{"as_of":"2026-08-12T18:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3196ecfb7f26625cc4b4b3a23812a0755a833d35c5cf32317b5269599c08a426","coverage":[{"denominator":54,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":54,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T22:44:47.910498Z","state":"measured"},{"denominator":54,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":54,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+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/2412.03219/citation-record","integrity":"/paper/2412.03219/integrity","json":"/paper/2412.03219/citation-record.json","paper":"/paper/2412.03219"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0509059","last_updated":"2005-11-23T15:31:30Z","snapshot_observed_at":"2026-08-03T14:27:42.408450Z","submitted_at":"2005-09-15T09:28:40Z","title":"The Power of General Relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0509059","snapshot_observed_at":"2026-08-11T22:44:45.380520Z","title":"Clifton and J.D","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.380520Z"},"links":{"cited_paper":"/paper/gr-qc/0509059","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:89b11386184671a68d21f32e83adf89d0919436f0441346b0811ddb1c4714209","observation_id":"505ea463-86ad-4506-bdce-365b1b3ead8b","resolution":{"observed_at":"2026-08-11T22:44:45.380520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0601213","last_updated":"2006-03-31T03:39:12Z","snapshot_observed_at":"2026-07-07T04:56:30.478178Z","submitted_at":"2006-01-29T22:31:37Z","title":"Introduction to Modified Gravity and Gravitational Alternative for Dark Energy","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0601213","snapshot_observed_at":"2026-08-11T22:44:45.424869Z","title":"Nojiri and S.D","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.424869Z"},"links":{"cited_paper":"/paper/hep-th/0601213","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:034fb8bd13eff3facbc0c4023502a5be3602174bd2bb2009283012931fa27172","observation_id":"fb4afd0f-8b49-488b-8d1d-eed7a30e7a6f","resolution":{"observed_at":"2026-08-11T22:44:45.424869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.0544","last_updated":"2011-05-29T07:12:32Z","snapshot_observed_at":"2026-07-31T03:11:20.673469Z","submitted_at":"2010-11-02T09:09:34Z","title":"Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.0544","snapshot_observed_at":"2026-08-11T22:44:45.464745Z","title":"Nojiri and S.D","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.464745Z"},"links":{"cited_paper":"/paper/1011.0544","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:857b1d12f7757f0007964ad915185f8a1de639c2304f2c63e375cd0cf3b1a941","observation_id":"92ecd01e-576c-49cc-95e2-395a74415ca6","resolution":{"observed_at":"2026-08-11T22:44:45.464745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1705.11098","last_updated":"2021-05-23T13:57:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2017-05-31T13:41:52Z","title":"Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1705.11098","snapshot_observed_at":"2026-08-11T22:44:45.508096Z","title":"Nojiri, S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.508096Z"},"links":{"cited_paper":"/paper/1705.11098","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:a548885e043c53cf237335032457dea85f8b626fad6975370e22961d0903d661","observation_id":"4c305cf5-4394-468c-a0c0-c99f56223f84","resolution":{"observed_at":"2026-08-11T22:44:45.508096Z","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":"2026-08-11T22:44:57.894511Z","title":"Starobinsky,A New Type of Isotropic Cosmological Models Without Singularity,Phys","venue":null,"work_id":"77dfbaf8-aba8-4b84-ae5b-845e18e40ef4","year":1980},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.525434Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:ff0c9d7c4b14836b042992246e630d08e1647c03de2d50c2f92d67418fdd941f","observation_id":"02fc99d3-dd53-4641-9e9d-ecc1abedf6c1","resolution":{"observed_at":"2026-08-11T22:44:57.944756Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-11T22:44:45.537763Z","title":"Kibble,Lorentz invarianceand the gravitational field, Journal of Mathematical Physics 2 (1961) 212 [https://doi.org/10.1063/1.1703702]","venue":null,"work_id":null,"year":1961},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.537763Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:60fd466b679e7fb87cb66fdf3040f6431821ff0663862a460a6d68805a3edcef","observation_id":"b77ab76e-d0eb-4e55-81ac-8e7d9e85e83e","resolution":{"observed_at":"2026-08-11T22:44:45.537763Z","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":"2026-08-11T22:44:57.704741Z","title":"SCIAMA,The physical structure of general relativity, Rev","venue":null,"work_id":"fbd34b81-c29c-4d36-85f0-be9fc75e9db5","year":1964},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.584897Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:f4bc9eff7422dcc8519107c78ec7e627029ce2a2de9af72adfe2d3857683716b","observation_id":"67fb662b-9bc6-40fc-b9c1-0cd094623aba","resolution":{"observed_at":"2026-08-11T22:44:57.760052Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1005.0893","last_updated":"2011-07-04T15:13:23Z","snapshot_observed_at":"2026-07-06T02:09:59.233701Z","submitted_at":"2010-05-06T06:25:14Z","title":"Cosmological constant from quarks and torsion","version":3},"cited_work":{"arxiv_id":"1005.0893","doi":null,"metadata_source":"pith","pith_arxiv_id":"1005.0893","snapshot_observed_at":"2026-08-11T22:44:55.594019Z","title":"Cosmological constant from quarks and torsion","venue":"gr-qc","work_id":"dd07d920-90c4-4104-8813-e46d990495b1","year":2010},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.630032Z"},"links":{"cited_paper":"/paper/1005.0893","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:ac8ad6e28a0146810e3e6c05302bc1ec2bab3a8456cce2540b94a8199b96be18","observation_id":"4917ba91-882e-4fc8-a5e0-eee86ffa5fda","resolution":{"observed_at":"2026-08-11T22:44:55.634751Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1212.0585","last_updated":"2013-05-03T20:20:19Z","snapshot_observed_at":"2026-07-06T03:01:13.244187Z","submitted_at":"2012-12-03T23:22:50Z","title":"Cosmology with a spin","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.0585","snapshot_observed_at":"2026-08-11T22:44:45.674848Z","title":"Magueijo, T.G","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.674848Z"},"links":{"cited_paper":"/paper/1212.0585","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:381c0314370e1f280c33c26d13a6fced76d5ebddec16fdc2557ad1f611f98601","observation_id":"b9d598bb-7b47-4695-a8e5-f08ba30f30ca","resolution":{"observed_at":"2026-08-11T22:44:45.674848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.1726","last_updated":"2010-06-04T00:50:27Z","snapshot_observed_at":"2026-08-12T13:39:46.870447Z","submitted_at":"2008-05-12T19:44:15Z","title":"f(R) Theories Of Gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.1726","snapshot_observed_at":"2026-08-11T22:44:45.734757Z","title":"Sotiriou and V","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.734757Z"},"links":{"cited_paper":"/paper/0805.1726","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:c81d3d650094cb81fa5be16fc8c2e57e25c3ceed9a7122465311568dd9fff7d5","observation_id":"fbf82321-5716-40f0-aa26-7182d625dce8","resolution":{"observed_at":"2026-08-11T22:44:45.734757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.1978","last_updated":"2013-12-10T21:03:44Z","snapshot_observed_at":"2026-07-06T03:22:28.603258Z","submitted_at":"2013-09-08T17:04:01Z","title":"Further stable neutron star models from f(R) gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.1978","snapshot_observed_at":"2026-08-11T22:44:45.794752Z","title":"Astashenok, S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.794752Z"},"links":{"cited_paper":"/paper/1309.1978","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:949db080960877492d5fd6fca22be9f1e6fbcee47eb899bb8e88aa3798b5c29b","observation_id":"4332e832-9a41-4881-ad9c-f45b38ad38ab","resolution":{"observed_at":"2026-08-11T22:44:45.794752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3856","last_updated":"2014-11-24T08:54:07Z","snapshot_observed_at":"2026-08-05T20:07:16.503615Z","submitted_at":"2014-08-17T20:19:08Z","title":"Extreme neutron stars from Extended Theories of Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.3856","snapshot_observed_at":"2026-08-11T22:44:45.845363Z","title":"Astashenok, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.845363Z"},"links":{"cited_paper":"/paper/1408.3856","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:07e985b958c13e57b05e3445e3d2ec18485c1f3167c76cd668cf85242acf9d6f","observation_id":"1d3da405-7744-4cf5-9e50-986f6329af49","resolution":{"observed_at":"2026-08-11T22:44:45.845363Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.08311","last_updated":"2017-09-27T07:52:44Z","snapshot_observed_at":"2026-07-06T05:39:29.289611Z","submitted_at":"2017-04-26T19:22:16Z","title":"The realistic models of relativistic stars in f(R) = R + alpha R^2 gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.08311","snapshot_observed_at":"2026-08-11T22:44:45.884917Z","title":"Astashenok, S.D","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.884917Z"},"links":{"cited_paper":"/paper/1704.08311","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:dc181561cad53848533dd2cc74db2372aeec0c4c045d6621b236f8c295cc0665","observation_id":"77d23181-f3a1-4839-a30e-fc26b7cc4a9b","resolution":{"observed_at":"2026-08-11T22:44:45.884917Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.08504","last_updated":"2020-01-23T13:48:59Z","snapshot_observed_at":"2026-07-06T08:52:18.015337Z","submitted_at":"2020-01-23T13:48:59Z","title":"Supermassive Neutron Stars in Axion $F(R)$ Gravity","version":1},"cited_work":{"arxiv_id":"2001.08504","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.08504","snapshot_observed_at":"2026-08-11T22:44:54.324638Z","title":"Supermassive Neutron Stars in Axion $F(R)$ Gravity","venue":"gr-qc","work_id":"e7f3d7f7-3658-48f4-a373-dd87a818f95a","year":2020},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.933933Z"},"links":{"cited_paper":"/paper/2001.08504","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:6aebc8237012aa52e26a11d85435895061b472aed5c7f55f4ce7668235fc4d50","observation_id":"5006a67c-a237-4458-a887-eaa45364fa49","resolution":{"observed_at":"2026-08-11T22:44:54.384745Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11271","last_updated":"2020-08-25T21:01:27Z","snapshot_observed_at":"2026-08-10T19:33:05.508951Z","submitted_at":"2020-08-25T21:01:27Z","title":"Rotating Neutron Stars in F(R) Gravity with Axions","version":1},"cited_work":{"arxiv_id":"2008.11271","doi":null,"metadata_source":"pith","pith_arxiv_id":"2008.11271","snapshot_observed_at":"2026-08-11T22:44:54.094771Z","title":"Rotating Neutron Stars in F(R) Gravity with Axions","venue":"gr-qc","work_id":"ed9e04d5-5b16-4e29-91b3-e3f5c2ffcd09","year":2020},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:45.974286Z"},"links":{"cited_paper":"/paper/2008.11271","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:116a8af8578d2af15e92c173356c4af3d0e0da09eae4e10fd830e249250b9674","observation_id":"5fee40d5-1d65-4fcd-9a7a-b75a75c5f6dc","resolution":{"observed_at":"2026-08-11T22:44:54.134753Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2103.04144","last_updated":"2021-03-15T15:43:40Z","snapshot_observed_at":"2026-07-06T10:47:29.160817Z","submitted_at":"2021-03-06T15:57:45Z","title":"Causal Limit of Neutron Star Maximum Mass in $f(R)$ Gravity in View of GW190814","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.04144","snapshot_observed_at":"2026-08-11T22:44:46.024817Z","title":"Astashenok, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.024817Z"},"links":{"cited_paper":"/paper/2103.04144","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:44cc72e85027e6efaa816be65aa7f5b1a9e82418dd77a51316365a68659c4910","observation_id":"46fa2641-73da-40c3-bfb9-8d7acae12f67","resolution":{"observed_at":"2026-08-11T22:44:46.024817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.01234","last_updated":"2021-06-02T15:31:02Z","snapshot_observed_at":"2026-07-06T11:15:13.839091Z","submitted_at":"2021-06-02T15:31:02Z","title":"Novel Stellar Astrophysics from Extended Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.01234","snapshot_observed_at":"2026-08-11T22:44:46.074750Z","title":"Astashenok, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.074750Z"},"links":{"cited_paper":"/paper/2106.01234","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:2b33b478abc867e47850b5e11c5605e7c744d2a0e104ed431604049fbc477e09","observation_id":"218d9889-0169-4afc-b15e-2ef54de40d44","resolution":{"observed_at":"2026-08-11T22:44:46.074750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.14179","last_updated":"2021-11-28T15:39:28Z","snapshot_observed_at":"2026-08-09T23:44:05.454818Z","submitted_at":"2021-11-28T15:39:28Z","title":"Maximum Baryon Masses for Static Neutron Stars in $f(R)$ Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.14179","snapshot_observed_at":"2026-08-11T22:44:46.124791Z","title":"Astashenok, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.124791Z"},"links":{"cited_paper":"/paper/2111.14179","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:c089732bab89ed73b318c55a1554400fb5ebb5c427645e67cf1cf372e1a070b3","observation_id":"2585e605-c8af-484d-830e-25aefe613179","resolution":{"observed_at":"2026-08-11T22:44:46.124791Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.04163","last_updated":"2015-11-30T21:35:03Z","snapshot_observed_at":"2026-07-06T04:29:49.038576Z","submitted_at":"2015-09-10T23:55:40Z","title":"The Mass-Radius relation for Neutron Stars in $f(R)$ gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.04163","snapshot_observed_at":"2026-08-11T22:44:46.175095Z","title":"Capozziello, M","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.175095Z"},"links":{"cited_paper":"/paper/1509.04163","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:7afc9d959e53b648c9b51cf884a92704729cd57c8957b04ee30047a7cc2d9d15","observation_id":"f895ad79-6da1-4d53-920c-b4a1d183569e","resolution":{"observed_at":"2026-08-11T22:44:46.175095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05515","last_updated":"2023-05-09T15:09:26Z","snapshot_observed_at":"2026-08-08T20:35:04.942745Z","submitted_at":"2023-05-09T15:09:26Z","title":"Inflationary Attractors Predictions for Static Neutron Stars in the Mass-Gap Region","version":1},"cited_work":{"arxiv_id":"2305.05515","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.05515","snapshot_observed_at":"2026-08-11T22:44:53.015280Z","title":"Inflationary Attractors Predictions for Static Neutron Stars in the Mass-Gap Region","venue":"gr-qc","work_id":"4a2de123-e004-4910-b995-f7acbad09102","year":2023},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.244845Z"},"links":{"cited_paper":"/paper/2305.05515","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:8dd7db6bcebe7efa9f47a8d71d0d44fe8180e06d490e400d0831ece5cb13842b","observation_id":"236c0624-fec9-4d69-b9f0-6ae9dbc43aba","resolution":{"observed_at":"2026-08-11T22:44:53.064897Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02660","last_updated":"2022-10-16T10:36:35Z","snapshot_observed_at":"2026-07-06T12:05:18.796351Z","submitted_at":"2021-11-04T06:57:40Z","title":"Compact Star in General $F(R)$ Gravity: Inevitable Degeneracy Problem and Non-Integer Power Correction","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.02660","snapshot_observed_at":"2026-08-11T22:44:46.294753Z","title":"Numajiri, T","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.294753Z"},"links":{"cited_paper":"/paper/2111.02660","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:d65d4ce49be9f813591f396c6697580630d135ebbeb1e04ef1e59ffeff66e4ad","observation_id":"c3d0c6a9-41c7-4018-afb7-0e8f7b470115","resolution":{"observed_at":"2026-08-11T22:44:46.294753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.12301","last_updated":"2024-11-04T07:21:15Z","snapshot_observed_at":"2026-08-09T13:16:43.425438Z","submitted_at":"2024-08-22T11:18:55Z","title":"Compact star in noninteger power model of $f(R)$ gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.12301","snapshot_observed_at":"2026-08-11T22:44:46.346601Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.346601Z"},"links":{"cited_paper":"/paper/2408.12301","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:6b4c08c6fa0978dbceefb465d8b59b8cbfd714cc972900b1614f7516c53f6d54","observation_id":"f91faa4d-5008-4b47-9dc0-62c01c5af528","resolution":{"observed_at":"2026-08-11T22:44:46.346601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-08-11T22:44:46.395251Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.395251Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:fa0773fe042a162354b00655094de5de2cad7905fc43623a5056ac02799576bd","observation_id":"dbd91b86-e141-485f-bd7b-58fd7537607b","resolution":{"observed_at":"2026-08-11T22:44:46.395251Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05705","last_updated":"2019-12-12T00:04:41Z","snapshot_observed_at":"2026-07-31T21:20:48.579404Z","submitted_at":"2019-12-12T00:04:41Z","title":"PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.05705","snapshot_observed_at":"2026-08-11T22:44:46.454846Z","title":"Miller et al., PSR J0030+0451 Mass and Radius fromN ICERData and Implications for the Properties of Neutron Star Matter, Astrophys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.454846Z"},"links":{"cited_paper":"/paper/1912.05705","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:85ccf7eba60ee9484ca6fc528ce11edfb2af3e8e54b293c73ff5b533d63cec83","observation_id":"efbe7fa7-d7a8-4d30-be60-548b6f6c7d68","resolution":{"observed_at":"2026-08-11T22:44:46.454846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.3510","last_updated":"2013-05-15T14:59:02Z","snapshot_observed_at":"2026-07-06T03:13:27.638618Z","submitted_at":"2013-05-15T14:59:02Z","title":"The Nuclear Equation of State and Neutron Star Masses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.3510","snapshot_observed_at":"2026-08-11T22:44:46.506550Z","title":"Lattimer,The nuclear equation of state and neutron star masses,Ann","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.506550Z"},"links":{"cited_paper":"/paper/1305.3510","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:f2b1cd42aa9a2b9b8df9260379324946cbbe3fa90e95eff6748e42054e66947f","observation_id":"b98bb841-625e-4c7c-9075-eb285df740a2","resolution":{"observed_at":"2026-08-11T22:44:46.506550Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.03313","last_updated":"2017-09-14T01:17:12Z","snapshot_observed_at":"2026-07-06T05:59:01.675704Z","submitted_at":"2017-09-11T09:56:33Z","title":"Gravitational Wave Polarizations in $f(R)$ Gravity and Scalar-Tensor Theory","version":2},"cited_work":{"arxiv_id":"1709.03313","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.03313","snapshot_observed_at":"2026-08-11T22:44:52.114979Z","title":"Gravitational Wave Polarizations in $f(R)$ Gravity and Scalar-Tensor Theory","venue":"gr-qc","work_id":"ac01c9f0-4bb3-44f1-8e38-a7d617250442","year":2017},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.551969Z"},"links":{"cited_paper":"/paper/1709.03313","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:8ecdeb43a07d02b8aa6bfb72888f8b2583ca00b6fe00ee75260a3562b3dfd1dc","observation_id":"706686a2-8a2c-473b-bb9a-88626ca12836","resolution":{"observed_at":"2026-08-11T22:44:52.174830Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01764","last_updated":"2016-12-21T23:19:17Z","snapshot_observed_at":"2026-07-06T05:06:04.268058Z","submitted_at":"2016-08-05T05:30:43Z","title":"Propagating degrees of freedom in f(R) gravity","version":2},"cited_work":{"arxiv_id":"1608.01764","doi":null,"metadata_source":"pith","pith_arxiv_id":"1608.01764","snapshot_observed_at":"2026-08-11T22:44:51.895302Z","title":"Propagating degrees of freedom in f(R) gravity","venue":"gr-qc","work_id":"412a794a-14b7-4725-acb0-09fa8c0743af","year":2016},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.605034Z"},"links":{"cited_paper":"/paper/1608.01764","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:4fa05ebe1a89ad20b5af509e522a63d9ac7257bc7c5b94406ee3635a2051381f","observation_id":"9054f117-c8ac-4f22-a7c0-4b1306e314b3","resolution":{"observed_at":"2026-08-11T22:44:51.934743Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.01899","last_updated":"2019-09-25T14:37:16Z","snapshot_observed_at":"2026-08-05T18:38:41.470131Z","submitted_at":"2019-06-05T09:20:13Z","title":"Gauge invariant formulation of gravitational waves in metric $f(R)$ gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.01899","snapshot_observed_at":"2026-08-11T22:44:46.655404Z","title":"Moretti, F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.655404Z"},"links":{"cited_paper":"/paper/1906.01899","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:332d1c97914c8f7ffbfa81d300fbf04cdd5617171607106195b6c00dd199cc57","observation_id":"bbb2049f-6c8e-46cc-b8f0-f93fd0ed2703","resolution":{"observed_at":"2026-08-11T22:44:46.655404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.08759","last_updated":"2020-01-23T19:00:10Z","snapshot_observed_at":"2026-07-06T08:52:26.716343Z","submitted_at":"2020-01-23T19:00:10Z","title":"The gauge symmetries of f(R) gravity with torsion in the Cartan formalism","version":1},"cited_work":{"arxiv_id":"2001.08759","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.08759","snapshot_observed_at":"2026-08-11T22:44:51.433403Z","title":"The gauge symmetries of f(R) gravity with torsion in the Cartan formalism","venue":"gr-qc","work_id":"2980073d-d670-4a71-a908-ed89fb4906e0","year":2020},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.705415Z"},"links":{"cited_paper":"/paper/2001.08759","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:1b8cfece3e8ccab914234feb486b30526adf9c6a0861076071f4dc592089ae6c","observation_id":"168f35da-1f53-4d9f-b69e-ffadd652fa77","resolution":{"observed_at":"2026-08-11T22:44:51.486704Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.01255","last_updated":"2022-09-06T00:38:05Z","snapshot_observed_at":"2026-08-11T07:12:06.724469Z","submitted_at":"2022-04-04T05:53:46Z","title":"Cartan $F(R)$ Gravity and Equivalent Scalar-Tensor Theory","version":2},"cited_work":{"arxiv_id":"2204.01255","doi":null,"metadata_source":"pith","pith_arxiv_id":"2204.01255","snapshot_observed_at":"2026-08-11T22:44:51.115266Z","title":"Cartan $F(R)$ Gravity and Equivalent Scalar-Tensor Theory","venue":"gr-qc","work_id":"71b3cb17-0242-40b5-814c-8d5ff6586c79","year":2022},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.755626Z"},"links":{"cited_paper":"/paper/2204.01255","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:9e0b7d5d42353a16578364fdb06bcb1f203ba037ff35e81252942577f4a4d158","observation_id":"db7edc1e-408d-45d9-a63c-4818cc4a48d9","resolution":{"observed_at":"2026-08-11T22:44:51.154823Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.11776","last_updated":"2023-12-19T01:10:37Z","snapshot_observed_at":"2026-08-03T16:11:00.141509Z","submitted_at":"2023-12-19T01:10:37Z","title":"Quintessential Inflation in Logarithmic Cartan $F(R)$ Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.11776","snapshot_observed_at":"2026-08-11T22:44:46.814832Z","title":"Inagaki and M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.814832Z"},"links":{"cited_paper":"/paper/2312.11776","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:1b42eeb24d6cc7765691b1d16705bf70afb84ea42369eeae513b4e0ff21a3a00","observation_id":"6776dbb2-d1d1-45fd-818e-0118244adeee","resolution":{"observed_at":"2026-08-11T22:44:46.814832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.14769","last_updated":"2023-09-22T13:54:07Z","snapshot_observed_at":"2026-07-06T15:21:08.450594Z","submitted_at":"2023-04-28T11:28:13Z","title":"Robustness of predicted CMB fluctuations in Cartan $F(R)$ gravity","version":2},"cited_work":{"arxiv_id":"2304.14769","doi":null,"metadata_source":"pith","pith_arxiv_id":"2304.14769","snapshot_observed_at":"2026-08-11T22:44:50.604753Z","title":"Robustness of predicted CMB fluctuations in Cartan $F(R)$ gravity","venue":"gr-qc","work_id":"8a8b662e-a6f8-49ff-8857-62b94bb53e70","year":2023},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.864847Z"},"links":{"cited_paper":"/paper/2304.14769","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:8d0329d20297cb3c3239486ce0cf9c8385912de9d8c95232d1a825b9baff6ac8","observation_id":"0952bcae-c962-45a3-a134-d151b47995c1","resolution":{"observed_at":"2026-08-11T22:44:50.654754Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:57.534736Z","title":null,"venue":null,"work_id":"68b07ed8-ebf2-4e21-bde5-96d351b7f5a5","year":1974},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.929960Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:440a1c67cb0df70b6dd863e961b65199e3c1a5e535e911bfece9c38bf8a6bdff","observation_id":"06b105dd-c29b-494b-9720-512cce510283","resolution":{"observed_at":"2026-08-11T22:44:57.564828Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:57.385524Z","title":"Kerlick, Cosmology and Particle Pair Production via Gravitational Spin Spin Interaction in the Einstein-Cartan-Sciama-Kibble Theory of Gravity, Phys","venue":null,"work_id":"938470ce-092b-47c4-a89a-13660e2e6fde","year":1975},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.954824Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:94a705659cc0b7989dcaae18d7334e413d1ff5fad84683369b41e9c5559aed99","observation_id":"ca20e33c-4432-4c36-86ce-26429644e2c4","resolution":{"observed_at":"2026-08-11T22:44:57.420991Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:57.328536Z","title":"Gasperini, Spin Dominated Inflation in the Einstein-cartan Theory,Phys","venue":null,"work_id":"901aafea-5f28-49a9-92cf-7cb171e0b69c","year":1986},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:46.980462Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:850063ff5e9dbcce9bf2e386c073271428b9ac029321492bb4369a10150a7dcc","observation_id":"37c52f5f-e700-4310-92eb-ca1be73374db","resolution":{"observed_at":"2026-08-11T22:44:57.342188Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:57.269086Z","title":"Hehl and B","venue":null,"work_id":"2ff77aef-e525-47c1-9aae-4a3116b36a1a","year":1971},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.044733Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:efe63205af387907a40364da7c51888a6258fe483da2da081f7a7bdfcc241a67","observation_id":"a8e26ad1-ff91-417b-aadc-0952f55f54de","resolution":{"observed_at":"2026-08-11T22:44:57.290345Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1606.09273","last_updated":"2017-02-10T21:51:09Z","snapshot_observed_at":"2026-07-06T05:01:49.181638Z","submitted_at":"2016-06-29T20:31:03Z","title":"Gravity-induced four-fermion contact interaction implies gravitational intermediate W and Z type gauge bosons","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.09273","snapshot_observed_at":"2026-08-11T22:44:47.095107Z","title":"Boos and F.W","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.095107Z"},"links":{"cited_paper":"/paper/1606.09273","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:253c0a3541f60435420b01cc6a79d77a43370fb7636ffd0d1e4c57b1ff9a1e2a","observation_id":"9ba04e54-80ee-4ef2-9902-078fb6c48209","resolution":{"observed_at":"2026-08-11T22:44:47.095107Z","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":"2026-08-11T22:44:57.200985Z","title":"Bardeen, L.N","venue":null,"work_id":"d829a407-71df-47d1-afb9-ed0f2cc73ac6","year":1957},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.154834Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:4d3a9454c184d214ef03547770da685626e4c69d2eef644f38643ffb264a0f0a","observation_id":"dcf7c754-bfed-4516-bfd5-f6cd20177b4c","resolution":{"observed_at":"2026-08-11T22:44:57.240964Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:57.134884Z","title":"Bardeen, L.N","venue":null,"work_id":"b0eb91be-3bf1-414d-88e9-4fe6fdc3a471","year":1957},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.210312Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:deb5bda88ad1311bb989f736531703265ee42fb243ea14e2e72b281a9e53ed46","observation_id":"e9241a59-5e3f-4d9a-9c7f-7302b27bdcdd","resolution":{"observed_at":"2026-08-11T22:44:57.164828Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:57.054740Z","title":"Nambu and G","venue":null,"work_id":"25c45cd4-8994-4030-8927-7fbb56bc375b","year":1961},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.254753Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:431101daa5aed406d6d370d04322802bb8fc12bd5b6e5066fee6759e4f6f55dc","observation_id":"439156cd-6aa3-4a4d-a616-09b481cb72d2","resolution":{"observed_at":"2026-08-11T22:44:57.084892Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:56.988330Z","title":"Nambu and G","venue":null,"work_id":"e03dc3e7-6d8f-4385-9cd9-7af8644fa216","year":1961},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.284762Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:03d31e38c8e8e8177451c5d870b3c0e1fcc129dd4732ddac7c052df059cb518c","observation_id":"2dafeb9c-f9b8-48d8-b547-f09c38f969d0","resolution":{"observed_at":"2026-08-11T22:44:56.998983Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:56.795264Z","title":"Weinberg,Implications of dynamical symmetry breaking: An addendum, Phys","venue":null,"work_id":"861ddce1-3e19-4f4c-875b-6bdfbc8840e0","year":1979},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.314881Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:d94dbbfd375af3d5a572b0b171a610b06d2e1c9482b6b1d0861febe2ec72f244","observation_id":"718cec48-e841-42a1-a2de-47d041548414","resolution":{"observed_at":"2026-08-11T22:44:56.854749Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-11T22:44:47.363375Z","title":"Miransky,Dynamical Symmetry Breaking in Quantum Field Theories, WORLD SCIENTIFIC (1994), 10.1142/2170, [https://www.worldscientific.com/doi/pdf/10.1142/2170]","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.363375Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:9a763a6d83a73a56a2141524c130937bb853a0468d93750859645bae03091a00","observation_id":"224660ee-110d-4443-8c3f-9dbdd45e4a4f","resolution":{"observed_at":"2026-08-11T22:44:47.363375Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T22:44:56.614728Z","title":"Harada and K","venue":null,"work_id":"ac4a30aa-8ed3-481c-aabb-418060f8a512","year":2003},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.410092Z"},"links":{"citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:f856444a0bbda47eff8b007f7f807972457e1ab002add23c141cfad5f4227fb3","observation_id":"632c80b4-1205-434f-8346-a5dae59e70fe","resolution":{"observed_at":"2026-08-11T22:44:56.664748Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9711084","last_updated":"1997-11-12T06:35:57Z","snapshot_observed_at":"2026-08-11T23:15:20.865075Z","submitted_at":"1997-11-12T06:35:57Z","title":"Dynamical symmetry breaking in curved spacetime -review-","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9711084","snapshot_observed_at":"2026-08-11T22:44:47.454756Z","title":"Inagaki, T","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.454756Z"},"links":{"cited_paper":"/paper/hep-th/9711084","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:2ae5c487dca8d31344f471c4bd7a9ce67ee2e19ec79a07532fa96547ce86d798","observation_id":"79a26343-645e-42c2-adc8-470b820be785","resolution":{"observed_at":"2026-08-11T22:44:47.454756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.08954","last_updated":"2019-10-03T08:03:16Z","snapshot_observed_at":"2026-08-08T05:03:04.714684Z","submitted_at":"2019-06-21T05:39:58Z","title":"Neutron stars in $f(R)$ gravity and scalar-tensor theories","version":3},"cited_work":{"arxiv_id":"1906.08954","doi":null,"metadata_source":"pith","pith_arxiv_id":"1906.08954","snapshot_observed_at":"2026-08-11T22:44:49.989673Z","title":"Neutron stars in $f(R)$ gravity and scalar-tensor theories","venue":"gr-qc","work_id":"eaa4a43b-25d6-4703-bcd1-80184bd2d6be","year":2019},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.506863Z"},"links":{"cited_paper":"/paper/1906.08954","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:c4f53afa4fecbedf1af7970a77705faba51e18a2f15dfff774c1ab1e73696786","observation_id":"58e4cf8d-9bcc-43ea-8c5d-f5f500e681cc","resolution":{"observed_at":"2026-08-11T22:44:50.025122Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0408324","last_updated":"2004-09-07T15:46:04Z","snapshot_observed_at":"2026-07-07T00:44:10.542942Z","submitted_at":"2004-08-18T10:49:48Z","title":"Analytical representations of unified equations of state of neutron-star matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0408324","snapshot_observed_at":"2026-08-11T22:44:47.554752Z","title":"Haensel and A.Y","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.554752Z"},"links":{"cited_paper":"/paper/astro-ph/0408324","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:90265e12259f50ba2883bbf8ea0b8476b1ea07eced7e518889911dc889d26205","observation_id":"69fd378f-6405-4a2e-b6d1-8c7188487e29","resolution":{"observed_at":"2026-08-11T22:44:47.554752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.07662","last_updated":"2018-06-12T11:55:15Z","snapshot_observed_at":"2026-07-06T06:10:30.224957Z","submitted_at":"2017-11-21T07:46:59Z","title":"Magnetic neutron star cooling and microphysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.07662","snapshot_observed_at":"2026-08-11T22:44:47.604753Z","title":"Potekhin and G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.604753Z"},"links":{"cited_paper":"/paper/1711.07662","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:1a1097a6687fa2aef640ca70fb728ac3aa6c2a18708560d9c5e647390793ef78","observation_id":"bc0c5c29-2754-447c-9916-4aebddefd23b","resolution":{"observed_at":"2026-08-11T22:44:47.604753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"nucl-th/9310003","last_updated":"1993-10-04T16:06:30Z","snapshot_observed_at":"2026-07-07T06:37:56.578830Z","submitted_at":"1993-10-04T16:06:30Z","title":"Experimental Nuclear Masses and the Ground State of Cold Dense Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"nucl-th/9310003","snapshot_observed_at":"2026-08-11T22:44:47.654853Z","title":"Haensel and B","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.654853Z"},"links":{"cited_paper":"/paper/nucl-th/9310003","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:27cdaad9035775f91cba2fa5f23eb46806cab89dcbf6a935a08d5af379e76bb9","observation_id":"6504c2b7-cc0b-42f3-88f2-b17e4f13e5e6","resolution":{"observed_at":"2026-08-11T22:44:47.654853Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.3955","last_updated":"2008-12-20T10:43:21Z","snapshot_observed_at":"2026-07-06T01:49:36.809572Z","submitted_at":"2008-12-20T10:43:21Z","title":"Physics of Neutron Star Crusts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.3955","snapshot_observed_at":"2026-08-11T22:44:47.724754Z","title":"Chamel and P","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.724754Z"},"links":{"cited_paper":"/paper/0812.3955","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:457320ef02ecaa7c95d23ac0e024542cc6ebea6de33a123df8ebb30322cbe99b","observation_id":"404a939f-0b78-49dd-b18f-a078b429ad87","resolution":{"observed_at":"2026-08-11T22:44:47.724754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.14196","last_updated":"2021-09-09T23:39:57Z","snapshot_observed_at":"2026-08-11T12:23:48.612413Z","submitted_at":"2020-04-29T13:39:22Z","title":"The Neutron Star Outer Crust Equation of State: A Machine Learning approach","version":2},"cited_work":{"arxiv_id":"2004.14196","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.14196","snapshot_observed_at":"2026-08-11T22:44:49.070268Z","title":"The Neutron Star Outer Crust Equation of State: A Machine Learning approach","venue":"physics.comp-ph","work_id":"affa4670-d3cd-4473-8a3b-e23b7f4224a2","year":2020},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.784752Z"},"links":{"cited_paper":"/paper/2004.14196","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:a54b4dcfaa247706863b7ad550fabb929a5103bd73de8ef477f011b5aeaba231","observation_id":"70c74412-2eee-4bd2-bd9e-a1a9ba661cdc","resolution":{"observed_at":"2026-08-11T22:44:49.114917Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0704.2558","last_updated":"2007-04-19T18:38:17Z","snapshot_observed_at":"2026-07-06T01:26:23.242296Z","submitted_at":"2007-04-19T18:38:17Z","title":"MeV Dark Matter and Small Scale Structure","version":1},"cited_work":{"arxiv_id":"0704.2558","doi":null,"metadata_source":"pith","pith_arxiv_id":"0704.2558","snapshot_observed_at":"2026-08-11T22:44:48.844749Z","title":"MeV Dark Matter and Small Scale Structure","venue":"astro-ph","work_id":"940ec9e0-f6fa-403f-8b7f-9cecbc57feb6","year":2007},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.828861Z"},"links":{"cited_paper":"/paper/0704.2558","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:06c44bca21e4055fd84031e81a6be0ad4b750948da1ba884034973ce9d3a6e14","observation_id":"61e0af38-cc4d-4127-b0f0-2ead79c08ba9","resolution":{"observed_at":"2026-08-11T22:44:48.894753Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1208.4347","last_updated":"2012-12-17T16:32:12Z","snapshot_observed_at":"2026-07-06T02:54:08.076078Z","submitted_at":"2012-08-21T19:16:52Z","title":"Limits on MeV Dark Matter from the Effective Number of Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1208.4347","snapshot_observed_at":"2026-08-11T22:44:47.874756Z","title":"Ho and R.J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.874756Z"},"links":{"cited_paper":"/paper/1208.4347","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:ed8c3b164e6f3cff1f38c32f8fafc8326da99f12bc619f8fb7144f89707de9b3","observation_id":"043d3a76-056e-4619-8c0e-d13e93a50450","resolution":{"observed_at":"2026-08-11T22:44:47.874756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.06049","last_updated":"2019-03-13T10:58:22Z","snapshot_observed_at":"2026-07-06T07:39:19.062840Z","submitted_at":"2019-03-13T10:58:22Z","title":"Model Independent analysis of MeV scale dark matter: I. Cosmological constraints","version":1},"cited_work":{"arxiv_id":"1903.06049","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.06049","snapshot_observed_at":"2026-08-11T22:44:48.424821Z","title":"Model Independent analysis of MeV scale dark matter: I. Cosmological constraints","venue":"hep-ph","work_id":"2be9d89f-fabd-457d-9b41-fce879782c28","year":2019},"citing_paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T22:44:47.910498Z"},"links":{"cited_paper":"/paper/1903.06049","citing_paper":"/paper/2412.03219"},"observation_digest":"sha256:161885c73bc512820eda83868b73c81941502ac8414c26662824f604d9c5d92b","observation_id":"5ee61a15-372f-4c58-9ee0-485c64057eba","resolution":{"observed_at":"2026-08-11T22:44:48.475055Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.03219","last_updated":"2025-03-11T05:04:22Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-12T03:48:42.313435Z","submitted_at":"2024-12-04T11:13:35Z","title":"Neutron star in Logarithmic model of Cartan $F(R)$ gravity"},"reference_resolution":{"displayed":54,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":29,"verified_exact":13,"verified_fuzzy":11},"total_outbound_references":54},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 0 inbound Pith citation observations for arXiv:2412.03219."}