{"as_of":"2026-08-21T21:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:726f20103ec54dbd15b08c4de03da6ab82be854a2e60056daa0a8413d77aa955","coverage":[{"denominator":107,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T20:12:23.748845Z","state":"measured"},{"denominator":103,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":103,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T09:40:49.196932Z","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":"2026-05-15T03:03:57.351285Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"cited_work":{"arxiv_id":"2511.21071","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2511.21071","snapshot_observed_at":"2026-06-30T02:16:11.740868Z","title":"Chiang, C","venue":null,"work_id":"6ad5b258-b878-49c6-b186-c32fd8084450","year":2025},"citing_paper":{"arxiv_id":"2604.21962","last_updated":"2026-04-23T16:55:04Z","snapshot_observed_at":"2026-08-11T19:25:50.223205Z","submitted_at":"2026-04-23T16:55:04Z","title":"Perturbation Dynamics and Structure Formation in Extended Proca-Nuevo Gravity","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-09T21:07:17.013920Z"},"links":{"cited_paper":"/paper/2511.21071","citing_paper":"/paper/2604.21962"},"observation_digest":"sha256:99993d9aa84bda3456df65ba31e2d8a879e9fd341f9898a6cec9ca1fc2214b99","observation_id":"b996d268-1f9e-49e4-97f0-60f43e98aacb","resolution":{"observed_at":"2026-06-30T02:16:11.740868Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"cited_work":{"arxiv_id":"2511.21071","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2511.21071","snapshot_observed_at":"2026-06-30T02:16:11.740868Z","title":"Chiang, C","venue":null,"work_id":"6ad5b258-b878-49c6-b186-c32fd8084450","year":2025},"citing_paper":{"arxiv_id":"2605.13920","last_updated":"2026-05-13T13:58:10Z","snapshot_observed_at":"2026-08-18T14:45:05.898191Z","submitted_at":"2026-05-13T13:58:10Z","title":"No-go theorem for spontaneous vectorization","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-15T03:02:56.428440Z"},"links":{"cited_paper":"/paper/2511.21071","citing_paper":"/paper/2605.13920"},"observation_digest":"sha256:e04f0e28cfe7c8293dcde3fd2304cbe1c70b6979d080dc21f6692a304d8a3374","observation_id":"ffe77a9f-5010-41cd-80cd-7ed63dcdb43f","resolution":{"observed_at":"2026-06-30T02:16:11.740868Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2511.21071","snapshot_observed_at":"2026-07-11T09:40:49.196932Z","title":"Chiang, C","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.05044","last_updated":"2026-07-06T13:21:04Z","snapshot_observed_at":"2026-08-15T13:09:12.340147Z","submitted_at":"2026-07-06T13:21:04Z","title":"Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-11T09:40:49.196932Z"},"links":{"cited_paper":"/paper/2511.21071","citing_paper":"/paper/2607.05044"},"observation_digest":"sha256:6eb42bff651aa926d44fcbfebea12985d6a0043703ee8058544f6d14cdbd5858","observation_id":"69966218-60ba-4489-9303-a79d492d8c35","resolution":{"observed_at":"2026-07-11T09:40:49.196932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2511.21071/citation-record","integrity":"/paper/2511.21071/integrity","json":"/paper/2511.21071/citation-record.json","paper":"/paper/2511.21071"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2205.10869","last_updated":"2022-11-11T13:29:22Z","snapshot_observed_at":"2026-08-13T11:09:25.799974Z","submitted_at":"2022-05-22T17:02:55Z","title":"CMB power spectra and cosmological parameters from Planck PR4 with CamSpec","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10869","snapshot_observed_at":"2026-08-03T20:12:23.298036Z","title":"Rosenberg, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.298036Z"},"links":{"cited_paper":"/paper/2205.10869","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:0df127b0121c6b145384f22c9569bac275873193489d98fb42f2c5f70cd42fde","observation_id":"1c461af5-ee77-46c5-9dcd-3e70ddd2adbc","resolution":{"observed_at":"2026-08-03T20:12:23.298036Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-08-03T20:12:23.302035Z","title":"Riess et al.,A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s−1 Mpc−1 Uncertainty from the Hubble Space Telescope and the SH0ES Team, Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.302035Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:200eb6cb4f0e69ffd2565d29df9187abdec1ff8186de0c59295125703c697684","observation_id":"06b9b025-406a-4cef-9aad-eefea4732a0c","resolution":{"observed_at":"2026-08-03T20:12:23.302035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-16T23:09:02.333007Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-08-03T20:12:23.305511Z","title":"Carron, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.305511Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:836f2d4b60864ba5b24f0217a7016dd3f1e926864a2982e47adce49ebd32bf61","observation_id":"b9006dac-69e9-4f3d-80fc-0cd7cf29ce19","resolution":{"observed_at":"2026-08-03T20:12:23.305511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03663","last_updated":"2019-09-16T21:35:34Z","snapshot_observed_at":"2026-08-17T00:55:38.317018Z","submitted_at":"2019-08-10T01:40:10Z","title":"The Hubble Hunter's Guide","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03663","snapshot_observed_at":"2026-08-03T20:12:23.308969Z","title":"Knox and M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.308969Z"},"links":{"cited_paper":"/paper/1908.03663","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:afede2b279f296cc8c7a1505cd6bf363e418a0f0a63d86dfa54d6ebe561b4c14","observation_id":"65d3f167-08ff-43fb-a9d8-584b2aa82a6a","resolution":{"observed_at":"2026-08-03T20:12:23.308969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-08-16T02:36:16.088814Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01183","snapshot_observed_at":"2026-08-03T20:12:23.312500Z","title":"Di Valentino, O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.312500Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:870fcba94a3c6b240bc5ada1efe1e29cc5060cd02dc53c75153e71d450ba0374","observation_id":"11f2f59f-cc5f-4699-a305-628fc1e9b548","resolution":{"observed_at":"2026-08-03T20:12:23.312500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-08-18T00:05:15.748844Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-08-03T20:12:23.315944Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.315944Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:199dec1bb1bbafb03c11ca1b228e43cf275e6fba09f4ef37b4c92c8843e73921","observation_id":"552f3597-a958-43a4-980b-f1b99f828bb8","resolution":{"observed_at":"2026-08-03T20:12:23.315944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.04492","last_updated":"2022-11-08T19:00:16Z","snapshot_observed_at":"2026-08-01T18:06:39.805867Z","submitted_at":"2022-11-08T19:00:16Z","title":"The Hubble Tension and Early Dark Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.04492","snapshot_observed_at":"2026-08-03T20:12:23.319396Z","title":"Kamionkowski and A.G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.319396Z"},"links":{"cited_paper":"/paper/2211.04492","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:de2abbeed397fb399f95ebd16eb736c862188a9c830b846a48c6b7cc519b1144","observation_id":"1b7671c3-c04f-4c0a-99e5-24a0decc45d4","resolution":{"observed_at":"2026-08-03T20:12:23.319396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.01669","last_updated":"2025-08-04T13:56:55Z","snapshot_observed_at":"2026-08-19T18:41:06.928690Z","submitted_at":"2025-04-02T12:17:19Z","title":"The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.01669","snapshot_observed_at":"2026-08-03T20:12:23.322346Z","title":"Di Valentino et al.,The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics, [2504.01669]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.322346Z"},"links":{"cited_paper":"/paper/2504.01669","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:73cf2b7589e7a88639cc0ce2065ba9995f16fc634fdf31a09229db4a16fbcd2c","observation_id":"bf9be9b5-3654-4c67-9a18-0412e62b0ef9","resolution":{"observed_at":"2026-08-03T20:12:23.322346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04929","last_updated":"2025-05-14T14:57:09Z","snapshot_observed_at":"2026-08-08T20:55:05.610325Z","submitted_at":"2025-02-07T13:49:14Z","title":"Robustness of dark energy phenomenology across different parameterizations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04929","snapshot_observed_at":"2026-08-03T20:12:23.326005Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.326005Z"},"links":{"cited_paper":"/paper/2502.04929","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:18ed9e5365762d5aa8be3c17cf2c1d3863cf2f399ebb2910978b91df587718fe","observation_id":"5f1a604b-c314-48d3-a17f-549ebd7d1285","resolution":{"observed_at":"2026-08-03T20:12:23.326005Z","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":"2026-08-03T20:12:23.329140Z","title":"Ferreira and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.329140Z"},"links":{"citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:66d85cef59d11d4f1080ecee35945a85246d2513f66ea32c72075c7e3c7a5ff3","observation_id":"b946c17b-226a-491d-8c05-00c6956d956f","resolution":{"observed_at":"2026-08-03T20:12:23.329140Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07679","last_updated":"2025-07-28T16:54:23Z","snapshot_observed_at":"2026-08-19T12:21:41.121466Z","submitted_at":"2025-04-10T12:07:47Z","title":"Assessing cosmological evidence for non-minimal coupling","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07679","snapshot_observed_at":"2026-08-03T20:12:23.332093Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.332093Z"},"links":{"cited_paper":"/paper/2504.07679","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:ef8830a6ad11f5b48e551a583c77157b5ec5f856842364b156ba344db0144428","observation_id":"9fb8dcec-55c0-463a-869f-08f3f2511d26","resolution":{"observed_at":"2026-08-03T20:12:23.332093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.17318","last_updated":"2025-02-05T13:48:08Z","snapshot_observed_at":"2026-08-20T00:05:01.215478Z","submitted_at":"2024-08-30T14:26:37Z","title":"Scant evidence for thawing quintessence","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.17318","snapshot_observed_at":"2026-08-03T20:12:23.335271Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.335271Z"},"links":{"cited_paper":"/paper/2408.17318","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:4fb851d50f871e2151c806f26f6ebfdef7b1f1214ba5081377fabb9bd9f17f07","observation_id":"798cccf1-b2d6-4624-8964-caf3e421e4d4","resolution":{"observed_at":"2026-08-03T20:12:23.335271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-18T11:01:42.213182Z","submitted_at":"2025-02-06T16:51:39Z","title":"The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-03T20:12:23.338390Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.338390Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:96fc96c2f0196b592c1da487948996a9b486212d4a1a2e6186cc64613d3d6596","observation_id":"b8466c79-980e-434b-abf6-38ca6c56517c","resolution":{"observed_at":"2026-08-03T20:12:23.338390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.02658","last_updated":"2025-05-14T19:17:47Z","snapshot_observed_at":"2026-08-17T07:25:31.274539Z","submitted_at":"2025-05-05T14:03:37Z","title":"Baryon Acoustic Oscillations from a Different Angle","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.02658","snapshot_observed_at":"2026-08-03T20:12:23.341750Z","title":"Efstathiou,Baryon Acoustic Oscillations from a Different Angle, [2505.02658]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.341750Z"},"links":{"cited_paper":"/paper/2505.02658","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:e7e487c31942fafacee5d41dd6e1de243215731c6e4c5b01949595b8802eee89","observation_id":"3cf67046-cc97-4b1f-b879-2b427e376a63","resolution":{"observed_at":"2026-08-03T20:12:23.341750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9908168","last_updated":"2002-09-15T22:50:49Z","snapshot_observed_at":"2026-07-07T01:27:53.812149Z","submitted_at":"1999-08-16T21:31:43Z","title":"A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9908168","snapshot_observed_at":"2026-08-03T20:12:23.345434Z","title":"Caldwell,A Phantom menace?,Phys","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.345434Z"},"links":{"cited_paper":"/paper/astro-ph/9908168","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:3a48e444d9669ffd7b48f1391fe683e759b2bba4adbc73fa1e0da32da8c93511","observation_id":"02cd6b67-dccf-42d2-8d93-887d680998c2","resolution":{"observed_at":"2026-08-03T20:12:23.345434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.0115","last_updated":"2007-09-30T08:11:41Z","snapshot_observed_at":"2026-08-15T10:31:15.167881Z","submitted_at":"2007-09-30T08:11:41Z","title":"Null Energy Condition and Dark Energy Models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.0115","snapshot_observed_at":"2026-08-03T20:12:23.348549Z","title":"Qiu, Y.-F","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.348549Z"},"links":{"cited_paper":"/paper/0710.0115","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:81cdb011d11fa8c934680a7f0f0c4e6b0adc8a0ea3b2d25eb4d9bce2ac00a787","observation_id":"e8323444-c8b7-44bd-a8ba-d7431b3a88a5","resolution":{"observed_at":"2026-08-03T20:12:23.348549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.1961","last_updated":"2013-10-05T08:56:41Z","snapshot_observed_at":"2026-08-15T00:22:22.422604Z","submitted_at":"2013-04-07T06:21:37Z","title":"Quintessence: A Review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.1961","snapshot_observed_at":"2026-08-03T20:12:23.351765Z","title":"Tsujikawa,Quintessence: A Review,Class","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.351765Z"},"links":{"cited_paper":"/paper/1304.1961","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:2ff06bdc9bf121e815624f6bca04175df90ef27503b2de587189f13ed6962096","observation_id":"e5b003d1-d906-4f04-9445-46c63d6e7a5d","resolution":{"observed_at":"2026-08-03T20:12:23.351765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2509.17586","last_updated":"2026-05-29T12:14:37Z","snapshot_observed_at":"2026-08-15T15:45:42.029788Z","submitted_at":"2025-09-22T11:09:31Z","title":"Cosmological constraints on Galileon dark energy with broken shift symmetry","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.17586","snapshot_observed_at":"2026-08-03T20:12:23.354832Z","title":"Wolf, P.G","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.354832Z"},"links":{"cited_paper":"/paper/2509.17586","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:33b423ae1582d5318292e04a299041b97cf080456e786a5ef060a6e46794c6e1","observation_id":"1660f88d-9212-4264-b7da-7e6389144775","resolution":{"observed_at":"2026-08-03T20:12:23.354832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.6450","last_updated":"2014-02-26T08:34:51Z","snapshot_observed_at":"2026-08-14T23:43:18.695614Z","submitted_at":"2014-02-26T08:34:51Z","title":"Cosmic Acceleration from Abelian Symmetry Breaking","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.6450","snapshot_observed_at":"2026-08-03T20:12:23.358465Z","title":"Tasinato,Cosmic Acceleration from Abelian Symmetry Breaking,JHEP04(2014) 067 [1402.6450]","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.358465Z"},"links":{"cited_paper":"/paper/1402.6450","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:8264f2e60294316f402130d9242db53f355f296844e443c0b0f60d756c0e404c","observation_id":"53eccc35-0872-400f-a2f1-5abfa1f9022d","resolution":{"observed_at":"2026-08-03T20:12:23.358465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.7026","last_updated":"2019-08-01T13:48:04Z","snapshot_observed_at":"2026-08-16T00:33:34.858404Z","submitted_at":"2014-02-27T19:14:27Z","title":"Generalization of the Proca Action","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.7026","snapshot_observed_at":"2026-08-03T20:12:23.361527Z","title":"Heisenberg,Generalization of the Proca Action,JCAP05(2014) 015 [1402.7026]","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.361527Z"},"links":{"cited_paper":"/paper/1402.7026","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:12ba13e34697379d824794f20f14569d887b0ed47da4d96565a24fff000b63ac","observation_id":"ca12b07b-a046-4ec6-ac88-6b9949652fd8","resolution":{"observed_at":"2026-08-03T20:12:23.361527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.07029","last_updated":"2016-03-29T11:32:20Z","snapshot_observed_at":"2026-08-19T18:44:35.392130Z","submitted_at":"2015-10-23T19:52:05Z","title":"Covariantised Vector Galileons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.07029","snapshot_observed_at":"2026-08-03T20:12:23.364685Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.364685Z"},"links":{"cited_paper":"/paper/1510.07029","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:6024e31c33cd8b32dffbe67610f7f5b2841c96a92b591cfbf8b22e24c032ba3d","observation_id":"ca38ae75-fb7a-44f0-80dd-2a8aa09c0f80","resolution":{"observed_at":"2026-08-03T20:12:23.364685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.05115","last_updated":"2017-06-15T23:43:46Z","snapshot_observed_at":"2026-08-16T00:34:18.842016Z","submitted_at":"2017-06-15T23:43:46Z","title":"Black holes in vector-tensor theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.05115","snapshot_observed_at":"2026-08-03T20:12:23.367673Z","title":"Heisenberg, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.367673Z"},"links":{"cited_paper":"/paper/1706.05115","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:472d34d417a9904c9ceb162c9617f799a904893444f74ee2c80007ae271ce458","observation_id":"318502a9-98f7-428a-a4b7-d16715fbe0d2","resolution":{"observed_at":"2026-08-03T20:12:23.367673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.09662","last_updated":"2017-10-26T15:27:08Z","snapshot_observed_at":"2026-08-14T20:57:55.242376Z","submitted_at":"2017-05-26T18:00:01Z","title":"Hairy black-hole solutions in generalized Proca theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.09662","snapshot_observed_at":"2026-08-03T20:12:23.370736Z","title":"Heisenberg, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.370736Z"},"links":{"cited_paper":"/paper/1705.09662","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:8b4f1b719b53ec1a6ae0670f756832c1a7e789a041d4f4b1c05e673a3382baf7","observation_id":"66e75b1e-747e-408f-9eec-13a71ba8012b","resolution":{"observed_at":"2026-08-03T20:12:23.370736Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.00634","last_updated":"2020-09-03T17:00:23Z","snapshot_observed_at":"2026-08-07T20:53:00.766956Z","submitted_at":"2020-05-31T23:07:02Z","title":"Rotating black holes in valid vector-tensor theories after GW170817","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.00634","snapshot_observed_at":"2026-08-03T20:12:23.373581Z","title":"Ajith, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.373581Z"},"links":{"cited_paper":"/paper/2006.00634","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:1b5dfe39f2f55ea90f8ab5e2928186090842570a080e34cf7c12d8d4b9534489","observation_id":"dcbdd605-a805-43bd-83f8-299980602089","resolution":{"observed_at":"2026-08-03T20:12:23.373581Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.01056","last_updated":"2017-10-06T22:26:36Z","snapshot_observed_at":"2026-08-18T07:50:52.440333Z","submitted_at":"2017-06-04T11:15:33Z","title":"Spontaneous growth of vector fields in gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.01056","snapshot_observed_at":"2026-08-03T20:12:23.376635Z","title":"Ramazanoğlu,Spontaneous growth of vector fields in gravity,Phys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.376635Z"},"links":{"cited_paper":"/paper/1706.01056","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:ac34a27470bfde2463510dc0b42aa94c4f7c17e19164001639747bc8f583c02a","observation_id":"4bfe60a6-4412-466c-95e2-7329735dcc19","resolution":{"observed_at":"2026-08-03T20:12:23.376635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.10701","last_updated":"2020-07-27T04:32:58Z","snapshot_observed_at":"2026-08-13T15:33:25.326558Z","submitted_at":"2020-01-29T06:18:43Z","title":"Neutron stars with a generalized Proca hair and spontaneous vectorization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.10701","snapshot_observed_at":"2026-08-03T20:12:23.379553Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.379553Z"},"links":{"cited_paper":"/paper/2001.10701","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:db39b8a3ba122f458b264c5cbcef51dc9ebeeddebe0d7da8ccf7ad736665b270","observation_id":"4fb2c0e6-42df-4ddd-99ee-074c7fa7a0fd","resolution":{"observed_at":"2026-08-03T20:12:23.379553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.08049","last_updated":"2021-10-14T21:45:14Z","snapshot_observed_at":"2026-08-16T18:31:06.986466Z","submitted_at":"2021-04-16T11:52:34Z","title":"Destabilization of black holes and stars by generalized Proca fields","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.08049","snapshot_observed_at":"2026-08-03T20:12:23.382607Z","title":"Garcia-Saenz, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.382607Z"},"links":{"cited_paper":"/paper/2104.08049","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:150195aba324a81773a1d50cdcf30f2a9644e02eb6e72cc1f7978e489c2769a2","observation_id":"130948b7-1740-45ec-8b63-0401f61eac54","resolution":{"observed_at":"2026-08-03T20:12:23.382607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04269","last_updated":"2021-12-09T14:21:01Z","snapshot_observed_at":"2026-08-18T08:52:53.479616Z","submitted_at":"2021-12-08T13:04:21Z","title":"Instability of vectorized stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04269","snapshot_observed_at":"2026-08-03T20:12:23.385495Z","title":"Demirboğa, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.385495Z"},"links":{"cited_paper":"/paper/2112.04269","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:6541af58bc000a10c9b8eae0d5e7c0ce6d49c4f7637bef3ac5912c6f2861539d","observation_id":"23b3e332-c17f-43c5-810b-ad9e1d8a35ea","resolution":{"observed_at":"2026-08-03T20:12:23.385495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.04779","last_updated":"2025-08-15T10:42:48Z","snapshot_observed_at":"2026-08-17T09:13:22.872858Z","submitted_at":"2025-04-07T07:14:36Z","title":"Black hole destabilization via trapped quasi-normal modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.04779","snapshot_observed_at":"2026-08-03T20:12:23.388646Z","title":"Chiang, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.388646Z"},"links":{"cited_paper":"/paper/2504.04779","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:05f5fe2f60fa8daaac98833cfc52a6f0f7c3abcc49446885e2100e496d25080a","observation_id":"9a4aafb3-26f5-4e58-9174-2e516e9523db","resolution":{"observed_at":"2026-08-03T20:12:23.388646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.05806","last_updated":"2016-07-03T03:58:14Z","snapshot_observed_at":"2026-08-16T07:21:36.858390Z","submitted_at":"2016-03-18T09:38:24Z","title":"Cosmology in generalized Proca theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.05806","snapshot_observed_at":"2026-08-03T20:12:23.391486Z","title":"De Felice, L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.391486Z"},"links":{"cited_paper":"/paper/1603.05806","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:bae61cd8fbef674c6688feeb5663fba3c06f2581a385bea1ffd0ae42d7df78a3","observation_id":"ffbd73d0-d27c-453f-bf39-a08133f1967c","resolution":{"observed_at":"2026-08-03T20:12:23.391486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.05066","last_updated":"2016-08-13T06:44:57Z","snapshot_observed_at":"2026-08-14T21:57:05.597539Z","submitted_at":"2016-05-17T09:07:52Z","title":"Effective gravitational couplings for cosmological perturbations in generalized Proca theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.05066","snapshot_observed_at":"2026-08-03T20:12:23.394743Z","title":"De Felice, L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.394743Z"},"links":{"cited_paper":"/paper/1605.05066","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:1d532933a3b22f1e40162fbaa008af23a8b1483466f69013a1df48b77bfaf013","observation_id":"53f6b8e9-e6b8-4f5e-9619-2a1641f86ecf","resolution":{"observed_at":"2026-08-03T20:12:23.394743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.08610","last_updated":"2017-05-09T02:45:15Z","snapshot_observed_at":"2026-08-14T21:14:26.323468Z","submitted_at":"2017-02-28T02:29:51Z","title":"Cosmology in beyond-generalized Proca theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.08610","snapshot_observed_at":"2026-08-03T20:12:23.397579Z","title":"Nakamura, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.397579Z"},"links":{"cited_paper":"/paper/1702.08610","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:c980f6a8f2628ebfab27a994218eff294faf8fbde6b3eac4f56f4b2200ba32f0","observation_id":"2cfe328a-e7d6-450c-a25e-7b5d602596a3","resolution":{"observed_at":"2026-08-03T20:12:23.397579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09573","last_updated":"2017-06-24T00:46:04Z","snapshot_observed_at":"2026-08-20T01:31:33.438513Z","submitted_at":"2017-03-28T13:51:29Z","title":"Observational constraints on generalized Proca theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.09573","snapshot_observed_at":"2026-08-03T20:12:23.400474Z","title":"de Felice, L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.400474Z"},"links":{"cited_paper":"/paper/1703.09573","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:b0f37c5fa5aefd2480c35b8272f88e85bd97828074c40984d8bf6feb728608f5","observation_id":"6a303ed7-a321-4d82-9862-4707cdd39d2d","resolution":{"observed_at":"2026-08-03T20:12:23.400474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06577","last_updated":"2021-04-14T01:44:25Z","snapshot_observed_at":"2026-08-20T08:51:45.925163Z","submitted_at":"2021-04-14T01:44:25Z","title":"A Dark Energy model from Generalized Proca Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.06577","snapshot_observed_at":"2026-08-03T20:12:23.403336Z","title":"Geng, Y.-T","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.403336Z"},"links":{"cited_paper":"/paper/2104.06577","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:16cb2af923d88668dc6aebda4910c03a3893da66628f61917bf3de54b378f3ae","observation_id":"ba75873f-02ae-497b-8a35-6e9c22b96a4b","resolution":{"observed_at":"2026-08-03T20:12:23.403336Z","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":"2026-08-03T20:12:23.406153Z","title":"Savaliya,Dynamical Dark Energy from a Massive Vector Field in Generalized Proca Theory, [2511.01700]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.406153Z"},"links":{"citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:686db89320ff0ddd82fba3eeda4d542ad1f49fb43eff2c80e94159cbeb92d8cf","observation_id":"a2ce98f5-1b05-45af-9e1e-b7a5c65ef08a","resolution":{"observed_at":"2026-08-03T20:12:23.406153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.00513","last_updated":"2020-10-01T16:01:37Z","snapshot_observed_at":"2026-08-20T12:04:11.382802Z","submitted_at":"2020-10-01T16:01:37Z","title":"Proca in the sky","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.00513","snapshot_observed_at":"2026-08-03T20:12:23.409456Z","title":"Heisenberg and H","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.409456Z"},"links":{"cited_paper":"/paper/2010.00513","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:1f3f21eb8182479c11c5fdacf775524db7a6fcbdfe69d22b732e7c911c069f76","observation_id":"81e25707-814b-41cd-964d-460560195778","resolution":{"observed_at":"2026-08-03T20:12:23.409456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.06782","last_updated":"2020-08-25T01:01:56Z","snapshot_observed_at":"2026-08-18T21:13:14.600832Z","submitted_at":"2020-02-17T05:52:08Z","title":"Reducing the $H_{0}$ tension with generalized Proca theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.06782","snapshot_observed_at":"2026-08-03T20:12:23.412625Z","title":"De Felice, C.-Q","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.412625Z"},"links":{"cited_paper":"/paper/2002.06782","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:0e3308acdc62d7c86e9f9908f60b44717dbc1b0384cf1413bcbc0d37a7e47b15","observation_id":"156b4896-104c-4b03-85e0-680dea2bcf78","resolution":{"observed_at":"2026-08-03T20:12:23.412625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.04805","last_updated":"2019-06-11T20:31:12Z","snapshot_observed_at":"2026-08-14T16:17:11.970438Z","submitted_at":"2019-06-11T20:31:12Z","title":"Generalized Proca and its Constraint Algebra","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.04805","snapshot_observed_at":"2026-08-03T20:12:23.415621Z","title":"Beltrán Jiménez, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.415621Z"},"links":{"cited_paper":"/paper/1906.04805","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:402df19190f8eb3fe4e60235fe0be53f3a3365801d8e78cce47d796ca6ddb30f","observation_id":"6e8f87d0-271f-47de-ad33-57fb931314df","resolution":{"observed_at":"2026-08-03T20:12:23.415621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.13773","last_updated":"2020-10-06T15:27:34Z","snapshot_observed_at":"2026-08-17T12:52:21.834435Z","submitted_at":"2020-03-30T19:40:19Z","title":"New class of Proca interactions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.13773","snapshot_observed_at":"2026-08-03T20:12:23.418564Z","title":"de Rham and V","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.418564Z"},"links":{"cited_paper":"/paper/2003.13773","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:810b560428d99b808120782fd9faa6412d9164f560022e5aa09b941e8ba2c9b7","observation_id":"7af0844e-9498-492c-be71-b070ef6c55c3","resolution":{"observed_at":"2026-08-03T20:12:23.418564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.14327","last_updated":"2021-10-27T10:11:29Z","snapshot_observed_at":"2026-08-20T14:26:06.265079Z","submitted_at":"2021-10-27T10:11:29Z","title":"Cosmology of Extended Proca-Nuevo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.14327","snapshot_observed_at":"2026-08-03T20:12:23.421451Z","title":"de Rham, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.421451Z"},"links":{"cited_paper":"/paper/2110.14327","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:38a01bb5c98278f3833c5645bafd041ff63bbab4c44ef50137fb9178df82ac04","observation_id":"ecf51f34-abc1-4c0f-bb50-0bf8dbdb7ceb","resolution":{"observed_at":"2026-08-03T20:12:23.421451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0105068","last_updated":"2001-05-04T00:22:53Z","snapshot_observed_at":"2026-08-20T22:58:11.883072Z","submitted_at":"2001-05-04T00:22:53Z","title":"Accelerated Universe from Gravity Leaking to Extra Dimensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0105068","snapshot_observed_at":"2026-08-03T20:12:23.424352Z","title":"Deffayet, G.R","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.424352Z"},"links":{"cited_paper":"/paper/astro-ph/0105068","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:26f2170facf2a6915fd5edd88c5371c10ac22678ca1781c13c3e14fd80a4c90c","observation_id":"4cfaef05-c5ca-4b8e-95dc-1a8a4c476ce1","resolution":{"observed_at":"2026-08-03T20:12:23.424352Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.2197","last_updated":"2009-11-27T10:54:20Z","snapshot_observed_at":"2026-08-15T10:02:03.916725Z","submitted_at":"2008-11-13T20:58:48Z","title":"The galileon as a local modification of gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.2197","snapshot_observed_at":"2026-08-03T20:12:23.427302Z","title":"Nicolis, R","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.427302Z"},"links":{"cited_paper":"/paper/0811.2197","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:457cff1be758bd3a9517641f3f7c6c3d95128445ce714a54eeca2b1286ac8f0f","observation_id":"c1025b36-e355-4307-a0fa-e90d6577f3b1","resolution":{"observed_at":"2026-08-03T20:12:23.427302Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.0443","last_updated":"2010-08-12T19:13:53Z","snapshot_observed_at":"2026-08-20T16:52:24.163533Z","submitted_at":"2010-07-02T20:11:53Z","title":"Generalization of the Fierz-Pauli Action","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.0443","snapshot_observed_at":"2026-08-03T20:12:23.430125Z","title":"de Rham and G","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.430125Z"},"links":{"cited_paper":"/paper/1007.0443","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:7774f35a78e467f2be2c7b5cbee6a0c40bf60e6781d2b2befd84b7453eb8ca25","observation_id":"1b22af35-cf68-4906-a887-248941271aaa","resolution":{"observed_at":"2026-08-03T20:12:23.430125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.1232","last_updated":"2010-11-08T18:31:49Z","snapshot_observed_at":"2026-08-15T05:03:53.059717Z","submitted_at":"2010-11-04T18:24:57Z","title":"Resummation of Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.1232","snapshot_observed_at":"2026-08-03T20:12:23.433096Z","title":"de Rham, G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.433096Z"},"links":{"cited_paper":"/paper/1011.1232","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:7e0b1f9634947cc0fb10f03d44716b14ff9cb7964f01e9cc6b3a6f5f5cb9870d","observation_id":"20aeb5d4-4bcc-4166-b6d5-2e097c03bccc","resolution":{"observed_at":"2026-08-03T20:12:23.433096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.4173","last_updated":"2014-03-14T20:27:41Z","snapshot_observed_at":"2026-08-14T23:48:05.360265Z","submitted_at":"2014-01-16T21:00:17Z","title":"Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.4173","snapshot_observed_at":"2026-08-03T20:12:23.436680Z","title":"de Rham,Massive Gravity,Living Rev","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.436680Z"},"links":{"cited_paper":"/paper/1401.4173","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:41f996d1c34254997892cf94812cca8e28eba1f9a63eba3f17bb6d0830be1cab","observation_id":"1e0a5876-5d62-4502-b36e-6ecb0b843963","resolution":{"observed_at":"2026-08-03T20:12:23.436680Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.01639","last_updated":"2020-09-11T12:59:02Z","snapshot_observed_at":"2026-07-06T09:17:30.757691Z","submitted_at":"2020-05-04T16:54:08Z","title":"Quantum Stability of Generalized Proca Theories","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.01639","snapshot_observed_at":"2026-08-03T20:12:23.439575Z","title":"Heisenberg and J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.439575Z"},"links":{"cited_paper":"/paper/2005.01639","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:3c4be364ccf34a08ec568aadfd6e93bceddc9331384e7836361dc8f1c816ec92","observation_id":"ba221ae9-3022-4982-84fa-182b0c03217f","resolution":{"observed_at":"2026-08-03T20:12:23.439575Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.12892","last_updated":"2021-08-29T18:42:12Z","snapshot_observed_at":"2026-08-16T18:00:14.741467Z","submitted_at":"2021-08-29T18:42:12Z","title":"Quantum stability of Proca-Nuevo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.12892","snapshot_observed_at":"2026-08-03T20:12:23.442395Z","title":"de Rham, L","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.442395Z"},"links":{"cited_paper":"/paper/2108.12892","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:7f448dc0881e512d9b33e9242772c234e66c4925a32a5eaa8b843b8c50c30daa","observation_id":"74e098ff-ac7d-4223-978a-b52fc0ced747","resolution":{"observed_at":"2026-08-03T20:12:23.442395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.12631","last_updated":"2022-09-09T08:12:47Z","snapshot_observed_at":"2026-08-20T08:09:25.942326Z","submitted_at":"2022-08-26T12:46:01Z","title":"Positivity bounds in vector theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.12631","snapshot_observed_at":"2026-08-03T20:12:23.445776Z","title":"de Rham, L","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.445776Z"},"links":{"cited_paper":"/paper/2208.12631","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:28d81f8edb27a4659934ea2ec49c653419a66ae30797d3352e519028b4f6abbf","observation_id":"4be5a411-8756-4418-99f0-902225a5b784","resolution":{"observed_at":"2026-08-03T20:12:23.445776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.08462","last_updated":"2017-05-08T15:52:06Z","snapshot_observed_at":"2026-08-14T21:50:56.213462Z","submitted_at":"2016-06-27T20:05:45Z","title":"Graviton Mass Bounds","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.08462","snapshot_observed_at":"2026-08-03T20:12:23.450083Z","title":"de Rham, J.T","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.450083Z"},"links":{"cited_paper":"/paper/1606.08462","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:db538caa8c6729e3f1ff1c5c7efe247cc422232350c4cf073b836c2ffff5e56a","observation_id":"7013b49f-ad53-43d4-a11c-d51a63dda667","resolution":{"observed_at":"2026-08-03T20:12:23.450083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.4128","last_updated":"2012-12-17T20:36:15Z","snapshot_observed_at":"2026-08-15T00:35:24.698357Z","submitted_at":"2012-12-17T20:36:15Z","title":"Non-Renormalization and Naturalness in a Class of Scalar-Tensor Theories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.4128","snapshot_observed_at":"2026-08-03T20:12:23.461113Z","title":"de Rham, G","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.461113Z"},"links":{"cited_paper":"/paper/1212.4128","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:3ffe1f8acead416b4df05f450be7c5df472f4ccc671bde679cf26818acb9b791","observation_id":"f83eca14-bf1f-43ba-91ff-feb277e80ca1","resolution":{"observed_at":"2026-08-03T20:12:23.461113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.7169","last_updated":"2013-08-19T19:21:08Z","snapshot_observed_at":"2026-08-15T00:08:54.006326Z","submitted_at":"2013-07-26T21:11:14Z","title":"Quantum Corrections in Massive Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.7169","snapshot_observed_at":"2026-08-03T20:12:23.478816Z","title":"de Rham, L","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.478816Z"},"links":{"cited_paper":"/paper/1307.7169","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:2e9251e97e669e05d1c657357c3be3c44befffbbcccafd805faea3f071098868","observation_id":"27fe2684-9de9-444d-9857-0e480e83bf58","resolution":{"observed_at":"2026-08-03T20:12:23.478816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0408246","last_updated":"2004-09-01T17:15:40Z","snapshot_observed_at":"2026-07-07T00:44:05.995496Z","submitted_at":"2004-08-12T22:42:33Z","title":"How a brane cosmological constant can trick us into thinking that w < -1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0408246","snapshot_observed_at":"2026-08-03T20:12:23.495325Z","title":"Lue and G.D","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.495325Z"},"links":{"cited_paper":"/paper/astro-ph/0408246","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:cf6a0fb632b20e80a9f43c5fd8a11b59ff88ae4f55ea8396f1dd52d715e3b2b4","observation_id":"caab8510-beca-4579-9a6c-8b835b197d81","resolution":{"observed_at":"2026-08-03T20:12:23.495325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.15483","last_updated":"2024-05-23T19:07:13Z","snapshot_observed_at":"2026-08-16T14:31:52.727064Z","submitted_at":"2023-12-24T13:48:47Z","title":"Observational constraints on extended Proca-Nuevo gravity and cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.15483","snapshot_observed_at":"2026-08-03T20:12:23.511651Z","title":"Anagnostopoulos and E.N","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.511651Z"},"links":{"cited_paper":"/paper/2312.15483","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:38ca69ac5f8f35b6b7fc9f07e4b525a946462f613e93b8b8071757504a65daae","observation_id":"aa7ef539-a0eb-4dc6-bc76-94c504106ea4","resolution":{"observed_at":"2026-08-03T20:12:23.511651Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.02707","last_updated":"2024-11-26T10:39:44Z","snapshot_observed_at":"2026-08-17T21:39:34.396120Z","submitted_at":"2024-11-26T10:39:44Z","title":"Unveiling the Effects of Coupling Extended Proca-Nuevo Gravity on Cosmic Expansion with Recent Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.02707","snapshot_observed_at":"2026-08-03T20:12:23.527623Z","title":"Sudharani, N.S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.527623Z"},"links":{"cited_paper":"/paper/2412.02707","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:4ae6617002524523a653e4b7828c6a322bd95ef9a20a66bd70e6afffd25d883d","observation_id":"937564ee-a309-41e9-9f81-ab1fdecd0c51","resolution":{"observed_at":"2026-08-03T20:12:23.527623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.01066","last_updated":"2018-07-26T12:53:35Z","snapshot_observed_at":"2026-08-18T21:45:48.893978Z","submitted_at":"2018-05-03T00:41:53Z","title":"Cosmology in scalar-vector-tensor theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.01066","snapshot_observed_at":"2026-08-03T20:12:23.541688Z","title":"Heisenberg, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.541688Z"},"links":{"cited_paper":"/paper/1805.01066","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:129936c927651b852ea6f49efd1cd2dab485740b78d8c3ec27557df56ad0e99d","observation_id":"1d2dcee2-2dcc-49ea-b82b-097d3fdd5754","resolution":{"observed_at":"2026-08-03T20:12:23.541688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.03042","last_updated":"2020-07-06T20:02:09Z","snapshot_observed_at":"2026-08-15T15:38:12.213968Z","submitted_at":"2020-07-06T20:02:09Z","title":"Proca-stinated Cosmology I: A N-body code for the vector Galileon","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.03042","snapshot_observed_at":"2026-08-03T20:12:23.561069Z","title":"Becker, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.561069Z"},"links":{"cited_paper":"/paper/2007.03042","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:a35a3298b7287521950fc92a9b2c299a44efab657a2701497176ef3dead84f71","observation_id":"411828f7-18d1-417a-98b3-2bee5071259f","resolution":{"observed_at":"2026-08-03T20:12:23.561069Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.11299","last_updated":"2024-06-17T08:06:19Z","snapshot_observed_at":"2026-08-16T13:42:22.629891Z","submitted_at":"2024-06-17T08:06:19Z","title":"Proca in an Expanding Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.11299","snapshot_observed_at":"2026-08-03T20:12:23.582884Z","title":"Fell and L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.582884Z"},"links":{"cited_paper":"/paper/2406.11299","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:c0df7fedba32ce28d094e7bb79257ed575a37fe42f1862a65771fcb9d916bd1f","observation_id":"963fd0d6-42b6-4bd9-b506-9e8304138aad","resolution":{"observed_at":"2026-08-03T20:12:23.582884Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.03977","last_updated":"2025-02-25T17:02:45Z","snapshot_observed_at":"2026-08-17T19:17:56.914214Z","submitted_at":"2024-12-05T08:53:18Z","title":"To bounce or not to bounce in generalized Proca theory and beyond","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.03977","snapshot_observed_at":"2026-08-03T20:12:23.601336Z","title":"Bohnenblust, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.601336Z"},"links":{"cited_paper":"/paper/2412.03977","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:b0e83de1a3eaed688edc3e8ceb546b3b0657af8e21752ff793ae15893a4840c2","observation_id":"a0071469-ea49-45ed-81a0-5d805458966d","resolution":{"observed_at":"2026-08-03T20:12:23.601336Z","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":"2026-08-03T20:12:23.621522Z","title":"Kavya, L","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.621522Z"},"links":{"citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:5868577ea2f3535236c083e46af6eda130102ce7b63139f11a7661350d2667c4","observation_id":"b630ad2f-f4c0-46f5-93d2-d811b4a884a3","resolution":{"observed_at":"2026-08-03T20:12:23.621522Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.06133","last_updated":"2025-04-08T15:26:58Z","snapshot_observed_at":"2026-08-20T06:06:33.979996Z","submitted_at":"2025-04-08T15:26:58Z","title":"Gravitational Baryogenesis in Extended Proca-Nuevo Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.06133","snapshot_observed_at":"2026-08-03T20:12:23.626049Z","title":"Sultan,Gravitational Baryogenesis in Extended Proca-Nuevo Gravity, [2504.06133]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.626049Z"},"links":{"cited_paper":"/paper/2504.06133","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:b70dc846497f06e54e595572bb4d344345d7605bf5ba8e1e6a4be6ff2fa8fad5","observation_id":"478f1153-0359-499d-9ece-382e6c94788c","resolution":{"observed_at":"2026-08-03T20:12:23.626049Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.07773","last_updated":"2022-09-09T15:06:46Z","snapshot_observed_at":"2026-08-21T10:11:16.311855Z","submitted_at":"2022-06-15T19:17:41Z","title":"CMB lensing from Planck PR4 maps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.07773","snapshot_observed_at":"2026-08-03T20:12:23.629368Z","title":"Carron, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.629368Z"},"links":{"cited_paper":"/paper/2206.07773","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:cf800dccedabf147e975dd5318744861cedfac873210d9a10a31679ae02b0219","observation_id":"0348d4a2-4fbd-4bcc-86dc-aff29328ce7c","resolution":{"observed_at":"2026-08-03T20:12:23.629368Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04077","last_updated":"2022-11-14T21:28:25Z","snapshot_observed_at":"2026-08-20T17:32:03.134684Z","submitted_at":"2022-02-08T19:00:00Z","title":"The Pantheon+ Analysis: Cosmological Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04077","snapshot_observed_at":"2026-08-03T20:12:23.632268Z","title":"Brout et al.,The Pantheon+ Analysis: Cosmological Constraints,Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.632268Z"},"links":{"cited_paper":"/paper/2202.04077","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:1f9f309969c0826920162c8db72ecf3cac59c71bc4e54e67635a25f3756f2e40","observation_id":"645fc957-b9a3-4b9c-b127-ac351388aa04","resolution":{"observed_at":"2026-08-03T20:12:23.632268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3242","last_updated":"2015-01-21T19:36:11Z","snapshot_observed_at":"2026-08-19T14:23:15.084260Z","submitted_at":"2014-09-10T20:02:29Z","title":"The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.3242","snapshot_observed_at":"2026-08-03T20:12:23.635987Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.635987Z"},"links":{"cited_paper":"/paper/1409.3242","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:3e8096cdedd6af984ca5721703b6484b6e1038a1d604ae789b61c2f1b1b26d2d","observation_id":"4eb0291a-d689-473e-ba32-6f4a07f96c27","resolution":{"observed_at":"2026-08-03T20:12:23.635987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.4725","last_updated":"2012-04-20T20:00:03Z","snapshot_observed_at":"2026-08-17T12:05:33.658452Z","submitted_at":"2012-04-20T20:00:03Z","title":"The 6dF Galaxy Survey: z \\approx 0 measurement of the growth rate and sigma_8","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.4725","snapshot_observed_at":"2026-08-03T20:12:23.638980Z","title":"Beutler, C","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.638980Z"},"links":{"cited_paper":"/paper/1204.4725","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:b98721264b7c9a11ccd327456b9cc1a0daf0ddecd72b1cc1b68c05698a0fb29f","observation_id":"ba7e1cff-8fd0-4635-8215-7aa0b8ee5c7b","resolution":{"observed_at":"2026-08-03T20:12:23.638980Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.02710","last_updated":"2019-01-25T15:36:51Z","snapshot_observed_at":"2026-08-14T20:05:52.223298Z","submitted_at":"2017-12-07T16:48:17Z","title":"Cosmological Constraints on Horndeski Gravity in Light of GW170817","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.02710","snapshot_observed_at":"2026-08-03T20:12:23.642035Z","title":"Kreisch and E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.642035Z"},"links":{"cited_paper":"/paper/1712.02710","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:9e591541ee3852f4b6892c53203d689829684fd693ea74b0dbade8f2f2eac8ef","observation_id":"a89a1b58-fbae-4b0d-9b40-d86e3a67c473","resolution":{"observed_at":"2026-08-03T20:12:23.642035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12928","last_updated":"2018-11-30T18:27:57Z","snapshot_observed_at":"2026-08-15T14:34:45.003744Z","submitted_at":"2018-11-30T18:27:57Z","title":"Cosmological parameter constraints for Horndeski scalar-tensor gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.12928","snapshot_observed_at":"2026-08-03T20:12:23.645215Z","title":"Noller and A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.645215Z"},"links":{"cited_paper":"/paper/1811.12928","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:222fa3cb7c296da852794464605eec262c8435585c61f3d6642c1a0908f7c655","observation_id":"db8bce5c-65de-4afb-af81-aa2a254a187c","resolution":{"observed_at":"2026-08-03T20:12:23.645215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03686","last_updated":"2019-10-24T08:49:26Z","snapshot_observed_at":"2026-08-18T03:31:51.922626Z","submitted_at":"2019-01-11T18:45:39Z","title":"KiDS+GAMA: Constraints on Horndeski gravity from combined large-scale structure probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03686","snapshot_observed_at":"2026-08-03T20:12:23.648060Z","title":"Spurio Mancini, F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.648060Z"},"links":{"cited_paper":"/paper/1901.03686","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:8100c2b0bbe048869bd0da787244450a142e62993e8e722974cd11007ae8d889","observation_id":"5807be5b-fd16-42e8-b9e6-bd40f5907ae6","resolution":{"observed_at":"2026-08-03T20:12:23.648060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.11171","last_updated":"2020-05-21T06:12:05Z","snapshot_observed_at":"2026-08-20T12:30:38.012148Z","submitted_at":"2020-05-21T06:12:05Z","title":"Constraints on dark energy models from the Horndeski theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.11171","snapshot_observed_at":"2026-08-03T20:12:23.650992Z","title":"Bayarsaikhan, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.650992Z"},"links":{"cited_paper":"/paper/2005.11171","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:22a892e5757e7cdce9e367f6f69212d2d972885aae085bd4ed6642a931b920f0","observation_id":"feb1ee71-9e06-4a92-a7ac-baf5acec90b4","resolution":{"observed_at":"2026-08-03T20:12:23.650992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.11195","last_updated":"2021-10-27T10:03:05Z","snapshot_observed_at":"2026-08-16T18:37:35.348833Z","submitted_at":"2021-03-20T15:14:26Z","title":"Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.11195","snapshot_observed_at":"2026-08-03T20:12:23.654427Z","title":"Traykova, E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.654427Z"},"links":{"cited_paper":"/paper/2103.11195","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:1b355be6e37bf72ddc83ab5792c294a7c6bf0e2e75119c08432ce242d29bed93","observation_id":"325eef62-0184-4851-b33b-74bc94e5589c","resolution":{"observed_at":"2026-08-03T20:12:23.654427Z","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":"2026-08-03T20:12:23.657416Z","title":"Capozziello, R","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.657416Z"},"links":{"citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:71154dd3d6a565fa3e5afa1b35119febd85764d397f807e414f92f3feaff5209","observation_id":"2de4958c-b2c7-4095-acb0-4a246d0c62c1","resolution":{"observed_at":"2026-08-03T20:12:23.657416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510519","last_updated":"2006-04-18T13:20:24Z","snapshot_observed_at":"2026-08-14T11:11:55.906107Z","submitted_at":"2005-10-18T12:29:56Z","title":"Cosmological constraints on f(R) gravity theories within the Palatini approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510519","snapshot_observed_at":"2026-08-03T20:12:23.660207Z","title":"Amarzguioui, O","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.660207Z"},"links":{"cited_paper":"/paper/astro-ph/0510519","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:fadba065d38e8af56faf1fbdcf47e17913fad6131277792ca70adc24f2f7128a","observation_id":"97ae3448-4631-4c14-9a03-872f26b373e0","resolution":{"observed_at":"2026-08-03T20:12:23.660207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.15335","last_updated":"2020-11-09T09:12:12Z","snapshot_observed_at":"2026-08-13T22:17:59.334987Z","submitted_at":"2020-06-27T10:34:54Z","title":"Updating constraints on f(T) teleparallel cosmology and the consistency with Big Bang Nucleosynthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.15335","snapshot_observed_at":"2026-08-03T20:12:23.663246Z","title":"Benetti, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.663246Z"},"links":{"cited_paper":"/paper/2006.15335","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:48de81336c0b5d73217591f402f6e0c32865d8566d3537e6d83c81e0860f84f3","observation_id":"0719e439-5a00-47ba-8211-feab5bcb4e1e","resolution":{"observed_at":"2026-08-03T20:12:23.663246Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.11131","last_updated":"2023-03-19T02:41:25Z","snapshot_observed_at":"2026-08-21T01:51:21.311548Z","submitted_at":"2022-09-22T16:18:03Z","title":"New cosmological constraints on $f(T)$ gravity in light of full Planck-CMB and type Ia supernovae data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.11131","snapshot_observed_at":"2026-08-03T20:12:23.666280Z","title":"Kumar, R.C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.666280Z"},"links":{"cited_paper":"/paper/2209.11131","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:ed5a7510a4851460eb4e97dd92821466550131527188c4d1251ff1cc7d4c0185","observation_id":"f6d1f16a-2039-41f3-a323-86c7192a1f5c","resolution":{"observed_at":"2026-08-03T20:12:23.666280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.10027","last_updated":"2021-04-12T15:47:27Z","snapshot_observed_at":"2026-08-18T21:12:35.163813Z","submitted_at":"2019-06-24T15:31:02Z","title":"Cosmology in $f(Q)$ geometry","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.10027","snapshot_observed_at":"2026-08-03T20:12:23.669450Z","title":"Beltrán Jiménez, L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.669450Z"},"links":{"cited_paper":"/paper/1906.10027","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:513ec7e8cdb9a315d8fcd7ac0ea3beed52256e550d6f305b4c1a694afcfe36fc","observation_id":"8f33c5a2-0001-4811-bda4-635c42223c7a","resolution":{"observed_at":"2026-08-03T20:12:23.669450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.00345","last_updated":"2017-06-21T13:26:47Z","snapshot_observed_at":"2026-08-14T21:27:34.995099Z","submitted_at":"2016-12-01T16:46:23Z","title":"Holographic Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.00345","snapshot_observed_at":"2026-08-03T20:12:23.672537Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.672537Z"},"links":{"cited_paper":"/paper/1612.00345","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:a0861043eec8083bda0502660933a3ef93a0198e1d440d672c2cc3eae918adc4","observation_id":"714481d6-c36e-42a9-bd0c-ec6453c89166","resolution":{"observed_at":"2026-08-03T20:12:23.672537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0301510","last_updated":"2003-01-25T00:34:08Z","snapshot_observed_at":"2026-07-07T00:30:57.641930Z","submitted_at":"2003-01-25T00:34:08Z","title":"Dark Energy as a Modification of the Friedmann Equation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0301510","snapshot_observed_at":"2026-08-03T20:12:23.675574Z","title":"Dvali and M.S","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.675574Z"},"links":{"cited_paper":"/paper/astro-ph/0301510","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:078210af76ae338644141fc44ff9f86b6488e129a739744dc47ac9ae11635df7","observation_id":"2a93ca97-ad96-47d0-bf08-bae1d434d3ea","resolution":{"observed_at":"2026-08-03T20:12:23.675574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9905012","last_updated":"1999-06-25T13:07:48Z","snapshot_observed_at":"2026-08-18T23:25:21.416014Z","submitted_at":"1999-05-03T13:40:58Z","title":"Non-conventional cosmology from a brane-universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9905012","snapshot_observed_at":"2026-08-03T20:12:23.679154Z","title":"Binetruy, C","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.679154Z"},"links":{"cited_paper":"/paper/hep-th/9905012","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:523a0bae1b5280a93f4d046760f62225089bf80908604382d7107d4298609100","observation_id":"c7df8826-7da8-4a65-9427-141a50182256","resolution":{"observed_at":"2026-08-03T20:12:23.679154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9910219","last_updated":"2000-02-04T12:04:02Z","snapshot_observed_at":"2026-08-08T00:48:08.012333Z","submitted_at":"1999-10-27T22:21:44Z","title":"Brane cosmological evolution in a bulk with cosmological constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9910219","snapshot_observed_at":"2026-08-03T20:12:23.682123Z","title":"Binetruy, C","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.682123Z"},"links":{"cited_paper":"/paper/hep-th/9910219","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:6e464ffeda9b4eb60f812634c480d7f76105f460e1b502acc3b3452644e93016","observation_id":"fbbf5ec8-8e17-44e9-9d97-dd8c54e559fa","resolution":{"observed_at":"2026-08-03T20:12:23.682123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0010186","last_updated":"2000-11-07T20:51:36Z","snapshot_observed_at":"2026-08-20T19:51:14.043707Z","submitted_at":"2000-10-23T22:34:39Z","title":"Cosmology on a Brane in Minkowski Bulk","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0010186","snapshot_observed_at":"2026-08-03T20:12:23.685084Z","title":"Deffayet,Cosmology on a brane in Minkowski bulk,Phys","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.685084Z"},"links":{"cited_paper":"/paper/hep-th/0010186","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:3222343cea25fbe8d656971a2fd845ed83361f47cde09b6735428389c3f1d71b","observation_id":"d1218532-4aca-48f6-8c83-e43997024dd4","resolution":{"observed_at":"2026-08-03T20:12:23.685084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.09417","last_updated":"2018-12-17T16:19:29Z","snapshot_observed_at":"2026-08-14T18:59:39.854853Z","submitted_at":"2018-06-25T12:28:32Z","title":"Gravitational Rainbows: LIGO and Dark Energy at its Cutoff","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.09417","snapshot_observed_at":"2026-08-03T20:12:23.687987Z","title":"de Rham and S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.687987Z"},"links":{"cited_paper":"/paper/1806.09417","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:f6694236e49f9236a979a657884bf05e8fee4aac13a9059cce6aaf953f004b2b","observation_id":"e5dc4596-c957-45de-95f0-94d45af0db70","resolution":{"observed_at":"2026-08-03T20:12:23.687987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.10096","last_updated":"2022-10-24T16:41:23Z","snapshot_observed_at":"2026-08-19T12:23:59.055302Z","submitted_at":"2022-07-20T18:00:02Z","title":"Probing the speed of gravity with LVK, LISA, and joint observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.10096","snapshot_observed_at":"2026-08-03T20:12:23.691114Z","title":"Harry and J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.691114Z"},"links":{"cited_paper":"/paper/2207.10096","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:8d2a9412a37bdeec7317d495f572bb18e3d8e940c835a98a1cc28b7d99efa411","observation_id":"a7cfa263-6cf5-4e3e-9005-1823c8996317","resolution":{"observed_at":"2026-08-03T20:12:23.691114Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14398","last_updated":"2023-03-27T21:58:47Z","snapshot_observed_at":"2026-08-18T04:30:54.035715Z","submitted_at":"2022-09-28T19:48:20Z","title":"Testing gravitational wave propagation with multiband detections","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.14398","snapshot_observed_at":"2026-08-03T20:12:23.694351Z","title":"Baker, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.694351Z"},"links":{"cited_paper":"/paper/2209.14398","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:16d5cb74b7ea1c5baa504cb09d44437005e65f0bf48d6b5db2e43ed5750206c4","observation_id":"e777f9e8-9bcb-45da-a9f9-9796221e50c5","resolution":{"observed_at":"2026-08-03T20:12:23.694351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9911177","last_updated":"2000-06-01T12:13:06Z","snapshot_observed_at":"2026-07-07T01:29:40.678750Z","submitted_at":"1999-11-10T17:57:36Z","title":"Efficient Computation of CMB anisotropies in closed FRW models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9911177","snapshot_observed_at":"2026-08-03T20:12:23.697452Z","title":"Lewis, A","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.697452Z"},"links":{"cited_paper":"/paper/astro-ph/9911177","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:7061b2e962fe31fa5c796c01caf91e1af4689b641c1f87657da9649e186205ee","observation_id":"a371ff6b-f0b2-476c-a8f4-81d178ed591e","resolution":{"observed_at":"2026-08-03T20:12:23.697452Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.3654","last_updated":"2012-04-19T11:36:17Z","snapshot_observed_at":"2026-08-19T23:50:01.657916Z","submitted_at":"2012-01-17T22:12:30Z","title":"CMB power spectrum parameter degeneracies in the era of precision cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.3654","snapshot_observed_at":"2026-08-03T20:12:23.700451Z","title":"Howlett, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.700451Z"},"links":{"cited_paper":"/paper/1201.3654","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:a488a1b3e21b48a5f1bc4f9a9abc8e2397a1852941c254f4b2b562972eb4f4dd","observation_id":"1fbe7653-7af9-4e7a-b03f-f56885a226db","resolution":{"observed_at":"2026-08-03T20:12:23.700451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0001493","last_updated":"2000-01-28T01:15:05Z","snapshot_observed_at":"2026-08-18T15:19:40.537398Z","submitted_at":"2000-01-28T01:15:05Z","title":"Analytic model for galaxy and dark matter clustering","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0001493","snapshot_observed_at":"2026-08-03T20:12:23.703715Z","title":"Seljak,Analytic model for galaxy and dark matter clustering,Mon","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.703715Z"},"links":{"cited_paper":"/paper/astro-ph/0001493","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:5c96d84169cb5411f1ccf8afe20fae21b5138b561e2e7c662d5676064690183b","observation_id":"3f274271-e2f7-403a-87fa-e39b80f6899b","resolution":{"observed_at":"2026-08-03T20:12:23.703715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.01858","last_updated":"2021-01-08T11:17:50Z","snapshot_observed_at":"2026-08-19T14:01:17.504877Z","submitted_at":"2020-09-03T18:00:09Z","title":"HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.01858","snapshot_observed_at":"2026-08-03T20:12:23.706623Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.706623Z"},"links":{"cited_paper":"/paper/2009.01858","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:107d8d9235b5f61e37d156e9ab22db7a9eda8953fe4aa462dd620ef690bc5d10","observation_id":"4f04fa9d-210b-4597-a0c9-5d395e8feb2b","resolution":{"observed_at":"2026-08-03T20:12:23.706623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9510117","last_updated":"1996-04-19T18:52:38Z","snapshot_observed_at":"2026-08-20T00:49:28.135726Z","submitted_at":"1995-10-23T16:35:10Z","title":"Small Scale Cosmological Perturbations: An Analytic Approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9510117","snapshot_observed_at":"2026-08-03T20:12:23.709676Z","title":"Hu and N","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.709676Z"},"links":{"cited_paper":"/paper/astro-ph/9510117","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:aa44d73aee39a76159b36687f7fdefdf881619de61a06110fde6dc36e347ec06","observation_id":"8e4ab252-811c-4071-80d7-daa8dd7d6ca3","resolution":{"observed_at":"2026-08-03T20:12:23.709676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.05290","last_updated":"2021-05-20T11:52:55Z","snapshot_observed_at":"2026-08-03T14:56:09.086229Z","submitted_at":"2020-05-11T17:49:03Z","title":"Cobaya: Code for Bayesian Analysis of hierarchical physical models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.05290","snapshot_observed_at":"2026-08-03T20:12:23.712718Z","title":"Torrado and A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.712718Z"},"links":{"cited_paper":"/paper/2005.05290","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:2a900c73091083c4e633177a2ed84a13ab893f46d7f176e321ffa92193e7f12f","observation_id":"465b945d-ae0b-4c09-97d0-e68e998fd399","resolution":{"observed_at":"2026-08-03T20:12:23.712718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205436","last_updated":"2002-10-14T18:03:43Z","snapshot_observed_at":"2026-07-07T00:26:35.863418Z","submitted_at":"2002-05-24T19:54:59Z","title":"Cosmological parameters from CMB and other data: a Monte-Carlo approach","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0205436","snapshot_observed_at":"2026-08-03T20:12:23.715621Z","title":"Lewis and S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.715621Z"},"links":{"cited_paper":"/paper/astro-ph/0205436","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:562c670055e35d855832f3ff39ca20ae1dde7cf0ea10ee4ea9c7b7e2f2b05cbc","observation_id":"fb3d858f-6a65-4b69-9c74-e5837be55644","resolution":{"observed_at":"2026-08-03T20:12:23.715621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.4473","last_updated":"2013-05-30T10:24:42Z","snapshot_observed_at":"2026-08-17T06:22:40.327358Z","submitted_at":"2013-04-16T14:43:03Z","title":"Efficient sampling of fast and slow cosmological parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.4473","snapshot_observed_at":"2026-08-03T20:12:23.719014Z","title":"Lewis,Efficient sampling of fast and slow cosmological parameters,Phys","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.719014Z"},"links":{"cited_paper":"/paper/1304.4473","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:6dc2e0fdd8087978aade3e74d7a0fcc2bdcda16da9b87e1cefecc459b02e0ae3","observation_id":"31ed3746-3340-4d10-b2f8-6a289f822e86","resolution":{"observed_at":"2026-08-03T20:12:23.719014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"math/0502099","last_updated":"2005-02-06T19:37:09Z","snapshot_observed_at":"2026-08-05T13:06:47.790593Z","submitted_at":"2005-02-06T19:37:09Z","title":"Taking Bigger Metropolis Steps by Dragging Fast Variables","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"math/0502099","snapshot_observed_at":"2026-08-03T20:12:23.721985Z","title":"Neal,Taking Bigger Metropolis Steps by Dragging Fast Variables,arXiv Mathematics e-prints(2005) math/0502099 [math/0502099]","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.721985Z"},"links":{"cited_paper":"/paper/math/0502099","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:06d78e78026a1435875a8b5f348315e495d796de38c784ef021b7b7bcadd4432","observation_id":"10816054-4dd1-4a63-8f6a-3a6723162aca","resolution":{"observed_at":"2026-08-03T20:12:23.721985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-08-12T19:40:10.586390Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-08-03T20:12:23.724908Z","title":"Lewis,GetDist: a Python package for analysing Monte Carlo samples, [1910.13970]","venue":null,"work_id":null,"year":1910},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.724908Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:c2cb5ddaa7d7c5190e660856e498c9210ad03020ebe6589fc897645cabd03f2d","observation_id":"8c225d9f-e5eb-4883-a09e-1903dd50229b","resolution":{"observed_at":"2026-08-03T20:12:23.724908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.07829","last_updated":"2022-07-01T21:01:39Z","snapshot_observed_at":"2026-08-21T04:11:12.377690Z","submitted_at":"2022-01-19T19:22:27Z","title":"Inferring $S_8(z)$ and $\\gamma(z)$ with cosmic growth rate measurements using machine learning","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.07829","snapshot_observed_at":"2026-08-03T20:12:23.728018Z","title":"Avila, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.728018Z"},"links":{"cited_paper":"/paper/2201.07829","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:552736fad51c3a66c7c0bb4b7f9e86bba3bbbe6588e03d48d447f49d85355894","observation_id":"8cc2143c-1c19-4bcd-bf6d-63653694831d","resolution":{"observed_at":"2026-08-03T20:12:23.728018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.0631","last_updated":"2011-11-07T17:33:47Z","snapshot_observed_at":"2026-08-15T04:30:08.764963Z","submitted_at":"2011-11-02T20:00:03Z","title":"Cosmic flows in the nearby universe from Type Ia Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.0631","snapshot_observed_at":"2026-08-03T20:12:23.730846Z","title":"Turnbull, M.J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.730846Z"},"links":{"cited_paper":"/paper/1111.0631","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:ac5d95bd1d63e9a3984c4d8d7ac9ecfe558278f05ff021c0fdefaa2a71e44b35","observation_id":"44a6d569-e0df-4fcd-935c-a460a3ddf656","resolution":{"observed_at":"2026-08-03T20:12:23.730846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.03092","last_updated":"2017-03-21T16:11:33Z","snapshot_observed_at":"2026-08-14T21:53:25.395015Z","submitted_at":"2016-06-09T20:00:01Z","title":"Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.03092","snapshot_observed_at":"2026-08-03T20:12:23.734153Z","title":"Achitouv, C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":105,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.734153Z"},"links":{"cited_paper":"/paper/1606.03092","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:25f38503ccda5331ed8dfe22b4b9b5b5d4a1b5f0193cdc05619c0cdd1022b859","observation_id":"a70407c6-89c7-4025-b820-7b8ba464d62b","resolution":{"observed_at":"2026-08-03T20:12:23.734153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.05945","last_updated":"2015-06-16T21:45:35Z","snapshot_observed_at":"2026-08-19T01:57:03.515590Z","submitted_at":"2015-03-19T21:00:22Z","title":"Growth rate of cosmological perturbations at z ~ 0.1 from a new observational test","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.05945","snapshot_observed_at":"2026-08-03T20:12:23.737024Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":106,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.737024Z"},"links":{"cited_paper":"/paper/1503.05945","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:4c3f731cf07ba5d2c9aad4d4212ba5b26b87df8e6f076bfdce11264c0d06fe60","observation_id":"67e9217c-a610-49d3-8e21-8e316117ea8b","resolution":{"observed_at":"2026-08-03T20:12:23.737024Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.3674","last_updated":"2012-06-12T13:33:50Z","snapshot_observed_at":"2026-08-15T10:30:30.630437Z","submitted_at":"2012-04-17T00:35:31Z","title":"The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.3674","snapshot_observed_at":"2026-08-03T20:12:23.740254Z","title":"Blake et al.,The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z<1,Mon","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":109,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.740254Z"},"links":{"cited_paper":"/paper/1204.3674","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:f49e31cf7de062c4bf970419a2e14ba3d1b9b738882df95f3812c617b0027e2e","observation_id":"3e7faaef-21c5-43e5-82c1-a9b8466c294f","resolution":{"observed_at":"2026-08-03T20:12:23.740254Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01030","last_updated":"2019-06-17T16:06:34Z","snapshot_observed_at":"2026-08-15T00:08:51.126316Z","submitted_at":"2019-04-01T18:00:51Z","title":"Beyond BAO: improving cosmological constraints from BOSS with measurement of the void-galaxy cross-correlation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.01030","snapshot_observed_at":"2026-08-03T20:12:23.743236Z","title":"Nadathur, P.M","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":110,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.743236Z"},"links":{"cited_paper":"/paper/1904.01030","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:0babb85d5e959cccee5faafd631ca7a4b65a2ca26cb30c718761c118091bb524","observation_id":"59c4fd3a-3e45-4133-b33c-1307ab5101a6","resolution":{"observed_at":"2026-08-03T20:12:23.743236Z","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":"2026-08-03T20:12:23.746221Z","title":"Wilson,Geometric and growth rate tests of General Relativity with recovered linear cosmological perturbations, Ph.D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.746221Z"},"links":{"citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:d84baaafd2fcd01dd55239470fd9f8ff477d5210627051a828fcca885d3d7cc5","observation_id":"395f75d4-a2f2-4cc3-8f55-f955982a873e","resolution":{"observed_at":"2026-08-03T20:12:23.746221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.08083","last_updated":"2016-03-25T15:00:13Z","snapshot_observed_at":"2026-08-14T22:21:20.493212Z","submitted_at":"2015-11-25T15:15:20Z","title":"The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at $z\\sim 1.4$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.08083","snapshot_observed_at":"2026-08-03T20:12:23.748845Z","title":"Okumura et al.,The Subaru FMOS galaxy redshift survey (FastSound)","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.748845Z"},"links":{"cited_paper":"/paper/1511.08083","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:22fef11d8145b6f0b1a642158678f186d216f7aae55e96b7bd621f4422bee04c","observation_id":"e6ff2c6f-f209-4bac-abe7-dc0f0131da1f","resolution":{"observed_at":"2026-08-03T20:12:23.748845Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","latest_version":2,"primary_category":"hep-th","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":100,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":107},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 100 of 107 outbound references and 3 inbound Pith citation observations for arXiv:2511.21071."}