{"as_of":"2026-08-10T17:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:79109ccc31d3138fd5ce5239d8dcd84cf218233ae62456c41bfaedec6202b1ce","coverage":[{"denominator":129,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T16:30:05.291479Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+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/2607.18008/citation-record","integrity":"/paper/2607.18008/integrity","json":"/paper/2607.18008/citation-record.json","paper":"/paper/2607.18008"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-01T16:29:56.669213Z","title":"Addressing observational tensions in cosmology with sys- tematics and fundamental physics","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:56.669213Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:de17e63891ea1528d3ebba1486d9060eafa6d13ed299904211ebf160739194c4","observation_id":"c96cb7b2-b834-40b3-9a26-7c063559847c","resolution":{"observed_at":"2026-08-01T16:29:56.669213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9805201","last_updated":"1998-05-15T03:59:02Z","snapshot_observed_at":"2026-08-04T06:34:53.046342Z","submitted_at":"1998-05-15T03:59:02Z","title":"Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9805201","snapshot_observed_at":"2026-08-01T16:29:56.755030Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:56.755030Z"},"links":{"cited_paper":"/paper/astro-ph/9805201","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:0b5876a3e2aa1ddf8e6f5ee136ece9a1ebd11ff2321641110ae9f927aace4a11","observation_id":"26a92dee-f699-4846-bba5-a9825192f378","resolution":{"observed_at":"2026-08-01T16:29:56.755030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9812133","last_updated":"1998-12-08T03:27:34Z","snapshot_observed_at":"2026-07-07T01:23:24.602283Z","submitted_at":"1998-12-08T03:27:34Z","title":"Measurements of Omega and Lambda from 42 High-Redshift Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9812133","snapshot_observed_at":"2026-08-01T16:29:56.801234Z","title":"Perlmutteret al.(Supernova Cosmology Project), Measurements ofΩandΛfrom 42 high redshift super- novae, Astrophys","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:56.801234Z"},"links":{"cited_paper":"/paper/astro-ph/9812133","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:c41bcbeb7d09de4ea127b2f5cd0b7a73354771da6abc66da6b41c4528bc2d5ed","observation_id":"ad137ab4-fa28-4e45-9d70-da42d587d6e3","resolution":{"observed_at":"2026-08-01T16:29:56.801234Z","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":"2026-08-01T16:29:56.891479Z","title":"Ratra and P","venue":null,"work_id":null,"year":1988},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:56.891479Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:210468f7940d55493a5a9933c8c9cfc8a5c0e9dff8b92daf9d7ca5f1b06e9889","observation_id":"0200b914-ac6c-4cfa-b94b-3cbcd00988e2","resolution":{"observed_at":"2026-08-01T16:29:56.891479Z","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":"2026-08-01T16:29:56.981949Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:56.981949Z"},"links":{"cited_paper":"/paper/astro-ph/9708069","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:3e39131e528590fbe255162765f1790f3623a00357aa75447c0b92b4ae4a1a46","observation_id":"2f6e1f5e-2694-4bce-952d-52d7dfcaee2f","resolution":{"observed_at":"2026-08-01T16:29:56.981949Z","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":"2026-08-01T16:29:57.040718Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.040718Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:3f93bceee28e8b4f5977583f8097bfbbb7e5879a8f38823943072a26bf81be95","observation_id":"f5201948-d2e8-481f-86ff-5fe69bab3312","resolution":{"observed_at":"2026-08-01T16:29:57.040718Z","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":"2026-08-01T16:29:57.130885Z","title":"Weinberg, The Cosmological Constant Problem, Rev","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.130885Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:65037611b70199a51766a65ae31dacef915261bef9357a8570880990eca0de14","observation_id":"0df1609d-95e7-41c4-bbca-baaa64c30199","resolution":{"observed_at":"2026-08-01T16:29:57.130885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207347","last_updated":"2002-11-20T20:31:52Z","snapshot_observed_at":"2026-07-07T00:27:27.276456Z","submitted_at":"2002-07-16T21:40:00Z","title":"The Cosmological Constant and Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207347","snapshot_observed_at":"2026-08-01T16:29:57.208246Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.208246Z"},"links":{"cited_paper":"/paper/astro-ph/0207347","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:7ab76bf1df6ef637434bdb4a577fe5b02fcc1146ba8c609a11b19cd08839c020","observation_id":"83065417-59f5-4ace-a84d-ad89646474d9","resolution":{"observed_at":"2026-08-01T16:29:57.208246Z","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":"2026-08-01T16:29:57.276380Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.276380Z"},"links":{"cited_paper":"/paper/hep-th/0603057","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:fee79c41388d9840f1626f5fca7ba953297cd9da5632e15155d1e1228f9fc712","observation_id":"f2998041-27d3-4080-a8ba-38d97bc5b8c5","resolution":{"observed_at":"2026-08-01T16:29:57.276380Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.0982","last_updated":"2008-03-07T16:00:09Z","snapshot_observed_at":"2026-07-06T01:37:47.018711Z","submitted_at":"2008-03-07T16:00:09Z","title":"Dark Energy and the Accelerating Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0803.0982","snapshot_observed_at":"2026-08-01T16:29:57.363622Z","title":"Frieman, M","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.363622Z"},"links":{"cited_paper":"/paper/0803.0982","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:bc391f330441422b18ef312c0aa65839f8914ae4867d507128ef5fd9f0818bf5","observation_id":"e6fd5ac4-8c7e-42a5-8ca5-01c536db1b80","resolution":{"observed_at":"2026-08-01T16:29:57.363622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0009008","last_updated":"2000-09-25T18:37:17Z","snapshot_observed_at":"2026-07-07T03:13:00.877347Z","submitted_at":"2000-09-04T15:09:00Z","title":"Accelerating Universes with Scaling Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0009008","snapshot_observed_at":"2026-08-01T16:29:57.413823Z","title":"Chevallier and D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.413823Z"},"links":{"cited_paper":"/paper/gr-qc/0009008","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:7be9799a6d40bf8d74791896290df85988d2e90366df628650b175fcf2427d8e","observation_id":"38069d33-7cb6-458e-82d5-f43b31103cc5","resolution":{"observed_at":"2026-08-01T16:29:57.413823Z","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":"2026-08-01T16:29:57.486740Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.486740Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:f82caebe8f08b118c882c8b76fa189a7eb7da4d194b054974403901cf985aa02","observation_id":"3624aaa4-c322-4523-a4a5-8edc5bae41b9","resolution":{"observed_at":"2026-08-01T16:29:57.486740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.2968","last_updated":"2008-03-07T16:55:10Z","snapshot_observed_at":"2026-07-06T01:33:44.862945Z","submitted_at":"2008-01-18T21:00:08Z","title":"Mapping the Cosmological Expansion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.2968","snapshot_observed_at":"2026-08-01T16:29:57.572158Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.572158Z"},"links":{"cited_paper":"/paper/0801.2968","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:c0f2bb276839a32c48228bb993c19464fa395f41040dae180dedb9111ed3ed2c","observation_id":"887e6bec-53e8-4127-b158-f9b5c8087450","resolution":{"observed_at":"2026-08-01T16:29:57.572158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.07953","last_updated":"2019-08-13T08:06:03Z","snapshot_observed_at":"2026-07-06T08:08:32.264223Z","submitted_at":"2019-07-18T09:40:36Z","title":"Revisiting a negative cosmological constant from low-redshift data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.07953","snapshot_observed_at":"2026-08-01T16:29:57.656786Z","title":"Visinelli, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.656786Z"},"links":{"cited_paper":"/paper/1907.07953","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:b69932d33ce9d69906e1b0ce8e568a661e509bc327fe9be443b65e3424e64d40","observation_id":"c679fa51-8ec3-4016-82d7-a138f61089d7","resolution":{"observed_at":"2026-08-01T16:29:57.656786Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.08751","last_updated":"2020-03-06T15:02:53Z","snapshot_observed_at":"2026-07-06T08:45:28.566259Z","submitted_at":"2019-12-18T17:31:25Z","title":"Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.08751","snapshot_observed_at":"2026-08-01T16:29:57.707445Z","title":"Akarsu, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.707445Z"},"links":{"cited_paper":"/paper/1912.08751","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:ab2e659874547eea204bdf191e5ebf5e996a444459ecd5850d8d4400bf9ffa6a","observation_id":"3ffb6349-c78a-45c9-a9f2-0640b43fdbf6","resolution":{"observed_at":"2026-08-01T16:29:57.707445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.10237","last_updated":"2021-01-25T18:15:48Z","snapshot_observed_at":"2026-07-06T09:49:32.303673Z","submitted_at":"2020-08-24T07:53:41Z","title":"Negative cosmological constant in the dark sector?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.10237","snapshot_observed_at":"2026-08-01T16:29:57.794865Z","title":"Calderón, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.794865Z"},"links":{"cited_paper":"/paper/2008.10237","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:0719e5dfc15973bbc5448c78f005c2e48abf99f564b79e871a8d5d3b9e9e7d0f","observation_id":"daad98d9-8355-473a-b6c8-107f438f839e","resolution":{"observed_at":"2026-08-01T16:29:57.794865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.10641","last_updated":"2022-09-26T09:55:28Z","snapshot_observed_at":"2026-08-10T00:29:58.739878Z","submitted_at":"2021-12-20T16:04:50Z","title":"Do cosmological observations allow a negative $\\Lambda$?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.10641","snapshot_observed_at":"2026-08-01T16:29:57.879187Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.879187Z"},"links":{"cited_paper":"/paper/2112.10641","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:6061b54017519d65ce2352c1803e2a7d011035d34d8cb564521d4c95200bc198","observation_id":"3b12916f-7ea0-4f97-8689-0ede07d21654","resolution":{"observed_at":"2026-08-01T16:29:57.879187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.12725","last_updated":"2024-03-21T12:36:42Z","snapshot_observed_at":"2026-07-06T14:45:55.345502Z","submitted_at":"2023-01-30T08:50:26Z","title":"On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.12725","snapshot_observed_at":"2026-08-01T16:29:57.952451Z","title":"Malekjani, R","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:57.952451Z"},"links":{"cited_paper":"/paper/2301.12725","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:53697fbeb92767a3eb5f995d80ee1839fec662d177aca81617cfa2117f9a399a","observation_id":"05f900e9-9814-42ae-90c8-f2f3c88933e2","resolution":{"observed_at":"2026-08-01T16:29:57.952451Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0511473","last_updated":"2006-03-18T13:20:23Z","snapshot_observed_at":"2026-07-07T00:56:06.332260Z","submitted_at":"2005-11-16T08:02:09Z","title":"Confronting Braneworld Cosmology with Supernova data and Baryon Oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0511473","snapshot_observed_at":"2026-08-01T16:29:58.025659Z","title":"Alam and V","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.025659Z"},"links":{"cited_paper":"/paper/astro-ph/0511473","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:4face9018dc1fac9e109eaed3fee44e7110653dce875d3aa9b84bbbb14c91a57","observation_id":"52d95ef7-8fd0-47d2-ac0b-7c65920949ac","resolution":{"observed_at":"2026-08-01T16:29:58.025659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.04707","last_updated":"2017-01-09T05:30:51Z","snapshot_observed_at":"2026-08-05T21:26:56.965774Z","submitted_at":"2016-05-16T10:10:48Z","title":"Constraining the Cosmology of the Phantom Brane using Distance Measures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.04707","snapshot_observed_at":"2026-08-01T16:29:58.110746Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.110746Z"},"links":{"cited_paper":"/paper/1605.04707","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:45014f2486802004ef41bcbf5986b9778e6759a947dbdd4aeedc44c8fbac856b","observation_id":"743ff7ab-c0c9-4ec5-8bc9-6d7c1c626bfe","resolution":{"observed_at":"2026-08-01T16:29:58.110746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04167","last_updated":"2022-09-08T16:25:49Z","snapshot_observed_at":"2026-08-09T00:49:26.830677Z","submitted_at":"2022-03-08T15:55:47Z","title":"Is the dark energy equation of state parameter singular?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.04167","snapshot_observed_at":"2026-08-01T16:29:58.180093Z","title":"Özülker, Is the dark energy equation of state pa- rameter singular?, Phys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.180093Z"},"links":{"cited_paper":"/paper/2203.04167","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:0be5149f795a1b8a868d0013598dcf92c497730b1fb802d30d8663937e5aee01","observation_id":"eb34fd8a-5273-49fc-abb2-bb7bec4693fa","resolution":{"observed_at":"2026-08-01T16:29:58.180093Z","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":"2026-08-01T16:29:58.244081Z","title":"Raychaudhuri, Relativistic cosmology","venue":null,"work_id":null,"year":1955},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.244081Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:6a2ce45d7adcd0f26783757ccd146ea343abd2f7da6f7e1a8e1e1ce0e25faa40","observation_id":"8dc23192-0e83-44b0-8158-e24480ffd2e3","resolution":{"observed_at":"2026-08-01T16:29:58.244081Z","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":"2026-08-01T16:29:58.304149Z","title":null,"venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.304149Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:85f489f67a09623bd2862dc619bac528e30d92ecedabb9956ea0a785b7da1158","observation_id":"e627880f-c270-492d-b68f-082b17902b01","resolution":{"observed_at":"2026-08-01T16:29:58.304149Z","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":"2026-08-01T16:29:58.383754Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.383754Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:2b774de24be6ac4085d9fdf2f5254159f34583a2e9815ec3cee0cebd339df755","observation_id":"37fbe8a1-d918-4660-a4e7-4635c73435fe","resolution":{"observed_at":"2026-08-01T16:29:58.383754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.12987","last_updated":"2026-04-14T17:22:34Z","snapshot_observed_at":"2026-08-08T20:13:05.608575Z","submitted_at":"2026-04-14T17:22:34Z","title":"Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.12987","snapshot_observed_at":"2026-08-01T16:29:58.431975Z","title":"Akarsu, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.431975Z"},"links":{"cited_paper":"/paper/2604.12987","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:3258c6125d498866d0d12c8d700051fb02c335283a9c04831cc7471f31b42861","observation_id":"a2c1a16b-11fb-4809-af06-a1f1b2a6a07b","resolution":{"observed_at":"2026-08-01T16:29:58.431975Z","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":"2026-08-01T16:29:58.490241Z","title":"Akarsu, M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.490241Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:faf4cea1fbc78f16fa2f5a7fa98fb7cbada02e5cc575922af0842e661fbcc159","observation_id":"33d3c417-d12d-47b0-af28-30ad0e7f6fc7","resolution":{"observed_at":"2026-08-01T16:29:58.490241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.13009","last_updated":"2026-07-14T17:51:30Z","snapshot_observed_at":"2026-08-10T10:24:21.584417Z","submitted_at":"2026-07-14T17:51:30Z","title":"Model-Independent Indication for a Localized Anomaly in the Late-Time Expansion History","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.13009","snapshot_observed_at":"2026-08-01T16:29:58.574228Z","title":"Gupta Choudhury, P","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.574228Z"},"links":{"cited_paper":"/paper/2607.13009","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:d08c2824ed4faa4ea308a4503a945e814bbaeca7dabb17584e4efc20b141f33d","observation_id":"f0b769d6-8482-4c60-8bb9-fe06bb1ff03f","resolution":{"observed_at":"2026-08-01T16:29:58.574228Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2603.14693","last_updated":"2026-07-14T04:50:03Z","snapshot_observed_at":"2026-08-10T07:05:44.565362Z","submitted_at":"2026-03-16T01:02:08Z","title":"Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.14693","snapshot_observed_at":"2026-08-01T16:29:58.644528Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.644528Z"},"links":{"cited_paper":"/paper/2603.14693","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:b311d83fe397a08b95468336e6ace6052a65fdc106183aad300a9a32bbf1c5dd","observation_id":"ecd7d264-b8ca-4cf5-a6da-79342dd07b6c","resolution":{"observed_at":"2026-08-01T16:29:58.644528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0702615","last_updated":"2007-02-27T17:34:49Z","snapshot_observed_at":"2026-07-07T01:07:31.397599Z","submitted_at":"2007-02-22T21:00:43Z","title":"The dark degeneracy: On the number and nature of dark components","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0702615","snapshot_observed_at":"2026-08-01T16:29:58.691747Z","title":"Kunz, The dark degeneracy: On the number and nature of dark components, Phys","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.691747Z"},"links":{"cited_paper":"/paper/astro-ph/0702615","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:1467faee4e0716d86110dfc123e97c64004c54321179f1c0b1ad9510ff0b8b93","observation_id":"fe9bfcff-e126-4d44-9159-928df702795d","resolution":{"observed_at":"2026-08-01T16:29:58.691747Z","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":"2026-08-01T16:29:58.757144Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.757144Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:f32e61cdf04f46d0425a06b69242c273377fa750cb144a6f5b489b24af458e99","observation_id":"30aa4955-9e9a-4609-a255-c14b4493e967","resolution":{"observed_at":"2026-08-01T16:29:58.757144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.27301","last_updated":"2026-06-02T16:18:10Z","snapshot_observed_at":"2026-08-07T14:11:27.638757Z","submitted_at":"2026-05-26T17:11:30Z","title":"Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.27301","snapshot_observed_at":"2026-08-01T16:29:58.802888Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.802888Z"},"links":{"cited_paper":"/paper/2605.27301","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:2942f0a015fa197095ed63718ad6cc04416a3b78c22bf39bdd9d342db6154285","observation_id":"7c6474be-5de1-4060-8dab-40695bc2cd83","resolution":{"observed_at":"2026-08-01T16:29:58.802888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-08-01T16:29:58.860258Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.860258Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:8ebee5d076ea3dbb12b0fb32f5b7c8a8c4b89110be6fb0d6036e8478377c0e68","observation_id":"e1a43f50-8861-42b5-b43e-1e79fdc47285","resolution":{"observed_at":"2026-08-01T16:29:58.860258Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-01T16:29:58.910686Z","title":"Abdul Karimet al.(DESI), DESI DR2 results","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.910686Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:253995d78fbcc2deb68a871335e67a40cbe45c7358a6ba9a1fc0856624785a10","observation_id":"69e1c686-5216-4533-86d5-dee8853c12aa","resolution":{"observed_at":"2026-08-01T16:29:58.910686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2602.11936","last_updated":"2026-05-18T12:54:32Z","snapshot_observed_at":"2026-08-02T13:51:44.487752Z","submitted_at":"2026-02-12T13:35:54Z","title":"Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2602.11936","snapshot_observed_at":"2026-08-01T16:29:58.956444Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:58.956444Z"},"links":{"cited_paper":"/paper/2602.11936","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:42bed66da49c977e5237a8f0f8a67f00ba063f58a66a6ceb5775374ba6d860b9","observation_id":"eb220936-4fc9-4a2b-ba66-ea8d29f329da","resolution":{"observed_at":"2026-08-01T16:29:58.956444Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.19053","last_updated":"2025-06-23T19:14:06Z","snapshot_observed_at":"2026-08-06T23:11:38.518427Z","submitted_at":"2025-06-23T19:14:06Z","title":"Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.19053","snapshot_observed_at":"2026-08-01T16:29:59.043020Z","title":"Özülker, E","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.043020Z"},"links":{"cited_paper":"/paper/2506.19053","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:86cba16d0fd58dbf22eec3b44171037b60192139f2e8114fd9d5acacd74f8055","observation_id":"ed8b5c59-eddd-4a72-ac01-8e500e2b0ed9","resolution":{"observed_at":"2026-08-01T16:29:59.043020Z","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":"2026-08-01T16:29:59.094544Z","title":"Gökçen, Ö","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.094544Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:27353765b52d5f088e440c3014cc8d6dabf868d186d18c6571149370becb7f89","observation_id":"95b0891b-5d62-41ae-aaf4-fba070c4725e","resolution":{"observed_at":"2026-08-01T16:29:59.094544Z","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":"2026-08-01T16:29:59.180874Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.180874Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:be53a143873ddad36155e0eec4f65ea02b1d73b277670b19e2c29ad53061b670","observation_id":"4c4b8d57-7e5c-403e-843b-9587e40fcdb4","resolution":{"observed_at":"2026-08-01T16:29:59.180874Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506748","last_updated":"2005-08-04T15:14:32Z","snapshot_observed_at":"2026-08-04T08:00:13.682092Z","submitted_at":"2005-06-30T08:25:04Z","title":"Observational constraints on low redshift evolution of dark energy: How consistent are different observations?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506748","snapshot_observed_at":"2026-08-01T16:29:59.232730Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.232730Z"},"links":{"cited_paper":"/paper/astro-ph/0506748","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:da3e6f39e1ae10d509677407a88137f1dc30fa9a4449c5d9321836b348dd1cda","observation_id":"1598ad28-8136-49cb-9d7f-b52d700878a2","resolution":{"observed_at":"2026-08-01T16:29:59.232730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.1713","last_updated":"2008-05-12T19:02:04Z","snapshot_observed_at":"2026-08-03T16:10:16.609694Z","submitted_at":"2008-05-12T19:02:04Z","title":"A parametric model for dark energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.1713","snapshot_observed_at":"2026-08-01T16:29:59.320244Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.320244Z"},"links":{"cited_paper":"/paper/0805.1713","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:7b920df54dd98a3a146fa469ba96cd3f561367329724b5b518a7404ed866c649","observation_id":"0459a579-ac7b-45bb-a1e5-5ff81ad56a66","resolution":{"observed_at":"2026-08-01T16:29:59.320244Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.07108","last_updated":"2020-03-17T22:52:15Z","snapshot_observed_at":"2026-08-05T14:12:44.327721Z","submitted_at":"2019-02-18T14:44:29Z","title":"Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.07108","snapshot_observed_at":"2026-08-01T16:29:59.403877Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.403877Z"},"links":{"cited_paper":"/paper/1902.07108","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:afe968ae2b8b506c4e70c389e5005fedbe9d5daccf182cfb5ca352f24ac0ea0a","observation_id":"3afcc579-a1b7-46af-a985-a5bbf5c32eb4","resolution":{"observed_at":"2026-08-01T16:29:59.403877Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14939","last_updated":"2024-07-20T17:12:45Z","snapshot_observed_at":"2026-07-06T18:49:33.987133Z","submitted_at":"2024-07-20T17:12:45Z","title":"Dynamical dark energy confronted with multiple CMB missions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14939","snapshot_observed_at":"2026-08-01T16:29:59.463576Z","title":"Najafi, S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.463576Z"},"links":{"cited_paper":"/paper/2407.14939","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:5366962a81ffffceceb2091f756879af249c35b985cb1fd7129b6f96c0802560","observation_id":"1dd5ee26-a9a3-4d6c-98da-19f5362cd690","resolution":{"observed_at":"2026-08-01T16:29:59.463576Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.01899","last_updated":"2017-03-24T10:40:48Z","snapshot_observed_at":"2026-07-06T05:17:35.666507Z","submitted_at":"2016-11-07T05:57:33Z","title":"Dark energy equation of state parameter and its variation at low redshifts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.01899","snapshot_observed_at":"2026-08-01T16:29:59.519903Z","title":"Tripathi, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.519903Z"},"links":{"cited_paper":"/paper/1611.01899","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:fb7ee9b6719780fca16e92d6d4ab7185c2b5e84bff044e4132accf6c3ec277f8","observation_id":"835709e8-706d-468d-915a-ae208f08b89a","resolution":{"observed_at":"2026-08-01T16:29:59.519903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.12587","last_updated":"2021-03-29T08:08:31Z","snapshot_observed_at":"2026-07-06T09:23:18.336357Z","submitted_at":"2020-05-26T09:14:59Z","title":"Dark Energy with Phantom Crossing and the $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.12587","snapshot_observed_at":"2026-08-01T16:29:59.600212Z","title":"Di Valentino, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.600212Z"},"links":{"cited_paper":"/paper/2005.12587","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:ee7035874c5544615411baea79e97aa331184e3caa903b6f8020710cbb40af9e","observation_id":"15949ada-fdd7-43c8-af70-b6421e0e415f","resolution":{"observed_at":"2026-08-01T16:29:59.600212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.08046","last_updated":"2024-01-15T10:47:22Z","snapshot_observed_at":"2026-07-06T15:42:14.659345Z","submitted_at":"2023-06-13T18:03:43Z","title":"Omnipotent dark energy: A phenomenological answer to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.08046","snapshot_observed_at":"2026-08-01T16:29:59.693064Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.693064Z"},"links":{"cited_paper":"/paper/2306.08046","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:ce93e83312f580e67487dbbd2549a2540a8c5383a39a30c26db2f30badefca2a","observation_id":"4765ad8d-3623-42e2-8587-9d769b0eb385","resolution":{"observed_at":"2026-08-01T16:29:59.693064Z","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":"2026-08-01T16:29:59.752406Z","title":"Montefalcone and R","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.752406Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:4763fb9243339cfe0a8bbbecd503550b4aab9e087254fd0bf7e5d3793fb93362","observation_id":"55d19238-f8bd-4baa-9063-e4119157ea6e","resolution":{"observed_at":"2026-08-01T16:29:59.752406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0708.1072","last_updated":"2008-01-14T04:57:26Z","snapshot_observed_at":"2026-07-06T01:32:54.552004Z","submitted_at":"2007-08-08T10:03:44Z","title":"Deviation from $\\Lambda$CDM: Pressure Parametrization","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0708.1072","snapshot_observed_at":"2026-08-01T16:29:59.811454Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.811454Z"},"links":{"cited_paper":"/paper/0708.1072","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:ffd93f12e12d6fc90adf73937aac32f7f7224e497a7848878ac942e40ee4cf34","observation_id":"255a1dec-97bb-4d34-a5ef-7db3fa7b008b","resolution":{"observed_at":"2026-08-01T16:29:59.811454Z","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":"2026-08-01T16:29:59.874998Z","title":"Cheng, E","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.874998Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:8cce8853146fcb0e11270579105797327bcfbf3ecc78a1959936062a9cc5e55a","observation_id":"eab15a74-11d9-4f9a-ae0f-26bb0b13c5b0","resolution":{"observed_at":"2026-08-01T16:29:59.874998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.02623","last_updated":"2021-07-08T10:41:12Z","snapshot_observed_at":"2026-08-04T12:09:57.875813Z","submitted_at":"2021-04-06T16:00:15Z","title":"Simple-graduated dark energy and spatial curvature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.02623","snapshot_observed_at":"2026-08-01T16:29:59.930218Z","title":"Acquaviva, Ö","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-01T16:29:59.930218Z"},"links":{"cited_paper":"/paper/2104.02623","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:931644bdda3cdb21b0f452928c3514d5c896cbde09c315430be0ea9db04b185b","observation_id":"a21ad628-4a68-4f50-9ccf-0924f6b35ed7","resolution":{"observed_at":"2026-08-01T16:29:59.930218Z","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":"2026-08-01T16:30:00.022086Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.022086Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:2302fc79e4b8d76c1f8848887d07def5d8a1b70bc7c97774ff68cd80222bfffd","observation_id":"6f4ed375-30af-4e8d-bfd8-43313e1ba579","resolution":{"observed_at":"2026-08-01T16:30:00.022086Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.16290","last_updated":"2023-11-17T01:15:05Z","snapshot_observed_at":"2026-08-09T08:59:17.524399Z","submitted_at":"2023-05-25T17:45:58Z","title":"Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.16290","snapshot_observed_at":"2026-08-01T16:30:00.085425Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.085425Z"},"links":{"cited_paper":"/paper/2305.16290","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:a280e076a23e1b5151e821a33c4940bc07b55bc4a3462607900a39598324bdbf","observation_id":"13af9fc1-9c2d-4e8c-a445-296ca11fcfbf","resolution":{"observed_at":"2026-08-01T16:30:00.085425Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.04223","last_updated":"2024-07-05T02:23:07Z","snapshot_observed_at":"2026-08-06T10:44:13.615258Z","submitted_at":"2024-07-05T02:23:07Z","title":"Exploring new physics in the late Universe's expansion through non-parametric inference","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.04223","snapshot_observed_at":"2026-08-01T16:30:00.139235Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.139235Z"},"links":{"cited_paper":"/paper/2407.04223","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:6da3ea5dd2f388c6ddff1bfc32833555e31053aeb121d9da2b0f7a6771a75bf6","observation_id":"eea9ecb5-60f8-438b-95b4-1d5f88512419","resolution":{"observed_at":"2026-08-01T16:30:00.139235Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10625","last_updated":"2019-07-24T18:00:09Z","snapshot_observed_at":"2026-07-06T08:09:59.842324Z","submitted_at":"2019-07-24T18:00:09Z","title":"Tensions between the Early and the Late Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10625","snapshot_observed_at":"2026-08-01T16:30:00.194329Z","title":"Verde, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.194329Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:61e7567983bc447aa76c95f8bf212324847751620585f7f754e1b39015b78c82","observation_id":"3db022b9-5433-43cd-bef3-2388045eeca2","resolution":{"observed_at":"2026-08-01T16:30:00.194329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11284","last_updated":"2020-10-13T11:06:51Z","snapshot_observed_at":"2026-08-10T16:06:25.522301Z","submitted_at":"2020-08-25T21:37:24Z","title":"Cosmology Intertwined II: The Hubble Constant Tension","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11284","snapshot_observed_at":"2026-08-01T16:30:00.248122Z","title":"Di Valentinoet al., Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension, Astropart","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.248122Z"},"links":{"cited_paper":"/paper/2008.11284","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:f899aa984386680f14f8290f04a40a593fa819ecaa415285e9289b39e5c4db6f","observation_id":"e1b0aae9-43fa-405c-bd4a-155194a65a96","resolution":{"observed_at":"2026-08-01T16:30:00.248122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-08-01T16:30:00.284697Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.284697Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:13aaf5e8ca4f630ab8ad9ae58f0b2269607225ff1b856cd40afb1c5a6a39db95","observation_id":"51794a81-a56e-49d1-a432-54b07bc5621b","resolution":{"observed_at":"2026-08-01T16:30:00.284697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08991","last_updated":"2024-07-09T09:56:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-07-17T14:09:48Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08991","snapshot_observed_at":"2026-08-01T16:30:00.356927Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.356927Z"},"links":{"cited_paper":"/paper/2007.08991","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:8d81ec749e2b0528db1d78eddd162d3f22902a4e80afdde47cee0a95e42508c4","observation_id":"1d00ba74-7ecb-4ea4-bd24-76fd3c3a831f","resolution":{"observed_at":"2026-08-01T16:30:00.356927Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01183","snapshot_observed_at":"2026-08-01T16:30:00.434818Z","title":"Di Valentino, O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.434818Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:9ccee7f0c09613990e49061f54de977e8c4c259ebf82f3855e7cdd59de73461b","observation_id":"61c15d37-7990-493a-aa34-e5400adb0a42","resolution":{"observed_at":"2026-08-01T16:30:00.434818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.05208","last_updated":"2022-04-06T12:16:37Z","snapshot_observed_at":"2026-08-04T21:52:15.150186Z","submitted_at":"2021-05-11T17:17:34Z","title":"Challenges for $\\Lambda$CDM: An update","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.05208","snapshot_observed_at":"2026-08-01T16:30:00.489315Z","title":"Perivolaropoulos and F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.489315Z"},"links":{"cited_paper":"/paper/2105.05208","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:2059668455193c59e034b3b5e776f9245d473bcecd68177f6ee1c522f53a26a9","observation_id":"bb99634d-cfe7-4be4-a457-152d564c2ddc","resolution":{"observed_at":"2026-08-01T16:30:00.489315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-08-01T16:30:00.523491Z","title":"High Energy Astrophys.34, 49 (2022), 2203.06142","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.523491Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:77f922f292118542269d8bc25e1ed345d20432941b46c4b5dbff60f0d95162ab","observation_id":"f3df5327-9418-440b-baab-1868e33bb12c","resolution":{"observed_at":"2026-08-01T16:30:00.523491Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04767","last_updated":"2024-07-22T12:19:28Z","snapshot_observed_at":"2026-07-06T17:26:47.184846Z","submitted_at":"2024-02-07T11:36:11Z","title":"$\\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.04767","snapshot_observed_at":"2026-08-01T16:30:00.570107Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.570107Z"},"links":{"cited_paper":"/paper/2402.04767","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:c812f8786287719cbd63281b7b14e2622332075475348bc790797b433db459ee","observation_id":"6f1a5949-45c4-4430-8764-6f4d8cb6f043","resolution":{"observed_at":"2026-08-01T16:30:00.570107Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.01669","last_updated":"2025-08-04T13:56:55Z","snapshot_observed_at":"2026-08-01T19:48:28.599955Z","submitted_at":"2025-04-02T12:17:19Z","title":"The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.01669","snapshot_observed_at":"2026-08-01T16:30:00.582509Z","title":"Di Valentinoet al.(CosmoVerse Network), The Cos- moVerseWhitePaper: Addressingobservationaltensions in cosmology with systematics and fundamental physics, Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.582509Z"},"links":{"cited_paper":"/paper/2504.01669","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:a7bf535e3ae8cb6ad4b0573528484d7b114f55c421a64c2be849592699a9cf82","observation_id":"5da7ac12-a4be-4caa-9491-c9804d99b094","resolution":{"observed_at":"2026-08-01T16:30:00.582509Z","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":"2026-07-06T02:11:23.670680Z","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":"2026-08-01T16:30:00.723892Z","title":"Aghanimet al.(Planck), Planck 2018 results","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.723892Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:4644bf942510532a76eadc33fc4db1e5c7bedac0be5bb8c5077cf48038cc05e8","observation_id":"93d469c5-fb5a-44b2-90d9-35c95ee58e63","resolution":{"observed_at":"2026-08-01T16:30:00.723892Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.20384","last_updated":"2025-09-01T12:16:33Z","snapshot_observed_at":"2026-08-08T08:25:47.915446Z","submitted_at":"2025-02-27T18:56:47Z","title":"Linear matter density perturbations in the $\\Lambda_{\\rm s}$CDM model: Examining growth dynamics and addressing the $S_8$ tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.20384","snapshot_observed_at":"2026-08-01T16:30:00.776751Z","title":"Akarsu, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.776751Z"},"links":{"cited_paper":"/paper/2502.20384","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:7f72bdd01bf2a5ae63f0d4b7805d7817fe2da792dec285a22df18e80dfe8e0d2","observation_id":"f7475c15-2ff3-4885-b140-c6290b4d2c3e","resolution":{"observed_at":"2026-08-01T16:30:00.776751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.09239","last_updated":"2021-12-04T18:24:37Z","snapshot_observed_at":"2026-08-08T22:51:57.914223Z","submitted_at":"2021-08-20T15:58:21Z","title":"Relaxing cosmological tensions with a sign switching cosmological constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.09239","snapshot_observed_at":"2026-08-01T16:30:00.821078Z","title":"Akarsu, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.821078Z"},"links":{"cited_paper":"/paper/2108.09239","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:0da997f79964d939795996fc1c56adf316d6d0b64faeaad1ed7145a7a1c5e02a","observation_id":"02760d5f-9b50-4c3e-9e58-95e048793bf8","resolution":{"observed_at":"2026-08-01T16:30:00.821078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.05742","last_updated":"2023-07-14T15:56:37Z","snapshot_observed_at":"2026-07-06T14:16:52.598523Z","submitted_at":"2022-11-10T18:18:52Z","title":"Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.05742","snapshot_observed_at":"2026-08-01T16:30:00.888425Z","title":"Akarsu, S","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.888425Z"},"links":{"cited_paper":"/paper/2211.05742","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:9f278cde13a1462e9a10b438911925789896196c919aa305d5da7c4333ac1cf6","observation_id":"15fc0b27-f801-4583-8232-87987e08faab","resolution":{"observed_at":"2026-08-01T16:30:00.888425Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.10899","last_updated":"2023-07-20T14:22:51Z","snapshot_observed_at":"2026-08-03T10:24:09.088585Z","submitted_at":"2023-07-20T14:22:51Z","title":"$\\Lambda_{\\rm s}$CDM model: A promising scenario for alleviation of cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.10899","snapshot_observed_at":"2026-08-01T16:30:00.991506Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:00.991506Z"},"links":{"cited_paper":"/paper/2307.10899","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:5f620b7eb54769936910ae0bcf090b8507aeac4f91fad29e5c8da3771939f613","observation_id":"db9aa56b-7912-467b-b3f8-94849ed69dc0","resolution":{"observed_at":"2026-08-01T16:30:00.991506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07716","last_updated":"2026-04-28T16:55:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-02-12T15:29:10Z","title":"$\\Lambda_{\\rm s}$CDM cosmology from a type-II minimally modified gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.07716","snapshot_observed_at":"2026-08-01T16:30:01.059838Z","title":"Akarsu, A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.059838Z"},"links":{"cited_paper":"/paper/2402.07716","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:012bd34ec555ef27d62a9347f317dccb6f70e9f68d02a5ddf33f7fc4256c830f","observation_id":"629f81f5-592c-48a4-9d26-5fe88923fe45","resolution":{"observed_at":"2026-08-01T16:30:01.059838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.07526","last_updated":"2024-11-25T11:51:36Z","snapshot_observed_at":"2026-08-07T01:21:02.056159Z","submitted_at":"2024-06-11T17:53:58Z","title":"Cosmological constraints on $\\Lambda_{\\rm s}$CDM scenario in a type II minimally modified gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.07526","snapshot_observed_at":"2026-08-01T16:30:01.136828Z","title":"Akarsu, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.136828Z"},"links":{"cited_paper":"/paper/2406.07526","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:6d0c47c62d9d5989f894619b88f20722b455621d9743b51fdc25966ed000ca3e","observation_id":"c000968e-fcb4-418e-bda5-a4701201baf1","resolution":{"observed_at":"2026-08-01T16:30:01.136828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.12945","last_updated":"2025-03-18T21:46:19Z","snapshot_observed_at":"2026-08-09T10:20:44.704305Z","submitted_at":"2025-03-17T08:58:49Z","title":"Exploring the Growth-Index ($\\gamma$) Tension with $\\Lambda_{\\rm s}$CDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.12945","snapshot_observed_at":"2026-08-01T16:30:01.181605Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.181605Z"},"links":{"cited_paper":"/paper/2503.12945","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:e225c087557446470816d8b94702de05d65bdab82d82170fbc0733f75e865c4e","observation_id":"381c2842-01c2-4580-aec5-2023d2b2c989","resolution":{"observed_at":"2026-08-01T16:30:01.181605Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.05908","last_updated":"2024-07-26T09:03:21Z","snapshot_observed_at":"2026-08-09T02:19:12.105209Z","submitted_at":"2024-02-08T18:43:39Z","title":"Transition dynamics in the $\\Lambda_{\\rm s}$CDM model: Implications for bound cosmic structures","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.05908","snapshot_observed_at":"2026-08-01T16:30:01.237751Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.237751Z"},"links":{"cited_paper":"/paper/2402.05908","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:f9a31ccb928d6b7930e32aa395dd679fe5db74f9a59c59e9333130ff69f11647","observation_id":"bc44e44b-0ab3-4f0b-8c59-43da02d96589","resolution":{"observed_at":"2026-08-01T16:30:01.237751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2510.18741","last_updated":"2026-04-10T13:03:33Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-21T15:46:25Z","title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.18741","snapshot_observed_at":"2026-08-01T16:30:01.348578Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.348578Z"},"links":{"cited_paper":"/paper/2510.18741","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:d0e4b0e515c50407908fd115515719a724ae06c02172b38634be60cb126212f1","observation_id":"8dc601db-9916-4a67-a884-bbd3dea00780","resolution":{"observed_at":"2026-08-01T16:30:01.348578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.18496","last_updated":"2025-01-13T14:51:38Z","snapshot_observed_at":"2026-08-05T11:56:53.858651Z","submitted_at":"2024-06-26T16:59:13Z","title":"$\\Lambda_{\\rm s}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.18496","snapshot_observed_at":"2026-08-01T16:30:01.459632Z","title":"Yadav, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.459632Z"},"links":{"cited_paper":"/paper/2406.18496","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:ea42c186446530b12f0e4039fb9b59f56e289e921207b5ae903594c633132208","observation_id":"b3807516-0022-4901-8538-7b25fbbd1a4a","resolution":{"observed_at":"2026-08-01T16:30:01.459632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.21456","last_updated":"2026-05-20T17:46:56Z","snapshot_observed_at":"2026-07-06T23:31:56.199912Z","submitted_at":"2026-05-20T17:46:56Z","title":"Negative neutrino mass or negative dark energy?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.21456","snapshot_observed_at":"2026-08-01T16:30:01.645095Z","title":"Kıbrıs, W","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.645095Z"},"links":{"cited_paper":"/paper/2605.21456","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:76974ea41098c332efaaf3cce6ed294e69601fd956b5b811eec625954deb99a9","observation_id":"8147402b-2012-462e-b7ce-0df4a2ef279a","resolution":{"observed_at":"2026-08-01T16:30:01.645095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.18031","last_updated":"2025-01-29T22:37:59Z","snapshot_observed_at":"2026-08-10T16:58:29.949696Z","submitted_at":"2025-01-29T22:37:59Z","title":"Mapping the $\\Lambda_{\\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.18031","snapshot_observed_at":"2026-08-01T16:30:01.807584Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.807584Z"},"links":{"cited_paper":"/paper/2501.18031","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:48c5b639849adf7fefd506f7d6c18f605c2ead7a7c0223f55ef595af2f6823f1","observation_id":"bdf99a8c-29a1-41ec-8ae0-cc1080240783","resolution":{"observed_at":"2026-08-01T16:30:01.807584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.10194","last_updated":"2018-03-01T09:52:18Z","snapshot_observed_at":"2026-08-09T15:19:02.818117Z","submitted_at":"2017-10-27T15:25:19Z","title":"Phase Portraits of general f(T) Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.10194","snapshot_observed_at":"2026-08-01T16:30:01.921602Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:01.921602Z"},"links":{"cited_paper":"/paper/1710.10194","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:61f10fab091ee449a0abfa9658a1ac4ba8552a8473ea9587ff093053dfc9439a","observation_id":"8b1b6448-7df6-4ce4-86dd-32d6df6c3f5f","resolution":{"observed_at":"2026-08-01T16:30:01.921602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14964","last_updated":"2021-04-16T18:59:42Z","snapshot_observed_at":"2026-07-06T10:09:24.408440Z","submitted_at":"2020-10-28T13:28:26Z","title":"Toward a concordance teleparallel Cosmology I: Background Dynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.14964","snapshot_observed_at":"2026-08-01T16:30:02.117779Z","title":"Hashim, W","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.117779Z"},"links":{"cited_paper":"/paper/2010.14964","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:a90e4bdfe0f229203dc6344a44b3a087ab1e0e0f4fd5dcc4c57e72807299fd1a","observation_id":"7cbf47aa-71a0-45e3-9131-95a20d6ba29a","resolution":{"observed_at":"2026-08-01T16:30:02.117779Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.08311","last_updated":"2021-04-16T18:52:10Z","snapshot_observed_at":"2026-07-06T11:00:28.950168Z","submitted_at":"2021-04-16T18:52:10Z","title":"Toward a concordance teleparallel Cosmology II: Linear perturbation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.08311","snapshot_observed_at":"2026-08-01T16:30:02.224144Z","title":"Hashim, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.224144Z"},"links":{"cited_paper":"/paper/2104.08311","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:2081761d85df98af197b76d8d9b90390d50dfc2776b8c4ebf73d23f11343d591","observation_id":"5a8388bd-1ee5-4177-9cb5-f00f0d9dc372","resolution":{"observed_at":"2026-08-01T16:30:02.224144Z","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":"2026-08-01T16:30:02.336295Z","title":"Akarsu, B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.336295Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:db014ce3a75d297ec1b767ddd7be8a8385e6f1cfd8e2deef42ec4f137b538624","observation_id":"a696a66d-55bc-462a-9b7c-760531a8b11d","resolution":{"observed_at":"2026-08-01T16:30:02.336295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0202346","last_updated":"2003-12-09T17:02:56Z","snapshot_observed_at":"2026-07-07T00:25:08.568215Z","submitted_at":"2002-02-19T07:22:19Z","title":"Braneworld models of dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0202346","snapshot_observed_at":"2026-08-01T16:30:02.471263Z","title":"Sahni and Y","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.471263Z"},"links":{"cited_paper":"/paper/astro-ph/0202346","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:4e40b9366f620d8c6c5cd1ddb4d97ec71fa4bed57d7b2cedabe96403200a12a2","observation_id":"644ff6ae-c4c4-46f7-9d48-d4354b6e6ffb","resolution":{"observed_at":"2026-08-01T16:30:02.471263Z","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":"2026-08-01T16:30:02.589817Z","title":"Sahni and Y","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.589817Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:47b69a2e809226b760b4a6a86b014a79a53ff13edf0a4e5a8b320194ed666686","observation_id":"8894b76a-4983-41fd-8934-4178382ae4c6","resolution":{"observed_at":"2026-08-01T16:30:02.589817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.03271","last_updated":"2021-12-27T06:02:23Z","snapshot_observed_at":"2026-08-03T18:11:34.202566Z","submitted_at":"2021-07-07T15:04:28Z","title":"Phantom braneworld and the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.03271","snapshot_observed_at":"2026-08-01T16:30:02.698081Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.698081Z"},"links":{"cited_paper":"/paper/2107.03271","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:17532bcf610975a2976963377985e2dd78e5f8cb4a448b6e56d9ceeaf07642d6","observation_id":"d775f40a-2485-46fa-b94d-908623d3a847","resolution":{"observed_at":"2026-08-01T16:30:02.698081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.12549","last_updated":"2020-09-16T16:13:19Z","snapshot_observed_at":"2026-08-04T03:15:32.538096Z","submitted_at":"2020-04-27T02:27:05Z","title":"A theory of type-II minimally modified gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.12549","snapshot_observed_at":"2026-08-01T16:30:02.821978Z","title":"De Felice, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.821978Z"},"links":{"cited_paper":"/paper/2004.12549","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:19b12ab9aa37bed5905d99217b2eace3c7f2a766b307491c8e52f195e895b75e","observation_id":"ec33ff6e-2b98-41bc-bbfe-fb2c03431839","resolution":{"observed_at":"2026-08-01T16:30:02.821978Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.08294","last_updated":"2022-10-01T09:00:02Z","snapshot_observed_at":"2026-08-10T07:25:51.885007Z","submitted_at":"2022-04-18T12:51:44Z","title":"VCDM and Cuscuton","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.08294","snapshot_observed_at":"2026-08-01T16:30:02.968944Z","title":"De Felice, K.-i","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:02.968944Z"},"links":{"cited_paper":"/paper/2204.08294","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:b11add06a3291870c0c2eeba5bbec1167f14126511b644864cc37fef244a8c4c","observation_id":"e574ae04-c6e9-49e5-a4b3-66db5a7ca095","resolution":{"observed_at":"2026-08-01T16:30:02.968944Z","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":"2026-08-01T16:30:03.093537Z","title":null,"venue":null,"work_id":null,"year":1935},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:03.093537Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:91fa9dffe2b17a400c9bc44a59af34e1c09ce3184b1a5d098490d9dfbd7b6c8e","observation_id":"5de1a88d-cda8-4f43-abc2-03ba2f2070a6","resolution":{"observed_at":"2026-08-01T16:30:03.093537Z","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":"2026-08-01T16:30:03.201443Z","title":null,"venue":null,"work_id":null,"year":1934},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:03.201443Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:2b1da34c5e5ca7981560f2db1c51f76111f37c5a1e5c1cf063ceb9e6f192238e","observation_id":"4066190d-30a7-4627-b279-09b330b4b539","resolution":{"observed_at":"2026-08-01T16:30:03.201443Z","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":"2026-08-01T16:30:03.367758Z","title":"Barcelo and M","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:03.367758Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:cf302e6052bc90fd1b9013e315156322ac9cb4b3f3955c7f65848fcd79d57044","observation_id":"211dffa6-6ea6-40cf-b03b-423c090a2a85","resolution":{"observed_at":"2026-08-01T16:30:03.367758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.0403","last_updated":"2014-04-30T23:42:53Z","snapshot_observed_at":"2026-08-10T16:38:30.230542Z","submitted_at":"2014-04-30T23:42:53Z","title":"A Primer on Energy Conditions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.0403","snapshot_observed_at":"2026-08-01T16:30:03.527781Z","title":"Curiel, A Primer on Energy Conditions, Einstein Stud","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:03.527781Z"},"links":{"cited_paper":"/paper/1405.0403","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:00ea360971ce4a45df104d8aca321c8e6767a810f80942bfe47f78d6fddc76b6","observation_id":"686b1c3e-6e34-4e06-8f7d-6e9a3ddd5253","resolution":{"observed_at":"2026-08-01T16:30:03.527781Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.01815","last_updated":"2020-06-05T02:22:16Z","snapshot_observed_at":"2026-08-03T19:12:52.798478Z","submitted_at":"2020-03-03T22:30:02Z","title":"Energy conditions in general relativity and quantum field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.01815","snapshot_observed_at":"2026-08-01T16:30:03.644633Z","title":"Kontou and K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:03.644633Z"},"links":{"cited_paper":"/paper/2003.01815","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:c713f327de83f4a379b4f8956511ed94384be10333cca5de19d3ff02930b4b60","observation_id":"cba7c4a9-b60c-466d-8ee0-7557f36911fe","resolution":{"observed_at":"2026-08-01T16:30:03.644633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.4024","last_updated":"2014-02-25T15:14:11Z","snapshot_observed_at":"2026-07-06T03:33:29.808294Z","submitted_at":"2014-01-16T13:41:06Z","title":"The Null Energy Condition and its violation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.4024","snapshot_observed_at":"2026-08-01T16:30:03.761602Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:03.761602Z"},"links":{"cited_paper":"/paper/1401.4024","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:d305c3c380b045e7a0b9ee8882c3ef45b39977249a9235769e9ef19bc5fe4018","observation_id":"e6a1baec-a75d-4023-b25f-337bd8ba8db3","resolution":{"observed_at":"2026-08-01T16:30:03.761602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0501025","last_updated":"2005-03-18T08:33:33Z","snapshot_observed_at":"2026-07-07T04:52:53.905903Z","submitted_at":"2005-01-05T07:43:00Z","title":"Properties of singularities in (phantom) dark energy universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0501025","snapshot_observed_at":"2026-08-01T16:30:03.839541Z","title":"Nojiri, S","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:03.839541Z"},"links":{"cited_paper":"/paper/hep-th/0501025","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:c3ee6d51d26cc7fa2a642eb9eb037fc3648fcae01721702c438b7dc53dd4f758","observation_id":"2e62ae18-686e-4e78-82d4-50614f03870a","resolution":{"observed_at":"2026-08-01T16:30:03.839541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9812046","last_updated":"2008-09-02T14:06:26Z","snapshot_observed_at":"2026-07-07T03:29:51.781434Z","submitted_at":"1998-12-14T14:58:03Z","title":"Cosmological models (Carg\\`{e}se lectures 1998)","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9812046","snapshot_observed_at":"2026-08-01T16:30:04.040685Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.040685Z"},"links":{"cited_paper":"/paper/gr-qc/9812046","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:b8ffab39b17598dd310897a65cfc48d0b437fe7f26505498f467d0d33fc814a9","observation_id":"363b250d-5a7d-4beb-825e-7ee30438a3bd","resolution":{"observed_at":"2026-08-01T16:30:04.040685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0407107","last_updated":"2005-01-20T18:35:48Z","snapshot_observed_at":"2026-07-07T00:43:29.764469Z","submitted_at":"2004-07-06T13:59:33Z","title":"Can dark energy evolve to the Phantom?","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0407107","snapshot_observed_at":"2026-08-01T16:30:04.188743Z","title":"Vikman, Can dark energy evolve to the phantom?, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.188743Z"},"links":{"cited_paper":"/paper/astro-ph/0407107","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:9b6aeff5611793abeca63ccc9a6e5976ca6350e53368f440b40fc664e01f9da5","observation_id":"adacd329-2e5b-4bc3-a850-09b3f3ac7653","resolution":{"observed_at":"2026-08-01T16:30:04.188743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.14667","last_updated":"2025-02-20T16:03:43Z","snapshot_observed_at":"2026-08-07T18:01:37.171780Z","submitted_at":"2025-02-20T16:03:43Z","title":"Dynamical dark energy with AdS-to-dS and dS-to-dS transitions: Implications for the $H_0$ tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.14667","snapshot_observed_at":"2026-08-01T16:30:04.343637Z","title":"Akarsu, L","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.343637Z"},"links":{"cited_paper":"/paper/2502.14667","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:a0a105dcc2efb032475276ef2b28a27d9bea738daecf6505ea361ccf95063c13","observation_id":"1793422d-2377-40aa-bec3-87ef896a007c","resolution":{"observed_at":"2026-08-01T16:30:04.343637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.11062","last_updated":"2026-06-09T16:23:08Z","snapshot_observed_at":"2026-08-01T22:02:37.358175Z","submitted_at":"2026-06-09T16:23:08Z","title":"A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.11062","snapshot_observed_at":"2026-08-01T16:30:04.470382Z","title":"Akarsu, L","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.470382Z"},"links":{"cited_paper":"/paper/2606.11062","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:9ef12a4636dd3724d5271fe1f0e7092c9087b414f7a1c1342b301f4835ac3fc7","observation_id":"81427007-32e0-434c-9e47-1bc376f43e07","resolution":{"observed_at":"2026-08-01T16:30:04.470382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.01132","last_updated":"2019-12-03T00:15:19Z","snapshot_observed_at":"2026-08-10T00:48:36.925431Z","submitted_at":"2019-12-03T00:15:19Z","title":"Big-Bang Nucleosynthesis After Planck","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.01132","snapshot_observed_at":"2026-08-01T16:30:04.620218Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.620218Z"},"links":{"cited_paper":"/paper/1912.01132","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:f49cb483f4486ada0223c5b5d7be64fd720a45184c51637dce31296665dc0eb0","observation_id":"658828d6-029a-44f3-9075-5298df5e48b0","resolution":{"observed_at":"2026-08-01T16:30:04.620218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.12139","last_updated":"2025-09-08T10:10:32Z","snapshot_observed_at":"2026-08-09T12:56:29.371423Z","submitted_at":"2025-06-13T18:01:48Z","title":"Cosmographic analysis of sign-switching dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.12139","snapshot_observed_at":"2026-08-01T16:30:04.715454Z","title":"Bouhmadi-López and B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.715454Z"},"links":{"cited_paper":"/paper/2506.12139","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:9ff43fdaeb6749abbf7d1f9ff656be64471dc6efcf64a39cbf5a2a927de9aafe","observation_id":"9711f70d-5725-4ecd-abd5-a6e998e3aa26","resolution":{"observed_at":"2026-08-01T16:30:04.715454Z","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":"2026-08-01T16:30:04.880951Z","title":"Bouhmadi-López and B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.880951Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:cfdd47d475cf6768ce050f411ee6eb70ee0e0fa99d0abaa8a40e8ed1f8070948","observation_id":"0d1fa235-2f9e-4e3c-9bdd-0b31f6c15496","resolution":{"observed_at":"2026-08-01T16:30:04.880951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2602.12347","last_updated":"2026-05-14T14:22:35Z","snapshot_observed_at":"2026-08-02T15:18:59.160316Z","submitted_at":"2026-02-12T19:08:27Z","title":"Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2602.12347","snapshot_observed_at":"2026-08-01T16:30:04.994870Z","title":"Ibarra-Uriondo and M","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:04.994870Z"},"links":{"cited_paper":"/paper/2602.12347","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:29362653999f5438c6c9cefd71528cd973f102294d15a9ccdb8f96ab7dcc6735","observation_id":"47795c49-9fe7-48e0-a3a1-14fca369d195","resolution":{"observed_at":"2026-08-01T16:30:04.994870Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.05044","last_updated":"2026-07-06T13:21:04Z","snapshot_observed_at":"2026-08-06T06:21:38.078437Z","submitted_at":"2026-07-06T13:21:04Z","title":"Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.05044","snapshot_observed_at":"2026-08-01T16:30:05.145692Z","title":"Bouhmadi-López, H.-W","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:05.145692Z"},"links":{"cited_paper":"/paper/2607.05044","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:f001430d703622ddaf4ab05ce43587a0aec34b20444a94cee678f1fb066eca54","observation_id":"e5de2e3d-cc6e-4093-8c6b-ad29fbad0534","resolution":{"observed_at":"2026-08-01T16:30:05.145692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07299","last_updated":"2025-05-04T15:00:56Z","snapshot_observed_at":"2026-08-07T16:07:02.612122Z","submitted_at":"2025-04-09T21:41:35Z","title":"Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07299","snapshot_observed_at":"2026-08-01T16:30:05.259299Z","title":"Akarsu, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:05.259299Z"},"links":{"cited_paper":"/paper/2504.07299","citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:fd82259d5a4a884d4c76c3265dc2afd4730321f5fe110d588f85b86467a135b2","observation_id":"e3c469d5-4e50-4853-831f-33546d211efd","resolution":{"observed_at":"2026-08-01T16:30:05.259299Z","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":"2026-08-01T16:30:05.291479Z","title":"Gómez-Valent and A","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-01T16:30:05.291479Z"},"links":{"citing_paper":"/paper/2607.18008"},"observation_digest":"sha256:34b4d67916690989ac48397d7c8013659ab6a8d6892b5a03c50d35f93f812391","observation_id":"6a061d47-ebc8-4e08-a661-bd4e63c14523","resolution":{"observed_at":"2026-08-01T16:30:05.291479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.18008","last_updated":"2026-07-20T14:41:08Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-07T08:10:36.780076Z","submitted_at":"2026-07-20T14:41:08Z","title":"Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":100,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":129},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 129 outbound references and 0 inbound Pith citation observations for arXiv:2607.18008."}