{"as_of":"2026-08-16T20:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3dc4e0caae7dbb7eb864e05e04720dcbabf840dd04a2ca194f9a0604f9694105","coverage":[{"denominator":33,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":33,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T23:48:04.604453Z","state":"measured"},{"denominator":33,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":33,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.04056/citation-record","integrity":"/paper/2505.04056/integrity","json":"/paper/2505.04056/citation-record.json","paper":"/paper/2505.04056"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-15T23:48:04.447097Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.447097Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:92c8c2e09a65ae54304cee1973d44b35c82c2eb17759f705487c657804573f6c","observation_id":"e42f9c6a-7553-449a-a2c4-7d26c385860c","resolution":{"observed_at":"2026-08-15T23:48:04.447097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.06324","last_updated":"2015-12-02T15:41:20Z","snapshot_observed_at":"2026-08-14T22:51:14.649270Z","submitted_at":"2015-04-23T20:00:36Z","title":"Dynamical constraints on the dark matter distribution in the Milky Way","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.06324","snapshot_observed_at":"2026-08-15T23:48:04.453128Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.453128Z"},"links":{"cited_paper":"/paper/1504.06324","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:e2aad7140ee4d228433a7d127f2cc1c461342d45e45586ec40e3e80b5ae9dac4","observation_id":"c07ae9dc-95e8-4f12-94c8-8263043b5e4a","resolution":{"observed_at":"2026-08-15T23:48:04.453128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.03821","last_updated":"2015-02-12T21:00:09Z","snapshot_observed_at":"2026-08-14T23:00:13.118308Z","submitted_at":"2015-02-12T21:00:09Z","title":"Evidence for dark matter in the inner Milky Way","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.03821","snapshot_observed_at":"2026-08-15T23:48:04.458628Z","title":"Iocco, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.458628Z"},"links":{"cited_paper":"/paper/1502.03821","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:545a1a9bbf03e187f449025671d1a8a23e4d4c41d24f48a8efdbfbb2c3b760dd","observation_id":"346d297f-7aed-42c2-96c5-68055094d728","resolution":{"observed_at":"2026-08-15T23:48:04.458628Z","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":"2026-08-15T23:48:04.463690Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.463690Z"},"links":{"citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:6e47b7300caa5815fe958ed10d0cbe2d717e6fd4227b4b3dd5e7fc54e25e7a16","observation_id":"fa127409-84d0-4374-bfe1-2532f29ea3f6","resolution":{"observed_at":"2026-08-15T23:48:04.463690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.12838","last_updated":"2023-05-26T18:08:45Z","snapshot_observed_at":"2026-08-16T15:46:08.584918Z","submitted_at":"2023-03-22T18:00:08Z","title":"The dark matter profile of the Milky Way inferred from its circular velocity curve","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.12838","snapshot_observed_at":"2026-08-15T23:48:04.468406Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.468406Z"},"links":{"cited_paper":"/paper/2303.12838","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:14b700f50a427a90452e2ef74f54f45fa002d6f1652ea5b6af07c92c5aebb288","observation_id":"c94dba1f-3f38-4f8b-a166-b9f06e4d7e3f","resolution":{"observed_at":"2026-08-15T23:48:04.468406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608407","last_updated":"2006-08-19T17:51:03Z","snapshot_observed_at":"2026-08-15T11:05:40.330161Z","submitted_at":"2006-08-19T17:51:03Z","title":"A direct empirical proof of the existence of dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0608407","snapshot_observed_at":"2026-08-15T23:48:04.473823Z","title":"Clowe, M","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.473823Z"},"links":{"cited_paper":"/paper/astro-ph/0608407","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:9caad4f0e7900f3e5a5b1c35fd85c0b4a5d6b33dc8251a71ba2786a4f7157e7e","observation_id":"402402d1-9aed-47c6-8b56-ccf6749a4aa9","resolution":{"observed_at":"2026-08-15T23:48:04.473823Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.03906","last_updated":"2017-03-18T15:25:05Z","snapshot_observed_at":"2026-08-14T21:25:53.168010Z","submitted_at":"2016-12-12T21:00:00Z","title":"Cosmic particle colliders: simulations of self-interacting dark matter with anisotropic scattering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.03906","snapshot_observed_at":"2026-08-15T23:48:04.480097Z","title":"Robertson, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.480097Z"},"links":{"cited_paper":"/paper/1612.03906","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:1fc5596a5b28a0e88e0da77985bbe6073e60838a9a879495f2eb02a657845c9f","observation_id":"a1167d7f-ce04-4a6f-b1b0-a51011182f55","resolution":{"observed_at":"2026-08-15T23:48:04.480097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504097","last_updated":"2005-04-06T08:50:45Z","snapshot_observed_at":"2026-08-05T05:39:13.755503Z","submitted_at":"2005-04-05T07:08:11Z","title":"Simulating the joint evolution of quasars, galaxies and their large-scale distribution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504097","snapshot_observed_at":"2026-08-15T23:48:04.485101Z","title":"Springel, S","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.485101Z"},"links":{"cited_paper":"/paper/astro-ph/0504097","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:4be130f3de337e949518c2941a45b960520a24e022eabe8bc1ae061b94654156","observation_id":"814a5a86-bd8c-40e6-aaae-bf50efdeeef4","resolution":{"observed_at":"2026-08-15T23:48:04.485101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0404175","last_updated":"2004-08-13T15:46:27Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2004-04-21T13:12:59Z","title":"Particle Dark Matter: Evidence, Candidates and Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0404175","snapshot_observed_at":"2026-08-15T23:48:04.489953Z","title":"Bertone, D","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.489953Z"},"links":{"cited_paper":"/paper/hep-ph/0404175","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:9ed20015bccda6b4e124dedb8a18c0dbd33b937b58e70c0268999d19e8f60ba2","observation_id":"785731ab-afa9-409f-9069-ba1f073d1524","resolution":{"observed_at":"2026-08-15T23:48:04.489953Z","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":"10.1016/0370-2693(85)90689-6","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:48:04.679640Z","title":"Nussinov, Phys","venue":null,"work_id":"9cf1a7e3-a9f9-4c65-9881-aa0bd7d7ee5b","year":1985},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.494757Z"},"links":{"citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:7d6f53d08e9ad6d5cbc210faa2969a4f8372790fdadf16fb404472ee068125bc","observation_id":"7006f436-d8b4-4f10-ac0b-533d7904397a","resolution":{"observed_at":"2026-08-15T23:48:04.684681Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-15T23:48:04.499659Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.499659Z"},"links":{"citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:d1984db5422959d5a0b212c4d37340efe8b14f0f7b2b4fcdb7ee7e1ac1291002","observation_id":"d35fa167-92d1-4a13-a142-10716aa1e61f","resolution":{"observed_at":"2026-08-15T23:48:04.499659Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.4463","last_updated":"2010-03-04T15:42:56Z","snapshot_observed_at":"2026-08-15T05:33:13.633295Z","submitted_at":"2009-11-23T18:27:04Z","title":"Leptogenesis as a Common Origin for Matter and Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.4463","snapshot_observed_at":"2026-08-15T23:48:04.504449Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.504449Z"},"links":{"cited_paper":"/paper/0911.4463","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:bafd1208fd5a1c2dc696133b067fb909554f3f951545f0ab5c3cac0969750569","observation_id":"b174a776-8df4-4dd4-9372-6c406c83c050","resolution":{"observed_at":"2026-08-15T23:48:04.504449Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.2035","last_updated":"2009-09-11T00:58:52Z","snapshot_observed_at":"2026-08-15T05:39:21.075106Z","submitted_at":"2009-09-11T00:58:52Z","title":"Leptophilic Dark Matter from the Lepton Asymmetry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.2035","snapshot_observed_at":"2026-08-15T23:48:04.509073Z","title":"Cohen and K","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.509073Z"},"links":{"cited_paper":"/paper/0909.2035","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:3b6f63f45ae750c59c73f000d7507231379fcb31c782161a9121a6215bbd924a","observation_id":"fde88fa3-f489-42f3-ae2c-16f7c35aef97","resolution":{"observed_at":"2026-08-15T23:48:04.509073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.1997","last_updated":"2010-08-11T20:16:23Z","snapshot_observed_at":"2026-08-15T05:11:39.667684Z","submitted_at":"2010-08-11T20:16:23Z","title":"Darkogenesis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.1997","snapshot_observed_at":"2026-08-15T23:48:04.513832Z","title":"Shelton and K","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.513832Z"},"links":{"cited_paper":"/paper/1008.1997","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:a864477a5e85a665e698a58b5f383c6743931fd38a7cbc6686f581615d88e24c","observation_id":"5af90d34-1544-430f-8f3a-5ce4f549e8db","resolution":{"observed_at":"2026-08-15T23:48:04.513832Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0410114","last_updated":"2004-12-14T17:34:02Z","snapshot_observed_at":"2026-07-07T04:05:12.693563Z","submitted_at":"2004-10-07T15:39:23Z","title":"Asymmetric Sneutrino Dark Matter and the Omega(b)/Omega(DM) Puzzle","version":2},"cited_work":{"arxiv_id":"hep-ph/0410114","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0410114","snapshot_observed_at":"2026-08-15T23:48:05.016250Z","title":"Asymmetric Sneutrino Dark Matter and the Omega(b)/Omega(DM) Puzzle","venue":"hep-ph","work_id":"fef8cceb-2ec6-4199-b8c6-b6cecab2124d","year":2004},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.518473Z"},"links":{"cited_paper":"/paper/hep-ph/0410114","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:b7413c948a1f1ba7937004ec3a004dfd328b35a87c6f4538ad939ad28765e84a","observation_id":"7b606f95-5ce7-4ff4-9a8f-496648d435e6","resolution":{"observed_at":"2026-08-15T23:48:05.020939Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0609140","last_updated":"2006-09-14T15:52:50Z","snapshot_observed_at":"2026-08-15T11:03:24.422509Z","submitted_at":"2006-09-14T15:52:50Z","title":"(Pseudo)-Dirac neutrinos and leptogenesis","version":1},"cited_work":{"arxiv_id":"hep-ph/0609140","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0609140","snapshot_observed_at":"2026-08-15T23:48:04.993580Z","title":"(Pseudo)-Dirac neutrinos and leptogenesis","venue":"hep-ph","work_id":"0b4f8c7f-d732-4413-9da5-15a5b2335249","year":2006},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.523346Z"},"links":{"cited_paper":"/paper/hep-ph/0609140","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:84787eb3f4ea02f2ef8b6c114684bf6d510b020524dd813e88044de75b64e943","observation_id":"28a6e490-19d0-43d3-9b0b-30831bcb3f69","resolution":{"observed_at":"2026-08-15T23:48:04.999778Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0901.4117","last_updated":"2009-01-27T16:17:41Z","snapshot_observed_at":"2026-08-15T05:56:32.712829Z","submitted_at":"2009-01-27T16:17:41Z","title":"Asymmetric Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.4117","snapshot_observed_at":"2026-08-15T23:48:04.528003Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.528003Z"},"links":{"cited_paper":"/paper/0901.4117","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:06edd662e7ebd6f28f4e45f216b3aefa039ee5ee3f1e895fdd00770c947a490e","observation_id":"2a14dd0d-8dae-45a0-b005-9fce2a70ae14","resolution":{"observed_at":"2026-08-15T23:48:04.528003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2549","last_updated":"2011-09-07T07:19:10Z","snapshot_observed_at":"2026-08-15T04:49:27.610011Z","submitted_at":"2011-04-13T17:02:49Z","title":"Dark Matter Results from 100 Live Days of XENON100 Data","version":3},"cited_work":{"arxiv_id":"1104.2549","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2549","snapshot_observed_at":"2026-08-15T23:48:04.956233Z","title":"Dark Matter Results from 100 Live Days of XENON100 Data","venue":"astro-ph.CO","work_id":"fc8c1273-cdac-4970-ab58-c9ec1b09b742","year":2011},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.532670Z"},"links":{"cited_paper":"/paper/1104.2549","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:15da59f5e07eaa57b96b58f8bf07331938a48b64bcdd9bd923441efc677bfc0f","observation_id":"8a062266-9ccb-4846-939b-25982075adea","resolution":{"observed_at":"2026-08-15T23:48:04.961511Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-15T23:48:05.343520Z","title":"Turner, Addison-Wesley (1990)","venue":null,"work_id":"bfd8d00c-d074-4179-9264-6f8f2df6d042","year":1990},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.537672Z"},"links":{"citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:bbb2d5aee06256b10d359aeced6dd17dd9409c84c506a51b594f7c1dd88da5f1","observation_id":"bba5b982-b760-4d68-98e4-667f849ddea0","resolution":{"observed_at":"2026-08-15T23:48:05.348472Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1205.0673","last_updated":"2012-06-23T12:19:07Z","snapshot_observed_at":"2026-08-16T13:12:05.290608Z","submitted_at":"2012-05-03T11:05:00Z","title":"Upper Bounds on Asymmetric Dark Matter Self Annihilation Cross Sections","version":3},"cited_work":{"arxiv_id":"1205.0673","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.0673","snapshot_observed_at":"2026-08-15T23:48:04.934928Z","title":"Upper Bounds on Asymmetric Dark Matter Self Annihilation Cross Sections","venue":"hep-ph","work_id":"dd318515-63b0-4734-ab76-422952841a7e","year":2012},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.542137Z"},"links":{"cited_paper":"/paper/1205.0673","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:694d46790f7f7efa0536bb93282d33d270c72125a5ddab7a2f961bd89942d93f","observation_id":"74d95eaf-9db0-4d54-8ce5-bdaefda43081","resolution":{"observed_at":"2026-08-15T23:48:04.939926Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.09155","last_updated":"2024-02-09T04:43:34Z","snapshot_observed_at":"2026-08-16T15:00:05.098761Z","submitted_at":"2023-09-17T04:43:05Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections in Non-standard Cosmological Scenarios","version":3},"cited_work":{"arxiv_id":"2309.09155","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.09155","snapshot_observed_at":"2026-08-15T23:48:04.914247Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections in Non-standard Cosmological Scenarios","venue":"hep-ph","work_id":"50663545-89ab-4bf8-850c-3d7de11ceee8","year":2023},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.546973Z"},"links":{"cited_paper":"/paper/2309.09155","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:93e1acb40574533d530e5c9978e94081df66863cabd87f993027f64b2562f939","observation_id":"d3ee1fdf-faa1-4937-bf4c-98347029d11f","resolution":{"observed_at":"2026-08-15T23:48:04.919140Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1308.0353","last_updated":"2013-08-01T20:49:45Z","snapshot_observed_at":"2026-08-15T00:08:06.532995Z","submitted_at":"2013-08-01T20:49:45Z","title":"Relic Abundance of Asymmetric Dark Matter in Quintessence","version":1},"cited_work":{"arxiv_id":"1308.0353","doi":null,"metadata_source":"pith","pith_arxiv_id":"1308.0353","snapshot_observed_at":"2026-08-15T23:48:04.893107Z","title":"Relic Abundance of Asymmetric Dark Matter in Quintessence","venue":"hep-ph","work_id":"a49654cf-36fd-461d-a3f1-87807150bcc0","year":2013},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.551652Z"},"links":{"cited_paper":"/paper/1308.0353","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:e5da65643b3271a51b0edac3fd1a4a0829e90eeb9d99b11d1bef14418cfb61a9","observation_id":"e890f3bd-52a8-4877-bb63-3c2b890bbc59","resolution":{"observed_at":"2026-08-15T23:48:04.898172Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1403.6934","last_updated":"2014-05-07T12:51:49Z","snapshot_observed_at":"2026-08-14T23:39:46.451074Z","submitted_at":"2014-03-27T07:35:09Z","title":"Asymmetric dark matter in braneworld cosmology","version":2},"cited_work":{"arxiv_id":"1403.6934","doi":null,"metadata_source":"pith","pith_arxiv_id":"1403.6934","snapshot_observed_at":"2026-08-15T23:48:04.871138Z","title":"Asymmetric dark matter in braneworld cosmology","venue":"astro-ph.CO","work_id":"d1888d13-3145-4316-af29-f8c429d09241","year":2014},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.556330Z"},"links":{"cited_paper":"/paper/1403.6934","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:30589c0d6c924df709082ef0a003a7641be218f3206b19eda08e640c0b652bc7","observation_id":"031d3c65-a1f1-44da-a61b-9ee44ca5ed99","resolution":{"observed_at":"2026-08-15T23:48:04.876166Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.03716","last_updated":"2016-02-25T17:47:41Z","snapshot_observed_at":"2026-08-14T22:48:35.247116Z","submitted_at":"2015-05-14T13:18:51Z","title":"Abundance of Asymmetric Dark Matter in Brane World Cosmology","version":2},"cited_work":{"arxiv_id":"1505.03716","doi":null,"metadata_source":"pith","pith_arxiv_id":"1505.03716","snapshot_observed_at":"2026-08-15T23:48:04.848116Z","title":"Abundance of Asymmetric Dark Matter in Brane World Cosmology","venue":"hep-ph","work_id":"2fb74529-33b5-41f2-abe6-a1d9f8eaba11","year":2015},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.561020Z"},"links":{"cited_paper":"/paper/1505.03716","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:2fa0620f589e8ef93eb023f09e27dc7fb7c057000962a7a420d11d0bd4b5cc94","observation_id":"2dbbd5c5-8389-4527-94a0-23ad1c249f19","resolution":{"observed_at":"2026-08-15T23:48:04.853975Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1508.05174","last_updated":"2015-10-19T06:16:02Z","snapshot_observed_at":"2026-08-14T22:35:45.532761Z","submitted_at":"2015-08-21T04:35:26Z","title":"Dark matter relic density in scalar-tensor gravity revisited","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1508.05174","snapshot_observed_at":"2026-08-15T23:48:04.565824Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.565824Z"},"links":{"cited_paper":"/paper/1508.05174","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:b337a8ff9e8747d4070a0e384291bdfca5b9ead9d374eebcdbddd70f2c2d9240","observation_id":"72a522b8-b14b-4d0c-a83f-ee94ca432d49","resolution":{"observed_at":"2026-08-15T23:48:04.565824Z","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":"10.1016/0550-3213(82)90233-4","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:48:04.652796Z","title":null,"venue":null,"work_id":"28510af3-7776-4a0f-9d56-4dbe3f65c2fe","year":1982},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.570579Z"},"links":{"citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:eaefbdf40e1cdef404350352c30efe9796c3f753583f6dff2645f15a4b09ed51","observation_id":"881dec6f-7267-4333-a724-3b740a4d5f52","resolution":{"observed_at":"2026-08-15T23:48:04.657478Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.42.3310","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:48:04.635763Z","title":"Kamionkowski and M","venue":null,"work_id":"564418c4-ca8f-452c-8a5a-e815f7e183b5","year":1990},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.575222Z"},"links":{"citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:d94baeebfb01ad9b07b517ab506213b712187335ddec322e288211ada1377c3d","observation_id":"d4690d82-23fe-427a-83de-90162d542407","resolution":{"observed_at":"2026-08-15T23:48:04.641786Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1604.04251","last_updated":"2016-08-01T15:04:31Z","snapshot_observed_at":"2026-08-14T22:01:38.984470Z","submitted_at":"2016-04-14T18:28:30Z","title":"Asymmetric Dark Matter in the Shear--dominated Universe","version":2},"cited_work":{"arxiv_id":"1604.04251","doi":null,"metadata_source":"pith","pith_arxiv_id":"1604.04251","snapshot_observed_at":"2026-08-15T23:48:04.808791Z","title":"Asymmetric Dark Matter in the Shear--dominated Universe","venue":"hep-ph","work_id":"6b65c6f0-c800-490c-93f0-c5f4b0315660","year":2016},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.579744Z"},"links":{"cited_paper":"/paper/1604.04251","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:25ae199a5dec7ff6f1001cfe8c6c16220865bc441c7972354cf34f8884b0c0c3","observation_id":"5e641c1a-fcf2-40e0-8ca8-da0393d21e92","resolution":{"observed_at":"2026-08-15T23:48:04.813702Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0209261","last_updated":"2002-09-30T14:46:50Z","snapshot_observed_at":"2026-08-12T01:48:13.123304Z","submitted_at":"2002-09-30T14:46:50Z","title":"Brane cosmology: an introduction","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0209261","snapshot_observed_at":"2026-08-15T23:48:04.584867Z","title":"Langlois, Prog","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.584867Z"},"links":{"cited_paper":"/paper/hep-th/0209261","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:f9e078326650899087af593b299865844788f69cd0d7e88bd8f168351c67d67e","observation_id":"47c884fb-4784-47f7-b1e9-3d8a3e9584ba","resolution":{"observed_at":"2026-08-15T23:48:04.584867Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0903.2384","last_updated":"2009-03-29T07:17:22Z","snapshot_observed_at":"2026-08-15T05:52:59.771797Z","submitted_at":"2009-03-13T13:33:26Z","title":"Gauss-Bonnet braneworld cosmological effect on relic density of dark matter","version":2},"cited_work":{"arxiv_id":"0903.2384","doi":null,"metadata_source":"pith","pith_arxiv_id":"0903.2384","snapshot_observed_at":"2026-08-15T23:48:04.767878Z","title":"Gauss-Bonnet braneworld cosmological effect on relic density of dark matter","venue":"hep-ph","work_id":"74be7684-96f2-4bbe-a825-7e2acbc8149d","year":2009},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.589962Z"},"links":{"cited_paper":"/paper/0903.2384","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:6dafe02490f9e3704b393c4c21b8956b1ebabb637f21176a7306b96f84304e0d","observation_id":"a04cab0c-7e26-4d8e-aeec-d53310cce273","resolution":{"observed_at":"2026-08-15T23:48:04.773457Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.4424","last_updated":"2014-11-18T03:28:08Z","snapshot_observed_at":"2026-08-14T23:37:14.260842Z","submitted_at":"2014-04-17T05:28:06Z","title":"Dark matter relic density in Gauss-Bonnet braneworld cosmology","version":3},"cited_work":{"arxiv_id":"1404.4424","doi":null,"metadata_source":"pith","pith_arxiv_id":"1404.4424","snapshot_observed_at":"2026-08-15T23:48:04.746161Z","title":"Dark matter relic density in Gauss-Bonnet braneworld cosmology","venue":"astro-ph.CO","work_id":"ee2b3b0f-fd14-445b-9aeb-f691eb2e5905","year":2014},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.594807Z"},"links":{"cited_paper":"/paper/1404.4424","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:2ec5a932240c83ba0e03af8f438f3979a76beaec9184f6f4afc96ba005f2678e","observation_id":"6fb133a0-aca8-48a0-af84-a53eb203807b","resolution":{"observed_at":"2026-08-15T23:48:04.751394Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1102.5644","last_updated":"2016-05-18T14:29:10Z","snapshot_observed_at":"2026-08-15T04:53:32.258466Z","submitted_at":"2011-02-28T12:23:47Z","title":"The Maximal $U(1)_L$ Inverse Seesaw from $d=5$ Operator and Oscillating Asymmetric Sneutrino Dark Matter","version":3},"cited_work":{"arxiv_id":"1102.5644","doi":null,"metadata_source":"pith","pith_arxiv_id":"1102.5644","snapshot_observed_at":"2026-08-15T23:48:04.718184Z","title":"The Maximal $U(1)_L$ Inverse Seesaw from $d=5$ Operator and Oscillating Asymmetric Sneutrino Dark Matter","venue":"hep-ph","work_id":"2a56e1ae-b8e5-42a4-a5c6-d7b0388e0c21","year":2011},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.599591Z"},"links":{"cited_paper":"/paper/1102.5644","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:da382a8ca31d60212041af396239a79d4fa05cf272adc59e77138d79ca99f65a","observation_id":"78c6de99-6fdf-48a8-890e-f595dcd8fc45","resolution":{"observed_at":"2026-08-15T23:48:04.724083Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0202009","last_updated":"2002-05-08T13:27:09Z","snapshot_observed_at":"2026-07-07T03:55:08.289874Z","submitted_at":"2002-02-02T08:11:59Z","title":"Exact Cross Sections for the Neutralino WIMP Pair-Annihilation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0202009","snapshot_observed_at":"2026-08-15T23:48:04.604453Z","title":"Nihei, L","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-15T23:48:04.604453Z"},"links":{"cited_paper":"/paper/hep-ph/0202009","citing_paper":"/paper/2505.04056"},"observation_digest":"sha256:589d45559e7b43b53a7c63e3fed01e19c889d41223c67968ccb91cb544c1cfcd","observation_id":"38aba995-0cdc-4d6d-b3e0-9ce352ff0ad1","resolution":{"observed_at":"2026-08-15T23:48:04.604453Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.04056","last_updated":"2025-05-07T01:54:22Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-16T18:16:57.829561Z","submitted_at":"2025-05-07T01:54:22Z","title":"Constraints on Asymmetric Dark Matter Self Annihilation Cross Sections"},"reference_resolution":{"displayed":33,"state_counts":{"malformed_identifier":1,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":16,"verified_exact":15,"verified_fuzzy":1},"total_outbound_references":33},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 33 of 33 outbound references and 0 inbound Pith citation observations for arXiv:2505.04056."}