Scientific, Virgo ) ( year 2017 b )","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.938278Z"},"links":{"cited_paper":"/paper/1608.01940","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:84dd88c46a0bd9cf71770462c28d87f5671d3001be14f2987c0d33376d1650c2","observation_id":"ca9b984f-3ae2-4894-bc5c-30eefa96f38e","resolution":{"observed_at":"2026-08-08T12:50:16.938278Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-08-08T12:50:16.944033Z","title":"( collaboration LIGO Scientific, Virgo ) ( year 2019 )","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.944033Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:4196cfc715e1e5870ef94c91550e11295dcb41bfade3c27bb4cb0f6a570bb3f8","observation_id":"5584f5bd-5521-4f52-96ca-cea7f5c5f8ce","resolution":{"observed_at":"2026-08-08T12:50:16.944033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14529","last_updated":"2025-09-10T17:43:53Z","snapshot_observed_at":"2026-08-07T22:54:59.574514Z","submitted_at":"2020-10-27T18:01:34Z","title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.14529","snapshot_observed_at":"2026-08-08T12:50:16.949806Z","title":"( collaboration LIGO Scientific, Virgo ) ( year 2021 a )","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.949806Z"},"links":{"cited_paper":"/paper/2010.14529","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:34676485dedf9d518451d1a4a9c75a7c8bbf7ae4f95f68e209fc7ae7ff85a956","observation_id":"1c502d3f-8cc0-4879-a4b2-85f739cde342","resolution":{"observed_at":"2026-08-08T12:50:16.949806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06861","last_updated":"2025-11-17T15:05:31Z","snapshot_observed_at":"2026-08-02T22:41:06.793496Z","submitted_at":"2021-12-13T18:19:04Z","title":"Tests of General Relativity with GWTC-3","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06861","snapshot_observed_at":"2026-08-08T12:50:16.955838Z","title":"( collaboration LIGO Scientific, VIRGO, KAGRA ) ( year 2021 b ), month 12","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.955838Z"},"links":{"cited_paper":"/paper/2112.06861","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:c24f6ff8b70805b55c68594de699791d582bff006aae051e5ce717041909c27f","observation_id":"6bc5d415-db6d-454f-9ccb-cffca72e93b3","resolution":{"observed_at":"2026-08-08T12:50:16.955838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03606","last_updated":"2023-10-23T13:37:50Z","snapshot_observed_at":"2026-08-08T16:18:10.684162Z","submitted_at":"2021-11-05T16:43:17Z","title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.03606","snapshot_observed_at":"2026-08-08T12:50:16.961179Z","title":"( collaboration KAGRA, VIRGO, LIGO Scientific ) ( year 2023 )","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.961179Z"},"links":{"cited_paper":"/paper/2111.03606","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:31f070099ffb54cb151f404c8aec13980c2471fd1183d4e3fe06c9f60ad99216","observation_id":"d6c4ffeb-99d0-4b5b-9e8a-daaa8a5383da","resolution":{"observed_at":"2026-08-08T12:50:16.961179Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01045","last_updated":"2022-05-10T14:16:51Z","snapshot_observed_at":"2026-07-29T23:10:57.700271Z","submitted_at":"2021-08-02T17:09:29Z","title":"GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.01045","snapshot_observed_at":"2026-08-08T12:50:16.966429Z","title":"( collaboration LIGO Scientific, VIRGO ) ( year 2024 )","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.966429Z"},"links":{"cited_paper":"/paper/2108.01045","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:d0a05ff1161122150681d35e6f3432e167695d6abc2fa2370acada74c24dc976","observation_id":"34b1a20a-e6dd-492b-8f85-88c819bfdf37","resolution":{"observed_at":"2026-08-08T12:50:16.966429Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.09409","last_updated":"2018-07-25T01:36:07Z","snapshot_observed_at":"2026-07-06T06:52:08.229941Z","submitted_at":"2018-07-25T01:36:07Z","title":"Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.09409","snapshot_observed_at":"2026-08-08T12:50:16.971694Z","title":"( collaboration GRAVITY ) ( year 2018 )","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.971694Z"},"links":{"cited_paper":"/paper/1807.09409","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:0de05a921b07a4ca6edb9231377fb04bd18e367ccec4b926fd423018a081f378","observation_id":"929d4a4c-c3ca-45c2-b5c9-56a204130ec0","resolution":{"observed_at":"2026-08-08T12:50:16.971694Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.43.965","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T12:50:18.894506Z","title":"title Constraints on the scalar field potential in inflationary models","venue":null,"work_id":"7d8cad64-80a0-41ed-8cd3-84bd9a966901","year":1991},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.976975Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:a9b56725dd5a1dc34969d325f896dd8ebb7e41f8558823944fca98e90343d285","observation_id":"578031e6-d377-42f0-8568-3474ea062623","resolution":{"observed_at":"2026-08-08T12:50:18.899873Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T12:50:16.982029Z","title":"( year 2022 a )","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.982029Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:4ba19a6f328bfb1cecab278bc5d34532f58dc1671fc9270beab71543dd08c4ac","observation_id":"4dd5a929-f195-4814-a3d3-e6d361cd6766","resolution":{"observed_at":"2026-08-08T12:50:16.982029Z","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":"2026-08-08T12:50:16.986869Z","title":"( collaboration LHAASO ) ( year 2022 b )","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.986869Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:91e7635e1040425cad4a6195c2f29b21a6e2b7f20b33e78581cd1a2d42d002fb","observation_id":"56ea2309-4ef8-430d-ab4b-ca8679d92e0d","resolution":{"observed_at":"2026-08-08T12:50:16.986869Z","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":"2026-08-08T12:50:16.991595Z","title":"title New tests of einstein's equivalence principle and newton's inverse-square law","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.991595Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:8cd62de4af8816320603761e19b75f6ae5762cf5f3c807d9239be1fc1cc66553","observation_id":"63ca37a6-0e79-490b-9fe8-3f34e4fad1cd","resolution":{"observed_at":"2026-08-08T12:50:16.991595Z","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":"2026-08-08T12:50:16.996354Z","title":"( year 2021 )","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:16.996354Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:f5493fbfeabe0a25c019348d8021f1615f96c1d4186a018c15424647a6b5493c","observation_id":"f2553658-43c9-4432-9299-fa4a2d230f7c","resolution":{"observed_at":"2026-08-08T12:50:16.996354Z","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":"2026-08-08T12:50:17.001365Z","title":"( collaboration Event Horizon Telescope ) ( year 2019 a )","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.001365Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:8b2ba5dca41de18e6e3f82cfa22ccbced0e3bc68b12ab96ce28da4347b2a5b34","observation_id":"c8afdc0a-5250-465f-92fc-2138ad6dfc4d","resolution":{"observed_at":"2026-08-08T12:50:17.001365Z","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":"2026-08-08T12:50:17.006429Z","title":"( collaboration Event Horizon Telescope ) ( year 2019 b )","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.006429Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:cfaf20dd1d98c6676278f112b75898928d71482b9336e53ceed5a01d0e2309e5","observation_id":"369df199-2c7a-41c1-9301-625a9d00176e","resolution":{"observed_at":"2026-08-08T12:50:17.006429Z","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":"2026-08-08T12:50:17.011334Z","title":"( collaboration Event Horizon Telescope ) ( year 2019 c )","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.011334Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:e5461a562342b607f8054b1d4c2cba832982cec50b792a0d2406b0040ba273ee","observation_id":"1693cbec-f55d-46d7-a6e7-1064ba03e4e6","resolution":{"observed_at":"2026-08-08T12:50:17.011334Z","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":"2026-08-08T12:50:17.016521Z","title":"( collaboration Event Horizon Telescope ) ( year 2022 a )","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.016521Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:61056ab31d51548978585f08e97b877a8d3f29634f7e660ca964c7c6ec4d657c","observation_id":"1df9bf98-c771-46c3-9ab5-e4aa2bc427e0","resolution":{"observed_at":"2026-08-08T12:50:17.016521Z","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":"2026-08-08T12:50:17.021434Z","title":"( collaboration Event Horizon Telescope ) ( year 2022 b )","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.021434Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ed7bbc33ddbd6d9d75d539f9db74085724cbc5dfba011be03e5480f281a9f11c","observation_id":"983d6d57-f038-438a-a510-1dec5a1205e6","resolution":{"observed_at":"2026-08-08T12:50:17.021434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.05697","last_updated":"2019-05-14T16:19:37Z","snapshot_observed_at":"2026-07-06T07:52:57.535245Z","submitted_at":"2019-05-14T16:19:37Z","title":"Planck 2018 results. IX. Constraints on primordial non-Gaussianity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.05697","snapshot_observed_at":"2026-08-08T12:50:17.026525Z","title":"( collaboration Planck ) ( year 2020 a )","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.026525Z"},"links":{"cited_paper":"/paper/1905.05697","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:30a8a45dc5c18d8bec0ad415c8a715139fb620ce3cc2d7b90c83e9250793b7ed","observation_id":"48ba96c9-9f28-4f17-9daf-c62c5bc66018","resolution":{"observed_at":"2026-08-08T12:50:17.026525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06211","last_updated":"2019-08-02T11:42:17Z","snapshot_observed_at":"2026-08-02T20:50:08.912618Z","submitted_at":"2018-07-17T04:05:09Z","title":"Planck 2018 results. X. Constraints on inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06211","snapshot_observed_at":"2026-08-08T12:50:17.031932Z","title":"( collaboration Planck ) ( year 2020 b )","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.031932Z"},"links":{"cited_paper":"/paper/1807.06211","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:6f8da68e68761b2a95f8e24ac63cf38c0632896330435e6d8ed26b61faca7612","observation_id":"a9f3bb6d-9924-4434-994e-2e8f150b9720","resolution":{"observed_at":"2026-08-08T12:50:17.031932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.4094","last_updated":"2008-08-09T09:33:37Z","snapshot_observed_at":"2026-07-06T01:35:49.862060Z","submitted_at":"2008-03-28T12:55:44Z","title":"Search for a stochastic background of 100-MHz gravitational waves with laser interferometers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.4094","snapshot_observed_at":"2026-08-08T12:50:17.037288Z","title":"( year 2008 )","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.037288Z"},"links":{"cited_paper":"/paper/0803.4094","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:df7da00b5779e9cd8e5487555238400d00c6bc38eb8f387fea4eb20e50a0a364","observation_id":"4c45e11e-57bb-4e33-bd9e-ccc329c446f5","resolution":{"observed_at":"2026-08-08T12:50:17.037288Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.06490","last_updated":"2020-12-23T17:40:07Z","snapshot_observed_at":"2026-08-04T01:07:32.912038Z","submitted_at":"2020-05-13T18:00:37Z","title":"The NANOGrav 12.5 yr Data Set: Observations and Narrowband Timing of 47 Millisecond Pulsars","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.06490","snapshot_observed_at":"2026-08-08T12:50:17.042895Z","title":"( collaboration NANOGrav ) ( year 2021 )","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.042895Z"},"links":{"cited_paper":"/paper/2005.06490","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:616b6e74319e55f8d14e3d49343476fd4b0d99fb345799edae7764feb7f234e9","observation_id":"d588d3f6-092e-435b-a50f-2066632ece24","resolution":{"observed_at":"2026-08-08T12:50:17.042895Z","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":"2026-08-08T12:50:17.048592Z","title":"title Massive gravity on curved background","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.048592Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:b4333a331cb058375c214d9848cabbaa076841abe540882f41757a9c4d804042","observation_id":"a7b54325-1153-4c9f-924c-7a5d195175d5","resolution":{"observed_at":"2026-08-08T12:50:17.048592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0907.2562","last_updated":"2009-08-16T13:32:43Z","snapshot_observed_at":"2026-07-06T01:56:36.639996Z","submitted_at":"2009-07-15T11:27:37Z","title":"Chern-Simons Modified General Relativity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.2562","snapshot_observed_at":"2026-08-08T12:50:17.053419Z","title":"title Chern-Simons Modified General Relativity","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.053419Z"},"links":{"cited_paper":"/paper/0907.2562","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:88ef138fc2993fc3d98a098765d78d415053755a16f221942fbe91252cb18eef","observation_id":"cde31dbf-a52a-4a90-b811-a10516328dea","resolution":{"observed_at":"2026-08-08T12:50:17.053419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0403069","last_updated":"2014-03-15T06:17:32Z","snapshot_observed_at":"2026-08-06T11:23:07.395458Z","submitted_at":"2004-03-05T20:07:42Z","title":"Leptogenesis from Gravity Waves in Models of Inflation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0403069","snapshot_observed_at":"2026-08-08T12:50:17.059193Z","title":"title Leptogenesis from gravity waves in models of inflation","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.059193Z"},"links":{"cited_paper":"/paper/hep-th/0403069","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:2ab42fbe28ca3f2aa58e056d4abfe532fd9c3543a9627476a23f0885b70fe8b2","observation_id":"e6a096cd-5ee5-4b92-b009-f0e6938507a3","resolution":{"observed_at":"2026-08-08T12:50:17.059193Z","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":"2026-08-08T12:50:17.064803Z","title":"title Tunnelling and dynamical violation of the null energy condition","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.064803Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:26cb038c69bac057f6b43c8527dec32d4df153d513cc13c9808ac72f6932135b","observation_id":"fb4b6381-b8db-41e9-b37e-15a943db4bdd","resolution":{"observed_at":"2026-08-08T12:50:17.064803Z","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":"2026-08-08T12:50:17.069900Z","title":"title Quantum gravity and lorentz invariance violation in the standard model","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.069900Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:4905ef1273dbab854be31aa64d0dcb5a37a3ba7b0a2696a4e1db259ebc280da5","observation_id":"76127873-5946-4995-8c6c-250bb891df87","resolution":{"observed_at":"2026-08-08T12:50:17.069900Z","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":"2026-08-08T12:50:17.074957Z","title":"title Slowly rotating black hole solutions to ho r ava-lifshitz gravity","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.074957Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ca3ed12f8c47cfeed83086b1d54909d36553b276ec6faddd8d04f30ce5cff927","observation_id":"2d8487bb-6a8f-4946-af3d-8fd0086cc728","resolution":{"observed_at":"2026-08-08T12:50:17.074957Z","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":"2026-08-08T12:50:17.079852Z","title":"( year 2020 )","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.079852Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:0c3546230e0887dd88032fe471fd6622da42b09b6eb94251013c663402947bad","observation_id":"ce13b27f-daaa-4b02-963c-1e6d362b9c4a","resolution":{"observed_at":"2026-08-08T12:50:17.079852Z","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":"2026-08-08T12:50:17.084815Z","title":"title Quantum-Spacetime phenomenology","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.084815Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:9201bc54c5113e582a84fe4cc08484295131ba62300a0b6d93a750e4dfcfb866","observation_id":"39fbbd91-4153-4fde-a444-996e533a4460","resolution":{"observed_at":"2026-08-08T12:50:17.084815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.02686","last_updated":"2020-06-02T21:49:26Z","snapshot_observed_at":"2026-07-06T09:02:29.692391Z","submitted_at":"2020-03-04T16:21:27Z","title":"Scaling solutions and weak gravity in dark energy with energy and momentum couplings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.02686","snapshot_observed_at":"2026-08-08T12:50:17.090054Z","title":"title Scaling solutions and weak gravity in dark energy with energy and momentum couplings","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.090054Z"},"links":{"cited_paper":"/paper/2003.02686","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:56dc1b294492d95d8c61c79ad8e3d918f8faff2af895c74993946fb24faff4a4","observation_id":"dfe3c06e-f593-4eb9-af1f-e75a1f110f69","resolution":{"observed_at":"2026-08-08T12:50:17.090054Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0612180","last_updated":"2007-03-14T01:35:47Z","snapshot_observed_at":"2026-07-07T03:23:34.977372Z","submitted_at":"2006-12-28T14:17:09Z","title":"Conditions for the cosmological viability of f(R) dark energy models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0612180","snapshot_observed_at":"2026-08-08T12:50:17.095492Z","title":"title Conditions for the cosmological viability of f(R) dark energy models","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.095492Z"},"links":{"cited_paper":"/paper/gr-qc/0612180","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:1f5ff8b42c7bb08e6b8ea86f7c614ff6970be1325f65dbd2e401b0afe1241dfd","observation_id":"f9b3aab5-9d19-4c25-9ba8-8ae5754f91e2","resolution":{"observed_at":"2026-08-08T12:50:17.095492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.00180","last_updated":"2016-06-01T09:03:30Z","snapshot_observed_at":"2026-08-03T14:25:39.514776Z","submitted_at":"2016-06-01T09:03:30Z","title":"Cosmology and Fundamental Physics with the Euclid Satellite","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.00180","snapshot_observed_at":"2026-08-08T12:50:17.101256Z","title":"( year 2018 )","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.101256Z"},"links":{"cited_paper":"/paper/1606.00180","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:b9cbefe37267362166cfbe60dbe318ddad923b9ba11c15e7a33ebe1c42242ace","observation_id":"7509a2fc-10e7-450d-a233-83d41c4e0397","resolution":{"observed_at":"2026-08-08T12:50:17.101256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.04352","last_updated":"2023-01-31T21:22:02Z","snapshot_observed_at":"2026-07-06T11:17:08.675456Z","submitted_at":"2021-06-08T13:59:59Z","title":"The First CHIME/FRB Fast Radio Burst Catalog","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.04352","snapshot_observed_at":"2026-08-08T12:50:17.106638Z","title":"( collaboration CHIME/FRB ) ( year 2021 )","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.106638Z"},"links":{"cited_paper":"/paper/2106.04352","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:bd3dc28fe78c2ef9e93672cc7fef7ecf0f0ae497983d600c8c16dda06909a694","observation_id":"08606104-0934-4ec2-9a93-06a6608faaf1","resolution":{"observed_at":"2026-08-08T12:50:17.106638Z","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":"2026-08-08T12:50:17.112116Z","title":"title Breaking diffeomorphism invariance and tests for the emergence of gravity","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.112116Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:7745238ac8a582ac87005632c46219f24802850f5b6e75cf556588f6897aa83f","observation_id":"2c93cd1a-674a-4d9c-963b-a376ad70cb87","resolution":{"observed_at":"2026-08-08T12:50:17.112116Z","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":"2026-08-08T12:50:17.117095Z","title":"title Gauge invariance and unitarity in higher-derivative quantum gravity","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.117095Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:b835737ce001cdc5e2a24871ab4ec7efdce0a9937e223c8caedb236dbc29374b","observation_id":"80ff6c90-0454-4a35-ad2d-e04c9920bf36","resolution":{"observed_at":"2026-08-08T12:50:17.117095Z","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":"2026-08-08T12:50:17.122063Z","title":"title Cosmology from an anti-de sitter--schwarzschild black hole via holography","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.122063Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:458ef2e9c7ffc678e318622b6e79006cba380d675d6f89b221bad7fc617b3086","observation_id":"f366ad83-c1f2-4fb0-a71d-c844e9809347","resolution":{"observed_at":"2026-08-08T12:50:17.122063Z","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":"2026-08-08T12:50:17.126902Z","title":"title The cosmological constant and ho r ava-lifshitz gravity","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.126902Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:f44fdca460c051f69877ac403c9c30942df47573fd81c7b71f01d638a851b90c","observation_id":"83b450bb-9990-4052-abde-a46137091de3","resolution":{"observed_at":"2026-08-08T12:50:17.126902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.3199","last_updated":"2007-06-04T13:21:10Z","snapshot_observed_at":"2026-07-06T01:27:35.546472Z","submitted_at":"2007-05-22T15:32:59Z","title":"Do consistent $F(R)$ models mimic General Relativity plus $\\Lambda$?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.3199","snapshot_observed_at":"2026-08-08T12:50:17.131941Z","title":"title Do consistent F(R) models mimic General Relativity plus ? journal Phys","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.131941Z"},"links":{"cited_paper":"/paper/0705.3199","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:f92ce7202b10b9a17bbd8da8bd321835ea647b554081922c423a5d67615ce7e1","observation_id":"ca8ce228-9226-496c-a275-704df5d28613","resolution":{"observed_at":"2026-08-08T12:50:17.131941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.116.231101","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T12:50:18.799776Z","title":"( year 2016 )","venue":null,"work_id":"dc7a5e1e-6744-4a62-9917-b1a580e92365","year":2016},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.137195Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ad3ce38c235d5eea0414d36c0109c3d67f644aa9fb21cc49c9164973e00ab389","observation_id":"368dea5a-1c1a-419d-a575-15d703482bd8","resolution":{"observed_at":"2026-08-08T12:50:18.804722Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T12:50:17.143424Z","title":"title Effective theory approach to the spontaneous breakdown of lorentz invariance","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.143424Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:bad3112186c110b43400fb7c1ecec380787e0e80aa47d6618c73434f334d39c6","observation_id":"2025269d-00f1-4f4e-8f0d-9d7c0b131ce1","resolution":{"observed_at":"2026-08-08T12:50:17.143424Z","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":"2026-08-08T12:50:17.148328Z","title":"title Supernova 1987A","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.148328Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:19a9049a14baa3add5d9480db110d57bac8907aaf60b4eac43e9bbd4ce1b93cd","observation_id":"831fb249-3234-4c9b-a159-e42942b39647","resolution":{"observed_at":"2026-08-08T12:50:17.148328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.01597","last_updated":"2022-05-03T16:20:16Z","snapshot_observed_at":"2026-08-06T07:21:34.520071Z","submitted_at":"2022-05-03T16:20:16Z","title":"New Horizons for Fundamental Physics with LISA","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.01597","snapshot_observed_at":"2026-08-08T12:50:17.153009Z","title":"( collaboration LISA ) ( year 2022 )","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.153009Z"},"links":{"cited_paper":"/paper/2205.01597","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ba2d1250759db050887e0744a62391b3ad4413356b56ec050f6c82913ef38d9d","observation_id":"9929e315-eaf6-4b57-ab1b-90f6c3c08380","resolution":{"observed_at":"2026-08-08T12:50:17.153009Z","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":"2026-08-08T12:50:17.158064Z","title":"title Shadow of rotating ho r ava-lifshitz black hole","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.158064Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:0e11bba67704b7baf86881c2692d800b25b80d6019194fbccab2c9ffa1978a6a","observation_id":"d8ce402f-d45b-4fc1-ba3b-a8ecd1af8966","resolution":{"observed_at":"2026-08-08T12:50:17.158064Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ex/0107013","last_updated":"2001-07-06T17:58:28Z","snapshot_observed_at":"2026-07-07T03:33:47.536350Z","submitted_at":"2001-07-06T17:58:28Z","title":"Observation of CP violation in the B^0 meson system","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ex/0107013","snapshot_observed_at":"2026-08-08T12:50:17.162754Z","title":"( collaboration BaBar ) ( year 2001 )","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.162754Z"},"links":{"cited_paper":"/paper/hep-ex/0107013","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:8a62a2628d5a5de31d50bdbc2870b2b5231548190fbf7d0860850e8a53cdad0e","observation_id":"1fb25b26-902b-47de-a5c6-52c28b2c4ebd","resolution":{"observed_at":"2026-08-08T12:50:17.162754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.5688","last_updated":"2009-09-30T18:21:24Z","snapshot_observed_at":"2026-07-06T01:58:39.748594Z","submitted_at":"2009-09-30T18:21:24Z","title":"Breaking and restoring of diffeomorphism symmetry in discrete gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.5688","snapshot_observed_at":"2026-08-08T12:50:17.167617Z","title":"title Breaking and restoring of diffeomorphism symmetry in discrete gravity","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.167617Z"},"links":{"cited_paper":"/paper/0909.5688","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:5fc090a5102b664d3b651e69f104b3ff240207e73b8ecc208ff09f3f299ec4dd","observation_id":"91a3e410-1b41-481c-b132-4eefd5416eee","resolution":{"observed_at":"2026-08-08T12:50:17.167617Z","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":"2026-08-08T12:50:17.172596Z","title":"title Topology of black hole thermodynamics in lovelock gravity","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.172596Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:8412bdd5e2b30212c6a767d173f4cebdeaf36807319dd58e601417e9b5194356","observation_id":"7f098e9a-ef48-48cd-b5bf-ac50fd5763eb","resolution":{"observed_at":"2026-08-08T12:50:17.172596Z","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":"2026-08-08T12:50:17.177727Z","title":"( year 2021 )","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.177727Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:aaf1b36934f4f94e7e2893ca74058e7399deafe5ca26ea051f168e4602139f4a","observation_id":"38869257-060e-4f8b-9c60-f537051c6540","resolution":{"observed_at":"2026-08-08T12:50:17.177727Z","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":"2026-08-08T12:50:17.183372Z","title":"title Short-range gravity and lorentz violation","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.183372Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:31e12a16325904860ec74c2c259bd142d401abc0bd15b1eaca9b7ca662fb7b0d","observation_id":"920b7ce3-795a-46d3-b6c1-9ff7ed085440","resolution":{"observed_at":"2026-08-08T12:50:17.183372Z","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":"2026-08-08T12:50:17.188196Z","title":"title Explicit diffeomorphism violation no-go constraints and discontinuities","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.188196Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:cbbe06b6faadbf6c830483ec5bd85cff6a966bcbc237f69c342a9589acea3c8e","observation_id":"364d62fb-cb54-4fef-b10d-0d31d1c1aeae","resolution":{"observed_at":"2026-08-08T12:50:17.188196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.3455","last_updated":"2015-06-08T11:35:43Z","snapshot_observed_at":"2026-07-06T04:03:12.627088Z","submitted_at":"2014-12-10T21:00:03Z","title":"Linking Tests of Gravity On All Scales: from the Strong-Field Regime to Cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.3455","snapshot_observed_at":"2026-08-08T12:50:17.193166Z","title":"title Linking Tests of Gravity On All Scales: from the Strong-Field Regime to Cosmology","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.193166Z"},"links":{"cited_paper":"/paper/1412.3455","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:54f84dd801433d5bb2eaa938cc60f7a6219e868e4be54479bce46f1439362be3","observation_id":"baa4a174-3d31-4e90-9e8b-281dfa8ac813","resolution":{"observed_at":"2026-08-08T12:50:17.193166Z","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":"2026-08-08T12:50:17.198888Z","title":"title Inflation with violation of the null energy condition","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.198888Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:fd201c95d34300a487ab20dec12ef43896e62a437831756f3c903955caa2b143","observation_id":"3e1d1487-1c1f-4436-89d2-ec69fe4422c1","resolution":{"observed_at":"2026-08-08T12:50:17.198888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.03884","last_updated":"2017-04-06T21:41:09Z","snapshot_observed_at":"2026-07-06T04:29:43.654622Z","submitted_at":"2015-09-13T19:05:18Z","title":"Testing black hole candidates with electromagnetic radiation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.03884","snapshot_observed_at":"2026-08-08T12:50:17.204227Z","title":"title Testing black hole candidates with electromagnetic radiation","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.204227Z"},"links":{"cited_paper":"/paper/1509.03884","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:b88f696dc95eb4df8812c29170ff4098025f2880b29616738abeb7f5ce65753c","observation_id":"30bcbe9c-875b-4003-a02b-fb0d5c63b09f","resolution":{"observed_at":"2026-08-08T12:50:17.204227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.12341","last_updated":"2024-12-13T07:36:24Z","snapshot_observed_at":"2026-07-06T19:04:35.538335Z","submitted_at":"2024-08-22T12:36:12Z","title":"Interacting dark sector from Horndeski theories and beyond: Mapping fields and fluids","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.12341","snapshot_observed_at":"2026-08-08T12:50:17.209144Z","title":"title Interacting dark sector from Horndeski theories and beyond: Mapping fields and fluids","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.209144Z"},"links":{"cited_paper":"/paper/2408.12341","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ff7df6f121642bfdbc087ae92cea76b790378b48a901c2e43a156dd6c02d4a4a","observation_id":"a7d9ad0e-1961-4fa1-b085-a458d4a0bcb8","resolution":{"observed_at":"2026-08-08T12:50:17.209144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.05195","last_updated":"2019-02-01T08:42:45Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-06-13T18:00:06Z","title":"Black holes, gravitational waves and fundamental physics: a roadmap","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.05195","snapshot_observed_at":"2026-08-08T12:50:17.213981Z","title":"( year 2019 )","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.213981Z"},"links":{"cited_paper":"/paper/1806.05195","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:79c54775a282510c2f196b180ce3657ef12c6430f16d180816ac4cbfac415765","observation_id":"29a79a6e-81da-4f73-b99c-00a148082b02","resolution":{"observed_at":"2026-08-08T12:50:17.213981Z","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":"2026-08-08T12:50:17.218935Z","title":"title Black holes in lorentz-violating gravity theories","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.218935Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ee0724cc0c9fdf6731f08151399b5393a8456ba6e388c2f757fe4c031a5b6a1b","observation_id":"a50e0687-3230-4cfb-b515-bab76fa424f9","resolution":{"observed_at":"2026-08-08T12:50:17.218935Z","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":"2026-08-08T12:50:17.223725Z","title":"title Slowly rotating black holes in ho r ava-lifshitz gravity","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.223725Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:8b4ee5ab2c40d3e8e2ba13f89c4f76cc3c50c9b210a6fd57ebf201506d2d87a8","observation_id":"69130a56-86e9-468d-85eb-fc3f89555d78","resolution":{"observed_at":"2026-08-08T12:50:17.223725Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.123.231102","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T12:50:18.775264Z","title":"title New test of lorentz invariance using the microscope space mission","venue":null,"work_id":"af774633-363d-412e-8782-f1ad8c41cc15","year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.228322Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:e60c31a5ca7f5cd04bf342b650d13995f4a75a56abbbcb6a31e871d93604ed1d","observation_id":"fb49fad7-9700-4784-a844-81ccc96b96cc","resolution":{"observed_at":"2026-08-08T12:50:18.780466Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T12:50:17.232961Z","title":"title Quantizing Fourth Order Gravity Theories","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.232961Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:235c8adaae87b9a56785bdb33a339499559568e4022b82afd251866042594213","observation_id":"736e5ab7-6207-4a04-8c6b-fea734754537","resolution":{"observed_at":"2026-08-08T12:50:17.232961Z","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":"2026-08-08T12:50:17.237483Z","title":"title Renormalization of ho r ava gravity","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.237483Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:43457e46b5bd3d075a62dd8810eea9fc1ca02ff281c26cf0ea3b7e59fc6b0e6f","observation_id":"65dc8912-890b-4114-89a8-89ded98c1a33","resolution":{"observed_at":"2026-08-08T12:50:17.237483Z","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":"2026-08-08T12:50:17.242523Z","title":"title Ho r ava gravity is asymptotically free in 2+ 1 dimensions","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.242523Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:50d0587fec5bd854de133652036f0166905a48577efb59bcb37e6902beb60842","observation_id":"d70b5514-0711-4d7c-8b54-3a70ca7276e5","resolution":{"observed_at":"2026-08-08T12:50:17.242523Z","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":"2026-08-08T12:50:17.247147Z","title":"title Towards the renormalization group flow of ho r ava gravity in 3+ 1 dimensions","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.247147Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:a3b579509d1d0140d27a2be721c2b1b47d00e5fedc6639e877a36f1aeff136fb","observation_id":"406c80d2-a9a6-4079-8c58-965daee473bf","resolution":{"observed_at":"2026-08-08T12:50:17.247147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507632","last_updated":"2006-02-02T00:51:44Z","snapshot_observed_at":"2026-08-08T07:20:25.695986Z","submitted_at":"2005-07-27T10:59:33Z","title":"Inflation Dynamics and Reheating","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507632","snapshot_observed_at":"2026-08-08T12:50:17.251735Z","title":"title Inflation dynamics and reheating","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.251735Z"},"links":{"cited_paper":"/paper/astro-ph/0507632","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:551ee71c4d636c3766cc744f3303dde74edb6106ae736d2572910f154b96ba69","observation_id":"6ec635d7-a475-4933-bdfc-f6ed52cec3a3","resolution":{"observed_at":"2026-08-08T12:50:17.251735Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.01820","last_updated":"2019-12-13T05:26:55Z","snapshot_observed_at":"2026-07-06T08:19:06.716790Z","submitted_at":"2019-09-03T12:29:11Z","title":"An Introduction to Spontaneous Symmetry Breaking","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.01820","snapshot_observed_at":"2026-08-08T12:50:17.256531Z","title":"title An Introduction to Spontaneous Symmetry Breaking","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.256531Z"},"links":{"cited_paper":"/paper/1909.01820","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:90048ce023e7455da5e5be2056eaafba38fc3c210a69382bd1c8107bdb0dbad8","observation_id":"658cda6f-0d97-4dd8-abe1-0acfde897571","resolution":{"observed_at":"2026-08-08T12:50:17.256531Z","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":"2026-08-08T12:50:17.261493Z","title":"title Black holes and entropy","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.261493Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:2109f51ed0e414993da20eb14f79a1751a005da6437dcc2e2f6a4bc8a682517c","observation_id":"a834693e-bcee-4b61-beb6-0c619fdc9ff6","resolution":{"observed_at":"2026-08-08T12:50:17.261493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9211017","last_updated":"1992-11-13T18:59:46Z","snapshot_observed_at":"2026-08-05T10:42:48.629740Z","submitted_at":"1992-11-13T18:59:46Z","title":"The Relation between Physical and Gravitational Geometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9211017","snapshot_observed_at":"2026-08-08T12:50:17.266030Z","title":"title The Relation between physical and gravitational geometry","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.266030Z"},"links":{"cited_paper":"/paper/gr-qc/9211017","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:07a94efd0b6b8bafe86fb44aea60f58af9ee28335d93abc279d60e0472ca8392","observation_id":"ec662904-c2a4-4044-90d7-f42f271b78fa","resolution":{"observed_at":"2026-08-08T12:50:17.266030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9808028","last_updated":"1998-11-02T10:33:31Z","snapshot_observed_at":"2026-07-07T03:29:21.367658Z","submitted_at":"1998-08-11T08:12:01Z","title":"Black Holes: Classical Properties, Thermodynamics and Heuristic Quantization","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9808028","snapshot_observed_at":"2026-08-08T12:50:17.275366Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.275366Z"},"links":{"cited_paper":"/paper/gr-qc/9808028","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:08fa47a26407bfa88cfa9e0939d4944bd8f5b4f24c77d92d01d2cadf0d06affd","observation_id":"4b983f7b-e80a-468b-b67a-10a0256fb62d","resolution":{"observed_at":"2026-08-08T12:50:17.275366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701848","last_updated":"2007-03-27T07:08:57Z","snapshot_observed_at":"2026-07-07T01:06:39.816950Z","submitted_at":"2007-01-30T08:58:43Z","title":"The modified Newtonian dynamics-MOND-and its implications for new physics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0701848","snapshot_observed_at":"2026-08-08T12:50:17.280033Z","title":"title The Modified Newtonian Dynamics: MOND and its implications for new physics","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.280033Z"},"links":{"cited_paper":"/paper/astro-ph/0701848","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:c8f22cb0656c6a8b68e44decaf393094a292a4adf54695da52effbcb2c75b5b1","observation_id":"ac9e36d2-9c16-4454-978c-ab73c9777b98","resolution":{"observed_at":"2026-08-08T12:50:17.280033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.07749","last_updated":"2017-06-21T13:56:34Z","snapshot_observed_at":"2026-07-06T05:23:54.695988Z","submitted_at":"2016-12-22T18:52:33Z","title":"Higher-order theories of gravity: diagnosis, extraction and reformulation via non-metric extra degrees of freedom","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.07749","snapshot_observed_at":"2026-08-08T12:50:17.284751Z","title":"title Higher-order theories of gravity: diagnosis, extraction and reformulation via non-metric extra degrees of freedom a review","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.284751Z"},"links":{"cited_paper":"/paper/1612.07749","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:61e122ae8409ca466dd7354decab0c900eac87deb4164afaf59e96fa889fa999","observation_id":"ef0f62d9-5e3e-4f2d-b4d8-1d6530d5abf0","resolution":{"observed_at":"2026-08-08T12:50:17.284751Z","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":"2026-08-08T12:50:17.289450Z","title":"title Spontaneous lorentz breaking and massive gravity","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.289450Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:d7b0fbbd43a768e27eca17bfe7fdb245cbe4a1adb4b3d0d57c5d2922393e77c2","observation_id":"e4af4e5a-5ae1-4f81-a1ca-4cba5ef73e17","resolution":{"observed_at":"2026-08-08T12:50:17.289450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1361-6633/acd203","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T12:50:18.741000Z","title":"title MICROSCOPE s view at gravitation","venue":null,"work_id":"442f828e-4a70-49f0-938f-5c78a9614087","year":2023},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.293847Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:4bb6d7f0890e2edeefff27ce53eae7d862c0897ed60b61d600307ec0184d5423","observation_id":"cd850be4-5e13-417e-a98f-e839c56e61f9","resolution":{"observed_at":"2026-08-08T12:50:18.746068Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01644","last_updated":"2015-01-07T21:07:42Z","snapshot_observed_at":"2026-07-06T04:05:35.886136Z","submitted_at":"2015-01-07T21:07:42Z","title":"Status of MICROSCOPE, a mission to test the Equivalence Principle in space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01644","snapshot_observed_at":"2026-08-08T12:50:17.298615Z","title":"title Status of MICROSCOPE, a mission to test the Equivalence Principle in space","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.298615Z"},"links":{"cited_paper":"/paper/1501.01644","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:65c82df2c9e7dbcb9c23bbce95228b0cbce68bf3382ea538d0a38dfb4340d61b","observation_id":"8c71a539-d3b3-47b6-8280-ad24b18c45bf","resolution":{"observed_at":"2026-08-08T12:50:17.298615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.07263","last_updated":"2020-12-07T15:23:48Z","snapshot_observed_at":"2026-08-06T13:41:54.221475Z","submitted_at":"2020-04-15T18:00:44Z","title":"Robustness of baryon acoustic oscillation constraints for early-Universe modifications to $\\Lambda$CDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.07263","snapshot_observed_at":"2026-08-08T12:50:17.303362Z","title":"title Robustness of baryon acoustic oscillation constraints for early-Universe modifications of CDM cosmology","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.303362Z"},"links":{"cited_paper":"/paper/2004.07263","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:f8ae44ba7a4f469e149d45ee79a60265e633e40c4e8b6e0658869c298a8c0993","observation_id":"8f2151bd-aba1-4df9-afc0-4edf76cf382a","resolution":{"observed_at":"2026-08-08T12:50:17.303362Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/revmodphys.46.7","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T12:50:18.725443Z","title":"title Spontaneous symmetry breaking, gauge theories, the higgs mechanism and all that","venue":null,"work_id":"af5d3872-6e97-43f5-a216-96725c41d80c","year":1975},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.307966Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:2fdba82929d5ebb6c5a6a3c66834a645f81a98e0230ae00670e2428c6bcfa0a5","observation_id":"bbd2db71-14cb-466a-b6d2-3440d447c38f","resolution":{"observed_at":"2026-08-08T12:50:18.730433Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T12:50:17.312620Z","title":"title Constraining the mass of the graviton with the planetary ephemeris inpop","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.312620Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:3d07ac3a5356397c8bd23ea105fde606f637d8e775c9c36e8d24a95623483894","observation_id":"193e3002-a79f-44fb-a248-3636cd234ff7","resolution":{"observed_at":"2026-08-08T12:50:17.312620Z","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":"2026-08-08T12:50:17.316811Z","title":"title Constraint on the yukawa suppression of the newtonian potential from the planetary ephemeris inpop19a","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.316811Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:867ba4c2794f4b2879ae3f249fa25bbfe2a4c26f9403d712222dfdca5855c275","observation_id":"48ef5276-8868-4b0c-9d13-f6b5f260e41b","resolution":{"observed_at":"2026-08-08T12:50:17.316811Z","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":"2026-08-08T12:50:17.321171Z","title":"title On the spontaneous breaking of lorentz invariance","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.321171Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:d6a2c576b8874f437cd8d8cdad315f5b4398ec84501416dc00ace781a7f46ece","observation_id":"4015cfb6-4877-4e73-847d-837dd20f3b2c","resolution":{"observed_at":"2026-08-08T12:50:17.321171Z","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":"2026-08-08T12:50:17.325484Z","title":"title Proposed astrophysical test of lorentz invariance","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.325484Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:4284e0204b9c96efa2082a9bd57271404a5d67fd681548e1cee87b18ca1a76b6","observation_id":"6f845cc1-c90d-48a5-8137-5a09a7549e37","resolution":{"observed_at":"2026-08-08T12:50:17.325484Z","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":"2026-08-08T12:50:17.329853Z","title":"title Ho r ava-lifshitz quantum cosmology","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.329853Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:74ce7b7a900629ef134dd4c8c1d1ee9ae7a265ca4d78c5d2aa365648644fafce","observation_id":"658ffe44-b994-4f8a-861d-a49ad3a11dd8","resolution":{"observed_at":"2026-08-08T12:50:17.329853Z","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":"2026-08-08T12:50:17.334441Z","title":"title Physics of the Solar System - Dynamics and Evolution, Space Physics, and Spacetime Structure","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.334441Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:a993833de3699ecec6013482fa31e91f5de2a6adac5fc2d6a7247699d31d0fc0","observation_id":"9215f3f3-1e4e-4ce4-8060-ee29a6889b76","resolution":{"observed_at":"2026-08-08T12:50:17.334441Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.04901","last_updated":"2024-06-07T12:51:40Z","snapshot_observed_at":"2026-07-06T18:27:07.473039Z","submitted_at":"2024-06-07T12:51:40Z","title":"Exotic compact objects: a recent numerical-relativity perspective","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.04901","snapshot_observed_at":"2026-08-08T12:50:17.339054Z","title":"title Exotic compact objects: a recent numerical-relativity perspective 2406.04901","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.339054Z"},"links":{"cited_paper":"/paper/2406.04901","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:29bbda4aa256f4101ce2495e1398761d3fd2e028a0ba619d5df286651cb7d383","observation_id":"f4accd91-2ec9-4b51-94b7-a5655ed62c3c","resolution":{"observed_at":"2026-08-08T12:50:17.339054Z","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":"2026-08-08T12:50:17.343626Z","title":"title Probing the Universe with Fast Radio Bursts","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.343626Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:69fbd7f518a7d8c1307a7942c241cf3329d62daf47ce75de30b7b7bf1f8ad21a","observation_id":"9e800524-b391-4fd0-a29a-8d795fb2bc29","resolution":{"observed_at":"2026-08-08T12:50:17.343626Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.07044","last_updated":"2017-08-30T14:31:28Z","snapshot_observed_at":"2026-07-06T05:38:57.709035Z","submitted_at":"2017-04-24T05:23:42Z","title":"Quasinormal modes as a distinguisher between general relativity and f(R) gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.07044","snapshot_observed_at":"2026-08-08T12:50:17.348075Z","title":"title Quasinormal modes as a distinguisher between general relativity and f(R) gravity","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.348075Z"},"links":{"cited_paper":"/paper/1704.07044","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:a2ac0e76727df4d1b734e6a9ddae9ece7712740ecf31b2d27dde09853b737031","observation_id":"bb027df1-3fbe-46ee-8d93-255964443472","resolution":{"observed_at":"2026-08-08T12:50:17.348075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.07576","last_updated":"2018-09-05T10:52:19Z","snapshot_observed_at":"2026-07-06T06:29:18.004290Z","submitted_at":"2018-03-20T18:02:32Z","title":"Quasinormal modes as a distinguisher between general relativity and f(R) gravity: Charged black-holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.07576","snapshot_observed_at":"2026-08-08T12:50:17.357209Z","title":"title Quasinormal modes as a distinguisher between general relativity and f(R) gravity: Charged black-holes","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.357209Z"},"links":{"cited_paper":"/paper/1803.07576","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:64b1fd0bd3991a09b7c3c2e10e63e71c94541fbdad2a9cc4e6b3a2b0792b64d0","observation_id":"6c6b627c-cf46-4227-baa3-a888bc127fbe","resolution":{"observed_at":"2026-08-08T12:50:17.357209Z","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":"2026-08-08T12:50:17.361413Z","title":"title Randall-sundrum versus holographic cosmology","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.361413Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:a6b482236dcbc15937d71b5e5f45d1f0775d120d9089af0560f5a5fbb837f3e9","observation_id":"69eefb30-64d9-45fa-ae5e-e0eb2e06ced8","resolution":{"observed_at":"2026-08-08T12:50:17.361413Z","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":"2026-08-08T12:50:17.365904Z","title":"title Quantum Fields in Curved Space , series Cambridge Monographs on Mathematical Physics , publisher Cambridge Univ","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.365904Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:d3bb4a3593bed5592930bf97410d1216be2531201fb01430442c9c5e45d0d52b","observation_id":"a388a1a2-4c74-4122-9b11-d0395c9e9c35","resolution":{"observed_at":"2026-08-08T12:50:17.365904Z","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":"2026-08-08T12:50:17.370825Z","title":"title Black hole thermodynamics in horava lifshitz gravity and the related geometry","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.370825Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:613f010be3d0aeca00e95cb1f777283f8b6580ec44c3ea9c516f5d1bb95938b0","observation_id":"5783e0e0-f0b7-43ac-945c-72588f892278","resolution":{"observed_at":"2026-08-08T12:50:17.370825Z","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":"2026-08-08T12:50:17.375340Z","title":"title Ho r ava gravity versus thermodynamics: the black hole case","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.375340Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:d971dce2a9cc17999dec9fd0bf6500d13b3868379bdee4a387aee5be7e53fc86","observation_id":"bbcd206d-f41b-48ba-b9cd-acd2bd55c7c3","resolution":{"observed_at":"2026-08-08T12:50:17.375340Z","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":"2026-08-08T12:50:17.379981Z","title":"title Lorentz-breaking massive gravity in curved space","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.379981Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:d27aaa3c59c3c3b1ff434fd55edada5ac037908d8e2f92943c4696496cff32bc","observation_id":"fe1e0584-29e8-422b-bcc8-6e6f9c232a66","resolution":{"observed_at":"2026-08-08T12:50:17.379981Z","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":"2026-08-08T12:50:17.384702Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.384702Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:9cf3e1ce588a680452be4abb6e7c76e616f15725cf408206e60d8a55be2ab6b9","observation_id":"b55462c9-7b9f-4a9b-b902-ee5fa21b5dca","resolution":{"observed_at":"2026-08-08T12:50:17.384702Z","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":"2026-08-08T12:50:17.389642Z","title":"title Explicit versus spontaneous diffeomorphism breaking in gravity","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.389642Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:ac88d7e5752d0b5927dd7ec06fb6c3c58ae8a6fd3d6129ca3c2486a2b3e65fe5","observation_id":"aa5edd8e-b651-444a-8587-3f192a305947","resolution":{"observed_at":"2026-08-08T12:50:17.389642Z","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":"2026-08-08T12:50:17.394486Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.394486Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:898ed0cfb9e458826f7b0d0a0dd19e327e76ab90420763adfdb50864a79824a3","observation_id":"59333a28-bf19-4759-84c7-ae685e4628a7","resolution":{"observed_at":"2026-08-08T12:50:17.394486Z","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":"2026-08-08T12:50:17.399202Z","title":"title Gravity with explicit diffeomorphism breaking","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.399202Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:278eeec1d93bf904bae520333b5c717d3af244fbdd7ba69a75ecac68f073fdb6","observation_id":"4d8383cd-15ad-4d4a-a5d2-a7dabb55f624","resolution":{"observed_at":"2026-08-08T12:50:17.399202Z","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":"2026-08-08T12:50:17.403618Z","title":"title Spontaneous lorentz and diffeomorphism violation, massive modes, and gravity","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.403618Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:4de50371b49a994de4f9f86a78da97454ddd570043b90b4b3d9905073625e488","observation_id":"e0c34319-ca8f-4e03-893a-cbcc30b50619","resolution":{"observed_at":"2026-08-08T12:50:17.403618Z","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":"2026-08-08T12:50:17.408742Z","title":"title Loop quantum gravity phenomenology and the issue of lorentz invariance","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.408742Z"},"links":{"citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:a40ac4d65980a8f89d3cb58e7b48516bfe3ba60add5cd9820373a57ba39b0e83","observation_id":"90eac858-7a82-4d2f-b560-e13f543027e4","resolution":{"observed_at":"2026-08-08T12:50:17.408742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.04896","last_updated":"2016-03-17T15:02:48Z","snapshot_observed_at":"2026-07-06T04:33:21.124930Z","submitted_at":"2015-10-16T14:29:32Z","title":"Phenomenological investigation of a quantum gravity extension of inflation with the Starobinsky potential","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.04896","snapshot_observed_at":"2026-08-08T12:50:17.413414Z","title":"title Phenomenological investigation of a quantum gravity extension of inflation with the Starobinsky potential","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.413414Z"},"links":{"cited_paper":"/paper/1510.04896","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:b2961cd4b250be77209ffce64cd86e5b4e4cf2b88328ec5581cede460653b43e","observation_id":"b91d28f8-e451-4928-b13e-b651797337cc","resolution":{"observed_at":"2026-08-08T12:50:17.413414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06457","last_updated":"2021-12-09T14:26:59Z","snapshot_observed_at":"2026-08-09T13:57:29.191771Z","submitted_at":"2020-04-14T13:00:57Z","title":"A null test of the equivalence principle using relativistic effects in galaxy surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.06457","snapshot_observed_at":"2026-08-08T12:50:17.418018Z","title":"title A null test of the equivalence principle using relativistic effects in galaxy surveys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":102,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:17.418018Z"},"links":{"cited_paper":"/paper/2004.06457","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:aac483ed2675657d3173cd38b39f4bf615147ced256fdb27555685e8d0988964","observation_id":"c0266666-5fde-41f1-8490-693bf2f4cfa1","resolution":{"observed_at":"2026-08-08T12:50:17.418018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-09T09:20:47.168444Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":95,"verified_exact":5,"verified_fuzzy":0},"total_outbound_references":298},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 100 of 298 outbound references and 5 inbound Pith citation observations for arXiv:2502.07437."}