{"as_of":"2026-08-07T19:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9499035fde6d2628dbfaac1490457f49a6c6e7be6e93adc2f2f25e6fcced2f91","coverage":[{"denominator":47,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":47,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T12:53:30.108590Z","state":"measured"},{"denominator":47,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":47,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2507.21523/citation-record","integrity":"/paper/2507.21523/integrity","json":"/paper/2507.21523/citation-record.json","paper":"/paper/2507.21523"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T12:53:35.118379Z","title":"Cosmological problems for the Polonyi potential,","venue":null,"work_id":"1ef91f40-565e-4ebf-82a5-ea0ede920d7a","year":1983},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.025892Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:456363aed71121bd8bfcc39d7db8bfb1f081c5ea58391bc12ba863d20d974529","observation_id":"dea1224e-4a0e-45cb-8325-4b95b311e6fd","resolution":{"observed_at":"2026-08-06T12:53:35.260869Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9308325","last_updated":"1993-08-24T00:05:07Z","snapshot_observed_at":"2026-07-07T04:15:56.490202Z","submitted_at":"1993-08-24T00:05:07Z","title":"Model Independent Properties and Cosmological Implications of the Dilaton and Moduli Sectors of 4-d Strings","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9308325","snapshot_observed_at":"2026-08-06T12:53:26.108683Z","title":"Model independent properties and cosmological implications of the dilaton and moduli sectors of 4-d strings,","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.108683Z"},"links":{"cited_paper":"/paper/hep-ph/9308325","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:d2a1f114ca5d82aa372ee1c4c4aae87be391f239d7fa3d45defec3ce353de631","observation_id":"153311fe-d869-463e-971c-c052b19dfa63","resolution":{"observed_at":"2026-08-06T12:53:26.108683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.07746","last_updated":"2015-02-26T21:00:03Z","snapshot_observed_at":"2026-07-06T04:10:25.102131Z","submitted_at":"2015-02-26T21:00:03Z","title":"Cosmological Moduli and the Post-Inflationary Universe: A Critical Review","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.07746","snapshot_observed_at":"2026-08-06T12:53:26.276118Z","title":"Cosmological Moduli and the Post-Inflationary Universe: A Critical Review,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.276118Z"},"links":{"cited_paper":"/paper/1502.07746","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:da97a7391495830fa1374a373955374764009acbddc9a136a79b4f9243fa8e04","observation_id":"171e7525-44bd-4048-8baa-a13f6f11b51f","resolution":{"observed_at":"2026-08-06T12:53:26.276118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9503303","last_updated":"1995-03-13T01:41:28Z","snapshot_observed_at":"2026-07-31T09:10:52.026386Z","submitted_at":"1995-03-12T04:57:44Z","title":"Supersymmetry Breaking in the Early Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9503303","snapshot_observed_at":"2026-08-06T12:53:26.367450Z","title":"Supersymmetry breaking in the early universe,","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.367450Z"},"links":{"cited_paper":"/paper/hep-ph/9503303","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:c905a646c9968d786b5be9f335153129da1f41eaca1f8e5002ae8c031b6b7c3f","observation_id":"80f87734-8103-4390-9030-8aa38e444bdb","resolution":{"observed_at":"2026-08-06T12:53:26.367450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0307181","last_updated":"2003-09-04T08:22:44Z","snapshot_observed_at":"2026-07-07T04:00:35.416001Z","submitted_at":"2003-07-14T16:20:51Z","title":"Gauge Couplings at High Temperature and the Relic Gravitino Abundance","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0307181","snapshot_observed_at":"2026-08-06T12:53:26.441379Z","title":"Gauge couplings at high temperature and the relic gravitino abundance,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.441379Z"},"links":{"cited_paper":"/paper/hep-ph/0307181","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:987fdaf47a93c78e919937de18a28190e549a1334ffae2d968103a681214e10a","observation_id":"7cdfe06b-0ea2-429d-8e17-28aba32e53be","resolution":{"observed_at":"2026-08-06T12:53:26.441379Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0404168","last_updated":"2004-04-22T12:10:30Z","snapshot_observed_at":"2026-07-07T04:50:19.819782Z","submitted_at":"2004-04-22T12:10:30Z","title":"Dilaton Destabilization at High Temperature","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0404168","snapshot_observed_at":"2026-08-06T12:53:26.520100Z","title":"Dilaton destabilization at high temperature,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.520100Z"},"links":{"cited_paper":"/paper/hep-th/0404168","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:9105d59025a0b29ecce1f47bb845d14e5ca8bef48278124ec004e97295f9a6c2","observation_id":"7d3fa49e-03b1-4dc7-822a-b7a4ad8b1e1a","resolution":{"observed_at":"2026-08-06T12:53:26.520100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0309800","last_updated":"2003-11-03T20:25:51Z","snapshot_observed_at":"2026-07-07T00:36:51.458757Z","submitted_at":"2003-09-30T19:40:39Z","title":"Dark Energy from Mass Varying Neutrinos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0309800","snapshot_observed_at":"2026-08-06T12:53:26.618797Z","title":"Dark energy from mass varying neutrinos,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.618797Z"},"links":{"cited_paper":"/paper/astro-ph/0309800","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:eecd36c70ff4f7c96ffca9d81a23d72ff96e1aff9b4d8ddb6972a330bf288540","observation_id":"4a03c706-f426-4226-a130-ce2db144a7ae","resolution":{"observed_at":"2026-08-06T12:53:26.618797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.03662","last_updated":"2018-04-10T18:00:04Z","snapshot_observed_at":"2026-07-06T06:32:44.292339Z","submitted_at":"2018-04-10T18:00:04Z","title":"The Flavor of Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.03662","snapshot_observed_at":"2026-08-06T12:53:26.713057Z","title":"The Flavor of Cosmology,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.713057Z"},"links":{"cited_paper":"/paper/1804.03662","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:409d1a7162e8bb91a56b9ae5c5682fd0f6238acc589ad4bf3f1cdbd486827a08","observation_id":"83fe3121-2792-4cdb-93aa-b0872975be36","resolution":{"observed_at":"2026-08-06T12:53:26.713057Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.02787","last_updated":"2022-09-02T18:32:20Z","snapshot_observed_at":"2026-07-06T10:20:52.839902Z","submitted_at":"2020-12-04T18:59:19Z","title":"A Time-Varying Fine Structure Constant from Naturally Ultralight Dark Matter","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.02787","snapshot_observed_at":"2026-08-06T12:53:26.780830Z","title":"Time-varying fine structure constant from naturally ultralight dark matter,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.780830Z"},"links":{"cited_paper":"/paper/2012.02787","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:195da0f8ebf1db33dd956fc5138f5b41196ce9c0b37adf1ddf05bccc5cfe3408","observation_id":"71fde872-18fd-47d8-8d35-85275f4817cd","resolution":{"observed_at":"2026-08-06T12:53:26.780830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.04476","last_updated":"2021-09-09T18:00:00Z","snapshot_observed_at":"2026-07-06T11:46:10.128480Z","submitted_at":"2021-09-09T18:00:00Z","title":"Thermal Misalignment of Scalar Dark Matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.04476","snapshot_observed_at":"2026-08-06T12:53:26.892439Z","title":"Thermal misalignment of scalar dark matter,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.892439Z"},"links":{"cited_paper":"/paper/2109.04476","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:53973c75186883baabd4bb309c5f9305ccb73cb0f7568a68875f923ac286ebe0","observation_id":"54ad9bfc-b854-4b95-a0e7-df0c174b7f8c","resolution":{"observed_at":"2026-08-06T12:53:26.892439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.13390","last_updated":"2022-01-11T00:43:20Z","snapshot_observed_at":"2026-08-05T10:05:04.659044Z","submitted_at":"2021-04-27T18:00:03Z","title":"Resurrecting Low-Mass Axion Dark Matter Via a Dynamical QCD Scale","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.13390","snapshot_observed_at":"2026-08-06T12:53:26.975341Z","title":"Resurrecting low-mass axion dark matter via a dynamical QCD scale,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:26.975341Z"},"links":{"cited_paper":"/paper/2104.13390","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:7ffa7ca7dec686b902641af745710562058634a7813e365104d898442626ca21","observation_id":"b686ff70-be1e-45c6-a56e-e8e295afaa87","resolution":{"observed_at":"2026-08-06T12:53:26.975341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06727","last_updated":"2020-07-31T02:30:01Z","snapshot_observed_at":"2026-08-07T11:00:12.559889Z","submitted_at":"2020-04-14T18:00:01Z","title":"Dark Matter Freeze Out during an Early Cosmological Period of QCD Confinement","version":2},"cited_work":{"arxiv_id":"2004.06727","doi":null,"metadata_source":"pith","pith_arxiv_id":"2004.06727","snapshot_observed_at":"2026-08-06T12:53:33.344115Z","title":"Dark Matter Freeze Out during an Early Cosmological Period of QCD Confinement","venue":"hep-ph","work_id":"41d0ba15-22d1-4c81-8800-5caf9d53b8c2","year":2020},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.051498Z"},"links":{"cited_paper":"/paper/2004.06727","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:0f3d3f9c7c8afe483a1297cb3782f67066860c9c924e90819cfaa5020705d14c","observation_id":"21216b6b-2247-4316-8d42-f926a6828896","resolution":{"observed_at":"2026-08-06T12:53:33.451204Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.09152","last_updated":"2021-12-16T19:00:52Z","snapshot_observed_at":"2026-07-31T22:16:32.151790Z","submitted_at":"2021-12-16T19:00:52Z","title":"Dark Matter Freeze-out during $\\mathrm{SU}(2)_{\\rm L}$ Confinement","version":1},"cited_work":{"arxiv_id":"2112.09152","doi":null,"metadata_source":"pith","pith_arxiv_id":"2112.09152","snapshot_observed_at":"2026-08-06T12:53:33.128742Z","title":"Dark Matter Freeze-out during $\\mathrm{SU}(2)_{\\rm L}$ Confinement","venue":"hep-ph","work_id":"a8281b26-707d-488b-98db-d847b16d6458","year":2021},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.132648Z"},"links":{"cited_paper":"/paper/2112.09152","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:a5d4fb5bcda770118127dd503fe73fbcf45c076cc3492925fbbc053285b28119","observation_id":"5c81d6d5-c2d0-4326-b210-ccf25777e722","resolution":{"observed_at":"2026-08-06T12:53:33.220401Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00559","last_updated":"2019-03-21T17:56:24Z","snapshot_observed_at":"2026-07-06T07:12:07.929259Z","submitted_at":"2018-11-01T18:00:02Z","title":"Early Cosmological Period of QCD Confinement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.00559","snapshot_observed_at":"2026-08-06T12:53:27.204035Z","title":"Early Cosmological Period of QCD Confinement,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.204035Z"},"links":{"cited_paper":"/paper/1811.00559","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:8d97e67bc6e021661577843bb20e52879ecd958b9f16a61ba3d1d24f47ed19ad","observation_id":"67be8ed3-52c2-467a-a239-a7af91688214","resolution":{"observed_at":"2026-08-06T12:53:27.204035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.11994","last_updated":"2019-05-28T18:00:00Z","snapshot_observed_at":"2026-07-06T07:56:11.645313Z","submitted_at":"2019-05-28T18:00:00Z","title":"Electroweak Baryogenesis from Temperature-Varying Couplings","version":1},"cited_work":{"arxiv_id":"1905.11994","doi":null,"metadata_source":"pith","pith_arxiv_id":"1905.11994","snapshot_observed_at":"2026-08-06T12:53:32.900735Z","title":"Electroweak Baryogenesis from Temperature-Varying Couplings","venue":"hep-ph","work_id":"bba48657-80cd-4023-ae56-f9f723679b07","year":2019},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.289446Z"},"links":{"cited_paper":"/paper/1905.11994","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:44d390a3914f4261419e22267582e3e5e0fcce247895fd3aa0277affb252a57e","observation_id":"4c088183-3dba-461d-97ec-2708f65996eb","resolution":{"observed_at":"2026-08-06T12:53:32.961299Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.01432","last_updated":"2020-03-31T20:50:11Z","snapshot_observed_at":"2026-07-06T08:34:37.822383Z","submitted_at":"2019-11-04T19:00:02Z","title":"QCD Baryogenesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.01432","snapshot_observed_at":"2026-08-06T12:53:27.430257Z","title":"QCD baryogenesis,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.430257Z"},"links":{"cited_paper":"/paper/1911.01432","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:c3953878b48861505e264daa7f3f6060c664bc440a83972c98e3194a46f45cb7","observation_id":"92383508-899e-47a8-b9da-599da1937138","resolution":{"observed_at":"2026-08-06T12:53:27.430257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2204.07584","last_updated":"2022-07-29T19:32:27Z","snapshot_observed_at":"2026-07-06T13:00:46.828547Z","submitted_at":"2022-04-15T18:00:00Z","title":"Archimedean Lever Leptogenesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2204.07584","snapshot_observed_at":"2026-08-06T12:53:27.529935Z","title":"Leptogenesis enabled by dark matter,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.529935Z"},"links":{"cited_paper":"/paper/2204.07584","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:0f480424a3224092ec5260351f78ce0e9a1d876fd217b0ec678ec02c166e1dec","observation_id":"68080c55-1d92-4637-a8cd-bdea46389470","resolution":{"observed_at":"2026-08-06T12:53:27.529935Z","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":"2026-08-06T12:53:27.648759Z","title":"Leptogenesis During an Era of Early SU(2) Confinement,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.648759Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:1542508dd377755a58c28d7183f635ecc280e41924ae8563002f6ad4a594c571","observation_id":"1c6630ee-4ef5-46b6-9494-699486e70d88","resolution":{"observed_at":"2026-08-06T12:53:27.648759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09747","last_updated":"2025-03-31T14:24:32Z","snapshot_observed_at":"2026-07-06T19:50:33.453131Z","submitted_at":"2024-11-14T19:01:28Z","title":"Thermo-Coupled Early Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.09747","snapshot_observed_at":"2026-08-06T12:53:27.733476Z","title":"Thermocoupled early dark energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.733476Z"},"links":{"cited_paper":"/paper/2411.09747","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:b317b5a7b7470dd8ed826c71fee53017c0adb57c0a7db0174710a077a2e36d74","observation_id":"662c9783-02d8-4331-828d-77e410320c07","resolution":{"observed_at":"2026-08-06T12:53:27.733476Z","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":"2507.13135","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T12:53:32.493304Z","title":"Gravitational Waves from First-Order Phase Transitions Assisted by Temperature-Enhanced Scatterings,","venue":null,"work_id":"1da7f561-71ec-432a-955b-d7b085556a81","year":null},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.836877Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:5d7e8411562baa560f4c6de50a9f56c2df4f7c1e96181bd95c349816467d4ce1","observation_id":"6f1b228a-5416-49d5-82ae-14793e152dc0","resolution":{"observed_at":"2026-08-06T12:53:32.608400Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T12:53:34.917354Z","title":"Effective Fermion Masses of Order gT in High Temperature Gauge Theories with Exact Chiral Invariance,","venue":null,"work_id":"3d51a1fb-8c19-4674-a4f3-4808a8cd3f43","year":1982},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:27.939938Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:8dfbe93e0df794b78ada80944fdf846894e02008ffd42a854f8af08d6d6659be","observation_id":"12698e7e-3556-4449-b3d7-7eb461edb7a2","resolution":{"observed_at":"2026-08-06T12:53:34.980862Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9408276","last_updated":"1994-08-12T01:38:40Z","snapshot_observed_at":"2026-07-07T04:17:51.194666Z","submitted_at":"1994-08-12T01:38:40Z","title":"The Three-Loop Free Energy for Pure Gauge QCD","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9408276","snapshot_observed_at":"2026-08-06T12:53:28.010663Z","title":"The Three loop free energy for pure gauge QCD,","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.010663Z"},"links":{"cited_paper":"/paper/hep-ph/9408276","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:4783016247cd56bf07c8da07e37f2d918e4015c5017fdbab949ca613f667b2c7","observation_id":"768597eb-5006-4833-9c14-d479deb8b92e","resolution":{"observed_at":"2026-08-06T12:53:28.010663Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9410360","last_updated":"1994-10-24T19:30:20Z","snapshot_observed_at":"2026-07-07T04:18:27.707106Z","submitted_at":"1994-10-24T19:30:20Z","title":"The Three-Loop Free Energy for High-Temperature QED and QCD with Fermions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9410360","snapshot_observed_at":"2026-08-06T12:53:28.106655Z","title":"The Three loop free energy for high temperature QED and QCD with fermions,","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.106655Z"},"links":{"cited_paper":"/paper/hep-ph/9410360","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:74ba18c837356e3a68bfce574cb9cdbb2b3f1efb3e11f0e65c24f66eb71b6f83","observation_id":"4de5971e-20b3-4d6c-901c-90612c60ae3a","resolution":{"observed_at":"2026-08-06T12:53:28.106655Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9507380","last_updated":"1995-11-09T16:58:37Z","snapshot_observed_at":"2026-07-07T04:20:28.532915Z","submitted_at":"1995-07-21T20:55:46Z","title":"The Free Energy of Hot Gauge Theories with Fermions Through g^5","version":2},"cited_work":{"arxiv_id":"hep-ph/9507380","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9507380","snapshot_observed_at":"2026-08-06T12:53:32.047796Z","title":"The Free Energy of Hot Gauge Theories with Fermions Through g^5","venue":"hep-ph","work_id":"f1060323-fa6b-4580-8cf8-c05d8dd8ad48","year":1995},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.168572Z"},"links":{"cited_paper":"/paper/hep-ph/9507380","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:faa943e457cb4bb4a02195988c33a0dc5c7fb2d0555168ee3dcad60c32ee094a","observation_id":"3a61c5f4-2fbd-4b95-af4d-018bfa4d6304","resolution":{"observed_at":"2026-08-06T12:53:32.197766Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0211321","last_updated":"2003-03-18T17:10:56Z","snapshot_observed_at":"2026-07-07T03:58:15.324410Z","submitted_at":"2002-11-20T16:27:55Z","title":"The pressure of hot QCD up to g^6 ln(1/g)","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0211321","snapshot_observed_at":"2026-08-06T12:53:28.257568Z","title":"The Pressure of hot QCD up to g6 ln(1/g),","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.257568Z"},"links":{"cited_paper":"/paper/hep-ph/0211321","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:a444695adfb35bfbe6704e2b716d804b066745ba6866f48ebfcf2f5a24971864","observation_id":"7ae56858-956e-4510-8a9d-bbc31a007001","resolution":{"observed_at":"2026-08-06T12:53:28.257568Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01554","last_updated":"2022-01-14T16:57:11Z","snapshot_observed_at":"2026-08-07T03:43:12.233502Z","submitted_at":"2017-01-06T06:39:49Z","title":"Basics of thermal field theory -- a tutorial on perturbative computations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.01554","snapshot_observed_at":"2026-08-06T12:53:28.327304Z","title":"Laine and A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.327304Z"},"links":{"cited_paper":"/paper/1701.01554","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:f233364e3a492321167e50dfc62964157b98032dc5cbdea224d73c24ad28fa64","observation_id":"2f1ce347-2481-40c2-af0d-89ffe321111a","resolution":{"observed_at":"2026-08-06T12:53:28.327304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.07479","last_updated":"2017-05-19T08:57:09Z","snapshot_observed_at":"2026-07-06T05:31:14.242311Z","submitted_at":"2017-02-24T07:16:16Z","title":"Thermal phase transition with full 2-loop effective potential","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.07479","snapshot_observed_at":"2026-08-06T12:53:28.388224Z","title":"Thermal phase transition with full 2-loop effective potential,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.388224Z"},"links":{"cited_paper":"/paper/1702.07479","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:b13f5a79743bbddf6d4606f90fe69bf29ccc9aac88829bfe915f17b847de4393","observation_id":"56732298-1ab6-4a1c-bdac-99284f90a5fa","resolution":{"observed_at":"2026-08-06T12:53:28.388224Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-lat/9805024","last_updated":"1998-05-26T14:12:06Z","snapshot_observed_at":"2026-07-07T03:46:19.522293Z","submitted_at":"1998-05-26T14:12:06Z","title":"Inverse Symmetry Breaking with 4d Lattice Simulations","version":1},"cited_work":{"arxiv_id":"hep-lat/9805024","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-lat/9805024","snapshot_observed_at":"2026-08-06T12:53:31.776063Z","title":"Inverse Symmetry Breaking with 4d Lattice Simulations","venue":"hep-lat","work_id":"d0fdc953-1e1a-46ef-89f4-09a6c7e7a05a","year":1998},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.485472Z"},"links":{"cited_paper":"/paper/hep-lat/9805024","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:16e844cafe2e2108b76f2f6629014713b6eb32dcc9db5e1bd7ee643944963185","observation_id":"063ea7e9-961e-4e00-9091-5ded17340818","resolution":{"observed_at":"2026-08-06T12:53:31.858645Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T12:53:34.768068Z","title":"Phase Structure of Scalar Compact QED,","venue":null,"work_id":"39eb685d-4223-4a47-b5e9-c8b588b3196f","year":1986},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.554822Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:b298ea54017a39509e5bba4e21dec5903d64ee97d7241f8bdc4c92dc23e2d5f2","observation_id":"3b42ec27-3292-42df-a83c-5f387a87b9d2","resolution":{"observed_at":"2026-08-06T12:53:34.847030Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.00957","last_updated":"2025-04-18T02:35:35Z","snapshot_observed_at":"2026-08-03T17:24:05.624970Z","submitted_at":"2024-10-01T18:00:00Z","title":"Displaced vertex signals of low temperature baryogenesis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.00957","snapshot_observed_at":"2026-08-06T12:53:28.612881Z","title":"Displaced vertex signals of low temperature baryogenesis,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.612881Z"},"links":{"cited_paper":"/paper/2410.00957","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:e374e9b249b9149ed632ee188df1e28b0877d209e35fd4accedac8b883d05cdd","observation_id":"788e7731-800e-458c-b9e2-99cf6ba1fbec","resolution":{"observed_at":"2026-08-06T12:53:28.612881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.00964","last_updated":"2025-04-18T02:39:05Z","snapshot_observed_at":"2026-07-06T19:25:28.300272Z","submitted_at":"2024-10-01T18:00:02Z","title":"Spontaneous breaking of baryon number, baryogenesis and the bajoron","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.00964","snapshot_observed_at":"2026-08-06T12:53:28.692266Z","title":"Spontaneous breaking of baryon number, baryogenesis and the bajoron,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.692266Z"},"links":{"cited_paper":"/paper/2410.00964","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:1d64b48ce6b1f116f29fd5d1d6d4bc6cf28bf2cceaa5576607d05d9ec48740dc","observation_id":"800aafb4-d7a3-4405-a8c1-9cf058225eb9","resolution":{"observed_at":"2026-08-06T12:53:28.692266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0510213","last_updated":"2005-12-02T20:18:06Z","snapshot_observed_at":"2026-07-07T04:09:01.741094Z","submitted_at":"2005-10-17T19:41:45Z","title":"Theory of Neutrinos: A White Paper","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0510213","snapshot_observed_at":"2026-08-06T12:53:28.808380Z","title":"Theory of neutrinos: A White paper,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.808380Z"},"links":{"cited_paper":"/paper/hep-ph/0510213","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:ca754c35168b43bde726bbbfe453360a8e3e4415f50785f03ce1381b03f99ae7","observation_id":"3a7b2955-fc05-4b3e-a9a7-65d3f7695361","resolution":{"observed_at":"2026-08-06T12:53:28.808380Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.03020","last_updated":"2019-05-30T06:25:35Z","snapshot_observed_at":"2026-08-05T07:33:02.749643Z","submitted_at":"2019-04-04T00:15:48Z","title":"Gravitational waves from the minimal gauged $U(1)_{B-L}$ model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.03020","snapshot_observed_at":"2026-08-06T12:53:28.885110Z","title":"Gravitational waves from the minimal gauged𝑈(1)𝐵−𝐿 model,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.885110Z"},"links":{"cited_paper":"/paper/1904.03020","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:1adbd87d6e526ebb7326fb605f310a50cfe8e27c33ee9e1981342f43d30ba3cf","observation_id":"d0ff55c1-119c-4153-bf83-270b7caae1dd","resolution":{"observed_at":"2026-08-06T12:53:28.885110Z","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":"2026-08-06T12:53:34.627103Z","title":"Low-energy remnants of superstring anomaly cancellation terms,","venue":null,"work_id":"58814294-2f77-451f-a0b2-69e054224938","year":1986},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:28.988111Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:02487bbe5e5c7c870a9b1f971a05737f8b62d8f04c03bb69ba5f8aaa5a3a7aa3","observation_id":"f8e85841-470d-4e39-ae40-971106a81c33","resolution":{"observed_at":"2026-08-06T12:53:34.706442Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T12:53:34.358250Z","title":"Moduli dependence of string loop corrections to gauge coupling constants,","venue":null,"work_id":"8d9a7085-4b91-4a81-9701-1e4fd81fb744","year":1991},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.053536Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:0680c1846a43b009725ba5778b9729d3c206092dad6b60ac1453d60b29273d0b","observation_id":"a84e00e0-86f3-416d-8c55-82e3ebbd8906","resolution":{"observed_at":"2026-08-06T12:53:34.492333Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9807124","last_updated":"1998-10-18T20:05:01Z","snapshot_observed_at":"2026-07-07T05:17:14.961280Z","submitted_at":"1998-07-17T14:48:18Z","title":"(0,2) Heterotic Gauge Couplings and their M-Theory Origin","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9807124","snapshot_observed_at":"2026-08-06T12:53:29.122222Z","title":"(0,2) heterotic gauge couplings and their M-theory origin,","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.122222Z"},"links":{"cited_paper":"/paper/hep-th/9807124","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:6e6b15a679e2d811bf7c25ad732b6d8b6640b450e77b86892ae4ad476defdddb","observation_id":"7e24d1d7-af4f-48e7-a562-a7c13b951d2d","resolution":{"observed_at":"2026-08-06T12:53:29.122222Z","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":"2026-08-06T12:53:34.079361Z","title":"Is the superstring weakly coupled?,","venue":null,"work_id":"2f07f10a-387b-4d0c-b468-2285b4f80860","year":1985},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.213981Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:a072511c703ee4a157ce2fee13ee9f041d16da472ec8436248f18ebdf4a37d04","observation_id":"e6a77273-db4f-4519-9106-0736bc4fbbfb","resolution":{"observed_at":"2026-08-06T12:53:34.164030Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9212049","last_updated":"1992-12-08T17:09:00Z","snapshot_observed_at":"2026-08-05T05:51:38.645188Z","submitted_at":"1992-12-08T17:09:00Z","title":"Challenges for Superstring Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9212049","snapshot_observed_at":"2026-08-06T12:53:29.302197Z","title":"Challenges for superstring cosmology,","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.302197Z"},"links":{"cited_paper":"/paper/hep-th/9212049","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:db6880e9dd3306e679979526b57488c540eb313c005a82d703622c8fd84ee54f","observation_id":"82f26575-4961-4761-a97a-3780d0bdd8cc","resolution":{"observed_at":"2026-08-06T12:53:29.302197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0411011","last_updated":"2005-01-29T20:06:57Z","snapshot_observed_at":"2026-07-07T04:52:14.427684Z","submitted_at":"2004-11-01T20:42:32Z","title":"Landscape, the Scale of SUSY Breaking, and Inflation","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0411011","snapshot_observed_at":"2026-08-06T12:53:29.396343Z","title":"Landscape, the scale of SUSY breaking, and inflation,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.396343Z"},"links":{"cited_paper":"/paper/hep-th/0411011","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:787f59913e5548ba522e955949d46a0d77a19251dc1fa9898d0c9601b33f5321","observation_id":"d6e8e2c6-20db-4b51-b21b-1b75ee0de35c","resolution":{"observed_at":"2026-08-06T12:53:29.396343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9509399","last_updated":"1995-09-26T22:59:57Z","snapshot_observed_at":"2026-07-07T04:20:54.183175Z","submitted_at":"1995-09-26T22:59:57Z","title":"Constraint on the Reheating Temperature from the Decay of the Polonyi Field","version":1},"cited_work":{"arxiv_id":"hep-ph/9509399","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/9509399","snapshot_observed_at":"2026-08-06T12:53:31.473357Z","title":"Constraint on the Reheating Temperature from the Decay of the Polonyi Field","venue":"hep-ph","work_id":"0093d44c-be43-427a-b44a-cebb017258f8","year":1995},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.468473Z"},"links":{"cited_paper":"/paper/hep-ph/9509399","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:30805d67c4371bcad75146848dddb8d155fe190904620e1a3425888b9ef75f65","observation_id":"6217126c-68a3-4571-894e-ba53c9fe14e0","resolution":{"observed_at":"2026-08-06T12:53:31.528424Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0110096","last_updated":"2002-06-04T07:57:25Z","snapshot_observed_at":"2026-07-07T03:53:49.720509Z","submitted_at":"2001-10-07T06:26:41Z","title":"Effects of Cosmological Moduli Fields on Cosmic Microwave Background","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0110096","snapshot_observed_at":"2026-08-06T12:53:29.550908Z","title":"Effects of cosmological moduli fields on cosmic microwave background,","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.550908Z"},"links":{"cited_paper":"/paper/hep-ph/0110096","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:6fa30dd6129d59349a7871c4b92993a1ad015e1c29b8af612754130a1cf8cf93","observation_id":"4038f800-1816-47f5-b2cf-bd2ea571cdf5","resolution":{"observed_at":"2026-08-06T12:53:29.550908Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0807.4313","last_updated":"2008-09-24T13:09:09Z","snapshot_observed_at":"2026-07-06T01:45:36.907045Z","submitted_at":"2008-07-27T17:25:58Z","title":"Unified origin of baryons and dark matter","version":2},"cited_work":{"arxiv_id":"0807.4313","doi":null,"metadata_source":"pith","pith_arxiv_id":"0807.4313","snapshot_observed_at":"2026-08-06T12:53:31.124098Z","title":"Unified origin of baryons and dark matter","venue":"hep-ph","work_id":"e760c55e-3963-4a7e-9d33-813676e62b87","year":2008},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.646010Z"},"links":{"cited_paper":"/paper/0807.4313","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:060ba540fcb2982164e55f8e7b9570a6d904da51d9c96b6c93079de885e9faee","observation_id":"8efbdda0-ffd4-4770-bd6d-79906c0fbc4c","resolution":{"observed_at":"2026-08-06T12:53:31.268556Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1812.09341","last_updated":"2019-05-26T19:45:59Z","snapshot_observed_at":"2026-08-01T16:04:13.666488Z","submitted_at":"2018-12-21T19:15:07Z","title":"Baryogenesis, Dark Matter, and Flavor Structure in Non-thermal Moduli Cosmology","version":2},"cited_work":{"arxiv_id":"1812.09341","doi":null,"metadata_source":"pith","pith_arxiv_id":"1812.09341","snapshot_observed_at":"2026-08-06T12:53:30.774407Z","title":"Baryogenesis, Dark Matter, and Flavor Structure in Non-thermal Moduli Cosmology","venue":"hep-ph","work_id":"2ef706c9-33a2-47dc-b04c-65727b3ecb54","year":2018},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.713265Z"},"links":{"cited_paper":"/paper/1812.09341","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:a725f49ea23c1971085b288189216a9753bb12d05cc1a707494aaa2a3c4fcd0e","observation_id":"d7081d6d-f8aa-4e18-9740-4ead3120f8ea","resolution":{"observed_at":"2026-08-06T12:53:30.935742Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.04705","last_updated":"2019-09-10T18:45:42Z","snapshot_observed_at":"2026-08-04T11:30:45.780998Z","submitted_at":"2019-09-10T18:45:42Z","title":"Baryogenesis from a Modulus Dominated Universe","version":1},"cited_work":{"arxiv_id":"1909.04705","doi":null,"metadata_source":"pith","pith_arxiv_id":"1909.04705","snapshot_observed_at":"2026-08-06T12:53:30.543462Z","title":"Baryogenesis from a Modulus Dominated Universe","venue":"hep-ph","work_id":"778ab9a6-4ef3-4907-ad80-73be05298c30","year":2019},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.809435Z"},"links":{"cited_paper":"/paper/1909.04705","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:f4205e6130355a53579a4b8b7ad739d084a5badecd567b6370254e7124f26b2f","observation_id":"c6adc3ad-36c9-44e9-a059-61f8c56d05df","resolution":{"observed_at":"2026-08-06T12:53:30.652040Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.12546","last_updated":"2023-01-29T21:29:09Z","snapshot_observed_at":"2026-08-02T22:38:24.717978Z","submitted_at":"2023-01-29T21:29:09Z","title":"Dark matter and dark radiation from the early universe with a modulus coupled to the PQMSSM","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.12546","snapshot_observed_at":"2026-08-06T12:53:29.882308Z","title":"Dark matter and dark radiation from the early universe with a modulus coupled to the PQMSSM,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.882308Z"},"links":{"cited_paper":"/paper/2301.12546","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:5dd8df9e0bd88bc489920eaa5dcdb4d6048c3fa2ee2f23424cfbfaa5f56fd7f7","observation_id":"78d034af-aea3-42a6-8253-760f86b36378","resolution":{"observed_at":"2026-08-06T12:53:29.882308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00470","last_updated":"2015-09-01T20:07:03Z","snapshot_observed_at":"2026-07-06T04:28:27.195947Z","submitted_at":"2015-09-01T20:07:03Z","title":"A Tale of Two Timescales: Mixing, Mass Generation, and Phase Transitions in the Early Universe","version":1},"cited_work":{"arxiv_id":"1509.00470","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.00470","snapshot_observed_at":"2026-08-06T12:53:30.284007Z","title":"A Tale of Two Timescales: Mixing, Mass Generation, and Phase Transitions in the Early Universe","venue":"hep-ph","work_id":"12d0e02d-6546-4783-94d8-f36d3fb43a6e","year":2015},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:29.969887Z"},"links":{"cited_paper":"/paper/1509.00470","citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:2c473429240c8167ff08e9a298e0a188e8d0a37f91db2137a8d0834b3fc7fb08","observation_id":"281aa60a-a140-43c3-8797-d5b3b75e926e","resolution":{"observed_at":"2026-08-06T12:53:30.401186Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+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":"2026-08-06T12:53:33.781185Z","title":"The Effective potential at finite temperature in the Standard Model,","venue":null,"work_id":"ac274674-ff96-409a-989c-2469cdbd5ee2","year":1992},"citing_paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T12:53:30.108590Z"},"links":{"citing_paper":"/paper/2507.21523"},"observation_digest":"sha256:5833e151c8380963fcb2b00c8ea7b54506318a56427ebba56191a0916956ef2c","observation_id":"74d8eaf5-e7be-42c3-8031-7a2a1d4317bb","resolution":{"observed_at":"2026-08-06T12:53:33.929194Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2507.21523","last_updated":"2025-07-29T06:20:09Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-06T12:53:21.021528Z","submitted_at":"2025-07-29T06:20:09Z","title":"Thermal History of Non-equilibrated Scalars"},"reference_resolution":{"displayed":47,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":29,"verified_exact":11,"verified_fuzzy":7},"total_outbound_references":47},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 47 of 47 outbound references and 0 inbound Pith citation observations for arXiv:2507.21523."}