{"as_of":"2026-08-20T00:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:44749829c26390bb58067f0104c87fa16ce575be218bb0bd6a921008be69d372","coverage":[{"denominator":206,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T12:45:38.988628Z","state":"measured"},{"denominator":101,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":101,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+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":"2026-08-12T13:07:15.846301Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-12T13:07:16.124175Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"cited_work":{"arxiv_id":"2607.19469","doi":null,"metadata_source":"pith","pith_arxiv_id":"2607.19469","snapshot_observed_at":"2026-08-12T13:07:16.124175Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","venue":"hep-ph","work_id":"28203bf6-58d9-4a11-a64f-3751dc38b21a","year":2026},"citing_paper":{"arxiv_id":"2608.10977","last_updated":"2026-08-11T14:33:24Z","snapshot_observed_at":"2026-08-19T11:30:33.026905Z","submitted_at":"2026-08-11T14:33:24Z","title":"Fine-tuning in mixed Dark Matter models with Primordial Black Hole relics","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-12T13:07:15.846301Z"},"links":{"cited_paper":"/paper/2607.19469","citing_paper":"/paper/2608.10977"},"observation_digest":"sha256:60e7368da2c3ab3cf36d80fef87da591fc7f1a9e9c5da8a3534fb974c2d4bc68","observation_id":"3445406c-8128-4772-b956-37b146b87523","resolution":{"observed_at":"2026-08-12T13:07:16.127653Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2607.19469/citation-record","integrity":"/paper/2607.19469/integrity","json":"/paper/2607.19469/citation-record.json","paper":"/paper/2607.19469"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9605288","last_updated":"1996-05-12T15:53:42Z","snapshot_observed_at":"2026-07-07T04:22:39.163372Z","submitted_at":"1996-05-12T15:53:42Z","title":"Is There a Hot Electroweak Phase Transition at $m_H\\gsim m_W$?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9605288","snapshot_observed_at":"2026-08-01T12:45:38.524788Z","title":"Kajantie, M","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.524788Z"},"links":{"cited_paper":"/paper/hep-ph/9605288","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:6f26c2beaad5790b7c51a3e32e92dcb1479171dc8412800250f4ea0dd112fc54","observation_id":"4ce8f01b-16f0-4d31-a1bb-99c0cc50f09a","resolution":{"observed_at":"2026-08-01T12:45:38.524788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-lat/0611014","last_updated":"2006-11-10T16:05:34Z","snapshot_observed_at":"2026-08-15T10:57:16.323277Z","submitted_at":"2006-11-10T16:05:34Z","title":"The order of the quantum chromodynamics transition predicted by the standard model of particle physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-lat/0611014","snapshot_observed_at":"2026-08-01T12:45:38.530766Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.530766Z"},"links":{"cited_paper":"/paper/hep-lat/0611014","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:c5fd9e11056b193f53918fd7dab52c2a02528baeed9eb9bc5503a6dc927d5a0d","observation_id":"8a24cc50-23ac-45b3-98c2-1beef4d9d027","resolution":{"observed_at":"2026-08-01T12:45:38.530766Z","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":"2026-08-01T12:45:38.535865Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.535865Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:c0d388aa2d1b9749ab0b062516d8ffd360ba74f2cd88f2e5a7e2641b3626a59c","observation_id":"9a681540-1d61-405c-ba31-52b8c7be7016","resolution":{"observed_at":"2026-08-01T12:45:38.535865Z","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":"2026-08-01T12:45:38.540560Z","title":null,"venue":null,"work_id":null,"year":1977},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.540560Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:ce1361968be1b15e23ea2a5c715edbe8ed039ce55986759ce1585db61270e282","observation_id":"3f5d74a3-9f41-446d-a1e1-a66f36c1c99c","resolution":{"observed_at":"2026-08-01T12:45:38.540560Z","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":"2026-08-01T12:45:38.544971Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.544971Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:c5b29f60f016946080a47cc374c1717be4dca1abb5bb5fea5944d9aaa12bc7a8","observation_id":"3837d2d7-32d2-4450-92dd-e39e6dec810c","resolution":{"observed_at":"2026-08-01T12:45:38.544971Z","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":"2026-08-01T12:45:38.550034Z","title":null,"venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.550034Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:b3cd2aebdb30f35ce45db54d3cf455ebcb06cc1adb2678489f778d60d97f470f","observation_id":"a830fb5e-fe44-46cd-94a0-44b37be45076","resolution":{"observed_at":"2026-08-01T12:45:38.550034Z","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":"2026-08-01T12:45:38.555468Z","title":"Gouttenoire, Beyond the Standard Model Cocktail","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.555468Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:2747a7aa2cf7ec1fc6fd2bc33469ccf82324709c5d9e5ccd29e76da3712098eb","observation_id":"92c9ade9-fa0c-456e-aeb3-8efc3cb66333","resolution":{"observed_at":"2026-08-01T12:45:38.555468Z","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":"2026-08-01T12:45:38.560268Z","title":null,"venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.560268Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:d67bcb7f053ae61773d7ac06313eb2561274c81601450ce291f609f2bfa8df3e","observation_id":"18ca16de-c94d-4102-aee0-e659cb9377d3","resolution":{"observed_at":"2026-08-01T12:45:38.560268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.08215","last_updated":"2017-05-12T18:56:59Z","snapshot_observed_at":"2026-08-14T21:10:18.041698Z","submitted_at":"2017-03-23T19:51:47Z","title":"Electroweak Bubble Wall Speed Limit","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.08215","snapshot_observed_at":"2026-08-01T12:45:38.565076Z","title":"Bodeker and G","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.565076Z"},"links":{"cited_paper":"/paper/1703.08215","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:8386bbad1082ca3fccab22da189a3ada33437133b1bed15fd79bda00efe4dde9","observation_id":"36427b95-6df5-448d-84b0-e2f99b4f5bee","resolution":{"observed_at":"2026-08-01T12:45:38.565076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.10343","last_updated":"2021-03-16T10:03:22Z","snapshot_observed_at":"2026-08-14T21:10:44.517931Z","submitted_at":"2020-07-20T18:00:01Z","title":"Towards an all-orders calculation of the electroweak bubble wall velocity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.10343","snapshot_observed_at":"2026-08-01T12:45:38.569958Z","title":"Höche, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.569958Z"},"links":{"cited_paper":"/paper/2007.10343","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:0ab0ed145fa3f74222d8ffa05d32cc58d57eb32b8d48a603c122a90bb49a0d09","observation_id":"45549496-02d5-4456-91c0-33368a63126c","resolution":{"observed_at":"2026-08-01T12:45:38.569958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.02590","last_updated":"2020-11-26T12:17:38Z","snapshot_observed_at":"2026-08-19T17:24:09.508044Z","submitted_at":"2020-10-06T10:00:44Z","title":"Bubble wall velocity: heavy physics effects","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.02590","snapshot_observed_at":"2026-08-01T12:45:38.574955Z","title":"Azatov and M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.574955Z"},"links":{"cited_paper":"/paper/2010.02590","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:909917eaacafe169c9b4f972139d12d3524a4b239d6f42620d134361543825ea","observation_id":"4ccacf4d-6e2c-4ef4-9808-1fea0b1aa231","resolution":{"observed_at":"2026-08-01T12:45:38.574955Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.07686","last_updated":"2022-07-14T14:04:23Z","snapshot_observed_at":"2026-08-16T17:34:38.941038Z","submitted_at":"2021-12-14T19:00:02Z","title":"Friction pressure on relativistic bubble walls","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.07686","snapshot_observed_at":"2026-08-01T12:45:38.580098Z","title":"Gouttenoire, R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.580098Z"},"links":{"cited_paper":"/paper/2112.07686","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:bf4df639caa3d1e2a59e9bf4031cbc1b48a54a9acd9d460689b2e8793de4ad00","observation_id":"623c9734-30d2-4bac-9c36-309648c2b0a8","resolution":{"observed_at":"2026-08-01T12:45:38.580098Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.06972","last_updated":"2024-07-13T10:30:47Z","snapshot_observed_at":"2026-08-18T14:00:26.954050Z","submitted_at":"2023-10-10T19:51:43Z","title":"Quantisation Across Bubble Walls and Friction","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.06972","snapshot_observed_at":"2026-08-01T12:45:38.584826Z","title":"Azatov, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.584826Z"},"links":{"cited_paper":"/paper/2310.06972","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:80fe214b39cec65905d2e320fe7796fbf320fcdde6a09763619c720e147e6dc2","observation_id":"201871e6-32dd-4a9e-976c-bc77d86ad44a","resolution":{"observed_at":"2026-08-01T12:45:38.584826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.13725","last_updated":"2025-08-12T19:54:01Z","snapshot_observed_at":"2026-08-17T21:27:10.939039Z","submitted_at":"2025-04-18T14:50:03Z","title":"Bubble wall dynamics from nonequilibrium quantum field theory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.13725","snapshot_observed_at":"2026-08-01T12:45:38.589335Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.589335Z"},"links":{"cited_paper":"/paper/2504.13725","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:3d08b4f8935874037bcb3efed50edd3b760026a2af25cb07f01b7b5bb62f1f1d","observation_id":"027f2343-1a4e-4da1-9da1-28109bf0a294","resolution":{"observed_at":"2026-08-01T12:45:38.589335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.01473","last_updated":"2018-08-28T16:24:26Z","snapshot_observed_at":"2026-08-14T19:19:04.974743Z","submitted_at":"2018-05-03T18:00:01Z","title":"Super-cool Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.01473","snapshot_observed_at":"2026-08-01T12:45:38.593728Z","title":"Hambye, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.593728Z"},"links":{"cited_paper":"/paper/1805.01473","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:20a145af25f5f8779b8e457b1f723da7c5aed87adc944823424ade5a7fa96d9b","observation_id":"6a96d2a9-951d-4c47-b747-120b7710720a","resolution":{"observed_at":"2026-08-01T12:45:38.593728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.02830","last_updated":"2020-10-13T15:09:33Z","snapshot_observed_at":"2026-08-15T00:55:33.605217Z","submitted_at":"2019-12-05T19:00:03Z","title":"Filtered Dark Matter at a First Order Phase Transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.02830","snapshot_observed_at":"2026-08-01T12:45:38.598277Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.598277Z"},"links":{"cited_paper":"/paper/1912.02830","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:d2a13aba90ce368f86741fe4fc3170cc6c2ee750c38b9d98b912cb9244b2ad32","observation_id":"778b9fba-4c30-481e-ae00-87dcaad30eb9","resolution":{"observed_at":"2026-08-01T12:45:38.598277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.06346","last_updated":"2024-05-28T08:46:15Z","snapshot_observed_at":"2026-08-19T13:48:55.219004Z","submitted_at":"2023-11-10T19:00:02Z","title":"Hunting WIMPs with LISA: Correlating dark matter and gravitational wave signals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.06346","snapshot_observed_at":"2026-08-01T12:45:38.603186Z","title":"Bringmann, T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.603186Z"},"links":{"cited_paper":"/paper/2311.06346","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:21b0693a5f35eaa039b4abbd987abf78ae71c9d11e13e5fa2ae362277e78e362","observation_id":"5203f113-3c44-4e84-83e9-42c65a0cba83","resolution":{"observed_at":"2026-08-01T12:45:38.603186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.10593","last_updated":"2025-04-14T18:00:11Z","snapshot_observed_at":"2026-08-16T12:41:12.421093Z","submitted_at":"2025-04-14T18:00:11Z","title":"Dark matter phase-in: producing feebly-interacting particles after a first-order phase transition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.10593","snapshot_observed_at":"2026-08-01T12:45:38.608010Z","title":"Benso, F","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.608010Z"},"links":{"cited_paper":"/paper/2504.10593","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:56e47d0825b7324a76850ede05378b7d086033de2fb67d975f74410d1d969590","observation_id":"eaca4221-0dda-4a32-8c17-874f14e17d4e","resolution":{"observed_at":"2026-08-01T12:45:38.608010Z","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":"2026-08-01T12:45:38.612835Z","title":"Watkins and L","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.612835Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:8b8e0ef4f470c57575587f5af4edd73f6698e9cd2ba6fa4d77ad505714ad6ffb","observation_id":"8be60396-8c79-4b62-b6f2-814a4361e802","resolution":{"observed_at":"2026-08-01T12:45:38.612835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9602095","last_updated":"1996-02-19T16:45:12Z","snapshot_observed_at":"2026-07-07T01:12:56.570699Z","submitted_at":"1996-02-19T16:45:12Z","title":"Preheating and symmetry restoration in collisions of vacuum bubbles","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9602095","snapshot_observed_at":"2026-08-01T12:45:38.617003Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.617003Z"},"links":{"cited_paper":"/paper/astro-ph/9602095","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:4934747e5ce07bd4e8f5cf09bdc8478f03ce50e1ee602fdf0e7ac3ab59f49216","observation_id":"df8e30e3-8833-4a1c-a342-9323925d5a65","resolution":{"observed_at":"2026-08-01T12:45:38.617003Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1104.4793","last_updated":"2011-07-21T20:47:04Z","snapshot_observed_at":"2026-08-15T04:48:28.345682Z","submitted_at":"2011-04-25T20:04:51Z","title":"Natural Cold Baryogenesis from Strongly Interacting Electroweak Symmetry Breaking","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1104.4793","snapshot_observed_at":"2026-08-01T12:45:38.621277Z","title":"Konstandin and G","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.621277Z"},"links":{"cited_paper":"/paper/1104.4793","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:d22e40f3e03418ee28d2cb2ef38663e085c14ebcba4f24ea924046051753c2dd","observation_id":"af8d6750-1c08-46d1-830c-5810b6e4919b","resolution":{"observed_at":"2026-08-01T12:45:38.621277Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.5615","last_updated":"2012-11-23T21:39:44Z","snapshot_observed_at":"2026-08-15T00:38:20.566156Z","submitted_at":"2012-11-23T21:39:44Z","title":"Non-thermal Dark Matter Production from the Electroweak Phase Transition: Multi-TeV WIMPs and \"Baby-Zillas\"","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.5615","snapshot_observed_at":"2026-08-01T12:45:38.625814Z","title":"Falkowski and J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.625814Z"},"links":{"cited_paper":"/paper/1211.5615","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:931b48d8a38e1b6ff9fa572875f8893b0e9c4a59ba1c76bef2dbc02c4cfb6e01","observation_id":"a31428a1-5bab-4781-8049-b12f33a2f132","resolution":{"observed_at":"2026-08-01T12:45:38.625814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.13070","last_updated":"2025-01-13T13:28:57Z","snapshot_observed_at":"2026-08-20T00:42:23.694039Z","submitted_at":"2023-08-24T20:25:39Z","title":"On Particle Production from Phase Transition Bubbles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.13070","snapshot_observed_at":"2026-08-01T12:45:38.630476Z","title":"Mansour and B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.630476Z"},"links":{"cited_paper":"/paper/2308.13070","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:6e607606e88741d153bc81c735b4b0420bc79de2ce4c01ab4ae65b5c357e7299","observation_id":"515628b1-1565-4b4a-9619-e585e8477c99","resolution":{"observed_at":"2026-08-01T12:45:38.630476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.16224","last_updated":"2025-01-11T12:03:37Z","snapshot_observed_at":"2026-08-16T15:04:31.612217Z","submitted_at":"2023-08-30T18:00:01Z","title":"Aspects of Particle Production from Bubble Dynamics at a First Order Phase Transition","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.16224","snapshot_observed_at":"2026-08-01T12:45:38.635152Z","title":"Shakya, Aspects of particle production from bubble dynamics at a first order phase transition , Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.635152Z"},"links":{"cited_paper":"/paper/2308.16224","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:cf83151b19de082ba919c856c9dd2bb21271df8821407ce31da18b2b85795038","observation_id":"8e8c7e03-b647-45ee-853a-e810b560704d","resolution":{"observed_at":"2026-08-01T12:45:38.635152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.03252","last_updated":"2025-01-09T15:09:17Z","snapshot_observed_at":"2026-08-19T17:35:01.084519Z","submitted_at":"2024-03-05T19:00:02Z","title":"Nonthermal Heavy Dark Matter from a First-Order Phase Transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.03252","snapshot_observed_at":"2026-08-01T12:45:38.639885Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.639885Z"},"links":{"cited_paper":"/paper/2403.03252","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:7d68f62040d217f3fcf88352612f80afacb15282f65cb2e4a0dad8525e14f909","observation_id":"1e1ec310-d154-4777-a9c0-0bbd9f339e5c","resolution":{"observed_at":"2026-08-01T12:45:38.639885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.15555","last_updated":"2025-02-18T13:50:47Z","snapshot_observed_at":"2026-08-16T15:20:42.362385Z","submitted_at":"2023-06-27T15:25:50Z","title":"Bubbletrons: Ultrahigh-Energy Particle Collisions and Heavy Dark Matter at Phase Transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.15555","snapshot_observed_at":"2026-08-01T12:45:38.645014Z","title":"Baldes, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.645014Z"},"links":{"cited_paper":"/paper/2306.15555","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:dd55092f84ee570d3c436dc689d765153b7f6e1f07b4d5df568257155c08d51c","observation_id":"83cff165-bd69-4910-b614-55416a182359","resolution":{"observed_at":"2026-08-01T12:45:38.645014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.03758","last_updated":"2026-05-05T13:42:19Z","snapshot_observed_at":"2026-07-06T23:16:40.201701Z","submitted_at":"2026-05-05T13:42:19Z","title":"Dark Matter Production from Bubble Collisions during a First-Order Phase Transition at the End of Inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.03758","snapshot_observed_at":"2026-08-01T12:45:38.649443Z","title":"Cheng and F","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.649443Z"},"links":{"cited_paper":"/paper/2605.03758","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:69bb26f8d307da7189a572171a5ec224f5b2675e27d5df646f023c90587ab6e7","observation_id":"d03f8571-43c6-4cc6-a076-142dbaa48962","resolution":{"observed_at":"2026-08-01T12:45:38.649443Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.15279","last_updated":"2026-07-16T17:59:59Z","snapshot_observed_at":"2026-08-16T22:35:58.429540Z","submitted_at":"2026-07-16T17:59:59Z","title":"Particle production from bubble collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.15279","snapshot_observed_at":"2026-08-01T12:45:38.654408Z","title":"Ghoshal, P","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.654408Z"},"links":{"cited_paper":"/paper/2607.15279","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:0a3e8758b4fc8fb30407cb9a2ae5de8610fa8eb8b19d732e19f78da368449031","observation_id":"ea4b74b7-d8ea-425a-b61b-2a818b045963","resolution":{"observed_at":"2026-08-01T12:45:38.654408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.16398","last_updated":"2026-07-17T18:00:02Z","snapshot_observed_at":"2026-08-13T09:10:41.720292Z","submitted_at":"2026-07-17T18:00:02Z","title":"Particle productions during collisions of highly boosted bubble walls","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.16398","snapshot_observed_at":"2026-08-01T12:45:38.659199Z","title":"An and H","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.659199Z"},"links":{"cited_paper":"/paper/2607.16398","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:79d12fd834049c5966c47a3554ab07f87248236b469506b0b26a2fec9565f4c4","observation_id":"faeb2ee3-2e1b-4572-9b48-8e680a7cc854","resolution":{"observed_at":"2026-08-01T12:45:38.659199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08440","last_updated":"2021-05-03T10:23:35Z","snapshot_observed_at":"2026-08-09T11:28:04.109486Z","submitted_at":"2020-07-16T16:25:29Z","title":"String Fragmentation in Supercooled Confinement and Implications for Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08440","snapshot_observed_at":"2026-08-01T12:45:38.663859Z","title":"Baldes, Y","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.663859Z"},"links":{"cited_paper":"/paper/2007.08440","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:13db8c7a4ba2a74d9634a86d0389245854691fae9a0b603439af6fa3d8b78bfe","observation_id":"0364d068-0d13-463f-8131-4b3ea8fbfa4d","resolution":{"observed_at":"2026-08-01T12:45:38.663859Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.13926","last_updated":"2022-07-13T19:56:13Z","snapshot_observed_at":"2026-08-16T17:46:21.496361Z","submitted_at":"2021-10-26T18:00:02Z","title":"Supercool Composite Dark Matter Beyond 100 TeV","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.13926","snapshot_observed_at":"2026-08-01T12:45:38.668598Z","title":"Baldes, Y","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.668598Z"},"links":{"cited_paper":"/paper/2110.13926","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:2023a6d5c6d520cc94e8bd490ac5181efc3c120f89074dfa27594a725d49f3e6","observation_id":"40c5a446-652e-4cb2-835b-8b8067dca450","resolution":{"observed_at":"2026-08-01T12:45:38.668598Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.05721","last_updated":"2021-01-14T16:55:29Z","snapshot_observed_at":"2026-08-18T15:35:39.220772Z","submitted_at":"2021-01-14T16:55:29Z","title":"Dark Matter production from relativistic bubble walls","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.05721","snapshot_observed_at":"2026-08-01T12:45:38.673119Z","title":"Azatov, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.673119Z"},"links":{"cited_paper":"/paper/2101.05721","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:a3c2772196034740fc5d3948fb7f55b428bbbaf107d8561def6224e09654fc10","observation_id":"1647a98b-bcc8-4618-93c7-0ad006686190","resolution":{"observed_at":"2026-08-01T12:45:38.673119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.05096","last_updated":"2022-12-05T16:30:56Z","snapshot_observed_at":"2026-08-19T17:25:51.305695Z","submitted_at":"2022-07-11T18:00:03Z","title":"Hot and heavy dark matter from a weak scale phase transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.05096","snapshot_observed_at":"2026-08-01T12:45:38.677794Z","title":"Baldes, Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.677794Z"},"links":{"cited_paper":"/paper/2207.05096","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:6f6df1e0b7b02f588c7273e2b284bccc0c32f77231c10fe5c707387ea63edab2","observation_id":"f887b64c-7445-473f-b7b5-ad100bc2d77f","resolution":{"observed_at":"2026-08-01T12:45:38.677794Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00029","last_updated":"2023-10-31T18:00:01Z","snapshot_observed_at":"2026-08-19T17:38:50.885431Z","submitted_at":"2023-10-31T18:00:01Z","title":"Heavy Baryon Dark Matter from $SU(N)$ Confinement: Bubble Wall Velocity and Boundary Effects","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00029","snapshot_observed_at":"2026-08-01T12:45:38.682078Z","title":"Gouttenoire, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.682078Z"},"links":{"cited_paper":"/paper/2311.00029","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:0b02765d5d391e3423e560a85d5de79aa5a14ed8b190e00da1cca92ba3bcf90f","observation_id":"6a30b6df-9154-4b99-bbb2-5422c8413f35","resolution":{"observed_at":"2026-08-01T12:45:38.682078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.05615","last_updated":"2024-05-21T09:30:40Z","snapshot_observed_at":"2026-08-17T02:01:15.356358Z","submitted_at":"2024-03-08T19:00:00Z","title":"Particle shells from relativistic bubble walls","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.05615","snapshot_observed_at":"2026-08-01T12:45:38.686751Z","title":"Baldes, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.686751Z"},"links":{"cited_paper":"/paper/2403.05615","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:3b531aa8133f836dbfb0b02dc41aace08b115a48b4444b6d553fd4e71d231001","observation_id":"b88e38dd-f3de-4c10-b8c7-7a113c18bffb","resolution":{"observed_at":"2026-08-01T12:45:38.686751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.12554","last_updated":"2024-06-18T12:30:31Z","snapshot_observed_at":"2026-08-16T13:41:51.686412Z","submitted_at":"2024-06-18T12:30:31Z","title":"Populating secluded dark sector with ultra-relativistic bubbles","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.12554","snapshot_observed_at":"2026-08-01T12:45:38.690880Z","title":"Azatov, X","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.690880Z"},"links":{"cited_paper":"/paper/2406.12554","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:14808c6d308d9a1b051c5113ff534c52a315c51dc2c3efaeaaa87e0c4db89946","observation_id":"511a78e7-f5a8-4be1-9374-fd2275bfe7ee","resolution":{"observed_at":"2026-08-01T12:45:38.690880Z","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":"2026-08-01T12:45:38.695384Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.695384Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:1091333eb874aadd11158e65c3578682a6d130d9cc56e08dadc5c7398bb593ea","observation_id":"ae987e47-5b48-4469-aee7-a82e2d48baa9","resolution":{"observed_at":"2026-08-01T12:45:38.695384Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.00583","last_updated":"2016-10-27T10:32:32Z","snapshot_observed_at":"2026-08-14T21:45:52.817481Z","submitted_at":"2016-08-01T20:00:06Z","title":"Baryogenesis and Gravitational Waves from Runaway Bubble Collisions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.00583","snapshot_observed_at":"2026-08-01T12:45:38.699598Z","title":"Katz and A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.699598Z"},"links":{"cited_paper":"/paper/1608.00583","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:40dd2242e62cfb4822c30d5b701c386fe13923a05781a77c5e5503d49b5da041","observation_id":"b552fa7b-1e40-4447-9503-df4aff6cb08f","resolution":{"observed_at":"2026-08-01T12:45:38.699598Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.14913","last_updated":"2021-09-15T08:54:13Z","snapshot_observed_at":"2026-08-19T10:17:19.576491Z","submitted_at":"2021-06-28T18:00:49Z","title":"Baryogenesis via relativistic bubble walls","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.14913","snapshot_observed_at":"2026-08-01T12:45:38.704403Z","title":"Azatov, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.704403Z"},"links":{"cited_paper":"/paper/2106.14913","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:3ae3cc57229af719d67544cb30a942529e883074347b1faa268bb83f9c4c5c6e","observation_id":"ac95b639-0c64-4edd-b1a2-41ca315689e1","resolution":{"observed_at":"2026-08-01T12:45:38.704403Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.15602","last_updated":"2021-12-01T08:59:06Z","snapshot_observed_at":"2026-08-19T10:17:22.180009Z","submitted_at":"2021-06-29T17:44:11Z","title":"Baryogenesis via relativistic bubble expansion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.15602","snapshot_observed_at":"2026-08-01T12:45:38.709234Z","title":"Baldes, S","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.709234Z"},"links":{"cited_paper":"/paper/2106.15602","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:cb8221bcf9d0b4da1ad1d93ca433e565c12057327dfcc3cacf51238449635c16","observation_id":"0cd4bd61-5c90-467c-bd36-73d2df01ce95","resolution":{"observed_at":"2026-08-01T12:45:38.709234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.10759","last_updated":"2023-09-14T15:17:35Z","snapshot_observed_at":"2026-08-18T03:58:11.372824Z","submitted_at":"2023-05-18T06:58:01Z","title":"Bubble-assisted Leptogenesis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.10759","snapshot_observed_at":"2026-08-01T12:45:38.713464Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.713464Z"},"links":{"cited_paper":"/paper/2305.10759","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:854519357b16f3db826789e6b2ce58d1e89abaac51d5bc0615807cab290954bd","observation_id":"17b8f807-a076-4f9e-a5c8-886cb78cc6b9","resolution":{"observed_at":"2026-08-01T12:45:38.713464Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.09282","last_updated":"2024-01-23T21:06:19Z","snapshot_observed_at":"2026-08-16T14:34:38.229679Z","submitted_at":"2023-12-14T19:00:03Z","title":"Baryogenesis and Leptogenesis from Supercooled Confinement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.09282","snapshot_observed_at":"2026-08-01T12:45:38.718298Z","title":"Dichtl, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.718298Z"},"links":{"cited_paper":"/paper/2312.09282","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:5e4e0738662fc1d28988e4a31f621360b9bb76000c8f4055fb223ebd6cb28994","observation_id":"886e0c4e-ca29-4165-afdf-31ab4e781a2d","resolution":{"observed_at":"2026-08-01T12:45:38.718298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.16747","last_updated":"2024-12-04T13:13:08Z","snapshot_observed_at":"2026-08-16T13:31:40.008402Z","submitted_at":"2024-07-23T18:00:01Z","title":"Leptogenesis via Bubble Collisions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.16747","snapshot_observed_at":"2026-08-01T12:45:38.722751Z","title":"Cataldi and B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.722751Z"},"links":{"cited_paper":"/paper/2407.16747","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:a3acfb10617f59f7cae4cbc79729102d5ba1c6393a6e553baecc7771c81e823a","observation_id":"1560c5ff-0d2f-411a-bf15-e2a31a3bf0a6","resolution":{"observed_at":"2026-08-01T12:45:38.722751Z","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":"2026-08-01T12:45:38.727214Z","title":"Cataldi, K","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.727214Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:d2bdbb1fb0afde432d26ef89b9db57c11f1fa2dfcaad3b37568f7525e94c08f5","observation_id":"f313c42f-12da-438f-bd5a-d661077265f2","resolution":{"observed_at":"2026-08-01T12:45:38.727214Z","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":"2026-08-01T12:45:38.731591Z","title":"Ai, High-frequency gravitational waves from a first-order phase transitions , Phys","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.731591Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:88ac01ccad29ce1813418c142a7585715158d268d43b865aa3222a422e6789cf","observation_id":"f3a6533d-e32f-4a7b-8a8d-0dea4981a800","resolution":{"observed_at":"2026-08-01T12:45:38.731591Z","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":"2026-08-01T12:45:38.735855Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.735855Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:7c0347a04deb4c147b4915826b163ec0d1f4455febc26485b83e98d93b110bf9","observation_id":"ff81eec5-4285-4a8b-b114-283297437e63","resolution":{"observed_at":"2026-08-01T12:45:38.735855Z","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":"2026-08-01T12:45:38.740197Z","title":"Sasaki, H","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.740197Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:9f4427a347057ff4841a2d16183c3932d52322313e3bd0eabb695af6fa204e4a","observation_id":"03d84d65-fb82-4ad6-b6b5-265e8a338c54","resolution":{"observed_at":"2026-08-01T12:45:38.740197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14086","last_updated":"2022-08-30T09:06:52Z","snapshot_observed_at":"2026-08-16T16:36:01.529041Z","submitted_at":"2022-08-30T09:06:52Z","title":"Constraining first-order phase transitions with curvature perturbations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14086","snapshot_observed_at":"2026-08-01T12:45:38.744542Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.744542Z"},"links":{"cited_paper":"/paper/2208.14086","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:ad0c8bd2bc39b67fdee714fe62c7675359035d83229bccbec371d4147bc113e0","observation_id":"bc1fd3d8-e16f-4be5-aac4-e2b8d582cbc3","resolution":{"observed_at":"2026-08-01T12:45:38.744542Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.12080","last_updated":"2023-08-29T12:38:14Z","snapshot_observed_at":"2026-08-16T15:14:08.159981Z","submitted_at":"2023-07-22T13:50:06Z","title":"General relativistic bubble growth in cosmological phase transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.12080","snapshot_observed_at":"2026-08-01T12:45:38.749224Z","title":"Giombi and M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.749224Z"},"links":{"cited_paper":"/paper/2307.12080","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:f778d0eb0f8f55b974cee6b45619583138c2f5989e8e2c2e83d30390269f549a","observation_id":"67632dce-2dd8-4ee0-8b42-352c8f14288b","resolution":{"observed_at":"2026-08-01T12:45:38.749224Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.16222","last_updated":"2023-11-27T19:00:00Z","snapshot_observed_at":"2026-08-16T14:39:55.254776Z","submitted_at":"2023-11-27T19:00:00Z","title":"Finite Bubble Statistics Constrain Late Cosmological Phase Transitions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.16222","snapshot_observed_at":"2026-08-01T12:45:38.754013Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.754013Z"},"links":{"cited_paper":"/paper/2311.16222","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:247cc9a8def95cfefe59570569df42af1effd1d43a6d2e92b7c05b94f33aea95","observation_id":"90c8c3c8-fc9c-448e-93b7-c0dd94fcd89b","resolution":{"observed_at":"2026-08-01T12:45:38.754013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04158","last_updated":"2024-10-31T11:51:17Z","snapshot_observed_at":"2026-08-16T14:20:56.751756Z","submitted_at":"2024-02-06T17:15:33Z","title":"Black holes and gravitational waves from slow phase transitions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.04158","snapshot_observed_at":"2026-08-01T12:45:38.758472Z","title":"Lewicki, P","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.758472Z"},"links":{"cited_paper":"/paper/2402.04158","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:403e17975cc9ab4bf63346a6abc51c7c90af2fd0c76e9e573c03200a2fe166d5","observation_id":"f7bdc762-e651-49dd-8ced-a8dd6559df7a","resolution":{"observed_at":"2026-08-01T12:45:38.758472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13309","last_updated":"2024-02-20T19:00:00Z","snapshot_observed_at":"2026-08-16T14:16:50.413297Z","submitted_at":"2024-02-20T19:00:00Z","title":"Dark Radiation Isocurvature from Cosmological Phase Transitions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.13309","snapshot_observed_at":"2026-08-01T12:45:38.762944Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.762944Z"},"links":{"cited_paper":"/paper/2402.13309","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:859aaec2db31ac46d3115c2c8194c215d9bdbc52e84b1287a2952742a477250d","observation_id":"ddb9b24c-2392-4356-a77e-843cf2dd84cf","resolution":{"observed_at":"2026-08-01T12:45:38.762944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.06506","last_updated":"2024-08-04T01:29:13Z","snapshot_observed_at":"2026-08-16T14:02:18.488386Z","submitted_at":"2024-04-09T17:54:42Z","title":"Primordial black holes and curvature perturbations from false vacuum islands","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.06506","snapshot_observed_at":"2026-08-01T12:45:38.767364Z","title":"Cai, Y.-S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.767364Z"},"links":{"cited_paper":"/paper/2404.06506","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:af9e91ad36af1fed0c59c3618fc56c6a2f22b768b499b7d3b866bcee37f4c832","observation_id":"21501903-28ff-4a35-a53b-76dc1205cdd0","resolution":{"observed_at":"2026-08-01T12:45:38.767364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.10770","last_updated":"2025-03-28T13:12:32Z","snapshot_observed_at":"2026-08-16T13:25:14.697764Z","submitted_at":"2024-08-20T12:05:13Z","title":"Gravitational effects on fluid dynamics in cosmological first-order phase transitions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.10770","snapshot_observed_at":"2026-08-01T12:45:38.771889Z","title":"Jinno and J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.771889Z"},"links":{"cited_paper":"/paper/2408.10770","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:567121fe40a5c82f5b026ab658ea4ec94fa1abbe02ac6e19c963d93ca3e7fc65","observation_id":"567008e5-c9c0-41c0-8468-3b40a5aac5d5","resolution":{"observed_at":"2026-08-01T12:45:38.771889Z","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":"2026-08-01T12:45:38.776918Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.776918Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:3492fe2e8f2ae4b3f8742267a2569d1f479ffb66ca7d2295f93a09976fea746d","observation_id":"f64e5972-22a0-425d-89f6-71a9dc873aed","resolution":{"observed_at":"2026-08-01T12:45:38.776918Z","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":"2026-08-01T12:45:38.781089Z","title":"Greene, D","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.781089Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:045c47bdd286005b3f6cb189a0511cd2777d8bf1a85d0553f9a7320cc5a438cf","observation_id":"e500d922-3f36-41e0-a05a-dc8f142cb4d0","resolution":{"observed_at":"2026-08-01T12:45:38.781089Z","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":"2026-08-01T12:45:38.785823Z","title":"Kodama, M","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.785823Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:2bf245d6214a0bdbac3eb1f70d4bdf6760f6a46c3fc6f434d8a0f0c738a2b755","observation_id":"9dc89b8b-1f08-403d-9bba-fdc2430125f6","resolution":{"observed_at":"2026-08-01T12:45:38.785823Z","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":"2026-08-01T12:45:38.790156Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.790156Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:fbbe35f286c0f88221b0f4043e59d41b88a0b8abd22ca89b07595b62564c9532","observation_id":"cc239c08-7099-41d1-9cde-7bf0d4a41d85","resolution":{"observed_at":"2026-08-01T12:45:38.790156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.05637","last_updated":"2022-01-14T11:58:31Z","snapshot_observed_at":"2026-08-19T03:18:04.200890Z","submitted_at":"2021-06-10T10:20:25Z","title":"Primordial black hole production during first-order phase transitions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.05637","snapshot_observed_at":"2026-08-01T12:45:38.794528Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.794528Z"},"links":{"cited_paper":"/paper/2106.05637","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:e5e1e9f8179fe3019080bbdedc96c5d7628ec90bf171f7c64ca785f3771e4875","observation_id":"efbf6911-65b5-47bb-8483-1ca5e2574820","resolution":{"observed_at":"2026-08-01T12:45:38.794528Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.13099","last_updated":"2022-06-22T07:03:03Z","snapshot_observed_at":"2026-08-19T03:18:56.861120Z","submitted_at":"2021-11-25T14:27:21Z","title":"Primordial black holes as a probe of strongly first-order electroweak phase transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.13099","snapshot_observed_at":"2026-08-01T12:45:38.799218Z","title":"Hashino, S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.799218Z"},"links":{"cited_paper":"/paper/2111.13099","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:0599566b6ae4d3fad6d00ecf74f1cee65f6816ae718dfdbf4f658decc42fde44","observation_id":"5cceae01-609c-4e67-a2d0-1d5f63a90f80","resolution":{"observed_at":"2026-08-01T12:45:38.799218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.14037","last_updated":"2023-11-28T21:08:23Z","snapshot_observed_at":"2026-08-16T16:05:34.729932Z","submitted_at":"2022-12-28T18:59:58Z","title":"PBH formation from overdensities in delayed vacuum transitions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.14037","snapshot_observed_at":"2026-08-01T12:45:38.803769Z","title":"Kawana, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.803769Z"},"links":{"cited_paper":"/paper/2212.14037","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:65e53ebd0bccd86009dc6a9e82bcacfa8500743fc3ff1b61425e970650f16096","observation_id":"d10aba4e-fd34-4a02-8bec-b7a249228459","resolution":{"observed_at":"2026-08-01T12:45:38.803769Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.04924","last_updated":"2023-09-19T14:45:26Z","snapshot_observed_at":"2026-08-19T03:43:03.109245Z","submitted_at":"2023-05-08T17:59:06Z","title":"Primordial black holes from strong first-order phase transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.04924","snapshot_observed_at":"2026-08-01T12:45:38.808144Z","title":"Lewicki, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.808144Z"},"links":{"cited_paper":"/paper/2305.04924","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:a74d77053a096580c3f6894813c1b972d956167cf31f269f46038f010bb21e8c","observation_id":"e1763091-c3f9-4cb3-95b6-d73317556ff8","resolution":{"observed_at":"2026-08-01T12:45:38.808144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.04942","last_updated":"2025-03-03T19:22:02Z","snapshot_observed_at":"2026-08-16T15:34:42.017793Z","submitted_at":"2023-05-08T18:00:00Z","title":"Primordial Black Holes from Supercooled Phase Transitions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.04942","snapshot_observed_at":"2026-08-01T12:45:38.813298Z","title":"Gouttenoire and T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.813298Z"},"links":{"cited_paper":"/paper/2305.04942","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:14f759467a09be8d1f75d0791bf22a7a74ca760ae796d77c87d4aed31c27e19f","observation_id":"245c3d81-d61f-486e-92db-ea7a0d89fa15","resolution":{"observed_at":"2026-08-01T12:45:38.813298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.11639","last_updated":"2024-01-17T12:38:01Z","snapshot_observed_at":"2026-08-16T15:14:18.964264Z","submitted_at":"2023-07-21T15:10:41Z","title":"Primordial black holes as dark matter: Interferometric tests of phase transition origin","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.11639","snapshot_observed_at":"2026-08-01T12:45:38.817971Z","title":"Baldes and M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.817971Z"},"links":{"cited_paper":"/paper/2307.11639","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:940611c0a3252497bbaff6e22a2736c2b777f6e3a97253d95bf3c35ea3ff4fa3","observation_id":"711d48c5-23bd-4d47-adf5-62299d842681","resolution":{"observed_at":"2026-08-01T12:45:38.817971Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04239","last_updated":"2023-11-15T13:51:03Z","snapshot_observed_at":"2026-08-16T15:17:37.124289Z","submitted_at":"2023-07-09T17:57:20Z","title":"First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.04239","snapshot_observed_at":"2026-08-01T12:45:38.822799Z","title":"Gouttenoire, First-Order Phase Transition Interpretation of Pulsar Timing Array Signal Is Consistent with Solar-Mass Black Holes , Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.822799Z"},"links":{"cited_paper":"/paper/2307.04239","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:638de5f533f7acd68af02b69c3841f6b9e01dbbd73424e9072c81e61aef238b1","observation_id":"b457e20a-5a6a-4355-bb32-2dc7cf2cedb8","resolution":{"observed_at":"2026-08-01T12:45:38.822799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.04694","last_updated":"2024-03-22T07:40:03Z","snapshot_observed_at":"2026-08-16T15:17:23.863731Z","submitted_at":"2023-07-10T16:46:46Z","title":"Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.04694","snapshot_observed_at":"2026-08-01T12:45:38.827465Z","title":"Salvio, Supercooling in Radiative Symmetry Breaking: Theory Extensions, Gravitational Wave Detection and Primordial Black Holes , JCAP 12 (2023) 046 , [ 2307.04694]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.827465Z"},"links":{"cited_paper":"/paper/2307.04694","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:f537ae03f0ba86eebb4463389b0c0119931746210b1c99ad5d3ebec16d7a3ec6","observation_id":"0841b523-7f58-45ab-b32f-006d0e40c2bb","resolution":{"observed_at":"2026-08-01T12:45:38.827465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.13640","last_updated":"2025-03-03T19:36:15Z","snapshot_observed_at":"2026-08-17T03:20:40.518003Z","submitted_at":"2023-11-22T19:00:02Z","title":"Primordial Black Holes from Conformal Higgs","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.13640","snapshot_observed_at":"2026-08-01T12:45:38.832122Z","title":"Gouttenoire, Primordial black holes from conformal Higgs , Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.832122Z"},"links":{"cited_paper":"/paper/2311.13640","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:aa55475d9732d019145504b4348dbc203890b84ef6befcc3ca2be894cb9c9e61","observation_id":"59f72654-452a-49fd-9899-434d44acdb5e","resolution":{"observed_at":"2026-08-01T12:45:38.832122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2402.13341","last_updated":"2024-03-04T17:52:04Z","snapshot_observed_at":"2026-08-16T14:16:49.678945Z","submitted_at":"2024-02-20T19:36:19Z","title":"Revisiting formation of primordial black holes in a supercooled first-order phase transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.13341","snapshot_observed_at":"2026-08-01T12:45:38.836726Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.836726Z"},"links":{"cited_paper":"/paper/2402.13341","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:ff77c89d6ad85c5884696c254f5d268bca1e0e75fca2efdcc7b24c3ba0b387fc","observation_id":"d89c1af5-4b8c-4b26-93d8-209d9058ee90","resolution":{"observed_at":"2026-08-01T12:45:38.836726Z","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":"2026-08-01T12:45:38.841461Z","title":"Lewicki, P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.841461Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:9dc2eaeb1bc16b8f7deffd9f9cb0828aa16fc2793574bde5d6c130e9027c811e","observation_id":"7b3ebdd2-6c72-4620-9607-fdbae3952000","resolution":{"observed_at":"2026-08-01T12:45:38.841461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00646","last_updated":"2024-05-21T08:16:54Z","snapshot_observed_at":"2026-08-16T14:04:52.671957Z","submitted_at":"2024-03-31T11:20:31Z","title":"Primordial black holes from slow phase transitions: a model-building perspective","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00646","snapshot_observed_at":"2026-08-01T12:45:38.845799Z","title":"Kanemura, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.845799Z"},"links":{"cited_paper":"/paper/2404.00646","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:015f3889efedb974c561a28bee55a98763ad7f3d86053fb4f1e943c99105ea5b","observation_id":"5264e752-467e-450a-9fa4-9bcb1445b085","resolution":{"observed_at":"2026-08-01T12:45:38.845799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.07622","last_updated":"2025-02-17T03:09:52Z","snapshot_observed_at":"2026-08-16T13:44:02.180703Z","submitted_at":"2024-06-11T18:00:05Z","title":"Primordial Black Holes from First-Order Phase Transition in the xSM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.07622","snapshot_observed_at":"2026-08-01T12:45:38.850623Z","title":"Gonçalves, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.850623Z"},"links":{"cited_paper":"/paper/2406.07622","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:cd83cb05dfee5cce52e60ced50c5ad53cb6037cd9347999ba9e1e12c18abf61c","observation_id":"2b371c78-8fc1-457f-81f3-a5f0ad920c2f","resolution":{"observed_at":"2026-08-01T12:45:38.850623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.12518","last_updated":"2024-12-05T17:27:48Z","snapshot_observed_at":"2026-08-16T13:41:53.004049Z","submitted_at":"2024-06-18T11:45:51Z","title":"Primordial Black Holes and Gravitational Waves in the $U(1)_{B-L}$ Extended Inert Doublet Model: A First-Order Phase Transition Perspective","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.12518","snapshot_observed_at":"2026-08-01T12:45:38.855154Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.855154Z"},"links":{"cited_paper":"/paper/2406.12518","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:fb63cbe6c4f3712dbe0c0bd6470e0aa0682d62fe31533e429f5bb3d5fd1e5673","observation_id":"a982c04f-31f5-4ff6-9529-1d070c842d3b","resolution":{"observed_at":"2026-08-01T12:45:38.855154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.04545","last_updated":"2025-03-05T08:30:39Z","snapshot_observed_at":"2026-08-16T13:20:39.990202Z","submitted_at":"2024-09-06T18:16:30Z","title":"Gravitational waves and black holes from the phase transition in models of dynamical symmetry breaking","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.04545","snapshot_observed_at":"2026-08-01T12:45:38.859852Z","title":"Arteaga, A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.859852Z"},"links":{"cited_paper":"/paper/2409.04545","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:b9764b8d82a9527d3a228ae8fbba9b59cdd739d0c8621c6d323706b679ad5cc8","observation_id":"9710d8de-bdc3-451d-bcf4-9b894d384cee","resolution":{"observed_at":"2026-08-01T12:45:38.859852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.06889","last_updated":"2025-07-03T09:50:22Z","snapshot_observed_at":"2026-08-14T18:45:19.051663Z","submitted_at":"2024-12-09T19:00:02Z","title":"Primordial Black Holes (as Dark Matter) from the Supercooled Phase Transitions with Radiative Symmetry Breaking","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.06889","snapshot_observed_at":"2026-08-01T12:45:38.864645Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.864645Z"},"links":{"cited_paper":"/paper/2412.06889","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:002fd4aba7ae8774dc134071977afa65bf5978c99c6ba1efd8083dd6f2eca8e1","observation_id":"b2acae78-dd36-45fc-b23c-4ba5ab753d23","resolution":{"observed_at":"2026-08-01T12:45:38.864645Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.11040","last_updated":"2025-01-19T13:17:40Z","snapshot_observed_at":"2026-08-14T10:43:37.911027Z","submitted_at":"2025-01-19T13:17:40Z","title":"Super-critical primordial black hole formation via delayed first-order electroweak phase transition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.11040","snapshot_observed_at":"2026-08-01T12:45:38.869225Z","title":"Hashino, S","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.869225Z"},"links":{"cited_paper":"/paper/2501.11040","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:7ecce3118ce53314d1f8f50f152eaa039eed8478006e287f67e192922d2bb62e","observation_id":"3814d914-6be8-4716-b37f-e05f1bdbae1a","resolution":{"observed_at":"2026-08-01T12:45:38.869225Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.03588","last_updated":"2025-07-09T10:02:13Z","snapshot_observed_at":"2026-08-18T07:27:38.715195Z","submitted_at":"2025-02-05T20:09:42Z","title":"Complementary Probes of Warped Extra Dimension: Colliders, Gravitational Waves and Primordial Black Holes from Phase Transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.03588","snapshot_observed_at":"2026-08-01T12:45:38.873915Z","title":"Ghoshal, E","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.873915Z"},"links":{"cited_paper":"/paper/2502.03588","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:52112bf48a6d9219c0fb2ee3610ad1f6786d677007181596b4d6af4cfc413647","observation_id":"9561fdaa-bb8b-4877-bcff-d605f9164b92","resolution":{"observed_at":"2026-08-01T12:45:38.873915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.20166","last_updated":"2026-04-10T10:30:19Z","snapshot_observed_at":"2026-08-16T20:25:47.115312Z","submitted_at":"2025-02-27T15:04:55Z","title":"Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.20166","snapshot_observed_at":"2026-08-01T12:45:38.878438Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.878438Z"},"links":{"cited_paper":"/paper/2502.20166","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:a4e517e2fb3ee88e4feef2684a16b1cbd3a693503b9b491f38b12a6a52a3b530","observation_id":"4512bf91-7485-4102-819b-faa7e036eb1b","resolution":{"observed_at":"2026-08-01T12:45:38.878438Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.01962","last_updated":"2026-05-06T17:35:03Z","snapshot_observed_at":"2026-07-06T20:45:59.818273Z","submitted_at":"2025-03-03T19:00:01Z","title":"Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.01962","snapshot_observed_at":"2026-08-01T12:45:38.883269Z","title":"Franciolini, Y","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.883269Z"},"links":{"cited_paper":"/paper/2503.01962","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:a0d256db668247508be2f4224eda3f877226ac14430cf33743e0a94517a26938","observation_id":"1b2b8d0c-6155-4d02-8345-a9d10d463096","resolution":{"observed_at":"2026-08-01T12:45:38.883269Z","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":"2026-08-01T12:45:38.888085Z","title":"Wang, Y.-l","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.888085Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:f13fd8234b9492bdad255e737e5a6de9fd30a71c0e89d8a05adad9cd934498a1","observation_id":"18c867e4-9564-4adc-a3ac-0b65f74ea7e4","resolution":{"observed_at":"2026-08-01T12:45:38.888085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2506.15496","last_updated":"2026-05-22T14:57:53Z","snapshot_observed_at":"2026-08-19T03:49:53.868682Z","submitted_at":"2025-06-18T14:34:48Z","title":"Thermodynamical uncertainties for primordial black holes from cosmological phase transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2506.15496","snapshot_observed_at":"2026-08-01T12:45:38.892952Z","title":"Kierkla, N","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.892952Z"},"links":{"cited_paper":"/paper/2506.15496","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:cad620bac6fadaf057b101531fb650d9cb4a5aa22d05813f8ef0ec4c5c3c4c5f","observation_id":"18d20ff0-7c97-4681-a63e-4aff92b7867f","resolution":{"observed_at":"2026-08-01T12:45:38.892952Z","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":"2026-08-01T12:45:38.897612Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.897612Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:2bc8303d8cdb1b0f1a305cbea6669386f517fef107401ffcf81d79f2bf47e4c2","observation_id":"e4f1fdd1-5282-4f63-9fdb-a439ed698911","resolution":{"observed_at":"2026-08-01T12:45:38.897612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.14412","last_updated":"2026-07-03T09:56:53Z","snapshot_observed_at":"2026-08-12T16:35:18.840084Z","submitted_at":"2026-01-20T19:16:41Z","title":"How large are curvature perturbations from slow first-order phase transitions? A gauge-invariant analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.14412","snapshot_observed_at":"2026-08-01T12:45:38.903122Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.903122Z"},"links":{"cited_paper":"/paper/2601.14412","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:34f4502e6ad079c6e0a7047c2153940f8ebb01be737b3c9b73ee26095ee3f6da","observation_id":"8017b042-1483-4f01-94a4-d148475bf655","resolution":{"observed_at":"2026-08-01T12:45:38.903122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2601.21878","last_updated":"2026-05-26T13:59:19Z","snapshot_observed_at":"2026-08-12T16:29:48.484004Z","submitted_at":"2026-01-29T15:45:48Z","title":"Numerical simulations of primordial black hole formation via delayed first-order phase transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2601.21878","snapshot_observed_at":"2026-08-01T12:45:38.908037Z","title":"Ning, X.-X","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.908037Z"},"links":{"cited_paper":"/paper/2601.21878","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:7f742a9f8f50fd619065d82e27830f190a09411461d30554664e0aa86df17b2d","observation_id":"2a8d3075-2800-495e-9757-80656112f7d3","resolution":{"observed_at":"2026-08-01T12:45:38.908037Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2605.11332","last_updated":"2026-05-21T02:44:30Z","snapshot_observed_at":"2026-08-10T22:03:20.681344Z","submitted_at":"2026-05-11T23:34:38Z","title":"Reviving primordial black hole formation in slow first-order phase transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.11332","snapshot_observed_at":"2026-08-01T12:45:38.913113Z","title":"Ai and K.-P","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.913113Z"},"links":{"cited_paper":"/paper/2605.11332","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:97197ed939e18b85ab581b983eec98815b5d165e71bf638cd1aa25cfa2916a62","observation_id":"74577814-b31d-496f-9971-bd261348ccbf","resolution":{"observed_at":"2026-08-01T12:45:38.913113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.09482","last_updated":"2026-06-08T13:39:21Z","snapshot_observed_at":"2026-08-01T15:02:27.551064Z","submitted_at":"2026-06-08T13:39:21Z","title":"Primordial Black Holes from Slow Phase Transitions with Delayed Reheating: A Peak-Theory Approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.09482","snapshot_observed_at":"2026-08-01T12:45:38.918138Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.918138Z"},"links":{"cited_paper":"/paper/2606.09482","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:9e92cd38331291b605056f34bb03166e7fa4b4059e43ffb34fc075b9a1852f1c","observation_id":"326431e5-afb1-40c7-8678-c38fd0c30388","resolution":{"observed_at":"2026-08-01T12:45:38.918138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.06901","last_updated":"2024-02-23T13:38:30Z","snapshot_observed_at":"2026-08-19T03:18:28.848887Z","submitted_at":"2023-10-10T18:00:50Z","title":"Super-slow phase transition catalyzed by BHs and the birth of baby BHs","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.06901","snapshot_observed_at":"2026-08-01T12:45:38.923252Z","title":"Jinno, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.923252Z"},"links":{"cited_paper":"/paper/2310.06901","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:052571dabeb20aa61e4a0a7b69193e79a6ef3c8344a80a618b3f9b1ce0d19565","observation_id":"b6de498f-91c9-46bb-962c-de2acb8a42c5","resolution":{"observed_at":"2026-08-01T12:45:38.923252Z","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":"2026-08-01T12:45:38.928490Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.928490Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:638e40ddc98dffee6acbef5b0d8bfa697471b451c012ee620779ea25716e84c7","observation_id":"129e169b-53bc-49ce-bfcb-cda1feac6421","resolution":{"observed_at":"2026-08-01T12:45:38.928490Z","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":"2026-08-01T12:45:38.932953Z","title":null,"venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.932953Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:127b489089132568a3871b27056631a8a5ac5b67c9c41c32cbb73decff4b704d","observation_id":"51dcda7d-a434-4db4-8278-246299eb8714","resolution":{"observed_at":"2026-08-01T12:45:38.932953Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.02291","last_updated":"2025-07-10T02:47:30Z","snapshot_observed_at":"2026-08-15T23:08:50.377919Z","submitted_at":"2025-02-04T12:59:54Z","title":"Primordial Black Hole Formation via Inverted Bubble Collapse","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.02291","snapshot_observed_at":"2026-08-01T12:45:38.937515Z","title":"Murai, K","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.937515Z"},"links":{"cited_paper":"/paper/2502.02291","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:81146633e0e8e35583349c468a4d1d43f2180efde089652d206a339b425ad7aa","observation_id":"5f318dad-c797-448f-92fd-5f8a25eee13c","resolution":{"observed_at":"2026-08-01T12:45:38.937515Z","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":"2026-08-01T12:45:38.942599Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.942599Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:dd0907a9b870d8efffe60d39bea122b4e575143a689b6e82efa37688dea5903e","observation_id":"582fa0c7-b64e-4359-85eb-e3ac1de24918","resolution":{"observed_at":"2026-08-01T12:45:38.942599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.02817","last_updated":"2021-06-09T17:12:29Z","snapshot_observed_at":"2026-08-16T19:00:53.079575Z","submitted_at":"2020-12-04T19:47:06Z","title":"Examining the end of inflation with primordial black holes mass distribution and gravitational waves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.02817","snapshot_observed_at":"2026-08-01T12:45:38.947245Z","title":"Ashoorioon, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.947245Z"},"links":{"cited_paper":"/paper/2012.02817","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:38d06612832f4e5cc61d4d68af20e947b9b387580aa0617d161903d21ade5616","observation_id":"e752d30c-a8c2-4911-9a81-515021b05ba5","resolution":{"observed_at":"2026-08-01T12:45:38.947245Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.04271","last_updated":"2024-11-19T12:21:30Z","snapshot_observed_at":"2026-08-17T08:48:17.268597Z","submitted_at":"2021-10-08T17:33:54Z","title":"Primordial black holes from bubble collisions during a first-order phase transition","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.04271","snapshot_observed_at":"2026-08-01T12:45:38.952137Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.952137Z"},"links":{"cited_paper":"/paper/2110.04271","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:2573b050c7c97c53cca1fed07d1e43c69de89a6bb8671c6bb119bdd42b6552e4","observation_id":"d8752ffb-5bd2-4e96-b270-5d6077d24010","resolution":{"observed_at":"2026-08-01T12:45:38.952137Z","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":"2026-08-01T12:45:38.956646Z","title":"Crawford and D","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.956646Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:57f451bdb1d09db0a288e9d4c2138010d712f27a014691ad049e1e915a031714","observation_id":"126024c1-47ce-47a5-b2ec-63585857c6ae","resolution":{"observed_at":"2026-08-01T12:45:38.956646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.02840","last_updated":"2022-04-03T18:22:09Z","snapshot_observed_at":"2026-08-16T18:26:32.364085Z","submitted_at":"2021-05-06T17:32:48Z","title":"Dark Matter as dark dwarfs and other macroscopic objects: multiverse relics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.02840","snapshot_observed_at":"2026-08-01T12:45:38.960959Z","title":"Gross, G","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.960959Z"},"links":{"cited_paper":"/paper/2105.02840","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:7724644f9db6a4c92a4fde9757d60c23252b4034220fc5e47c8222a184aba434","observation_id":"e1e8272c-8f45-40f1-8b8e-34c1919574ce","resolution":{"observed_at":"2026-08-01T12:45:38.960959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.00005","last_updated":"2025-08-18T19:56:10Z","snapshot_observed_at":"2026-08-19T12:50:07.968803Z","submitted_at":"2021-09-30T18:00:00Z","title":"Detailed Calculation of Primordial Black Hole Formation During First-Order Cosmological Phase Transitions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.00005","snapshot_observed_at":"2026-08-01T12:45:38.965756Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.965756Z"},"links":{"cited_paper":"/paper/2110.00005","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:b64afecc6e307e2a1acfc38a68764b8aa00ce785a77be12555c7ab7847322b9d","observation_id":"ad8df484-8568-444b-ab00-37a68241609a","resolution":{"observed_at":"2026-08-01T12:45:38.965756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.00111","last_updated":"2021-11-21T23:38:00Z","snapshot_observed_at":"2026-08-19T03:18:48.396117Z","submitted_at":"2021-05-31T21:36:22Z","title":"Primordial black holes from a cosmic phase transition: The collapse of Fermi-balls","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.00111","snapshot_observed_at":"2026-08-01T12:45:38.970816Z","title":"Kawana and K.-P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.970816Z"},"links":{"cited_paper":"/paper/2106.00111","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:7d26cbc7c5787bdc4cc2e52a48888e03bd3f5de90ea1ff1e6e4995a8303fa344","observation_id":"7df1dbe7-d823-4599-bbf5-e7bd5792652e","resolution":{"observed_at":"2026-08-01T12:45:38.970816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.07243","last_updated":"2022-06-10T22:24:36Z","snapshot_observed_at":"2026-08-16T17:27:31.593974Z","submitted_at":"2022-01-18T19:00:01Z","title":"Primordial black holes from an electroweak phase transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.07243","snapshot_observed_at":"2026-08-01T12:45:38.975323Z","title":"Huang and K.-P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.975323Z"},"links":{"cited_paper":"/paper/2201.07243","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:9264f6c235f8911ab0d3cd2d065e302645241ce1a7de0b734eaa0d78d59ce66a","observation_id":"814a20b5-b50e-4ab4-8a01-cd0d1c905b5c","resolution":{"observed_at":"2026-08-01T12:45:38.975323Z","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":"2026-08-01T12:45:38.979921Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.979921Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:1de034524a4d8d8b54694417ec9a67809814a96de1286d84686480e1503c292a","observation_id":"af25a6e0-9d99-4cb3-83ad-20d0ea1baf82","resolution":{"observed_at":"2026-08-01T12:45:38.979921Z","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":"2026-08-01T12:45:38.984273Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.984273Z"},"links":{"citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:4b2c7bc3125c1d0a8346875977e087d0eea155a1c2af275434c8ffc3b402074e","observation_id":"c52a5ec3-3aef-4f8f-a219-4b3fecf1a2e3","resolution":{"observed_at":"2026-08-01T12:45:38.984273Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9507429","last_updated":"1995-07-26T23:11:22Z","snapshot_observed_at":"2026-08-12T12:15:08.935850Z","submitted_at":"1995-07-26T23:11:22Z","title":"Magnetic Fields Produced by Phase Transition Bubbles in the Electroweak Phase Transition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9507429","snapshot_observed_at":"2026-08-01T12:45:38.988628Z","title":null,"venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-01T12:45:38.988628Z"},"links":{"cited_paper":"/paper/hep-ph/9507429","citing_paper":"/paper/2607.19469"},"observation_digest":"sha256:f9d4a34e01a6910a7c9e712c37eb6c19c3463e694b6be90dba0e150e9462ba04","observation_id":"d7f8090f-4f30-4d1a-8f1c-7d699e95bdba","resolution":{"observed_at":"2026-08-01T12:45:38.988628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.19469","last_updated":"2026-07-21T18:00:02Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-17T19:29:30.238726Z","submitted_at":"2026-07-21T18:00:02Z","title":"Can the universe be matter-dominated after a supercooled first-order phase transition?"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":100,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":206},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 100 of 206 outbound references and 1 inbound Pith citation observation for arXiv:2607.19469."}