{"as_of":"2026-08-18T00:44:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bf042cc159c60a1b597c56cb74ca70dce68bb6376d7c378a1d7b7dd70cbac8b7","coverage":[{"denominator":89,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":89,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T12:26:09.132708Z","state":"measured"},{"denominator":95,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":95,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T11:11:26.534597Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-21T21:04:21.923950Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.14322","snapshot_observed_at":"2026-08-16T11:11:26.534597Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.16910","last_updated":"2025-04-23T17:37:57Z","snapshot_observed_at":"2026-08-17T21:08:07.977731Z","submitted_at":"2025-04-23T17:37:57Z","title":"Self-interacting dark matter with observable $\\Delta N_{\\rm eff}$","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-16T11:11:26.534597Z"},"links":{"cited_paper":"/paper/2412.14322","citing_paper":"/paper/2504.16910"},"observation_digest":"sha256:635b9852265b9252a4184789741e38f233f5ddea96b01e85469be6f41d3d1700","observation_id":"b92cd589-5e59-40f1-a93b-4e218f17ca1b","resolution":{"observed_at":"2026-08-16T11:11:26.534597Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"cited_work":{"arxiv_id":"2412.14322","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.14322","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Long and M","venue":null,"work_id":"0c7b75ab-9b99-4861-ad59-1bfb7720b3f1","year":null},"citing_paper":{"arxiv_id":"2506.12131","last_updated":"2025-06-13T18:00:01Z","snapshot_observed_at":"2026-08-17T20:56:01.391326Z","submitted_at":"2025-06-13T18:00:01Z","title":"Early Growth of Structure in Warm Wave Dark Matter","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-19T09:22:41.197004Z"},"links":{"cited_paper":"/paper/2412.14322","citing_paper":"/paper/2506.12131"},"observation_digest":"sha256:04def74af20d4837b171d304e1ab6d26962a98cea1f11599ab679023beec7615","observation_id":"fee87f93-564c-40f8-91e9-0b330b8b4258","resolution":{"observed_at":"2026-05-19T09:23:02.973570Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.14322","snapshot_observed_at":"2026-08-06T20:54:53.479439Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.01956","last_updated":"2025-07-02T17:59:21Z","snapshot_observed_at":"2026-08-15T22:31:44.446769Z","submitted_at":"2025-07-02T17:59:21Z","title":"Universal lower bound on the axion decay constant from free streaming effects","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T20:54:53.479439Z"},"links":{"cited_paper":"/paper/2412.14322","citing_paper":"/paper/2507.01956"},"observation_digest":"sha256:98b6b0d590a77eb4bef8e943a66d3023918343a41f399ce108e8c442ff22785f","observation_id":"634724f2-74f6-4ef0-be2a-eba4b6fee805","resolution":{"observed_at":"2026-08-06T20:54:53.479439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"cited_work":{"arxiv_id":"2412.14322","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.14322","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Long and M","venue":null,"work_id":"0c7b75ab-9b99-4861-ad59-1bfb7720b3f1","year":null},"citing_paper":{"arxiv_id":"2510.15046","last_updated":"2026-05-15T21:17:07Z","snapshot_observed_at":"2026-07-31T16:02:14.376653Z","submitted_at":"2025-10-16T18:03:25Z","title":"Multi-species Dark Matter with Warmth and Randomness","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-21T21:01:12.105296Z"},"links":{"cited_paper":"/paper/2412.14322","citing_paper":"/paper/2510.15046"},"observation_digest":"sha256:50222fb2de95c621c4e97d8d92977a2f0f08f43c6f5f35a6447dd86e14b841dc","observation_id":"c1554b15-0182-4114-9d6e-c926dd192b0f","resolution":{"observed_at":"2026-05-21T21:04:21.926029Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"cited_work":{"arxiv_id":"2412.14322","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.14322","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Long and M","venue":null,"work_id":"0c7b75ab-9b99-4861-ad59-1bfb7720b3f1","year":null},"citing_paper":{"arxiv_id":"2510.17977","last_updated":"2026-05-19T19:21:08Z","snapshot_observed_at":"2026-08-14T08:19:17.311125Z","submitted_at":"2025-10-20T18:00:10Z","title":"Growth of Structure in Multi-species Wave Dark Matter","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-21T20:59:52.011652Z"},"links":{"cited_paper":"/paper/2412.14322","citing_paper":"/paper/2510.17977"},"observation_digest":"sha256:d1533e1687e2019ae83716064ff221f39d964713c4d6f09d574b35c6034e704f","observation_id":"c5d206e6-e507-4582-8120-7978799af48a","resolution":{"observed_at":"2026-05-21T21:00:37.995242Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"cited_work":{"arxiv_id":"2412.14322","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.14322","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Long and M","venue":null,"work_id":"0c7b75ab-9b99-4861-ad59-1bfb7720b3f1","year":null},"citing_paper":{"arxiv_id":"2604.15241","last_updated":"2026-04-16T17:16:56Z","snapshot_observed_at":"2026-08-17T18:45:44.298536Z","submitted_at":"2026-04-16T17:16:56Z","title":"Echoes of Global Cosmic Strings","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-10T10:29:31.299981Z"},"links":{"cited_paper":"/paper/2412.14322","citing_paper":"/paper/2604.15241"},"observation_digest":"sha256:1328eeb71b50ba6f179735a277b44e1c1f1951c81a5a029fcb8455e959939595","observation_id":"46a4d6ee-decd-4456-a397-f0a8551a55ba","resolution":{"observed_at":"2026-05-10T11:00:04.619629Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2412.14322/citation-record","integrity":"/paper/2412.14322/integrity","json":"/paper/2412.14322/citation-record.json","paper":"/paper/2412.14322"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T12:26:08.645805Z","title":"and others, New Horizons: Scalar and Vector Ultralight Dark Matter,2203.14915","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.645805Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:bf3d731c5373a8adb9d3d33c2a33ae4acd823fa0688a1399bb4c33fe6ec5ccfc","observation_id":"d361afeb-9ce2-4ee7-ae4f-a3b7a63441fe","resolution":{"observed_at":"2026-08-11T12:26:08.645805Z","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":"2026-08-11T12:26:08.651404Z","title":"and Wilczek, Frank, Cosmology of the Invisible Axion, Phys","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.651404Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:933623cf94263df1b4ec9dad75a9c2081f7c9da72c9f2d2b756f4b158d83c82f","observation_id":"0deecff3-c08d-4b35-8248-77be0747eae5","resolution":{"observed_at":"2026-08-11T12:26:08.651404Z","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":"2026-08-11T12:26:08.656685Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.656685Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:845d7bbba80444153cd6ed04087603229fa880a4c53c203fa1a584098578919c","observation_id":"0e195b6f-738c-4fcc-9543-fba514b2185a","resolution":{"observed_at":"2026-08-11T12:26:08.656685Z","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":"2026-08-11T12:26:08.661902Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.661902Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:9deb9db5966ed7bdc8b78fb4aa8bd6ccfdb63b42ac62aab8da8998a3907217f3","observation_id":"12552e35-1545-451d-92f0-8b06e0cb22b5","resolution":{"observed_at":"2026-08-11T12:26:08.661902Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.09042","last_updated":"2025-01-27T21:39:19Z","snapshot_observed_at":"2026-08-16T14:34:44.126067Z","submitted_at":"2023-12-14T15:39:27Z","title":"Cosmological gravitational particle production and its implications for cosmological relics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.09042","snapshot_observed_at":"2026-08-11T12:26:08.668052Z","title":"and Long, Andrew J., Cosmological gravitational particle production and its implications for cosmological relics, Rev","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.668052Z"},"links":{"cited_paper":"/paper/2312.09042","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:b13a853bc0a9d7cad787efa51a67a7c7e0cc1868b6dd9172138548ddea49dbf3","observation_id":"c1da706a-0d60-49e0-9ae9-d62d3e41a027","resolution":{"observed_at":"2026-08-11T12:26:08.668052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.02102","last_updated":"2015-04-08T20:01:23Z","snapshot_observed_at":"2026-08-16T10:45:09.243617Z","submitted_at":"2015-04-08T20:01:23Z","title":"Vector Dark Matter from Inflationary Fluctuations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.02102","snapshot_observed_at":"2026-08-11T12:26:08.673773Z","title":"and Mardon, Jeremy and Rajendran, Surjeet, Vector Dark Matter from Inflationary Fluctuations, Phys","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.673773Z"},"links":{"cited_paper":"/paper/1504.02102","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:69ee997baadbddcc67a267433c60216b9ccf5b43e18b38b7c6f054c2cd3428f6","observation_id":"21098b96-2f39-4265-b1d9-760751172624","resolution":{"observed_at":"2026-08-11T12:26:08.673773Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.04677","last_updated":"2018-06-12T18:00:00Z","snapshot_observed_at":"2026-08-14T19:04:35.470991Z","submitted_at":"2018-06-12T18:00:00Z","title":"Axions from Strings: the Attractive Solution","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.04677","snapshot_observed_at":"2026-08-11T12:26:08.679940Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.679940Z"},"links":{"cited_paper":"/paper/1806.04677","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:ab4b3df00285266b1354772c86c525d7c3db8521bde467639845d739cb9e3723","observation_id":"cccb0b7b-0267-4c97-aa20-5ecacecc22e8","resolution":{"observed_at":"2026-08-11T12:26:08.679940Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07188","last_updated":"2018-10-16T18:00:00Z","snapshot_observed_at":"2026-08-16T14:09:47.716896Z","submitted_at":"2018-10-16T18:00:00Z","title":"Relic Abundance of Dark Photon Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07188","snapshot_observed_at":"2026-08-11T12:26:08.685706Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.685706Z"},"links":{"cited_paper":"/paper/1810.07188","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:ebe70ddb7c1769f46b8d0893577c144edfae58f517aff9674783405851b36ff2","observation_id":"1e81ab53-699e-45c2-8904-9718b19b4050","resolution":{"observed_at":"2026-08-11T12:26:08.685706Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07195","last_updated":"2019-03-01T18:44:59Z","snapshot_observed_at":"2026-08-16T03:17:56.472926Z","submitted_at":"2018-10-16T18:00:05Z","title":"Parametric Resonance Production of Ultralight Vector Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07195","snapshot_observed_at":"2026-08-11T12:26:08.691121Z","title":"and Harigaya, Keisuke and Narayan, Vijay, Parametric Resonance Production of Ultralight Vector Dark Matter, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.691121Z"},"links":{"cited_paper":"/paper/1810.07195","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:fc693be878a7f86cae11601b03ce22642a96f3b2f296226934b46ab460a6d811","observation_id":"5a33a547-e2fc-4ac3-aae2-de9623f48699","resolution":{"observed_at":"2026-08-11T12:26:08.691121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07196","last_updated":"2019-05-02T17:21:11Z","snapshot_observed_at":"2026-08-14T18:13:39.927837Z","submitted_at":"2018-10-16T18:00:06Z","title":"Dark Photon Dark Matter Produced by Axion Oscillations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07196","snapshot_observed_at":"2026-08-11T12:26:08.696924Z","title":"and Pierce, Aaron and Zhang, Zhengkang and Zhao, Yue, Dark Photon Dark Matter Produced by Axion Oscillations, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.696924Z"},"links":{"cited_paper":"/paper/1810.07196","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:1d6499ebf019a24c97d74f88c15479ea023d03aca565e9ff2193e973435c929a","observation_id":"a5ddccb3-1ffe-40af-9ced-362b3db07cbf","resolution":{"observed_at":"2026-08-11T12:26:08.696924Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.07208","last_updated":"2019-03-28T16:35:31Z","snapshot_observed_at":"2026-08-14T18:13:39.531904Z","submitted_at":"2018-10-16T18:04:45Z","title":"Vector dark matter production at the end of inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.07208","snapshot_observed_at":"2026-08-11T12:26:08.702271Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.702271Z"},"links":{"cited_paper":"/paper/1810.07208","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:349d7a64134ae3df4d1946166f344754e3674156069177261dcff982c93e4378","observation_id":"5e212577-68b9-471f-82de-5b371543cc49","resolution":{"observed_at":"2026-08-11T12:26:08.702271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03312","last_updated":"2019-03-18T13:09:59Z","snapshot_observed_at":"2026-08-15T02:54:03.163821Z","submitted_at":"2019-01-10T18:31:28Z","title":"Dark Photon Dark Matter from a Network of Cosmic Strings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03312","snapshot_observed_at":"2026-08-11T12:26:08.708212Z","title":"and Wang, Lian-Tao, Dark Photon Dark Matter from a Network of Cosmic Strings, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.708212Z"},"links":{"cited_paper":"/paper/1901.03312","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:dc96928492753fadfac40dd41e706616a2a6940262c7019983279b7c4cf258ca","observation_id":"6a247104-eb06-43ca-9a80-99183d8ab12d","resolution":{"observed_at":"2026-08-11T12:26:08.708212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.04990","last_updated":"2021-03-22T14:29:48Z","snapshot_observed_at":"2026-08-17T13:59:27.859228Z","submitted_at":"2020-07-09T18:00:00Z","title":"More Axions from Strings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.04990","snapshot_observed_at":"2026-08-11T12:26:08.712999Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.712999Z"},"links":{"cited_paper":"/paper/2007.04990","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:b3ee601bd36b4a03c6717e1c384d3499871e6699adafa07192da54c96e6782b6","observation_id":"fd8665bd-27d7-4192-8517-06718ec169cf","resolution":{"observed_at":"2026-08-11T12:26:08.712999Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.02077","last_updated":"2021-04-05T18:00:01Z","snapshot_observed_at":"2026-08-16T18:33:46.717318Z","submitted_at":"2021-04-05T18:00:01Z","title":"Gravitational Waves and Dark Photon Dark Matter from Axion Rotations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.02077","snapshot_observed_at":"2026-08-11T12:26:08.718077Z","title":"and Harigaya, Keisuke and Pierce, Aaron, Gravitational waves and dark photon dark matter from axion rotations, JHEP12(2021) 099, [2104.02077]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.718077Z"},"links":{"cited_paper":"/paper/2104.02077","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:0032e0f4f68365769285dcd8fdcf49de7d13035613552c85801d7c91dda3b891","observation_id":"b97200ab-1b3e-40b5-a62c-abe33047436f","resolution":{"observed_at":"2026-08-11T12:26:08.718077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.06421","last_updated":"2023-05-08T09:59:45Z","snapshot_observed_at":"2026-08-16T16:16:49.668480Z","submitted_at":"2022-11-11T18:59:51Z","title":"The meso-inflationary QCD axion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.06421","snapshot_observed_at":"2026-08-11T12:26:08.723298Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.723298Z"},"links":{"cited_paper":"/paper/2211.06421","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:e95ff2c4310b038dfdc8f99b8895882befc71088f476914e93dafd4dfcd3b766","observation_id":"16b4470c-060c-4858-b3a4-16e4d5503bd1","resolution":{"observed_at":"2026-08-11T12:26:08.723298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.08289","last_updated":"2022-11-15T16:44:25Z","snapshot_observed_at":"2026-08-16T16:15:58.395470Z","submitted_at":"2022-11-15T16:44:25Z","title":"More axions from diluted domain walls","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.08289","snapshot_observed_at":"2026-08-11T12:26:08.728837Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.728837Z"},"links":{"cited_paper":"/paper/2211.08289","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:7668cdbbb31ee8ecd883c6f08e4bb8f427984d8093db3d800007499e55f35b2d","observation_id":"bc012fe1-781e-4bde-b920-3c16cb46225f","resolution":{"observed_at":"2026-08-11T12:26:08.728837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.09775","last_updated":"2024-08-13T12:13:09Z","snapshot_observed_at":"2026-08-16T16:15:18.586273Z","submitted_at":"2022-11-17T18:50:28Z","title":"A lower bound on dark matter mass","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.09775","snapshot_observed_at":"2026-08-11T12:26:08.734040Z","title":"and Mirbabayi, Mehrdad, A Lower Bound on Dark Matter Mass, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.734040Z"},"links":{"cited_paper":"/paper/2211.09775","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:b116dfcf1de85a3e204b9247a3d5d8a3f307e33efd90600d65c9c38ee3ef608d","observation_id":"ffdd7388-05dc-460a-a61a-7f49c1a17b94","resolution":{"observed_at":"2026-08-11T12:26:08.734040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.12970","last_updated":"2025-09-10T16:39:14Z","snapshot_observed_at":"2026-08-16T13:41:43.162675Z","submitted_at":"2024-06-18T18:00:01Z","title":"Warm and Fuzzy Dark Matter: Free Streaming of Wave Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.12970","snapshot_observed_at":"2026-08-11T12:26:08.739544Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.739544Z"},"links":{"cited_paper":"/paper/2406.12970","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:a47a6cbfb00be0e02bcbc8ac0a2deac0187b39bdeed45cb26007fc5853e29383","observation_id":"1da3e7c3-0ece-4257-8b74-f602d9f0b8b0","resolution":{"observed_at":"2026-08-11T12:26:08.739544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.05591","last_updated":"2024-12-11T04:06:10Z","snapshot_observed_at":"2026-08-16T13:27:15.581593Z","submitted_at":"2024-08-10T16:32:10Z","title":"Free Streaming in Warm Wave Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.05591","snapshot_observed_at":"2026-08-11T12:26:08.744620Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.744620Z"},"links":{"cited_paper":"/paper/2408.05591","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:f33aff59ee84989f1d4ea9844425ac5d839cce1568458edde1d573f4dc65c4b6","observation_id":"2fb04a7e-3d5f-41f2-83b8-6af48a28194a","resolution":{"observed_at":"2026-08-11T12:26:08.744620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0812.0010","last_updated":"2009-05-20T12:33:57Z","snapshot_observed_at":"2026-08-15T10:00:34.915654Z","submitted_at":"2008-12-01T18:34:55Z","title":"Lyman-alpha constraints on warm and on warm-plus-cold dark matter models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0812.0010","snapshot_observed_at":"2026-08-11T12:26:08.749615Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.749615Z"},"links":{"cited_paper":"/paper/0812.0010","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:9aed2599f62be1bcb916f813fe053ef700f284f3354eb58e8420d13cea5e8498","observation_id":"ea4c1675-6a75-4f5f-847e-fe73c92ed303","resolution":{"observed_at":"2026-08-11T12:26:08.749615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.2314","last_updated":"2013-08-26T15:18:02Z","snapshot_observed_at":"2026-08-15T00:14:33.621993Z","submitted_at":"2013-06-10T20:00:03Z","title":"Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.2314","snapshot_observed_at":"2026-08-11T12:26:08.754300Z","title":"and Bolton, James S","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.754300Z"},"links":{"cited_paper":"/paper/1306.2314","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:2d8704e47265cd5168eb9e484581f2397f92249b3c90518361dbc4ff04de09d7","observation_id":"22853e9d-a3bc-4a73-b16d-dfc06a779f3a","resolution":{"observed_at":"2026-08-11T12:26:08.754300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14220","last_updated":"2023-06-09T18:41:55Z","snapshot_observed_at":"2026-08-16T16:29:10.651893Z","submitted_at":"2022-09-28T16:47:30Z","title":"New Constraints on Warm Dark Matter from the Lyman-$\\alpha$ Forest Power Spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.14220","snapshot_observed_at":"2026-08-11T12:26:08.759129Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.759129Z"},"links":{"cited_paper":"/paper/2209.14220","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:ec6055870e83a8a223704a069f6e9f28318a26fd027961c2fb6dfd08ab098fd8","observation_id":"7a8f35b4-076a-4651-b15c-250f7facde37","resolution":{"observed_at":"2026-08-11T12:26:08.759129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.01352","last_updated":"2024-06-18T10:41:08Z","snapshot_observed_at":"2026-08-16T15:11:15.323994Z","submitted_at":"2023-08-02T18:00:13Z","title":"Revisiting signatures of thermal axions in nonstandard cosmologies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.01352","snapshot_observed_at":"2026-08-11T12:26:08.764808Z","title":"and Roszkowski, Leszek and Venegas, Moira, Revisiting signatures of thermal axions in nonstandard cosmologies, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.764808Z"},"links":{"cited_paper":"/paper/2308.01352","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:35172c596f5798bfcee96d7a723e14c909d5bacbe7ccb8b61cec854a0eefec4d","observation_id":"cd4a4a03-b69a-41f6-8323-9a807f242555","resolution":{"observed_at":"2026-08-11T12:26:08.764808Z","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":"2026-08-11T12:26:08.770548Z","title":"Cambridge University Press, 7, 2022, 10.1017/9781108937092","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.770548Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:1b44455a3dd85ed1c67b379bd80c95e8e7a1c771c5ebf4df5c8a99d3e286048c","observation_id":"8dbdd3d0-3517-4649-8001-440391211301","resolution":{"observed_at":"2026-08-11T12:26:08.770548Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.16182","last_updated":"2021-01-27T20:25:20Z","snapshot_observed_at":"2026-08-14T11:40:17.942200Z","submitted_at":"2020-06-29T16:47:30Z","title":"The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.16182","snapshot_observed_at":"2026-08-11T12:26:08.775538Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.775538Z"},"links":{"cited_paper":"/paper/2006.16182","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:d7ef28507b31dc11182db346433ff28f5811002f6b5ff1bfa529ab9ad5b53628","observation_id":"939d3d24-dafe-4f5f-882e-8a68959ae508","resolution":{"observed_at":"2026-08-11T12:26:08.775538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.04780","last_updated":"2024-11-07T15:18:55Z","snapshot_observed_at":"2026-08-16T13:02:04.211380Z","submitted_at":"2024-11-07T15:18:55Z","title":"Conversations and Deliberations: Non-Standard Cosmological Epochs and Expansion Histories","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.04780","snapshot_observed_at":"2026-08-11T12:26:08.780364Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.780364Z"},"links":{"cited_paper":"/paper/2411.04780","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:cf56f7c3b99d98ee6b92a26b9043526b3a5d8935691162cf38598cdf0883bdbb","observation_id":"86cf8a8b-0af9-498c-b5e6-ba15483a8ed9","resolution":{"observed_at":"2026-08-11T12:26:08.780364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.05208","last_updated":"2022-04-06T12:16:37Z","snapshot_observed_at":"2026-08-04T21:52:15.150186Z","submitted_at":"2021-05-11T17:17:34Z","title":"Challenges for $\\Lambda$CDM: An update","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.05208","snapshot_observed_at":"2026-08-11T12:26:08.785098Z","title":"Rev.95 (2022) 101659, [2105.05208]","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.785098Z"},"links":{"cited_paper":"/paper/2105.05208","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:91052a27e38476c90bbf2b38a1a350a4cae2a25e1a00785b378fd4e53cb8a973","observation_id":"745b79cc-3164-496f-87e7-1f2fb3989530","resolution":{"observed_at":"2026-08-11T12:26:08.785098Z","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":"2026-08-16T02:36:16.088814Z","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":"2026-08-11T12:26:08.789622Z","title":"and Riess, Adam G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.789622Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:68e8d85b1b43d3c31b10468c5eb9591289a20db626960d22d45d54f1a8cf05f0","observation_id":"e70f11fd-097a-4e0a-b94a-26810eceabb5","resolution":{"observed_at":"2026-08-11T12:26:08.789622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.15656","last_updated":"2021-06-29T18:09:57Z","snapshot_observed_at":"2026-08-16T18:13:32.550098Z","submitted_at":"2021-06-29T18:09:57Z","title":"Measurements of the Hubble Constant: Tensions in Perspective","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.15656","snapshot_observed_at":"2026-08-11T12:26:08.794067Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.794067Z"},"links":{"cited_paper":"/paper/2106.15656","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:b56300fb52476582772ddceb6b21c666428aff6662691d55fb12feb996219533","observation_id":"1bf7be99-12d9-4c6e-a813-14c94bc509db","resolution":{"observed_at":"2026-08-11T12:26:08.794067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.4546","last_updated":"2012-06-04T18:01:58Z","snapshot_observed_at":"2026-08-15T04:43:09.967596Z","submitted_at":"2011-06-22T20:00:02Z","title":"Dynamical Dark Matter: I. Theoretical Overview","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.4546","snapshot_observed_at":"2026-08-11T12:26:08.799078Z","title":"and Thomas, Brooks, Dynamical Dark Matter: I","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.799078Z"},"links":{"cited_paper":"/paper/1106.4546","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:209e7c67262c3437de59fc9ba27a410dbfdf4d304c7bb71a1542822f37d9eef3","observation_id":"27c1d7c6-b8db-4b9d-8309-739f250838e1","resolution":{"observed_at":"2026-08-11T12:26:08.799078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.07746","last_updated":"2015-02-26T21:00:03Z","snapshot_observed_at":"2026-08-14T22:58:26.808313Z","submitted_at":"2015-02-26T21:00:03Z","title":"Cosmological Moduli and the Post-Inflationary Universe: A Critical Review","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.07746","snapshot_observed_at":"2026-08-11T12:26:08.804477Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.804477Z"},"links":{"cited_paper":"/paper/1502.07746","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:eabecfb38e93bf696202319688a30ca117f217c7debc9618463fb459d0ea757a","observation_id":"17b391ee-d53a-45b0-b345-70048c7a6016","resolution":{"observed_at":"2026-08-11T12:26:08.804477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.04753","last_updated":"2022-01-18T18:50:20Z","snapshot_observed_at":"2026-08-17T06:14:27.149894Z","submitted_at":"2021-11-08T19:00:02Z","title":"Stasis in an Expanding Universe: A Recipe for Stable Mixed-Component Cosmological Eras","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.04753","snapshot_observed_at":"2026-08-11T12:26:08.809881Z","title":"and Heurtier, Lucien and Huang, Fei and Kim, Doojin and Tait, Tim M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.809881Z"},"links":{"cited_paper":"/paper/2111.04753","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:24df28d7fd5ae73d79b3c5f8395ad07031408d376b7f00c42c4d21d6b46c2956","observation_id":"4038c750-2ecd-4cd2-a358-269f264ad3d3","resolution":{"observed_at":"2026-08-11T12:26:08.809881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.04819","last_updated":"2023-05-05T10:33:53Z","snapshot_observed_at":"2026-08-16T15:49:43.775705Z","submitted_at":"2023-03-08T19:00:01Z","title":"String Cosmology: from the Early Universe to Today","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.04819","snapshot_observed_at":"2026-08-11T12:26:08.814999Z","title":"and Maharana, Anshuman and Parameswaran, Susha and Quevedo, Fernando and Zavala, Ivonne, String cosmology: From the early universe to today, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.814999Z"},"links":{"cited_paper":"/paper/2303.04819","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:84f252f29fcabf1671819bc816f64b1a11688b1da9f0b61800fc031f6654248c","observation_id":"9cc671b9-5e2a-48f8-8daf-26f0d3409b83","resolution":{"observed_at":"2026-08-11T12:26:08.814999Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.06165","last_updated":"2016-01-19T18:25:13Z","snapshot_observed_at":"2026-08-14T22:17:49.215298Z","submitted_at":"2015-12-19T00:10:37Z","title":"Dark Matter Direct Detection with Accelerometers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.06165","snapshot_observed_at":"2026-08-11T12:26:08.820201Z","title":"and Kaplan, David E","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.820201Z"},"links":{"cited_paper":"/paper/1512.06165","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:a26bbd3ecb0b28390f401299a25bc216bc27993619d95aec30583eba90773842","observation_id":"48f509e1-5252-404f-93d4-001fef458e5f","resolution":{"observed_at":"2026-08-11T12:26:08.820201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0803.2349","last_updated":"2008-08-20T04:56:12Z","snapshot_observed_at":"2026-08-15T10:19:26.384084Z","submitted_at":"2008-03-17T13:10:16Z","title":"Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies","version":2},"cited_work":{"arxiv_id":"0803.2349","doi":null,"metadata_source":"pith","pith_arxiv_id":"0803.2349","snapshot_observed_at":"2026-08-11T12:26:10.225483Z","title":"Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies","venue":"astro-ph","work_id":"17b6d0e6-cd5e-400b-bf43-2e71b9a0d9a4","year":2008},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.825152Z"},"links":{"cited_paper":"/paper/0803.2349","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:8e6a4f1ff4745e83a5611560b2015bc874242826ae76228fcd37add5528c9acb","observation_id":"a98a4a25-a9fa-45af-ab08-d4ee3dbe636c","resolution":{"observed_at":"2026-08-11T12:26:10.230406Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0808.3994","last_updated":"2008-12-16T16:19:59Z","snapshot_observed_at":"2026-08-17T07:11:58.528274Z","submitted_at":"2008-08-29T17:15:43Z","title":"Changes in Dark Matter Properties After Freeze-Out","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0808.3994","snapshot_observed_at":"2026-08-11T12:26:08.830187Z","title":"and Pierce, Aaron, Changes in Dark Matter Properties After Freeze-Out, Phys","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.830187Z"},"links":{"cited_paper":"/paper/0808.3994","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:96a4e19e5ee7e28ad8142b35b2f509e9ae71bea8fe8cdca3c854b9482091654e","observation_id":"8d91268c-591f-4df4-b996-59e0c2809407","resolution":{"observed_at":"2026-08-11T12:26:08.830187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.5034","last_updated":"2011-08-10T16:04:58Z","snapshot_observed_at":"2026-08-15T04:48:21.984391Z","submitted_at":"2011-04-26T21:12:09Z","title":"Probing the Cosmological Constant and Phase Transitions with Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.5034","snapshot_observed_at":"2026-08-11T12:26:08.835311Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.835311Z"},"links":{"cited_paper":"/paper/1104.5034","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:8714d1ac269b351d6b70c209c67d974a01507d5e6fc1427428ff5209d4c5b54c","observation_id":"815b2405-d9c7-493a-a2a7-a4b7a02768f7","resolution":{"observed_at":"2026-08-11T12:26:08.835311Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.5193","last_updated":"2011-08-29T17:44:49Z","snapshot_observed_at":"2026-08-15T04:37:17.740367Z","submitted_at":"2011-08-25T20:28:03Z","title":"Cosmological Constant, Dark Matter, and Electroweak Phase Transition","version":2},"cited_work":{"arxiv_id":"1108.5193","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.5193","snapshot_observed_at":"2026-08-11T12:26:10.175192Z","title":"Cosmological Constant, Dark Matter, and Electroweak Phase Transition","venue":"astro-ph.CO","work_id":"3deadfa2-0f24-49d0-a031-a987ecc44cb5","year":2011},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.840872Z"},"links":{"cited_paper":"/paper/1108.5193","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:0df6ba71449135cad19f3a3d61ce28405d753c233ea8deb2c1347f1615e48797","observation_id":"95eac473-30a0-4144-a895-ffdde511e9a8","resolution":{"observed_at":"2026-08-11T12:26:10.180099Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.04979","last_updated":"2017-01-26T14:09:24Z","snapshot_observed_at":"2026-08-14T21:39:34.474923Z","submitted_at":"2016-09-16T10:11:12Z","title":"On Effective Degrees of Freedom in the Early Universe","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.04979","snapshot_observed_at":"2026-08-11T12:26:08.847697Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.847697Z"},"links":{"cited_paper":"/paper/1609.04979","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:1878e3b39ef893dc5a091a96507c5210b6982bfcdd05dd027ccd0575a01837fe","observation_id":"c61ac622-38cf-482e-8abf-c2d9baf19abe","resolution":{"observed_at":"2026-08-11T12:26:08.847697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9605054","last_updated":"1996-05-10T17:41:05Z","snapshot_observed_at":"2026-08-06T03:08:48.294553Z","submitted_at":"1996-05-10T17:41:05Z","title":"The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9605054","snapshot_observed_at":"2026-08-11T12:26:08.852814Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.852814Z"},"links":{"cited_paper":"/paper/astro-ph/9605054","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:594e7d17f2c0feef4b5c196b085ebccc7d8995adce77d54e2e3db11d4bda3b39","observation_id":"f9c4515f-9cb8-478e-83d1-c5f66b1d4340","resolution":{"observed_at":"2026-08-11T12:26:08.852814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0003365","last_updated":"2000-03-26T22:50:24Z","snapshot_observed_at":"2026-07-07T00:10:35.167895Z","submitted_at":"2000-03-24T00:29:30Z","title":"Cold and Fuzzy Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0003365","snapshot_observed_at":"2026-08-11T12:26:08.858887Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.858887Z"},"links":{"cited_paper":"/paper/astro-ph/0003365","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:0478269405f72239c2c72c2dc006f70d3a9417baf959c0a9200f5eb3731e28b3","observation_id":"8eb6c5c6-413a-4894-8647-b60727050dda","resolution":{"observed_at":"2026-08-11T12:26:08.858887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.08297","last_updated":"2017-02-24T21:01:45Z","snapshot_observed_at":"2026-08-14T21:33:28.298458Z","submitted_at":"2016-10-26T12:25:05Z","title":"Ultralight scalars as cosmological dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.08297","snapshot_observed_at":"2026-08-11T12:26:08.864591Z","title":"and Tremaine, Scott and Witten, Edward, Ultralight scalars as cosmological dark matter, Phys","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.864591Z"},"links":{"cited_paper":"/paper/1610.08297","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:1e20934e90fdd1e7dd02a8fdff0e8cf046f455518570fcba203e3614229462a9","observation_id":"5e17e199-852e-40d8-8909-ae06b02bb10f","resolution":{"observed_at":"2026-08-11T12:26:08.864591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2108.05368","last_updated":"2021-08-11T18:00:06Z","snapshot_observed_at":"2026-08-16T18:03:46.856535Z","submitted_at":"2021-08-11T18:00:06Z","title":"Dark Matter from Axion Strings with Adaptive Mesh Refinement","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2108.05368","snapshot_observed_at":"2026-08-11T12:26:08.870426Z","title":"and Hook, Anson and Peterson, Adam and Willcox, Don E","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.870426Z"},"links":{"cited_paper":"/paper/2108.05368","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:855b8e1da39936fef9a9de06baf1433fa2d6275d57906585978d3439bb4a2395","observation_id":"32659e54-1963-4e99-abd7-437cb4c61e73","resolution":{"observed_at":"2026-08-11T12:26:08.870426Z","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":"2026-08-11T12:26:08.875858Z","title":"and Delos, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.875858Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:6cc69811347ea37a13d416cefeb170d31e4b56c530c37ae4faa42085f2133207","observation_id":"39eee101-61f2-4b41-a311-71d989e5ac56","resolution":{"observed_at":"2026-08-11T12:26:08.875858Z","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":"2026-08-11T12:26:08.883132Z","title":"H., Axions and inflation: Sitting in the vacuum, Phys","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.883132Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:ad7301cf78ecd0b023e3cf7fa1155617b3fde391d2c7dabf79d3b8802bac4514","observation_id":"5ec38fc2-615b-4dff-ab4b-e79575085bc0","resolution":{"observed_at":"2026-08-11T12:26:08.883132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9912349","last_updated":"1999-12-16T16:13:27Z","snapshot_observed_at":"2026-07-07T01:30:36.512180Z","submitted_at":"1999-12-16T16:13:27Z","title":"Perturbation amplitude in isocurvature inflation scenarios","version":1},"cited_work":{"arxiv_id":"astro-ph/9912349","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9912349","snapshot_observed_at":"2026-08-11T12:26:09.982998Z","title":"Perturbation amplitude in isocurvature inflation scenarios","venue":"astro-ph","work_id":"b84ab346-49cf-463b-8bf2-97a00135462f","year":1999},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.887956Z"},"links":{"cited_paper":"/paper/astro-ph/9912349","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:94afee0530b40ea79ddccd6a0f016d9ac06707399402b694deb10a5aa2fc1fe6","observation_id":"b33bf476-656b-4a01-b506-abbba505a5a5","resolution":{"observed_at":"2026-08-11T12:26:09.987912Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0411468","last_updated":"2004-11-16T19:42:27Z","snapshot_observed_at":"2026-07-07T00:46:08.717211Z","submitted_at":"2004-11-16T19:42:27Z","title":"Isocurvature constraints on gravitationally produced superheavy dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0411468","snapshot_observed_at":"2026-08-11T12:26:08.893017Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.893017Z"},"links":{"cited_paper":"/paper/astro-ph/0411468","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:d0710369ab1f347923e380ed2fe2be14fdb7fb807d9ef960f0ff6dad9fefe7b0","observation_id":"f85a8208-4ab6-414b-952a-bf705cc8b11b","resolution":{"observed_at":"2026-08-11T12:26:08.893017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.5931","last_updated":"2013-01-09T18:04:52Z","snapshot_observed_at":"2026-08-15T04:30:51.882940Z","submitted_at":"2011-10-26T21:08:43Z","title":"Isocurvature Perturbations and Non-Gaussianity of Gravitationally Produced Nonthermal Dark Matter","version":2},"cited_work":{"arxiv_id":"1110.5931","doi":null,"metadata_source":"pith","pith_arxiv_id":"1110.5931","snapshot_observed_at":"2026-08-11T12:26:09.947221Z","title":"Isocurvature Perturbations and Non-Gaussianity of Gravitationally Produced Nonthermal Dark Matter","venue":"astro-ph.CO","work_id":"6a45da44-6140-4d7e-bfb3-5748ab885113","year":2011},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.899333Z"},"links":{"cited_paper":"/paper/1110.5931","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:7d53657758550caac98f02dc98954e4a0f4c25340bed78d4a7ea44959ad4962e","observation_id":"9a1d4898-efee-459f-8e51-25d1d4a97197","resolution":{"observed_at":"2026-08-11T12:26:09.952220Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11621","last_updated":"2021-05-11T19:27:03Z","snapshot_observed_at":"2026-08-16T18:49:33.226273Z","submitted_at":"2021-01-27T19:00:00Z","title":"Superheavy scalar dark matter from gravitational particle production in $\\alpha$-attractor models of inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11621","snapshot_observed_at":"2026-08-11T12:26:08.904290Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.904290Z"},"links":{"cited_paper":"/paper/2101.11621","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:7b53fae297bdb148d617e43ab0df7ade134571cb1cc1d38e327bd2815bebac58","observation_id":"c3925c78-3827-4e4f-9b6e-08c9c7d9153b","resolution":{"observed_at":"2026-08-11T12:26:08.904290Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.08103","last_updated":"2019-09-06T12:45:19Z","snapshot_observed_at":"2026-08-14T16:29:40.968764Z","submitted_at":"2019-05-20T13:32:43Z","title":"Matter power spectrum: from Ly$\\alpha$ forest to CMB scales","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.08103","snapshot_observed_at":"2026-08-11T12:26:08.909633Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.909633Z"},"links":{"cited_paper":"/paper/1905.08103","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:fe3d876eb604079ffe1f5d5dd18eaf726bb51203c66c02b759b81926cff27aa9","observation_id":"718c9ca5-bd79-4a70-876e-0ebf356c5c87","resolution":{"observed_at":"2026-08-11T12:26:08.909633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12220","last_updated":"2025-01-24T17:14:52Z","snapshot_observed_at":"2026-08-16T13:51:13.547055Z","submitted_at":"2024-05-20T17:59:59Z","title":"CMB-HD as a Probe of Dark Matter on Sub-Galactic Scales","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12220","snapshot_observed_at":"2026-08-11T12:26:08.914668Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.914668Z"},"links":{"cited_paper":"/paper/2405.12220","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:4b105917681169bcaafed5ce7492f244a79c7371d308e3605bb92b6b1b1391f7","observation_id":"15b25411-88c7-4eca-ba1e-f100f2127eaf","resolution":{"observed_at":"2026-08-11T12:26:08.914668Z","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":"2026-08-11T12:26:08.919795Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.919795Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:9695e73fb18e4924229b09a22095a19071feabcb048ff866b830497e7dd44d90","observation_id":"c98d14aa-e10e-4210-a5dd-74ca5c1aae11","resolution":{"observed_at":"2026-08-11T12:26:08.919795Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.08215","last_updated":"2022-12-14T04:14:44Z","snapshot_observed_at":"2026-08-16T16:31:53.503509Z","submitted_at":"2022-09-17T02:09:33Z","title":"Report of the Topical Group on Cosmic Probes of Dark Matter for Snowmass 2021","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.08215","snapshot_observed_at":"2026-08-11T12:26:08.924850Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.924850Z"},"links":{"cited_paper":"/paper/2209.08215","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:5e71e4eff75c72a4055ea5de20c34a5a465447adeccee341ff1ff49e94491b38","observation_id":"d6887054-c191-4a3a-9c46-34de512f74df","resolution":{"observed_at":"2026-08-11T12:26:08.924850Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207047","last_updated":"2002-09-17T21:33:40Z","snapshot_observed_at":"2026-07-07T00:27:12.891058Z","submitted_at":"2002-07-02T19:08:42Z","title":"Separating the Early Universe from the Late Universe: cosmological parameter estimation beyond the black box","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207047","snapshot_observed_at":"2026-08-11T12:26:08.929888Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.929888Z"},"links":{"cited_paper":"/paper/astro-ph/0207047","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:b61033c1689cb60e32b1cae487bc4035ac9b6c19e3542824f42d3e593bdd2028","observation_id":"6a1b6fb4-d0a2-4ddd-b2f7-2f25b71b0756","resolution":{"observed_at":"2026-08-11T12:26:08.929888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0012324","last_updated":"2002-08-21T15:35:03Z","snapshot_observed_at":"2026-08-11T00:20:06.197676Z","submitted_at":"2000-12-14T19:29:32Z","title":"Towards a Precise Measurement of Matter Clustering: Lyman-alpha Forest Data at Redshifts 2-4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0012324","snapshot_observed_at":"2026-08-11T12:26:08.935695Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.935695Z"},"links":{"cited_paper":"/paper/astro-ph/0012324","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:fe5e52afb61b8db3c5541a0c8b4bea4c891f9254bcf7f74b37c93736c83f3964","observation_id":"67790afe-fde9-468d-a88d-b91a44cbd6ae","resolution":{"observed_at":"2026-08-11T12:26:08.935695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.07838","last_updated":"2017-11-24T17:09:58Z","snapshot_observed_at":"2026-08-14T21:04:46.982798Z","submitted_at":"2017-04-25T18:00:35Z","title":"\"Non-cold\" dark matter at small scales: a general approach","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.07838","snapshot_observed_at":"2026-08-11T12:26:08.940671Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.940671Z"},"links":{"cited_paper":"/paper/1704.07838","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:6f3cb8c515c6fe61a386c23b2651f1504399159dbeb74159fa323036ecadaac3","observation_id":"1de96594-ff9f-4e66-9ccc-de6511d8cc4b","resolution":{"observed_at":"2026-08-11T12:26:08.940671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.08371","last_updated":"2018-10-16T09:24:58Z","snapshot_observed_at":"2026-08-16T08:05:55.364773Z","submitted_at":"2018-06-21T18:04:22Z","title":"Novel constraints on non-cold (non-thermal) Dark Matter from Lyman-$\\alpha$ forest data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.08371","snapshot_observed_at":"2026-08-11T12:26:08.946382Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.946382Z"},"links":{"cited_paper":"/paper/1806.08371","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:e4b1dba2453097e7be7fcb3a2129ba4d0abc1aa4c7ebbe99a4e3dcedbdb7eab6","observation_id":"4a1710ee-7567-4692-af47-df513c826b4f","resolution":{"observed_at":"2026-08-11T12:26:08.946382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.02876","last_updated":"2023-04-05T23:50:50Z","snapshot_observed_at":"2026-08-16T16:47:51.736725Z","submitted_at":"2022-07-06T18:00:05Z","title":"Small-scale clumping of dark matter and the mean free path of ionizing photons at $z=6$","version":2},"cited_work":{"arxiv_id":"2207.02876","doi":null,"metadata_source":"pith","pith_arxiv_id":"2207.02876","snapshot_observed_at":"2026-08-11T12:26:09.700031Z","title":"Small-scale clumping of dark matter and the mean free path of ionizing photons at $z=6$","venue":"astro-ph.CO","work_id":"f090818a-6068-4fe0-b208-08fecdd03fef","year":2022},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.951982Z"},"links":{"cited_paper":"/paper/2207.02876","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:536297007414ddcae0d604338e9ff6de14f5f20a5b081a8b98759e3602b96af5","observation_id":"61b31ffb-5566-4343-aeb2-a84f6641a52a","resolution":{"observed_at":"2026-08-11T12:26:09.705152Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.04533","last_updated":"2024-02-15T15:11:47Z","snapshot_observed_at":"2026-08-16T15:02:11.045908Z","submitted_at":"2023-09-08T18:00:07Z","title":"Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.04533","snapshot_observed_at":"2026-08-11T12:26:08.957703Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.957703Z"},"links":{"cited_paper":"/paper/2309.04533","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:23cfe84ad2af62fe2691b9c3c481d0e6922b0ba23853061ab19657e69cb9fbc4","observation_id":"1f1e9ec6-93b1-4b81-bf2f-4edb21f45b68","resolution":{"observed_at":"2026-08-11T12:26:08.957703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.10000","last_updated":"2020-06-16T20:15:54Z","snapshot_observed_at":"2026-08-17T04:18:54.940446Z","submitted_at":"2019-04-22T18:00:05Z","title":"Constraints on Dark Matter Microphysics from the Milky Way Satellite Population","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.10000","snapshot_observed_at":"2026-08-11T12:26:08.962973Z","title":"and Gluscevic, Vera and Boddy, Kimberly K","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.962973Z"},"links":{"cited_paper":"/paper/1904.10000","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:1495834da2762da5efb11bb399a61c5637f4e70779a6ef6176e5457e2b3b24ad","observation_id":"57fa8940-186f-4c6b-a2e4-6e90eb5faaaa","resolution":{"observed_at":"2026-08-11T12:26:08.962973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.13161","last_updated":"2022-04-01T14:27:37Z","snapshot_observed_at":"2026-08-16T22:12:29.845942Z","submitted_at":"2021-10-25T18:00:02Z","title":"New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.13161","snapshot_observed_at":"2026-08-11T12:26:08.968541Z","title":"and Blas, Diego, New Roads to the Small-scale Universe: Measurements of the Clustering of Matter with the High-redshift UV Galaxy Luminosity Function, Astrophys","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.968541Z"},"links":{"cited_paper":"/paper/2110.13161","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:3ced9260c61c507a87394fad0e5b2c54135cbc81d478ae4805659d1fa6184d5a","observation_id":"9f0f8203-8ab5-40d4-b8ee-8bb008932f7d","resolution":{"observed_at":"2026-08-11T12:26:08.968541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.04284","last_updated":"2016-10-13T22:34:28Z","snapshot_observed_at":"2026-08-14T21:35:18.755588Z","submitted_at":"2016-10-13T22:34:28Z","title":"A Bump in the Blue Axion Isocurvature Spectrum","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.04284","snapshot_observed_at":"2026-08-11T12:26:08.975541Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.975541Z"},"links":{"cited_paper":"/paper/1610.04284","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:ca0a7220f08a77ad8f0530a70d19fb763dfa661299465cfa2b0b168ba6146984","observation_id":"a25165c0-aeee-4a60-959c-a379a4f9c0ec","resolution":{"observed_at":"2026-08-11T12:26:08.975541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.09456","last_updated":"2023-07-24T18:56:26Z","snapshot_observed_at":"2026-08-16T15:23:31.666399Z","submitted_at":"2023-06-15T19:22:49Z","title":"Search for Isocurvature with Large-scale Structure: A Forecast for Euclid and MegaMapper using EFTofLSS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.09456","snapshot_observed_at":"2026-08-11T12:26:08.981628Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.981628Z"},"links":{"cited_paper":"/paper/2306.09456","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:89c9f813a66e5ba3081dfaf5bec2030b597bc85bc397cf0fd5f5fc03779d5c03","observation_id":"7ae9d7dc-c49c-4b40-be05-9f2b692bc151","resolution":{"observed_at":"2026-08-11T12:26:08.981628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.04991","last_updated":"2025-03-13T10:55:55Z","snapshot_observed_at":"2026-08-16T13:27:28.961708Z","submitted_at":"2024-08-09T10:50:18Z","title":"Searching for blue in the dark","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.04991","snapshot_observed_at":"2026-08-11T12:26:08.987404Z","title":"and Raccanelli, Alvise and Bartolo, Nicola, Searching for blue in the dark,2408.04991","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.987404Z"},"links":{"cited_paper":"/paper/2408.04991","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:95aa0086d24bc63df63cec6bdf07b3277e17a9b37ab6cfd7b48742352dd3b21a","observation_id":"02f86f19-4ccf-4aa7-92a0-c365c8dc3ed5","resolution":{"observed_at":"2026-08-11T12:26:08.987404Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0005123","last_updated":"2000-12-22T19:12:29Z","snapshot_observed_at":"2026-07-07T03:48:27.439970Z","submitted_at":"2000-05-12T18:51:26Z","title":"Largest temperature of the radiation era and its cosmological implications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0005123","snapshot_observed_at":"2026-08-11T12:26:08.993504Z","title":"and Riotto, Antonio, Largest temperature of the radiation era and its cosmological implications, Phys","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:08.993504Z"},"links":{"cited_paper":"/paper/hep-ph/0005123","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:f3fa90ba2250a2bff4cba391d943bf15e9e4987f12acbbf644b1991c5090fdb4","observation_id":"6802cb4c-1732-4c45-b68b-495f3f2bdce1","resolution":{"observed_at":"2026-08-11T12:26:08.993504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.0536","last_updated":"2011-09-26T21:46:06Z","snapshot_observed_at":"2026-08-15T04:44:52.856420Z","submitted_at":"2011-06-02T23:57:55Z","title":"Reheating Effects in the Matter Power Spectrum and Implications for Substructure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.0536","snapshot_observed_at":"2026-08-11T12:26:09.000797Z","title":"and Sigurdson, Kris, Reheating Effects in the Matter Power Spectrum and Implications for Substructure, Phys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.000797Z"},"links":{"cited_paper":"/paper/1106.0536","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:3edf09efd6ce077f2685b6bf2baf917c4cb4ffc3aefa83300afd4a8b10731ab6","observation_id":"676665d5-1625-4e31-9dc3-bb2a6b4f5f8b","resolution":{"observed_at":"2026-08-11T12:26:09.000797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.05927","last_updated":"2017-07-10T19:59:06Z","snapshot_observed_at":"2026-08-14T21:39:08.405736Z","submitted_at":"2016-09-19T20:22:35Z","title":"Quasidecoupled state for dark matter in nonstandard thermal histories","version":2},"cited_work":{"arxiv_id":"1609.05927","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.05927","snapshot_observed_at":"2026-08-11T12:26:09.546618Z","title":"Quasidecoupled state for dark matter in nonstandard thermal histories","venue":"astro-ph.CO","work_id":"98f30b30-6f37-4d5d-a313-fe2dc461e64f","year":2016},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.006675Z"},"links":{"cited_paper":"/paper/1609.05927","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:2d3d7e7a686c935b9113dd1c0651828e068f12e61185ab2e58ce4479b65b28ba","observation_id":"a4dbdd8b-664f-47af-9a8b-c0bcdaf1b0d9","resolution":{"observed_at":"2026-08-11T12:26:09.552608Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.05007","last_updated":"2018-03-13T19:07:18Z","snapshot_observed_at":"2026-08-16T08:05:56.033306Z","submitted_at":"2017-11-14T09:16:09Z","title":"Dark Matter Production in an Early Matter Dominated Era","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.05007","snapshot_observed_at":"2026-08-11T12:26:09.011988Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.011988Z"},"links":{"cited_paper":"/paper/1711.05007","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:8a718a6823909c975ebd26466d5c48c34ff1cd58f216f9fa7170c285cd15a9cf","observation_id":"db92f281-cb15-41c1-9162-e223f0005fed","resolution":{"observed_at":"2026-08-11T12:26:09.011988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.08553","last_updated":"2020-01-03T04:57:43Z","snapshot_observed_at":"2026-08-16T01:46:19.588773Z","submitted_at":"2019-10-18T18:00:00Z","title":"Breaking a dark degeneracy: The gamma-ray signature of early matter domination","version":2},"cited_work":{"arxiv_id":"1910.08553","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.08553","snapshot_observed_at":"2026-08-11T12:26:09.507664Z","title":"Breaking a dark degeneracy: The gamma-ray signature of early matter domination","venue":"astro-ph.CO","work_id":"ce1e37cd-93aa-4913-93b1-09bf6e4c8e4e","year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.016915Z"},"links":{"cited_paper":"/paper/1910.08553","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:c857ae8fcc7ae580c92d59882a75774598c8ea7e3e417512716f6590b9f2dcde","observation_id":"01e9ae3e-e566-404d-ae8c-befd60bfadeb","resolution":{"observed_at":"2026-08-11T12:26:09.512815Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.04311","last_updated":"2021-05-04T19:26:49Z","snapshot_observed_at":"2026-07-06T09:46:00.543674Z","submitted_at":"2020-08-10T18:00:01Z","title":"Cannibal domination and the matter power spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.04311","snapshot_observed_at":"2026-08-11T12:26:09.022578Z","title":"and Ralegankar, Pranjal and Shelton, Jessie, Cannibal domination and the matter power spectrum, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.022578Z"},"links":{"cited_paper":"/paper/2008.04311","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:5619149619ea124048d138b4947b8df4aca2d2bcfe103e22c6d8d160bd43f228","observation_id":"83304915-738a-4ed0-a07d-c154387eac6c","resolution":{"observed_at":"2026-08-11T12:26:09.022578Z","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":"2026-08-11T12:26:09.028560Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.028560Z"},"links":{"citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:f67c701dd05b09880a4bca245572dea350aee4333f6b3001142d5a1303191596","observation_id":"d8eaba13-1663-4a70-919a-a404919a3316","resolution":{"observed_at":"2026-08-11T12:26:09.028560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9308292","last_updated":"1993-08-18T19:00:23Z","snapshot_observed_at":"2026-08-03T06:48:51.556829Z","submitted_at":"1993-08-18T19:00:23Z","title":"Cosmological Implications of Dynamical Supersymmetry Breaking","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9308292","snapshot_observed_at":"2026-08-11T12:26:09.040120Z","title":"and Nelson, Ann E., Cosmological implications of dynamical supersymmetry breaking, Phys","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.040120Z"},"links":{"cited_paper":"/paper/hep-ph/9308292","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:ddc0c1af54667dde944d2d00537387d8669ca7be4e8911062abb8a8b8ffdeed7","observation_id":"09f8a1f6-34c2-4327-8b80-ce4c3c7269a2","resolution":{"observed_at":"2026-08-11T12:26:09.040120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9308325","last_updated":"1993-08-24T00:05:07Z","snapshot_observed_at":"2026-07-07T04:15:56.490202Z","submitted_at":"1993-08-24T00:05:07Z","title":"Model Independent Properties and Cosmological Implications of the Dilaton and Moduli Sectors of 4-d Strings","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9308325","snapshot_observed_at":"2026-08-11T12:26:09.045347Z","title":"and Casas, J","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.045347Z"},"links":{"cited_paper":"/paper/hep-ph/9308325","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:d1f3796f2fccc61471788fb4e3fcd62e665c17c1c9cae15bb35034d771214fcd","observation_id":"ecae310d-e522-43a1-bb4e-ce6b51f585f9","resolution":{"observed_at":"2026-08-11T12:26:09.045347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0602081","last_updated":"2006-02-21T11:40:38Z","snapshot_observed_at":"2026-07-07T04:10:12.548715Z","submitted_at":"2006-02-09T13:20:14Z","title":"Gravitino Production from Heavy Moduli Decay and Cosmological Moduli Problem Revived","version":2},"cited_work":{"arxiv_id":"hep-ph/0602081","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0602081","snapshot_observed_at":"2026-08-11T12:26:09.438889Z","title":"Gravitino Production from Heavy Moduli Decay and Cosmological Moduli Problem Revived","venue":"hep-ph","work_id":"040fc817-4af1-48f1-90d6-abf674fcc446","year":2006},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.050820Z"},"links":{"cited_paper":"/paper/hep-ph/0602081","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:612af4c98f1345c2b2ceb17abb022dbd819b5a8aadaaf7bef67d55479321665c","observation_id":"c3df690a-1acd-4f72-bbba-fe281a41d7e0","resolution":{"observed_at":"2026-08-11T12:26:09.443988Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0605030","last_updated":"2006-06-01T15:25:28Z","snapshot_observed_at":"2026-07-07T04:10:52.885684Z","submitted_at":"2006-05-02T20:47:47Z","title":"Moduli decay in the hot early Universe","version":2},"cited_work":{"arxiv_id":"hep-ph/0605030","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0605030","snapshot_observed_at":"2026-08-11T12:26:09.417500Z","title":"Moduli decay in the hot early Universe","venue":"hep-ph","work_id":"ce585d24-e1a7-4883-896f-e3a803e22e16","year":2006},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.056575Z"},"links":{"cited_paper":"/paper/hep-ph/0605030","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:b7521315b91be5e78b3e5ce4e97a1950d8162895bd5d3dd8bdc86edf627f02f8","observation_id":"1d0ed9f7-94b8-4323-ad99-dfaf16c63a05","resolution":{"observed_at":"2026-08-11T12:26:09.423138Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9805405","last_updated":"2005-08-12T16:39:02Z","snapshot_observed_at":"2026-07-07T04:29:33.482732Z","submitted_at":"1998-05-20T22:50:30Z","title":"Radiative Decay of a Long-Lived Particle and Big-Bang Nucleosynthesis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9805405","snapshot_observed_at":"2026-08-11T12:26:09.061777Z","title":"and Kohri, Kazunori and Moroi, Takeo, Radiative decay of a longlived particle and big bang nucleosynthesis, Phys","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.061777Z"},"links":{"cited_paper":"/paper/hep-ph/9805405","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:5e556e8f6ccfb87ed80556b8f83a8036bf4e6097ce517e75a1c45161f277a230","observation_id":"c415ff7b-7093-49cf-b25d-ec86887af712","resolution":{"observed_at":"2026-08-11T12:26:09.061777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0211258","last_updated":"2002-11-12T17:46:01Z","snapshot_observed_at":"2026-08-05T20:40:16.418986Z","submitted_at":"2002-11-12T17:46:01Z","title":"Updated Nucleosynthesis Constraints on Unstable Relic Particles","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0211258","snapshot_observed_at":"2026-08-11T12:26:09.067492Z","title":"and Ellis, John R","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.067492Z"},"links":{"cited_paper":"/paper/astro-ph/0211258","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:f8ace1129e171fb878d48eeb25db2eaaffa4e0ff36173a9c556a15d5f755bbbb","observation_id":"490285ea-bdac-4dc8-8e4a-46c62c67f9ce","resolution":{"observed_at":"2026-08-11T12:26:09.067492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0408426","last_updated":"2005-03-02T00:24:33Z","snapshot_observed_at":"2026-07-07T00:44:15.134454Z","submitted_at":"2004-08-24T03:38:54Z","title":"Big-Bang Nucleosynthesis and Hadronic Decay of Long-Lived Massive Particles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0408426","snapshot_observed_at":"2026-08-11T12:26:09.072283Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.072283Z"},"links":{"cited_paper":"/paper/astro-ph/0408426","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:886ccab4b3832ce8cd37cb979f5a79be754a39554b3a9d541735f932d53cf5e0","observation_id":"fd5bf5eb-52d9-48e0-8844-8431505f29df","resolution":{"observed_at":"2026-08-11T12:26:09.072283Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0804.3745","last_updated":"2008-04-23T15:47:26Z","snapshot_observed_at":"2026-08-15T10:16:59.031549Z","submitted_at":"2008-04-23T15:47:26Z","title":"Big-Bang Nucleosynthesis and Gravitino","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0804.3745","snapshot_observed_at":"2026-08-11T12:26:09.078072Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.078072Z"},"links":{"cited_paper":"/paper/0804.3745","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:b8d8b61f06ce6ba0bafc5e59cf2efdc63a84e78d1032135fce99139f15a04fde","observation_id":"77cc9234-a1a4-4dae-95f0-dce6197b3839","resolution":{"observed_at":"2026-08-11T12:26:09.078072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.01211","last_updated":"2018-12-03T12:14:01Z","snapshot_observed_at":"2026-08-14T20:36:11.300466Z","submitted_at":"2017-09-05T01:48:13Z","title":"Revisiting Big-Bang Nucleosynthesis Constraints on Long-Lived Decaying Particles","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.01211","snapshot_observed_at":"2026-08-11T12:26:09.083276Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.083276Z"},"links":{"cited_paper":"/paper/1709.01211","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:78185e50458dead6f23800360960ae41ba5a37f23ae13cc16ba5dd2abecccf4e","observation_id":"0db62f2e-1cf1-46ae-9ec2-c446b172e888","resolution":{"observed_at":"2026-08-11T12:26:09.083276Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07688","last_updated":"2024-11-25T17:56:50Z","snapshot_observed_at":"2026-08-16T14:43:39.551884Z","submitted_at":"2023-11-13T19:13:07Z","title":"Updated Big Bang Nucleosynthesis Bounds on Long-lived Particles from Dark Sectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.07688","snapshot_observed_at":"2026-08-11T12:26:09.088533Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.088533Z"},"links":{"cited_paper":"/paper/2311.07688","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:c44b18efb95713bd7cc89f038b88259570a86f72ddf0c67445578029b8aa508d","observation_id":"13fd440e-626d-4efd-85d0-c2f04e927114","resolution":{"observed_at":"2026-08-11T12:26:09.088533Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.00672","last_updated":"2015-11-02T20:49:57Z","snapshot_observed_at":"2026-08-14T22:25:10.644894Z","submitted_at":"2015-11-02T20:49:57Z","title":"Bounds on very low reheating scenarios after Planck","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.00672","snapshot_observed_at":"2026-08-11T12:26:09.093738Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.093738Z"},"links":{"cited_paper":"/paper/1511.00672","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:fc812121b472357745ed9546a9e50a5bf911ab56fb93b270205d81e16236ee67","observation_id":"3f745944-bfa2-4e10-abb9-6d3ab9d5455b","resolution":{"observed_at":"2026-08-11T12:26:09.093738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.08534","last_updated":"2021-01-02T03:10:22Z","snapshot_observed_at":"2026-08-16T18:58:16.423917Z","submitted_at":"2020-12-15T19:00:03Z","title":"Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.08534","snapshot_observed_at":"2026-08-11T12:26:09.099572Z","title":"and Casertano, Stefano and Yuan, Wenlong and Bowers, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.099572Z"},"links":{"cited_paper":"/paper/2012.08534","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:799f2fb629b36805dd22222ed53f9511aec61c0d14c64fb6182bc05db842f2ca","observation_id":"a6cccc37-0179-4a42-ba4b-3c731c15b214","resolution":{"observed_at":"2026-08-11T12:26:09.099572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01309","last_updated":"2016-11-06T23:41:15Z","snapshot_observed_at":"2026-08-14T21:45:33.346929Z","submitted_at":"2016-08-03T20:00:01Z","title":"Early dark energy, the Hubble-parameter tension, and the string axiverse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01309","snapshot_observed_at":"2026-08-11T12:26:09.105353Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.105353Z"},"links":{"cited_paper":"/paper/1608.01309","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:bb9e9e0fb2b5a6c9b6e12bd5c1cfd0f7a854471e8f35bedd8ab15e7a71750991","observation_id":"409ec080-5549-4e10-b4ae-bf50aacb469d","resolution":{"observed_at":"2026-08-11T12:26:09.105353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.04083","last_updated":"2019-06-11T10:04:20Z","snapshot_observed_at":"2026-08-14T18:01:28.256190Z","submitted_at":"2018-11-09T19:00:00Z","title":"Early Dark Energy Can Resolve The Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.04083","snapshot_observed_at":"2026-08-11T12:26:09.110604Z","title":"and Karwal, Tanvi and Kamionkowski, Marc, Early Dark Energy Can Resolve The Hubble Tension, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.110604Z"},"links":{"cited_paper":"/paper/1811.04083","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:c9b9aee7955697053c877f0f5540e16878f50c053ae551ebddff8007f9f1bef8","observation_id":"6f4bf347-7c0a-49b0-a23a-848a41918ae8","resolution":{"observed_at":"2026-08-11T12:26:09.110604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06995","last_updated":"2019-08-19T18:00:08Z","snapshot_observed_at":"2026-08-17T06:03:23.038237Z","submitted_at":"2019-08-19T18:00:08Z","title":"Oscillating scalar fields and the Hubble tension: a resolution with novel signatures","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06995","snapshot_observed_at":"2026-08-11T12:26:09.116193Z","title":"and Poulin, Vivian and Amin, Mustafa A., Oscillating scalar fields and the Hubble tension: a resolution with novel signatures, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.116193Z"},"links":{"cited_paper":"/paper/1908.06995","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:10294f617c2d8debf1ebd3cc8ba4f6682487ddfa87e5b1666e0d33ca4b6e1fb3","observation_id":"23377524-f775-40d8-8daf-26fc9f23102a","resolution":{"observed_at":"2026-08-11T12:26:09.116193Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.10733","last_updated":"2021-03-03T11:10:28Z","snapshot_observed_at":"2026-08-13T21:32:29.554748Z","submitted_at":"2020-09-22T18:00:02Z","title":"Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.10733","snapshot_observed_at":"2026-08-11T12:26:09.122282Z","title":"and Poulin, Vivian, Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies, Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.122282Z"},"links":{"cited_paper":"/paper/2009.10733","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:4513feb52f2f52fd250e2a3667a98a5c74767a696fe0dcedcc2c2723e3d2b051","observation_id":"4891e197-4014-4d1a-aec0-e8eec9f0841f","resolution":{"observed_at":"2026-08-11T12:26:09.122282Z","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":"2026-08-16T02:57:47.718860Z","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":"2026-08-11T12:26:09.127367Z","title":"and Cyr-Racine, Francis-Yan and Dor´ e, Olivier, Neutrino puzzle: Anomalies, interactions, and cosmological tensions, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.127367Z"},"links":{"cited_paper":"/paper/1902.00534","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:3313f7f334d1c4f7966f9e0092133084e5e33f5f46b79fed0f674655211ae97f","observation_id":"196c0ec1-e455-4cfd-b691-10d5884dbb95","resolution":{"observed_at":"2026-08-11T12:26:09.127367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.06778","last_updated":"2025-06-18T17:15:46Z","snapshot_observed_at":"2026-08-17T20:20:40.659441Z","submitted_at":"2024-09-10T18:00:01Z","title":"Signatures of Very Early Dark Energy in the Matter Power Spectrum","version":2},"cited_work":{"arxiv_id":"2409.06778","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.06778","snapshot_observed_at":"2026-08-11T12:26:09.183858Z","title":"Signatures of Very Early Dark Energy in the Matter Power Spectrum","venue":"astro-ph.CO","work_id":"24c2d703-0441-4406-b98a-acd66cead9fc","year":2024},"citing_paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-11T12:26:09.132708Z"},"links":{"cited_paper":"/paper/2409.06778","citing_paper":"/paper/2412.14322"},"observation_digest":"sha256:e7b76350108de71025b518c898f5761eb1d1a2108893e5a4c51469e856db043b","observation_id":"7bddafd6-1b56-43a5-b93c-0278d12f3934","resolution":{"observed_at":"2026-08-11T12:26:09.191849Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2412.14322","last_updated":"2025-06-20T23:55:24Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T06:44:57.038564Z","submitted_at":"2024-12-18T20:37:50Z","title":"Free streaming of warm wave dark matter in modified expansion histories"},"reference_resolution":{"displayed":89,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":79,"verified_exact":9,"verified_fuzzy":0},"total_outbound_references":89},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 89 of 89 outbound references and 6 inbound Pith citation observations for arXiv:2412.14322."}