{"as_of":"2026-08-18T05:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e100a8a91484f3f26e7a6cf6c509240b88ed0e0abb1c12288226a28f7981d9a3","coverage":[{"denominator":85,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":85,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T14:28:01.559660Z","state":"measured"},{"denominator":99,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":99,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":14,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":14,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T00:18:02.137555Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T13:27:05.810571Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-14T13:43:27.302744Z","title":"Observing Dirac neutrinos in the cosmic microwave background","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"1908.04818","last_updated":"2020-03-11T20:58:42Z","snapshot_observed_at":"2026-08-17T07:27:39.516034Z","submitted_at":"2019-08-13T18:45:36Z","title":"Dark CP Violation and Gauged Lepton/Baryon Number for Electroweak Baryogenesis","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T13:43:27.302744Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/1908.04818"},"observation_digest":"sha256:682fdd897429e00ff35e7b0360ce3680e8755edd6a2722260ac6f729b38f6926","observation_id":"8b944121-ee72-4218-b960-f014e015ede5","resolution":{"observed_at":"2026-08-14T13:43:27.302744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-11T14:23:09.861533Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.12267","last_updated":"2025-07-02T13:35:16Z","snapshot_observed_at":"2026-08-12T19:41:39.332891Z","submitted_at":"2024-12-16T19:00:04Z","title":"Minimal Dirac seesaw dark matter","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T14:23:09.861533Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2412.12267"},"observation_digest":"sha256:0b3a7d68410ef7c0785cb96c81f64ce062b3bb551a527908328cfa5253aeba38","observation_id":"4cbe62d8-5350-47fd-a34f-b65a22abecc1","resolution":{"observed_at":"2026-08-11T14:23:09.861533Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-10T16:42:04.522403Z","title":"Abazajian and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.13150","last_updated":"2025-05-09T12:08:44Z","snapshot_observed_at":"2026-08-17T08:30:18.132130Z","submitted_at":"2025-01-22T19:00:00Z","title":"Electromagnetic leptogenesis with light-heavy sterile neutrinos","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-10T16:42:04.522403Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2501.13150"},"observation_digest":"sha256:b118ab28cae3e89c53c29f8fe3eaef77df5583d248622910056d49ca56a6d8a0","observation_id":"41d2c167-9adf-49fa-9f7d-de4b3e201dc7","resolution":{"observed_at":"2026-08-10T16:42:04.522403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-09T14:51:07.122310Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.01760","last_updated":"2025-06-05T05:43:35Z","snapshot_observed_at":"2026-08-17T23:39:25.938994Z","submitted_at":"2025-02-03T19:02:37Z","title":"Type-II Seesaw Mechanism for Dirac Neutrinos and its Implications on $N_{\\text{eff}}$ and Lepton Flavor Violation in a 3-3-1 model","version":5},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-09T14:51:07.122310Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2502.01760"},"observation_digest":"sha256:fd6fb3b40fd0298d17634b9eaaabe1433b02f3744dcfb9bcf309750cf7b9716c","observation_id":"bc91d913-9704-4024-b4ab-fd86bb3e233c","resolution":{"observed_at":"2026-08-09T14:51:07.122310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-07T20:54:27.995186Z","title":"Abazajian and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.09699","last_updated":"2025-04-28T09:41:56Z","snapshot_observed_at":"2026-08-13T03:57:06.902778Z","submitted_at":"2025-02-13T19:00:00Z","title":"Custodial Naturalness","version":2},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-08-07T20:54:27.995186Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2502.09699"},"observation_digest":"sha256:b7f4c95ae40d83ff366aa3e10660ec2a9f5103972e818774df35c84e0bd94d4d","observation_id":"2113558e-b4e1-4006-a5d6-b681d59bab6b","resolution":{"observed_at":"2026-08-07T20:54:27.995186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-07T18:46:02.122192Z","title":"Observing Dirac neutrinos in the cosmic microwave background,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.10318","last_updated":"2025-08-29T06:34:53Z","snapshot_observed_at":"2026-08-16T12:07:21.856592Z","submitted_at":"2025-02-14T17:23:14Z","title":"Effective theory of light Dirac neutrino portal dark matter with observable ${\\Delta N_{\\rm eff}}$","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-07T18:46:02.122192Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2502.10318"},"observation_digest":"sha256:3c5b3014c8333378b2f98830aefcd4766cc23f11cca1895f3d671fe89da4ff52","observation_id":"6c80421f-6582-4ba2-a35f-f93b32c88cc1","resolution":{"observed_at":"2026-08-07T18:46:02.122192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-15T23:29:59.001883Z","title":"Abazajian and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.04695","last_updated":"2025-05-07T18:00:03Z","snapshot_observed_at":"2026-08-16T12:07:51.026997Z","submitted_at":"2025-05-07T18:00:03Z","title":"Improved cosmological limits on $Z^\\prime$ models with light right-handed neutrinos","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T23:29:59.001883Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2505.04695"},"observation_digest":"sha256:d5ede12efed53fda740b26c5bee4a3c872919d375cd19e3fd2874a9f951a766c","observation_id":"c2895de3-28c0-4c96-ad37-b843b16e4bf5","resolution":{"observed_at":"2026-08-15T23:29:59.001883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":"1908.03286","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-07-10T13:27:05.810571Z","title":"Abazajian and J","venue":"hep-ph","work_id":"6bc066d0-aa76-40a7-9bfa-fa913a2d84ad","year":2019},"citing_paper":{"arxiv_id":"2506.23290","last_updated":"2026-04-17T09:16:11Z","snapshot_observed_at":"2026-08-16T19:20:08.201319Z","submitted_at":"2025-06-29T15:26:07Z","title":"Type II Seesaw Leptogenesis in a Majoron background","version":2},"reference_index":211,"source":"pdf_text","source_observed_at":"2026-05-19T07:47:44.372827Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2506.23290"},"observation_digest":"sha256:63ed7b48096dd1d5edf7a1067137e2cb552da8218ba7a4a422a7bdb6d1845ebb","observation_id":"d3299d7c-bc27-4b04-85ba-7efcc3cac060","resolution":{"observed_at":"2026-05-19T07:52:10.383937Z","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":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-06T17:15:42.128050Z","title":"Abazajian and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.11607","last_updated":"2025-07-15T18:00:00Z","snapshot_observed_at":"2026-08-16T06:49:23.888282Z","submitted_at":"2025-07-15T18:00:00Z","title":"Electromagnetic Dirac Cogenesis","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-06T17:15:42.128050Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2507.11607"},"observation_digest":"sha256:aed71e82d7c4957d40385a5e6d80fe33283f74d5c6a45da057afa0fe6c419780","observation_id":"3e6bfec9-2244-4963-ac0a-765d7427b1fb","resolution":{"observed_at":"2026-08-06T17:15:42.128050Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":"1908.03286","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-07-10T13:27:05.810571Z","title":"Abazajian and J","venue":"hep-ph","work_id":"6bc066d0-aa76-40a7-9bfa-fa913a2d84ad","year":2019},"citing_paper":{"arxiv_id":"2601.02458","last_updated":"2026-04-24T10:01:41Z","snapshot_observed_at":"2026-08-15T19:14:50.428226Z","submitted_at":"2026-01-05T18:57:49Z","title":"Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter","version":3},"reference_index":148,"source":"pdf_text","source_observed_at":"2026-05-16T17:29:31.382479Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2601.02458"},"observation_digest":"sha256:0c13d5be030f216f600b5961cb5278b8c75a9ab05eb6a62102c28e948cc9ccc5","observation_id":"3b888da7-b459-440e-b51d-2b113c8bfae4","resolution":{"observed_at":"2026-05-16T17:31:08.814622Z","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":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":"1908.03286","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-07-10T13:27:05.810571Z","title":"Abazajian and J","venue":"hep-ph","work_id":"6bc066d0-aa76-40a7-9bfa-fa913a2d84ad","year":2019},"citing_paper":{"arxiv_id":"2604.09356","last_updated":"2026-04-10T14:29:55Z","snapshot_observed_at":"2026-08-15T10:30:20.262269Z","submitted_at":"2026-04-10T14:29:55Z","title":"CMB signatures of gravity-mediated dark radiation in $\\mathbf{\\Delta N_{\\rm eff}}$","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-10T17:18:29.352423Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2604.09356"},"observation_digest":"sha256:80e02f7081cd0591965e8a3e5a836a28067286ea72870217371c7c399a6d5a56","observation_id":"becdf804-c13b-41d1-9903-7c1d0a194e25","resolution":{"observed_at":"2026-05-11T07:06:04.910585Z","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":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":"1908.03286","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-07-10T13:27:05.810571Z","title":"Abazajian and J","venue":"hep-ph","work_id":"6bc066d0-aa76-40a7-9bfa-fa913a2d84ad","year":2019},"citing_paper":{"arxiv_id":"2607.08082","last_updated":"2026-07-09T03:32:31Z","snapshot_observed_at":"2026-08-17T15:53:10.818796Z","submitted_at":"2026-07-09T03:32:31Z","title":"$Z^\\prime$ Portal Dark Matter with Observable $\\Delta N_{\\rm eff}$","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-10T13:24:30.519761Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2607.08082"},"observation_digest":"sha256:67a1563c8eb49c6744435561759b55f82442728382bf569ad6a948f8e6e69296","observation_id":"5f43e80b-d247-477c-89e6-04538019f65e","resolution":{"observed_at":"2026-07-10T13:27:05.812064Z","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":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-15T14:31:26.814265Z","title":"Observing Dirac Neutrinos in the Cosmic Microwave Background","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.07453","last_updated":"2026-08-07T17:46:01Z","snapshot_observed_at":"2026-08-16T08:22:36.354092Z","submitted_at":"2026-08-07T17:46:01Z","title":"Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics","version":1},"reference_index":190,"source":"pdf_text","source_observed_at":"2026-08-15T14:31:26.814265Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2608.07453"},"observation_digest":"sha256:63fbfd9c5f5ca5d85ab7d9f34220a8c5a17475cd9cd99db8381671b5dfc12dea","observation_id":"f0751715-a218-4ffb-9c5b-f72d6e37cbb5","resolution":{"observed_at":"2026-08-15T14:31:26.814265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03286","snapshot_observed_at":"2026-08-16T00:18:02.137555Z","title":"Abazajian and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2608.12483","last_updated":"2026-08-12T18:04:19Z","snapshot_observed_at":"2026-08-18T03:16:14.766281Z","submitted_at":"2026-08-12T18:04:19Z","title":"Singlet-Doublet fermion origin of dark matter, neutrino mass and inverse first-order electroweak phase transition","version":1},"reference_index":132,"source":"pdf_text","source_observed_at":"2026-08-16T00:18:02.137555Z"},"links":{"cited_paper":"/paper/1908.03286","citing_paper":"/paper/2608.12483"},"observation_digest":"sha256:11ba0cfe715dd7097444a8ef864d0457f535d879a9c6a3ae889cda6062567869","observation_id":"4964a15c-4652-4b35-a916-2455ae5bce9c","resolution":{"observed_at":"2026-08-16T00:18:02.137555Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1908.03286/citation-record","integrity":"/paper/1908.03286/integrity","json":"/paper/1908.03286/citation-record.json","paper":"/paper/1908.03286"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:00.904383Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.904383Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:23725c840ed6665a89e1bc3d285c902a7bd62756a6969eeefefc37d9b2af2a7f","observation_id":"d170a4ea-3150-4d64-8669-fdb9635ec623","resolution":{"observed_at":"2026-08-14T14:28:00.904383Z","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":"2026-08-14T14:28:00.913538Z","title":"This is a strong assumption since we technically only know that the Universe was at least ∼ 5 MeV hot [20], everything beyond being speculation","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.913538Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:dab6b08644dc761060fe559b20eb6bf59747499d0969b889a3047faa456d6429","observation_id":"417ecd11-3e64-4ae5-ad94-3a9d36649c37","resolution":{"observed_at":"2026-08-14T14:28:00.913538Z","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":"2026-08-14T14:28:00.922571Z","title":"To dilute three νR down to ∆Neﬀ < 0.06 via Eq","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.922571Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:22e745edf6f9169f3866e1d357db01f61bf5a2c0665c87a66735c2966dcb8b84","observation_id":"104161a9-9048-4cda-a78b-334deaf74331","resolution":{"observed_at":"2026-08-14T14:28:00.922571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9512139","last_updated":"1996-05-23T17:57:30Z","snapshot_observed_at":"2026-07-07T01:12:30.057746Z","submitted_at":"1995-12-20T22:29:37Z","title":"Cosmological-Parameter Determination with Microwave Background Maps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9512139","snapshot_observed_at":"2026-08-14T14:28:00.939017Z","title":"Cosmological parameter determination with microwave background maps ,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.939017Z"},"links":{"cited_paper":"/paper/astro-ph/9512139","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:e9376af1b131a88ce9b62767ad4e3e1f0a219ac85f0c53c9785cf5e2248c4b7d","observation_id":"f05ebed3-567f-4ac4-abaa-107bf0918a0a","resolution":{"observed_at":"2026-08-14T14:28:00.939017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-14T14:28:00.951893Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.951893Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:5cbbf825227e9c2d73bf64ce4d06dbcbfd035ac13abcd1b9be080d9337f4f13c","observation_id":"78326dae-2c3c-41b0-aafd-6919bf6e1257","resolution":{"observed_at":"2026-08-14T14:28:00.951893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0506164","last_updated":"2005-06-16T12:46:17Z","snapshot_observed_at":"2026-08-07T17:28:13.660004Z","submitted_at":"2005-06-16T12:46:17Z","title":"Relic neutrino decoupling including flavour oscillations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0506164","snapshot_observed_at":"2026-08-14T14:28:00.959881Z","title":"Relic neutrino decoupling including ﬂavor oscillations ,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.959881Z"},"links":{"cited_paper":"/paper/hep-ph/0506164","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:4172cb6dd1460345530b3b59fa6e47e696d0aa6a7ac5c34f1d3c0a44c2d7fd25","observation_id":"1b21ee38-34c0-4628-9999-dc91d6a89073","resolution":{"observed_at":"2026-08-14T14:28:00.959881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.02205","last_updated":"2016-03-27T14:45:25Z","snapshot_observed_at":"2026-08-15T19:48:12.793905Z","submitted_at":"2015-12-07T20:41:18Z","title":"Neutrino energy transport in weak decoupling and big bang nucleosynthesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.02205","snapshot_observed_at":"2026-08-14T14:28:00.973182Z","title":"Neutrino energy transport in weak decoupling and big bang nucleosynthesis ,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.973182Z"},"links":{"cited_paper":"/paper/1512.02205","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:d52a69a5c7f9763bf8eb9e02bcd2a0df845b2da0f7e500e823773eedd813eadb","observation_id":"c72056c4-d89d-41e6-94bd-2458a2b1ce03","resolution":{"observed_at":"2026-08-14T14:28:00.973182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.06986","last_updated":"2016-06-22T15:29:30Z","snapshot_observed_at":"2026-08-14T21:51:36.566366Z","submitted_at":"2016-06-22T15:29:30Z","title":"Relic neutrino decoupling with flavour oscillations revisited","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.06986","snapshot_observed_at":"2026-08-14T14:28:00.980526Z","title":"Relic neutrino decoupling with ﬂavour oscillations revisited ,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.980526Z"},"links":{"cited_paper":"/paper/1606.06986","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:120b3f1d0bbd652e744f7dbd05d36078f525ac0bf3e5a439fcef60ef8c32d142","observation_id":"7af8753b-a393-41f0-9a93-b62f4f278cae","resolution":{"observed_at":"2026-08-14T14:28:00.980526Z","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":"2026-08-14T14:28:00.988993Z","title":"Neutrino Physics from the Cosmic Microwave Background and Large-Scale Structure,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:00.988993Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:82af29a97874fb0fcfffeaf4b8f0beac6b92a3033719b01103c3e01dc4bfcc6f","observation_id":"755e6f34-941f-43c1-babf-d9ddf3328d72","resolution":{"observed_at":"2026-08-14T14:28:00.988993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04473","last_updated":"2019-07-10T01:01:01Z","snapshot_observed_at":"2026-08-10T23:33:51.688803Z","submitted_at":"2019-07-10T01:01:01Z","title":"CMB-S4 Science Case, Reference Design, and Project Plan","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04473","snapshot_observed_at":"2026-08-14T14:28:01.001298Z","title":"CMB-S4 Science Case, Reference Design, and Project Plan ,","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.001298Z"},"links":{"cited_paper":"/paper/1907.04473","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:ea7cca18db518d30f7a28e56f032500f1710cd3baa339a68e1336ce68eef1e75","observation_id":"2f7dc97b-0f9c-4e65-959e-911a05bb69c5","resolution":{"observed_at":"2026-08-14T14:28:01.001298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.08614","last_updated":"2016-11-05T21:55:37Z","snapshot_observed_at":"2026-08-17T21:45:11.526259Z","submitted_at":"2016-04-28T20:52:00Z","title":"A New Target for Cosmic Axion Searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.08614","snapshot_observed_at":"2026-08-14T14:28:01.009542Z","title":"New Target for Cosmic Axion Searches ,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.009542Z"},"links":{"cited_paper":"/paper/1604.08614","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:58629bfd7321ad2fd409b256845fc36cbe9e0375b965859ffb02fc05d085f6dd","observation_id":"77b896b7-9003-4dca-ad8a-cb85ddd93e75","resolution":{"observed_at":"2026-08-14T14:28:01.009542Z","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":"2026-08-14T14:28:01.016202Z","title":"Do Neutrino Rest Masses Aﬀect Cosmological Helium Production?,","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.016202Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:64f03ecf430cef0f8da2dde0398fe19914ebff68670c583400952eb2fe8c2dcc","observation_id":"a85b4bfe-f426-4bcd-8b8b-041c1fc44dea","resolution":{"observed_at":"2026-08-14T14:28:01.016202Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.317918Z","title":"Right-handed Neutrino Interactions in the Early Universe,","venue":null,"work_id":"2698ac06-6c63-483f-ac6e-16928d892080","year":1981},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.024832Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:4bd30a4048563b8a75a978487af91d4483d1cd798d7b17d4f31bc220f4b1b23a","observation_id":"ea8259bd-eca5-4368-8173-b6472c39c928","resolution":{"observed_at":"2026-08-14T14:28:04.325852Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.292398Z","title":"Cosmological Constraints on Superweak Particles ,","venue":null,"work_id":"d1e25004-843e-410c-b03d-5fc1aa5646d3","year":1979},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.033517Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:21ecb4521ee0b827ce1c372061d1a9e2a05a582a3c7f89dcf8489a0c242474ab","observation_id":"ead426ac-df3c-408b-ab5d-ffdce69decc5","resolution":{"observed_at":"2026-08-14T14:28:04.298803Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.271373Z","title":"Limits on New Superweakly Interacting Particles from Primordial Nucleosynthesis,","venue":null,"work_id":"d0741715-cfba-4283-9151-203e3513701c","year":1981},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.044320Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:73a9022204afdfe6dab5137e4471add6ab1b8ea40ec2005003bc630dd07cb5e1","observation_id":"5f98ad40-b8de-4936-8655-2c8f038e97d8","resolution":{"observed_at":"2026-08-14T14:28:04.278489Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.242819Z","title":"Cosmology and Elementary Particles,","venue":null,"work_id":"41d787de-4044-4ace-b976-f81bd1a1b590","year":1981},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.053642Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:7e42196eaa5d9c9ea685a99d3de5dbaddc0a5e66a82e0a9260302c446726de06","observation_id":"f3fc2c75-6fcc-4ee5-9b34-a7ae8d8fcd0a","resolution":{"observed_at":"2026-08-14T14:28:04.249721Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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/9905320","last_updated":"1999-05-25T19:41:33Z","snapshot_observed_at":"2026-07-07T01:26:23.951745Z","submitted_at":"1999-05-25T19:41:33Z","title":"Primordial Nucleosynthesis: Theory and Observations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9905320","snapshot_observed_at":"2026-08-14T14:28:01.059149Z","title":"Primordial nucleosynthesis: Theory and observations ,","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.059149Z"},"links":{"cited_paper":"/paper/astro-ph/9905320","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:8f226eac8efa32c196cec9d1b804fa105febb6a40a97b98c9055ac5a832aeed5","observation_id":"35d1f095-3ca1-4b3f-8bdf-5c455391f76a","resolution":{"observed_at":"2026-08-14T14:28:01.059149Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0202122","last_updated":"2002-04-19T20:15:29Z","snapshot_observed_at":"2026-08-16T16:04:09.117875Z","submitted_at":"2002-02-13T15:46:20Z","title":"Neutrinos in cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0202122","snapshot_observed_at":"2026-08-14T14:28:01.067060Z","title":"Neutrinos in cosmology,","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.067060Z"},"links":{"cited_paper":"/paper/hep-ph/0202122","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:38aba8a08ef6e278a9fd7359efbdfcad31f77cea3a0d614532b2098a030b40b5","observation_id":"0876c8f5-a947-4439-9aca-5beee6b43afa","resolution":{"observed_at":"2026-08-14T14:28:01.067060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2333","last_updated":"2012-08-03T21:57:32Z","snapshot_observed_at":"2026-08-15T20:11:14.482750Z","submitted_at":"2011-04-12T20:03:59Z","title":"How Massless Neutrinos Affect the Cosmic Microwave Background Damping Tail","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.2333","snapshot_observed_at":"2026-08-14T14:28:01.073212Z","title":"How Massless Neutrinos Aﬀect the Cosmic Microwave Background Damping Tail ,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.073212Z"},"links":{"cited_paper":"/paper/1104.2333","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:a893cfe1eb5f40fd06aecc83b4273d72f3b55016ca4f3619f820dd4b7dbedec1","observation_id":"b139a309-e83c-467f-ba03-45f26cb3080d","resolution":{"observed_at":"2026-08-14T14:28:01.073212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.07863","last_updated":"2015-08-14T22:39:45Z","snapshot_observed_at":"2026-08-14T22:54:45.738076Z","submitted_at":"2015-03-26T20:00:20Z","title":"A First Detection of the Acoustic Oscillation Phase Shift Expected from the Cosmic Neutrino Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.07863","snapshot_observed_at":"2026-08-14T14:28:01.079306Z","title":"First Detection of the Acoustic Oscillation Phase Shift Expected from the Cosmic Neutrino Background ,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.079306Z"},"links":{"cited_paper":"/paper/1503.07863","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:48af9272fa694677a4540c0e6f47f2499ec639da518c374f87c5ec45966a9996","observation_id":"5ce566d9-f09c-488b-b978-7cefdb90ba3a","resolution":{"observed_at":"2026-08-14T14:28:01.079306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.2973","last_updated":"2014-07-10T21:32:57Z","snapshot_observed_at":"2026-08-14T23:27:08.853027Z","submitted_at":"2014-07-10T21:32:57Z","title":"SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2973","snapshot_observed_at":"2026-08-14T14:28:01.086552Z","title":"SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope ,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.086552Z"},"links":{"cited_paper":"/paper/1407.2973","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:9447887db850f1ecee775acb9fa717047d853c3775f5a3b916911e310a20e384","observation_id":"e328e108-36cd-4cd9-ba71-3bccbdac6580","resolution":{"observed_at":"2026-08-14T14:28:01.086552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.08284","last_updated":"2019-07-17T00:52:52Z","snapshot_observed_at":"2026-08-15T00:17:47.964796Z","submitted_at":"2019-07-17T00:52:52Z","title":"The Simons Observatory: Astro2020 Decadal Project Whitepaper","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.08284","snapshot_observed_at":"2026-08-14T14:28:01.093261Z","title":"The Simons Observatory: Astro2020 Decadal Project Whitepaper,","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.093261Z"},"links":{"cited_paper":"/paper/1907.08284","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:48258109cf33fd97d2715f6f0e2948ce00f98eccff5962b557c4d4d3cf77e7fe","observation_id":"e9198ef4-078b-4a73-be9f-512a20a648d2","resolution":{"observed_at":"2026-08-14T14:28:01.093261Z","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":"2026-08-14T14:28:01.102824Z","title":"Bounds on very low reheating scenarios after Planck ,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.102824Z"},"links":{"cited_paper":"/paper/1511.00672","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:1b7668c150ae2eb904f4b6fd27df7a993b07fa8aad3433d9add9971e1965a00a","observation_id":"03889990-8f1d-4d5c-95c2-ee9d01a86fba","resolution":{"observed_at":"2026-08-14T14:28:01.102824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.221304Z","title":"Decaying Particles Do Not Heat Up the Universe ,","venue":null,"work_id":"e1b38f10-4ee6-4143-9265-b0ca93fb8d3e","year":1985},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.112188Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:630f15480b89af95e8f4d76a69b1e42b2d3599827eb47caff8ac82edc514ecff","observation_id":"939f5f9b-be1f-4886-996a-181a3810779b","resolution":{"observed_at":"2026-08-14T14:28:04.228700Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"0912.4415","last_updated":"2010-05-12T13:21:30Z","snapshot_observed_at":"2026-08-15T05:30:33.780464Z","submitted_at":"2009-12-22T18:41:32Z","title":"keV sterile neutrino dark matter in gauge extensions of the standard model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0912.4415","snapshot_observed_at":"2026-08-14T14:28:01.118000Z","title":"keV sterile neutrino Dark Matter in gauge extensions of the Standard Model,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.118000Z"},"links":{"cited_paper":"/paper/0912.4415","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:a5e4314dc1118e454a15ba7c1b5c7a54edc12d1f4f9acd33414c4c35621ac6a3","observation_id":"e308713e-79d4-4b88-a106-5e5998792211","resolution":{"observed_at":"2026-08-14T14:28:01.118000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00481","last_updated":"2016-01-07T14:31:42Z","snapshot_observed_at":"2026-08-14T22:34:13.166111Z","submitted_at":"2015-09-01T20:12:51Z","title":"Non-thermal cosmic neutrino background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.00481","snapshot_observed_at":"2026-08-14T14:28:01.126534Z","title":"Nonthermal cosmic neutrino background,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.126534Z"},"links":{"cited_paper":"/paper/1509.00481","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:1746be2254270efd7819476f1fbaaf17eb33b4c8dfc322e4dc3ccf632541abf9","observation_id":"792bdffb-5b8b-4cb2-bb3e-a709196702b4","resolution":{"observed_at":"2026-08-14T14:28:01.126534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.02274","last_updated":"2015-12-25T02:25:34Z","snapshot_observed_at":"2026-08-14T22:33:22.511804Z","submitted_at":"2015-09-08T08:02:52Z","title":"Relic Right-handed Dirac Neutrinos and Implications for Detection of Cosmic Neutrino Background","version":2},"cited_work":{"arxiv_id":"1509.02274","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.02274","snapshot_observed_at":"2026-08-14T14:28:03.646541Z","title":"Relic Right-handed Dirac Neutrinos and Implications for Detection of Cosmic Neutrino Background","venue":"hep-ph","work_id":"4ac0c3a4-f313-48d3-b62e-315c1efb5677","year":2015},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.132575Z"},"links":{"cited_paper":"/paper/1509.02274","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:c5aeefb04f5f398e09a08a650540598466b3d83ae82737a7561c72519d57825c","observation_id":"d4b11664-da0b-4f74-b12c-da8d687b7d5f","resolution":{"observed_at":"2026-08-14T14:28:03.660251Z","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":"1610.01347","last_updated":"2016-12-08T06:54:12Z","snapshot_observed_at":"2026-08-14T21:36:39.726110Z","submitted_at":"2016-10-05T10:23:27Z","title":"Discriminating between Thermal and Nonthermal Cosmic Relic Neutrinos through Annual Modulation at PTOLEMY","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.01347","snapshot_observed_at":"2026-08-14T14:28:01.138739Z","title":"Discriminating between thermal and nonthermal cosmic relic neutrinos through an annual modulation at PTOLEMY ,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.138739Z"},"links":{"cited_paper":"/paper/1610.01347","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:38a13a39bf4a5a4623f96316ef128383c97dd52738f914f27930276be814b115","observation_id":"bd573afa-2b24-408d-9fee-b16c382750a2","resolution":{"observed_at":"2026-08-14T14:28:01.138739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.01892","last_updated":"2018-08-06T13:35:52Z","snapshot_observed_at":"2026-08-14T18:44:07.643982Z","submitted_at":"2018-08-06T13:35:52Z","title":"PTOLEMY: A Proposal for Thermal Relic Detection of Massive Neutrinos and Directional Detection of MeV Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.01892","snapshot_observed_at":"2026-08-14T14:28:01.144919Z","title":"PTOLEMY: A Proposal for Thermal Relic Detection of Massive Neutrinos and Directional Detection of MeV Dark Matter,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.144919Z"},"links":{"cited_paper":"/paper/1808.01892","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:c17b9c190eb8337ecdb1cb994c986226b89dda234b34c35e456a9559ecb85972","observation_id":"50a3ee28-be6b-4768-8514-97c615dab62e","resolution":{"observed_at":"2026-08-14T14:28:01.144919Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0806.0876","last_updated":"2008-06-30T23:11:19Z","snapshot_observed_at":"2026-08-15T10:13:55.190960Z","submitted_at":"2008-06-04T23:47:53Z","title":"Heavy Majorana Neutrinos in the Effective Lagrangian Description: Application to Hadron Colliders","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.0876","snapshot_observed_at":"2026-08-14T14:28:01.154700Z","title":"Heavy Majorana Neutrinos in the Eﬀective Lagrangian Description: Application to Hadron Colliders ,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.154700Z"},"links":{"cited_paper":"/paper/0806.0876","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:27a9810a52a118edecfd7d1aaf7434bf974f55e2e997fb65a0276d5d39fa305a","observation_id":"5bd0f548-eb1c-4e14-b7b4-bfb688bfeaaa","resolution":{"observed_at":"2026-08-14T14:28:01.154700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.3244","last_updated":"2009-04-21T13:00:33Z","snapshot_observed_at":"2026-08-15T05:50:06.982397Z","submitted_at":"2009-04-21T13:00:33Z","title":"Right-handed neutrino magnetic moments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.3244","snapshot_observed_at":"2026-08-14T14:28:01.166157Z","title":"Right-handed neutrino magnetic moments ,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.166157Z"},"links":{"cited_paper":"/paper/0904.3244","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:4c6b701b77d9443f46d885592c0c97337b8b6097791dc47259c05f2c7a991175","observation_id":"1b39afd8-bf74-4de4-9b36-c07f956dee33","resolution":{"observed_at":"2026-08-14T14:28:01.166157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05264","last_updated":"2016-09-21T07:47:30Z","snapshot_observed_at":"2026-08-14T22:47:52.233436Z","submitted_at":"2015-05-20T07:27:33Z","title":"Dimension Seven Operators in Standard Model with Right handed Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.05264","snapshot_observed_at":"2026-08-14T14:28:01.173795Z","title":"Dimension-seven operators in the standard model with right handed neutrinos,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.173795Z"},"links":{"cited_paper":"/paper/1505.05264","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:07cd0eecc899deccca2d23d1b992671bd938d47c8b882821c051fe9962cca7b7","observation_id":"08e0fcd8-ef47-4d9d-96a3-9dc47b867e26","resolution":{"observed_at":"2026-08-14T14:28:01.173795Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.04527","last_updated":"2016-12-14T08:26:56Z","snapshot_observed_at":"2026-08-17T20:30:47.706520Z","submitted_at":"2016-12-14T08:26:56Z","title":"Operators up to Dimension Seven in Standard Model Effective Field Theory Extended with Sterile Neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.04527","snapshot_observed_at":"2026-08-14T14:28:01.182372Z","title":"Operators up to Dimension Seven in Standard Model Eﬀective Field Theory Extended with Sterile Neutrinos ,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.182372Z"},"links":{"cited_paper":"/paper/1612.04527","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:dcaf3e7744e59daf5b238a8043514ab3eb3f879a265f9ae6bef317c63d7cbcd9","observation_id":"c3f3d487-b5e1-4dfa-97a5-cdea3d37adfc","resolution":{"observed_at":"2026-08-14T14:28:01.182372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.08699","last_updated":"2019-09-04T11:47:50Z","snapshot_observed_at":"2026-08-17T16:57:46.750036Z","submitted_at":"2019-05-21T15:29:09Z","title":"General Neutrino Interactions from an Effective Field Theory Perspective","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.08699","snapshot_observed_at":"2026-08-14T14:28:01.188817Z","title":"General Neutrino Interactions from an Eﬀective Field Theory Perspective,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.188817Z"},"links":{"cited_paper":"/paper/1905.08699","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:32faee9e137e1d519622c86ab1b7baa81862c093d057cf8fd658a0d5973065e5","observation_id":"6eed3e3f-4aef-4a59-a4bf-c77cf51bcd6f","resolution":{"observed_at":"2026-08-14T14:28:01.188817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.11375","last_updated":"2019-08-23T17:40:02Z","snapshot_observed_at":"2026-08-14T16:25:44.375920Z","submitted_at":"2019-05-27T17:59:02Z","title":"Probes of the Standard Model effective field theory extended with a right-handed neutrino","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.11375","snapshot_observed_at":"2026-08-14T14:28:01.197086Z","title":"Probes of the Standard Model eﬀective ﬁeld theory extended with a right-handed neutrino ,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.197086Z"},"links":{"cited_paper":"/paper/1905.11375","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:439f24cda7907422ce267f95e3d137af1912d405f4033532e37a2177b5142a4a","observation_id":"9bb82f1e-5798-43d5-95d0-c5317d24b1a8","resolution":{"observed_at":"2026-08-14T14:28:01.197086Z","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":"2026-08-14T14:28:01.204395Z","title":"An improved upper limit on the neutrino mass from a direct kinematic method by KATRIN ,","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.204395Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:6452ae3de1122f9870d156abdbf4ed8e04b1c4a41e06b2b29f3830be62456a97","observation_id":"16bdafd9-c0fd-415c-9a21-b6933a4dad31","resolution":{"observed_at":"2026-08-14T14:28:01.204395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00036","snapshot_observed_at":"2026-08-14T14:28:01.213145Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.213145Z"},"links":{"cited_paper":"/paper/1611.00036","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:7ad173696bd1cf32df92c6046b0ba1082b3ea4a90b3d17c6a18b8f8528fc78b2","observation_id":"54dc1be7-90c8-4f09-9941-89afa58d6db4","resolution":{"observed_at":"2026-08-14T14:28:01.213145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.5120","last_updated":"2011-01-23T00:56:11Z","snapshot_observed_at":"2026-08-15T05:02:12.603100Z","submitted_at":"2010-11-23T14:48:08Z","title":"Symmetries and Strings in Field Theory and Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.5120","snapshot_observed_at":"2026-08-14T14:28:01.219367Z","title":"Symmetries and Strings in Field Theory and Gravity ,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.219367Z"},"links":{"cited_paper":"/paper/1011.5120","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:c8f21a5f07f76cdc35a0397da00bc0601598064a8cf774fb327c8907ca670efd","observation_id":"55b2a61a-3c7c-44ab-8e4b-91df76ae8afb","resolution":{"observed_at":"2026-08-14T14:28:01.219367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.2901","last_updated":"2011-09-27T19:38:16Z","snapshot_observed_at":"2026-08-15T04:35:21.336759Z","submitted_at":"2011-09-13T20:00:08Z","title":"R-parity Conservation via the Stueckelberg Mechanism: LHC and Dark Matter Signals","version":2},"cited_work":{"arxiv_id":"1109.2901","doi":null,"metadata_source":"pith","pith_arxiv_id":"1109.2901","snapshot_observed_at":"2026-08-14T14:28:03.128891Z","title":"R-parity Conservation via the Stueckelberg Mechanism: LHC and Dark Matter Signals","venue":"hep-ph","work_id":"a1d8a91e-d9b3-4f40-907b-31a809e64361","year":2011},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.225490Z"},"links":{"cited_paper":"/paper/1109.2901","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:56dff71780d386772127801375589a77912eca29b1c6703293f7960f5b9e3d53","observation_id":"02c78a89-2f8c-4a0f-9a39-7e4077496102","resolution":{"observed_at":"2026-08-14T14:28:03.138271Z","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":"1408.6845","last_updated":"2014-11-10T09:05:32Z","snapshot_observed_at":"2026-08-14T23:21:34.152570Z","submitted_at":"2014-08-28T20:00:13Z","title":"Unbroken B-L Symmetry","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.6845","snapshot_observed_at":"2026-08-14T14:28:01.231789Z","title":"UnbrokenB−L symmetry,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.231789Z"},"links":{"cited_paper":"/paper/1408.6845","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:0fc69b829b128df6daac2b30b7fa197d835513b068d51eb1a05598f604e1df8f","observation_id":"1bc5d47e-5370-42db-912b-417fda4f7cda","resolution":{"observed_at":"2026-08-14T14:28:01.231789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.196743Z","title":"Limits On A New U(1) Coupling,","venue":null,"work_id":"2aaa49b5-9fdd-4717-98d3-82b4627028d9","year":1987},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.240108Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:3879e4d44e56c41b105e2c04bf26153aea27bae1157f1e0dbe9a483166bf191f","observation_id":"50d75d0d-116a-434b-ba33-5e689efd094a","resolution":{"observed_at":"2026-08-14T14:28:04.206434Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1202.6073","last_updated":"2015-08-03T15:27:01Z","snapshot_observed_at":"2026-08-15T04:17:58.176011Z","submitted_at":"2012-02-27T21:18:57Z","title":"Exploring nu signals in dark matter detectors","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.6073","snapshot_observed_at":"2026-08-14T14:28:01.245472Z","title":"Exploring nu Signals in Dark Matter Detectors ,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.245472Z"},"links":{"cited_paper":"/paper/1202.6073","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:716d383113653ca9bfebd79478205e663a910756dccde8c7517a3cc6e8d387f2","observation_id":"7e31a5ae-af22-41c3-bab2-a82042c003bf","resolution":{"observed_at":"2026-08-14T14:28:01.245472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04847","last_updated":"2018-07-09T13:36:00Z","snapshot_observed_at":"2026-08-14T19:55:01.765132Z","submitted_at":"2018-01-15T15:25:50Z","title":"Serendipity in dark photon searches","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04847","snapshot_observed_at":"2026-08-14T14:28:01.251136Z","title":"Serendipity in dark photon searches ,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.251136Z"},"links":{"cited_paper":"/paper/1801.04847","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:7c6f8bdc5d65ae8c82ca0f53a3ed02cb08c1d43970d7ddc35d456ea42c7999ea","observation_id":"13f3eead-7ee1-4b97-b789-f97dcb0a1a02","resolution":{"observed_at":"2026-08-14T14:28:01.251136Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.05466","last_updated":"2019-09-26T12:03:42Z","snapshot_observed_at":"2026-08-14T19:36:07.069586Z","submitted_at":"2018-03-14T18:33:37Z","title":"Hunting All the Hidden Photons","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.05466","snapshot_observed_at":"2026-08-14T14:28:01.257354Z","title":"Hunting All the Hidden Photons ,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.257354Z"},"links":{"cited_paper":"/paper/1803.05466","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:5cc2ea285119ab4a624502a88ec07e419d2687745d01eaee38220574d00eef8a","observation_id":"238c392f-812d-4e24-9fe3-c39f73d11901","resolution":{"observed_at":"2026-08-14T14:28:01.257354Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.07708","last_updated":"2015-03-26T12:43:34Z","snapshot_observed_at":"2026-08-14T22:54:49.389668Z","submitted_at":"2015-03-26T12:43:34Z","title":"Lepton Number Violation with and without Majorana Neutrinos","version":1},"cited_work":{"arxiv_id":"1503.07708","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.07708","snapshot_observed_at":"2026-08-14T14:28:02.941369Z","title":"Lepton Number Violation with and without Majorana Neutrinos","venue":"hep-ph","work_id":"ce852eba-defe-446a-90f7-1f9c86e1e091","year":2015},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.263632Z"},"links":{"cited_paper":"/paper/1503.07708","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:c787451885c059896c204d60152dc23366bc361b2b144a218ca0043fced64cb0","observation_id":"254b8d0e-1013-4927-bf5c-becfeceda030","resolution":{"observed_at":"2026-08-14T14:28:02.948152Z","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":"1306.0580","last_updated":"2013-07-25T14:41:56Z","snapshot_observed_at":"2026-08-15T00:15:21.801419Z","submitted_at":"2013-06-03T20:01:21Z","title":"Neutrinoless Quadruple Beta Decay","version":2},"cited_work":{"arxiv_id":"1306.0580","doi":null,"metadata_source":"pith","pith_arxiv_id":"1306.0580","snapshot_observed_at":"2026-08-14T14:28:02.892795Z","title":"Neutrinoless Quadruple Beta Decay","venue":"hep-ph","work_id":"73e2d938-401a-4311-85e5-1a4e4fc92d23","year":2013},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.275592Z"},"links":{"cited_paper":"/paper/1306.0580","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:ed983dd71736080842fcdea84737ab92b8256020d9f978e3db3ae00758e13e33","observation_id":"bc690bb5-3a0e-44fa-b490-d19251cb3021","resolution":{"observed_at":"2026-08-14T14:28:02.901791Z","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":"1307.2241","last_updated":"2013-10-08T20:03:26Z","snapshot_observed_at":"2026-08-17T13:54:51.055792Z","submitted_at":"2013-07-08T20:00:03Z","title":"Leptogenesis with Lepton-Number-Violating Dirac Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.2241","snapshot_observed_at":"2026-08-14T14:28:01.282401Z","title":"Leptogenesis with Lepton-Number-Violating Dirac Neutrinos,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.282401Z"},"links":{"cited_paper":"/paper/1307.2241","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:a40f161050688a80a13a28193969f5b18a8bf013d060c3688f32f0b71897a15a","observation_id":"613c9ddf-3a92-4760-b961-4db8e8f097e7","resolution":{"observed_at":"2026-08-14T14:28:01.282401Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0302066","last_updated":"2003-02-13T21:09:20Z","snapshot_observed_at":"2026-08-12T15:18:44.406996Z","submitted_at":"2003-02-10T14:40:49Z","title":"Primordial Nucleosynthesis Constraints on Z' Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0302066","snapshot_observed_at":"2026-08-14T14:28:01.289434Z","title":"Primordial nucleosynthesis constraints on Z′ properties,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.289434Z"},"links":{"cited_paper":"/paper/hep-ph/0302066","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:bdc42555e2ac3b9683e6537654faee020128c4a8c77c1b0f365a44278459701f","observation_id":"059b6c23-313f-4d8b-838d-0cbc2f667b41","resolution":{"observed_at":"2026-08-14T14:28:01.289434Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.7264","last_updated":"2011-12-30T15:23:36Z","snapshot_observed_at":"2026-08-17T03:28:54.521263Z","submitted_at":"2011-11-30T18:27:44Z","title":"Neutrino Cosmology after WMAP and LHC7","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.7264","snapshot_observed_at":"2026-08-14T14:28:01.296730Z","title":"Neutrino cosmology after WMAP 7-Year data and LHC ﬁrst Z′ bounds,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.296730Z"},"links":{"cited_paper":"/paper/1111.7264","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:a663893588b5837968f40dbf49a81545927f38ebfc47de834d232d2a1853c3d6","observation_id":"7d6194a1-3700-4f69-81ed-63a280126808","resolution":{"observed_at":"2026-08-14T14:28:01.296730Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.0186","last_updated":"2012-11-01T14:10:06Z","snapshot_observed_at":"2026-08-15T00:40:48.902597Z","submitted_at":"2012-11-01T14:10:06Z","title":"Right-Handed Neutrinos as the Dark Radiation: Status and Forecasts for the LHC","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.0186","snapshot_observed_at":"2026-08-14T14:28:01.304280Z","title":"Right-Handed Neutrinos as the Dark Radiation: Status and Forecasts for the LHC ,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.304280Z"},"links":{"cited_paper":"/paper/1211.0186","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:5cab2a0dcf18c91b36512cee41abc183a5b57c75b91529fedf494086e2a46c5b","observation_id":"8bffecad-4d9e-43bd-85e9-942354a7a146","resolution":{"observed_at":"2026-08-14T14:28:01.304280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.6350","last_updated":"2012-10-23T20:00:02Z","snapshot_observed_at":"2026-08-17T09:15:11.853182Z","submitted_at":"2012-10-23T20:00:02Z","title":"Dark Radiation Confronting LHC in Z' Models","version":1},"cited_work":{"arxiv_id":"1210.6350","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.6350","snapshot_observed_at":"2026-08-14T14:28:02.692704Z","title":"Dark Radiation Confronting LHC in Z' Models","venue":"hep-ph","work_id":"962b302a-b4af-4ab5-a1a9-915d733f13c5","year":2012},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.310922Z"},"links":{"cited_paper":"/paper/1210.6350","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:d38b691387f87c24895dd6b3c28761f4d4fa83685eb7733d789c4bbe19a8bc8e","observation_id":"ef15dfca-f17f-4718-b114-8edce1efd550","resolution":{"observed_at":"2026-08-14T14:28:02.713741Z","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/9404339","last_updated":"1994-04-26T13:13:16Z","snapshot_observed_at":"2026-07-07T04:17:10.896188Z","submitted_at":"1994-04-26T13:13:16Z","title":"Constraints on Neutrino-Neutrino Interactions from Primordial Nucleosynthesis","version":1},"cited_work":{"arxiv_id":"hep-ph/9404339","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9404339","snapshot_observed_at":"2026-08-14T14:28:02.649353Z","title":"Constraints on Neutrino-Neutrino Interactions from Primordial Nucleosynthesis","venue":"hep-ph","work_id":"1b463daa-3d23-4324-8b8c-943d26ee7ae2","year":1994},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.318328Z"},"links":{"cited_paper":"/paper/hep-ph/9404339","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:fd269c48566981166d6ce054154c48d3c61ecd325ef1af4a3c876709f5a2c4aa","observation_id":"ea419298-a6cb-43a0-86b0-9c19099c08d6","resolution":{"observed_at":"2026-08-14T14:28:02.659651Z","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":"1309.0991","last_updated":"2013-09-04T11:58:14Z","snapshot_observed_at":"2026-08-15T00:04:25.276059Z","submitted_at":"2013-09-04T11:58:14Z","title":"Comment on \"Is Dark Matter with Long-Range Interactions a Solution to All Small-Scale Problems of \\Lambda CDM Cosmology?\"","version":1},"cited_work":{"arxiv_id":"1309.0991","doi":null,"metadata_source":"pith","pith_arxiv_id":"1309.0991","snapshot_observed_at":"2026-08-14T14:28:02.610154Z","title":"Comment on \"Is Dark Matter with Long-Range Interactions a Solution to All Small-Scale Problems of \\Lambda CDM Cosmology?\"","venue":"hep-ph","work_id":"96a7696f-0c13-4634-9fe0-504c0f9d800b","year":2013},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.326446Z"},"links":{"cited_paper":"/paper/1309.0991","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:a5823a0b67494f6e539593ac7b9692f1b55549ef2e94a57262c65365336d19f4","observation_id":"6297eb98-d20c-4283-ae32-76dc9ed5500b","resolution":{"observed_at":"2026-08-14T14:28:02.617988Z","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":"1905.06344","last_updated":"2019-08-23T18:22:45Z","snapshot_observed_at":"2026-08-15T22:19:10.216941Z","submitted_at":"2019-05-15T18:00:03Z","title":"Neutrino-Dark Matter Connections in Gauge Theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06344","snapshot_observed_at":"2026-08-14T14:28:01.333494Z","title":"Neutrino-Dark Matter Connections in Gauge Theories,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.333494Z"},"links":{"cited_paper":"/paper/1905.06344","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:89aa7bc54ced31540562e60f9d5bd5cc18d105167909e60bc385e2d6f3fc1352","observation_id":"b046ca02-8aa3-4c16-b64d-86a1892f55d3","resolution":{"observed_at":"2026-08-14T14:28:01.333494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.07046","last_updated":"2018-03-02T01:01:11Z","snapshot_observed_at":"2026-08-14T20:52:28.693814Z","submitted_at":"2017-06-21T18:00:00Z","title":"Thermal Dark Matter Below an MeV","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.07046","snapshot_observed_at":"2026-08-14T14:28:01.341538Z","title":"Thermal Dark Matter Below an MeV,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.341538Z"},"links":{"cited_paper":"/paper/1706.07046","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:188d9340cc98d7251c418d675263ffeaa6f339d6b1954a85d6aa267db23cb120","observation_id":"cdb4c847-63dd-4944-9d12-330e59ac4d42","resolution":{"observed_at":"2026-08-14T14:28:01.341538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.04282","last_updated":"2018-07-11T18:00:01Z","snapshot_observed_at":"2026-08-14T18:53:04.804756Z","submitted_at":"2018-07-11T18:00:01Z","title":"A Thermal Neutrino Portal to Sub-MeV Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.04282","snapshot_observed_at":"2026-08-14T14:28:01.349274Z","title":"Thermal neutrino portal to sub-MeV dark matter ,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.349274Z"},"links":{"cited_paper":"/paper/1807.04282","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:8afc2c794f76307807153a6935e3c6853ce9dd8a3a2b7025e15c51e1ef522d5c","observation_id":"c813d68c-d830-463f-a988-7ca1d0581079","resolution":{"observed_at":"2026-08-14T14:28:01.349274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.2920","last_updated":"2013-05-13T20:00:03Z","snapshot_observed_at":"2026-08-17T13:31:22.287388Z","submitted_at":"2013-05-13T20:00:03Z","title":"Solar constraints on hidden photons re-visited","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.2920","snapshot_observed_at":"2026-08-14T14:28:01.355936Z","title":"Solar constraints on hidden photons re-visited,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.355936Z"},"links":{"cited_paper":"/paper/1305.2920","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:ad88032a38b0caed89c734e1eb364d614c5f4d8b0a5e1911582752bbb416a049","observation_id":"759f34a7-153a-47b8-af16-5b66a2171dee","resolution":{"observed_at":"2026-08-14T14:28:01.355936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1406.2980","last_updated":"2014-09-18T22:17:20Z","snapshot_observed_at":"2026-08-15T07:30:54.957793Z","submitted_at":"2014-06-11T17:54:39Z","title":"Search for a dark photon in e+e- collisions at BABAR","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1406.2980","snapshot_observed_at":"2026-08-14T14:28:01.361977Z","title":"Search for a Dark Photon in e+e− Collisions at BaBar ,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.361977Z"},"links":{"cited_paper":"/paper/1406.2980","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:99c1a2b326719abd7223c079eb5441d38eb6b997ebd9d999fda865cd77c61781","observation_id":"c3aae57a-eb09-44f4-876c-99f71c967a44","resolution":{"observed_at":"2026-08-14T14:28:01.361977Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.02867","last_updated":"2018-02-09T18:09:55Z","snapshot_observed_at":"2026-08-14T20:25:49.562173Z","submitted_at":"2017-10-08T18:43:24Z","title":"Search for dark photons produced in 13 TeV $pp$ collisions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.02867","snapshot_observed_at":"2026-08-14T14:28:01.367334Z","title":"Search for Dark Photons Produced in 13 TeV pp Collisions,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.367334Z"},"links":{"cited_paper":"/paper/1710.02867","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:ebdbeaf71b1f77b2d945249556adefaa72d574462bf7b44bfc1ae79f3f07ce80","observation_id":"8923d75f-c1dd-4ac6-8a0d-6856b5472b22","resolution":{"observed_at":"2026-08-14T14:28:01.367334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.02424","last_updated":"2017-11-15T13:57:08Z","snapshot_observed_at":"2026-08-14T20:48:55.120562Z","submitted_at":"2017-07-08T10:06:48Z","title":"Search for new high-mass phenomena in the dilepton final state using 36 fb$^{-1}$ of proton-proton collision data at $\\sqrt{s}$ = 13 TeV with the ATLAS detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.02424","snapshot_observed_at":"2026-08-14T14:28:01.374063Z","title":"Search for new high-mass phenomena in the dilepton ﬁnal state using 36 fb−1 of proton-proton collision data at √s = 13 TeV with the ATLAS detector ,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.374063Z"},"links":{"cited_paper":"/paper/1707.02424","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:ed2d6ff8ba012e4222f8d380040c22f1da88b983e3e0af770f41cc2de929b1ac","observation_id":"ebb72ff1-8239-4924-9f4b-d6c11af332e9","resolution":{"observed_at":"2026-08-14T14:28:01.374063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.02823","last_updated":"2018-09-18T18:00:02Z","snapshot_observed_at":"2026-08-14T19:06:20.304745Z","submitted_at":"2018-06-07T17:59:59Z","title":"The Dispirited Case of Gauged $U(1)_{B-L}$ Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.02823","snapshot_observed_at":"2026-08-14T14:28:01.381676Z","title":"The dispirited case of gauged U(1)B−L dark matter,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.381676Z"},"links":{"cited_paper":"/paper/1806.02823","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:6ec904f2188069575c5626d789c9cd360e1427346244d790cb782f803d8920dc","observation_id":"087ce976-9efc-4787-9044-62310299303a","resolution":{"observed_at":"2026-08-14T14:28:01.381676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.07763","last_updated":"2015-04-01T11:01:38Z","snapshot_observed_at":"2026-08-17T17:37:54.732390Z","submitted_at":"2015-02-26T21:21:06Z","title":"Constraints on Dark Photon from Neutrino-Electron Scattering Experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.07763","snapshot_observed_at":"2026-08-14T14:28:01.388489Z","title":"Constraints on Dark Photon from Neutrino-Electron Scattering Experiments,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.388489Z"},"links":{"cited_paper":"/paper/1502.07763","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:96be59ded3dd6a2b365e35716a2da432727371a1514e4ef2d5d12f6336bfb00b","observation_id":"fb5beac9-0a9c-4a12-82bd-8fe3ff5f9ead","resolution":{"observed_at":"2026-08-14T14:28:01.388489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00060","last_updated":"2018-02-28T20:06:23Z","snapshot_observed_at":"2026-08-14T19:40:57.846616Z","submitted_at":"2018-02-28T20:06:23Z","title":"Neutrino-Electron Scattering: General Constraints on Z' and Dark Photon Models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.00060","snapshot_observed_at":"2026-08-14T14:28:01.395861Z","title":"Neutrino-electron scattering: general constraints on Z′ and dark photon models ,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.395861Z"},"links":{"cited_paper":"/paper/1803.00060","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:d360cae4b3d612a9553d4d0834582f6130578634e71ad3c6f1f4b262e86bcf73","observation_id":"2a3257f5-2265-4b0c-b6f7-7eed56146355","resolution":{"observed_at":"2026-08-14T14:28:01.395861Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.0580","last_updated":"2009-06-03T19:34:38Z","snapshot_observed_at":"2026-08-17T14:14:19.093340Z","submitted_at":"2009-06-03T19:34:38Z","title":"New Fixed-Target Experiments to Search for Dark Gauge Forces","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.0580","snapshot_observed_at":"2026-08-14T14:28:01.402973Z","title":"New Fixed-Target Experiments to Search for Dark Gauge Forces,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.402973Z"},"links":{"cited_paper":"/paper/0906.0580","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:985897c036e8d4ae68b27bdf4e9d28addf6edaffb9beac8b0b0380bca45d95ae","observation_id":"074be3d8-1b22-475c-8321-4619bfa15f8e","resolution":{"observed_at":"2026-08-14T14:28:01.402973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1209.6083","last_updated":"2012-11-14T09:03:01Z","snapshot_observed_at":"2026-08-15T00:45:13.003476Z","submitted_at":"2012-09-26T21:24:06Z","title":"New Limits on Hidden Photons from Past Electron Beam Dumps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1209.6083","snapshot_observed_at":"2026-08-14T14:28:01.409257Z","title":"New Limits on Hidden Photons from Past Electron Beam Dumps ,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.409257Z"},"links":{"cited_paper":"/paper/1209.6083","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:a346e8496845638ce295c7dbcd2455e727eb2fbbf9cc2669f53dea912dd949a8","observation_id":"e8bb1246-1388-4e84-be67-31081d4000b3","resolution":{"observed_at":"2026-08-14T14:28:01.409257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.3870","last_updated":"2013-11-15T15:07:01Z","snapshot_observed_at":"2026-08-14T23:55:09.246814Z","submitted_at":"2013-11-15T15:07:01Z","title":"New Exclusion Limits on Dark Gauge Forces from Proton Bremsstrahlung in Beam-Dump Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.3870","snapshot_observed_at":"2026-08-14T14:28:01.416334Z","title":"New Exclusion Limits on Dark Gauge Forces from Proton Bremsstrahlung in Beam-Dump Data,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.416334Z"},"links":{"cited_paper":"/paper/1311.3870","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:47c005674134aeebcbd7f296eefb7caf501808086dcd7554bbaacd94364bc5bb","observation_id":"76242702-a1ba-4048-a0c7-e532131a06ec","resolution":{"observed_at":"2026-08-14T14:28:01.416334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00993","last_updated":"2018-09-17T04:50:13Z","snapshot_observed_at":"2026-08-14T19:40:10.034578Z","submitted_at":"2018-03-02T18:46:17Z","title":"Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.00993","snapshot_observed_at":"2026-08-14T14:28:01.423738Z","title":"Supernova 1987A Constraints on Sub-GeV Dark Sectors, Millicharged Particles, the QCD Axion, and an Axion-like Particle,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.423738Z"},"links":{"cited_paper":"/paper/1803.00993","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:82519d8c831f8f3e34257257354163b38dcf87c99e30b52eac891171a7a01765","observation_id":"9044d6e1-6afa-42dc-8c59-25d340e769c4","resolution":{"observed_at":"2026-08-14T14:28:01.423738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0612017","last_updated":"2006-12-02T05:28:40Z","snapshot_observed_at":"2026-08-15T10:54:49.277534Z","submitted_at":"2006-12-02T05:28:40Z","title":"Gauge Trimming of Neutrino Masses","version":1},"cited_work":{"arxiv_id":"hep-ph/0612017","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0612017","snapshot_observed_at":"2026-08-14T14:28:02.119773Z","title":"Gauge Trimming of Neutrino Masses","venue":"hep-ph","work_id":"8499bb3d-51db-4ee3-bfd9-8169aa3a844c","year":2006},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.430216Z"},"links":{"cited_paper":"/paper/hep-ph/0612017","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:91be76c7d56ea28744323cd323ace2fcecd364e4d526d6460cf810c4a56df49e","observation_id":"ffddb30a-c8d4-483a-b46f-74bb4d4428c6","resolution":{"observed_at":"2026-08-14T14:28:02.126870Z","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":"1902.05802","last_updated":"2019-08-09T04:14:55Z","snapshot_observed_at":"2026-08-15T03:18:59.233265Z","submitted_at":"2019-02-15T13:15:12Z","title":"Alternative formulation of left-right symmetry with $B-L$ conservation and purely Dirac neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.05802","snapshot_observed_at":"2026-08-14T14:28:01.436458Z","title":"Alternative formulation of left-right symmetry with B−L conservation and purely Dirac neutrinos,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.436458Z"},"links":{"cited_paper":"/paper/1902.05802","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:843290f21a40aac20b84dd1d909c9720456f1d94b60697c2acef5b5f82316211","observation_id":"c58ec2cb-ce5d-47ef-beff-e8a6e1ba07bb","resolution":{"observed_at":"2026-08-14T14:28:01.436458Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.08172","last_updated":"2017-11-15T16:14:42Z","snapshot_observed_at":"2026-08-14T21:19:09.497639Z","submitted_at":"2017-01-27T19:08:47Z","title":"Unveiling $\\nu$ secrets with cosmological data: neutrino masses and mass hierarchy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.08172","snapshot_observed_at":"2026-08-14T14:28:01.444843Z","title":"Unveiling ν secrets with cosmological data: neutrino masses and mass hierarchy,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.444843Z"},"links":{"cited_paper":"/paper/1701.08172","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:d19604c63873aeb04831d4f4796d05b18e3ae965a09d9cdff3da600ca28812e4","observation_id":"9d97aac3-d247-4212-a51a-4905134fc779","resolution":{"observed_at":"2026-08-14T14:28:01.444843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.12598","last_updated":"2020-07-15T18:17:09Z","snapshot_observed_at":"2026-08-18T02:06:47.775221Z","submitted_at":"2019-07-29T18:45:46Z","title":"Updated results on neutrino mass and mass hierarchy from cosmology with Planck 2018 likelihoods","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.12598","snapshot_observed_at":"2026-08-14T14:28:01.452916Z","title":"Updated results on neutrino mass and mass hierarchy from cosmology ,","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.452916Z"},"links":{"cited_paper":"/paper/1907.12598","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:90635efb74621e35abdb9f71c7b50e8f052e6f64c542045f473a37466e1cdc5d","observation_id":"6b2c6bd8-cd71-4964-bf4d-d7fa3531eeb0","resolution":{"observed_at":"2026-08-14T14:28:01.452916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.168256Z","title":"Naturally Light Dirac Neutrinos in Gauge Theories ,","venue":null,"work_id":"6596d76c-c805-42cb-89a3-b6bcd8522694","year":1983},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.459384Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:c0d0b4bb41f377329c865532bd3c38c4ec274eb4365b2a70d81ef8e5510ddc7d","observation_id":"13f9e436-e3e6-4611-992f-e23b0ceef1d7","resolution":{"observed_at":"2026-08-14T14:28:04.178255Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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/0502176","last_updated":"2005-02-18T21:16:03Z","snapshot_observed_at":"2026-08-03T12:48:16.071178Z","submitted_at":"2005-02-18T21:16:03Z","title":"Models of Neutrino Mass with a Low Cutoff Scale","version":1},"cited_work":{"arxiv_id":"hep-ph/0502176","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0502176","snapshot_observed_at":"2026-08-14T14:28:01.991778Z","title":"Models of Neutrino Mass with a Low Cutoff Scale","venue":"hep-ph","work_id":"c0720304-b3fb-42da-9f2d-fb5a7631090c","year":2005},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.466948Z"},"links":{"cited_paper":"/paper/hep-ph/0502176","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:0296635666905e00b53111682d06b1ea7739f2ca39a95098a40da198c8ccde67","observation_id":"7d847939-8368-47e5-a77d-2458489b9310","resolution":{"observed_at":"2026-08-14T14:28:01.998820Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.148762Z","title":"Left-right Symmetry and Finite One Loop Dirac Neutrino Mass ,","venue":null,"work_id":"e166bbfd-ed53-4d06-85ac-6854d1dedc57","year":1988},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.473367Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:53568a2948c9794b2d21f616b0920d87fa690945876281b6f85e3b4010b9d16a","observation_id":"7148312a-0d36-4a1a-8f91-03e0d4c4439e","resolution":{"observed_at":"2026-08-14T14:28:04.154546Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1802.05231","last_updated":"2018-02-14T17:39:49Z","snapshot_observed_at":"2026-08-14T19:45:50.865021Z","submitted_at":"2018-02-14T17:39:49Z","title":"Systematic Analysis of Dirac Neutrino Masses at Dimension Five","version":1},"cited_work":{"arxiv_id":"1802.05231","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.05231","snapshot_observed_at":"2026-08-14T14:28:01.959060Z","title":"Systematic Analysis of Dirac Neutrino Masses at Dimension Five","venue":"hep-ph","work_id":"0614169d-f688-4d0c-949a-d19a9443cc10","year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.482781Z"},"links":{"cited_paper":"/paper/1802.05231","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:be74fa07880b3afc83f98bfcc386c0baf5c7b1c315438028023580f9ed6e2ca9","observation_id":"df3e7c05-e7d3-4da2-887a-0ce54a01212a","resolution":{"observed_at":"2026-08-14T14:28:01.966688Z","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T14:28:04.123585Z","title":"Observable Neutrino Dirac Mass and Supergrand Uniﬁcation,","venue":null,"work_id":"100e5f8d-69ff-49cd-846c-d0f5dc67c779","year":1984},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.489099Z"},"links":{"citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:b33aa32e49fc9e88c38f2f3aea15a3d7cbf00f4de226930f6a8ab9d88ac2fb40","observation_id":"33891ba1-ab4d-405b-ba7b-137b3d5c64ce","resolution":{"observed_at":"2026-08-14T14:28:04.130622Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1609.02538","last_updated":"2016-11-18T19:41:29Z","snapshot_observed_at":"2026-08-14T21:40:42.315419Z","submitted_at":"2016-09-08T19:20:15Z","title":"Pathways to Naturally Small Dirac Neutrino Masses","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.02538","snapshot_observed_at":"2026-08-14T14:28:01.495918Z","title":"Pathways to Naturally Small Dirac Neutrino Masses ,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.495918Z"},"links":{"cited_paper":"/paper/1609.02538","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:6277494838b8e1bc27ed0899988a138ebee595e70dd6f543d57bd434b5af0048","observation_id":"d6ddb2ef-0008-40fe-8b2a-7c66ee5b7bce","resolution":{"observed_at":"2026-08-14T14:28:01.495918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.05722","last_updated":"2018-05-03T10:10:25Z","snapshot_observed_at":"2026-08-14T19:45:26.573927Z","submitted_at":"2018-02-15T19:00:06Z","title":"Seesaw roadmap to neutrino mass and dark matter","version":2},"cited_work":{"arxiv_id":"1802.05722","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.05722","snapshot_observed_at":"2026-08-14T14:28:01.890564Z","title":"Seesaw roadmap to neutrino mass and dark matter","venue":"hep-ph","work_id":"34726e3a-b4ff-4561-8bee-9ef248e3885a","year":2018},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.508280Z"},"links":{"cited_paper":"/paper/1802.05722","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:390e1de994dcaf0b9443abfe6c84e4e62c60e832549b4b8e01c352f11fc48b6e","observation_id":"0a26e830-1720-4bc4-9063-28067688ff9f","resolution":{"observed_at":"2026-08-14T14:28:01.901656Z","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/0601018","last_updated":"2006-10-25T06:54:37Z","snapshot_observed_at":"2026-07-07T04:09:52.500383Z","submitted_at":"2006-01-03T15:32:00Z","title":"Split Two-Higgs-Doublet Model and Neutrino Condensation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0601018","snapshot_observed_at":"2026-08-14T14:28:01.516082Z","title":"Split two-Higgs-doublet model and neutrino condensation ,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.516082Z"},"links":{"cited_paper":"/paper/hep-ph/0601018","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:1decf0baa9e3735682c25ece793637cf91598726816f54db4d7837fc81656302","observation_id":"449ba7d3-9448-4b96-a413-8408f649f5d6","resolution":{"observed_at":"2026-08-14T14:28:01.516082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0610253","last_updated":"2006-11-29T18:05:31Z","snapshot_observed_at":"2026-08-15T10:59:38.636166Z","submitted_at":"2006-10-19T17:42:20Z","title":"A New Two Higgs Doublet Model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0610253","snapshot_observed_at":"2026-08-14T14:28:01.522410Z","title":"A New two Higgs doublet model,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.522410Z"},"links":{"cited_paper":"/paper/hep-ph/0610253","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:62b2a6d3b2bd0e0bf1b0a5e5ca799d5b66ea50271974547b93f7d64ae9877316","observation_id":"1a2d784e-6d35-4d32-a6ea-16958d2d54c9","resolution":{"observed_at":"2026-08-14T14:28:01.522410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.4844","last_updated":"2011-06-10T18:23:20Z","snapshot_observed_at":"2026-08-15T04:45:46.157449Z","submitted_at":"2011-05-24T17:42:58Z","title":"Astrophysical Consequences of a Neutrinophilic Two-Higgs-Doublet Model","version":2},"cited_work":{"arxiv_id":"1105.4844","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.4844","snapshot_observed_at":"2026-08-14T14:28:01.791133Z","title":"Astrophysical Consequences of a Neutrinophilic Two-Higgs-Doublet Model","venue":"hep-ph","work_id":"a491269c-e2cf-452f-8101-2bc217086024","year":2011},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.530949Z"},"links":{"cited_paper":"/paper/1105.4844","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:b57bbd55abfd6a417b4bb0dad34c677d1bd9f24fdcfdce6c2ffd4ad7a40d9c0c","observation_id":"fd049e37-ecfb-492f-b848-a6c28367b556","resolution":{"observed_at":"2026-08-14T14:28:01.798595Z","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":"1106.3880","last_updated":"2011-07-28T10:01:35Z","snapshot_observed_at":"2026-08-15T04:43:27.523255Z","submitted_at":"2011-06-20T12:31:58Z","title":"Comment on astrophysical consequences of a neutrinophilic 2HDM","version":2},"cited_work":{"arxiv_id":"1106.3880","doi":null,"metadata_source":"pith","pith_arxiv_id":"1106.3880","snapshot_observed_at":"2026-08-14T14:28:01.743693Z","title":"Comment on astrophysical consequences of a neutrinophilic 2HDM","venue":"hep-ph","work_id":"69c1af66-6042-4f00-92e1-7fe2c66d8313","year":2011},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.538610Z"},"links":{"cited_paper":"/paper/1106.3880","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:b97abe4761f417f5454fae4fc40f31e9935b4835576817bb249e370c71b1db63","observation_id":"8405a83f-2af6-4b30-8d82-9cc4a26452cb","resolution":{"observed_at":"2026-08-14T14:28:01.753230Z","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":"0906.3335","last_updated":"2009-10-15T16:34:53Z","snapshot_observed_at":"2026-08-15T05:45:37.632973Z","submitted_at":"2009-06-18T19:26:58Z","title":"Dirac neutrinos from a second Higgs doublet","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.3335","snapshot_observed_at":"2026-08-14T14:28:01.545337Z","title":"Dirac neutrinos from a second Higgs doublet ,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.545337Z"},"links":{"cited_paper":"/paper/0906.3335","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:d61c6b9668913475621109d2309da92621f0a721a8390323463a6ac527cf278c","observation_id":"a3adddaa-24b6-4637-819f-79bec5937852","resolution":{"observed_at":"2026-08-14T14:28:01.545337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9907562","last_updated":"2000-03-14T22:25:10Z","snapshot_observed_at":"2026-07-07T04:33:58.410808Z","submitted_at":"1999-07-30T12:16:20Z","title":"Leptogenesis with Dirac Neutrinos","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9907562","snapshot_observed_at":"2026-08-14T14:28:01.552774Z","title":"Leptogenesis with Dirac neutrinos ,","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.552774Z"},"links":{"cited_paper":"/paper/hep-ph/9907562","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:4f019a11d81caabd25c4c5540eaf9e0aa68f1991505b5f3355d6f89f0e640649","observation_id":"c0dc8860-bfca-42f5-b933-25e30d3c0646","resolution":{"observed_at":"2026-08-14T14:28:01.552774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0206177","last_updated":"2002-07-02T18:07:58Z","snapshot_observed_at":"2026-08-15T16:28:38.219963Z","submitted_at":"2002-06-19T23:23:33Z","title":"Realistic Dirac Leptogenesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0206177","snapshot_observed_at":"2026-08-14T14:28:01.559660Z","title":"Realistic Dirac leptogenesis,","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-14T14:28:01.559660Z"},"links":{"cited_paper":"/paper/hep-ph/0206177","citing_paper":"/paper/1908.03286"},"observation_digest":"sha256:5adf6aa8c7137569fe5c4a2d16ef0a7b06db4518be5a315d0d1a33c6758ed9fd","observation_id":"b1081935-8f0c-4898-b236-bf2c967fa22f","resolution":{"observed_at":"2026-08-14T14:28:01.559660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.03286","last_updated":"2019-10-22T14:38:40Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-15T20:11:25.172170Z","submitted_at":"2019-08-08T22:59:53Z","title":"Observing Dirac neutrinos in the cosmic microwave background"},"reference_resolution":{"displayed":85,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":63,"verified_exact":13,"verified_fuzzy":9},"total_outbound_references":85},"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 85 of 85 outbound references and 14 inbound Pith citation observations for arXiv:1908.03286."}