{"as_of":"2026-08-10T02:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:896ac1d26fa61de5b7d3cf115f0e8c465c1647dcbb5329edf98f1bb966aa0b1d","coverage":[{"denominator":55,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":55,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T18:27:00.803333Z","state":"measured"},{"denominator":58,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":58,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T18:26:56.823671Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-18T08:51:08.660494Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.08479","snapshot_observed_at":"2026-08-06T18:26:56.823671Z","title":"While the value has since been revised down significantly, there is now some disagreement, or tension, in the current measured value","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:56.823671Z"},"links":{"cited_paper":"/paper/2507.08479","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:3c074fc8535d9e0f5db486cde76cdad06832f64cbf5d9d125cb38517479a3e99","observation_id":"73ac2f0b-b993-4703-8596-37cdeb8b4e99","resolution":{"observed_at":"2026-08-06T18:26:56.823671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.08479","snapshot_observed_at":"2026-08-04T12:53:41.053313Z","title":"Simpson, K","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.01974","last_updated":"2026-01-19T10:15:04Z","snapshot_observed_at":"2026-08-04T12:53:22.243014Z","submitted_at":"2025-10-02T12:47:51Z","title":"BAO miscalibration cannot rescue late-time solutions to the Hubble tension","version":2},"reference_index":105,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:41.053313Z"},"links":{"cited_paper":"/paper/2507.08479","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:e4d1bbf11794ad765446d6fdf829b58189344bcb79b67dcf1c46d5e81326856c","observation_id":"4cbb841a-035d-4e4b-a97b-4d3fda97e780","resolution":{"observed_at":"2026-08-04T12:53:41.053313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"cited_work":{"arxiv_id":"2507.08479","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.08479","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"b9f2a8e9-2282-4d68-9fc9-7fbcc81d267f","year":null},"citing_paper":{"arxiv_id":"2510.05400","last_updated":"2026-05-12T18:57:13Z","snapshot_observed_at":"2026-08-08T20:19:36.745595Z","submitted_at":"2025-10-06T21:46:05Z","title":"Binary Neutron Stars from the Moon: Early Warnings and Precision Science for the Artemis Era","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-18T08:50:34.604521Z"},"links":{"cited_paper":"/paper/2507.08479","citing_paper":"/paper/2510.05400"},"observation_digest":"sha256:a1fa81c3f686e7213d785291bb294eef6f4d7ea7c95979f70c150b9e88a81e05","observation_id":"bdcb4bb8-2d42-486a-a665-9679067ca8ff","resolution":{"observed_at":"2026-05-18T08:51:08.662596Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.08479/citation-record","integrity":"/paper/2507.08479/integrity","json":"/paper/2507.08479/citation-record.json","paper":"/paper/2507.08479"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.08479","snapshot_observed_at":"2026-08-06T18:26:56.823671Z","title":"While the value has since been revised down significantly, there is now some disagreement, or tension, in the current measured value","venue":null,"work_id":null,"year":1927},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:56.823671Z"},"links":{"cited_paper":"/paper/2507.08479","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:3c074fc8535d9e0f5db486cde76cdad06832f64cbf5d9d125cb38517479a3e99","observation_id":"73ac2f0b-b993-4703-8596-37cdeb8b4e99","resolution":{"observed_at":"2026-08-06T18:26:56.823671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:06.103371Z","title":"Interactions between photons and baryons in this fluid created perturbations in the plasma which propagated at the speed of sound","venue":null,"work_id":"4692eb31-8874-4e13-b917-bb573d6946f5","year":null},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:56.998288Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:a319522195114633006a723c757d83a70c250fc422fd844257bfb690f7e7f730","observation_id":"0123381e-43c2-459a-a8e2-918eff5c944a","resolution":{"observed_at":"2026-08-06T18:27:06.108941Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"0467.0848","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:01.926261Z","title":"The addition of the simple fluid Ω X results in essentially just Gaussian noise, as shown in Figure 6","venue":null,"work_id":"da835d2e-389b-4450-9f8a-ff2f21d656e3","year":2018},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.316516Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:51d7db9ad28c75c0619c6428743ba13dee214ad885d516b914d0b60d8918f4e7","observation_id":"246111ac-9cb4-47b5-882a-74ac423243d8","resolution":{"observed_at":"2026-08-06T18:27:01.974318Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.713849Z","title":"In this paper we have reviewed a number of papers that each modified the conditions in the early universe, reducing the sound horizon and raising the value of H0","venue":null,"work_id":"75011430-23ac-4526-b51c-0e0c816e13a9","year":null},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.440394Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:6926fbd2d327afc5ec3fe93fb6dc66b636cd988365a198ef410ba4c68f781bda","observation_id":"e6b1825a-af55-41eb-ab43-3fa74b34d58d","resolution":{"observed_at":"2026-08-06T18:27:05.800595Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14454","last_updated":"2025-06-24T17:02:01Z","snapshot_observed_at":"2026-08-07T12:22:01.678561Z","submitted_at":"2025-03-18T17:30:26Z","title":"The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14454","snapshot_observed_at":"2026-08-06T18:26:57.877289Z","title":"Colin Hill, Hidde T","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.877289Z"},"links":{"cited_paper":"/paper/2503.14454","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:3f24b523a407743039934a3712819470ecfa78aab0618432acc061e4796c0c18","observation_id":"118bbfb5-3f48-449a-99ff-8b3167f2758d","resolution":{"observed_at":"2026-08-06T18:26:57.877289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09091","last_updated":"2023-02-17T19:00:05Z","snapshot_observed_at":"2026-08-08T23:57:59.090819Z","submitted_at":"2023-02-17T19:00:05Z","title":"Neutrino-Assisted Early Dark Energy is a Natural Resolution of the Hubble Tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09091","snapshot_observed_at":"2026-08-06T18:26:57.954202Z","title":"Neutrino-Assisted Early Dark Energy is a Natural Resolution of the Hubble Tension","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.954202Z"},"links":{"cited_paper":"/paper/2302.09091","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:ce58f87dc639caba80f26f8b1a42f61f27d07e0c2d911a8e7300e8b4ab833295","observation_id":"f6de4cd5-c153-4dee-9d45-b56de89ec487","resolution":{"observed_at":"2026-08-06T18:26:57.954202Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.121869Z","title":"Pedro, and Marco Scalisi","venue":null,"work_id":"f3091399-255c-4d92-996f-5a8356c21db1","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.023219Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:9125ac5581aaeb3d3922b8d7a9861a18746e442fd81f36a4ecbbc1a2a744d861","observation_id":"c0cf4192-e4a5-412b-99d7-7e1a71ee748e","resolution":{"observed_at":"2026-08-06T18:27:05.175203Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.082974Z","title":"Cruz, Steen Hannestad, Emil Brinch Holm, Florian Niedermann, Martin S","venue":null,"work_id":"42d2a8b9-87bf-4787-9804-53b854cfeeb4","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.117263Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:8ff1bde31d88d8eb8472129c6873ed872d1ba52fe47a83c2ca36367626142781","observation_id":"7e7294d3-8321-4bc6-8e54-ff35f224eee8","resolution":{"observed_at":"2026-08-06T18:27:05.087909Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.524041Z","title":"Sen, and M","venue":null,"work_id":"f2a05394-9f7e-4fa1-80ce-aa039b491485","year":2024},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.535698Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:940d7de97d83391f6780f9abbff47349fbf0fa112b914e662973caaad1a45451","observation_id":"a8fe7733-968c-49ed-a8ef-49ced9da349f","resolution":{"observed_at":"2026-08-06T18:27:05.624279Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.00067","last_updated":"2023-01-31T20:01:05Z","snapshot_observed_at":"2026-08-10T02:15:37.562584Z","submitted_at":"2023-01-31T20:01:05Z","title":"Emergent Unparticles Dark Energy can restore cosmological concordance","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.00067","snapshot_observed_at":"2026-08-06T18:26:57.615345Z","title":"Emergent Unparticles Dark Energy can restore cosmological concordance","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.615345Z"},"links":{"cited_paper":"/paper/2302.00067","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:3c43032dfbd139d71801d08f8cac502e08ebbd2e050bbbfb24faf20b700abe82","observation_id":"987daaf8-5593-4f85-8250-0b95afefaf86","resolution":{"observed_at":"2026-08-06T18:26:57.615345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.05917","last_updated":"2023-07-12T05:05:41Z","snapshot_observed_at":"2026-07-06T15:53:03.616093Z","submitted_at":"2023-07-12T05:05:41Z","title":"Early dark energy induced by non-linear electrodynamics","version":1},"cited_work":{"arxiv_id":"2307.05917","doi":null,"metadata_source":"pith","pith_arxiv_id":"2307.05917","snapshot_observed_at":"2026-08-06T18:27:01.540830Z","title":"Early dark energy induced by non-linear electrodynamics","venue":"gr-qc","work_id":"8a13fb84-df9b-4368-b438-e028672d73b4","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.699671Z"},"links":{"cited_paper":"/paper/2307.05917","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:d747f9055079cdfc3b4d66f36bf243e74ce1222807b63dbfd596cf7d996a5402","observation_id":"20895633-329b-40f0-ad94-7f53b5e49c22","resolution":{"observed_at":"2026-08-06T18:27:01.704690Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.272840Z","title":"Riess, et al","venue":null,"work_id":"5ef4668d-a30c-4812-8787-eea8b579ae7a","year":2022},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.768790Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:336111a37d6a15bbc1b67a59fe2f540fe2c6c3c11428f320d17d6d7912494ac0","observation_id":"3c011422-dd99-46c3-a2e6-057751169807","resolution":{"observed_at":"2026-08-06T18:27:05.371763Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.051511Z","title":"Feroz, M","venue":null,"work_id":"c96bfb60-1a91-43a4-a1d7-2229b3ebb180","year":2009},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.327851Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:1c1b0ff5fafe8e6fb12a1f7c648a7c3ff1cf783dc8584ffa5bf7781d3518b791","observation_id":"240b5958-d01d-43d4-88dc-39b205ebee3a","resolution":{"observed_at":"2026-08-06T18:27:05.057035Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.034951Z","title":"corner.py: Scatterplot matrices in python","venue":null,"work_id":"1e519dc8-b484-4b68-9303-180ad96ae016","year":2016},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.392912Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:90b49692aff6bd219a31d479be7e33f87860bc9023a7df1c2b1f117cd04a9ca2","observation_id":"96f87584-05ab-4fcc-ac0a-b7ab765a6e19","resolution":{"observed_at":"2026-08-06T18:27:05.040284Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.935783Z","title":"The values of θs and its uncertainty, along with a calculated DA were used in the probability of acceptance in the MCMC analysis, with constraints 0 < f < 1 and zc > 1100","venue":null,"work_id":"65a7a848-cedd-4ea7-92c0-dc0a55517d8f","year":null},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.256450Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:e25642a0edc177ecec8f5d2538d53aff8cae941a74d12ff874c689638e980bbf","observation_id":"70140696-a4f8-4b6f-80b8-9c1ae012f7e6","resolution":{"observed_at":"2026-08-06T18:27:06.008958Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.00746","last_updated":"2023-10-17T19:53:44Z","snapshot_observed_at":"2026-08-09T16:24:55.014971Z","submitted_at":"2023-03-01T18:59:00Z","title":"Canonical Hubble-Tension-Resolving Early Dark Energy Cosmologies are Inconsistent with the Lyman-$\\alpha$ Forest","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.00746","snapshot_observed_at":"2026-08-06T18:26:58.508074Z","title":"Colin Hill, Vid Irˇ siˇ c, and Blake D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.508074Z"},"links":{"cited_paper":"/paper/2303.00746","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:3ea209c87085569f77d3b007ce4c8b3e291b72b099b5aca29a79f080c2afa42f","observation_id":"a8e24222-735f-49cd-b38f-37a49890eb50","resolution":{"observed_at":"2026-08-06T18:26:58.508074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.04644","last_updated":"2023-07-13T17:41:20Z","snapshot_observed_at":"2026-08-09T08:05:40.029064Z","submitted_at":"2023-02-09T13:57:11Z","title":"Can neutrino-assisted early dark energy models ameliorate the $H_0$ tension in a natural way?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.04644","snapshot_observed_at":"2026-08-06T18:26:58.160601Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.160601Z"},"links":{"cited_paper":"/paper/2302.04644","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:ee663109133b312c8ff7e4653acf65609e836e4aa87ee073ab4738265cbddd56","observation_id":"91bba2e7-c963-4a4a-a4be-f23807ae45a2","resolution":{"observed_at":"2026-08-06T18:26:58.160601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.067632Z","title":"COLOSSUS: A Python Toolkit for Cosmology, Large-scale Structure, and Dark Matter Halos","venue":null,"work_id":"c0b43d06-7f3b-492e-96c4-ef6832327e5c","year":2018},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.234963Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:bba3a1385e1f74dd3ad61f558226f8f7cd2d683a2428043f15da30bd59c83332","observation_id":"251d1757-ea47-4c37-b78a-1cfe23cceb48","resolution":{"observed_at":"2026-08-06T18:27:05.072660Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:06.071843Z","title":"This is in tension with the value of H0 derived from SNIa observations, which is H0 = 73.30 ± 1.04 km s −1 Mpc−1 [37]","venue":null,"work_id":"d0fe86b7-b62c-47ae-914a-336cd2fc3cd1","year":2000},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.160242Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:899172b7b960d841add769f396e41751703c6fc64e52f0afdcf43c4343ce187d","observation_id":"7c3226fd-a532-4388-89a9-de364923a624","resolution":{"observed_at":"2026-08-06T18:27:06.076807Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.14802","last_updated":"2024-05-06T12:13:27Z","snapshot_observed_at":"2026-08-04T17:24:21.885351Z","submitted_at":"2023-07-27T12:12:13Z","title":"The state of the dark energy equation of state circa 2023","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.14802","snapshot_observed_at":"2026-08-06T18:26:58.274568Z","title":"Escamilla, William Giar` e, Eleonora Di Valentino, Rafael C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.274568Z"},"links":{"cited_paper":"/paper/2307.14802","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:e4d11896f2086103089d71b91a8bd88216687e614787226c5ad99ddf1e19ae0d","observation_id":"fd183383-5156-4cbe-a9c7-20bd1f7c0f14","resolution":{"observed_at":"2026-08-06T18:26:58.274568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.15369","last_updated":"2023-08-30T08:24:11Z","snapshot_observed_at":"2026-08-06T02:48:25.532692Z","submitted_at":"2023-03-27T16:35:37Z","title":"Constraint on Early Dark Energy from Isotropic Cosmic Birefringence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.15369","snapshot_observed_at":"2026-08-06T18:26:58.297275Z","title":"Eskilt, Laura Herold, Eiichiro Komatsu, Kai Murai, Toshiya Namikawa, and Fumihiro Naokawa","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.297275Z"},"links":{"cited_paper":"/paper/2303.15369","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:757f5c60f12850ef323dc42c664c8e0246b488ac61ec167f74d76f5019b60078","observation_id":"71b55359-9ec2-4f9b-854d-41379d1f4c94","resolution":{"observed_at":"2026-08-06T18:26:58.297275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.925039Z","title":"Toward early dark energy and n s=1 with P l a n c k , ACT, and SPT observations","venue":null,"work_id":"2e2440e4-9a8b-44ab-8cc7-22aebeaa6b85","year":2022},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.885718Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:2a65c4b628c5ae9cf0687d23415c2a51731b2c225f87d1b5623d2a2c04be6bc1","observation_id":"1030c871-1bf4-4838-8723-f641bd6d02a3","resolution":{"observed_at":"2026-08-06T18:27:04.929924Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.017326Z","title":"Hogg, Dustin Lang, and Jonathan Goodman","venue":null,"work_id":"97333414-a350-435c-8db1-d0ef1b61eb02","year":2013},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.456049Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:6caf5697d3c022b5d7da88d562b77c92201f65587cc615422499b4e4ee0d71f1","observation_id":"c56cc847-ad82-4146-afcc-887f53784976","resolution":{"observed_at":"2026-08-06T18:27:05.022392Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.888581Z","title":"Hubble tension as a guide for refining the early Universe: Cosmologies with explicit local Lorentz and diffeomorphism violation","venue":null,"work_id":"0682a7b0-a529-4ac4-b7c5-51c25ce03348","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.010256Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:ec39dc29e8d809e0582e4117d9550519a3f7671dd91c51290b8dd9de52bb0847","observation_id":"2c3da395-06f1-45e9-8ff4-7d6e4cd809d7","resolution":{"observed_at":"2026-08-06T18:27:04.893501Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:05.000604Z","title":"Harris, K","venue":null,"work_id":"fc6f1b7f-2270-4370-9492-0d12d312f275","year":2020},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.571117Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:f169a82e9b40681cc3ec67b9f32c6c5dd265ccdee65deed6ad420f7589f51a6f","observation_id":"afc05d0d-8ea5-421a-a595-1e1e62f0e2ad","resolution":{"observed_at":"2026-08-06T18:27:05.005664Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.984586Z","title":null,"venue":null,"work_id":"ba669b70-b654-4a7b-9ef2-df2dd7a24d04","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.639481Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:c470ea0cb594297d380ed324fd378fe520bd8b0622f26e03be61b6a5f75b48bd","observation_id":"6c85b707-4277-4904-b0b3-0571fa993094","resolution":{"observed_at":"2026-08-06T18:27:04.989873Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.968473Z","title":"Hinshaw, D","venue":null,"work_id":"a2769972-c3a9-4a59-8978-9a330ba73bbd","year":2013},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.690133Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:7ba6bf927385d458ee70f3b7bfc4724acf46c4e9bbe67aae6d77f7cec0bc41b0","observation_id":"e5ace9ad-f499-478a-a3bd-b65ecdb1868c","resolution":{"observed_at":"2026-08-06T18:27:04.973179Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.950489Z","title":"Hubble Tension: The Evidence of New Physics","venue":null,"work_id":"e88b5955-dda0-4df5-9e15-62f65a78ea05","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.755026Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:7adee9bc68bf8704c2e069d3728f00efb4aa11108fa199614bf482b9e72ecabe","observation_id":"b6dfee78-b01d-4ca3-b0db-5ca59a15d7db","resolution":{"observed_at":"2026-08-06T18:27:04.957187Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:26:58.805213Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.805213Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:c4fe2a3fd88f8aae6066cea996af444c9faf1555d77a54036ee4489147d12dcc","observation_id":"d7a8bcda-03af-4838-b1c5-d7039f25a171","resolution":{"observed_at":"2026-08-06T18:26:58.805213Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.276637Z","title":"Colin Hill, and Wayne Hu","venue":null,"work_id":"e149ef8a-f518-4478-8367-e03e1bb2ed60","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.364759Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:ab94db5b59a1104d55d91f527c6c79ce0455118861f09e10ccb2011e139b6045","observation_id":"a135dd74-bed8-4a59-aea2-a9dffeefc0f8","resolution":{"observed_at":"2026-08-06T18:27:04.314034Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:06.123902Z","title":"They discussed triggers at a microscopic level, either an ultralight scalar field or a dark sector temperature","venue":null,"work_id":"9c1a5f1e-b835-4fd3-97f2-2f3f0f047da1","year":null},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:56.904142Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:291fd5a851790e38934163ebeb40388f93c622f6a7fcd89a036e38d4c5267531","observation_id":"c0802a2b-f586-4058-8917-3e20f073b10f","resolution":{"observed_at":"2026-08-06T18:27:06.129671Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.908193Z","title":null,"venue":null,"work_id":"f3a8dc79-a970-4b63-9800-ec256fc7626e","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:58.977197Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:3959d48510aae163b65c2675112e2a191e2862d236a7472c87d43a687a5ca8bd","observation_id":"6c8d40a4-91aa-4612-9f7b-684c76bcd043","resolution":{"observed_at":"2026-08-06T18:27:04.913486Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.873160Z","title":"joshspeagle/dynesty: v2.1.4, June 2024","venue":null,"work_id":"bf85da8e-3d10-4cd2-b8e0-fc47e6bd8591","year":2024},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.033588Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:c4b5231235d1cb85ed078ab28511e733414a13f72532cab182d62110939533f7","observation_id":"70f9c3a4-4d08-4f25-8fc7-6d30412ccdef","resolution":{"observed_at":"2026-08-06T18:27:04.877480Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.16394","last_updated":"2024-02-11T13:30:53Z","snapshot_observed_at":"2026-07-06T14:24:38.200194Z","submitted_at":"2022-11-29T17:20:17Z","title":"The Hubble tension from the standpoint of quantum cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.16394","snapshot_observed_at":"2026-08-06T18:26:59.096670Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.096670Z"},"links":{"cited_paper":"/paper/2211.16394","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:6933abdc1712b4fd9b9c4977c44aafff08b26c4fd94e2c881a5c0adc64ba5547","observation_id":"42e76a89-b55b-4677-bb3f-5d96263d6698","resolution":{"observed_at":"2026-08-06T18:26:59.096670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.748432Z","title":"What It Takes to Solve the Hubble Tension through Modifications of Cosmological Recombination","venue":null,"work_id":"d27a97e8-e25f-4ee9-9ee3-f17a1b5506d8","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.176818Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:f7b6304707f964f5c32a2d706f6b94ad6f8765c993693eaf6be2b3d7d357c164","observation_id":"4a23415a-d5f4-4049-be25-f2da64a81082","resolution":{"observed_at":"2026-08-06T18:27:04.859946Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.566499Z","title":"Ruchika, Carvalho, and Jailson Alcaniz","venue":null,"work_id":"9f6ecdac-4ca0-42b6-b801-5283daf66183","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.228508Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:0bcecf25bab6fcd33e5a1238d01163b76270f3f6dd7b8fe658d504792a3f15e3","observation_id":"d8da4392-bb9b-4ba2-bf70-e2615d870a3c","resolution":{"observed_at":"2026-08-06T18:27:04.594104Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:06.086955Z","title":"Figure 1 is a simple illustration of various physical models briefly reviewed in Section 1","venue":null,"work_id":"8a5e1634-34cd-42ff-b170-35fae80d7759","year":null},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:57.065992Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:d3d1df5a8974fc58e4358698c887818881c0a365d5e48aa5e1081cca8467f36b","observation_id":"d958f503-3e19-4750-baf2-37d25f61d548","resolution":{"observed_at":"2026-08-06T18:27:06.091994Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.429371Z","title":"CAMB: Code for Anisotropies in the Microwave Background","venue":null,"work_id":"d80ab833-067b-4a49-9665-85aa7edecd53","year":2011},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.298359Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:ab69213f9130421381ae28ed9658d867d06a382e40eb5f0190568abfa7190268","observation_id":"c9dfe20b-1c71-4478-994c-578909033d3f","resolution":{"observed_at":"2026-08-06T18:27:04.512952Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03481","last_updated":"2023-07-07T09:40:01Z","snapshot_observed_at":"2026-08-09T04:52:27.889398Z","submitted_at":"2023-07-07T09:40:01Z","title":"New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.03481","snapshot_observed_at":"2026-08-06T18:26:59.449208Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.449208Z"},"links":{"cited_paper":"/paper/2307.03481","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:6a1d8b04b39771ab7e90151e2eaa3998fda8e100d6f89f6960b18ce57ec5cf11","observation_id":"b3b8bc49-b13b-4b67-bba6-54b3f426cf2f","resolution":{"observed_at":"2026-08-06T18:26:59.449208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.118296Z","title":"Odintsov, V","venue":null,"work_id":"027cb10d-5765-45ea-924e-44dc9b9906d2","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.499339Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:57090eceae492a952672df0c6f6747ed10e46e9e39e73fe5762a169fbc729311","observation_id":"ccf4b556-a1e5-4b19-9f3c-fd216473da5b","resolution":{"observed_at":"2026-08-06T18:27:04.221003Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:04.004689Z","title":"Odintsov, Diego S´ aez-Chill´ on G´ omez, and German S","venue":null,"work_id":"12f74099-ca00-402c-a97b-f29cd0149ac1","year":2021},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.540659Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:914e7ce13f8182c05a50b7ee2aca44fcb158016b8c8b821d6ae51cd13bd679b6","observation_id":"cf53c73b-68a4-40c8-bf51-f877c5cca703","resolution":{"observed_at":"2026-08-06T18:27:04.030778Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:03.810963Z","title":"Planck 2018 results","venue":null,"work_id":"34141687-3617-482f-a8c7-49503c5cf91d","year":2018},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.667180Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:9a2f3d3b8e29c777386673ff89df1f2ca35bcceac1cf93d3c3d785a53843976a","observation_id":"8dc02e18-dc61-4cdb-89dd-43aaed8e99ff","resolution":{"observed_at":"2026-08-06T18:27:03.885111Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09032","last_updated":"2023-10-11T16:29:49Z","snapshot_observed_at":"2026-08-06T15:14:38.094991Z","submitted_at":"2023-02-17T17:57:56Z","title":"The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.09032","snapshot_observed_at":"2026-08-06T18:26:59.751326Z","title":"Smith, and Tanvi Karwal","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.751326Z"},"links":{"cited_paper":"/paper/2302.09032","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:5b5229aa82db179adde2251628ede472b44f4fe797aaec5cf6937abed041a92e","observation_id":"956bad7e-51ef-432a-843f-d0442a894154","resolution":{"observed_at":"2026-08-06T18:26:59.751326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:03.630163Z","title":"Smith, and Tanvi Karwal","venue":null,"work_id":"30953dd0-297d-4eae-b1cd-af5b788973ff","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.851351Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:d214ca551413e51a8a1609bd36a5e076e8449dc26d94bb3ba9908a54693d3909","observation_id":"edc26784-1f33-4fbf-be74-5c9be68a55f4","resolution":{"observed_at":"2026-08-06T18:27:03.689659Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:03.418602Z","title":"Riess, Wenlong Yuan, Lucas M","venue":null,"work_id":"24bd2a73-71ba-4ecf-9fc2-3cacad34dc0e","year":2022},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T18:26:59.975978Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:3f82dcb228a58b48f05a471a07b7dd1e0335255c82b8724b0afe7e5cea90a6ff","observation_id":"efcf6428-1ba4-4e91-93e3-4a60a1b4c465","resolution":{"observed_at":"2026-08-06T18:27:03.542246Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:03.187125Z","title":"Nested Sampling","venue":null,"work_id":"52168c83-23c5-4999-905c-673579982d50","year":2004},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.081548Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:d6c53473b0d7ec32e3236a468eda84fe537ac3833b6cd735306acd3c9be17a9c","observation_id":"c3d7dde4-a269-4c55-9aa1-b87d155f066f","resolution":{"observed_at":"2026-08-06T18:27:03.317178Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:02.970305Z","title":"Nested sampling for general Bayesian computation","venue":null,"work_id":"ee51b80e-f06d-46e8-8d31-f3a95f28afab","year":2006},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.085994Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:97a4dfd9f9be768dcb05e916a6f446aa8db0292d392aef675185592d84d2fd58","observation_id":"5c0d8115-2fa5-444a-a5a4-8d29c5f1d158","resolution":{"observed_at":"2026-08-06T18:27:03.091420Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:02.817808Z","title":null,"venue":null,"work_id":"26628366-83fb-4b4b-b534-98677da295b9","year":2020},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.125486Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:61be896ddc0deba086b298891d629610bc2236b8131b0cbf49241d9f4b25da1b","observation_id":"8f0b36ae-50d0-45df-99c6-230ec742115b","resolution":{"observed_at":"2026-08-06T18:27:02.895019Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.00454","last_updated":"2023-06-01T08:53:26Z","snapshot_observed_at":"2026-07-06T15:36:26.422696Z","submitted_at":"2023-06-01T08:53:26Z","title":"Impact of big bang nucleosynthesis on the H0 tension","version":1},"cited_work":{"arxiv_id":"2306.00454","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.00454","snapshot_observed_at":"2026-08-06T18:27:01.177498Z","title":"Impact of big bang nucleosynthesis on the H0 tension","venue":"astro-ph.CO","work_id":"392022ef-01f8-476a-9e46-3e55fdfb2527","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.244530Z"},"links":{"cited_paper":"/paper/2306.00454","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:9f4bccad58f50926d709900eb354c8a0e04764037f125ad1d54d1e10747cd80d","observation_id":"1e0892c0-f0d2-4391-861e-41367d8e7cc4","resolution":{"observed_at":"2026-08-06T18:27:01.260958Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:02.602876Z","title":null,"venue":null,"work_id":"d722140e-5e84-4fb9-8276-84ccb264ef80","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.402918Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:0004be576ddc82fd88c7e27957c8130c1174cf6f43ca37b8763acc4c3e58b712","observation_id":"aa02b7f2-5103-4bb7-993e-5ad9843f8165","resolution":{"observed_at":"2026-08-06T18:27:02.709265Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:02.472622Z","title":"Seven Hints That Early-Time New Physics Alone Is Not Sufficient to Solve the Hubble Tension","venue":null,"work_id":"080de0dd-967f-4367-842e-1a448ff73a27","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.496655Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:727f0dfcff151eed6801bb4a202ce35fe743ed63981dd8604f8e7425dab17dbb","observation_id":"39e8a440-b509-4ba2-81e6-09ac5ed18507","resolution":{"observed_at":"2026-08-06T18:27:02.541014Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:02.309152Z","title":"Oliphant, et al","venue":null,"work_id":"7a398763-cd3e-430e-8d95-6ccb268b6ca1","year":2020},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.596212Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:a1271faef840850cff07c8892796209495496b2d2c9d6ffb9b59490fbb7a756e","observation_id":"2e96f37b-1b3f-4ed5-af95-b2a369dd7cf1","resolution":{"observed_at":"2026-08-06T18:27:02.388885Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.09685","last_updated":"2023-10-25T07:18:40Z","snapshot_observed_at":"2026-08-05T19:28:31.464992Z","submitted_at":"2022-09-20T12:40:11Z","title":"Does the fraction of dark matter diminish with early dark energy?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.09685","snapshot_observed_at":"2026-08-06T18:27:00.674274Z","title":"A fraction of dark matter faded with early dark energy ? arXiv e-prints, page arXiv:2209.09685, September 2022","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.674274Z"},"links":{"cited_paper":"/paper/2209.09685","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:ff59b666bf695160150d830e46da2831d36d22ede6b69abfe059d10d67ab4dcb","observation_id":"1d1649c0-0666-4deb-986a-d84ff2ede0d7","resolution":{"observed_at":"2026-08-06T18:27:00.674274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T18:27:02.103009Z","title":"Testing dark energy after pre-recombination early dark energy","venue":null,"work_id":"c4e4c0af-40f9-4c79-a563-f4f8547b6c53","year":2022},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.751675Z"},"links":{"citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:a358d9ea535ce2614f623bbca32fd8475eafb5604ca2023ccc4d005c87550216","observation_id":"cd955db5-103f-4387-a36b-3beb01713c1b","resolution":{"observed_at":"2026-08-06T18:27:02.193288Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.18873","last_updated":"2023-09-13T08:05:02Z","snapshot_observed_at":"2026-07-06T15:35:19.167704Z","submitted_at":"2023-05-30T09:12:00Z","title":"Shape of CMB lensing in the early dark energy cosmology","version":3},"cited_work":{"arxiv_id":"2305.18873","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.18873","snapshot_observed_at":"2026-08-06T18:27:00.929032Z","title":"Shape of CMB lensing in the early dark energy cosmology","venue":"astro-ph.CO","work_id":"2e63be99-b2b9-44e4-9308-3f38e2d248d2","year":2023},"citing_paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T18:27:00.803333Z"},"links":{"cited_paper":"/paper/2305.18873","citing_paper":"/paper/2507.08479"},"observation_digest":"sha256:7dc630bdfd9e073eb38d395152e2d225213f108d32c0f363d336de4440da9876","observation_id":"e2a14ad6-a62e-4b9c-9f84-f638e6adbe4c","resolution":{"observed_at":"2026-08-06T18:27:01.049828Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.08479","last_updated":"2025-07-11T10:42:57Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-08T23:59:08.641357Z","submitted_at":"2025-07-11T10:42:57Z","title":"Beyond LambdaCDM: How the Hubble tension challenges early universe physics"},"reference_resolution":{"displayed":55,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":17,"verified_exact":4,"verified_fuzzy":34},"total_outbound_references":55},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 55 of 55 outbound references and 3 inbound Pith citation observations for arXiv:2507.08479."}