{"as_of":"2026-08-16T01:35:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9b6cd09a5abf008d45994626fb6bb4a677d339f254ba5a8d2905b1c2ca86cf5c","coverage":[{"denominator":124,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T15:18:28.526376Z","state":"measured"},{"denominator":109,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":109,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T13:18:39.221110Z","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":"2026-07-02T09:36:50.093976Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-08-12T13:18:39.221110Z","title":"Bertólez-Martínez, I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.16356","last_updated":"2025-04-01T18:58:29Z","snapshot_observed_at":"2026-08-16T00:39:31.806993Z","submitted_at":"2024-11-25T13:10:29Z","title":"New parameter region in sterile neutrino searches: a scenario to alleviate cosmological neutrino mass bound and its testability at oscillation experiments","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T13:18:39.221110Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2411.16356"},"observation_digest":"sha256:a04ba623f66111b0912e5d358ea059f761cdcb130bee819f41c1b53a55a85a0e","observation_id":"b2a6dc35-9bfd-4331-9e60-ab42d4549ef6","resolution":{"observed_at":"2026-08-12T13:18:39.221110Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-08-10T23:18:06.675541Z","title":"Bert´ olez-Mart ´ ınez, I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.20766","last_updated":"2025-03-26T20:06:08Z","snapshot_observed_at":"2026-08-14T23:37:32.755281Z","submitted_at":"2024-12-30T07:30:48Z","title":"Probing Long-Range Forces Between Neutrinos with Cosmic Structures","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T23:18:06.675541Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2412.20766"},"observation_digest":"sha256:17e5f413e1cf40fe807a82c8b48bd15fd9001552f4928cf2cbb8c7d928cae781","observation_id":"0bb3c9bb-cfbd-4698-a001-27f80992c3f0","resolution":{"observed_at":"2026-08-10T23:18:06.675541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-08-10T18:12:34.622123Z","title":"Bertólez-Martínez, I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11571","last_updated":"2025-06-17T07:05:51Z","snapshot_observed_at":"2026-08-10T20:17:39.475166Z","submitted_at":"2025-01-20T16:20:59Z","title":"Illustrating the consequences of a misuse of $\\sigma_8$ in cosmology","version":2},"reference_index":198,"source":"pdf_text","source_observed_at":"2026-08-10T18:12:34.622123Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2501.11571"},"observation_digest":"sha256:86d643705536f74cba02a2c40b52810359cfee6651c0dedbf32bace89605aa4a","observation_id":"489dfcd1-1ad1-4a37-b8de-cfa4d5a4cec1","resolution":{"observed_at":"2026-08-10T18:12:34.622123Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":"2411.14524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-07-02T09:36:50.093976Z","title":"Bert´ olez-Mart´ ınez, I","venue":null,"work_id":"9f1da4d1-559b-4076-846f-3dccd61aafdf","year":2025},"citing_paper":{"arxiv_id":"2503.14744","last_updated":"2025-10-07T13:00:34Z","snapshot_observed_at":"2026-07-06T20:55:04.493800Z","submitted_at":"2025-03-18T21:14:18Z","title":"Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape","version":3},"reference_index":160,"source":"pdf_text","source_observed_at":"2026-05-16T17:46:22.581000Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2503.14744"},"observation_digest":"sha256:a45130971e58b7730f0c4fbec7fe05bc6fc2903c3113aab8f76313278de78e68","observation_id":"41f93d7b-a609-4f7f-b2f6-f4ed668fc907","resolution":{"observed_at":"2026-05-16T17:46:23.270238Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":"2411.14524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-07-02T09:36:50.093976Z","title":"Bert´ olez-Mart´ ınez, I","venue":null,"work_id":"9f1da4d1-559b-4076-846f-3dccd61aafdf","year":2025},"citing_paper":{"arxiv_id":"2601.02077","last_updated":"2026-04-04T13:29:01Z","snapshot_observed_at":"2026-08-14T19:15:34.404775Z","submitted_at":"2026-01-05T12:58:36Z","title":"Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-16T18:00:59.984076Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2601.02077"},"observation_digest":"sha256:49ad59c0b4aa6f42a1559cd5c328de4be4347fbe7fafd425718700d2bf444c7e","observation_id":"0d9f1632-83aa-45a8-b77d-2d1a12f55157","resolution":{"observed_at":"2026-05-16T18:01:09.274019Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-08-02T19:14:23.662659Z","title":"Bert´ olez-Mart ´ ınez, I","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.03284","last_updated":"2026-06-08T15:46:11Z","snapshot_observed_at":"2026-08-06T18:27:37.693141Z","submitted_at":"2026-03-03T18:59:58Z","title":"Neutrino mass limits and decaying dark matter: background evolution versus perturbations","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-02T19:14:23.662659Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2603.03284"},"observation_digest":"sha256:4c6a10f0c680033208ac0bbdfbd938b0df9cbbed748cc4ce9a8a6e82c31c44d6","observation_id":"55ba86dc-7606-421c-912d-daf33e1f0417","resolution":{"observed_at":"2026-08-02T19:14:23.662659Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":"2411.14524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-07-02T09:36:50.093976Z","title":"Bert´ olez-Mart´ ınez, I","venue":null,"work_id":"9f1da4d1-559b-4076-846f-3dccd61aafdf","year":2025},"citing_paper":{"arxiv_id":"2605.28923","last_updated":"2026-05-27T18:00:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-27T18:00:00Z","title":"A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-29T11:15:53.860139Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2605.28923"},"observation_digest":"sha256:1cfb8fe4750f473e5bf93922e8b2b1697016774f71462317baae9157bf820208","observation_id":"68cd9f4f-f00e-49e9-af1b-ab0f7714334f","resolution":{"observed_at":"2026-06-29T11:23:21.736426Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":"2411.14524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-07-02T09:36:50.093976Z","title":"Bert´ olez-Mart´ ınez, I","venue":null,"work_id":"9f1da4d1-559b-4076-846f-3dccd61aafdf","year":2025},"citing_paper":{"arxiv_id":"2606.05291","last_updated":"2026-06-03T18:00:04Z","snapshot_observed_at":"2026-07-06T23:45:19.055840Z","submitted_at":"2026-06-03T18:00:04Z","title":"The Future of Lepton Flavor","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-06-28T05:25:55.116276Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2606.05291"},"observation_digest":"sha256:5cc5b0bc17183aa0ef54f652e6e7f184673de9b898364020392cc7e729f0808a","observation_id":"4b5b2bf6-525d-4ab1-b891-2a4c47a0966e","resolution":{"observed_at":"2026-07-02T09:36:50.095603Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14524","snapshot_observed_at":"2026-07-31T11:14:46.730070Z","title":"Origin of cosmological neutrino mass bounds: background versus perturbations","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28326","last_updated":"2026-07-30T14:57:39Z","snapshot_observed_at":"2026-08-08T20:27:05.702904Z","submitted_at":"2026-07-30T14:57:39Z","title":"Growth, geometry, and early-universe split of the matter density parameter $\\Omega_{\\rm m}$","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-07-31T11:14:46.730070Z"},"links":{"cited_paper":"/paper/2411.14524","citing_paper":"/paper/2607.28326"},"observation_digest":"sha256:3182673e2b55b249767f07e9db8d18bfc5a62e110656d1358f4d5a9dc176ad3a","observation_id":"a736548e-0bbd-4339-9c03-19620a994604","resolution":{"observed_at":"2026-07-31T11:14:46.730070Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2411.14524/citation-record","integrity":"/paper/2411.14524/integrity","json":"/paper/2411.14524/citation-record.json","paper":"/paper/2411.14524"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2006.11237","last_updated":"2021-01-19T09:50:37Z","snapshot_observed_at":"2026-08-12T17:30:15.613475Z","submitted_at":"2020-06-19T17:21:48Z","title":"2020 Global reassessment of the neutrino oscillation picture","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.11237","snapshot_observed_at":"2026-08-12T15:18:26.205162Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.205162Z"},"links":{"cited_paper":"/paper/2006.11237","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:d4ab35be64a71974ced57318caaf5f6ff66de112bf3b9869d61989f406b7bfb4","observation_id":"da6248b6-cd19-4466-a059-0d6a476881ab","resolution":{"observed_at":"2026-08-12T15:18:26.205162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05380","last_updated":"2025-10-28T13:33:51Z","snapshot_observed_at":"2026-08-13T20:34:18.192890Z","submitted_at":"2024-10-07T18:00:02Z","title":"NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05380","snapshot_observed_at":"2026-08-12T15:18:26.210807Z","title":"Esteban, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.210807Z"},"links":{"cited_paper":"/paper/2410.05380","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:3f10e0b482d4e52ac4c2e79857ec239e30c5a3a74d47d6a56a27604ffb24457d","observation_id":"7b89029a-9373-4151-9be4-c2909ee063c1","resolution":{"observed_at":"2026-08-12T15:18:26.210807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.00532","last_updated":"2021-09-28T14:23:27Z","snapshot_observed_at":"2026-08-14T17:26:56.364833Z","submitted_at":"2021-07-01T15:24:24Z","title":"The unfinished fabric of the three neutrino paradigm","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.00532","snapshot_observed_at":"2026-08-12T15:18:26.215298Z","title":"Capozzi, E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.215298Z"},"links":{"cited_paper":"/paper/2107.00532","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:54158c86e09fb0c5ed849b96171dc3fb73ad75c5ec36dad287e0cef64dbd9cdc","observation_id":"a4e32049-4bfc-4f78-bcbb-9473c7ab0dd0","resolution":{"observed_at":"2026-08-12T15:18:26.215298Z","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":"2026-08-12T15:18:26.221646Z","title":"Abe et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.221646Z"},"links":{"citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:292483e2d66783ccc7150cb710aa2758708c4fa0dd7d0ea76d8ae1c8a7f7e126","observation_id":"b1a17b02-465b-4616-95f9-9a53b78f7c37","resolution":{"observed_at":"2026-08-12T15:18:26.221646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.08219","last_updated":"2022-08-08T18:53:56Z","snapshot_observed_at":"2026-08-09T23:21:30.226221Z","submitted_at":"2021-08-18T16:06:47Z","title":"An Improved Measurement of Neutrino Oscillation Parameters by the NOvA Experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.08219","snapshot_observed_at":"2026-08-12T15:18:26.226091Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.226091Z"},"links":{"cited_paper":"/paper/2108.08219","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:e7382423a72f227540f11f9d9823c04a19f2205533230af92b61e6e8badabd56","observation_id":"8a858a7a-004c-4b1e-b76a-df0243806dfe","resolution":{"observed_at":"2026-08-12T15:18:26.226091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.05613","last_updated":"2015-10-18T19:39:47Z","snapshot_observed_at":"2026-08-14T22:39:43.005777Z","submitted_at":"2015-07-20T19:18:45Z","title":"Neutrino Physics with JUNO","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.05613","snapshot_observed_at":"2026-08-12T15:18:26.231438Z","title":"An et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.231438Z"},"links":{"cited_paper":"/paper/1507.05613","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:a7031cd80081fe295f120792da942cbbf5fd1fca6e8892fe665a73e7d8236eb6","observation_id":"7816e3e6-df7b-48dc-9557-b3df4de0282c","resolution":{"observed_at":"2026-08-12T15:18:26.231438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.04163","last_updated":"2018-11-28T18:17:02Z","snapshot_observed_at":"2026-08-14T19:17:12.629864Z","submitted_at":"2018-05-09T14:24:05Z","title":"Hyper-Kamiokande Design Report","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.04163","snapshot_observed_at":"2026-08-12T15:18:26.236564Z","title":"Abe et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.236564Z"},"links":{"cited_paper":"/paper/1805.04163","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:350fc970037a0e3804abdf19a5dd19c4323df6d9ff9ec1ee571afb76d5ce474c","observation_id":"89fb149b-f5fd-4c61-94a2-79a390bbdbe2","resolution":{"observed_at":"2026-08-12T15:18:26.236564Z","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":"2026-08-12T15:18:26.241719Z","title":"Abi et al","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.241719Z"},"links":{"citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:84fd60b8683cc7d3b1c1781f0d15d04bf6081241f35f272ec311de8b61dcb770","observation_id":"69155af1-0355-483e-bafe-488ae371a9f6","resolution":{"observed_at":"2026-08-12T15:18:26.241719Z","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":"2026-08-12T15:18:26.246991Z","title":"Aker et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.246991Z"},"links":{"citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:9aeed42892cc5b61dc0e40d156ec01756f5969cca4f7086a7996447e73c132de","observation_id":"ddb7eefc-c46c-4108-8bc6-4e83806d3cc1","resolution":{"observed_at":"2026-08-12T15:18:26.246991Z","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":"2026-08-12T15:18:26.251855Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.251855Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:26ad7f8d07cee3916baaefe3e77d1a30ca3b864f539e146fb25ef1e29222f879","observation_id":"e24940a1-0626-4fc2-9eaa-e346eac8cbbf","resolution":{"observed_at":"2026-08-12T15:18:26.251855Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12022","last_updated":"2024-11-21T16:47:10Z","snapshot_observed_at":"2026-07-06T19:52:15.853216Z","submitted_at":"2024-11-18T20:03:35Z","title":"DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12022","snapshot_observed_at":"2026-08-12T15:18:26.296695Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.296695Z"},"links":{"cited_paper":"/paper/2411.12022","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:587a3bfc7af2bb18cc2f364416359596e16d977a66d5eceb5e79fe6cb88b3b0b","observation_id":"954a3874-4d0d-4b7c-8cf6-3f4d0a69ae48","resolution":{"observed_at":"2026-08-12T15:18:26.296695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18047","last_updated":"2025-01-07T13:04:09Z","snapshot_observed_at":"2026-08-12T23:14:52.200350Z","submitted_at":"2024-07-25T13:54:27Z","title":"Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.18047","snapshot_observed_at":"2026-08-12T15:18:26.385759Z","title":"Jiang, W","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.385759Z"},"links":{"cited_paper":"/paper/2407.18047","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:6c3ad24b4646f94b2410a9fcf809bb070066ba0e5e66a752f93d7b0375d02095","observation_id":"18205fa4-9ece-4f75-a796-5a0abe34492b","resolution":{"observed_at":"2026-08-12T15:18:26.385759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.03368","last_updated":"2024-12-13T15:58:40Z","snapshot_observed_at":"2026-08-13T00:14:05.452774Z","submitted_at":"2024-05-06T11:23:31Z","title":"Updating neutrino mass constraints with Background measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.03368","snapshot_observed_at":"2026-08-12T15:18:26.424644Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.424644Z"},"links":{"cited_paper":"/paper/2405.03368","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:328269aec6d5389d3bb4996ddc77546b7c7c7a46b6901ee84db63cb37b925d15","observation_id":"2d38541c-3419-433f-b3ef-790ee2ce12bd","resolution":{"observed_at":"2026-08-12T15:18:26.424644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.13022","last_updated":"2024-11-17T16:25:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-09-19T18:00:26Z","title":"Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.13022","snapshot_observed_at":"2026-08-12T15:18:26.429984Z","title":"Roy Choudhury and T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.429984Z"},"links":{"cited_paper":"/paper/2409.13022","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:8ea912766d1a0b14fd1dfeac2255b02b6b55173e2758ec06d49d7bb38fb80b70","observation_id":"aa93ac52-7145-4317-a931-8eb4aaf9f674","resolution":{"observed_at":"2026-08-12T15:18:26.429984Z","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":"2026-08-12T15:18:26.434482Z","title":"Archidiacono et al., Euclid preparation","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.434482Z"},"links":{"citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:7db180eecdcc8bc156057e0c9a1b8aae9ed5e02f3a2b1ae6f4cdeda55bc5dd37","observation_id":"ad234d3d-ddc5-4781-9621-6fb99c3d4b33","resolution":{"observed_at":"2026-08-12T15:18:26.434482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00036","snapshot_observed_at":"2026-08-12T15:18:26.443249Z","title":"Aghamousa et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.443249Z"},"links":{"cited_paper":"/paper/1611.00036","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:ea9c6ade92601235167ce2da611c00159175763677b826ad2a173c20ed6d80d5","observation_id":"ff0e9405-5fc2-489a-92a8-418f2aa0e21e","resolution":{"observed_at":"2026-08-12T15:18:26.443249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.07445","last_updated":"2019-03-01T10:51:03Z","snapshot_observed_at":"2026-08-15T01:11:26.803228Z","submitted_at":"2018-08-22T17:19:17Z","title":"The Simons Observatory: Science goals and forecasts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.07445","snapshot_observed_at":"2026-08-12T15:18:26.448965Z","title":"Ade et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.448965Z"},"links":{"cited_paper":"/paper/1808.07445","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:dffd37f1e243c7896afa206c0f28ed5cd66d840d47243df9316b52efd9924cc5","observation_id":"b9263146-acc8-41e0-878e-2687d076c440","resolution":{"observed_at":"2026-08-12T15:18:26.448965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.02773","last_updated":"2023-03-27T05:15:34Z","snapshot_observed_at":"2026-08-15T08:54:58.594490Z","submitted_at":"2022-02-06T13:17:44Z","title":"Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.02773","snapshot_observed_at":"2026-08-12T15:18:26.454329Z","title":"Allys et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.454329Z"},"links":{"cited_paper":"/paper/2202.02773","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:94e043afc349f24e074c3d41f0ff7362aa9a5a2142edde625906f1076cc2309a","observation_id":"5f9557f0-aa61-447a-a920-c960d94b1f80","resolution":{"observed_at":"2026-08-12T15:18:26.454329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0505551","last_updated":"2005-10-12T07:32:01Z","snapshot_observed_at":"2026-07-07T00:50:53.931729Z","submitted_at":"2005-05-27T19:54:45Z","title":"Neutrino masses and the dark energy equation of state - relaxing the cosmological neutrino mass bound","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0505551","snapshot_observed_at":"2026-08-12T15:18:26.458677Z","title":"Hannestad, Neutrino masses and the dark energy equation of state - Relaxing the cosmological neutrino mass bound, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.458677Z"},"links":{"cited_paper":"/paper/astro-ph/0505551","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:c4d6d018c56e4b7cc7a42b5e1b228da56d01c7d6515965862093921ef4489e1c","observation_id":"30359be0-fa1d-48e4-9f54-aebe0fb69f02","resolution":{"observed_at":"2026-08-12T15:18:26.458677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.02927","last_updated":"2021-01-14T06:28:12Z","snapshot_observed_at":"2026-08-14T07:08:11.080467Z","submitted_at":"2020-07-06T17:57:03Z","title":"Emergent Dark Energy, neutrinos and cosmological tensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.02927","snapshot_observed_at":"2026-08-12T15:18:26.463656Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.463656Z"},"links":{"cited_paper":"/paper/2007.02927","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:4055aca59801448b12c892e5055f55a7186d4d6aa2dded96aeba05c5137f133e","observation_id":"aae248bb-8e0c-4a98-879a-745402700dd3","resolution":{"observed_at":"2026-08-12T15:18:26.463656Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.08553","last_updated":"2018-09-16T14:07:28Z","snapshot_observed_at":"2026-08-14T19:51:57.968707Z","submitted_at":"2018-01-25T19:00:46Z","title":"Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z) \\geq -1$ are tighter than those obtained in $\\Lambda$CDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.08553","snapshot_observed_at":"2026-08-12T15:18:26.469332Z","title":"Vagnozzi, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.469332Z"},"links":{"cited_paper":"/paper/1801.08553","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:ba86a14ad2de4ba15c5d724ff3677db8aac2dc2c214b2fc518e3f84d1ac29ede","observation_id":"ef5cac44-1c13-441f-b3c9-11f371687172","resolution":{"observed_at":"2026-08-12T15:18:26.469332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.02860","last_updated":"2019-03-29T14:31:18Z","snapshot_observed_at":"2026-08-14T18:54:30.674773Z","submitted_at":"2018-07-08T18:00:11Z","title":"Strong Bounds on Sum of Neutrino Masses in a 12 Parameter Extended Scenario with Non-Phantom Dynamical Dark Energy ($w(z)\\geq -1$)","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.02860","snapshot_observed_at":"2026-08-12T15:18:26.474541Z","title":"Roy Choudhury and A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.474541Z"},"links":{"cited_paper":"/paper/1807.02860","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:76d522565fa1995f75da4691975fe561ebbe27c0322d66772e3d509fd731d5d3","observation_id":"58c3ad1a-6015-410e-a03a-f6121a173073","resolution":{"observed_at":"2026-08-12T15:18:26.474541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05167","last_updated":"2022-08-23T03:03:10Z","snapshot_observed_at":"2026-08-13T15:06:47.394151Z","submitted_at":"2022-07-11T20:04:34Z","title":"Model marginalized constraints on neutrino properties from cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05167","snapshot_observed_at":"2026-08-12T15:18:26.484345Z","title":"di Valentino, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.484345Z"},"links":{"cited_paper":"/paper/2207.05167","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:6b9553a7445f9414f0d3b25d17b84fcdcd66895f533879be52c6d9b1bd49e91a","observation_id":"b47704bf-41fb-4ff6-996e-ed5f9b90536c","resolution":{"observed_at":"2026-08-12T15:18:26.484345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01219","last_updated":"2017-05-08T09:15:14Z","snapshot_observed_at":"2026-08-14T21:45:35.562658Z","submitted_at":"2016-08-03T15:12:23Z","title":"Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\\Lambda$CDM cosmology","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01219","snapshot_observed_at":"2026-08-12T15:18:26.584595Z","title":"Zhao, Y.-H","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.584595Z"},"links":{"cited_paper":"/paper/1608.01219","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:4071a1c9cf51b1ea4b4869d7376cf7e371104be8bdce1fde1deafe6fe2673dc2","observation_id":"7b915614-0b7b-493b-ab10-ab1fc035724d","resolution":{"observed_at":"2026-08-12T15:18:26.584595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.02651","last_updated":"2016-04-21T12:59:56Z","snapshot_observed_at":"2026-08-14T22:24:16.586781Z","submitted_at":"2015-11-09T12:07:35Z","title":"Impacts of dark energy on weighing neutrinos after Planck 2015","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.02651","snapshot_observed_at":"2026-08-12T15:18:26.662109Z","title":"Zhang, Impacts of dark energy on weighing neutrinos after Planck 2015 , Phys","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.662109Z"},"links":{"cited_paper":"/paper/1511.02651","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:43784937929657291150e19100139143a4e2cace4987ec7838d3a73fa8c8ceaa","observation_id":"53417b94-f64b-4c14-ab69-e203fb8bdbfe","resolution":{"observed_at":"2026-08-12T15:18:26.662109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.06910","last_updated":"2018-08-29T09:34:37Z","snapshot_observed_at":"2026-08-14T19:34:49.153014Z","submitted_at":"2018-03-19T13:42:10Z","title":"Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.06910","snapshot_observed_at":"2026-08-12T15:18:26.670325Z","title":"Guo, J.-F","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.670325Z"},"links":{"cited_paper":"/paper/1803.06910","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:1ad867279920a4413d6183df2a90ce57f29964e4354d00d60cf475b41ee4dffc","observation_id":"2c7fad74-9a1f-49de-ab0a-5ab66d4b82bb","resolution":{"observed_at":"2026-08-12T15:18:26.670325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.12598","last_updated":"2020-07-15T18:17:09Z","snapshot_observed_at":"2026-08-14T16:00:50.094747Z","submitted_at":"2019-07-29T18:45:46Z","title":"Updated results on neutrino mass and mass hierarchy from cosmology with Planck 2018 likelihoods","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.12598","snapshot_observed_at":"2026-08-12T15:18:26.683528Z","title":"Roy Choudhury and S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.683528Z"},"links":{"cited_paper":"/paper/1907.12598","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:b34287b2640d09ce68669dbbb10bec119d1f279502641f3d4a34db19780b33f9","observation_id":"4f597690-7209-488a-be42-41f332649b0c","resolution":{"observed_at":"2026-08-12T15:18:26.683528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.4071","last_updated":"2012-06-11T08:05:56Z","snapshot_observed_at":"2026-08-15T04:18:56.202756Z","submitted_at":"2012-02-18T11:47:51Z","title":"Constraining dynamical dark energy with a divergence-free parametrization in the presence of spatial curvature and massive neutrinos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.4071","snapshot_observed_at":"2026-08-12T15:18:26.696921Z","title":"Li and X","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.696921Z"},"links":{"cited_paper":"/paper/1202.4071","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:a27164ca118a7d8af34b4c9dfe09c2a94df24cd3e52c369f802a37ff6b33eb8b","observation_id":"041e1fe6-300f-4ee7-b2ac-ebd9d42b7c01","resolution":{"observed_at":"2026-08-12T15:18:26.696921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6679","last_updated":"2013-01-29T14:13:31Z","snapshot_observed_at":"2026-08-15T00:51:48.882102Z","submitted_at":"2012-07-28T02:45:45Z","title":"Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.6679","snapshot_observed_at":"2026-08-12T15:18:26.709053Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.709053Z"},"links":{"cited_paper":"/paper/1207.6679","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:2aa907bf40f5e93fb1bcc8b91f5e842322b0dae176eb89de057e45503c68d44d","observation_id":"2d16362a-ec1b-4f7a-ba65-5f5bf0435cde","resolution":{"observed_at":"2026-08-12T15:18:26.709053Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.3598","last_updated":"2014-07-21T08:51:00Z","snapshot_observed_at":"2026-08-14T23:37:35.734702Z","submitted_at":"2014-04-14T14:50:10Z","title":"Cosmological constraints on neutrinos after BICEP2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.3598","snapshot_observed_at":"2026-08-12T15:18:26.714825Z","title":"Zhang, Y.-H","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.714825Z"},"links":{"cited_paper":"/paper/1404.3598","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:25bc855fa1341e2b8a6a82f4ed29926a37b018114d9aa20f4bb0b4f82dc13b01","observation_id":"63c39db1-669f-4abf-b00c-f082cc5720e8","resolution":{"observed_at":"2026-08-12T15:18:26.714825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.04028","last_updated":"2015-03-27T01:17:44Z","snapshot_observed_at":"2026-08-14T23:00:07.311322Z","submitted_at":"2015-02-13T15:32:06Z","title":"Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.04028","snapshot_observed_at":"2026-08-12T15:18:26.719641Z","title":"Zhang, M.-M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.719641Z"},"links":{"cited_paper":"/paper/1502.04028","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:1468e55955ca6ba73a2c25fba22423b842cb51f1d590263fc87d8e7c1837142d","observation_id":"8856d5c8-ed64-4857-a5d8-fb09730d475a","resolution":{"observed_at":"2026-08-12T15:18:26.719641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.08141","last_updated":"2016-01-12T12:29:37Z","snapshot_observed_at":"2026-08-14T22:50:26.387446Z","submitted_at":"2015-04-30T09:38:52Z","title":"Observational constraints on varying neutrino-mass cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.08141","snapshot_observed_at":"2026-08-12T15:18:26.724766Z","title":"Geng, C.-C","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.724766Z"},"links":{"cited_paper":"/paper/1504.08141","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:feae08f6fea404e57ba711619b3e4efeb701faad93387d7e2b3045b297941bd1","observation_id":"4697bac2-ca93-46b9-bad2-38f9fbfd3db9","resolution":{"observed_at":"2026-08-12T15:18:26.724766Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.02008","last_updated":"2015-12-11T07:41:29Z","snapshot_observed_at":"2026-08-14T22:41:21.510899Z","submitted_at":"2015-07-08T02:59:41Z","title":"Galaxy clustering, CMB and supernova data constraints on $\\phi$CDM model with massive neutrinos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.02008","snapshot_observed_at":"2026-08-12T15:18:26.729137Z","title":"Chen and L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.729137Z"},"links":{"cited_paper":"/paper/1507.02008","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:d4d0b369ff9eb81a895cef8cf0f009de6f79be5f27dbbdf5de60ce6525a2a648","observation_id":"06e4e115-fcc5-4b2e-9b72-7d5ab4634ace","resolution":{"observed_at":"2026-08-12T15:18:26.729137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.02578","last_updated":"2019-08-27T13:26:18Z","snapshot_observed_at":"2026-08-14T18:03:11.234838Z","submitted_at":"2018-11-06T19:00:05Z","title":"Upper Bound of Neutrino Masses from Combined Cosmological Observations and Particle Physics Experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.02578","snapshot_observed_at":"2026-08-12T15:18:26.734133Z","title":"Loureiro et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.734133Z"},"links":{"cited_paper":"/paper/1811.02578","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:a00345e7d42d2b16466c9ac07641ba9ae3f0e61d9475cc823908d84cd6f2e2b2","observation_id":"14bc9692-9585-4f85-9285-f096428b3443","resolution":{"observed_at":"2026-08-12T15:18:26.734133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.00672","last_updated":"2016-10-10T08:31:12Z","snapshot_observed_at":"2026-08-14T21:45:51.074230Z","submitted_at":"2016-08-02T01:47:53Z","title":"Impacts of dark energy on weighing neutrinos: mass hierarchies considered","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.00672","snapshot_observed_at":"2026-08-12T15:18:26.739334Z","title":"Wang, Y.-F","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.739334Z"},"links":{"cited_paper":"/paper/1608.00672","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5ba12254869a91d22664fc219755bd171ae3555eabb5cb62ad0bd6d137331d03","observation_id":"cfa6e6a0-2a84-4ff5-a832-c7c5fe082d8f","resolution":{"observed_at":"2026-08-12T15:18:26.739334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.02556","last_updated":"2017-06-01T15:18:10Z","snapshot_observed_at":"2026-08-14T21:13:01.623036Z","submitted_at":"2017-03-07T19:02:00Z","title":"Effects of neutrino mass hierarchies on dynamical dark energy models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.02556","snapshot_observed_at":"2026-08-12T15:18:26.744645Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.744645Z"},"links":{"cited_paper":"/paper/1703.02556","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5fde7e396254a9ff75ecfe1b85621dc4ca7715ab4080c61b839b884c40ef8647","observation_id":"5211c675-f4ac-4afd-ada0-a1a3846725cb","resolution":{"observed_at":"2026-08-12T15:18:26.744645Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.05899","last_updated":"2016-03-24T09:37:44Z","snapshot_observed_at":"2026-08-14T22:17:56.645004Z","submitted_at":"2015-12-18T11:10:18Z","title":"Constraints on the neutrino mass and mass hierarchy from cosmological observations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.05899","snapshot_observed_at":"2026-08-12T15:18:26.749619Z","title":"Huang, K","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.749619Z"},"links":{"cited_paper":"/paper/1512.05899","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:92b836110edefdbaedba19ef6688e2e41d62b680d1db2fae441bb24afb664fa5","observation_id":"474620cc-779e-4530-a786-2df7a68fdedf","resolution":{"observed_at":"2026-08-12T15:18:26.749619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.01749","last_updated":"2022-06-19T05:52:29Z","snapshot_observed_at":"2026-08-04T20:25:47.174963Z","submitted_at":"2022-02-03T18:16:40Z","title":"Implications of an extended dark energy model with massive neutrinos","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.01749","snapshot_observed_at":"2026-08-12T15:18:26.780553Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.780553Z"},"links":{"cited_paper":"/paper/2202.01749","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:b772eb63d022361512bf858e3d7e14dde42dec5d080de605a1a0b808802d2ce9","observation_id":"5c4fb697-8e15-4f98-b1a5-0c5b2efbe182","resolution":{"observed_at":"2026-08-12T15:18:26.780553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.04647","last_updated":"2020-05-10T12:38:52Z","snapshot_observed_at":"2026-07-06T09:19:05.084387Z","submitted_at":"2020-05-10T12:38:52Z","title":"Impacts of dark energy on constraining neutrino mass after Planck 2018","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.04647","snapshot_observed_at":"2026-08-12T15:18:26.838476Z","title":"Zhang, J.-F","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.838476Z"},"links":{"cited_paper":"/paper/2005.04647","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:a8a18fb2cb0030e15ac178db98a2a0e8ab8a51baabd707b533d7ff5c63eb9eeb","observation_id":"b82339b1-8ca2-4bfe-a5ce-ea44eb723d2c","resolution":{"observed_at":"2026-08-12T15:18:26.838476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.07973","last_updated":"2021-10-25T08:45:35Z","snapshot_observed_at":"2026-08-14T17:46:07.725433Z","submitted_at":"2021-05-17T15:57:46Z","title":"Distinguishing Dark Energy Models with Neutrino Oscillations","version":2},"cited_work":{"arxiv_id":"2105.07973","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.07973","snapshot_observed_at":"2026-08-12T15:18:30.571666Z","title":"Distinguishing Dark Energy Models with Neutrino Oscillations","venue":"astro-ph.CO","work_id":"cbea3691-172d-480d-bb67-03d15e007a36","year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.861680Z"},"links":{"cited_paper":"/paper/2105.07973","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:b5346c582d742ba87ad93748c99721ea216f5b8862f1f5be73be80f6116b86e7","observation_id":"099a147d-d735-431a-b7ab-f3127f4498b7","resolution":{"observed_at":"2026-08-12T15:18:30.577160Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.07115","last_updated":"2016-07-19T09:19:28Z","snapshot_observed_at":"2026-08-14T22:04:50.493268Z","submitted_at":"2016-03-23T10:16:15Z","title":"Constraints on non-flat cosmologies with massive neutrinos after Planck 2015","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.07115","snapshot_observed_at":"2026-08-12T15:18:26.866905Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.866905Z"},"links":{"cited_paper":"/paper/1603.07115","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:cc0445c349a17c51b6ab15dfc4121bdef095f8c31efc052049415bb37f000fa9","observation_id":"dc1eb512-2fb6-4167-ac30-ae53e37cc4ae","resolution":{"observed_at":"2026-08-12T15:18:26.866905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-12T15:18:26.871496Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.871496Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5918c80413debca56f05cf5e3ff0272bfde409e6e149b26964635e3ff38ccf9d","observation_id":"69d856af-a6db-430f-862c-72ac4829a306","resolution":{"observed_at":"2026-08-12T15:18:26.871496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.2154","last_updated":"2012-11-09T15:02:31Z","snapshot_observed_at":"2026-08-15T00:39:54.945843Z","submitted_at":"2012-11-09T15:02:31Z","title":"Testing standard and non-standard neutrino physics with cosmological data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.2154","snapshot_observed_at":"2026-08-12T15:18:26.882567Z","title":"Giusarma, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.882567Z"},"links":{"cited_paper":"/paper/1211.2154","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:3962eca7bc4e8b3633a508928270b70399d9df990c99f2c0218a5cc8efcaed1c","observation_id":"52feb4e7-7bc4-447b-b9a5-953dcc548a88","resolution":{"observed_at":"2026-08-12T15:18:26.882567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.05709","last_updated":"2023-02-11T14:51:33Z","snapshot_observed_at":"2026-08-13T12:46:54.224821Z","submitted_at":"2023-02-11T14:51:33Z","title":"Hubble Tension: The Evidence of New Physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.05709","snapshot_observed_at":"2026-08-12T15:18:26.902261Z","title":"Hu and F.-Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.902261Z"},"links":{"cited_paper":"/paper/2302.05709","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:3b296b5608f4e462d7ed70f9739e8cbebd70482d6d2d5f6311c8a29da42c1cfc","observation_id":"87a3d6b1-4823-4138-99f1-36503580d47f","resolution":{"observed_at":"2026-08-12T15:18:26.902261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.10291","last_updated":"2021-10-15T15:48:33Z","snapshot_observed_at":"2026-08-14T02:04:58.036108Z","submitted_at":"2021-07-21T18:15:15Z","title":"The $H_0$ Olympics: A fair ranking of proposed models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.10291","snapshot_observed_at":"2026-08-12T15:18:26.908383Z","title":"Sch¨ oneberg, G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.908383Z"},"links":{"cited_paper":"/paper/2107.10291","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:24c33b1607a542c7f502cef67534776ea15a722333af805e1918898ab7b31007","observation_id":"4425bc96-80b8-45f5-9090-1548745f00e2","resolution":{"observed_at":"2026-08-12T15:18:26.908383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.02411","last_updated":"2018-03-13T10:20:24Z","snapshot_observed_at":"2026-08-14T20:06:07.269095Z","submitted_at":"2017-12-06T21:16:32Z","title":"The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.02411","snapshot_observed_at":"2026-08-12T15:18:26.913157Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.913157Z"},"links":{"cited_paper":"/paper/1712.02411","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:33d7f33361c1a8237b083d9eb54ecf5f6e699a942872712a810f36d5c9ccc38b","observation_id":"6679f482-741e-4125-95a6-2d0cb8824c2c","resolution":{"observed_at":"2026-08-12T15:18:26.913157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.11696","last_updated":"2019-10-23T00:51:13Z","snapshot_observed_at":"2026-08-14T16:01:52.242754Z","submitted_at":"2019-07-26T17:54:13Z","title":"Hidden Treasures: sterile neutrinos as dark matter with miraculous abundance, structure formation for different production mechanisms, and a solution to the sigma-8 problem","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.11696","snapshot_observed_at":"2026-08-12T15:18:26.917633Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.917633Z"},"links":{"cited_paper":"/paper/1907.11696","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:e50bc5600339e8dd2d1bd0fca2ad3c2402db210946ca0a089c45435751e2ec9a","observation_id":"0e9eb8a0-79ad-4eaf-a0b7-d5e99f2cd593","resolution":{"observed_at":"2026-08-12T15:18:26.917633Z","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":"2026-08-12T15:18:26.923154Z","title":"Abdalla et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.923154Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:cb75b36e829daa08b785b24fd407f6fcb478e5d9a4db08110f92368e92a407b9","observation_id":"d15e81a0-f181-4518-b57a-b2001de6e11b","resolution":{"observed_at":"2026-08-12T15:18:26.923154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-08-15T03:36:47.689228Z","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":"2026-08-12T15:18:26.929467Z","title":"Di Valentino, O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.929467Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:4127fdc294b36a3d43bfff55b41c525ad2a2a9310a6212a25f1dbb94093d83d3","observation_id":"e11b44da-1392-46a3-b6d7-92c97d6f4200","resolution":{"observed_at":"2026-08-12T15:18:26.929467Z","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":"2026-08-15T06:22:52.301428Z","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":"2026-08-12T15:18:26.962952Z","title":"Verde, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:26.962952Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:44a40072363b05dafd721be4ab6ae36ca7e3db36ed857292fd4e8f86e4f00b1d","observation_id":"a6c1611d-881c-48d0-b4b4-c32a2949c1c0","resolution":{"observed_at":"2026-08-12T15:18:26.962952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.13305","last_updated":"2023-11-22T10:53:59Z","snapshot_observed_at":"2026-08-13T05:19:46.612370Z","submitted_at":"2023-11-22T10:53:59Z","title":"A tale of many $H_0$","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.13305","snapshot_observed_at":"2026-08-12T15:18:27.012621Z","title":"Verde, N","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.012621Z"},"links":{"cited_paper":"/paper/2311.13305","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:c67d7f6dcd52ad7210ee98be3f9fd17016d7f79d1b06032ad0e734dc9b6901bc","observation_id":"2efae235-aebd-4618-bff6-7186017b0f29","resolution":{"observed_at":"2026-08-12T15:18:27.012621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11285","last_updated":"2020-10-13T11:11:55Z","snapshot_observed_at":"2026-08-10T13:14:09.209280Z","submitted_at":"2020-08-25T21:41:42Z","title":"Cosmology Intertwined III: $f \\sigma_8$ and $S_8$","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11285","snapshot_observed_at":"2026-08-12T15:18:27.073714Z","title":"Di Valentino et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.073714Z"},"links":{"cited_paper":"/paper/2008.11285","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:39df840f968f007d7db6353f4afe08911d12c9c51b31e2b66533a6a78f5a409e","observation_id":"0556cc26-61b6-4be6-8476-38438b22685b","resolution":{"observed_at":"2026-08-12T15:18:27.073714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.10832","last_updated":"2018-09-11T18:00:48Z","snapshot_observed_at":"2026-08-14T18:58:10.063743Z","submitted_at":"2018-06-28T08:57:29Z","title":"Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.10832","snapshot_observed_at":"2026-08-12T15:18:27.087208Z","title":"Roy Choudhury and S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.087208Z"},"links":{"cited_paper":"/paper/1806.10832","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:779bf9bbcc3b351190da797b698d4e1e68ff067978be79bafe9ca0738ddc6b02","observation_id":"84e8f4e5-8b4d-4eb5-a5c1-1cb9f6986f04","resolution":{"observed_at":"2026-08-12T15:18:27.087208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.02993","last_updated":"2021-12-06T13:12:55Z","snapshot_observed_at":"2026-08-15T15:14:58.391990Z","submitted_at":"2021-12-06T13:12:55Z","title":"Neutrino Mass Bounds in the era of Tension Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.02993","snapshot_observed_at":"2026-08-12T15:18:27.105836Z","title":"Di Valentino and A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.105836Z"},"links":{"cited_paper":"/paper/2112.02993","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:b61ede7d73e9eb04b64494b50093483c6c6c92afe9472f35d7893d57d273ca3e","observation_id":"81916918-b6d9-4b94-83a6-7367f710bdce","resolution":{"observed_at":"2026-08-12T15:18:27.105836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.14204","last_updated":"2023-11-29T18:35:33Z","snapshot_observed_at":"2026-08-14T23:27:51.581351Z","submitted_at":"2023-07-26T14:03:32Z","title":"Lensing impact on cosmic relics and tensions","version":2},"cited_work":{"arxiv_id":"2307.14204","doi":null,"metadata_source":"pith","pith_arxiv_id":"2307.14204","snapshot_observed_at":"2026-08-12T15:18:30.271607Z","title":"Lensing impact on cosmic relics and tensions","venue":"astro-ph.CO","work_id":"b20389e1-e9a0-41cd-b43d-6448ce49c334","year":2023},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.111045Z"},"links":{"cited_paper":"/paper/2307.14204","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:468080978439adab8c6138159c0f58be382860c0675c3b1c29e3131147154664","observation_id":"ee077ace-13b2-4fba-b0ba-efe93e000fdb","resolution":{"observed_at":"2026-08-12T15:18:30.320580Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.00836","last_updated":"2024-05-23T20:18:53Z","snapshot_observed_at":"2026-08-14T18:21:57.032224Z","submitted_at":"2024-05-01T19:48:30Z","title":"No $\\nu$s is Good News","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.00836","snapshot_observed_at":"2026-08-12T15:18:27.116684Z","title":"Craig, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.116684Z"},"links":{"cited_paper":"/paper/2405.00836","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:093460b80416effce622eafc13b689e5bd5eec31284327fec06e6a8b5f3569a1","observation_id":"d8c95e29-637e-47c8-a947-e9a88c96e977","resolution":{"observed_at":"2026-08-12T15:18:27.116684Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07878","last_updated":"2024-07-10T17:46:41Z","snapshot_observed_at":"2026-08-15T03:26:26.559075Z","submitted_at":"2024-07-10T17:46:41Z","title":"The Cosmological Preference for Negative Neutrino Mass","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.07878","snapshot_observed_at":"2026-08-12T15:18:27.122848Z","title":"Green and J","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.122848Z"},"links":{"cited_paper":"/paper/2407.07878","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:a6b829985922b82c144a9873436f23bf848017ab3d87689c996eee6c623708e4","observation_id":"fa0fa3f2-47fe-4e79-b704-6b36304a60ab","resolution":{"observed_at":"2026-08-12T15:18:27.122848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.00090","last_updated":"2024-12-16T21:08:02Z","snapshot_observed_at":"2026-08-14T09:26:12.162316Z","submitted_at":"2024-09-30T18:00:00Z","title":"Massive neutrinos and cosmic composition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.00090","snapshot_observed_at":"2026-08-12T15:18:27.127232Z","title":"Loverde and Z","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.127232Z"},"links":{"cited_paper":"/paper/2410.00090","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:ad362d710ff4e4a4760af1570c69e6a7d9a57dd16b4f89bd53f1897196caf4f6","observation_id":"20ba2403-0c99-4291-910d-e8ff6c73cc74","resolution":{"observed_at":"2026-08-12T15:18:27.127232Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.13831","last_updated":"2024-10-28T14:18:53Z","snapshot_observed_at":"2026-08-12T23:19:11.578633Z","submitted_at":"2024-07-18T18:05:32Z","title":"Living at the Edge: A Critical Look at the Cosmological Neutrino Mass Bound","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.13831","snapshot_observed_at":"2026-08-12T15:18:27.156739Z","title":"Naredo-Tuero, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.156739Z"},"links":{"cited_paper":"/paper/2407.13831","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:dfdc167c1f6138b39c38ec61ea8b00360865eb08188356366bea9631e53f5e94","observation_id":"fc46e258-7c02-4ad3-8b6f-ea9fa2c8b76f","resolution":{"observed_at":"2026-08-12T15:18:27.156739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.14554","last_updated":"2024-12-10T18:58:04Z","snapshot_observed_at":"2026-08-12T23:38:07.448683Z","submitted_at":"2024-06-20T17:58:39Z","title":"Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.14554","snapshot_observed_at":"2026-08-12T15:18:27.234399Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.234399Z"},"links":{"cited_paper":"/paper/2406.14554","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:4dead1287feeabbf41f8a5aa1908f1d81fcc836d56247fa99d91cb2144e90e6e","observation_id":"418d81b4-bf56-4d3d-baf7-6ba05e500b1b","resolution":{"observed_at":"2026-08-12T15:18:27.234399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.11526","last_updated":"2018-06-05T22:06:43Z","snapshot_observed_at":"2026-08-14T19:30:38.793188Z","submitted_at":"2018-03-30T16:09:03Z","title":"Tensions between direct measurements of the lens power spectrum from Planck data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.11526","snapshot_observed_at":"2026-08-12T15:18:27.316285Z","title":"Motloch and W","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.316285Z"},"links":{"cited_paper":"/paper/1803.11526","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:b677adf513930350fc75dea14cf1d092629d0f93dfbc9f71dceb6dfb637876f0","observation_id":"bce3acc0-0565-433e-b958-e56b1fa2fa0f","resolution":{"observed_at":"2026-08-12T15:18:27.316285Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.10034","last_updated":"2023-10-25T13:40:13Z","snapshot_observed_at":"2026-08-13T10:10:37.575056Z","submitted_at":"2023-09-18T18:00:02Z","title":"Cosmological parameters derived from the final (PR4) Planck data release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.10034","snapshot_observed_at":"2026-08-12T15:18:27.357571Z","title":"Tristram et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.357571Z"},"links":{"cited_paper":"/paper/2309.10034","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:10471acb9a6b4519898c9fda51d4166877c31533bfe9182fd146646eb87f72fb","observation_id":"1e7a93a3-28aa-4dd3-8383-dd194a962fab","resolution":{"observed_at":"2026-08-12T15:18:27.357571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.10869","last_updated":"2022-11-11T13:29:22Z","snapshot_observed_at":"2026-08-13T11:09:25.799974Z","submitted_at":"2022-05-22T17:02:55Z","title":"CMB power spectra and cosmological parameters from Planck PR4 with CamSpec","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.10869","snapshot_observed_at":"2026-08-12T15:18:27.364081Z","title":"Rosenberg, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.364081Z"},"links":{"cited_paper":"/paper/2205.10869","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:06b58d508191042ba4abe78f73b58a5bc1c19baa84774202bf4f4a38f9a39702","observation_id":"cc393d53-1926-4701-b223-fbab8bab2782","resolution":{"observed_at":"2026-08-12T15:18:27.364081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.05804","last_updated":"2021-05-11T18:00:00Z","snapshot_observed_at":"2026-08-12T16:17:41.142236Z","submitted_at":"2021-01-14T18:59:59Z","title":"Long Range Interactions in Cosmology: Implications for Neutrinos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.05804","snapshot_observed_at":"2026-08-12T15:18:27.369456Z","title":"Esteban and J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.369456Z"},"links":{"cited_paper":"/paper/2101.05804","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5aed2173afa64d5b9a1d16b49dfa0085d379120ce1bac006f279512f73b4ae44","observation_id":"324a546a-fbbe-4ef9-8a8e-8eea5c19af9f","resolution":{"observed_at":"2026-08-12T15:18:27.369456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04656","last_updated":"2022-10-13T16:15:48Z","snapshot_observed_at":"2026-08-13T16:44:02.068701Z","submitted_at":"2022-02-09T19:00:00Z","title":"Non-standard neutrino cosmology dilutes the lensing anomaly","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04656","snapshot_observed_at":"2026-08-12T15:18:27.374654Z","title":"Esteban, O","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.374654Z"},"links":{"cited_paper":"/paper/2202.04656","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:412788c9d8d2969377999b6856e3f5bc32deef8c41e8904a48a72375fe36bc6b","observation_id":"24a5e9eb-f481-48b1-b7c5-ac37626e211b","resolution":{"observed_at":"2026-08-12T15:18:27.374654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.00534","last_updated":"2019-04-02T14:25:47Z","snapshot_observed_at":"2026-08-14T17:22:11.245313Z","submitted_at":"2019-02-01T19:38:17Z","title":"The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.00534","snapshot_observed_at":"2026-08-12T15:18:27.379790Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.379790Z"},"links":{"cited_paper":"/paper/1902.00534","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5e479a9f3f8ed92ababdcd07d6aca6bb092b6299036a1ded41b21de90ea720e9","observation_id":"98207bcb-38bc-4863-88d2-c86cb2341885","resolution":{"observed_at":"2026-08-12T15:18:27.379790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.07109","last_updated":"2017-12-19T18:50:34Z","snapshot_observed_at":"2026-08-14T20:02:01.982335Z","submitted_at":"2017-12-19T18:50:34Z","title":"Status of neutrino properties and future prospects - Cosmological and astrophysical constraints","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.07109","snapshot_observed_at":"2026-08-12T15:18:27.385946Z","title":"Lattanzi and M","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.385946Z"},"links":{"cited_paper":"/paper/1712.07109","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:49e63c4abbf4246c27fc66c708ae8e5e6a703ccc5701abc5f0376fd683f98e2f","observation_id":"af29986b-4b01-4c8a-a5fc-dc17847263bb","resolution":{"observed_at":"2026-08-12T15:18:27.385946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05275","last_updated":"2020-05-01T01:54:47Z","snapshot_observed_at":"2026-08-05T06:45:21.221188Z","submitted_at":"2019-09-11T18:01:52Z","title":"Cosmological Limits on the Neutrino Mass and Lifetime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05275","snapshot_observed_at":"2026-08-12T15:18:27.391278Z","title":"Chacko, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.391278Z"},"links":{"cited_paper":"/paper/1909.05275","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:4d950d6692dd17a54168ca68093a9635297873ca7c843d27fa30a6338865d3e3","observation_id":"bbb83abc-c94a-4c4a-aed8-c86585865654","resolution":{"observed_at":"2026-08-12T15:18:27.391278Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.08401","last_updated":"2020-02-19T19:28:40Z","snapshot_observed_at":"2026-07-06T08:58:36.557649Z","submitted_at":"2020-02-19T19:28:40Z","title":"Determining the Neutrino Lifetime from Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.08401","snapshot_observed_at":"2026-08-12T15:18:27.396905Z","title":"Chacko, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.396905Z"},"links":{"cited_paper":"/paper/2002.08401","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:cc4b3c4300226269eb5cfa49585a3b582ef822b96a153ce051489421e09da6b4","observation_id":"a30b6802-4107-4a6a-af8b-a9966daaac36","resolution":{"observed_at":"2026-08-12T15:18:27.396905Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.04994","last_updated":"2021-09-03T10:15:10Z","snapshot_observed_at":"2026-08-13T01:56:43.555749Z","submitted_at":"2020-07-09T18:00:01Z","title":"Relaxing Cosmological Neutrino Mass Bounds with Unstable Neutrinos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.04994","snapshot_observed_at":"2026-08-12T15:18:27.402757Z","title":"Escudero, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.402757Z"},"links":{"cited_paper":"/paper/2007.04994","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:1c4affe5f60b6226de1582af1009e42ad206e298e7aa104201163d678fff2613","observation_id":"6136392d-d9a5-4ded-8578-fdbcb7202fb9","resolution":{"observed_at":"2026-08-12T15:18:27.402757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.13862","last_updated":"2022-08-16T18:19:24Z","snapshot_observed_at":"2026-08-09T13:24:18.456822Z","submitted_at":"2021-12-27T19:00:07Z","title":"Improved cosmological constraints on the neutrino mass and lifetime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.13862","snapshot_observed_at":"2026-08-12T15:18:27.407722Z","title":"Franco Abell´ an, Z","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.407722Z"},"links":{"cited_paper":"/paper/2112.13862","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:53d13a929affddbf91230a06d9930eee734b5e28e7e392105f1afcc5f7039be7","observation_id":"c1dd6352-e238-47a8-aad3-bfba028e1aa2","resolution":{"observed_at":"2026-08-12T15:18:27.407722Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.02598","last_updated":"2017-03-31T12:37:15Z","snapshot_observed_at":"2026-08-14T21:26:31.059590Z","submitted_at":"2016-12-08T11:20:00Z","title":"Hiding neutrino mass in modified gravity cosmologies","version":2},"cited_work":{"arxiv_id":"1612.02598","doi":null,"metadata_source":"pith","pith_arxiv_id":"1612.02598","snapshot_observed_at":"2026-08-12T15:18:29.860971Z","title":"Hiding neutrino mass in modified gravity cosmologies","venue":"astro-ph.CO","work_id":"dff61abc-c512-4ecb-8274-a59245d3f17e","year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.413760Z"},"links":{"cited_paper":"/paper/1612.02598","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:e9dd4227c645874350427e7417d91d12981f99db915dadd572cbe9cb13bbe32c","observation_id":"719df777-f90e-4c3f-a981-5b99fb93904d","resolution":{"observed_at":"2026-08-12T15:18:29.957125Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03191","last_updated":"2016-09-28T09:34:05Z","snapshot_observed_at":"2026-08-15T10:33:59.712456Z","submitted_at":"2016-02-09T21:00:41Z","title":"Small neutrino masses from gravitational $\\theta$-term","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1602.03191","snapshot_observed_at":"2026-08-12T15:18:27.475611Z","title":"Dvali and L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.475611Z"},"links":{"cited_paper":"/paper/1602.03191","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:002758447e9a4646dde62d737e943b1dcfe0abb8aa5f0d279feb029822f0bb5b","observation_id":"c28ffb60-09d2-4b97-8077-e7da63531546","resolution":{"observed_at":"2026-08-12T15:18:27.475611Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.01991","last_updated":"2018-12-14T10:19:27Z","snapshot_observed_at":"2026-08-14T18:03:53.972538Z","submitted_at":"2018-11-05T19:32:49Z","title":"Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the $\\Omega_m$-$\\sigma_8$ plane","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.01991","snapshot_observed_at":"2026-08-12T15:18:27.539430Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.539430Z"},"links":{"cited_paper":"/paper/1811.01991","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:17c63586e9e4d66cca7cf755e8dec2099d5ceac1059746545e419898c526b01e","observation_id":"26987842-35bf-45a8-986f-f27451a6f20a","resolution":{"observed_at":"2026-08-12T15:18:27.539430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.02107","last_updated":"2023-08-09T08:02:59Z","snapshot_observed_at":"2026-08-13T17:22:20.416704Z","submitted_at":"2021-12-03T19:00:01Z","title":"Time- and Space-Varying Neutrino Mass Matrix from Soft Topological Defects","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.02107","snapshot_observed_at":"2026-08-12T15:18:27.555668Z","title":"Dvali, L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.555668Z"},"links":{"cited_paper":"/paper/2112.02107","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:e1031ad9a662d8292945f322b2afb68385607b39a8b5ab8b67f54d40c553d6e4","observation_id":"e465e599-5e3a-48f8-8b30-2dd0f5cf61f4","resolution":{"observed_at":"2026-08-12T15:18:27.555668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.13618","last_updated":"2021-11-29T10:14:26Z","snapshot_observed_at":"2026-07-06T10:44:59.832110Z","submitted_at":"2021-02-26T17:38:15Z","title":"Reconstruction of the neutrino mass as a function of redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.13618","snapshot_observed_at":"2026-08-12T15:18:27.561018Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.561018Z"},"links":{"cited_paper":"/paper/2102.13618","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:c46a1c099efc53307ea1716b9845e0469b606bd001b4b31c14249720e3c6dc72","observation_id":"a85b6603-2671-44bf-8ca3-9176a8acb9fa","resolution":{"observed_at":"2026-08-12T15:18:27.561018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01729","last_updated":"2024-06-21T11:48:21Z","snapshot_observed_at":"2026-08-13T13:50:11.354748Z","submitted_at":"2022-11-03T11:42:07Z","title":"A seesaw model for large neutrino masses in concordance with cosmology","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.01729","snapshot_observed_at":"2026-08-12T15:18:27.567389Z","title":"Escudero, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.567389Z"},"links":{"cited_paper":"/paper/2211.01729","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:6bcd535d2d5b7bcf618a95ac873557fbd4a179dfe6a5feb85f710df14031278a","observation_id":"5752a92c-3bb9-411c-b9be-7139df964e68","resolution":{"observed_at":"2026-08-12T15:18:27.567389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.15718","last_updated":"2023-11-10T10:34:41Z","snapshot_observed_at":"2026-08-13T11:08:09.365074Z","submitted_at":"2023-06-27T18:00:01Z","title":"Refractive neutrino masses, ultralight dark matter and cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.15718","snapshot_observed_at":"2026-08-12T15:18:27.606990Z","title":"Sen and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.606990Z"},"links":{"cited_paper":"/paper/2306.15718","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:f7c8639ae59dc2567b250c9441b1e0564f06ffbafd87130bd76e8e994ddac6ee","observation_id":"bb51593c-a199-4e00-8e7c-fa02f01838eb","resolution":{"observed_at":"2026-08-12T15:18:27.606990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.02201","last_updated":"2015-10-08T05:10:47Z","snapshot_observed_at":"2026-08-14T22:29:05.132336Z","submitted_at":"2015-10-08T05:10:47Z","title":"Neutrinos secretly converting to lighter particles to please both KATRIN and the cosmos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.02201","snapshot_observed_at":"2026-08-12T15:18:27.742348Z","title":"Farzan and S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.742348Z"},"links":{"cited_paper":"/paper/1510.02201","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5b6420e14772252174403c167432524a0aa56ff8840c891ec789de0688960a85","observation_id":"1ab4608e-6b06-46b8-b6ca-9608649db052","resolution":{"observed_at":"2026-08-12T15:18:27.742348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.14870","last_updated":"2022-03-08T18:18:16Z","snapshot_observed_at":"2026-08-13T17:25:19.952695Z","submitted_at":"2021-11-29T19:00:03Z","title":"Cosmic Neutrino Background Detection in Large-Neutrino-Mass Cosmologies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.14870","snapshot_observed_at":"2026-08-12T15:18:27.871233Z","title":"Alvey, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.871233Z"},"links":{"cited_paper":"/paper/2111.14870","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:8d6cac70b5bc925ddfcecea9796907ea769f84e7b3dda0c2dbb1df532b89bdd3","observation_id":"7ec518e2-7d3d-4609-a28f-14b16ceaf8be","resolution":{"observed_at":"2026-08-12T15:18:27.871233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.04352","last_updated":"2019-05-29T14:13:17Z","snapshot_observed_at":"2026-08-14T17:31:17.953519Z","submitted_at":"2019-01-14T14:47:18Z","title":"How to relax the cosmological neutrino mass bound","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.04352","snapshot_observed_at":"2026-08-12T15:18:27.896767Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.896767Z"},"links":{"cited_paper":"/paper/1901.04352","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:4e343e1330b5dd5bb8b2685d5bffa0bccfa48bf7cd0a1f06ba795e1bab45d088","observation_id":"38374a1d-f16f-413e-9dfd-64fb6d211ee3","resolution":{"observed_at":"2026-08-12T15:18:27.896767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.12726","last_updated":"2022-03-08T18:15:47Z","snapshot_observed_at":"2026-08-13T17:28:12.035675Z","submitted_at":"2021-11-24T19:00:04Z","title":"What can CMB observations tell us about the neutrino distribution function?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.12726","snapshot_observed_at":"2026-08-12T15:18:27.909349Z","title":"Alvey, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.909349Z"},"links":{"cited_paper":"/paper/2111.12726","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:63c142309ad3ce48ec8c10f5e5d2b93f38b0565a9a6e62e0cc466fabb23ec269","observation_id":"6f6ebba6-5b7d-4e40-b923-ee5f3a15ba35","resolution":{"observed_at":"2026-08-12T15:18:27.909349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0502465","last_updated":"2005-05-10T16:35:09Z","snapshot_observed_at":"2026-07-07T00:48:17.559513Z","submitted_at":"2005-02-22T20:20:50Z","title":"Do observations prove that cosmological neutrinos are thermally distributed?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0502465","snapshot_observed_at":"2026-08-12T15:18:27.915031Z","title":"Cuoco, J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.915031Z"},"links":{"cited_paper":"/paper/astro-ph/0502465","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5fa61d9a6dab7ea69b48286d474837050df66ad05316e50b46626cdadf8a2e48","observation_id":"bcdd9e5a-2f5b-44e3-987d-dc7bf914cf12","resolution":{"observed_at":"2026-08-12T15:18:27.915031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.16822","last_updated":"2024-04-25T17:59:40Z","snapshot_observed_at":"2026-08-14T03:09:16.470835Z","submitted_at":"2024-04-25T17:59:40Z","title":"Cosmological probes of Dark Radiation from Neutrino Mixing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.16822","snapshot_observed_at":"2026-08-12T15:18:27.921791Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.921791Z"},"links":{"cited_paper":"/paper/2404.16822","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:b827c3e051956d3547ed9002bf9a481bed5de21d2bbac88d6de2c66b9fd5781a","observation_id":"19ee7dda-821b-4db3-9ab2-3dc66ced1135","resolution":{"observed_at":"2026-08-12T15:18:27.921791Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.23926","last_updated":"2025-04-19T14:35:15Z","snapshot_observed_at":"2026-08-13T04:10:32.059867Z","submitted_at":"2024-10-31T13:33:51Z","title":"Large neutrino mass in cosmology and keV sterile neutrino dark matter from a dark sector","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.23926","snapshot_observed_at":"2026-08-12T15:18:27.927326Z","title":"Benso, T","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.927326Z"},"links":{"cited_paper":"/paper/2410.23926","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:30b65e38b870a7013bb0e3d4d5c5f4811ffe132f4064a2fbda5c18db3e3c609e","observation_id":"5ad380eb-3892-4142-8c1a-42242295af59","resolution":{"observed_at":"2026-08-12T15:18:27.927326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9508126","last_updated":"2009-07-16T22:05:06Z","snapshot_observed_at":"2026-07-07T01:11:44.541828Z","submitted_at":"1995-08-26T17:15:34Z","title":"Wandering in the Background: A CMB Explorer","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9508126","snapshot_observed_at":"2026-08-12T15:18:27.933529Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.933529Z"},"links":{"cited_paper":"/paper/astro-ph/9508126","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:24501c65cb1cf1bf9852b5fcab708938a431b13870335f3d1afc89c4c23672e0","observation_id":"256213cc-20f5-42c5-ad43-29c01f804e2c","resolution":{"observed_at":"2026-08-12T15:18:27.933529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.5948","last_updated":"2015-02-16T17:29:38Z","snapshot_observed_at":"2026-08-14T23:06:56.957596Z","submitted_at":"2014-12-18T17:10:16Z","title":"Robustness of cosmic neutrino background detection in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":"1412.5948","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.5948","snapshot_observed_at":"2026-08-12T15:18:29.539645Z","title":"Robustness of cosmic neutrino background detection in the cosmic microwave background","venue":"astro-ph.CO","work_id":"6403940f-9747-4e88-96a9-0241427978d6","year":2014},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:27.984261Z"},"links":{"cited_paper":"/paper/1412.5948","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:2f3d5e22e858eb47b392c74b600233f867619dfde8570284da32647266755d70","observation_id":"0e3af853-6c75-4c76-a0a8-d40f9a847000","resolution":{"observed_at":"2026-08-12T15:18:29.623946Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.1740","last_updated":"2014-04-07T10:58:40Z","snapshot_observed_at":"2026-08-14T23:38:25.665894Z","submitted_at":"2014-04-07T10:58:40Z","title":"Neutrino cosmology and Planck","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.1740","snapshot_observed_at":"2026-08-12T15:18:28.111922Z","title":"Lesgourgues and S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.111922Z"},"links":{"cited_paper":"/paper/1404.1740","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:22806872fb8ce29856994a0b46bd16702d6654741ab590e2d10328d122b2a256","observation_id":"b6218a6e-1c46-4cb0-8ff1-d953636abae1","resolution":{"observed_at":"2026-08-12T15:18:28.111922Z","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":"2026-08-12T15:18:28.223915Z","title":"Lesgourgues, G","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.223915Z"},"links":{"citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:138fc234a2dbd66a4f15f8b8b652156187305cc2f447f982ea33c686ce271d5e","observation_id":"9afb3ea6-74a0-453c-aa63-e7c571cd5b01","resolution":{"observed_at":"2026-08-12T15:18:28.223915Z","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":"2026-08-12T15:18:28.247900Z","title":"Bert´ olez-Mart ´ ınez, I","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.247900Z"},"links":{"citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:24d093c3f25af5993d86e23e2c4493e822b7a41725586fd2f8fd0b7b4a300c25","observation_id":"7d53d9cc-2a0c-4784-b15e-7a3789826ee3","resolution":{"observed_at":"2026-08-12T15:18:28.247900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.09678","last_updated":"2018-04-25T16:59:36Z","snapshot_observed_at":"2026-08-15T17:39:47.934259Z","submitted_at":"2018-04-25T16:59:36Z","title":"Current unknowns in the three neutrino framework","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.09678","snapshot_observed_at":"2026-08-12T15:18:28.259386Z","title":"Capozzi, E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.259386Z"},"links":{"cited_paper":"/paper/1804.09678","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:19484129cb41ade24fd769ecd0d50bcc1bfb2d70c1fcea54183fef1c427a27ac","observation_id":"b918814e-8b0d-4caf-9b64-558a9a761fb8","resolution":{"observed_at":"2026-08-12T15:18:28.259386Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9506072","last_updated":"1995-06-11T21:40:56Z","snapshot_observed_at":"2026-07-07T01:11:24.120621Z","submitted_at":"1995-06-11T21:40:56Z","title":"Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9506072","snapshot_observed_at":"2026-08-12T15:18:28.265586Z","title":"Ma and E","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.265586Z"},"links":{"cited_paper":"/paper/astro-ph/9506072","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:8b3b389546e2aaa8a52ec25b49643fc5d58a3a046041aede48c932b95c08d56b","observation_id":"09c6b538-f377-4cf1-bd81-af6701488af7","resolution":{"observed_at":"2026-08-12T15:18:28.265586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410680","last_updated":"2005-01-27T20:41:34Z","snapshot_observed_at":"2026-07-07T00:45:40.229852Z","submitted_at":"2004-10-28T01:31:44Z","title":"Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0410680","snapshot_observed_at":"2026-08-12T15:18:28.271009Z","title":"Hu, Crossing the phantom divide: Dark energy internal degrees of freedom, Phys","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.271009Z"},"links":{"cited_paper":"/paper/astro-ph/0410680","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:9f701c011e89034e299089e8dd1ddb11d67a8bc7dc9d11dd7273973d5ac5faed","observation_id":"28d6eb16-4470-4a49-b336-cc4c20b94a85","resolution":{"observed_at":"2026-08-12T15:18:28.271009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9904176","last_updated":"1999-04-26T15:19:14Z","snapshot_observed_at":"2026-08-15T22:51:56.647120Z","submitted_at":"1999-04-26T15:19:14Z","title":"Perturbations in k-inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9904176","snapshot_observed_at":"2026-08-12T15:18:28.275958Z","title":"Garriga and V","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.275958Z"},"links":{"cited_paper":"/paper/hep-th/9904176","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:5ddac1884f441e0ba4f92e0c81d424ed92b858d84b60960307494980d987cd8d","observation_id":"aeb556ca-bab2-4fc4-9152-98be5c545c7a","resolution":{"observed_at":"2026-08-12T15:18:28.275958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9801234","last_updated":"1998-05-26T17:32:50Z","snapshot_observed_at":"2026-08-13T17:45:15.728089Z","submitted_at":"1998-01-24T16:15:48Z","title":"Structure Formation with Generalized Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9801234","snapshot_observed_at":"2026-08-12T15:18:28.281264Z","title":"Hu, Structure formation with generalized dark matter, Astrophys","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.281264Z"},"links":{"cited_paper":"/paper/astro-ph/9801234","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:a157eeaba7798a7f21dc11a3e34e9d4cf2c494fa77199f413eb1e831961fcee3","observation_id":"d4792643-2e97-4b4c-bfd6-3db26084d529","resolution":{"observed_at":"2026-08-12T15:18:28.281264Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.09580","last_updated":"2023-07-06T21:15:47Z","snapshot_observed_at":"2026-08-13T12:23:08.479624Z","submitted_at":"2023-03-16T18:01:28Z","title":"An accurate fluid approximation for massive neutrinos in cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.09580","snapshot_observed_at":"2026-08-12T15:18:28.286946Z","title":"Nascimento, Accurate fluid approximation for massive neutrinos in cosmology , Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.286946Z"},"links":{"cited_paper":"/paper/2303.09580","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:7ca500f23241c2315e42e4e5882a83e9a1fe684df3937d95f330babfe00bc742","observation_id":"6bcb7cb7-ca29-40ea-a695-08e686026e6d","resolution":{"observed_at":"2026-08-12T15:18:28.286946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2935","last_updated":"2015-10-13T09:17:12Z","snapshot_observed_at":"2026-08-15T04:49:17.510482Z","submitted_at":"2011-04-14T22:10:03Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2935","snapshot_observed_at":"2026-08-12T15:18:28.381752Z","title":"Lesgourgues and T","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.381752Z"},"links":{"cited_paper":"/paper/1104.2935","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:20968116ea5a7e5ac752f60486083764528de38b9891acf606a79b93df3033b1","observation_id":"cd502454-308d-4674-bb77-aff5c1685fa4","resolution":{"observed_at":"2026-08-12T15:18:28.381752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2932","last_updated":"2011-05-14T09:45:16Z","snapshot_observed_at":"2026-08-15T04:49:17.337493Z","submitted_at":"2011-04-14T22:06:14Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2932","snapshot_observed_at":"2026-08-12T15:18:28.458124Z","title":"Lesgourgues, The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview , 1104.2932","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.458124Z"},"links":{"cited_paper":"/paper/1104.2932","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:883f3deec3bbbc6fb0af1cf978652d597e4872ef70b978f92673d92b78f3ee98","observation_id":"1a4c9238-0351-4690-921a-287d93c1c2d8","resolution":{"observed_at":"2026-08-12T15:18:28.458124Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2933","last_updated":"2011-08-17T09:25:04Z","snapshot_observed_at":"2026-08-09T14:29:15.405022Z","submitted_at":"2011-04-14T22:06:43Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2933","snapshot_observed_at":"2026-08-12T15:18:28.511816Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.511816Z"},"links":{"cited_paper":"/paper/1104.2933","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:678245e3b1907a6654d2a2bdc3440fa21df60d70f1c9661ea7f9eb6f449b8408","observation_id":"33fa2a56-ff20-4c6f-a9d7-9c2d81faaa3d","resolution":{"observed_at":"2026-08-12T15:18:28.511816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2934","last_updated":"2011-05-16T19:26:16Z","snapshot_observed_at":"2026-08-15T04:49:17.309428Z","submitted_at":"2011-04-14T22:09:26Z","title":"The Cosmic Linear Anisotropy Solving System (CLASS) III: Comparision with CAMB for LambdaCDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2934","snapshot_observed_at":"2026-08-12T15:18:28.526376Z","title":"Lesgourgues, The Cosmic Linear Anisotropy Solving System (CLASS) III: Comparision with CAMB for LambdaCDM, 1104.2934","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-12T15:18:28.526376Z"},"links":{"cited_paper":"/paper/1104.2934","citing_paper":"/paper/2411.14524"},"observation_digest":"sha256:447c638d6d57abec368f51162d9214ed9719a6ced1f7b5103df804597f60c3b3","observation_id":"908b8a37-3501-4aef-99a8-196b3da589b3","resolution":{"observed_at":"2026-08-12T15:18:28.526376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2411.14524","last_updated":"2025-05-28T09:06:33Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T01:58:22.711453Z","submitted_at":"2024-11-21T19:00:01Z","title":"Origin of cosmological neutrino mass bounds: background $\\textit{versus}$ perturbations"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":96,"verified_exact":4,"verified_fuzzy":0},"total_outbound_references":124},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 100 of 124 outbound references and 9 inbound Pith citation observations for arXiv:2411.14524."}