{"as_of":"2026-08-16T06:08:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9fdec9f753459bbec31ec7d8bf2f64fe27ebd854863b2e01e62c4cf2decb2d6e","coverage":[{"denominator":69,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":69,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T17:14:14.408010Z","state":"measured"},{"denominator":69,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":69,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2508.17795/citation-record","integrity":"/paper/2508.17795/integrity","json":"/paper/2508.17795/citation-record.json","paper":"/paper/2508.17795"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.105500Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.105500Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:83824198b285cf9c64a446d2b8cacf7426a944a3cadbac57809f402f8297cb9d","observation_id":"29319ec0-ed2b-4a56-9bc3-d0dbf03c219a","resolution":{"observed_at":"2026-08-15T17:14:14.105500Z","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":"2026-08-15T17:14:14.111119Z","title":"Perlmutter et al","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.111119Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:2b6b760c12239da5b69098fab35e2fa6c57f9f4864dc4d531756e3dedaa1def3","observation_id":"391eee47-8e12-4f81-9d35-7236846b1c5d","resolution":{"observed_at":"2026-08-15T17:14:14.111119Z","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":"2026-08-15T17:14:14.115439Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.115439Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:cb80920bec3efd5f6d3b88f8142d250998450b93616f352097d282e965ee9176","observation_id":"520dc287-3a56-4525-a84d-1c7e7173b94e","resolution":{"observed_at":"2026-08-15T17:14:14.115439Z","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":"2026-08-15T17:14:14.119613Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.119613Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:fd6eed4f203abcb19f14f4bdfd509b312b2b310d27bee24504b4a38864161776","observation_id":"bf9a9eef-a456-4038-b8c9-f05a89c2ba04","resolution":{"observed_at":"2026-08-15T17:14:14.119613Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-15T17:14:14.123639Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.123639Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:654ee2c6770178ca542e311b0f5d9d8ad5400a743967458c399b937861ee80c3","observation_id":"8847f85c-95f0-4405-acbb-debeab70f9ab","resolution":{"observed_at":"2026-08-15T17:14:14.123639Z","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":"2026-08-15T17:14:14.128052Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.128052Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:7984f53376cb837ca7aaab433873af14f5b390b09c74a8135220c3af8d499e2a","observation_id":"06ea5b26-017c-435f-bc59-20b111a0a3cf","resolution":{"observed_at":"2026-08-15T17:14:14.128052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.2476","last_updated":"2012-03-12T12:39:47Z","snapshot_observed_at":"2026-07-06T02:29:12.672489Z","submitted_at":"2011-06-13T16:06:49Z","title":"Modified Gravity and Cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.2476","snapshot_observed_at":"2026-08-15T17:14:14.132504Z","title":"Clifton, P","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.132504Z"},"links":{"cited_paper":"/paper/1106.2476","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:51a8c624a3c6ab50db1a6d1f5b0a7764f48d4abe91b15c2fb0da5b8ccfc73c8b","observation_id":"192461d1-a2b3-4bd0-a340-3cec43e5c1ef","resolution":{"observed_at":"2026-08-15T17:14:14.132504Z","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":"2026-08-15T17:14:14.136771Z","title":"Ishak, Living Rev","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.136771Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:2177956b0375b3951dc2930fe51bf38347885deb505550aa053ec87c14b049e0","observation_id":"3853269a-6c71-4143-8cfc-2b71eeb67a60","resolution":{"observed_at":"2026-08-15T17:14:14.136771Z","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":"2026-08-15T17:14:14.140663Z","title":"Yoo and Y","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.140663Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:bb17d9f13f2ed88b6cf0ce3530a796cbd8b07903dcbd2da7e7c60bacb094fb84","observation_id":"24ca1231-a637-4f95-8100-391b377c9cf6","resolution":{"observed_at":"2026-08-15T17:14:14.140663Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2024/05/033","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.753904Z","title":"Patil, Ruchika and S","venue":null,"work_id":"41c55deb-d029-425c-90eb-1df82861393c","year":2024},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.144913Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:d56c6c3bbf3eb19d5097b2b34c0df638774452134d13aae81828d1e6639141d3","observation_id":"621035c3-c548-40a2-b892-f0902ae4a465","resolution":{"observed_at":"2026-08-15T17:14:14.757992Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.148919Z","title":"Bousso, Gen","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.148919Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:0a481cdcd906d0626734365a3ce9279ac077b67fe89a2984c682eeb0a74bba72","observation_id":"bbd93252-1521-4e67-ab82-ea16c8a20830","resolution":{"observed_at":"2026-08-15T17:14:14.148919Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.04190","last_updated":"2024-03-01T16:17:27Z","snapshot_observed_at":"2026-08-14T18:10:22.944753Z","submitted_at":"2024-01-08T19:03:59Z","title":"Is it possible to know cosmological fine-tuning?","version":2},"cited_work":{"arxiv_id":"2401.04190","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.04190","snapshot_observed_at":"2026-08-15T17:14:15.777790Z","title":"Is it possible to know cosmological fine-tuning?","venue":"astro-ph.CO","work_id":"6b408c17-b072-47bb-af0f-7876e031dded","year":2024},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.153108Z"},"links":{"cited_paper":"/paper/2401.04190","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:3c0294a32940e8011920b821c0cdfedb1189f7f7a27bef5e0a0340253d4cd655","observation_id":"51231db4-79dd-42b8-b85d-5b88cb7f8470","resolution":{"observed_at":"2026-08-15T17:14:15.782763Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.157086Z","title":"Gubitosi, F","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.157086Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:3ce03ac8673cedc17cf64ba8cc2616dd4952c20c32ed5c518ee2c4e41d875739","observation_id":"3eb38ae9-6c79-498b-a8e3-92af545a77dc","resolution":{"observed_at":"2026-08-15T17:14:14.157086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16911","last_updated":"2024-04-12T13:44:53Z","snapshot_observed_at":"2026-08-13T05:40:26.006507Z","submitted_at":"2023-10-25T18:22:34Z","title":"Observational Constraints on Dynamical Dark Energy Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16911","snapshot_observed_at":"2026-08-15T17:14:14.161015Z","title":"Avsajanishvili, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.161015Z"},"links":{"cited_paper":"/paper/2310.16911","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:fd492883740359037aeac9cb1f14263a6486c989cdc53dbfb1683bbe996a0e68","observation_id":"379b8973-301d-48da-b01c-e6e4d39b4ece","resolution":{"observed_at":"2026-08-15T17:14:14.161015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0603057","last_updated":"2006-06-16T10:46:50Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2006-03-08T01:25:15Z","title":"Dynamics of dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0603057","snapshot_observed_at":"2026-08-15T17:14:14.165185Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.165185Z"},"links":{"cited_paper":"/paper/hep-th/0603057","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:69a4a65906e37ec8d7418ceaa919c060ed3509b4c907f8de4a909a688aab58b9","observation_id":"1d51d278-2676-4ffc-a1a6-5af1884c0ac5","resolution":{"observed_at":"2026-08-15T17:14:14.165185Z","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":"2026-08-15T17:14:14.169100Z","title":"Ratra and P","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.169100Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:efeb1dfd9f8a8dff10a90cbfc5215c60a2e826d060ed67adb326f434b1370447","observation_id":"e28a98d1-feb1-4218-b3c7-26721e4f36be","resolution":{"observed_at":"2026-08-15T17:14:14.169100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.03844","last_updated":"2017-11-08T15:29:09Z","snapshot_observed_at":"2026-08-14T20:15:39.634804Z","submitted_at":"2017-11-08T15:29:09Z","title":"Cosmology and the Fate of Dilatation Symmetry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.03844","snapshot_observed_at":"2026-08-15T17:14:14.173257Z","title":"Wetterich, Nucl","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.173257Z"},"links":{"cited_paper":"/paper/1711.03844","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:68280002a38c98fbd1d00e450347812794a45de9778a111133ba3afdedd62ff4","observation_id":"8454b864-bf18-4540-ab5b-c5cad74de1e5","resolution":{"observed_at":"2026-08-15T17:14:14.173257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9708069","last_updated":"1998-02-06T00:41:37Z","snapshot_observed_at":"2026-08-04T03:32:57.284631Z","submitted_at":"1997-08-07T19:39:25Z","title":"Cosmological Imprint of an Energy Component with General Equation of State","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9708069","snapshot_observed_at":"2026-08-15T17:14:14.177681Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.177681Z"},"links":{"cited_paper":"/paper/astro-ph/9708069","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:46c3496423ed14b7ab70fdb21e09bc0180ab2ad098b9ae603293da3acbe1adad","observation_id":"49a736a5-7ce1-4ab0-b1f2-1be98c1f05d8","resolution":{"observed_at":"2026-08-15T17:14:14.177681Z","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":"2026-08-15T17:14:14.183121Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.183121Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:debc8b6b908e33e9bd3f21fe6b22d6628672306ee0590c13b2eb677884c1541f","observation_id":"9ee83415-0e56-4f14-b60c-c676162ceea9","resolution":{"observed_at":"2026-08-15T17:14:14.183121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.0056","last_updated":"2012-02-11T01:52:47Z","snapshot_observed_at":"2026-08-15T04:45:05.124456Z","submitted_at":"2011-05-31T23:08:46Z","title":"Kinetic k-essence ghost dark energy model","version":3},"cited_work":{"arxiv_id":"1106.0056","doi":null,"metadata_source":"pith","pith_arxiv_id":"1106.0056","snapshot_observed_at":"2026-08-15T17:14:15.626140Z","title":"Kinetic k-essence ghost dark energy model","venue":"astro-ph.CO","work_id":"a46078b0-c04e-4605-8f4a-ef7e83133fa9","year":2011},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.187292Z"},"links":{"cited_paper":"/paper/1106.0056","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:c336c872c914bd67ed20216decb3682d461be35c61b940c8df0f93e78b37023b","observation_id":"911b4965-f42f-4ced-b9d9-c1445dc4fc8a","resolution":{"observed_at":"2026-08-15T17:14:15.632042Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.06981","last_updated":"2017-09-24T19:20:20Z","snapshot_observed_at":"2026-08-14T20:39:40.646194Z","submitted_at":"2017-08-23T12:55:53Z","title":"The Viability of Phantom Dark Energy: A Brief Review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.06981","snapshot_observed_at":"2026-08-15T17:14:14.191795Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.191795Z"},"links":{"cited_paper":"/paper/1708.06981","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:87f297229bb9795cebb3b816b5d332e22ae12bfca1c515061bfbd84b3a195302","observation_id":"e7cb59f6-a8e5-4568-bea4-9eb510653726","resolution":{"observed_at":"2026-08-15T17:14:14.191795Z","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":"stro-ph/0606003","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:15.584278Z","title":"Calcagni and A","venue":null,"work_id":"d0a4552c-e257-426d-976e-f6fe1ad7fe70","year":2006},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.196447Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:26bac4813c5ab11b4a0df1d57b96512b1c6224e7b9f2f74e217fdc6ee1a92d69","observation_id":"ed8acd0f-4280-42fb-a0f2-4e87af351825","resolution":{"observed_at":"2026-08-15T17:14:15.593775Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.26565/2312-4334-2024-4-04","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.709802Z","title":"Basumatary and C","venue":null,"work_id":"c64723fb-e0bc-4f42-9025-f5597893c90f","year":2024},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.200950Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:ff91b70c5ddadcdc8c4996f2799f0eaf6588077f2478664874d5491c7deb922b","observation_id":"d1924084-9fae-49df-b50f-1ffb0ef4e97d","resolution":{"observed_at":"2026-08-15T17:14:14.714613Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1140/epjp/s13360-022-02957-4","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.695304Z","title":"Sobhanbabu and M","venue":null,"work_id":"d174438d-8dac-4b77-958e-0ab49c642ab0","year":2022},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.204547Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:57db8f9f3dd65b752e82edba2502e60ea1f123cfc630ead0f9b8c737fd7f2455","observation_id":"450fd6bf-e123-4c4d-915d-70cd20ea0ba4","resolution":{"observed_at":"2026-08-15T17:14:14.699998Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.208678Z","title":"Hinshaw et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.208678Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:31fd9ea6253ec64ad9191866b3f7a949fd0d590671f58d87f32446ba63626b85","observation_id":"018731bd-63aa-4d27-bbdf-d016e60eefb0","resolution":{"observed_at":"2026-08-15T17:14:14.208678Z","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":"ep-th/0307288","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:15.506813Z","title":"Nojiri and S","venue":null,"work_id":"ba4a6574-849d-4d01-b853-67923212862a","year":2003},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.212926Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:fd3ea113cd06263abc98faf035d36eccc692d341816667c49cc089a8c5618f6a","observation_id":"865e03ea-6158-4464-9fc3-ad32f0be07ad","resolution":{"observed_at":"2026-08-15T17:14:15.514216Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.216673Z","title":"Nojiri, S","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.216673Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:045e1eaa017e6db4806ae5567140ad639e598466813b21895653ce56fa57ac46","observation_id":"acfa4899-5e8b-4cb0-a7d6-7b26bc3c9cda","resolution":{"observed_at":"2026-08-15T17:14:14.216673Z","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":"2026-08-15T17:14:14.220355Z","title":"de Rham, G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.220355Z"},"links":{"cited_paper":"/paper/1011.1232","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:996566dce079dfca523362fda538b738a70dacb70dadb31805b22f190d5eff03","observation_id":"7bd0d8d9-868e-4e15-abbb-16f7605d0ac9","resolution":{"observed_at":"2026-08-15T17:14:14.220355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.3470","last_updated":"2011-05-17T19:56:59Z","snapshot_observed_at":"2026-08-15T04:46:34.027705Z","submitted_at":"2011-05-17T19:56:59Z","title":"The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.3470","snapshot_observed_at":"2026-08-15T17:14:14.224068Z","title":"Suzuki et al","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.224068Z"},"links":{"cited_paper":"/paper/1105.3470","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:3c0ea4efbc41a1ccb1258f869549ea534c5404716b8c0a5a679c2d3a42764324","observation_id":"fbed3a6e-f038-4ad7-811e-851cc8906669","resolution":{"observed_at":"2026-08-15T17:14:14.224068Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.13793","last_updated":"2023-02-21T10:54:43Z","snapshot_observed_at":"2026-08-13T18:57:11.013994Z","submitted_at":"2021-06-25T17:45:41Z","title":"Teleparallel Gravity: From Theory to Cosmology","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.13793","snapshot_observed_at":"2026-08-15T17:14:14.228956Z","title":"Bahamonde, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.228956Z"},"links":{"cited_paper":"/paper/2106.13793","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:5eede2f28dfafd1039429934f584f9b2b7eee1190a2b929c2851de24f5127f45","observation_id":"63d516ee-6f40-48eb-a3b7-579cfa615dac","resolution":{"observed_at":"2026-08-15T17:14:14.228956Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.07586","last_updated":"2016-09-08T17:34:46Z","snapshot_observed_at":"2026-08-15T23:14:20.744854Z","submitted_at":"2015-11-24T06:36:47Z","title":"f(T) teleparallel gravity and cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.07586","snapshot_observed_at":"2026-08-15T17:14:14.233031Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.233031Z"},"links":{"cited_paper":"/paper/1511.07586","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:5c4f616238f497ac06f863d0de67daeb8e3fcae6bc97fd1c82f0b4f61091c7c3","observation_id":"f936ebbd-b683-45ee-805d-42774b31d6ce","resolution":{"observed_at":"2026-08-15T17:14:14.233031Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-15T17:14:14.238738Z","title":"Aldrovandi and J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.238738Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:424a809f9eca423abe35df54f9100a0bfc953bf6b194eb5aa4a56e8cfe0b5128","observation_id":"f0e79383-b058-4085-b384-b26cb5c46f5d","resolution":{"observed_at":"2026-08-15T17:14:14.238738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02832","last_updated":"2015-06-18T07:00:28Z","snapshot_observed_at":"2026-08-14T22:57:01.282022Z","submitted_at":"2015-03-10T09:45:29Z","title":"Transition redshift in $f(T)$ cosmology and observational constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.02832","snapshot_observed_at":"2026-08-15T17:14:14.242772Z","title":"Capozziello, O","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.242772Z"},"links":{"cited_paper":"/paper/1503.02832","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:3490815d240938ac5560946e0dd22a9551529f032f7982bbfcb238e8529d716b","observation_id":"d5fd5d9d-58ea-4060-97a6-88bcf8096185","resolution":{"observed_at":"2026-08-15T17:14:14.242772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3390/e14091627","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.662515Z","title":"Myrzakulov, Entropy 14 (2012), 1627-1651 doi:10.3390/e14091627 [arXiv:1212.21 55 [gr-qc]]","venue":null,"work_id":"5749191b-f368-4697-9c08-480e3cf23c00","year":2012},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.247374Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:8d61476038e5198dbf2fc8be2fffb1d1b5b5aaddae04e1d792bbc55dd1eb98c5","observation_id":"9d79803c-9d8d-4b8a-b19c-d28a0e008ff1","resolution":{"observed_at":"2026-08-15T17:14:14.666337Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.cjph.2022.12.005","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.649725Z","title":"Kucukakca, A","venue":null,"work_id":"64120a42-c9e4-4f89-9e55-13a8f376a05a","year":2023},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.251293Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:8272399b3781ee877c4e72a542e403d1d41a749afc8932349d8f0b30d12ddb3a","observation_id":"aec7aa14-2bef-4fb7-9348-5302684b710c","resolution":{"observed_at":"2026-08-15T17:14:14.653639Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1142/s0219887824502852","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.633715Z","title":"Amiri, A","venue":null,"work_id":"04cb12e7-ee9a-4e11-a873-e7a548f851ba","year":2025},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.255353Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:f11234a31978c300ef2a0c7197d7b739cf682e9d203564dd6d67322296b98926","observation_id":"adfce618-5e9c-4b5b-9059-584db63f051e","resolution":{"observed_at":"2026-08-15T17:14:14.639048Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1140/epjc/s10052-024-12874-8","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.619547Z","title":"Kucukakca, A","venue":null,"work_id":"e16ed84b-d734-4e78-a1aa-5fb8bb422933","year":2024},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.259409Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:49e6030070ffabb4edf49dc4ac2173b30f7d13d0a31382bf7e326a369d23b2e4","observation_id":"3ee2a25a-faad-484d-8718-5b58e88a03d9","resolution":{"observed_at":"2026-08-15T17:14:14.623581Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04828","last_updated":"2025-02-07T11:02:36Z","snapshot_observed_at":"2026-08-12T17:46:21.570179Z","submitted_at":"2025-02-07T11:02:36Z","title":"Observational constraints on vector-like dark energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04828","snapshot_observed_at":"2026-08-15T17:14:14.263350Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.263350Z"},"links":{"cited_paper":"/paper/2502.04828","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:7bccb38395b61d2f5b204b4d5f16dfbc796787936303b0d36fb8438bb721a079","observation_id":"1d550590-c2bd-4873-b83d-0b468365a23d","resolution":{"observed_at":"2026-08-15T17:14:14.263350Z","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":"stro-ph/0405267","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:15.253652Z","title":"Armendariz-Picon, JCAP 07 (2004), 007 doi:10.1088/1475-7516/2004/07/007 [arXiv:a stro-ph/0405267 [astro-ph]]","venue":null,"work_id":"a2802172-6fe2-4ebc-8e4f-a256bcec2c47","year":2004},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.268067Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:050a0f0e5cf0014f1107da4e029303ca629212810d221a7ca52d47e9e3600610","observation_id":"56e040b8-edd7-4e3b-bad5-64b4530caab2","resolution":{"observed_at":"2026-08-15T17:14:15.261026Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2019/12/032","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.606179Z","title":"Nakamura, R","venue":null,"work_id":"aa328080-552f-47a7-99dc-f942aa66782f","year":2019},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.272093Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:179b855ac06228569c1255553b1184b1ab3ffc1f1232896d611c8e9b67c71835","observation_id":"761eb7cb-7e36-4a46-b61e-ce71d1eacac8","resolution":{"observed_at":"2026-08-15T17:14:14.610219Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0908.2362","last_updated":"2009-11-07T15:12:17Z","snapshot_observed_at":"2026-08-15T05:41:27.385350Z","submitted_at":"2009-08-15T21:16:51Z","title":"Noether symmetry approach in phantom quintessence cosmology","version":2},"cited_work":{"arxiv_id":"0908.2362","doi":null,"metadata_source":"pith","pith_arxiv_id":"0908.2362","snapshot_observed_at":"2026-08-15T17:14:15.167060Z","title":"Noether symmetry approach in phantom quintessence cosmology","venue":"astro-ph.CO","work_id":"ff7b2108-84d5-4ed7-8a1f-24085a7c761a","year":2009},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.276666Z"},"links":{"cited_paper":"/paper/0908.2362","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:d455475c7bcc28ce6844ae339be807bf5bd495cdb0e28521f1443bcbdcfc30fc","observation_id":"f231dc9d-59ac-4dec-8121-bca93dc42230","resolution":{"observed_at":"2026-08-15T17:14:15.173695Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.76.084023","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.593074Z","title":"Camci and Y","venue":null,"work_id":"964f0031-f183-44c5-97a3-c4e88e509e52","year":2007},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.281822Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:baf9cd1766ee4516afc3b606eed52aa241f56b003910436ad9f6b8ab3aebf63e","observation_id":"5ed578ab-d40c-4436-8813-49aa08a090d9","resolution":{"observed_at":"2026-08-15T17:14:14.597153Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.6410","last_updated":"2012-04-28T14:23:43Z","snapshot_observed_at":"2026-08-15T04:11:39.469411Z","submitted_at":"2012-04-28T14:23:43Z","title":"LRS Bianchi type I universes exhibiting Noether symmetry in the scalar-tensor Brans-Dicke theory","version":1},"cited_work":{"arxiv_id":"1204.6410","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.6410","snapshot_observed_at":"2026-08-15T17:14:15.146550Z","title":"LRS Bianchi type I universes exhibiting Noether symmetry in the scalar-tensor Brans-Dicke theory","venue":"gr-qc","work_id":"38a4121c-4e60-427f-a792-8b433392bac5","year":2012},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.286084Z"},"links":{"cited_paper":"/paper/1204.6410","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:7a6831d45438b152d3a223293b0b7df97c86fc14b3d1c99997dd0f86480e9df1","observation_id":"77eb821a-e648-4f0d-a0c6-b29791805d6e","resolution":{"observed_at":"2026-08-15T17:14:15.151725Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.291236Z","title":"Paliathanasis, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.291236Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:9c01d3ac4d62f3c1d93dd97747238b49e50d30446bed82986a37bd69f8eb4bbf","observation_id":"b725b0a4-b906-46da-9070-3637f9cc88ef","resolution":{"observed_at":"2026-08-15T17:14:14.291236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:15.981673Z","title":"Noether symmetries of Einstein-aether scalar field cosmology,","venue":null,"work_id":"c2160ea3-bac3-41bd-ad83-9063bd5dc90e","year":2020},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.295727Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:d93b69a2d44d1c953c34b2d87cb65742317e1a802c3f774dada60d4c6300df9c","observation_id":"8e433452-e0b6-4ac3-8281-19a36d9f4a48","resolution":{"observed_at":"2026-08-15T17:14:15.988693Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1140/epjc/s10052-023-11875-3","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.579999Z","title":null,"venue":null,"work_id":"0073423a-0ce7-4cf2-b1ab-0bb75f3057c8","year":2023},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.299483Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:cfd87b1d8d422888ee92ae7a2024041f783fa17a4af622a5975134568ddcc00f","observation_id":"513d6847-0373-42f3-9c05-21dac2888286","resolution":{"observed_at":"2026-08-15T17:14:14.583931Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1139/cjp-2017-0765","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.564008Z","title":null,"venue":null,"work_id":"1abd6352-5e0e-4418-9289-60e61982c418","year":2018},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.303170Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:76f27b469d8ca685e2376cfcb5ae6a46a9e589bf1eb7c5189532101962aff0d6","observation_id":"e9ba97b1-8a0c-4689-9aa6-9a0329bb058c","resolution":{"observed_at":"2026-08-15T17:14:14.568771Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1142/s0219887820501790","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.550505Z","title":"Kucukakca, Int","venue":null,"work_id":"658f48c3-4a4e-4887-9598-daed3db2668f","year":2020},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.307200Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:3ef31d063ea0ed85869c4f3525ae077ecc526d13203736017e514784c72da51d","observation_id":"063a9903-8bf1-4881-bc49-5ac1ec5323b8","resolution":{"observed_at":"2026-08-15T17:14:14.554484Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1407.1188","last_updated":"2014-09-17T07:23:35Z","snapshot_observed_at":"2026-08-14T23:27:56.853715Z","submitted_at":"2014-07-04T10:54:37Z","title":"Teleparallel dark energy model with a fermionic field via Noether symmetry","version":2},"cited_work":{"arxiv_id":"1407.1188","doi":null,"metadata_source":"pith","pith_arxiv_id":"1407.1188","snapshot_observed_at":"2026-08-15T17:14:15.053972Z","title":"Teleparallel dark energy model with a fermionic field via Noether symmetry","venue":"gr-qc","work_id":"11ad054b-e552-4e0b-8074-4f9acaee9b1f","year":2014},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.311263Z"},"links":{"cited_paper":"/paper/1407.1188","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:8161eb9a6981406d5b6b359f7412f5a800efb10db9c550826af19adb7276a31a","observation_id":"8416a2cd-4026-463f-968d-e798a1e084a9","resolution":{"observed_at":"2026-08-15T17:14:15.058378Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.5283","last_updated":"2015-02-17T13:29:07Z","snapshot_observed_at":"2026-08-14T23:15:02.952725Z","submitted_at":"2014-10-20T14:06:32Z","title":"Noether gauge symmetry of Dirac field in $2+1$ dimensional gravity","version":2},"cited_work":{"arxiv_id":"1410.5283","doi":null,"metadata_source":"pith","pith_arxiv_id":"1410.5283","snapshot_observed_at":"2026-08-15T17:14:15.032047Z","title":"Noether gauge symmetry of Dirac field in $2+1$ dimensional gravity","venue":"gr-qc","work_id":"d3228ba7-52ce-455b-aea1-8e90cc3080a9","year":2014},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.315904Z"},"links":{"cited_paper":"/paper/1410.5283","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:b296ca2367e947a2197abb2e67ea568f1ec9c186977ccaadb4322169e632064d","observation_id":"85b78f87-0d8c-4b32-aef9-f0ba7771afd4","resolution":{"observed_at":"2026-08-15T17:14:15.037276Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1134/s1063776116070207","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.536033Z","title":"Motavalli, A","venue":null,"work_id":"1b9d0c6b-5129-4bdb-86c5-25f7cb1e45a8","year":2016},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.320099Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:2536e159550ecefdab09a4a69065ede86b5ccff4dc5723418ca9c4fecc762cee","observation_id":"ee9219e2-a3e9-4218-894f-74c17292fdb7","resolution":{"observed_at":"2026-08-15T17:14:14.540713Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1142/s0219887823501062","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.519439Z","title":null,"venue":null,"work_id":"ce70d512-7cd7-4c80-b6ef-2e3fee602fba","year":2023},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.324335Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:2a5d385efaa01115d8bd083d430dc992dfea7ff086c6de4b489368b4cf4df836","observation_id":"841665a4-9dcb-43d8-a043-d76d3c87fb2f","resolution":{"observed_at":"2026-08-15T17:14:14.524727Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2008/08/016","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.501496Z","title":"Capozziello and A","venue":null,"work_id":"de94d30a-626a-45c2-8938-351c7d25676a","year":2008},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.329851Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:95d4834a74ff421aef29bf49190303ec045160376ada014d12f6ae098d37ee6a","observation_id":"08a71f01-52d0-49ed-b97c-8d7dc4602f62","resolution":{"observed_at":"2026-08-15T17:14:14.507157Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s10509-011-0921-5","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.486727Z","title":"Kucuakca and U","venue":null,"work_id":"f331e73c-efe7-45b3-9924-178f63ec27d4","year":2012},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.334276Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:9e7d9ffbccda9b8cc7cbac84e42ed6fe5ab05bf5ee4a2798288f776294a5ece4","observation_id":"da7ea4d7-973b-45e3-b98d-0fc05dc7fa9a","resolution":{"observed_at":"2026-08-15T17:14:14.490936Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s10509-016-2667-6","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.472608Z","title":"Kucukakca, Astrophys","venue":null,"work_id":"1ee5a632-7a53-4fac-8e20-327f3c6765ca","year":2016},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.339112Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:939494bf3e3d5d1148ef3b7e91e3b9de79af16f92411ad20443a89a5abbc3f69","observation_id":"fc7084ea-be6e-4346-8a9d-4190449dbac9","resolution":{"observed_at":"2026-08-15T17:14:14.477145Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1112.2270","last_updated":"2012-01-08T12:24:00Z","snapshot_observed_at":"2026-08-15T04:26:14.352109Z","submitted_at":"2011-12-10T12:00:00Z","title":"Noether Symmetry in $f(T)$ Theory","version":3},"cited_work":{"arxiv_id":"1112.2270","doi":null,"metadata_source":"pith","pith_arxiv_id":"1112.2270","snapshot_observed_at":"2026-08-15T17:14:15.009800Z","title":"Noether Symmetry in $f(T)$ Theory","venue":"gr-qc","work_id":"c82ef3ee-235b-411f-a5e1-b2d05d1e056d","year":2011},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.343413Z"},"links":{"cited_paper":"/paper/1112.2270","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:22522d711d531cd5c3fffd9b124a3a593482bb6c34dced56ca6b8c8e2c6ec6c7","observation_id":"b2fffe60-b8ea-4030-9ed6-857a7ba6757d","resolution":{"observed_at":"2026-08-15T17:14:15.014507Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1112.2824","last_updated":"2012-05-10T10:32:40Z","snapshot_observed_at":"2026-08-15T04:25:47.980589Z","submitted_at":"2011-12-13T09:03:01Z","title":"$f(T)$ cosmology via Noether symmetry","version":3},"cited_work":{"arxiv_id":"1112.2824","doi":null,"metadata_source":"pith","pith_arxiv_id":"1112.2824","snapshot_observed_at":"2026-08-15T17:14:14.988331Z","title":"$f(T)$ cosmology via Noether symmetry","venue":"physics.gen-ph","work_id":"0b095da2-d679-4af7-896e-b40637b8303f","year":2011},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.348387Z"},"links":{"cited_paper":"/paper/1112.2824","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:fb975ebd4b69f8ebe16207e28e728954f7c33cb8c6aaa2dbcaac2fce3570fc88","observation_id":"3003a1e0-7a6f-4817-8425-d06d60405253","resolution":{"observed_at":"2026-08-15T17:14:14.993607Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01620","last_updated":"2017-03-27T07:24:52Z","snapshot_observed_at":"2026-08-14T21:22:18.464342Z","submitted_at":"2017-01-06T12:41:40Z","title":"Studying the Intervention of an Unusual Term in $f(T)$ Gravity via Noether Symmetry","version":2},"cited_work":{"arxiv_id":"1701.01620","doi":null,"metadata_source":"pith","pith_arxiv_id":"1701.01620","snapshot_observed_at":"2026-08-15T17:14:14.968507Z","title":"Studying the Intervention of an Unusual Term in $f(T)$ Gravity via Noether Symmetry","venue":"gr-qc","work_id":"97b04029-d031-439d-904f-b00659c50385","year":2017},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.353140Z"},"links":{"cited_paper":"/paper/1701.01620","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:0ca406019b3985671cadd0eef461a825ab1865c38326390fceaba08cff76d749","observation_id":"36f5f797-05fb-4d47-8eef-2decd7024e83","resolution":{"observed_at":"2026-08-15T17:14:14.973239Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.7315","last_updated":"2014-04-29T11:30:46Z","snapshot_observed_at":"2026-08-14T23:35:55.178459Z","submitted_at":"2014-04-29T11:30:46Z","title":"Scalar Tensor Teleparallel Dark Gravity via Noether Symmetry","version":1},"cited_work":{"arxiv_id":"1404.7315","doi":null,"metadata_source":"pith","pith_arxiv_id":"1404.7315","snapshot_observed_at":"2026-08-15T17:14:14.949254Z","title":"Scalar Tensor Teleparallel Dark Gravity via Noether Symmetry","venue":"gr-qc","work_id":"3dd4b2b6-2dec-4a33-be56-993a69751726","year":2014},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.358033Z"},"links":{"cited_paper":"/paper/1404.7315","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:7b45b0314456fe14e12f8a5d7a9cb204e603e88b704134b860413fabffa14c44","observation_id":"1f1cde9d-532a-4fe3-8760-7b74d2d9a237","resolution":{"observed_at":"2026-08-15T17:14:14.953524Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1708.07430","last_updated":"2017-08-24T14:13:24Z","snapshot_observed_at":"2026-08-14T20:39:18.713456Z","submitted_at":"2017-08-24T14:13:24Z","title":"Scalar-Tensor Teleparallel Gravity With Boundary Term by Noether Symmetries","version":1},"cited_work":{"arxiv_id":"1708.07430","doi":null,"metadata_source":"pith","pith_arxiv_id":"1708.07430","snapshot_observed_at":"2026-08-15T17:14:14.929056Z","title":"Scalar-Tensor Teleparallel Gravity With Boundary Term by Noether Symmetries","venue":"gr-qc","work_id":"26a40ba3-903e-4ce9-acde-54aedd12521a","year":2017},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.363108Z"},"links":{"cited_paper":"/paper/1708.07430","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:6155a177f70c79e2093650a60a84b61c97d4e07f2d142af0ca9440e8b6d9b8ae","observation_id":"866d1edf-8424-4aab-ba78-3da06572dca4","resolution":{"observed_at":"2026-08-15T17:14:14.933776Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1612.01299","last_updated":"2016-12-05T10:29:43Z","snapshot_observed_at":"2026-08-14T21:27:08.726851Z","submitted_at":"2016-12-05T10:29:43Z","title":"Noether Symmetry Approach in $f(T,B)$ teleparallel cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.01299","snapshot_observed_at":"2026-08-15T17:14:14.368046Z","title":"Bahamonde and S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.368046Z"},"links":{"cited_paper":"/paper/1612.01299","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:a38f16b43da4d7894c5c3945298654ed59beabc723a759ab96b03a34161d176d","observation_id":"801f226a-d80f-4bc1-a27e-40e28df2e6b7","resolution":{"observed_at":"2026-08-15T17:14:14.368046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:15.963302Z","title":"Kucukakca, Turk","venue":null,"work_id":"f3677e5d-fd2a-4529-bfa9-684fb4ea5e14","year":2018},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.373364Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:0840cf7599ab6776db6bf5011f7641dea18ae3d006af42bcc738db90ce139ccb","observation_id":"673bcad2-a0a8-4211-bdf6-7ea749e19a57","resolution":{"observed_at":"2026-08-15T17:14:15.968847Z","resolver_source":"raw_fallback","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.08575","last_updated":"2022-07-18T12:58:40Z","snapshot_observed_at":"2026-08-13T15:02:15.848510Z","submitted_at":"2022-07-18T12:58:40Z","title":"Anisotropic spacetimes in $f(T,B)$ theory IV: Noether symmetry analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.08575","snapshot_observed_at":"2026-08-15T17:14:14.377743Z","title":"Paliathanasis, Eur","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.377743Z"},"links":{"cited_paper":"/paper/2207.08575","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:37f7ea90a368c408a9a8808ef647341662f77b7d0ce943cd44f1cdc9a5464f83","observation_id":"5b5b7f24-8b48-4d3b-b00e-fa2e5b7d838c","resolution":{"observed_at":"2026-08-15T17:14:14.377743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.11944","last_updated":"2023-07-18T05:17:20Z","snapshot_observed_at":"2026-08-13T14:02:08.659117Z","submitted_at":"2022-10-19T09:54:41Z","title":"Noether Symmetry Approach in Scalar-Torsion $f(T,\\phi)$ Gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.11944","snapshot_observed_at":"2026-08-15T17:14:14.382998Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.382998Z"},"links":{"cited_paper":"/paper/2210.11944","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:ab3bb0994fa6bfa9a219e068e27d4ea6e3f714b076ed713dc85141fb856a8880","observation_id":"69b926d7-7e9d-4036-8434-39cc60af297c","resolution":{"observed_at":"2026-08-15T17:14:14.382998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/bf02742992","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.458096Z","title":"Capozziello, R","venue":null,"work_id":"b0f3d79b-7f11-43e5-8029-c1668ac97aa2","year":1996},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.387163Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:bca7c1330b15286678af1ae902e066bd47a653be433e6c4f54de07429f72c21a","observation_id":"828fd44e-0faf-416b-8a4f-e894945a9c97","resolution":{"observed_at":"2026-08-15T17:14:14.462364Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410445","last_updated":"2004-10-19T16:31:47Z","snapshot_observed_at":"2026-07-07T00:45:26.190743Z","submitted_at":"2004-10-19T16:31:47Z","title":"Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational data","version":1},"cited_work":{"arxiv_id":"astro-ph/0410445","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0410445","snapshot_observed_at":"2026-08-15T17:14:14.854295Z","title":"Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational data","venue":"astro-ph","work_id":"b681dc32-0652-49b0-811b-d7cb3e21eeb5","year":2004},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.392296Z"},"links":{"cited_paper":"/paper/astro-ph/0410445","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:9d259a9e506f3e5f9f61910d5806fdabfd367994f037109d5c9445d71c874136","observation_id":"d512543e-cf58-4498-a8f8-10e1a5ba1c1d","resolution":{"observed_at":"2026-08-15T17:14:14.860997Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.69.103510","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T17:14:14.441957Z","title":"Rubano, P","venue":null,"work_id":"faeef8ec-7a7f-4cfd-bdea-c117eb3d0634","year":2004},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.397007Z"},"links":{"citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:748f6c6b5dbaaa60f80605adc3f1e6e74210f0c42ee20575d6068dc13da76321","observation_id":"b70a56c7-ac49-4273-8a63-08eb0aba6810","resolution":{"observed_at":"2026-08-15T17:14:14.447364Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-08-15T17:14:14.401683Z","title":"Abdul Karim et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.401683Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:480e91cac79c17fb505def46223622608dc010ad94a343ca19e5182dfc8106d0","observation_id":"79460a2b-1e82-4ee4-ae94-33c87b0b8c9d","resolution":{"observed_at":"2026-08-15T17:14:14.401683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.10704","last_updated":"2025-01-08T06:34:27Z","snapshot_observed_at":"2026-08-15T23:48:46.518660Z","submitted_at":"2024-08-20T09:59:06Z","title":"$\\Lambda$CDM model against cosmography: A possible deviation after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.10704","snapshot_observed_at":"2026-08-15T17:14:14.408010Z","title":"Pourojaghi, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-15T17:14:14.408010Z"},"links":{"cited_paper":"/paper/2408.10704","citing_paper":"/paper/2508.17795"},"observation_digest":"sha256:35fd1d86b31653fc79670a6fb63a5b1ce311115a9cb0d3189fa524af2efa0d97","observation_id":"561719ee-248b-4d56-9bfe-8ca0349db6a0","resolution":{"observed_at":"2026-08-15T17:14:14.408010Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2508.17795","last_updated":"2025-08-25T08:41:32Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-15T23:14:56.112014Z","submitted_at":"2025-08-25T08:41:32Z","title":"Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry"},"reference_resolution":{"displayed":69,"state_counts":{"malformed_identifier":3,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":32,"verified_exact":32,"verified_fuzzy":1},"total_outbound_references":69},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 69 of 69 outbound references and 0 inbound Pith citation observations for arXiv:2508.17795."}