{"as_of":"2026-08-12T19:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6efa7cd504cb37ebc3204986adcd06a0f9874942fa9a95bd96710e71d3cb43cb","coverage":[{"denominator":94,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":94,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T00:08:19.083346Z","state":"measured"},{"denominator":96,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":96,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T05:54:27.588432Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-13T03:07:09.195258Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.02027","snapshot_observed_at":"2026-08-11T05:54:27.588432Z","title":"Agudelo, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.17141","last_updated":"2025-05-15T13:07:35Z","snapshot_observed_at":"2026-08-11T06:39:13.498822Z","submitted_at":"2024-12-22T19:26:05Z","title":"Prospecting bipartite Dark Matter through Gravitational Waves","version":2},"reference_index":109,"source":"pdf_text","source_observed_at":"2026-08-11T05:54:27.588432Z"},"links":{"cited_paper":"/paper/2412.02027","citing_paper":"/paper/2412.17141"},"observation_digest":"sha256:e7c713730c0e6ebeb71afab262990f08c213209c9752d4efdad9cdf955b8dda3","observation_id":"98f4b99c-f931-4045-b007-ff03b13acbb4","resolution":{"observed_at":"2026-08-11T05:54:27.588432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"cited_work":{"arxiv_id":"2412.02027","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2412.02027","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Agudelo, D","venue":null,"work_id":"c333f157-650f-4abb-9c29-0f9362e298b8","year":2025},"citing_paper":{"arxiv_id":"2605.11082","last_updated":"2026-05-11T18:00:08Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-11T18:00:08Z","title":"Dark Matter as a Source for Lepton Flavor Violation","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-13T03:02:31.859366Z"},"links":{"cited_paper":"/paper/2412.02027","citing_paper":"/paper/2605.11082"},"observation_digest":"sha256:a79bab17feb27980fbdabc1869bc98af9c12eb03691bef1ccffc8f78e0fb18db","observation_id":"0b841967-8f47-4adf-b83a-906c5e738cb7","resolution":{"observed_at":"2026-05-13T03:07:09.197074Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2412.02027/citation-record","integrity":"/paper/2412.02027/integrity","json":"/paper/2412.02027/citation-record.json","paper":"/paper/2412.02027"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T00:08:18.664697Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.664697Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:5fd832ddd127ac6f50fb2e03eba973b427e52a05d3d2251f45e91d12ea0176be","observation_id":"726783b6-13f1-4ab8-b0c7-0a6f1c6d412b","resolution":{"observed_at":"2026-08-12T00:08:18.664697Z","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":"2026-08-12T00:08:18.645142Z","title":"(12) Regarding the fermion spectrum, in this model, we have two DM particles (DM1 and DM2) that are connected by the dark photonZ ′ and the Higgs portal S as is shown in Fig","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.645142Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:80ac9cc5578379d2778b93e9fc10e4c3eb6c002f260a0af1d9fbfaf2c9a96d45","observation_id":"707c13e8-5194-4058-bf9b-a695bc348a29","resolution":{"observed_at":"2026-08-12T00:08:18.645142Z","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":"2026-08-12T00:08:18.649792Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.649792Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:09e2fb2558e94707d9c327e92fbad26219f3fe0fdfbe16029d05da4fef33f27c","observation_id":"5dbde60a-f4a4-4854-9eea-90b265a9105a","resolution":{"observed_at":"2026-08-12T00:08:18.649792Z","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":"2026-08-12T00:08:18.654771Z","title":"The DM annihilation into SM model particles via mass mixing of the scalars hi or kinetic mixing is extremely suppressed","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.654771Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:d226e5db129bca94558a7af6210dadc6bea4ce5cc5f22b80d5e723173a0cd700","observation_id":"9be1c703-3c66-4201-a5b2-964c5cb6b19d","resolution":{"observed_at":"2026-08-12T00:08:18.654771Z","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":"2026-08-12T00:08:18.659918Z","title":"The 2 → 2 processes allowed in this model that can modify the relic density of DM particles","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.659918Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:0b0bd5a528cf4ff02d64b4ce278dd4fd89defbf6734db9f29cfb805ad810ca0f","observation_id":"7bf10703-9aea-4b75-94d4-5f428b74128a","resolution":{"observed_at":"2026-08-12T00:08:18.659918Z","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":"2026-08-12T00:08:18.669229Z","title":"left-right equilibration","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.669229Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:929412ffea1dae34fef49be531db33e9ec92ac101631acf6cbc2474c4bdd7912","observation_id":"5455d22d-a6db-46ee-9372-d3a85554ac21","resolution":{"observed_at":"2026-08-12T00:08:18.669229Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-12T00:08:18.674853Z","title":"In addition, the interaction between the two candidates for DM gives the value Ωh2 ≈ 0.12 [41]","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.674853Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:ab8825e9a0be92f9a2a590e0902be64de332506de4305c424bbbd7e303f9dba1","observation_id":"6934d0c2-396a-4dc8-bfd5-2a7dcb1af6ea","resolution":{"observed_at":"2026-08-12T00:08:18.674853Z","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":"2026-08-12T00:08:18.679178Z","title":"where µ = MN mΨi/(MN + mΨi) is the reduced mass, MN ≈ 939 MeV is the nucleon mass (neutron or proton), BΨ1 = (qχL − qχR) = 1, BΨ2 = (qψL − qψR) = 9 (see Tab","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.679178Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:28747bdfd522f61cd549eb65d9b6ce63205d349de51ac6e75c8db82cfa71fc9e","observation_id":"7d8e1389-0e68-42be-bbd7-08012608f4b5","resolution":{"observed_at":"2026-08-12T00:08:18.679178Z","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":"2026-08-12T00:08:18.684639Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.684639Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:157a47ef4dc111b7993a75aabf4097aea5ba90a8b541dfd6f7cddbbd663458de","observation_id":"45d23da6-f42d-4692-91ea-c7c454c354e1","resolution":{"observed_at":"2026-08-12T00:08:18.684639Z","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":"2026-08-12T00:08:18.689023Z","title":"Cosmological Constraints on the Properties of Weakly Interacting Massive Particles,","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.689023Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:37230d49a9e45ee08df8445d822ea492ff5f881de62fa14b4478c677d3678d6d","observation_id":"16db47eb-fc0d-44bd-a168-2ec567a8cba5","resolution":{"observed_at":"2026-08-12T00:08:18.689023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.8327","last_updated":"2013-11-03T20:09:30Z","snapshot_observed_at":"2026-07-06T03:26:58.920943Z","submitted_at":"2013-10-30T21:17:06Z","title":"Snowmass CF1 Summary: WIMP Dark Matter Direct Detection","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.8327","snapshot_observed_at":"2026-08-12T00:08:18.693327Z","title":"Working Group Report: WIMP Dark Matter Direct Detection,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.693327Z"},"links":{"cited_paper":"/paper/1310.8327","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:9bb0c010d5a5ff195b691e528c2eeb08fa5e7a346729fe6ef98df84e11b8e841","observation_id":"a8665909-88be-494f-8a6d-da5391602120","resolution":{"observed_at":"2026-08-12T00:08:18.693327Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1605.04909","last_updated":"2016-05-24T21:37:46Z","snapshot_observed_at":"2026-07-06T04:56:28.645608Z","submitted_at":"2016-05-16T20:00:02Z","title":"A History of Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1605.04909","snapshot_observed_at":"2026-08-12T00:08:18.697621Z","title":"History of dark matter,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.697621Z"},"links":{"cited_paper":"/paper/1605.04909","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:94b582038697b500c04f394af9630f28219b0f3938ccadf38310426522ce7c9e","observation_id":"2d98bd5f-1a09-4546-9dd3-32c645310730","resolution":{"observed_at":"2026-08-12T00:08:18.697621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.02479","last_updated":"2023-04-27T17:52:08Z","snapshot_observed_at":"2026-08-10T23:23:23.580484Z","submitted_at":"2022-12-05T18:38:45Z","title":"The WIMP Paradigm: Theme and Variations","version":2},"cited_work":{"arxiv_id":"2212.02479","doi":null,"metadata_source":"pith","pith_arxiv_id":"2212.02479","snapshot_observed_at":"2026-08-12T00:08:20.494281Z","title":"The WIMP Paradigm: Theme and Variations","venue":"hep-ph","work_id":"947df55d-3c1f-4dde-83cc-f5f1cd10e863","year":2022},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.702154Z"},"links":{"cited_paper":"/paper/2212.02479","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:09af22f85058304ce457cf11fd9e6e4bb3cadeca1db2b66d864c717373a0fe3f","observation_id":"ecf1a839-591f-449c-a176-41ba5f74926f","resolution":{"observed_at":"2026-08-12T00:08:20.501684Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T00:08:18.706918Z","title":"Cosmology of the Invisible Axion,","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.706918Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:590daad69a0152a5f6eb5aee16accf4a8c7dc847fa03567525b730711b054af0","observation_id":"04ede11e-b40d-42f9-b1ca-91c388eb8b6f","resolution":{"observed_at":"2026-08-12T00:08:18.706918Z","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":"2026-08-12T00:08:18.712109Z","title":"A Cosmological Bound on the Invisible Axion,","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.712109Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:8e5e4a515a899a9f24728ac664471d32ca4ca036920e9ec758ef657977a1be97","observation_id":"2a5bc5e9-a383-4057-ada1-608a392abbff","resolution":{"observed_at":"2026-08-12T00:08:18.712109Z","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":"2026-08-12T00:08:18.716838Z","title":"The Not So Harmless Axion,","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.716838Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:69d4509f7c6b2e7428170a9b42747656e0eaccbcd6f1a8386159d5f5f4dbd147","observation_id":"48d27fd4-4ada-415f-8f48-0f12e6ea2996","resolution":{"observed_at":"2026-08-12T00:08:18.716838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.00767","last_updated":"2021-10-26T09:33:30Z","snapshot_observed_at":"2026-08-10T00:37:34.081809Z","submitted_at":"2021-09-02T08:05:36Z","title":"Sterile Neutrinos as Dark Matter Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.00767","snapshot_observed_at":"2026-08-12T00:08:18.721739Z","title":"Sterile neutrinos as dark matter candidates,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.721739Z"},"links":{"cited_paper":"/paper/2109.00767","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:a4582ee78c6c6f5788ba2313435b45d740d4b5d2b31551d1e43024e37414593f","observation_id":"88d0dba5-2cb8-4e67-801d-a5b77f93742e","resolution":{"observed_at":"2026-08-12T00:08:18.721739Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.12778","last_updated":"2021-05-09T18:33:50Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-02-27T05:17:54Z","title":"Constraints on Primordial Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.12778","snapshot_observed_at":"2026-08-12T00:08:18.726531Z","title":"Constraints on primordial black holes,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.726531Z"},"links":{"cited_paper":"/paper/2002.12778","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:ffb9d570f50b0c6c8aa235120b72905727e58dadca3126d29c9b6683f73b7ec0","observation_id":"b836f363-b3f0-44e3-a5fc-9a802093cf29","resolution":{"observed_at":"2026-08-12T00:08:18.726531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1603.00464","last_updated":"2016-05-30T19:22:03Z","snapshot_observed_at":"2026-08-09T21:18:21.835672Z","submitted_at":"2016-03-01T21:00:01Z","title":"Did LIGO detect dark matter?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1603.00464","snapshot_observed_at":"2026-08-12T00:08:18.731478Z","title":"Did LIGO detect dark matter?","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.731478Z"},"links":{"cited_paper":"/paper/1603.00464","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:60773a5a81bcf53c7c14b7792d5e6cdb611f4bd8de4367e82fab6b0f016ec3f9","observation_id":"fbe207e3-7e9b-4b89-a41f-4e17a97cf551","resolution":{"observed_at":"2026-08-12T00:08:18.731478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.13254","last_updated":"2025-01-27T11:42:47Z","snapshot_observed_at":"2026-08-11T13:16:31.897991Z","submitted_at":"2024-12-17T19:00:01Z","title":"Asymmetries from a charged memory-burdened PBH","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.13254","snapshot_observed_at":"2026-08-12T00:08:18.736043Z","title":"Asymmetries from a charged memory- burdened PBH,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.736043Z"},"links":{"cited_paper":"/paper/2412.13254","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:e18694343e91db5018c52bc5489cd8ffd5b533343842fe05a724f176531ad444","observation_id":"82b9859b-7bd2-449e-87b1-9f0029d0904d","resolution":{"observed_at":"2026-08-12T00:08:18.736043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.15755","last_updated":"2021-10-29T13:04:29Z","snapshot_observed_at":"2026-08-08T16:12:02.573780Z","submitted_at":"2021-10-29T13:04:29Z","title":"Theory and phenomenology of Dirac neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.15755","snapshot_observed_at":"2026-08-12T00:08:18.740039Z","title":"Theory and phenomenology of Dirac neutrinos,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.740039Z"},"links":{"cited_paper":"/paper/2110.15755","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:f85000a706dc175b80711b15b52cb4f60b2c7996332d22e7e385d7f24cd77e19","observation_id":"75171854-33cb-4674-b29e-5885081b5a46","resolution":{"observed_at":"2026-08-12T00:08:18.740039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.08524","last_updated":"2017-11-25T05:56:16Z","snapshot_observed_at":"2026-07-06T05:48:30.254634Z","submitted_at":"2017-06-26T18:00:01Z","title":"From the trees to the forest: a review of radiative neutrino mass models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.08524","snapshot_observed_at":"2026-08-12T00:08:18.744831Z","title":"From the trees to the forest: a review of radiative neutrino mass models,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.744831Z"},"links":{"cited_paper":"/paper/1706.08524","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:0f5ebe5b44de0aec9978a5621b3330693b270d25489c4357c993c68024957760","observation_id":"28cb399a-79dd-4372-a19e-aa19547a9095","resolution":{"observed_at":"2026-08-12T00:08:18.744831Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.4866","last_updated":"2007-11-30T04:11:22Z","snapshot_observed_at":"2026-08-12T14:38:03.140170Z","submitted_at":"2007-11-30T04:11:22Z","title":"Secluded WIMP Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.4866","snapshot_observed_at":"2026-08-12T00:08:18.749539Z","title":"Secluded WIMP Dark Matter,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.749539Z"},"links":{"cited_paper":"/paper/0711.4866","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:de8559aa57d7bd31ad40601bfbaf87bf32ae0bf0c7dfb15cf77b40c39a06a341","observation_id":"420eab84-7e24-4573-8bbe-462bb3a42273","resolution":{"observed_at":"2026-08-12T00:08:18.749539Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.1030","last_updated":"2008-11-06T20:34:30Z","snapshot_observed_at":"2026-07-06T01:45:38.508472Z","submitted_at":"2008-11-06T20:34:30Z","title":"Secluded U(1) below the weak scale","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.1030","snapshot_observed_at":"2026-08-12T00:08:18.753979Z","title":"Secluded U(1) below the weak scale,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.753979Z"},"links":{"cited_paper":"/paper/0811.1030","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:9e8d2f38cf0e81b7a453db6ce73ccfbe2a6b3c731e60a5202e75cf23de8f54c0","observation_id":"4c8ed1af-23c9-484f-b855-9e14bb6b42fb","resolution":{"observed_at":"2026-08-12T00:08:18.753979Z","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":"2026-08-12T00:08:18.758558Z","title":"Two U(1)’s and Epsilon Charge Shifts,","venue":null,"work_id":null,"year":1986},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.758558Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:a2538a8c858259594e9844cbd4e4053b99a010f575a193018a9257658aba123d","observation_id":"104e0537-c2ae-4f12-9a9f-965541477f79","resolution":{"observed_at":"2026-08-12T00:08:18.758558Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.7691","last_updated":"2014-12-20T19:46:46Z","snapshot_observed_at":"2026-08-10T10:14:42.464031Z","submitted_at":"2014-05-29T19:59:52Z","title":"The windows for kinetically mixed Z'-mediated dark matter and the galactic center gamma ray excess","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.7691","snapshot_observed_at":"2026-08-12T00:08:18.763172Z","title":"The windows for kinetically mixed Z’-mediated dark matter and the galactic center gamma ray excess,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.763172Z"},"links":{"cited_paper":"/paper/1405.7691","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:e3d7264f97f9517b2db8eb30dd44babc1c3d847b71f52d4827fe43b1766a9444","observation_id":"e5c6bcfe-a4b4-45a4-bcd3-d361103ee2b7","resolution":{"observed_at":"2026-08-12T00:08:18.763172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.01515","last_updated":"2020-10-16T18:38:00Z","snapshot_observed_at":"2026-07-06T09:17:28.084328Z","submitted_at":"2020-05-04T14:31:03Z","title":"The Dark Photon","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.01515","snapshot_observed_at":"2026-08-12T00:08:18.767728Z","title":"X,78, arXiv:2005.01515 [hep-ph]","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.767728Z"},"links":{"cited_paper":"/paper/2005.01515","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:caf3cf42b84a97e88120e3e6bd5af5b42ff09c9fdab6a67354a58c5429c46eb8","observation_id":"2383b2d6-bc3e-4b8e-a2aa-2edca94676f1","resolution":{"observed_at":"2026-08-12T00:08:18.767728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.03063","last_updated":"2016-10-10T20:00:01Z","snapshot_observed_at":"2026-08-10T07:34:39.164297Z","submitted_at":"2016-10-10T20:00:01Z","title":"Impact of Mass Generation for Simplified Dark Matter Models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.03063","snapshot_observed_at":"2026-08-12T00:08:18.772315Z","title":"Impact of mass generation for spin-1 mediator simplified models,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.772315Z"},"links":{"cited_paper":"/paper/1610.03063","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:d91a100cc65ab852a32684afb38aefe249214d4752c18cf822ea061cd29bece3","observation_id":"d6aa1b2f-3fab-4603-8f36-1320ba228515","resolution":{"observed_at":"2026-08-12T00:08:18.772315Z","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":"2026-08-12T00:08:20.618013Z","title":"Interaction energy in electrodynamics and in the field theory of nuclear forces,","venue":null,"work_id":"8bdb4ff0-07a7-4afe-9c22-026b7b9ff440","year":1938},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.776771Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:4f5a897b471f9b76b39c04ccd115f4495a6e2e688f279f130a950db42db0c085","observation_id":"6a24e03f-5a87-43a1-a7f6-92379fb3d7f4","resolution":{"observed_at":"2026-08-12T00:08:20.629343Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.09864","last_updated":"2019-08-26T18:12:31Z","snapshot_observed_at":"2026-08-11T04:24:28.763660Z","submitted_at":"2019-08-26T18:12:31Z","title":"Dark matter from dark photons: a taxonomy of dark matter production","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.09864","snapshot_observed_at":"2026-08-12T00:08:18.780502Z","title":"Dark matter from dark photons: a taxonomy of dark matter production,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.780502Z"},"links":{"cited_paper":"/paper/1908.09864","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:11b814274ec1113daaaf50d9cf81c8375a21c75bc3ecba0f23611146b840dc0c","observation_id":"d547a69d-b182-48d3-a61c-1b13dd6f186d","resolution":{"observed_at":"2026-08-12T00:08:18.780502Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.13729","last_updated":"2019-05-31T17:29:33Z","snapshot_observed_at":"2026-07-06T07:57:04.916745Z","submitted_at":"2019-05-31T17:29:33Z","title":"General solution to the U(1) anomaly equations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.13729","snapshot_observed_at":"2026-08-12T00:08:18.784461Z","title":"General Solution to the U(1) Anomaly Equations,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.784461Z"},"links":{"cited_paper":"/paper/1905.13729","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:718ccaf7d395d7ca2fd2c9ff4995e4b417c85d13d08391bf27cc9d2ad5cbaa0c","observation_id":"f5296f3d-1e80-4dab-803e-bf346d6cb046","resolution":{"observed_at":"2026-08-12T00:08:18.784461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.09524","last_updated":"2021-12-17T14:21:50Z","snapshot_observed_at":"2026-07-06T12:19:58.682860Z","submitted_at":"2021-12-17T14:21:50Z","title":"Effective Dirac neutrino mass operator in the Standard Model with a local Abelian extension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.09524","snapshot_observed_at":"2026-08-12T00:08:18.788851Z","title":"Effective Dirac Neutrino Mass Operator in the Standard Model With a Local Abelian Extension,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.788851Z"},"links":{"cited_paper":"/paper/2112.09524","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:5ba18df06aad7a73a3267ae1122880b7948e383c80e9b0f68161881d0d18ad3f","observation_id":"28f00167-4b9a-4593-84c3-668c59607a1b","resolution":{"observed_at":"2026-08-12T00:08:18.788851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.08573","last_updated":"2021-04-19T10:50:45Z","snapshot_observed_at":"2026-07-06T09:48:28.426619Z","submitted_at":"2020-08-19T17:56:27Z","title":"Anomaly-free chiral $U(1)_{D}$ and its scotogenic implication","version":2},"cited_work":{"arxiv_id":"2008.08573","doi":null,"metadata_source":"pith","pith_arxiv_id":"2008.08573","snapshot_observed_at":"2026-08-12T00:08:20.275461Z","title":"Anomaly-free chiral $U(1)_{D}$ and its scotogenic implication","venue":"hep-ph","work_id":"4731aebf-6f51-4a0c-b68c-d76d5225a8b2","year":2020},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.793385Z"},"links":{"cited_paper":"/paper/2008.08573","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:9fd3bbbbff2a5875a3be5c74225f1d38b54924df0c5d4a83abc8a4d1c13f3b1f","observation_id":"bc8f01f5-ae0b-4863-88eb-4cc8e71ec632","resolution":{"observed_at":"2026-08-12T00:08:20.284211Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2102.06211","last_updated":"2021-05-12T13:42:35Z","snapshot_observed_at":"2026-08-09T12:09:08.864720Z","submitted_at":"2021-02-11T19:00:02Z","title":"Anomaly-free Abelian gauge symmetries with Dirac scotogenic models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.06211","snapshot_observed_at":"2026-08-12T00:08:18.798658Z","title":"Anomaly-free Abelian gauge symmetries with Dirac scotogenic models,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.798658Z"},"links":{"cited_paper":"/paper/2102.06211","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:1251edd51355f584ba56e4e57b8f8597e8acb11c181b9a235682599118b633b5","observation_id":"fd0c94c3-8731-43c2-a649-9608ab0e7d6b","resolution":{"observed_at":"2026-08-12T00:08:18.798658Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0312285","last_updated":"2003-12-30T05:34:47Z","snapshot_observed_at":"2026-08-10T11:30:59.948672Z","submitted_at":"2003-12-19T20:46:58Z","title":"Simple Model for (3+2) Neutrino Oscillations","version":2},"cited_work":{"arxiv_id":"hep-ph/0312285","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0312285","snapshot_observed_at":"2026-08-12T00:08:20.233273Z","title":"Simple Model for (3+2) Neutrino Oscillations","venue":"hep-ph","work_id":"7c787afd-fbd2-4514-962d-6157538c708e","year":2003},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.803136Z"},"links":{"cited_paper":"/paper/hep-ph/0312285","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:e87f1f469ba927aea3f824e7b7faa4328c91d6ecd1dd1ddfc7101d3f1260c8d4","observation_id":"2b628af8-6b60-4ce1-a650-ba38ceef302d","resolution":{"observed_at":"2026-08-12T00:08:20.241618Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0510181","last_updated":"2005-10-13T20:42:49Z","snapshot_observed_at":"2026-07-07T04:08:56.920357Z","submitted_at":"2005-10-13T20:42:49Z","title":"Anomaly-Free Sets of Fermions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0510181","snapshot_observed_at":"2026-08-12T00:08:18.808793Z","title":"Anomaly-free sets of fermions,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.808793Z"},"links":{"cited_paper":"/paper/hep-ph/0510181","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:465f1e0549e8c6519991e1109a2ef3ab5cef5cd70ab7941a00fc293ceb7b6b90","observation_id":"a4882878-ad87-423d-b269-7b2674f13e92","resolution":{"observed_at":"2026-08-12T00:08:18.808793Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1507.00916","last_updated":"2015-07-03T14:01:53Z","snapshot_observed_at":"2026-08-07T15:47:44.557844Z","submitted_at":"2015-07-03T14:01:53Z","title":"New Chiral Fermions, a New Gauge Interaction, Dirac Neutrinos, and Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1507.00916","snapshot_observed_at":"2026-08-12T00:08:18.813316Z","title":"New Chiral Fermions, a New Gauge Interaction, Dirac Neutrinos, and Dark Matter,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.813316Z"},"links":{"cited_paper":"/paper/1507.00916","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:7ada7c3dd09f6bc07112738883dd44f13580cf1a90289ab2873a132775596062","observation_id":"fc15c5b0-8288-4c42-8e69-fdb489a9ea35","resolution":{"observed_at":"2026-08-12T00:08:18.813316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.11991","last_updated":"2020-01-31T18:29:34Z","snapshot_observed_at":"2026-08-11T02:35:31.963343Z","submitted_at":"2020-01-31T18:29:34Z","title":"Chiral Abelian gauge theories with few fermions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.11991","snapshot_observed_at":"2026-08-12T00:08:18.818078Z","title":"Chiral Abelian gauge theories with few fermions,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.818078Z"},"links":{"cited_paper":"/paper/2001.11991","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:dea2fc6feaec873dbd8817258ab16323a5f22db7f63cb38305e6f05c984f73da","observation_id":"63dac64c-392c-4ae1-b6df-085c9a03598c","resolution":{"observed_at":"2026-08-12T00:08:18.818078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.17987","last_updated":"2023-11-29T19:00:00Z","snapshot_observed_at":"2026-07-06T16:54:37.940527Z","submitted_at":"2023-11-29T19:00:00Z","title":"Closing the dark photon window to thermal dark matter","version":1},"cited_work":{"arxiv_id":"2311.17987","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.17987","snapshot_observed_at":"2026-08-12T00:08:20.171430Z","title":"Closing the dark photon window to thermal dark matter","venue":"hep-ph","work_id":"bf938dbb-8fea-4923-8a31-88791c4b9b0c","year":2023},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.822892Z"},"links":{"cited_paper":"/paper/2311.17987","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:37a052d6e75e18b26a9769ee63eb402b6348a22dcee6230671eef19274dc5ee6","observation_id":"6f0504ac-c5af-479f-b606-bc172f8463e1","resolution":{"observed_at":"2026-08-12T00:08:20.176054Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.12138","last_updated":"2021-01-30T20:16:16Z","snapshot_observed_at":"2026-08-11T02:15:38.534351Z","submitted_at":"2021-01-28T17:38:07Z","title":"Linkage of Dirac Neutrinos to Dark U(1) Gauge Symmetry","version":2},"cited_work":{"arxiv_id":"2101.12138","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.12138","snapshot_observed_at":"2026-08-12T00:08:20.149393Z","title":"Linkage of Dirac Neutrinos to Dark U(1) Gauge Symmetry","venue":"hep-ph","work_id":"e4df8294-f32d-4e8d-91c3-ce666368c671","year":2021},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.827149Z"},"links":{"cited_paper":"/paper/2101.12138","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:cbd77630d8555480edaa2d01de0890a8d8cde9006958b8aecfbe36e39387a33d","observation_id":"73086be1-0774-4ab3-841b-d1b33c20714f","resolution":{"observed_at":"2026-08-12T00:08:20.156058Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1101.2755","last_updated":"2011-03-23T17:05:08Z","snapshot_observed_at":"2026-07-06T02:22:02.393781Z","submitted_at":"2011-01-14T10:08:57Z","title":"The Reactor Antineutrino Anomaly","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.2755","snapshot_observed_at":"2026-08-12T00:08:18.831876Z","title":"The Reactor Antineutrino Anomaly,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.831876Z"},"links":{"cited_paper":"/paper/1101.2755","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:1a41e6f1eef2d0ccf722508d9adc5539a3ead6842a2734df2fa4a4e6965bc9c3","observation_id":"927d9df7-f83c-4d0e-8fcc-762f5347a6f6","resolution":{"observed_at":"2026-08-12T00:08:18.831876Z","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":"2026-08-12T00:08:18.836349Z","title":"Mod- els of neutrino mass with a low cutoff scale,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.836349Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:f37a561fc4447f86ffee5649d8ceb912d04dfafea380a2735d8ec0b545f64b64","observation_id":"f0448c0e-4883-4d9f-a646-2c5489b4226d","resolution":{"observed_at":"2026-08-12T00:08:18.836349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.0538","last_updated":"2013-05-28T15:20:32Z","snapshot_observed_at":"2026-07-06T02:59:03.986539Z","submitted_at":"2012-11-02T19:58:39Z","title":"Exotic Charges, Multicomponent Dark Matter and Light Sterile Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.0538","snapshot_observed_at":"2026-08-12T00:08:18.841604Z","title":"Exotic Charges, Multicomponent Dark Matter and Light Sterile Neutrinos,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.841604Z"},"links":{"cited_paper":"/paper/1211.0538","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:ea0ef036ad85240e99d80dd84fab7a879995bdc0d23cd2ae2541d80dab33e749","observation_id":"88dada79-7d08-46b0-bac0-246d45cd1ce6","resolution":{"observed_at":"2026-08-12T00:08:18.841604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.0045","last_updated":"2010-07-23T21:33:29Z","snapshot_observed_at":"2026-08-12T19:07:21.697580Z","submitted_at":"2010-06-30T23:03:37Z","title":"Dark Discrete Gauge Symmetries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.0045","snapshot_observed_at":"2026-08-12T00:08:18.846037Z","title":"Dark Discrete Gauge Symmetries,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.846037Z"},"links":{"cited_paper":"/paper/1007.0045","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:8da879af62f261a69bac9516c16e219afdd190a5db8f6a1644bb506d065a4726","observation_id":"e4fb4fe4-414b-4196-866a-955054bbb769","resolution":{"observed_at":"2026-08-12T00:08:18.846037Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.09574","last_updated":"2020-02-05T18:50:47Z","snapshot_observed_at":"2026-07-06T08:23:26.829198Z","submitted_at":"2019-09-20T15:54:34Z","title":"Dirac neutrino mass generation from Majorana messenger","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.09574","snapshot_observed_at":"2026-08-12T00:08:18.851656Z","title":"Dirac neutrino mass generation from a Majorana messenger,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.851656Z"},"links":{"cited_paper":"/paper/1909.09574","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:dd64986262e67ea13484e0bd612d7a95a59d70d4dc623759d10063a37104e7f7","observation_id":"3daa2de7-c519-4719-8913-c7f33b99bf4c","resolution":{"observed_at":"2026-08-12T00:08:18.851656Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.01186","last_updated":"2018-04-27T17:50:13Z","snapshot_observed_at":"2026-07-06T05:53:58.450457Z","submitted_at":"2017-08-03T15:51:21Z","title":"Status of neutrino oscillations 2018: first hint for normal mass ordering and improved CP sensitivity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.01186","snapshot_observed_at":"2026-08-12T00:08:18.856637Z","title":"Status of neutrino oscillations 2018: 3 σ hint for normal mass ordering and improved CP sensitivity,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.856637Z"},"links":{"cited_paper":"/paper/1708.01186","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:7d0425ab7c7b247eaf6281b7c4ed20b55cd5975de3167180f0e388525ae2b539","observation_id":"924d0ee8-026f-48a8-ae1f-c0c5f696a30f","resolution":{"observed_at":"2026-08-12T00:08:18.856637Z","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":"2026-08-06T02:25:35.932935Z","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":"2026-08-12T00:08:18.861714Z","title":"Hunting All the Hidden Photons,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.861714Z"},"links":{"cited_paper":"/paper/1803.05466","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:7ed80531ea635e9ed0d632b88decd436d2421c1f4cd7d9acde111510e659d242","observation_id":"b8eba957-75ff-4062-8480-01913eb2acef","resolution":{"observed_at":"2026-08-12T00:08:18.861714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.6129","last_updated":"2014-12-04T20:18:19Z","snapshot_observed_at":"2026-08-10T10:50:13.353156Z","submitted_at":"2014-07-23T08:21:40Z","title":"micrOMEGAs4.1: two dark matter candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.6129","snapshot_observed_at":"2026-08-12T00:08:18.867150Z","title":"micrOMEGAs4.1: two dark matter candidates,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.867150Z"},"links":{"cited_paper":"/paper/1407.6129","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:d8a35d5b640a0506a6b8dc372cad895d41b76757e38479975dc8696e34037600","observation_id":"fea8fdb8-7ad0-431b-917f-926aba3f4daf","resolution":{"observed_at":"2026-08-12T00:08:18.867150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.14894","last_updated":"2024-02-26T10:36:11Z","snapshot_observed_at":"2026-08-06T22:01:14.026511Z","submitted_at":"2023-12-22T18:16:08Z","title":"micrOMEGAs 6.0: N-component dark matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.14894","snapshot_observed_at":"2026-08-12T00:08:18.871717Z","title":"micrOMEGAs 6.0: N-component dark matter,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.871717Z"},"links":{"cited_paper":"/paper/2312.14894","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:50578e3cda87de6a056dbae5852080b74316db55292ea93e0ad238d4708c850c","observation_id":"4d531174-6b31-454c-b214-e34da370231e","resolution":{"observed_at":"2026-08-12T00:08:18.871717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-12T00:08:18.876322Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.876322Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:23852fc12b5f0d2d93fa77f92425d55d352dc52ecc42df4338e41513960668a4","observation_id":"a827434d-3f15-4336-9bed-608f984f60aa","resolution":{"observed_at":"2026-08-12T00:08:18.876322Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9506015","last_updated":"1995-06-02T12:33:52Z","snapshot_observed_at":"2026-07-07T01:11:17.861816Z","submitted_at":"1995-06-02T12:33:52Z","title":"Neutrino decoupling in the early Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9506015","snapshot_observed_at":"2026-08-12T00:08:18.881932Z","title":"Neutrino decoupling in the early universe,","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.881932Z"},"links":{"cited_paper":"/paper/astro-ph/9506015","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:5fbd7b01d1c259ca77462806859fed7f42ed32c73b7c777a859bbf60e2490680","observation_id":"366f7883-8d1a-4314-8fb4-9cf7d82d8119","resolution":{"observed_at":"2026-08-12T00:08:18.881932Z","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":"ph/0002127","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T00:08:19.807660Z","title":"MeV scale reheating temperature and thermalization of neutrino background,","venue":null,"work_id":"18168eb6-e794-45e4-8814-be1120d5981a","year":2000},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.887541Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:c1c61327cbb0d44d9e2d467f61e2c539f15ad5805efdf82d863e383be638bc45","observation_id":"ee61ded7-b0fa-4b22-8197-ca96cdbbbe59","resolution":{"observed_at":"2026-08-12T00:08:19.815596Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.10792","last_updated":"2025-04-24T10:16:19Z","snapshot_observed_at":"2026-08-12T17:00:53.026971Z","submitted_at":"2024-05-17T14:02:13Z","title":"Light from darkness: history of a hot dark sector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.10792","snapshot_observed_at":"2026-08-12T00:08:18.892181Z","title":"Light from darkness: history of a hot dark sector,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.892181Z"},"links":{"cited_paper":"/paper/2405.10792","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:b08e2f64e4c096a4d1b354550acd585c4ceca1e2d031ef03a8c573b682955ac4","observation_id":"084050f8-11eb-476e-9fb4-f35fbe0390a5","resolution":{"observed_at":"2026-08-12T00:08:18.892181Z","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":"2026-07-06T04:28:27.195947Z","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":"2026-08-12T00:08:18.896670Z","title":"Nonthermal cosmic neutrino back- ground,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.896670Z"},"links":{"cited_paper":"/paper/1509.00481","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:8b27b67dfaae613d6733e54552a72e7eeb0d783af17313f2688c87cd1dc5b11b","observation_id":"39910c4b-9a8a-4234-973f-2b17729cbc15","resolution":{"observed_at":"2026-08-12T00:08:18.896670Z","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":"2026-08-12T00:08:20.597509Z","title":"The Early Universe,","venue":null,"work_id":"1e28d788-be64-457f-ba52-336899812059","year":1990},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.901811Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:d745a3cb01e50680e52cd9f3a674d5d962e56f438055bf3c357de4225c4a0078","observation_id":"1e56eaba-8463-4012-b07c-ed38d38e50cb","resolution":{"observed_at":"2026-08-12T00:08:20.602382Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-12T00:08:20.583590Z","title":"Calculations of Relic Densities in the Early Universe,","venue":null,"work_id":"5bda41de-45ff-4dbc-9b81-6f9e31b9286c","year":1988},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.906304Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:b4f83b1866acd5270893ff8bbf285c6e226982a79a0e9fd92794742322bbf4e1","observation_id":"f92039eb-7d53-43b8-b55e-bbc8c4f69ccf","resolution":{"observed_at":"2026-08-12T00:08:20.588080Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0012260","last_updated":"2001-05-16T16:07:13Z","snapshot_observed_at":"2026-07-07T03:50:56.660518Z","submitted_at":"2000-12-20T19:20:02Z","title":"Generating Feynman Diagrams and Amplitudes with FeynArts 3","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0012260","snapshot_observed_at":"2026-08-12T00:08:18.909937Z","title":"Generating Feynman diagrams and amplitudes with FeynArts 3,","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.909937Z"},"links":{"cited_paper":"/paper/hep-ph/0012260","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:f597a48baf1ca296cf9f329ecc5838c859595cc02e61d66e6c2cbe4b56098673","observation_id":"21d155f3-ce3d-4d33-95f6-88782356cb2f","resolution":{"observed_at":"2026-08-12T00:08:18.909937Z","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":"2026-08-12T00:08:20.559889Z","title":"FEYN CALC: Computer algebraic calculation of Feynman amplitudes,","venue":null,"work_id":"b759721a-3ced-4d0e-aec5-3d8cfed85e9e","year":1991},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.914901Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:48bce3dd9ba5540a17b5133dbbe5d2b6611e73b54adbb5a7d0d5f5a501b3ded0","observation_id":"01650216-9ae0-40ff-a21b-bc9998e53391","resolution":{"observed_at":"2026-08-12T00:08:20.573228Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.01167","last_updated":"2018-01-28T11:47:02Z","snapshot_observed_at":"2026-08-06T15:00:48.007405Z","submitted_at":"2016-01-06T13:06:32Z","title":"New Developments in FeynCalc 9.0","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.01167","snapshot_observed_at":"2026-08-12T00:08:18.919306Z","title":"New Developments in FeynCalc 9.0,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.919306Z"},"links":{"cited_paper":"/paper/1601.01167","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:a3183a773d7dd02c1d24b088a7f6a7d9ba3e372cd3e878a91560b30a0fbbed5a","observation_id":"76292532-11a2-4efe-8c54-ed77d3894cf3","resolution":{"observed_at":"2026-08-12T00:08:18.919306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.04407","last_updated":"2020-07-16T15:20:10Z","snapshot_observed_at":"2026-08-08T11:28:10.808082Z","submitted_at":"2020-01-13T17:17:50Z","title":"FeynCalc 9.3: New features and improvements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.04407","snapshot_observed_at":"2026-08-12T00:08:18.923851Z","title":"FeynCalc 9.3: New features and improvements,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.923851Z"},"links":{"cited_paper":"/paper/2001.04407","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:8779af5dac9b2b2265a785a58ac1e5540ea092282be1d5d4785e5cd211923c85","observation_id":"fde745d3-7a0b-4ba1-a4ed-dba0f25cac41","resolution":{"observed_at":"2026-08-12T00:08:18.923851Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.12034","last_updated":"2022-03-22T20:50:14Z","snapshot_observed_at":"2026-07-06T12:51:01.741759Z","submitted_at":"2022-03-22T20:50:14Z","title":"Connecting Dark Gauge Symmetry to the Standard Model","version":1},"cited_work":{"arxiv_id":"2203.12034","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.12034","snapshot_observed_at":"2026-08-12T00:08:19.587496Z","title":"Connecting Dark Gauge Symmetry to the Standard Model","venue":"hep-ph","work_id":"86dfdc19-c382-4ea7-b1de-75f85d4405e8","year":2022},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.928753Z"},"links":{"cited_paper":"/paper/2203.12034","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:3ea32f02121474e4c2b8d507d2df354b640204a91cb9d797fb57aac2811b24a7","observation_id":"48129fcc-a12a-4300-80a4-6ccd2fd8f0bd","resolution":{"observed_at":"2026-08-12T00:08:19.593338Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.03490","last_updated":"2015-09-28T07:35:08Z","snapshot_observed_at":"2026-07-06T04:06:13.590546Z","submitted_at":"2015-01-14T20:59:24Z","title":"Dark Matter Complementarity and the Z$^\\prime$ Portal","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.03490","snapshot_observed_at":"2026-08-12T00:08:18.933164Z","title":"Dark Matter Complementarity and the Z ′ Portal,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.933164Z"},"links":{"cited_paper":"/paper/1501.03490","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:e0d29883cc92f745b6d54c9a3126ca9e74dc709f698b69f65fa44cbb0bb2eeab","observation_id":"8d1d6cc6-3a80-4063-9e9e-aa3d629ff337","resolution":{"observed_at":"2026-08-12T00:08:18.933164Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.06767","last_updated":"2015-09-28T07:26:53Z","snapshot_observed_at":"2026-07-06T04:21:39.911736Z","submitted_at":"2015-06-22T20:01:48Z","title":"Dirac-Fermionic Dark Matter in $U(1)_X$ Models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.06767","snapshot_observed_at":"2026-08-12T00:08:18.937806Z","title":"Dirac-fermionic dark matter in U(1) X models,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.937806Z"},"links":{"cited_paper":"/paper/1506.06767","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:a56c2b407f1cf480fcc439a783852edab2577d7b573df5c37a0b1a8cac70706e","observation_id":"c69e9275-1106-4752-8a81-592d75facf8e","resolution":{"observed_at":"2026-08-12T00:08:18.937806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0806.0538","last_updated":"2012-11-06T09:49:18Z","snapshot_observed_at":"2026-08-08T14:58:52.293749Z","submitted_at":"2008-06-03T13:36:09Z","title":"Sarah","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0806.0538","snapshot_observed_at":"2026-08-12T00:08:18.942104Z","title":"Staub, “SARAH,” (6 2008), arXiv:0806.0538 [hep-ph]","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.942104Z"},"links":{"cited_paper":"/paper/0806.0538","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:8a43b85157496bcf9595f84fa65e2a0fe3d239d8ec12cd98a9a00f05910d281f","observation_id":"d2b216c7-a2f8-4210-9f2f-193113f87fd9","resolution":{"observed_at":"2026-08-12T00:08:18.942104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.2863","last_updated":"2009-09-15T20:00:36Z","snapshot_observed_at":"2026-08-05T13:06:06.524381Z","submitted_at":"2009-09-15T20:00:36Z","title":"From Superpotential to Model Files for FeynArts and CalcHep/CompHep","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.2863","snapshot_observed_at":"2026-08-12T00:08:18.947317Z","title":"From Superpotential to Model Files for FeynArts and CalcHep/CompHep,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.947317Z"},"links":{"cited_paper":"/paper/0909.2863","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:cc53ab0c22d9f192b21dbb529cb33daa427522cb8572e672d6147903085b97ab","observation_id":"ee790490-e80e-4b81-a82c-53fb1e2d6f0d","resolution":{"observed_at":"2026-08-12T00:08:18.947317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.0840","last_updated":"2011-01-11T12:33:04Z","snapshot_observed_at":"2026-08-10T16:58:18.311302Z","submitted_at":"2010-02-03T21:00:56Z","title":"Automatic Calculation of supersymmetric Renormalization Group Equations and Self Energies","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.0840","snapshot_observed_at":"2026-08-12T00:08:18.951750Z","title":"Automatic Calculation of supersymmetric Renormalization Group Equations and Self Energies,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.951750Z"},"links":{"cited_paper":"/paper/1002.0840","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:59294d3d3b8463d153d7d1409a434b6daeec20bcc34728c54c27a64aefe21d29","observation_id":"53fa127d-f92f-444b-8dc7-9f39319c8519","resolution":{"observed_at":"2026-08-12T00:08:18.951750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.0906","last_updated":"2013-02-12T21:10:50Z","snapshot_observed_at":"2026-08-04T10:26:59.108896Z","submitted_at":"2012-07-04T06:06:47Z","title":"SARAH 3.2: Dirac Gauginos, UFO output, and more","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.0906","snapshot_observed_at":"2026-08-12T00:08:18.955688Z","title":"SARAH 3.2: Dirac Gauginos, UFO output, and more,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.955688Z"},"links":{"cited_paper":"/paper/1207.0906","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:9d970a84d41a6c533a3cb8cfbbdd1c4ef08500799c5069ba804b4fa9280a6f83","observation_id":"cf188a2b-fd31-4c56-be62-b07627570d93","resolution":{"observed_at":"2026-08-12T00:08:18.955688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.7223","last_updated":"2014-02-14T10:03:23Z","snapshot_observed_at":"2026-07-06T03:24:09.535709Z","submitted_at":"2013-09-27T12:35:15Z","title":"SARAH 4: A tool for (not only SUSY) model builders","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.7223","snapshot_observed_at":"2026-08-12T00:08:18.959618Z","title":"SARAH 4 : A tool for (not only SUSY) model builders,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.959618Z"},"links":{"cited_paper":"/paper/1309.7223","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:95e150db070d5aee9ad28972179680d6025ec3aa099ce507575708994432e7a2","observation_id":"41e04d30-41d2-4288-8d58-d732ebc8f247","resolution":{"observed_at":"2026-08-12T00:08:18.959618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0301101","last_updated":"2004-03-15T11:30:58Z","snapshot_observed_at":"2026-07-07T03:58:50.379254Z","submitted_at":"2003-01-15T11:21:22Z","title":"SPheno, a program for calculating supersymmetric spectra, SUSY particle decays and SUSY particle production at e+ e- colliders","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0301101","snapshot_observed_at":"2026-08-12T00:08:18.964095Z","title":"SPheno, a program for calculating supersymmetric spectra, SUSY particle decays and SUSY particle production at e+ e- colliders,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.964095Z"},"links":{"cited_paper":"/paper/hep-ph/0301101","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:709dae5279da6a04f8df8b81818e345c73343bd6cc96c3d9adf4b20fffd73df7","observation_id":"fcc39200-d79f-4e57-8914-86e78453435f","resolution":{"observed_at":"2026-08-12T00:08:18.964095Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.1573","last_updated":"2011-09-24T13:58:57Z","snapshot_observed_at":"2026-08-04T09:35:21.584354Z","submitted_at":"2011-04-08T13:48:02Z","title":"SPheno 3.1: extensions including flavour, CP-phases and models beyond the MSSM","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.1573","snapshot_observed_at":"2026-08-12T00:08:18.968961Z","title":"SPheno 3.1: Extensions including flavour, CP-phases and models beyond the MSSM,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.968961Z"},"links":{"cited_paper":"/paper/1104.1573","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:a93b7b7ced852b1aa4dd85a60acef365796a5c206d21fb911a922a6ddc42b000","observation_id":"fab3547c-0b53-4385-92d9-eff1fc186a2b","resolution":{"observed_at":"2026-08-12T00:08:18.968961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.01361","last_updated":"2015-04-15T13:22:06Z","snapshot_observed_at":"2026-07-06T04:08:14.591998Z","submitted_at":"2015-02-04T21:21:31Z","title":"A second Higgs from the Higgs portal","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01361","snapshot_observed_at":"2026-08-12T00:08:18.973758Z","title":"A second Higgs from the Higgs portal,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.973758Z"},"links":{"cited_paper":"/paper/1502.01361","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:5c8d52013908548e342c21c12f92565c864eb26e5cbcbd4d2e2f79014fbbd2e1","observation_id":"aa96d97b-498f-4bd8-9c61-67f4cd1748aa","resolution":{"observed_at":"2026-08-12T00:08:18.973758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.03616","last_updated":"2019-03-08T17:21:16Z","snapshot_observed_at":"2026-08-10T10:47:20.426778Z","submitted_at":"2019-03-08T17:21:16Z","title":"Dark Matter through the Higgs portal","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.03616","snapshot_observed_at":"2026-08-12T00:08:18.978525Z","title":"Dark Matter through the Higgs portal,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.978525Z"},"links":{"cited_paper":"/paper/1903.03616","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:7dec43e8628a914b0defddbfa4908e373ad7581c712e0116a55f9716da8ed47f","observation_id":"bb4efe68-8a81-4e2f-8772-c466deeddc42","resolution":{"observed_at":"2026-08-12T00:08:18.978525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.16169","last_updated":"2024-02-19T15:03:41Z","snapshot_observed_at":"2026-08-10T10:29:53.972803Z","submitted_at":"2023-05-25T15:29:56Z","title":"Dark Higgs Bosons at Colliders","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.16169","snapshot_observed_at":"2026-08-12T00:08:18.983046Z","title":"Dark Higgs bosons at colliders,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.983046Z"},"links":{"cited_paper":"/paper/2305.16169","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:9aeb70843558882b65cfe6b55542fc7e540cf3076181cadfdcb431bab2bd1d5c","observation_id":"4c8d2ea2-1cd6-4ef7-960c-695113ea1614","resolution":{"observed_at":"2026-08-12T00:08:18.983046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.00043","last_updated":"2023-03-13T18:21:23Z","snapshot_observed_at":"2026-08-08T10:34:02.264900Z","submitted_at":"2022-06-30T18:24:16Z","title":"A portrait of the Higgs boson by the CMS experiment ten years after the discovery","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.00043","snapshot_observed_at":"2026-08-12T00:08:18.988297Z","title":"A portrait of the Higgs boson by the CMS experiment ten years after the discovery","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.988297Z"},"links":{"cited_paper":"/paper/2207.00043","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:ab6b13a5d64cf9571609f7aa7418a63a0b62fc3b11827e805b6fb082df144cbd","observation_id":"542f9891-a8d4-4b93-9222-278df4cd6ef0","resolution":{"observed_at":"2026-08-12T00:08:18.988297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.09008","last_updated":"2024-09-13T17:37:38Z","snapshot_observed_at":"2026-08-12T19:12:03.155152Z","submitted_at":"2024-09-13T17:37:38Z","title":"Chiral dark matter and radiative neutrino masses from gauged U(1) symmetry","version":1},"cited_work":{"arxiv_id":"2409.09008","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.09008","snapshot_observed_at":"2026-08-12T00:08:19.389127Z","title":"Chiral dark matter and radiative neutrino masses from gauged U(1) symmetry","venue":"hep-ph","work_id":"1d40018c-f5e6-4b23-8e28-853a1d4da3b3","year":2024},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.992792Z"},"links":{"cited_paper":"/paper/2409.09008","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:ddaa69a02366afa53f707e069453fa40c81733a61e530d01d2d9aea4c8a14a99","observation_id":"8c1b4dbb-97a9-4751-bcca-98f4f18cfa9a","resolution":{"observed_at":"2026-08-12T00:08:19.394211Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+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":"2026-08-12T00:08:20.540767Z","title":"Remarks on the unified model of ele- mentary particles,","venue":null,"work_id":"a1cc0471-844d-4ab9-b489-c52620b8b6bf","year":1962},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:18.997243Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:fe256dc7908695ce81a799f13188c5a33d052239b29607da8640fc12f7469e42","observation_id":"f9c8ef3e-5cf2-471f-a5e3-ba2bf1157469","resolution":{"observed_at":"2026-08-12T00:08:20.545975Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.8165","last_updated":"2015-04-20T13:18:00Z","snapshot_observed_at":"2026-07-06T03:55:53.426338Z","submitted_at":"2014-09-29T16:05:25Z","title":"Theory for Baryon Number and Dark Matter at the LHC","version":2},"cited_work":{"arxiv_id":"1409.8165","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.8165","snapshot_observed_at":"2026-08-12T00:08:19.368791Z","title":"Theory for Baryon Number and Dark Matter at the LHC","venue":"hep-ph","work_id":"bf393488-8d24-444c-a469-af57f95b5f13","year":2014},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.001125Z"},"links":{"cited_paper":"/paper/1409.8165","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:b9d1824c748861fe44915bc5112fb6c75c1eb7a85f160f31acafc56e136dd228","observation_id":"e2f6cf48-0f35-47b9-8938-bf661dd46b64","resolution":{"observed_at":"2026-08-12T00:08:19.374370Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.05762","last_updated":"2022-09-16T14:56:06Z","snapshot_observed_at":"2026-07-06T13:09:03.269759Z","submitted_at":"2022-05-11T20:18:03Z","title":"Dirac dark matter, neutrino masses, and dark baryogenesis","version":3},"cited_work":{"arxiv_id":"2205.05762","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.05762","snapshot_observed_at":"2026-08-12T00:08:19.348861Z","title":"Dirac dark matter, neutrino masses, and dark baryogenesis","venue":"hep-ph","work_id":"db539e5f-0126-4915-87df-edeb5ad82789","year":2022},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.005343Z"},"links":{"cited_paper":"/paper/2205.05762","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:157f1052c80bc156d51e41af3109bcdb6fee78f6d8cd9877e2744d6a0ee2fae5","observation_id":"da786118-b55c-4eab-a78d-18cef0d5f09e","resolution":{"observed_at":"2026-08-12T00:08:19.353765Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.13101","last_updated":"2024-06-19T14:39:52Z","snapshot_observed_at":"2026-08-10T12:14:26.761843Z","submitted_at":"2024-01-23T21:29:22Z","title":"Singlet Dirac dark matter streamlined","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.13101","snapshot_observed_at":"2026-08-12T00:08:19.010378Z","title":"Singlet Dirac dark matter streamlined,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.010378Z"},"links":{"cited_paper":"/paper/2401.13101","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:a4a63c4fa47d82cbf6c1baab683b5f0f59f637d7473fd24b8682490b9b5bc303","observation_id":"7442cbe4-8adb-4c31-87f8-5ee3e5c29f43","resolution":{"observed_at":"2026-08-12T00:08:19.010378Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.14729","last_updated":"2023-08-05T21:12:39Z","snapshot_observed_at":"2026-08-12T12:00:40.671579Z","submitted_at":"2023-03-26T14:13:02Z","title":"First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.14729","snapshot_observed_at":"2026-08-12T00:08:19.015065Z","title":"First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.015065Z"},"links":{"cited_paper":"/paper/2303.14729","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:0b7d5a47d9903cc91c76f7e29ddfeb668601173e0d0a095f52751d06dc2c6b2d","observation_id":"729033ac-8bba-4e4b-bd72-24e6c92b03b0","resolution":{"observed_at":"2026-08-12T00:08:19.015065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.03764","last_updated":"2023-08-02T15:16:09Z","snapshot_observed_at":"2026-07-06T13:29:08.763456Z","submitted_at":"2022-07-08T09:10:04Z","title":"First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.03764","snapshot_observed_at":"2026-08-12T00:08:19.019454Z","title":"First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.019454Z"},"links":{"cited_paper":"/paper/2207.03764","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:584551e2f9fab3682c2894bf2100654801383947368e714f5550314744c1db39","observation_id":"55034f8d-01f3-46f5-90f4-eb026cc1fee1","resolution":{"observed_at":"2026-08-12T00:08:19.019454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.07001","last_updated":"2016-06-22T16:15:17Z","snapshot_observed_at":"2026-08-08T04:42:20.546683Z","submitted_at":"2016-06-22T16:15:17Z","title":"DARWIN: towards the ultimate dark matter detector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.07001","snapshot_observed_at":"2026-08-12T00:08:19.024587Z","title":"DAR WIN: towards the ultimate dark matter detector,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.024587Z"},"links":{"cited_paper":"/paper/1606.07001","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:438849cfe083d578f9f55119b8f59e88a4498bf36b46fd54024e5a31fa1b7d8a","observation_id":"35cff4e5-a717-413f-8749-a63724619d38","resolution":{"observed_at":"2026-08-12T00:08:19.024587Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5458","last_updated":"2014-01-19T18:10:55Z","snapshot_observed_at":"2026-07-06T03:18:44.842041Z","submitted_at":"2013-07-20T20:16:11Z","title":"Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.5458","snapshot_observed_at":"2026-08-12T00:08:19.029236Z","title":"Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.029236Z"},"links":{"cited_paper":"/paper/1307.5458","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:f244027e79f638d7ee4401aaddccdfa3a73d62eba5bad48dd0cc3a0417bd8554","observation_id":"18e7c1b6-77b4-40d3-8948-454827ae446b","resolution":{"observed_at":"2026-08-12T00:08:19.029236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.13710","last_updated":"2022-09-29T13:41:27Z","snapshot_observed_at":"2026-08-06T02:55:57.318748Z","submitted_at":"2022-06-28T02:52:32Z","title":"Concealing Dirac neutrinos from cosmic microwave background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.13710","snapshot_observed_at":"2026-08-12T00:08:19.033897Z","title":"Concealing Dirac neutrinos from cosmic microwave background,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.033897Z"},"links":{"cited_paper":"/paper/2206.13710","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:be6d15a2163b601faa5d8e69b787aec10fe2d1bc9f64b659c549f5bb524248d0","observation_id":"93879d33-73b3-481b-a63c-97061424de92","resolution":{"observed_at":"2026-08-12T00:08:19.033897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.03234","last_updated":"2019-04-30T15:16:12Z","snapshot_observed_at":"2026-07-06T07:32:03.637300Z","submitted_at":"2019-02-08T18:53:58Z","title":"Constraining the Spin-Dependent WIMP-Nucleon Cross Sections with XENON1T","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.03234","snapshot_observed_at":"2026-08-12T00:08:19.038789Z","title":"Constraining the spin-dependent WIMP-nucleon cross sections with XENON1T,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.038789Z"},"links":{"cited_paper":"/paper/1902.03234","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:eaed849bf79a529067c4c76b607749486e831f32f876f542236ba0930aa842e1","observation_id":"0097d2f8-edd1-449c-bbf4-aa026b5da86a","resolution":{"observed_at":"2026-08-12T00:08:19.038789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.2926","last_updated":"2009-01-30T23:37:56Z","snapshot_observed_at":"2026-08-02T10:08:54.917456Z","submitted_at":"2009-01-20T18:41:08Z","title":"Dark Matter Signals from Cascade Annihilations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.2926","snapshot_observed_at":"2026-08-12T00:08:19.042794Z","title":"Dark Matter Signals from Cascade Annihilations,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.042794Z"},"links":{"cited_paper":"/paper/0901.2926","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:cff1e9e62a9a57d6b56d5564989881a96f34a8ac454356c17ff435b091f6763e","observation_id":"eac92d5b-f2df-4327-8002-94b182c5995f","resolution":{"observed_at":"2026-08-12T00:08:19.042794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.04053","last_updated":"2021-09-30T18:12:19Z","snapshot_observed_at":"2026-08-12T17:54:18.728516Z","submitted_at":"2021-07-08T18:05:59Z","title":"Indirect Searches for Secluded Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.04053","snapshot_observed_at":"2026-08-12T00:08:19.048292Z","title":"Indirect Searches for Secluded Dark Matter,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.048292Z"},"links":{"cited_paper":"/paper/2107.04053","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:e3041788ac66a742268624780a2dfa19eee297e7a0499d55394126e521de6b57","observation_id":"2af140f4-d458-493a-87dd-0550a92f717e","resolution":{"observed_at":"2026-08-12T00:08:19.048292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02641","last_updated":"2015-11-03T08:32:32Z","snapshot_observed_at":"2026-07-06T04:11:25.940565Z","submitted_at":"2015-03-09T19:41:42Z","title":"Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi-LAT Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.02641","snapshot_observed_at":"2026-08-12T00:08:19.052993Z","title":"Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.052993Z"},"links":{"cited_paper":"/paper/1503.02641","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:ecbe588e410e05bceaae2d91672e8bb1da6fb15da1fe0e2b71dee7736b5b0d48","observation_id":"f528f8b6-833e-4415-9766-99dddfd9c905","resolution":{"observed_at":"2026-08-12T00:08:19.052993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08142","last_updated":"2016-07-27T15:19:00Z","snapshot_observed_at":"2026-08-11T00:39:28.074384Z","submitted_at":"2016-07-27T15:19:00Z","title":"Search for dark matter annihilations towards the inner Galactic halo from 10 years of observations with H.E.S.S","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.08142","snapshot_observed_at":"2026-08-12T00:08:19.058448Z","title":"Search for dark matter annihilations towards the inner Galac- tic halo from 10 years of observations with H.E.S.S,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.058448Z"},"links":{"cited_paper":"/paper/1607.08142","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:ee41e2bf5475324fbcfdd1f8365ea4654f775b7def2c4e1cecbdef4a344ef49c","observation_id":"3e7153dc-d2b7-48db-8ee6-3ecb65f28c56","resolution":{"observed_at":"2026-08-12T00:08:19.058448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.16129","last_updated":"2021-01-30T18:51:36Z","snapshot_observed_at":"2026-08-11T00:41:04.986550Z","submitted_at":"2020-07-31T15:14:59Z","title":"Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.16129","snapshot_observed_at":"2026-08-12T00:08:19.063969Z","title":"Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.063969Z"},"links":{"cited_paper":"/paper/2007.16129","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:274ce7c8965a9aa96f8ab51346d5a1fd00df9a1b817b1b34f1b9413fe667e4c1","observation_id":"57203758-97ea-414d-b382-f1d8a7437e11","resolution":{"observed_at":"2026-08-12T00:08:19.063969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.08858","last_updated":"2019-08-23T15:02:37Z","snapshot_observed_at":"2026-08-12T14:37:16.464474Z","submitted_at":"2019-08-23T15:02:37Z","title":"A next-generation ground-based wide field-of-view gamma-ray observatory in the southern hemisphere","version":1},"cited_work":{"arxiv_id":"1908.08858","doi":null,"metadata_source":"pith","pith_arxiv_id":"1908.08858","snapshot_observed_at":"2026-08-12T00:08:19.158262Z","title":"A next-generation ground-based wide field-of-view gamma-ray observatory in the southern hemisphere","venue":"astro-ph.HE","work_id":"0dd294d8-a428-4169-bfaf-bf64c4cb66ba","year":2019},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.068734Z"},"links":{"cited_paper":"/paper/1908.08858","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:a8c5b6a59e4310f1b739d1f8ad9cb2fca4b8aaa31192c1dc6e19cabfa60d757a","observation_id":"50163a51-9040-4862-a43f-7f2f75dcb327","resolution":{"observed_at":"2026-08-12T00:08:19.165062Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.11363","last_updated":"2019-11-13T23:25:07Z","snapshot_observed_at":"2026-08-11T00:12:03.206802Z","submitted_at":"2019-03-27T11:45:39Z","title":"Neutrinos and gamma rays from long-lived mediator decays in the Sun","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.11363","snapshot_observed_at":"2026-08-12T00:08:19.074137Z","title":"Neutrinos and gamma rays from long-lived mediator decays in the Sun,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.074137Z"},"links":{"cited_paper":"/paper/1903.11363","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:e9af664c4769c51e61fc14bf6986c9817684177d78e9273700ded26ea3fb8564","observation_id":"b893ebde-64e1-48af-bca1-bbbec035663c","resolution":{"observed_at":"2026-08-12T00:08:19.074137Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.16794","last_updated":"2021-09-19T08:20:36Z","snapshot_observed_at":"2026-08-11T04:05:47.189364Z","submitted_at":"2021-03-31T04:05:16Z","title":"Solar Gamma Ray Constraints on Dark Matter Annihilation to Secluded Mediators","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.16794","snapshot_observed_at":"2026-08-12T00:08:19.078820Z","title":"Solar gamma ray constraints on dark matter annihilation to secluded mediators,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.078820Z"},"links":{"cited_paper":"/paper/2103.16794","citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:cd08c3d11c4516e0d611d3b13fe1f4160af690b2cec852ad81fda56360943d68","observation_id":"762c1694-259d-4bd2-b014-e95a7f2c6281","resolution":{"observed_at":"2026-08-12T00:08:19.078820Z","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":"2026-08-12T00:08:19.083346Z","title":"Review of particle physics,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry","version":3},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-12T00:08:19.083346Z"},"links":{"citing_paper":"/paper/2412.02027"},"observation_digest":"sha256:d394b753727253caf0cdd6faf877557744d3fdf31c6075189e0b2e10edc375b0","observation_id":"d11e2f8a-c820-4bf1-a890-d257607d2db4","resolution":{"observed_at":"2026-08-12T00:08:19.083346Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.02027","last_updated":"2025-05-08T12:12:28Z","latest_version":3,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-12T17:54:38.801796Z","submitted_at":"2024-12-02T23:17:07Z","title":"Multi-component secluded WIMP dark matter and Dirac neutrino masses with an extra Abelian gauge symmetry"},"reference_resolution":{"displayed":94,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":77,"verified_exact":11,"verified_fuzzy":5},"total_outbound_references":94},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 94 of 94 outbound references and 2 inbound Pith citation observations for arXiv:2412.02027."}