{"as_of":"2026-08-09T10:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9281128fc1ade204c2aa7cc7af23529fb0328ff0b4c615f09809cab8a3a835b5","coverage":[{"denominator":84,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":84,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T11:30:49.227031Z","state":"measured"},{"denominator":85,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":85,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-08T18:11:15.319148Z","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":"2026-05-09T06:45:40.009147Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"cited_work":{"arxiv_id":"2502.07932","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.07932","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Asymmetric dark matter in SUSY with approximate R-symmetry","venue":null,"work_id":"2693612f-9e56-4d9e-a003-dad8f3cfdca2","year":2025},"citing_paper":{"arxiv_id":"2605.04146","last_updated":"2026-05-05T18:00:01Z","snapshot_observed_at":"2026-07-06T23:16:59.568304Z","submitted_at":"2026-05-05T18:00:01Z","title":"(Pseudo-)Dirac Gravitinos","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-08T18:11:15.319148Z"},"links":{"cited_paper":"/paper/2502.07932","citing_paper":"/paper/2605.04146"},"observation_digest":"sha256:2eb068d0ac722c72bfcfe60bb98615e110db8b9245da0f1de78e8961df698828","observation_id":"91a20208-9144-4d01-8f1a-7e9f2190c737","resolution":{"observed_at":"2026-05-09T06:45:40.012619Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2502.07932/citation-record","integrity":"/paper/2502.07932/integrity","json":"/paper/2502.07932/citation-record.json","paper":"/paper/2502.07932"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-08T11:30:48.780612Z","title":"Zwicky,Die Rotverschiebung von extragalaktischen Nebeln, Helv","venue":null,"work_id":null,"year":1933},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.780612Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:ddbb20fd878cf9837e3d8b8bf95098ae185c40f415fcbe9c2028d9ae253c1cf3","observation_id":"40c67da2-c57e-48f0-909b-b19a36847158","resolution":{"observed_at":"2026-08-08T11:30:48.780612Z","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":"2026-08-08T11:30:48.787403Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.787403Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:58bda229667e0e54e696357415449e03d7d645b4fbe1519fdbbc66d470468673","observation_id":"a4f50af9-437a-4f32-bad4-c09203a042c5","resolution":{"observed_at":"2026-08-08T11:30:48.787403Z","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":"2026-08-08T11:30:48.792885Z","title":"Bertone, D","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.792885Z"},"links":{"cited_paper":"/paper/hep-ph/0404175","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:8b988400fee82c6262971a6fcad1b910a90a1deebf34da12ccc05b20ddd233a0","observation_id":"e84acaee-6530-4bd5-a4d9-fd23f86c011f","resolution":{"observed_at":"2026-08-08T11:30:48.792885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9506380","last_updated":"1995-06-22T03:59:24Z","snapshot_observed_at":"2026-08-06T22:00:10.863471Z","submitted_at":"1995-06-22T03:59:24Z","title":"Supersymmetric Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9506380","snapshot_observed_at":"2026-08-08T11:30:48.804621Z","title":"Jungman, M","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.804621Z"},"links":{"cited_paper":"/paper/hep-ph/9506380","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:889d845bf5454151328ea441de9b6ac51ac7b757ff029d6e6bd91599975e0046","observation_id":"fb18387e-2f50-4afb-9f4e-5a0d2ec170a8","resolution":{"observed_at":"2026-08-08T11:30:48.804621Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.01705","last_updated":"2025-12-03T08:11:10Z","snapshot_observed_at":"2026-08-06T19:42:34.309381Z","submitted_at":"2024-06-03T18:03:11Z","title":"Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.01705","snapshot_observed_at":"2026-08-08T11:30:48.810539Z","title":"Cirelli, A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.810539Z"},"links":{"cited_paper":"/paper/2406.01705","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:ab81c0c984a5607a46544f34460653aa8293e24cc6ca301bcbd1bb828c928c96","observation_id":"36798638-1657-4a55-a32b-8d17e74ccba0","resolution":{"observed_at":"2026-08-08T11:30:48.810539Z","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":"2026-08-08T11:30:48.816390Z","title":"Aghanim et al.,Planck 2018 results","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.816390Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:8f371b03f3b4164b2f94a08ff6ccdde02e91dcc3b470f002175d23da1c75c2a7","observation_id":"c45f861a-1933-462d-8a61-9ff633bfa8da","resolution":{"observed_at":"2026-08-08T11:30:48.816390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9312215","last_updated":"1993-12-02T21:29:29Z","snapshot_observed_at":"2026-07-07T04:16:25.965552Z","submitted_at":"1993-12-02T21:29:29Z","title":"Standard Model CP-violation and Baryon asymmetry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9312215","snapshot_observed_at":"2026-08-08T11:30:48.822260Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.822260Z"},"links":{"cited_paper":"/paper/hep-ph/9312215","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:bc6dac4e44e454b771926d7f1aa7e2c0ff9d9cc97815595077335c3fa54d9d76","observation_id":"1adf4f14-1f5d-43c1-b495-0ad6c15919ae","resolution":{"observed_at":"2026-08-08T11:30:48.822260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9404302","last_updated":"1994-04-20T03:34:00Z","snapshot_observed_at":"2026-08-05T18:43:03.854724Z","submitted_at":"1994-04-20T03:34:00Z","title":"Electroweak Baryogenesis and Standard Model CP Violation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9404302","snapshot_observed_at":"2026-08-08T11:30:48.828406Z","title":"Huet and E","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.828406Z"},"links":{"cited_paper":"/paper/hep-ph/9404302","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:cbe65164109f25f6d4a4d9be2bcba0a186d525d9d405e11e88a3f367250104b8","observation_id":"38b6f4c4-4842-41ae-95b8-479e0e9ea396","resolution":{"observed_at":"2026-08-08T11:30:48.828406Z","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":"2026-08-08T11:30:48.834676Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.834676Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:a64b6c6dc161cef6cd850ab1e70e47ab138f34c2efc692c0e01f6ac5baee354f","observation_id":"d2ca6bf8-80f8-4f85-80b9-0bc226453903","resolution":{"observed_at":"2026-08-08T11:30:48.834676Z","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":"2026-08-08T11:30:48.839541Z","title":"Nussinov,TECHNOCOSMOLOGY: COULD A TECHNIBARYON EXCESS PROVIDE A ’NATURAL’ MISSING MASS CANDIDATE?, Phys","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.839541Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:d5f9be574fbdfbfbdd5091a9c3d5aa73eef833cdfe648a08118a319fe924bdcd","observation_id":"3bfd9e4c-04dd-4439-809d-4a17ada615ba","resolution":{"observed_at":"2026-08-08T11:30:48.839541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.4153","last_updated":"2008-11-25T19:22:20Z","snapshot_observed_at":"2026-07-06T01:51:37.939453Z","submitted_at":"2008-11-25T19:22:20Z","title":"Decaying Dark Matter can explain the electron/positron excesses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.4153","snapshot_observed_at":"2026-08-08T11:30:48.844435Z","title":"Nardi, F","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.844435Z"},"links":{"cited_paper":"/paper/0811.4153","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:46f395d002260aee37d51c6c0934e425f212fc776578236a1ee45c3da8c6c296","observation_id":"ce4bdfc5-d699-4ec5-bad9-29bdecb26b1a","resolution":{"observed_at":"2026-08-08T11:30:48.844435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.4117","last_updated":"2009-01-27T16:17:41Z","snapshot_observed_at":"2026-07-06T01:50:51.146843Z","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":"2026-08-08T11:30:48.849917Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.849917Z"},"links":{"cited_paper":"/paper/0901.4117","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:706d8a42195d7a33241ddcab4b380fe429ddd162cf907931240333e182f1cdba","observation_id":"ef882e47-b5da-4529-b8e0-f3acfc3a19ea","resolution":{"observed_at":"2026-08-08T11:30:48.849917Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1305.4939","last_updated":"2013-08-01T08:24:44Z","snapshot_observed_at":"2026-07-06T03:13:53.392996Z","submitted_at":"2013-05-21T20:00:07Z","title":"Review of asymmetric dark matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1305.4939","snapshot_observed_at":"2026-08-08T11:30:48.855247Z","title":"Petraki and R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.855247Z"},"links":{"cited_paper":"/paper/1305.4939","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:419f1795a050d7371a381f7ada4598b19ab48feefc4a2c448ba6867bdb3e4864","observation_id":"7be82982-d6cf-4bfc-8407-a79f06caa083","resolution":{"observed_at":"2026-08-08T11:30:48.855247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.0338","last_updated":"2013-11-19T15:00:01Z","snapshot_observed_at":"2026-07-06T03:19:47.291095Z","submitted_at":"2013-08-01T20:00:07Z","title":"Asymmetric Dark Matter: Theories, Signatures, and Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.0338","snapshot_observed_at":"2026-08-08T11:30:48.860196Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.860196Z"},"links":{"cited_paper":"/paper/1308.0338","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:c56994ae7d4b30d7f786f28ecfac6c2d99e5494afb773c21aa88b7383f435305","observation_id":"fad466b1-f8a0-4775-b732-8f0944f3bdb3","resolution":{"observed_at":"2026-08-08T11:30:48.860196Z","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":"2026-07-06T02:14:04.582357Z","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":"2026-08-08T11:30:48.865044Z","title":"Shelton and K","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.865044Z"},"links":{"cited_paper":"/paper/1008.1997","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:c9ae392283e127b35bb1649fe851fb06c8a75095fe93475dac0a3385e8bb4f85","observation_id":"4988a4d8-3e13-473d-abf9-066b0ff91c9f","resolution":{"observed_at":"2026-08-08T11:30:48.865044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.2487","last_updated":"2011-05-24T06:08:09Z","snapshot_observed_at":"2026-07-06T02:14:09.821466Z","submitted_at":"2010-08-15T01:30:06Z","title":"Baryogenesis from Dark Sector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.2487","snapshot_observed_at":"2026-08-08T11:30:48.870112Z","title":"Haba and S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.870112Z"},"links":{"cited_paper":"/paper/1008.2487","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:a6f615e37ad282a8e9f66d1e18542009deb9a2830519fc06e53276420796c875","observation_id":"95c3fce5-c71d-465d-8ffe-323c10df570e","resolution":{"observed_at":"2026-08-08T11:30:48.870112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.4350","last_updated":"2011-03-22T19:14:05Z","snapshot_observed_at":"2026-07-06T02:25:13.374071Z","submitted_at":"2011-03-22T19:14:05Z","title":"Light asymmetric dark matter from new strong dynamics","version":1},"cited_work":{"arxiv_id":"1103.4350","doi":null,"metadata_source":"pith","pith_arxiv_id":"1103.4350","snapshot_observed_at":"2026-08-08T11:30:50.130328Z","title":"Light asymmetric dark matter from new strong dynamics","venue":"hep-ph","work_id":"bbe82c75-cf3e-4953-921d-f95917396f0c","year":2011},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.875584Z"},"links":{"cited_paper":"/paper/1103.4350","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:03cf77035fba0909d2fd9a1cd85e993f49c27770901de403408dc674b04954cb","observation_id":"c4ac2260-23c8-45a6-8ee8-a07a1ed0477e","resolution":{"observed_at":"2026-08-08T11:30:50.135834Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.768119Z","title":null,"venue":null,"work_id":"ac877989-75b4-4bcc-b60e-c782051362e9","year":1985},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.881131Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:6d3adaa719a15afd4f0a27bfa16c56bfeaee630731358c33165f6f9a324f6f22","observation_id":"58ed042d-3e46-4715-b5b9-f52b2d897627","resolution":{"observed_at":"2026-08-08T11:30:50.773040Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.749751Z","title":null,"venue":null,"work_id":"d8218bb3-6380-4a51-bd37-b7931151e5c2","year":1984},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.885769Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:1e66f209b8f51a11727c99dc03652eeceb63518951ab3c19ed1891ba3bf4e5db","observation_id":"c4b82c4c-3392-4af0-8e86-8a37f6a68132","resolution":{"observed_at":"2026-08-08T11:30:50.756324Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0312378","last_updated":"2003-12-30T16:44:46Z","snapshot_observed_at":"2026-07-07T04:02:26.341456Z","submitted_at":"2003-12-30T16:44:46Z","title":"The Soft Supersymmetry-Breaking Lagrangian: Theory and Applications","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0312378","snapshot_observed_at":"2026-08-08T11:30:48.890934Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.890934Z"},"links":{"cited_paper":"/paper/hep-ph/0312378","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:6d41c335c9c1d27e5c03a0f1b996ef0077c42ea3bea9541ce824524740d93439","observation_id":"d8ff5be6-3ce9-40a0-ba74-707efb00590c","resolution":{"observed_at":"2026-08-08T11:30:48.890934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.7313","last_updated":"2012-11-29T20:47:18Z","snapshot_observed_at":"2026-08-09T01:37:55.065520Z","submitted_at":"2011-11-30T20:45:55Z","title":"Asymmetric Origin for Gravitino Relic Density in the Hybrid Gravity-Gauge Mediated Supersymmetry Breaking","version":3},"cited_work":{"arxiv_id":"1111.7313","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.7313","snapshot_observed_at":"2026-08-08T11:30:50.090819Z","title":"Asymmetric Origin for Gravitino Relic Density in the Hybrid Gravity-Gauge Mediated Supersymmetry Breaking","venue":"hep-ph","work_id":"5c275dcf-0a61-4489-8bd6-32aa1356e5ed","year":2011},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.896450Z"},"links":{"cited_paper":"/paper/1111.7313","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:1de3f74b0e46c5342ce748e2cf45f3de34b0bea9dd550badcd7c665b8b965e4d","observation_id":"755e7aaf-b732-438f-bcae-2d60f7dbe76d","resolution":{"observed_at":"2026-08-08T11:30:50.096316Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.5615","last_updated":"2012-03-07T15:48:35Z","snapshot_observed_at":"2026-07-06T02:38:06.755490Z","submitted_at":"2011-11-23T21:00:02Z","title":"Dark Matter Assimilation into the Baryon Asymmetry","version":3},"cited_work":{"arxiv_id":"1111.5615","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.5615","snapshot_observed_at":"2026-08-08T11:30:50.065565Z","title":"Dark Matter Assimilation into the Baryon Asymmetry","venue":"hep-ph","work_id":"d1811716-956f-4c69-9d10-3b0ebf8ba133","year":2011},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.901472Z"},"links":{"cited_paper":"/paper/1111.5615","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:6f61003778cfcf9d157d8aa9a6445b6d336c047fdc22b2c52249b455ae022a00","observation_id":"3746bbea-147d-48ba-a2f7-4be7a1a20dfc","resolution":{"observed_at":"2026-08-08T11:30:50.071502Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0802.2962","last_updated":"2008-06-06T18:05:54Z","snapshot_observed_at":"2026-07-06T01:35:41.376119Z","submitted_at":"2008-02-20T23:35:35Z","title":"Leptogenesis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0802.2962","snapshot_observed_at":"2026-08-08T11:30:48.906362Z","title":"Davidson, E","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.906362Z"},"links":{"cited_paper":"/paper/0802.2962","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:823c689af032d6bdbb1ed414e981631110ccf05162a9c35e5dcb34fe92b02232","observation_id":"49f7f666-dff7-49ce-8c6d-3f1795ce256d","resolution":{"observed_at":"2026-08-08T11:30:48.906362Z","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":"2026-08-08T11:30:50.731819Z","title":"Affleck and M","venue":null,"work_id":"9e47fce6-3905-47b5-8b3a-a22e283f9537","year":1985},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.911583Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:0481e3e205088a37af9847268bdf75d47411b2ff4ac542d6ba52ba7e0f4ce281","observation_id":"49e67936-41cc-4a64-a9e8-46282d959b92","resolution":{"observed_at":"2026-08-08T11:30:50.737999Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9707235","last_updated":"1997-07-03T12:07:40Z","snapshot_observed_at":"2026-07-07T04:26:14.581072Z","submitted_at":"1997-07-03T12:07:40Z","title":"CP Violation and Baryogenesis due to Heavy Majorana Neutrinos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9707235","snapshot_observed_at":"2026-08-08T11:30:48.916624Z","title":"Pilaftsis,CP violation and baryogenesis due to heavy Majorana neutrinos, Phys","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.916624Z"},"links":{"cited_paper":"/paper/hep-ph/9707235","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:5fb0c4d6869f2c535269f5ba5bcfe76fbb8f92ccaa4f20acd90c5fc4bf8a498b","observation_id":"d84d8983-ba1c-4e1c-9f97-9deb3992cdac","resolution":{"observed_at":"2026-08-08T11:30:48.916624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0006173","last_updated":"2000-06-15T14:40:09Z","snapshot_observed_at":"2026-07-07T03:48:52.589439Z","submitted_at":"2000-06-15T14:40:09Z","title":"Leptogenesis from Neutralino Decay with Nonholomorphic R-Parity Violation","version":1},"cited_work":{"arxiv_id":"hep-ph/0006173","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0006173","snapshot_observed_at":"2026-08-08T11:30:50.005603Z","title":"Leptogenesis from Neutralino Decay with Nonholomorphic R-Parity Violation","venue":"hep-ph","work_id":"462e92cd-7d6d-4360-9a6a-8c4791e67075","year":2000},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.921734Z"},"links":{"cited_paper":"/paper/hep-ph/0006173","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:4376b8ab0a30783c168cdc311cb20bea3c4bac4770117d5484691b954eb98baa","observation_id":"fd81a7fa-4e76-43d5-b731-32903c53e5cb","resolution":{"observed_at":"2026-08-08T11:30:50.010778Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0111089","last_updated":"2002-04-16T11:01:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2001-11-08T18:17:08Z","title":"Leptogenesis at the TeV scale","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0111089","snapshot_observed_at":"2026-08-08T11:30:48.926853Z","title":"Hambye,Leptogenesis at the TeV scale, Nucl","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.926853Z"},"links":{"cited_paper":"/paper/hep-ph/0111089","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:13319d24e2869895e5f2719ee14e24314c8176e9aea62288498761c70915b72b","observation_id":"418a2f48-420b-4113-ab2b-06b37f823d89","resolution":{"observed_at":"2026-08-08T11:30:48.926853Z","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":"2026-08-08T11:30:50.715612Z","title":"Moroi,Effects of the gravitino on the inflationary universe, other thesis, 3, 1995","venue":null,"work_id":"60838ed8-1a00-4eb1-8d3e-f2dbf97c3321","year":1995},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.931967Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:39207d7115302cc44f48889e4c03900f3b4704b2b03031aec5a40fa916794539","observation_id":"5686cbb8-0839-43e5-979f-5437f08906ad","resolution":{"observed_at":"2026-08-08T11:30:50.720894Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.699601Z","title":null,"venue":null,"work_id":"120845fd-b423-4a52-bc78-e319ae2ff28f","year":1988},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.936716Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:7bfbcae691f3a202fdb28da6413d6c40c5011dfdc6b44b5100629fb651c387d8","observation_id":"e012e488-7d68-4a65-a233-49d049a7df0d","resolution":{"observed_at":"2026-08-08T11:30:50.704688Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.683174Z","title":null,"venue":null,"work_id":"88a3a69a-e0bf-48da-8ba9-52ed5b70a1ac","year":1990},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.941773Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:a0f9c8952f1fa376adf7d847ffda868d1eee0b750de25b5c565becbd2ccfd23e","observation_id":"a8650329-57a0-475f-8fc0-2794deac05c7","resolution":{"observed_at":"2026-08-08T11:30:50.688334Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0005136","last_updated":"2000-08-15T10:17:45Z","snapshot_observed_at":"2026-07-07T03:48:32.282227Z","submitted_at":"2000-05-15T09:41:17Z","title":"Cosmological Gravitino Problem in Gauge-Mediated Supersymmetry Breaking Models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0005136","snapshot_observed_at":"2026-08-08T11:30:48.946993Z","title":"Asaka, K","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.946993Z"},"links":{"cited_paper":"/paper/hep-ph/0005136","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:b6959865e22a6814768517a791bcc1c8ac0c91c67df78921d0d2b6eebaa612e6","observation_id":"3bb34622-1a9a-47a5-98a1-931477491fc0","resolution":{"observed_at":"2026-08-08T11:30:48.946993Z","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":"2026-08-08T11:30:50.664080Z","title":"Fayet,Supergauge Invariant Extension of the Higgs Mechanism and a Model for the electron and Its Neutrino, Nucl","venue":null,"work_id":"07eb22df-7b07-40ba-80a0-d61102258864","year":1975},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.952548Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:12142b383f2317a48fa691028475e33172b14115e0a57323e2169f61d90e3321","observation_id":"f61f69d3-e20b-48f0-981e-c2699039b6e9","resolution":{"observed_at":"2026-08-08T11:30:50.670631Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.645866Z","title":null,"venue":null,"work_id":"7406e54d-5018-432d-92bc-b6d7f269a413","year":1991},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.957973Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:18a70af7fa150df3c90943bc6f99575c01ebd0ae7e241a0640d014c3e4a4947b","observation_id":"c9125e4c-a0c9-4bb3-ace5-01a928d4252d","resolution":{"observed_at":"2026-08-08T11:30:50.651518Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.629554Z","title":"Randall and N","venue":null,"work_id":"aa97eb3f-2bb7-47ba-a000-7ec538c35170","year":1992},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.963027Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:12a42c210f4bd8f45fb71adf20f2baf7615db7e89085a141d5712f85728d2619","observation_id":"d7aa56dc-d284-473d-bd17-a3e946c324e9","resolution":{"observed_at":"2026-08-08T11:30:50.634869Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0206102","last_updated":"2002-06-27T18:22:21Z","snapshot_observed_at":"2026-08-08T15:46:40.395284Z","submitted_at":"2002-06-11T18:54:52Z","title":"The Minimal Supersymmetric Model without a mu term","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0206102","snapshot_observed_at":"2026-08-08T11:30:48.968159Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.968159Z"},"links":{"cited_paper":"/paper/hep-ph/0206102","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:f5d6062e8ff3a142a08d9a104d0fc05336160cdfba37af9dc5c60b75779ad37e","observation_id":"26c980b2-86c4-461c-a9e8-9bc2d4c92f4a","resolution":{"observed_at":"2026-08-08T11:30:48.968159Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0206096","last_updated":"2006-10-21T03:03:18Z","snapshot_observed_at":"2026-07-07T03:56:23.289831Z","submitted_at":"2002-06-11T18:17:39Z","title":"Dirac Gaugino Masses and Supersoft Supersymmetry Breaking","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0206096","snapshot_observed_at":"2026-08-08T11:30:48.973527Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.973527Z"},"links":{"cited_paper":"/paper/hep-ph/0206096","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:ff925c37f97231d4fd16674249b8be48c4d7f1102c25434dae5c36597c29df26","observation_id":"58a1d0df-644d-4a0f-b826-b358d42c2da0","resolution":{"observed_at":"2026-08-08T11:30:48.973527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.6323","last_updated":"2013-12-04T11:05:21Z","snapshot_observed_at":"2026-08-09T09:09:57.552164Z","submitted_at":"2013-06-26T19:40:05Z","title":"Mapping Dirac gaugino masses","version":3},"cited_work":{"arxiv_id":"1306.6323","doi":null,"metadata_source":"pith","pith_arxiv_id":"1306.6323","snapshot_observed_at":"2026-08-08T11:30:49.913440Z","title":"Mapping Dirac gaugino masses","venue":"hep-th","work_id":"63d8b46a-7836-498a-af7f-24c7b91d7c37","year":2013},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.978577Z"},"links":{"cited_paper":"/paper/1306.6323","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:f64f1fc648df00577cc0cc4ba3df0e1266def1ec71b6538bad5005fabdb2405c","observation_id":"bf7ce1a0-34be-4840-ae4d-632ae9012fee","resolution":{"observed_at":"2026-08-08T11:30:49.918599Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.4791","last_updated":"2014-12-23T15:11:21Z","snapshot_observed_at":"2026-07-06T03:57:44.420626Z","submitted_at":"2014-10-17T16:42:09Z","title":"Higgs boson mass and electroweak observables in the MRSSM","version":2},"cited_work":{"arxiv_id":"1410.4791","doi":null,"metadata_source":"pith","pith_arxiv_id":"1410.4791","snapshot_observed_at":"2026-08-08T11:30:49.889737Z","title":"Higgs boson mass and electroweak observables in the MRSSM","venue":"hep-ph","work_id":"2ff77aba-56f3-4711-8bfd-36301166b783","year":2014},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.984222Z"},"links":{"cited_paper":"/paper/1410.4791","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:296f486195afba41b251fc952522513cdaacddfdbd4598c2494835c51e03f4a6","observation_id":"57b84193-4b80-48a4-a390-b64c7b5c8ef2","resolution":{"observed_at":"2026-08-08T11:30:49.895878Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.614206Z","title":"Abel and M","venue":null,"work_id":"0f840edd-33e1-4e90-90a5-622f24cd30a8","year":2011},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.989332Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:1734c9c8e7d1a034f650a757daa8c10bda0e7c4ced069afb8f5cdda0257afe23","observation_id":"edef0a13-4d0e-47c6-8b0e-8b8a725e6a1e","resolution":{"observed_at":"2026-08-08T11:30:50.619068Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.598686Z","title":"Benakli,Dirac gauginos: a user manual, Fortschritte der Physik59 (2011), no","venue":null,"work_id":"4ec63439-e104-4175-bafc-bd6317433e36","year":2011},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:48.994791Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:c72b59c118c11b6479b6961d24caa1041f47527fe3026ca58af04dda0442c92e","observation_id":"17e09129-789f-4944-adaa-e63fd295539f","resolution":{"observed_at":"2026-08-08T11:30:50.603703Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.582304Z","title":"Benakli, M","venue":null,"work_id":"b9232098-d357-46ad-ba57-682799d0c3a2","year":2013},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.000115Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:25094bd148abf89a05a6083c94745d3cd9fe1dede663a9305e6d8469166d4a9f","observation_id":"38b01599-be42-4c73-b5bf-4462c1787008","resolution":{"observed_at":"2026-08-08T11:30:50.587855Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.565357Z","title":"Benakli,A framework for unified dirac gauginos, inEPJ Web of Conferences, vol","venue":null,"work_id":"24fdfcf2-56db-4775-a2b1-3b200bfc19fa","year":2017},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.006090Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:c27780c6e47995cd186dc5b3d1de85b3548df4ae132674ade5d5628c77357871","observation_id":"349090ce-6514-438f-a9c3-8579e5efc5aa","resolution":{"observed_at":"2026-08-08T11:30:50.570794Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0610249","last_updated":"2006-10-19T14:33:17Z","snapshot_observed_at":"2026-07-07T04:12:36.996696Z","submitted_at":"2006-10-19T14:33:17Z","title":"Non-perturbative Effect on Thermal Relic Abundance of Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0610249","snapshot_observed_at":"2026-08-08T11:30:49.011507Z","title":"Hisano, S","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.011507Z"},"links":{"cited_paper":"/paper/hep-ph/0610249","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:3bd860701a437efab1eea5567cc7f276079695fa09b8d78010c1acf9067a0236","observation_id":"e81a4492-03e3-4c28-8ba4-2121001586eb","resolution":{"observed_at":"2026-08-08T11:30:49.011507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0404198","last_updated":"2004-09-22T21:28:50Z","snapshot_observed_at":"2026-07-07T04:03:27.435650Z","submitted_at":"2004-04-23T18:58:41Z","title":"SuperWIMP Gravitino Dark Matter from Slepton and Sneutrino Decays","version":2},"cited_work":{"arxiv_id":"hep-ph/0404198","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0404198","snapshot_observed_at":"2026-08-08T11:30:49.847722Z","title":"SuperWIMP Gravitino Dark Matter from Slepton and Sneutrino Decays","venue":"hep-ph","work_id":"fa3d7aca-835c-4aab-a5a0-f16ab3603b0a","year":2004},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.016488Z"},"links":{"cited_paper":"/paper/hep-ph/0404198","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:821c27a6fd7c2b217c1bc89eee4a37e1564259639c68b49c133a3165e852d214","observation_id":"5b116cfe-4ee1-49a7-b457-3fb25354df49","resolution":{"observed_at":"2026-08-08T11:30:49.853584Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1002.0340","last_updated":"2010-04-07T13:14:27Z","snapshot_observed_at":"2026-07-06T02:05:57.735088Z","submitted_at":"2010-02-02T16:27:10Z","title":"The degenerate gravitino scenario","version":2},"cited_work":{"arxiv_id":"1002.0340","doi":null,"metadata_source":"pith","pith_arxiv_id":"1002.0340","snapshot_observed_at":"2026-08-08T11:30:49.823527Z","title":"The degenerate gravitino scenario","venue":"hep-ph","work_id":"156c5500-7d77-4157-b98a-d8aabbf8d112","year":2010},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.021928Z"},"links":{"cited_paper":"/paper/1002.0340","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:b42c2c99e567ee00d08899e4313ac4c581f17226c165f648e2e8ef2a5b10be3f","observation_id":"ee20f7c8-9dfc-484a-822b-00ba5aa94805","resolution":{"observed_at":"2026-08-08T11:30:49.828576Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0402490","last_updated":"2004-06-17T05:37:01Z","snapshot_observed_at":"2026-07-07T00:40:38.849273Z","submitted_at":"2004-02-20T14:18:40Z","title":"Hadronic Decay of Late-Decaying Particles and Big-Bang Nucleosynthesis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0402490","snapshot_observed_at":"2026-08-08T11:30:49.027058Z","title":"Kawasaki, K","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.027058Z"},"links":{"cited_paper":"/paper/astro-ph/0402490","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:e0a4360e8fa4ed1d7e6a7d7cc24b7ef727cc5c5c8d3138cd07892b51fb408ba2","observation_id":"b44d147d-782c-4f00-ba22-c84ffb69cad1","resolution":{"observed_at":"2026-08-08T11:30:49.027058Z","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":"2026-08-08T11:30:50.548639Z","title":"Porod,Spheno, a program for calculating supersymmetric spectra, susy particle decays and susy particle production at e+ e- colliders, Computer Physics Communications 153 (2003), no","venue":null,"work_id":"59293a26-6d4c-48cc-a835-d317359d2836","year":2003},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.032180Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:9f69a3448e7d066d6b4feadb8985c2d5704d0f5679881760e582625bc358941f","observation_id":"c67608b3-129d-47bb-9497-c920646a7717","resolution":{"observed_at":"2026-08-08T11:30:50.554107Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.531875Z","title":"Porod and F","venue":null,"work_id":"e33fbc6e-607b-431d-a8a1-5e42386d5b0a","year":2012},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.036918Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:d97ff9e0d1d87fe48db165b22be86b4146b9e7ae3ba8d0de0ef3ee0c10ea9d62","observation_id":"ac1cfadf-1bfa-49ce-988b-d56fa6461404","resolution":{"observed_at":"2026-08-08T11:30:50.537131Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9606211","last_updated":"1997-02-07T02:01:07Z","snapshot_observed_at":"2026-07-07T04:22:49.406873Z","submitted_at":"1996-06-04T00:19:16Z","title":"Precision Corrections in the Minimal Supersymmetric Standard Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9606211","snapshot_observed_at":"2026-08-08T11:30:49.042253Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.042253Z"},"links":{"cited_paper":"/paper/hep-ph/9606211","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:12f7603d8ddef1b1b3a9a494b2a1cc962621c4eafface263b9e73bba2ecc817a","observation_id":"20ce59b0-3e27-4685-bdf4-0922fd7458e5","resolution":{"observed_at":"2026-08-08T11:30:49.042253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0105096","last_updated":"2001-05-24T10:49:07Z","snapshot_observed_at":"2026-07-07T03:52:20.795503Z","submitted_at":"2001-05-10T21:47:34Z","title":"On the neutral Higgs boson masses in the MSSM for arbitrary stop mixing","version":2},"cited_work":{"arxiv_id":"hep-ph/0105096","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0105096","snapshot_observed_at":"2026-08-08T11:30:49.763832Z","title":"On the neutral Higgs boson masses in the MSSM for arbitrary stop mixing","venue":"hep-ph","work_id":"0fdfe7be-b90e-4602-9c50-76356deb0357","year":2001},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.047386Z"},"links":{"cited_paper":"/paper/hep-ph/0105096","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:78fdb75f9f3f809144d0facbbe743996e5e32fc82479c71d7f648cbe5b6d63a8","observation_id":"dd8ec5c7-aa7e-44a1-8ab9-4fde69317a1f","resolution":{"observed_at":"2026-08-08T11:30:49.769202Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0112177","last_updated":"2002-04-08T18:05:17Z","snapshot_observed_at":"2026-07-07T03:54:38.864648Z","submitted_at":"2001-12-13T18:43:52Z","title":"On the O(alpha_t^2) two-loop corrections to the neutral Higgs boson masses in the MSSM","version":2},"cited_work":{"arxiv_id":"hep-ph/0112177","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0112177","snapshot_observed_at":"2026-08-08T11:30:49.740034Z","title":"On the O(alpha_t^2) two-loop corrections to the neutral Higgs boson masses in the MSSM","venue":"hep-ph","work_id":"1fd72b87-6a10-4af9-b149-406ba6d9982d","year":2001},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.053612Z"},"links":{"cited_paper":"/paper/hep-ph/0112177","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:5a2c8d71657ce6a18a6dc71be494177af0d01445929765075159e26ef102ad1d","observation_id":"883263c4-7bae-4e93-9321-36df16acecb5","resolution":{"observed_at":"2026-08-08T11:30:49.745689Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0206101","last_updated":"2002-09-10T12:18:33Z","snapshot_observed_at":"2026-07-07T03:56:23.289831Z","submitted_at":"2002-06-11T18:49:56Z","title":"On the two-loop sbottom corrections to the neutral Higgs boson masses in the MSSM","version":2},"cited_work":{"arxiv_id":"hep-ph/0206101","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0206101","snapshot_observed_at":"2026-08-08T11:30:49.717342Z","title":"On the two-loop sbottom corrections to the neutral Higgs boson masses in the MSSM","venue":"hep-ph","work_id":"9d71ba78-a1c9-4cab-bf33-3fcd5c976ae0","year":2002},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.058950Z"},"links":{"cited_paper":"/paper/hep-ph/0206101","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:480aae7efd4071baa3ebb90a2bf6b5a01c707f1567816940d9e6ef53813792f3","observation_id":"84aa5b63-f8ae-4d3c-9784-c8c31a7cdc29","resolution":{"observed_at":"2026-08-08T11:30:49.722708Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0212132","last_updated":"2003-03-14T15:22:38Z","snapshot_observed_at":"2026-07-07T03:58:30.344772Z","submitted_at":"2002-12-09T23:53:18Z","title":"Two-loop corrections to Radiative Electroweak Symmetry Breaking in the MSSM","version":2},"cited_work":{"arxiv_id":"hep-ph/0212132","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0212132","snapshot_observed_at":"2026-08-08T11:30:49.694122Z","title":"Two-loop corrections to Radiative Electroweak Symmetry Breaking in the MSSM","venue":"hep-ph","work_id":"554d0152-7953-4bcf-a709-91deeb055ef8","year":2002},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.064010Z"},"links":{"cited_paper":"/paper/hep-ph/0212132","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:9fca1c23f0d4f8fc72bbd574600d152c4b6358af1d4c9684790ebea92ac7c66b","observation_id":"e4c1c26d-df1c-405e-ae63-1f54c8abaf50","resolution":{"observed_at":"2026-08-08T11:30:49.699944Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0305127","last_updated":"2003-10-03T14:10:34Z","snapshot_observed_at":"2026-08-07T14:44:58.628863Z","submitted_at":"2003-05-12T18:00:23Z","title":"On the two-loop Yukawa corrections to the MSSM Higgs boson masses at large tan(beta)","version":3},"cited_work":{"arxiv_id":"hep-ph/0305127","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0305127","snapshot_observed_at":"2026-08-08T11:30:49.669441Z","title":"On the two-loop Yukawa corrections to the MSSM Higgs boson masses at large tan(beta)","venue":"hep-ph","work_id":"5884893e-2edf-4a01-aa93-5b128410508a","year":2003},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.069426Z"},"links":{"cited_paper":"/paper/hep-ph/0305127","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:2a681a0fb4ba1ab61a6d7c2f8d6bc902684a45775be571486c4b79c052aaf77a","observation_id":"5de9f369-d975-4b49-8109-99877d470625","resolution":{"observed_at":"2026-08-08T11:30:49.675558Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.515757Z","title":"Staub,Sarah, 2012","venue":null,"work_id":"60bbb54c-aa42-416d-85fc-573b1fa08d22","year":2012},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.074541Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:6cd61e92cad5d783476f8e1a73560aada73712d787170b5d9cba13c1266c8a7d","observation_id":"365c14c4-87e4-4d5d-afe9-030e0f8d37c0","resolution":{"observed_at":"2026-08-08T11:30:50.520805Z","resolver_source":"raw_fallback","status":"parse_uncertain"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.497179Z","title":"Staub,Sarah 4: A tool for (not only susy) model builders, Computer Physics Communications 185 (June, 2014) 1773–1790","venue":null,"work_id":"acb623c0-56ac-45d0-90f5-b9ab295badd1","year":2014},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.079487Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:657437985c781ae23ac1f22e4e64c34c88bf08615965f00622cdb37eaafcaf2d","observation_id":"ec719f56-927a-4579-be04-30538c0e309e","resolution":{"observed_at":"2026-08-08T11:30:50.503159Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.477705Z","title":null,"venue":null,"work_id":"dd3b11ff-9501-4048-92ed-f9770d7df4b2","year":2023},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.084528Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:a9940fe175e91866aa166f48f910b5f082336cce6d9a7dfa08947704d677ffd2","observation_id":"711fa387-c2af-45c9-b768-489ffbe013f4","resolution":{"observed_at":"2026-08-08T11:30:50.483845Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.459992Z","title":"Kotlarski,Analysis of the r-symmetric supersymmetric models including quantum corrections, 2016","venue":null,"work_id":"a9597ff7-6152-4924-a46a-bd26471798bd","year":2016},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.089977Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:306ee874c505cf4c7c2facbdedbf6b2bf3c8671e7e71f7485bfeb2bb9f8e8f2d","observation_id":"6f1f4e0c-eeaa-4573-93d8-c14e6bc3aae8","resolution":{"observed_at":"2026-08-08T11:30:50.465562Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.443729Z","title":null,"venue":null,"work_id":"9c2c0b9b-564e-48ca-86ce-68ca0cc7099d","year":1983},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.095309Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:acc632f60172b662627510e75b5c5fda113ca0fe1d91bfe8e45fae7d398f57a4","observation_id":"db17b67a-a5ef-475a-8d28-551f3e89ce68","resolution":{"observed_at":"2026-08-08T11:30:50.448897Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.425337Z","title":"Alvarez-Gaume, J","venue":null,"work_id":"a76463d5-ccda-4397-a87e-04148cc06cc3","year":1983},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.100198Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:ac7e896b33eb52f8cfa9436e3f687409eacda3239d00e90fa3ee25ebe6afe5c4","observation_id":"4413196e-07af-4bd3-9efa-b4ca575a81aa","resolution":{"observed_at":"2026-08-08T11:30:50.430926Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.407488Z","title":"Claudson, L","venue":null,"work_id":"386acaf5-b3de-44a9-b094-5cb003c5c50b","year":1983},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.105039Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:a5669874d7efc7ce3f4433cabe3a8acf673a49bbb5f998bbca94b4d780118a73","observation_id":"c51708a3-5c47-445a-b0ff-49676b8f5c1e","resolution":{"observed_at":"2026-08-08T11:30:50.412587Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.391261Z","title":null,"venue":null,"work_id":"3fae2031-75c8-49e3-bb58-4c4896ba28e0","year":1988},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.110080Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:7a9043bb164a54f59ec79857a8e06f1658c4e2489d5fa537610aaa86e4f4542b","observation_id":"642d5ea8-1d4f-4243-b104-818c2d52992f","resolution":{"observed_at":"2026-08-08T11:30:50.396176Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9507294","last_updated":"1995-07-27T12:04:05Z","snapshot_observed_at":"2026-07-07T04:20:23.387060Z","submitted_at":"1995-07-12T17:42:41Z","title":"Strong Constraints on the Parameter Space of the MSSM from Charge and Color Breaking Minima","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9507294","snapshot_observed_at":"2026-08-08T11:30:49.114699Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.114699Z"},"links":{"cited_paper":"/paper/hep-ph/9507294","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:9e11ad1ddbeb92088a7bdcba08c4ae41137f830f26d0bdbb7fdf81990d8fc7c3","observation_id":"ce924454-1ce2-468e-8a07-b165c10e723e","resolution":{"observed_at":"2026-08-08T11:30:49.114699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.7376","last_updated":"2014-09-01T14:38:51Z","snapshot_observed_at":"2026-07-06T03:44:56.585883Z","submitted_at":"2014-05-28T20:00:31Z","title":"Constraining the Natural MSSM through tunneling to color-breaking vacua at zero and non-zero temperature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.7376","snapshot_observed_at":"2026-08-08T11:30:49.119936Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.119936Z"},"links":{"cited_paper":"/paper/1405.7376","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:a89668bf36930261a294280f1b290db725cc7a757edb295e46e6feb20b288d9e","observation_id":"70be1c98-bd87-4b82-b614-cd628950545d","resolution":{"observed_at":"2026-08-08T11:30:49.119936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.02332","last_updated":"2018-06-26T11:03:38Z","snapshot_observed_at":"2026-08-05T06:53:17.746799Z","submitted_at":"2017-12-06T18:55:54Z","title":"Search for squarks and gluinos in final states with jets and missing transverse momentum using 36 fb$^{-1}$ of $\\sqrt{s}$=13 TeV $pp$ collision data with the ATLAS detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.02332","snapshot_observed_at":"2026-08-08T11:30:49.125318Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.125318Z"},"links":{"cited_paper":"/paper/1712.02332","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:f98394a29d901171770efefeb7033852cbe99e62880e82c355d5df66c0579dd0","observation_id":"9625409b-25f3-437f-878d-1caea825c388","resolution":{"observed_at":"2026-08-08T11:30:49.125318Z","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":"2026-08-08T11:30:50.375707Z","title":"Chalons, M","venue":null,"work_id":"ea37c17f-0bf7-4dfc-bc41-6067972d0227","year":2019},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.130693Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:0699835a0394f7fdd1807db26aa1b228dc6a46def5f3c5fac6e3ddfcc6c61e67","observation_id":"bc23aeb0-c9e6-46fd-9ff6-8ebe39274a8f","resolution":{"observed_at":"2026-08-08T11:30:50.380571Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1606.07090","last_updated":"2016-06-22T20:17:56Z","snapshot_observed_at":"2026-07-06T05:00:59.523166Z","submitted_at":"2016-06-22T20:17:56Z","title":"Dirac vs Majorana gauginos at a 100 TeV collider","version":1},"cited_work":{"arxiv_id":"1606.07090","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.07090","snapshot_observed_at":"2026-08-08T11:30:49.592533Z","title":"Dirac vs Majorana gauginos at a 100 TeV collider","venue":"hep-ph","work_id":"6a1e9596-a43a-4661-b6bf-8a089285a232","year":2016},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.135745Z"},"links":{"cited_paper":"/paper/1606.07090","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:c14cdb0d6d28ec5a000636152129abf4ac09ca1ae7d815f5caae245af22d5c98","observation_id":"8f0eb7fb-98da-4326-aa2c-bfb49b654790","resolution":{"observed_at":"2026-08-08T11:30:49.598125Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08498","last_updated":"2020-08-31T16:54:39Z","snapshot_observed_at":"2026-08-09T07:26:48.794809Z","submitted_at":"2020-07-16T17:50:33Z","title":"Constraining Electroweakinos in the Minimal Dirac Gaugino Model","version":2},"cited_work":{"arxiv_id":"2007.08498","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.08498","snapshot_observed_at":"2026-08-08T11:30:49.566343Z","title":"Constraining Electroweakinos in the Minimal Dirac Gaugino Model","venue":"hep-ph","work_id":"9e0ceca4-b19e-44e8-88e0-f0beea0d5f82","year":2020},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.140617Z"},"links":{"cited_paper":"/paper/2007.08498","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:7937a02b695c5cfd56245f1fd4a0125312432369a81f54293a3aeb93ed09c5da","observation_id":"36a2841e-ea95-40e7-bc1a-bd0459448488","resolution":{"observed_at":"2026-08-08T11:30:49.573501Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.02795","last_updated":"2022-01-31T19:16:57Z","snapshot_observed_at":"2026-08-05T21:30:01.803379Z","submitted_at":"2021-08-05T18:00:57Z","title":"Exploring the phenomenology of weak adjoint scalars in minimal $R$-symmetric models","version":3},"cited_work":{"arxiv_id":"2108.02795","doi":null,"metadata_source":"pith","pith_arxiv_id":"2108.02795","snapshot_observed_at":"2026-08-08T11:30:49.541420Z","title":"Exploring the phenomenology of weak adjoint scalars in minimal $R$-symmetric models","venue":"hep-ph","work_id":"9ff0a79c-6004-4115-b271-4eaeadef7149","year":2021},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.146167Z"},"links":{"cited_paper":"/paper/2108.02795","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:3eda98f8faab10d25b9c374f47524b004fec32bd566ba8f250a53bae452dd3ca","observation_id":"d069fdf3-8b35-489d-8ba4-ac222bb601f2","resolution":{"observed_at":"2026-08-08T11:30:49.547376Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1505.02996","last_updated":"2016-02-14T08:18:11Z","snapshot_observed_at":"2026-07-06T04:17:37.737618Z","submitted_at":"2015-05-12T13:19:29Z","title":"Long-Lived Sleptons at the LHC and a 100 TeV Proton Collider","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.02996","snapshot_observed_at":"2026-08-08T11:30:49.151471Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.151471Z"},"links":{"cited_paper":"/paper/1505.02996","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:a964e13a6044b81ee84c1ea2e15eff3d2af1e5bd39ae2ebb76a4c7f3d4651fdc","observation_id":"827117ed-69d4-46a4-bedc-95d77faa79a1","resolution":{"observed_at":"2026-08-08T11:30:49.151471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.02118","last_updated":"2018-06-19T14:41:13Z","snapshot_observed_at":"2026-07-06T06:13:02.537882Z","submitted_at":"2017-12-06T10:29:28Z","title":"Search for long-lived charginos based on a disappearing-track signature in $pp$ collisions at $\\sqrt{s} = 13$ TeV with the ATLAS detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.02118","snapshot_observed_at":"2026-08-08T11:30:49.156888Z","title":"Aaboud et al.,Search for long-lived charginos based on a disappearing-track signature in pp collisions at√s = 13 TeV with the ATLAS detector, JHEP 06 (2018) 022, [arXiv:1712.02118]","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.156888Z"},"links":{"cited_paper":"/paper/1712.02118","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:f5a331bbe2744f7ea5ff5c786d24886760840d9745534d3a016ae10bd85d5c0a","observation_id":"b289d9e8-5c52-4021-8423-ab066ed507d3","resolution":{"observed_at":"2026-08-08T11:30:49.156888Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.02472","last_updated":"2022-07-26T22:16:03Z","snapshot_observed_at":"2026-08-09T10:18:11.155024Z","submitted_at":"2022-01-07T14:44:10Z","title":"Search for long-lived charginos based on a disappearing-track signature using 136 fb$^{-1}$ of $pp$ collisions at $\\sqrt{s}$ = 13 TeV with the ATLAS detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.02472","snapshot_observed_at":"2026-08-08T11:30:49.162395Z","title":"Aad et al.,Search for long-lived charginos based on a disappearing-track signature using 136 fb−1 of pp collisions at√s = 13 TeV with the ATLAS detector, Eur","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.162395Z"},"links":{"cited_paper":"/paper/2201.02472","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:8bf79972e283511218f497740b9c773ea94cd507a70a6872f4e41ed4a8ddefb7","observation_id":"63fe2268-ce0d-4e27-b842-4bbc11e13398","resolution":{"observed_at":"2026-08-08T11:30:49.162395Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.07321","last_updated":"2018-08-13T23:10:45Z","snapshot_observed_at":"2026-08-05T08:23:52.225453Z","submitted_at":"2018-04-19T18:15:31Z","title":"Search for disappearing tracks as a signature of new long-lived particles in proton-proton collisions at $\\sqrt{s} =$ 13 TeV","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.07321","snapshot_observed_at":"2026-08-08T11:30:49.167848Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.167848Z"},"links":{"cited_paper":"/paper/1804.07321","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:020b615779eda8f9fc325356bfbe607bf8c02f327e95131624d71919f41e1163","observation_id":"8bc2debf-62c5-4494-b5fd-af01087b2a3f","resolution":{"observed_at":"2026-08-08T11:30:49.167848Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.05153","last_updated":"2020-06-08T20:14:59Z","snapshot_observed_at":"2026-08-03T10:03:26.480709Z","submitted_at":"2020-04-10T17:56:41Z","title":"Search for disappearing tracks in proton-proton collisions at $\\sqrt{s} =$ 13 TeV","version":2},"cited_work":{"arxiv_id":"2004.05153","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.05153","snapshot_observed_at":"2026-08-08T11:30:49.445667Z","title":"Search for disappearing tracks in proton-proton collisions at $\\sqrt{s} =$ 13 TeV","venue":"hep-ex","work_id":"08e2a219-cb4c-40a4-b429-53e0f19e0526","year":2020},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.173559Z"},"links":{"cited_paper":"/paper/2004.05153","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:f1b0a2f5c85055cd08bdda1f861e1e2edfad6d43727f2f70ed5c83b65690a2da","observation_id":"7f4980f6-f286-4206-8f62-ea54c62189e4","resolution":{"observed_at":"2026-08-08T11:30:49.451348Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2106.08815","last_updated":"2021-06-16T14:27:16Z","snapshot_observed_at":"2026-08-04T07:45:34.279636Z","submitted_at":"2021-06-16T14:27:16Z","title":"Long Dead Winos","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.08815","snapshot_observed_at":"2026-08-08T11:30:49.179023Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.179023Z"},"links":{"cited_paper":"/paper/2106.08815","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:c9ade0d05bcc9a5229c47f9c6ef55480d2f4c3e9a55130c5fac130e2bc5dc557","observation_id":"0f75fe93-ef94-487c-8215-a60bc5620f46","resolution":{"observed_at":"2026-08-08T11:30:49.179023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.7662","last_updated":"2014-08-28T19:16:01Z","snapshot_observed_at":"2026-07-06T03:45:01.662746Z","submitted_at":"2014-05-29T19:16:21Z","title":"The Physics Programme Of The MoEDAL Experiment At The LHC","version":4},"cited_work":{"arxiv_id":"1405.7662","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.7662","snapshot_observed_at":"2026-08-08T11:30:49.403714Z","title":"The Physics Programme Of The MoEDAL Experiment At The LHC","venue":"hep-ph","work_id":"bf1b0331-3836-4e2b-91c4-eee87a246075","year":2014},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.184956Z"},"links":{"cited_paper":"/paper/1405.7662","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:dbbcbc5a4130eccb3f45be2e075958d1047371dac585dc53457148fea4b9da5d","observation_id":"7252e7e2-eb58-49be-a727-9eb7ded41952","resolution":{"observed_at":"2026-08-08T11:30:49.409061Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+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":"2026-08-08T11:30:50.359502Z","title":null,"venue":null,"work_id":"601feaa5-3ab3-4c6c-9ca8-12e8301bba94","year":2019},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.190163Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:3acffd288fb42c188ffaa96b825fc9a40073f390aa116775a7d7759db032a120","observation_id":"eda0be04-b02d-4085-bb56-53a4c1280e38","resolution":{"observed_at":"2026-08-08T11:30:50.364844Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.00481","last_updated":"2021-01-07T17:47:10Z","snapshot_observed_at":"2026-07-06T08:34:07.664147Z","submitted_at":"2019-11-01T17:46:24Z","title":"Expression of Interest for the CODEX-b Detector","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.00481","snapshot_observed_at":"2026-08-08T11:30:49.195328Z","title":"Aielli et al.,Expression of interest for the CODEX-b detector, Eur","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.195328Z"},"links":{"cited_paper":"/paper/1911.00481","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:f44ac3a3f781346e9a0c760a230b108241b2890472e7805169f8eb05f4e31b98","observation_id":"0d821c74-c89c-49a6-991a-2280f89e96f0","resolution":{"observed_at":"2026-08-08T11:30:49.195328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.07396","last_updated":"2019-03-05T16:17:41Z","snapshot_observed_at":"2026-07-06T06:45:40.133221Z","submitted_at":"2018-06-19T18:00:04Z","title":"Long-Lived Particles at the Energy Frontier: The MATHUSLA Physics Case","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.07396","snapshot_observed_at":"2026-08-08T11:30:49.200879Z","title":"Curtin et al.,Long-Lived Particles at the Energy Frontier: The MATHUSLA Physics Case, Rept","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.200879Z"},"links":{"cited_paper":"/paper/1806.07396","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:2b9736b8c9ee02c9f51dab87aed429d1e8ca6ce0b674afcecb5bacebb002ce36","observation_id":"30cec334-67fc-42e1-8380-6e0e129700e7","resolution":{"observed_at":"2026-08-08T11:30:49.200879Z","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":"2026-08-08T11:30:50.343276Z","title":"Bertolini, F","venue":null,"work_id":"74b35cad-54f7-4117-bd42-a090fb6bba3a","year":1987},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.206216Z"},"links":{"citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:4a03b330007a1b86acd9ab713a7c935df0c0229acb2dbe8ed5dde438579cf59d","observation_id":"be92eff9-2709-4943-a114-3b5971b6418a","resolution":{"observed_at":"2026-08-08T11:30:50.348226Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9512396","last_updated":"1997-06-26T17:44:54Z","snapshot_observed_at":"2026-07-07T04:21:39.561201Z","submitted_at":"1995-12-21T19:58:30Z","title":"The Muon Anomalous Magnetic Dipole Moment in the Minimal Supersymmetric Standard Model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9512396","snapshot_observed_at":"2026-08-08T11:30:49.211373Z","title":"Moroi,The Muon anomalous magnetic dipole moment in the minimal supersymmetric standard model, Phys","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.211373Z"},"links":{"cited_paper":"/paper/hep-ph/9512396","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:d4f10c26888ad9372cfab45a376f30d17053f55e7402f87b960da102fd3e416e","observation_id":"b974160e-c1a6-40a3-8976-c4f6902e85cd","resolution":{"observed_at":"2026-08-08T11:30:49.211373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0103067","last_updated":"2001-03-06T23:50:21Z","snapshot_observed_at":"2026-07-07T03:51:41.576227Z","submitted_at":"2001-03-06T23:50:21Z","title":"Muon anomalous magnetic dipole moment in supersymmetric theories","version":1},"cited_work":{"arxiv_id":"hep-ph/0103067","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0103067","snapshot_observed_at":"2026-08-08T11:30:49.324064Z","title":"Muon anomalous magnetic dipole moment in supersymmetric theories","venue":"hep-ph","work_id":"09f05dd1-c3d9-4b4d-b481-f3a93ffc3f15","year":2001},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.216383Z"},"links":{"cited_paper":"/paper/hep-ph/0103067","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:7cd70d57d89157a3d32d1a552dde5681d4eafeed287bc9ec21746d307c906725","observation_id":"52c138a4-3f55-445e-b30a-b007529c4177","resolution":{"observed_at":"2026-08-08T11:30:49.330115Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0103324","last_updated":"2001-04-10T17:28:19Z","snapshot_observed_at":"2026-07-07T03:51:56.176029Z","submitted_at":"2001-03-29T18:12:51Z","title":"General Flavor Blind MSSM and CP Violation","version":2},"cited_work":{"arxiv_id":"hep-ph/0103324","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0103324","snapshot_observed_at":"2026-08-08T11:30:49.299277Z","title":"General Flavor Blind MSSM and CP Violation","venue":"hep-ph","work_id":"5b46a8c7-2093-4d47-a18e-01520b9cc154","year":2001},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.221636Z"},"links":{"cited_paper":"/paper/hep-ph/0103324","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:e370c7af8ba8d668ec33a39623444ec65c3e4de7fc53c3f150b61b0b21ec18d8","observation_id":"fa243d61-4cde-4366-a963-0a938df0f6ee","resolution":{"observed_at":"2026-08-08T11:30:49.304765Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1504.05386","last_updated":"2015-04-21T11:05:13Z","snapshot_observed_at":"2026-07-06T04:15:34.255373Z","submitted_at":"2015-04-21T11:05:13Z","title":"Two-loop correction to the Higgs boson mass in the MRSSM","version":1},"cited_work":{"arxiv_id":"1504.05386","doi":null,"metadata_source":"pith","pith_arxiv_id":"1504.05386","snapshot_observed_at":"2026-08-08T11:30:49.271181Z","title":"Two-loop correction to the Higgs boson mass in the MRSSM","venue":"hep-ph","work_id":"635a94e5-8db5-4fcd-83e2-3b194ce3df8d","year":2015},"citing_paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-08T11:30:49.227031Z"},"links":{"cited_paper":"/paper/1504.05386","citing_paper":"/paper/2502.07932"},"observation_digest":"sha256:56d336334ff55c33699a13817acb25a84bcc5faf4505d27663c40b1344bb4304","observation_id":"35d3af14-ce57-46c4-bdc4-fbba8ecdacdb","resolution":{"observed_at":"2026-08-08T11:30:49.279752Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2502.07932","last_updated":"2025-02-11T20:19:17Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-08T11:20:56.834872Z","submitted_at":"2025-02-11T20:19:17Z","title":"Asymmetric Dark Matter in SUSY with approximate $R-$symmetry"},"reference_resolution":{"displayed":84,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":1,"unresolved":46,"verified_exact":20,"verified_fuzzy":16},"total_outbound_references":84},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 84 of 84 outbound references and 1 inbound Pith citation observation for arXiv:2502.07932."}