{"as_of":"2026-08-08T09:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d1b3135146ac3e3444eb156898398ea8fc3cf764f9d663623918205154f62fb1","coverage":[{"denominator":59,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":59,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T20:12:32.858554Z","state":"measured"},{"denominator":62,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":62,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T20:35:54.879775Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T12:48:11.582981Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.03610","snapshot_observed_at":"2026-08-03T20:35:54.879775Z","title":"Gonzalez Quaglia, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.19610","last_updated":"2025-12-01T15:35:41Z","snapshot_observed_at":"2026-08-03T20:35:49.631218Z","submitted_at":"2025-11-24T19:00:04Z","title":"Fibre Inflation Meets Quintessence: Implications of Perturbative Stabilisation","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-03T20:35:54.879775Z"},"links":{"cited_paper":"/paper/2507.03610","citing_paper":"/paper/2511.19610"},"observation_digest":"sha256:bfb943d4c44896cf1e8f45be4dd01ee71c0ad1b7cb744cfd4eba2c31bf980fc8","observation_id":"a3b58280-fed3-4403-bfc4-6dea962484e6","resolution":{"observed_at":"2026-08-03T20:35:54.879775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2507.03610","snapshot_observed_at":"2026-08-02T19:14:20.487673Z","title":"Gonzalez Quaglia, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2603.03204","last_updated":"2026-06-24T10:11:04Z","snapshot_observed_at":"2026-08-07T18:13:08.430083Z","submitted_at":"2026-03-03T17:57:50Z","title":"Ultra slow-turn inflation","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-02T19:14:20.487673Z"},"links":{"cited_paper":"/paper/2507.03610","citing_paper":"/paper/2603.03204"},"observation_digest":"sha256:5cc139bf3c71165c4b026148374f08b6a9a3480145ecae0c72261d5b1b530a12","observation_id":"db68b1de-2948-460a-a1b7-f818fc54393b","resolution":{"observed_at":"2026-08-02T19:14:20.487673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"cited_work":{"arxiv_id":"2507.03610","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2507.03610","snapshot_observed_at":"2026-07-03T12:48:11.582981Z","title":"Gonzalez Quaglia, M","venue":null,"work_id":"fa39882d-ad20-40c4-b672-99eca577e0d6","year":null},"citing_paper":{"arxiv_id":"2606.12549","last_updated":"2026-06-10T18:01:01Z","snapshot_observed_at":"2026-07-06T23:51:27.152983Z","submitted_at":"2026-06-10T18:01:01Z","title":"Tachyonic Encore: A universal shift of inflationary observables","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-27T08:46:10.099222Z"},"links":{"cited_paper":"/paper/2507.03610","citing_paper":"/paper/2606.12549"},"observation_digest":"sha256:ab2d44a81e11e197a78d68a2c7064697f3411cbbd0652d7a904639cf5a3330a7","observation_id":"dcd7e251-26f6-45ab-9151-61a15dc28da3","resolution":{"observed_at":"2026-07-03T12:48:11.584419Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.03610/citation-record","integrity":"/paper/2507.03610/integrity","json":"/paper/2507.03610/citation-record.json","paper":"/paper/2507.03610"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:12:33.501469Z","title":null,"venue":null,"work_id":"c39a3b1d-36a5-4255-8077-c6f2b0ae8351","year":1981},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.512035Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:e4542ef4023a3f83b6ad8aa63567e57434658f1651f9106e950aafee77f29c72","observation_id":"7c674012-3e72-4ac3-b401-8b8a3b03fdb1","resolution":{"observed_at":"2026-08-06T20:12:33.504647Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:12:33.491802Z","title":null,"venue":null,"work_id":"c02b283b-c2d9-4779-9480-c77b0d09add0","year":1984},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.606921Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:c31de9200f6c7c1e6ae5644d308842cc636c31eb62f03ae4e3f6609dde95ea5d","observation_id":"74061cd5-50ae-475b-96d1-43fc07a4895c","resolution":{"observed_at":"2026-08-06T20:12:33.495216Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9807278","last_updated":"1999-03-16T13:17:32Z","snapshot_observed_at":"2026-07-07T04:29:58.562230Z","submitted_at":"1998-07-07T14:37:00Z","title":"Particle Physics Models of Inflation and the Cosmological Density Perturbation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9807278","snapshot_observed_at":"2026-08-06T20:12:32.654954Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.654954Z"},"links":{"cited_paper":"/paper/hep-ph/9807278","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:3c45061cc27b2ee6e5b11d38deb0aa17a7a46b8b0d4b56e638500aae45a6e712","observation_id":"76af84c4-7268-466d-a548-f0d14e6177c2","resolution":{"observed_at":"2026-08-06T20:12:32.654954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:12:33.481582Z","title":null,"venue":null,"work_id":"24100d66-92c0-477b-86f9-a9394751090b","year":1983},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.699218Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:15fbe59738aea63a84cdadab5ba20d7a07c0e5db04078c0d34cf4d2fb8fb9702","observation_id":"63e0ebe3-c3d2-4808-939e-fdf7066265f0","resolution":{"observed_at":"2026-08-06T20:12:33.485382Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9307002","last_updated":"1993-09-27T03:53:11Z","snapshot_observed_at":"2026-08-06T13:42:44.135417Z","submitted_at":"1993-07-01T23:39:12Z","title":"Hybrid Inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9307002","snapshot_observed_at":"2026-08-06T20:12:32.702597Z","title":null,"venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.702597Z"},"links":{"cited_paper":"/paper/astro-ph/9307002","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:ebe9f0cf757f4cfbe45556aee1dabfedae6c382b7a7e1d703c1147c77d74ddd4","observation_id":"9f2ba670-de4b-46f8-95cc-cb1f50bacaf6","resolution":{"observed_at":"2026-08-06T20:12:32.702597Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0401139","last_updated":"2004-01-19T18:39:36Z","snapshot_observed_at":"2026-08-02T14:33:42.178567Z","submitted_at":"2004-01-19T18:39:36Z","title":"Warm inflation solution to the eta-problem","version":1},"cited_work":{"arxiv_id":"hep-ph/0401139","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0401139","snapshot_observed_at":"2026-08-06T20:12:33.418437Z","title":"Warm inflation solution to the eta-problem","venue":"hep-ph","work_id":"1658a63e-6fe7-4efd-81e1-ddb79d61ddfc","year":2004},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.705756Z"},"links":{"cited_paper":"/paper/hep-ph/0401139","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:00007dc0cebe63e8b4fa0d191366a03deb6c9608bb6c99dc6fd87eca48d84752","observation_id":"a98938a8-ee1f-4fa1-a5a7-811ea3acc957","resolution":{"observed_at":"2026-08-06T20:12:33.421901Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0902.1798","last_updated":"2009-10-09T04:12:57Z","snapshot_observed_at":"2026-07-06T01:50:52.765254Z","submitted_at":"2009-02-11T14:05:01Z","title":"Circumventing the eta problem in building an inflationary model in string theory","version":3},"cited_work":{"arxiv_id":"0902.1798","doi":null,"metadata_source":"pith","pith_arxiv_id":"0902.1798","snapshot_observed_at":"2026-08-06T20:12:33.403898Z","title":"Circumventing the eta problem in building an inflationary model in string theory","venue":"hep-th","work_id":"acff445f-4ce1-4ddc-9b03-a120f77a6217","year":2009},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.709273Z"},"links":{"cited_paper":"/paper/0902.1798","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:6d4ae1ced19659f02b5c0478129a53481d15fe6240b9571d1ffee5aa235cbfde","observation_id":"3c996f39-02df-43ff-89ab-609b7b96d76b","resolution":{"observed_at":"2026-08-06T20:12:33.407750Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1112.2272","last_updated":"2011-12-10T12:18:15Z","snapshot_observed_at":"2026-07-06T02:39:09.649574Z","submitted_at":"2011-12-10T12:18:15Z","title":"1/N Resolution to Inflationary eta-Problem","version":1},"cited_work":{"arxiv_id":"1112.2272","doi":null,"metadata_source":"pith","pith_arxiv_id":"1112.2272","snapshot_observed_at":"2026-08-06T20:12:33.388993Z","title":"1/N Resolution to Inflationary eta-Problem","venue":"hep-th","work_id":"26417e74-699b-4164-a99c-7dd19f65a276","year":2011},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.712266Z"},"links":{"cited_paper":"/paper/1112.2272","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:b67ec0604c9d0655092dbc7c23a5426d9d93ec94977351a0a83d6d63e73f4015","observation_id":"9de01a22-ca34-4a3e-8e23-956f360716e1","resolution":{"observed_at":"2026-08-06T20:12:33.393173Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:12:33.472292Z","title":"Freese, J","venue":null,"work_id":"42a29ecf-1dfc-4ea5-be81-6530fb128886","year":1990},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.715303Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:0bc2feacbf19ca198415618fb482caf0078d6c5d23c1f046c59f04675fb724c0","observation_id":"9ab7a142-15db-42af-8c03-76f11736e6fb","resolution":{"observed_at":"2026-08-06T20:12:33.475950Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9207245","last_updated":"1992-07-17T09:48:42Z","snapshot_observed_at":"2026-07-07T04:14:26.763884Z","submitted_at":"1992-07-17T09:48:42Z","title":"Natural Inflation: Particle Physics Models, Power Law Spectra for Large Scale Structure, and Constraints from COBE","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9207245","snapshot_observed_at":"2026-08-06T20:12:32.718027Z","title":null,"venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.718027Z"},"links":{"cited_paper":"/paper/hep-ph/9207245","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:99678207f9da7790cf49cd07055f6857d5693f6bbbdc4238f6a489a6805c91ea","observation_id":"d5f71b58-62f2-4533-a2b0-90994e5b657c","resolution":{"observed_at":"2026-08-06T20:12:32.718027Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.05203","last_updated":"2024-10-10T17:41:57Z","snapshot_observed_at":"2026-07-06T18:58:56.504337Z","submitted_at":"2024-08-09T17:49:16Z","title":"$SL(2,\\mathbb{Z})$ Cosmological Attractors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.05203","snapshot_observed_at":"2026-08-06T20:12:32.720969Z","title":"Kallosh and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.720969Z"},"links":{"cited_paper":"/paper/2408.05203","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:dc4cc260898bf2e94d6984085a21134f47c9a768e6a1c258a3a21c94842b8076","observation_id":"8b2e49f3-c3a1-4dc8-8050-0f146aaae036","resolution":{"observed_at":"2026-08-06T20:12:32.720969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.07552","last_updated":"2024-11-12T05:00:31Z","snapshot_observed_at":"2026-07-06T19:48:54.023688Z","submitted_at":"2024-11-12T05:00:31Z","title":"Landscape of Modular Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.07552","snapshot_observed_at":"2026-08-06T20:12:32.723538Z","title":"Kallosh and A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.723538Z"},"links":{"cited_paper":"/paper/2411.07552","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:3476734cea0304580625620468db33fab294d4128496f2dc2046239406bc704e","observation_id":"e2e74f20-9edd-46d8-85a7-e2d30c89228f","resolution":{"observed_at":"2026-08-06T20:12:32.723538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.19324","last_updated":"2025-06-19T15:57:59Z","snapshot_observed_at":"2026-07-30T18:39:00.212308Z","submitted_at":"2024-12-26T18:53:57Z","title":"Double Exponents in $SL(2,\\mathbb{Z})$ Cosmology","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.19324","snapshot_observed_at":"2026-08-06T20:12:32.726376Z","title":"Kallosh and A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.726376Z"},"links":{"cited_paper":"/paper/2412.19324","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:e3af6599a48608ffb3d9ebd08c10f65b21f7808ec053ed1d0ab84106ea343de0","observation_id":"49d82e45-0d82-4497-a64c-16fb0f7e46a8","resolution":{"observed_at":"2026-08-06T20:12:32.726376Z","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":"2026-08-06T20:12:32.729194Z","title":"Ding, S.-Y","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.729194Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:92eb0539b5f5dc906b1c36b77692b7f45d771cb7afb5e4826209559bb40c3d5e","observation_id":"9d57431e-6da4-4797-84a9-d5c2319db6f3","resolution":{"observed_at":"2026-08-06T20:12:32.729194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08467","last_updated":"2025-08-07T21:02:45Z","snapshot_observed_at":"2026-07-06T19:49:38.886114Z","submitted_at":"2024-11-13T09:37:35Z","title":"Inflationary constraints on the moduli-dependent species scale in modular invariant theories","version":2},"cited_work":{"arxiv_id":"2411.08467","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08467","snapshot_observed_at":"2026-08-06T20:12:33.238039Z","title":"Inflationary constraints on the moduli-dependent species scale in modular invariant theories","venue":"hep-th","work_id":"60a78541-b376-4eba-b534-73802df864b9","year":2024},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.731873Z"},"links":{"cited_paper":"/paper/2411.08467","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:6bd52d5bc343d5380f0a9b74a326588939350dc5fa9e880517a51d9808315eed","observation_id":"fc7237ac-a4d1-4d7a-8e75-b4f9324dc123","resolution":{"observed_at":"2026-08-06T20:12:33.241522Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14904","last_updated":"2025-06-09T17:56:11Z","snapshot_observed_at":"2026-08-07T16:53:07.434571Z","submitted_at":"2025-03-19T05:10:21Z","title":"Axion Stabilization in Modular Cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14904","snapshot_observed_at":"2026-08-06T20:12:32.734744Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.734744Z"},"links":{"cited_paper":"/paper/2503.14904","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:da709b030819821d88ecd40f4645a66c5380f97e9e704ccff58ee5bad2a69b13","observation_id":"95333df5-0580-4da2-b0fd-d6a313a548e6","resolution":{"observed_at":"2026-08-06T20:12:32.734744Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.01622","last_updated":"2025-08-05T07:18:47Z","snapshot_observed_at":"2026-08-07T22:25:13.410880Z","submitted_at":"2025-04-02T11:30:09Z","title":"Higgs-Modular Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.01622","snapshot_observed_at":"2026-08-06T20:12:32.737595Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.737595Z"},"links":{"cited_paper":"/paper/2504.01622","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:77c25cbdb13b59ddd847f35d144229e1affb7eeda9cbf527bfd4eea0f8acb614","observation_id":"f3e615c5-37e8-4df3-b2d1-5a0a10aeeda3","resolution":{"observed_at":"2026-08-06T20:12:32.737595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.5220","last_updated":"2013-09-08T21:28:06Z","snapshot_observed_at":"2026-07-06T03:16:29.883839Z","submitted_at":"2013-06-21T19:43:00Z","title":"Universality Class in Conformal Inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.5220","snapshot_observed_at":"2026-08-06T20:12:32.740872Z","title":"Kallosh and A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.740872Z"},"links":{"cited_paper":"/paper/1306.5220","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:f5f44c1faf388235a5eb606f47fbca1c4bfc08c87be2060415380c10aba31c92","observation_id":"34ef721a-228c-47d3-909d-fb1a4308c654","resolution":{"observed_at":"2026-08-06T20:12:32.740872Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.1285","last_updated":"2013-12-23T15:52:46Z","snapshot_observed_at":"2026-07-06T03:22:17.104475Z","submitted_at":"2013-09-05T09:07:38Z","title":"Universality classes of inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.1285","snapshot_observed_at":"2026-08-06T20:12:32.743934Z","title":"Roest, Universality classes of inflation , JCAP 01 (2014) 007 [ 1309.1285]","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.743934Z"},"links":{"cited_paper":"/paper/1309.1285","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:5fbc117f99bba5c76af891ec21b50ff3c1b1331ad9eca4cdeeacd940ef2e5a73","observation_id":"030344ff-85d7-4735-8c85-160da9b6c8fc","resolution":{"observed_at":"2026-08-06T20:12:32.743934Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.7696","last_updated":"2013-10-21T02:53:26Z","snapshot_observed_at":"2026-08-07T13:43:38.619352Z","submitted_at":"2013-07-29T19:38:41Z","title":"Minimal Supergravity Models of Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.7696","snapshot_observed_at":"2026-08-06T20:12:32.746958Z","title":"Ferrara, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.746958Z"},"links":{"cited_paper":"/paper/1307.7696","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:8398978b34b005f91e951ebc29dd7f44488188945bcaf05559505267561a1503","observation_id":"34c6b01e-eed3-4e94-8d58-8725fcc65fc2","resolution":{"observed_at":"2026-08-06T20:12:32.746958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.7938","last_updated":"2013-09-08T21:21:02Z","snapshot_observed_at":"2026-07-06T03:19:30.663280Z","submitted_at":"2013-07-30T12:25:18Z","title":"Non-minimal Inflationary Attractors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.7938","snapshot_observed_at":"2026-08-06T20:12:32.749712Z","title":"Kallosh and A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.749712Z"},"links":{"cited_paper":"/paper/1307.7938","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:c8bbdaeba0e415f6ae3f5cdb316c9e9d00fbf68e85c6a4ecc03eec4ebb852e44","observation_id":"23069b3a-ff09-44ca-b0bd-157c6c7c463d","resolution":{"observed_at":"2026-08-06T20:12:32.749712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.2015","last_updated":"2013-09-08T22:38:32Z","snapshot_observed_at":"2026-07-06T03:22:30.095986Z","submitted_at":"2013-09-08T22:38:32Z","title":"Multi-field Conformal Cosmological Attractors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.2015","snapshot_observed_at":"2026-08-06T20:12:32.752774Z","title":"Kallosh and A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.752774Z"},"links":{"cited_paper":"/paper/1309.2015","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:0c32c1589424d0d24535a6b867ab5cabbafd46cbeed03fe2c94b0b98c2dff1fc","observation_id":"49146aab-9ad1-43e0-a601-67ee05a74709","resolution":{"observed_at":"2026-08-06T20:12:32.752774Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.0472","last_updated":"2013-11-03T14:35:55Z","snapshot_observed_at":"2026-08-01T16:33:36.867806Z","submitted_at":"2013-11-03T14:35:55Z","title":"Superconformal Inflationary $\\alpha$-Attractors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.0472","snapshot_observed_at":"2026-08-06T20:12:32.755724Z","title":"Kallosh, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.755724Z"},"links":{"cited_paper":"/paper/1311.0472","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:db148c0584077d7f83f8e01a10f714b77d428f83b6bd8a170aeb85bd242654aa","observation_id":"270866db-8908-43e6-b439-b1307f6ace76","resolution":{"observed_at":"2026-08-06T20:12:32.755724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1310.3950","last_updated":"2014-03-11T19:27:32Z","snapshot_observed_at":"2026-08-05T16:17:42.867599Z","submitted_at":"2013-10-15T08:16:35Z","title":"A universal attractor for inflation at strong coupling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1310.3950","snapshot_observed_at":"2026-08-06T20:12:32.758505Z","title":"Kallosh, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.758505Z"},"links":{"cited_paper":"/paper/1310.3950","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:c1c74913ded764b4000e7bc21a2e0c9787f70105dba7a3ceba076a6263bd9288","observation_id":"4aaf67b9-0f99-4717-b1bf-810bce856b8d","resolution":{"observed_at":"2026-08-06T20:12:32.758505Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1403.2932","last_updated":"2014-03-12T13:47:28Z","snapshot_observed_at":"2026-07-06T03:38:16.525969Z","submitted_at":"2014-03-12T13:47:28Z","title":"Cosmological Attractor Models and Higher Curvature Supergravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1403.2932","snapshot_observed_at":"2026-08-06T20:12:32.761312Z","title":"Cecotti and R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.761312Z"},"links":{"cited_paper":"/paper/1403.2932","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:486b0434c7cc03c592ee4b3d1d0de70402be0a73dc99409d1c0a07dd9aa5ffe1","observation_id":"1c127177-eb29-4fcf-a472-a49f0f6d9e69","resolution":{"observed_at":"2026-08-06T20:12:32.761312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.3646","last_updated":"2014-08-11T09:20:08Z","snapshot_observed_at":"2026-07-06T03:43:43.427464Z","submitted_at":"2014-05-14T19:51:46Z","title":"Large Field Inflation and Double $\\alpha$-Attractors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.3646","snapshot_observed_at":"2026-08-06T20:12:32.764471Z","title":"Kallosh, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.764471Z"},"links":{"cited_paper":"/paper/1405.3646","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:8e457a2f6f2fdeb950445790f80870c39fb7795d958b2a8205294bc1bb0d6ed7","observation_id":"2584f8c4-f969-4b4e-8ecc-934a68f69d38","resolution":{"observed_at":"2026-08-06T20:12:32.764471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.4471","last_updated":"2014-09-01T11:40:36Z","snapshot_observed_at":"2026-07-06T03:49:13.703108Z","submitted_at":"2014-07-16T20:00:28Z","title":"The double attractor behavior of induced inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.4471","snapshot_observed_at":"2026-08-06T20:12:32.767143Z","title":"Kallosh, A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.767143Z"},"links":{"cited_paper":"/paper/1407.4471","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:20e2734490d0d685b858be3403a51c8b4c2417c46bd36d1ced386d490b0e0951","observation_id":"ebf3b46a-d0f8-4a0e-9e03-7abd56127c44","resolution":{"observed_at":"2026-08-06T20:12:32.767143Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.3797","last_updated":"2015-02-02T23:11:54Z","snapshot_observed_at":"2026-07-06T04:03:20.231427Z","submitted_at":"2014-12-11T20:59:25Z","title":"The Unity of Cosmological Attractors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.3797","snapshot_observed_at":"2026-08-06T20:12:32.769948Z","title":"Galante, R","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.769948Z"},"links":{"cited_paper":"/paper/1412.3797","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:6e302bb3d535a2b1995e1c13ea3ce07e375341aca9ce301ff6d27b429c397eb8","observation_id":"fdd11f4c-5407-486d-9085-d0d19fa14780","resolution":{"observed_at":"2026-08-06T20:12:32.769948Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.01708","last_updated":"2015-07-03T19:22:22Z","snapshot_observed_at":"2026-08-01T00:02:08.850893Z","submitted_at":"2015-06-04T19:58:08Z","title":"$\\alpha $-Attractors: Planck, LHC and Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.01708","snapshot_observed_at":"2026-08-06T20:12:32.772827Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.772827Z"},"links":{"cited_paper":"/paper/1506.01708","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:bc4b288d0b5189d64cbc9bcfcd60da7455e7bad9e0676dfcbfc32edf62663dc8","observation_id":"bd73ce33-d69c-425f-be1a-5adb25f5f6cd","resolution":{"observed_at":"2026-08-06T20:12:32.772827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.00936","last_updated":"2015-07-17T17:56:02Z","snapshot_observed_at":"2026-07-06T04:19:40.901517Z","submitted_at":"2015-06-02T16:05:56Z","title":"Cosmological Attractors and Initial Conditions for Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.00936","snapshot_observed_at":"2026-08-06T20:12:32.775703Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.775703Z"},"links":{"cited_paper":"/paper/1506.00936","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:8c6443f2e551a81e58db6809e151f0de19f39b61c379a10af550d5db20772714","observation_id":"046e5c03-a44f-47d6-a2a9-9836eed8188f","resolution":{"observed_at":"2026-08-06T20:12:32.775703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.00546","last_updated":"2015-12-02T02:33:34Z","snapshot_observed_at":"2026-08-03T03:44:10.064390Z","submitted_at":"2015-12-02T02:33:34Z","title":"Inflatino-less Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.00546","snapshot_observed_at":"2026-08-06T20:12:32.778319Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.778319Z"},"links":{"cited_paper":"/paper/1512.00546","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:b7c162c1f26cb5a959f0e6eaec13ce64728e54957d859a563554b1214399d38c","observation_id":"2719b800-9c8c-449d-869f-1cf6f47ee451","resolution":{"observed_at":"2026-08-06T20:12:32.778319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08854","last_updated":"2016-11-18T21:29:13Z","snapshot_observed_at":"2026-07-06T05:05:22.910483Z","submitted_at":"2016-07-29T15:47:16Z","title":"Sneutrino Inflation with $\\alpha$-attractors","version":2},"cited_work":{"arxiv_id":"1607.08854","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.08854","snapshot_observed_at":"2026-08-06T20:12:33.087193Z","title":"Sneutrino Inflation with $\\alpha$-attractors","venue":"hep-th","work_id":"f920cedb-24e8-4c0c-a2ce-4379e7fcc398","year":2016},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.781033Z"},"links":{"cited_paper":"/paper/1607.08854","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:461e4743bb1210902321752de50bc6107c671359247774cc7dc104c1c75b21be","observation_id":"5ecdfa5a-f706-4491-b315-d20fbc3fb84d","resolution":{"observed_at":"2026-08-06T20:12:33.091966Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.02544","last_updated":"2025-06-07T13:41:10Z","snapshot_observed_at":"2026-07-06T20:01:01.384985Z","submitted_at":"2024-12-03T16:36:16Z","title":"Testing inflation on all scales: a case study with $\\alpha$-attractors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.02544","snapshot_observed_at":"2026-08-06T20:12:32.783708Z","title":"Iacconi, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.783708Z"},"links":{"cited_paper":"/paper/2412.02544","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:cdde32bfba5a14850cc0d9582484d540fc7f50831099db1e85ea66fa97a3673d","observation_id":"be8a247f-9409-4c9e-aeb3-d4a16bdb7798","resolution":{"observed_at":"2026-08-06T20:12:32.783708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.03730","last_updated":"2023-02-07T20:07:58Z","snapshot_observed_at":"2026-08-05T05:49:31.902733Z","submitted_at":"2022-12-03T17:23:47Z","title":"Model independent bounds for the number of $e$-folds during the evolution of the universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.03730","snapshot_observed_at":"2026-08-06T20:12:32.787014Z","title":"Germ´ an, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.787014Z"},"links":{"cited_paper":"/paper/2212.03730","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:77824fe08e5aa8b32d5d70f57a513332dc5dca5513058a550ec5843cfce2c190","observation_id":"74817fbf-c9ee-46a0-ac0a-5c30d0de205a","resolution":{"observed_at":"2026-08-06T20:12:32.787014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.00918","last_updated":"2023-09-19T18:07:04Z","snapshot_observed_at":"2026-08-05T07:24:31.432198Z","submitted_at":"2023-06-01T17:20:21Z","title":"Novel CMB constraints on the $\\alpha$ parameter in alpha-attractor models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.00918","snapshot_observed_at":"2026-08-06T20:12:32.789952Z","title":"Iacconi, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.789952Z"},"links":{"cited_paper":"/paper/2306.00918","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:dc287848fbf57a97859fec80309939a8a307dc2822248ee94b3a4838828ba898","observation_id":"d7848838-921f-4806-abc1-12ddd17447e1","resolution":{"observed_at":"2026-08-06T20:12:32.789952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1504.05557","last_updated":"2015-04-21T19:15:48Z","snapshot_observed_at":"2026-08-03T21:37:10.494673Z","submitted_at":"2015-04-21T19:15:48Z","title":"The Hyperbolic Geometry of Cosmological Attractors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.05557","snapshot_observed_at":"2026-08-06T20:12:32.792956Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.792956Z"},"links":{"cited_paper":"/paper/1504.05557","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:fcb404b22d13bb5ce989fd3dad21c0564025dfcbf865f9220d465828dc76a77b","observation_id":"614bb752-c785-4038-a344-d9268194039d","resolution":{"observed_at":"2026-08-06T20:12:32.792956Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.13682","last_updated":"2025-03-17T19:39:25Z","snapshot_observed_at":"2026-08-07T16:56:42.537913Z","submitted_at":"2025-03-17T19:39:25Z","title":"Attractors in Supergravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.13682","snapshot_observed_at":"2026-08-06T20:12:32.795607Z","title":"Kallosh and A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.795607Z"},"links":{"cited_paper":"/paper/2503.13682","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:4c48a918214b4a8d6cdcb8a030f14e32594e17952171f978763341b7c870f4e3","observation_id":"f568984b-f7ba-4d0e-af06-a181dacee92a","resolution":{"observed_at":"2026-08-06T20:12:32.795607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.00528","last_updated":"2020-05-01T17:57:03Z","snapshot_observed_at":"2026-08-07T21:25:50.215290Z","submitted_at":"2020-05-01T17:57:03Z","title":"Multi-field inflation and preheating in asymmetric $\\alpha$-attractors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.00528","snapshot_observed_at":"2026-08-06T20:12:32.798609Z","title":"Iarygina, E","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.798609Z"},"links":{"cited_paper":"/paper/2005.00528","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:0a042d25de36af55295a1f6fa5f77c7bf587dd8ebfddd512eecf8974eb486859","observation_id":"81737883-c320-4966-9a99-334a4e7cee50","resolution":{"observed_at":"2026-08-06T20:12:32.798609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.09478","last_updated":"2018-04-09T17:36:26Z","snapshot_observed_at":"2026-08-02T16:51:29.239637Z","submitted_at":"2017-11-26T22:40:19Z","title":"Universality of multi-field $\\alpha$-attractors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.09478","snapshot_observed_at":"2026-08-06T20:12:32.801226Z","title":"Ach´ ucarro, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.801226Z"},"links":{"cited_paper":"/paper/1711.09478","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:a4da21c503add084c06888dcc5713fc3382cc9ae8ff61aef980ee9f26ed1494c","observation_id":"2b50b693-6ff6-4687-b619-7fa750a8a5df","resolution":{"observed_at":"2026-08-06T20:12:32.801226Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0702187","last_updated":"2007-02-07T10:02:04Z","snapshot_observed_at":"2026-07-07T01:06:57.044264Z","submitted_at":"2007-02-07T10:02:04Z","title":"Multiple field inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0702187","snapshot_observed_at":"2026-08-06T20:12:32.803789Z","title":"Wands, Multiple field inflation , Lect","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.803789Z"},"links":{"cited_paper":"/paper/astro-ph/0702187","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:811d0e2fac37ef786e2037e13ac094eed57714bdac41d9c1f7a92839b6f4e798","observation_id":"2772d3fa-5d53-4b4f-a654-a3fd09e218ec","resolution":{"observed_at":"2026-08-06T20:12:32.803789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:12:33.463331Z","title":"Bartolo, S","venue":null,"work_id":"a503e967-1def-4fcd-b5a1-062301a15286","year":2001},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.806701Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:1d884661b662ba79a55618585093a7ce296bae1ed9f6b320ae66ab6611777beb","observation_id":"f942a21f-5d0d-4a82-8236-7664253d2abb","resolution":{"observed_at":"2026-08-06T20:12:33.466345Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:12:33.454193Z","title":"Pinol, Multifield aspects in the early Universe : Inflation and Reheating , Ph.D","venue":null,"work_id":"8d53d5e4-2479-48f5-af34-9532eef1b512","year":2021},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.809403Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:cc50b140e414eb577d949c07a25cd57fbb42b40296c3a73b224568a612b6868a","observation_id":"7ccfc001-3b0e-4ee8-860a-411ffea722d6","resolution":{"observed_at":"2026-08-06T20:12:33.457490Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.05092","last_updated":"2022-06-17T22:38:56Z","snapshot_observed_at":"2026-07-06T12:17:07.084920Z","submitted_at":"2021-12-09T18:33:16Z","title":"Revisiting small-scale fluctuations in $\\alpha$-attractor models of inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.05092","snapshot_observed_at":"2026-08-06T20:12:32.812562Z","title":"Iacconi, H","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.812562Z"},"links":{"cited_paper":"/paper/2112.05092","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:178a0006f1f5bb50c1a9917a53d6bac8ae7195498b8c5769269eb41d854638ca","observation_id":"e0878a10-5926-4f6b-bd4f-2bcde0b317e7","resolution":{"observed_at":"2026-08-06T20:12:32.812562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.03221","last_updated":"2019-10-25T20:01:26Z","snapshot_observed_at":"2026-07-06T07:32:01.087939Z","submitted_at":"2019-02-08T18:30:24Z","title":"Hyper non-Gaussianities in inflation with strongly non-geodesic motion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.03221","snapshot_observed_at":"2026-08-06T20:12:32.815483Z","title":"Fumagalli, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.815483Z"},"links":{"cited_paper":"/paper/1902.03221","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:c641c052b0f488a76fd61a4e0baf40935cae8a3df684ee879cba76c5b1fe5e30","observation_id":"8f1e82fb-5006-420d-8c2e-3753bbfe4951","resolution":{"observed_at":"2026-08-06T20:12:32.815483Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.06116","last_updated":"2019-07-29T13:26:00Z","snapshot_observed_at":"2026-07-06T07:39:19.062840Z","submitted_at":"2019-03-14T16:50:07Z","title":"Scaling attractors in multi-field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.06116","snapshot_observed_at":"2026-08-06T20:12:32.818409Z","title":"Christodoulidis, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.818409Z"},"links":{"cited_paper":"/paper/1903.06116","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:6d9759556375635e7dd3f1e74f1682fc520dec4f3279c84cad3acad02276dcf1","observation_id":"99446751-e602-4a2d-a8b0-55a938af2a70","resolution":{"observed_at":"2026-08-06T20:12:32.818409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10529","last_updated":"2019-05-29T07:08:41Z","snapshot_observed_at":"2026-07-06T07:35:48.510196Z","submitted_at":"2019-02-27T13:51:32Z","title":"The rapid-turn inflationary attractor","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10529","snapshot_observed_at":"2026-08-06T20:12:32.821100Z","title":"Bjorkmo, Rapid-Turn Inflationary Attractors, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.821100Z"},"links":{"cited_paper":"/paper/1902.10529","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:8e26ed0a58198f1dd061504807c8346fa7b26f606396ae35e0bfb6021c9b662d","observation_id":"94a3c931-4523-4e5b-8ee5-89fa270cab74","resolution":{"observed_at":"2026-08-06T20:12:32.821100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.02020","last_updated":"2019-07-03T16:37:50Z","snapshot_observed_at":"2026-08-01T17:23:18.409994Z","submitted_at":"2019-07-03T16:37:50Z","title":"Orbital Inflation: inflating along an angular isometry of field space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.02020","snapshot_observed_at":"2026-08-06T20:12:32.823712Z","title":"Ach´ ucarro and Y","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.823712Z"},"links":{"cited_paper":"/paper/1907.02020","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:bfca967b438ed4fdc4202df23e63aa35024a7655b7126ef82db6b767bea55f83","observation_id":"7afebbac-be36-4b12-9596-d0e2954b3414","resolution":{"observed_at":"2026-08-06T20:12:32.823712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03657","last_updated":"2020-07-24T14:42:51Z","snapshot_observed_at":"2026-07-06T07:26:13.408937Z","submitted_at":"2019-01-11T17:22:42Z","title":"Shift-Symmetric Orbital Inflation: single field or multi-field?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03657","snapshot_observed_at":"2026-08-06T20:12:32.826516Z","title":"Ach´ ucarro, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.826516Z"},"links":{"cited_paper":"/paper/1901.03657","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:b1ba9238f9cac379e242b5852770730aae78b6508e9b83bb6730e20cb0fab8dd","observation_id":"f3c15be0-3857-4692-80b7-d5f1599c2f95","resolution":{"observed_at":"2026-08-06T20:12:32.826516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.14156","last_updated":"2024-06-19T14:13:04Z","snapshot_observed_at":"2026-08-08T03:32:00.790638Z","submitted_at":"2023-03-24T17:08:50Z","title":"Non-Gaussianity in rapid-turn multi-field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.14156","snapshot_observed_at":"2026-08-06T20:12:32.830150Z","title":"Iarygina, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.830150Z"},"links":{"cited_paper":"/paper/2303.14156","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:09ef7479dcef1f08ade47b4301c24dacbc91c2411b019c4c061ccf0cc00b171f","observation_id":"89477366-0e30-4262-b951-3175e7d6912d","resolution":{"observed_at":"2026-08-06T20:12:32.830150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1011.6675","last_updated":"2010-12-14T19:30:53Z","snapshot_observed_at":"2026-07-06T02:19:58.630471Z","submitted_at":"2010-11-30T20:57:01Z","title":"Non-Gaussianity in Two-Field Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.6675","snapshot_observed_at":"2026-08-06T20:12:32.833099Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.833099Z"},"links":{"cited_paper":"/paper/1011.6675","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:feec9723790f93616b2cdd403466c646cbe6ed484e64b74556dea2a99eebccf3","observation_id":"d5cb1344-fef3-41e3-b246-97e02ce635b4","resolution":{"observed_at":"2026-08-06T20:12:32.833099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0503203","last_updated":"2005-03-26T05:05:07Z","snapshot_observed_at":"2026-07-07T04:53:40.441347Z","submitted_at":"2005-03-26T05:05:07Z","title":"Particle Physics and Inflationary Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0503203","snapshot_observed_at":"2026-08-06T20:12:32.835758Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.835758Z"},"links":{"cited_paper":"/paper/hep-th/0503203","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:d770974308e379f750bdbe2f9ab935ec866a03e8058ad018d73bac934ca0d395","observation_id":"d6c3cdb1-e0fd-4b3b-83d7-c6cfaf9878de","resolution":{"observed_at":"2026-08-06T20:12:32.835758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9909467","last_updated":"1999-10-20T12:44:24Z","snapshot_observed_at":"2026-08-02T08:32:12.776280Z","submitted_at":"1999-09-22T12:47:40Z","title":"Reheating Temperature and Inflaton Mass Bounds from Thermalization After Inflation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9909467","snapshot_observed_at":"2026-08-06T20:12:32.838416Z","title":"McDonald, Reheating temperature and inflaton mass bounds from thermalization after inflation, Phys","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.838416Z"},"links":{"cited_paper":"/paper/hep-ph/9909467","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:03bea10922dd99931e86bad88fc48161b428d5b7ee75243c0d9d142150e9990b","observation_id":"d592afb0-5cb4-448a-8a42-aa726a1a2dbc","resolution":{"observed_at":"2026-08-06T20:12:32.838416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0307241","last_updated":"2003-07-18T18:53:02Z","snapshot_observed_at":"2026-07-07T04:00:40.769582Z","submitted_at":"2003-07-18T18:53:02Z","title":"On the reheating stage after inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0307241","snapshot_observed_at":"2026-08-06T20:12:32.841520Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.841520Z"},"links":{"cited_paper":"/paper/hep-ph/0307241","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:312b9e9c0e86dd6585d02438e550e830996f7f5c0ef021c5f1a83c72dd2c3b1d","observation_id":"fd3a0d06-b6b0-47fb-a676-0c139fa63369","resolution":{"observed_at":"2026-08-06T20:12:32.841520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T20:12:33.444698Z","title":null,"venue":null,"work_id":"ee3d7ffd-0dc6-47ee-b138-e17e28cb5617","year":1980},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.844759Z"},"links":{"citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:58f95e01b4b6f6a86b141cb241f233193e79286d5e20576aaca698c29f6d080c","observation_id":"b63b8e8c-5083-4646-ac27-d3f288c944fb","resolution":{"observed_at":"2026-08-06T20:12:33.448187Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1009.2448","last_updated":"2011-05-17T17:48:12Z","snapshot_observed_at":"2026-07-31T19:59:12.568888Z","submitted_at":"2010-09-13T16:49:02Z","title":"Scalaron the mighty: producing dark matter and baryon asymmetry at reheating","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1009.2448","snapshot_observed_at":"2026-08-06T20:12:32.847237Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.847237Z"},"links":{"cited_paper":"/paper/1009.2448","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:39b92637d33e334b160c7321826a4f07027e88bd207cddd9a4cfb17248fcc390","observation_id":"487e92f7-d321-45b9-b867-9cf2e12c11e4","resolution":{"observed_at":"2026-08-06T20:12:32.847237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.04673","last_updated":"2015-03-10T21:07:04Z","snapshot_observed_at":"2026-07-06T04:09:23.043748Z","submitted_at":"2015-02-16T19:31:21Z","title":"Reheating predictions in single field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.04673","snapshot_observed_at":"2026-08-06T20:12:32.849899Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.849899Z"},"links":{"cited_paper":"/paper/1502.04673","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:1069b3c8d0282bf50bd7256967e67eb7e4e2eab43c6962ec9c12dcc16de04361","observation_id":"6984b8b1-0bfa-48ff-a9d4-7d7d7327ddd7","resolution":{"observed_at":"2026-08-06T20:12:32.849899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.15831","last_updated":"2023-11-17T22:37:41Z","snapshot_observed_at":"2026-07-06T15:47:34.431636Z","submitted_at":"2023-06-27T23:30:57Z","title":"Reheating constraints and consistency relations of the Starobinsky model and some of its generalizations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.15831","snapshot_observed_at":"2026-08-06T20:12:32.852607Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.852607Z"},"links":{"cited_paper":"/paper/2306.15831","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:5ddafeb06a83b5f7a03bcce15871d69744b831c50269c758b28831bd3a18c455","observation_id":"77b7c27d-2940-4efd-8937-bf710b195b85","resolution":{"observed_at":"2026-08-06T20:12:32.852607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9405187","last_updated":"1994-10-12T02:18:47Z","snapshot_observed_at":"2026-07-07T05:05:39.294414Z","submitted_at":"1994-05-30T07:16:24Z","title":"Reheating after Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/9405187","snapshot_observed_at":"2026-08-06T20:12:32.855665Z","title":"Kofman, A","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.855665Z"},"links":{"cited_paper":"/paper/hep-th/9405187","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:2ece7435e14119d190d0d7e0cb539d161fa681d2d5913898098a59aa506b28f8","observation_id":"d6c0c1ea-f05e-4fce-9756-bfff11cb59a5","resolution":{"observed_at":"2026-08-06T20:12:32.855665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/9704452","last_updated":"1997-08-13T01:23:10Z","snapshot_observed_at":"2026-07-07T04:25:39.785066Z","submitted_at":"1997-04-30T18:17:10Z","title":"Towards the Theory of Reheating After Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/9704452","snapshot_observed_at":"2026-08-06T20:12:32.858554Z","title":"Kofman, A","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-06T20:12:32.858554Z"},"links":{"cited_paper":"/paper/hep-ph/9704452","citing_paper":"/paper/2507.03610"},"observation_digest":"sha256:c0da3cd33496f08c677fab6a1ab24bca7a42853a7a0459ecfff287b1bc6ae62a","observation_id":"e60e31c4-2fb1-490e-aea6-37ff9927442c","resolution":{"observed_at":"2026-08-06T20:12:32.858554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.03610","last_updated":"2025-07-04T14:32:44Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T22:25:42.549520Z","submitted_at":"2025-07-04T14:32:44Z","title":"Post-inflationary enhancement of adiabatic perturbations in modular cosmology"},"reference_resolution":{"displayed":59,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":51,"verified_exact":5,"verified_fuzzy":3},"total_outbound_references":59},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 59 of 59 outbound references and 3 inbound Pith citation observations for arXiv:2507.03610."}