{"as_of":"2026-08-14T18:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5516acf8b48dae4aea79b49e722d825282f1b1f77d85164d1e02886afa8a4379","coverage":[{"denominator":111,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T01:54:33.033479Z","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":"2026-08-14T06:32:32.682623+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":"2026-08-01T15:39:43.435944Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.14529","snapshot_observed_at":"2026-08-01T15:39:43.435944Z","title":"Huenupi, C","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18369","last_updated":"2026-07-20T18:00:00Z","snapshot_observed_at":"2026-08-13T16:32:14.782157Z","submitted_at":"2026-07-20T18:00:00Z","title":"Dissecting the Scalar Cosmological Collider with the Cosmic Microwave Background","version":1},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-08-01T15:39:43.435944Z"},"links":{"cited_paper":"/paper/2607.14529","citing_paper":"/paper/2607.18369"},"observation_digest":"sha256:dabc60b395c18e2b30c483129a8e0e00a3b391ef2f6ae3f8f55d2a3a0141e96e","observation_id":"44d3036a-34b3-4c2b-b750-b61501e8934b","resolution":{"observed_at":"2026-08-01T15:39:43.435944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2607.14529/citation-record","integrity":"/paper/2607.14529/integrity","json":"/paper/2607.14529/citation-record.json","paper":"/paper/2607.14529"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-02T01:54:22.262568Z","title":"The Inflationary Universe: A Possible So- lution to the Horizon and Flatness Problems,","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.262568Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:349dd8a7fdb0e56b3484feec49f7bd0fe50db66855dcd46d238d6b14d48d999c","observation_id":"fbf6ff71-d00b-450b-ac01-35e98b279c6e","resolution":{"observed_at":"2026-08-02T01:54:22.262568Z","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":"2026-08-02T01:54:22.381818Z","title":"A New Type of Isotropic Cosmo- logical Models Without Singularity,","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.381818Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:5cf2502b5079ac3cc7555cd7e21d957e424453d44f82a5fd4886d34206629020","observation_id":"2e079238-c482-40a0-a521-687cf9ef5cd1","resolution":{"observed_at":"2026-08-02T01:54:22.381818Z","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":"2026-08-02T01:54:22.500215Z","title":"A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homo- geneity, Isotropy and Primordial Monopole Problems,","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.500215Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:a2b9e801d24b46408e012aad95bc0501ca54f90b8b6c41c5e531763bf2b67c7f","observation_id":"cb2ec0a0-60a6-4109-8d8a-80caebe0efb3","resolution":{"observed_at":"2026-08-02T01:54:22.500215Z","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":"2026-08-02T01:54:22.555304Z","title":"Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking,","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.555304Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:a4866769537f0344c05bfb8252f013f2596a6eb7207f41205e584b8e4f74e251","observation_id":"4f307c89-f887-464a-a5c6-e18d1ed0fef2","resolution":{"observed_at":"2026-08-02T01:54:22.555304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.08128","last_updated":"2022-09-29T17:53:00Z","snapshot_observed_at":"2026-08-13T16:22:35.227820Z","submitted_at":"2022-03-15T17:54:21Z","title":"Inflation: Theory and Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.08128","snapshot_observed_at":"2026-08-02T01:54:22.643863Z","title":"Inflation: Theory and Observations,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.643863Z"},"links":{"cited_paper":"/paper/2203.08128","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:d78538a7b41ac1679b3027811a846719c9fd513f756fcb92c200c49d2f3ac74e","observation_id":"ae82448f-15f0-4b51-93bb-3de6b54558b5","resolution":{"observed_at":"2026-08-02T01:54:22.643863Z","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":"2026-08-02T01:54:22.729798Z","title":"Non-Gaussianity from inflation: Theory and observa- tions,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.729798Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:25e18d43d2a2daa201fbbddce6bba56b14186a72445f98bace16912c266987c0","observation_id":"03efb78c-8fcd-4022-baee-e15c1c7884e4","resolution":{"observed_at":"2026-08-02T01:54:22.729798Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.1416","last_updated":"2010-06-04T18:05:42Z","snapshot_observed_at":"2026-08-13T22:21:24.598737Z","submitted_at":"2010-02-08T20:58:08Z","title":"Primordial Non-Gaussianities from Inflation Models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.1416","snapshot_observed_at":"2026-08-02T01:54:22.822450Z","title":"Primordial Non-Gaussianities from Infla- tion Models,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.822450Z"},"links":{"cited_paper":"/paper/1002.1416","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:a12ade43326c62235e1bb9fa83aa74c659f6e2446262eafd4934c726f5e8d5d2","observation_id":"17f1de07-0018-420f-bd22-888327fe827d","resolution":{"observed_at":"2026-08-02T01:54:22.822450Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1523","last_updated":"2013-06-05T06:59:11Z","snapshot_observed_at":"2026-07-06T03:08:07.485036Z","submitted_at":"2013-03-06T21:00:01Z","title":"Inflation, Cosmic Perturbations and Non-Gaussianities","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1523","snapshot_observed_at":"2026-08-02T01:54:22.882474Z","title":"Inflation, Cosmic Perturbations and Non- Gaussianities,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.882474Z"},"links":{"cited_paper":"/paper/1303.1523","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:5eb7436cd6a514ebc5ed8191533d8d1580881a5706db6975c409bbbba01d3abb","observation_id":"84b36112-ba6d-4e7d-9ca5-d98f3386445e","resolution":{"observed_at":"2026-08-02T01:54:22.882474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.05202","last_updated":"2018-10-17T17:41:14Z","snapshot_observed_at":"2026-07-06T06:44:41.329034Z","submitted_at":"2018-06-13T18:08:23Z","title":"Reconstructing the Inflationary Landscape with Cosmological Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.05202","snapshot_observed_at":"2026-08-02T01:54:22.966633Z","title":"Reconstructing the Inflationary Landscape with Cosmological Data,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:22.966633Z"},"links":{"cited_paper":"/paper/1806.05202","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:42c30223b190ad935272b43b34648089e66fb363b04c95082ac6e4c0eb94d407","observation_id":"3bc4d071-3632-4d73-a4ef-2af8245fc297","resolution":{"observed_at":"2026-08-02T01:54:22.966633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.07315","last_updated":"2018-10-17T17:06:57Z","snapshot_observed_at":"2026-08-13T16:14:05.174081Z","submitted_at":"2018-04-19T18:03:50Z","title":"Landscape tomography through primordial non-Gaussianity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.07315","snapshot_observed_at":"2026-08-02T01:54:23.052812Z","title":"Landscape tomography through primordial non-Gaussianity,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.052812Z"},"links":{"cited_paper":"/paper/1804.07315","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:6027bd15be0c8a5499f8bee5537e944255065bac7e369fb4234e4df6dc793402","observation_id":"08261f60-62b1-44b1-96ca-a2ebf2aa2d42","resolution":{"observed_at":"2026-08-02T01:54:23.052812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10166","last_updated":"2017-12-05T16:28:14Z","snapshot_observed_at":"2026-08-04T04:38:52.879136Z","submitted_at":"2017-03-29T18:00:01Z","title":"Schwinger-Keldysh Diagrammatics for Primordial Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.10166","snapshot_observed_at":"2026-08-02T01:54:23.197332Z","title":"Schwinger- Keldysh Diagrammatics for Primordial Perturbations,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.197332Z"},"links":{"cited_paper":"/paper/1703.10166","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:fec0e65381d4873ceef52bd12ceb919fb16d094b7c9cbad9c1a59f9c3ab68649","observation_id":"7ffe9905-fa6e-428c-a21c-ed337f2014c1","resolution":{"observed_at":"2026-08-02T01:54:23.197332Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0506236","last_updated":"2005-06-28T13:54:18Z","snapshot_observed_at":"2026-08-11T01:23:23.363094Z","submitted_at":"2005-06-28T13:54:18Z","title":"Quantum Contributions to Cosmological Correlations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0506236","snapshot_observed_at":"2026-08-02T01:54:23.248919Z","title":"Quantum contributions to cosmologi- cal correlations,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.248919Z"},"links":{"cited_paper":"/paper/hep-th/0506236","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:bd394f59164142eec24d16522a9caf67d524dae14153a1dc0909f048912e90f9","observation_id":"e7c1a22d-ebd6-4aeb-976a-0ecfb92e776b","resolution":{"observed_at":"2026-08-02T01:54:23.248919Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0904.4207","last_updated":"2009-08-17T21:41:54Z","snapshot_observed_at":"2026-07-06T01:53:51.815591Z","submitted_at":"2009-04-27T16:23:45Z","title":"The \"in-in\" Formalism and Cosmological Perturbations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.4207","snapshot_observed_at":"2026-08-02T01:54:23.304326Z","title":"The ’in-in’ For- malism and Cosmological Perturbations,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.304326Z"},"links":{"cited_paper":"/paper/0904.4207","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:6b60cc9f211399efb5ac7923ae25fdb2a3131e9f1e7627713a2c4d71c9d35aa7","observation_id":"7e7ba53e-dfbb-4e00-824d-931e12aa9822","resolution":{"observed_at":"2026-08-02T01:54:23.304326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9312033","last_updated":"1993-12-15T18:45:54Z","snapshot_observed_at":"2026-07-07T01:09:16.203858Z","submitted_at":"1993-12-15T18:45:54Z","title":"The Three--Point Correlation Function of the Cosmic Microwave Background in Inflationary Models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9312033","snapshot_observed_at":"2026-08-02T01:54:23.357973Z","title":"The Three point correlation function of the cosmic mi- crowave background in inflationary models,","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.357973Z"},"links":{"cited_paper":"/paper/astro-ph/9312033","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:9626eb1b3262e8f742a25cbf00c1dd08115a1e9931e0589ee81179156def0a9a","observation_id":"3b698d7d-f2e1-4822-bace-ce5f781a0a46","resolution":{"observed_at":"2026-08-02T01:54:23.357973Z","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":"2026-08-02T01:54:23.414547Z","title":"Second order cosmological perturbations from infla- tion,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.414547Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:65458a62e65e9c871536355669fded2adb1f817c01ba36035626669d1634a500","observation_id":"c52a83c4-99db-480c-96ce-c78242a6dfdd","resolution":{"observed_at":"2026-08-02T01:54:23.414547Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210603","last_updated":"2005-05-06T20:21:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2002-10-28T19:20:43Z","title":"Non-Gaussian features of primordial fluctuations in single field inflationary models","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0210603","snapshot_observed_at":"2026-08-02T01:54:23.463751Z","title":"Non-Gaussian features of primordial fluctuations in single field inflationary models,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.463751Z"},"links":{"cited_paper":"/paper/astro-ph/0210603","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:7017e18b2453f73c03343b8ce1387c369156cda2cb4a2863528daac59f12c2b1","observation_id":"534e2b5f-fa9a-4621-bea6-57faf19ce6bd","resolution":{"observed_at":"2026-08-02T01:54:23.463751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4707","last_updated":"2010-01-25T23:04:56Z","snapshot_observed_at":"2026-08-11T03:22:51.144758Z","submitted_at":"2010-01-25T23:04:56Z","title":"Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4707","snapshot_observed_at":"2026-08-02T01:54:23.541506Z","title":"Primordial non-Gaussianity and Bis- pectrum Measurements in the Cosmic Microwave Back- ground and Large-Scale Structure,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.541506Z"},"links":{"cited_paper":"/paper/1001.4707","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:b92a5bd01148bf24508918951003c2478377745223c8804bad7c45b6f0ebac2d","observation_id":"3936fb67-b2a7-44bc-ac81-166546801036","resolution":{"observed_at":"2026-08-02T01:54:23.541506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0293","last_updated":"2008-03-05T10:54:07Z","snapshot_observed_at":"2026-08-12T17:39:56.093868Z","submitted_at":"2007-09-04T19:32:50Z","title":"The Effective Field Theory of Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.0293","snapshot_observed_at":"2026-08-02T01:54:23.602052Z","title":"The Effective Field Theory of Infla- tion,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.602052Z"},"links":{"cited_paper":"/paper/0709.0293","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:5c1cba4c60e88d50d4899d3f484a4123302d0dcfe26daa9441d6f5c1338cf501","observation_id":"fa041d4d-d8bc-4b43-9c34-0434b9769fe2","resolution":{"observed_at":"2026-08-02T01:54:23.602052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0405356","last_updated":"2004-05-18T20:04:28Z","snapshot_observed_at":"2026-08-02T12:23:38.295819Z","submitted_at":"2004-05-18T20:04:28Z","title":"The shape of non-Gaussianities","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0405356","snapshot_observed_at":"2026-08-02T01:54:23.663201Z","title":"The Shape of non-Gaussianities,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.663201Z"},"links":{"cited_paper":"/paper/astro-ph/0405356","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:a599c957cb6c0959812ab3f308f9d750cbbef179a502a97446e5674315b15594","observation_id":"214ac827-c715-4911-ba15-b6ae3b2d6c57","resolution":{"observed_at":"2026-08-02T01:54:23.663201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.05697","last_updated":"2019-05-14T16:19:37Z","snapshot_observed_at":"2026-08-14T16:32:26.859930Z","submitted_at":"2019-05-14T16:19:37Z","title":"Planck 2018 results. IX. Constraints on primordial non-Gaussianity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.05697","snapshot_observed_at":"2026-08-02T01:54:23.714589Z","title":"Planck 2018 results. IX. Con- straints on primordial non-Gaussianity,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.714589Z"},"links":{"cited_paper":"/paper/1905.05697","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:acd943227a2facb8e1f0587fdfb9c722607cd620c9f7dc6abc2084dcfaae0ded","observation_id":"29ffe80b-a6c6-4393-9523-485e3302765e","resolution":{"observed_at":"2026-08-02T01:54:23.714589Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0905.3746","last_updated":"2011-01-03T11:35:16Z","snapshot_observed_at":"2026-08-03T19:35:05.540840Z","submitted_at":"2009-05-22T20:00:14Z","title":"Non-Gaussianities in Single Field Inflation and their Optimal Limits from the WMAP 5-year Data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0905.3746","snapshot_observed_at":"2026-08-02T01:54:23.766969Z","title":"Non- Gaussianities in Single Field Inflation and their Optimal Limits from the WMAP 5-year Data,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.766969Z"},"links":{"cited_paper":"/paper/0905.3746","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:0f8d3f3005627bfee81dc7d8239975fa15bfdb4e57706e11100bda1f6bf6a561","observation_id":"5b4366a8-5b4a-401a-acce-9b9f1efe87b9","resolution":{"observed_at":"2026-08-02T01:54:23.766969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.2601","last_updated":"2014-04-09T20:00:20Z","snapshot_observed_at":"2026-08-14T10:41:31.346010Z","submitted_at":"2014-04-09T20:00:20Z","title":"Inflation and String Theory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.2601","snapshot_observed_at":"2026-08-02T01:54:23.826113Z","title":"Inflation and String Theory,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.826113Z"},"links":{"cited_paper":"/paper/1404.2601","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:cd8fb6a9f07fa0b55e4b6c8c39933c28381ff09329154c9cd3045fef54eead3e","observation_id":"2cf829ca-5bd4-4273-a9a4-a7782ac16d20","resolution":{"observed_at":"2026-08-02T01:54:23.826113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005036","last_updated":"2000-12-09T02:38:05Z","snapshot_observed_at":"2026-07-07T00:11:03.390868Z","submitted_at":"2000-05-02T20:03:52Z","title":"Acoustic Signatures in the Primary Microwave Background Bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005036","snapshot_observed_at":"2026-08-02T01:54:23.879677Z","title":"Acoustic signatures in the primary microwave background bispectrum,","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.879677Z"},"links":{"cited_paper":"/paper/astro-ph/0005036","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:d2ee1c716057dd0ae37c582fbed7476688b65555c9f04aa63649d525531a648e","observation_id":"f3d0f1ed-5a25-4489-a075-a06213a9285f","resolution":{"observed_at":"2026-08-02T01:54:23.879677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0504045","last_updated":"2005-09-18T14:16:25Z","snapshot_observed_at":"2026-08-05T20:10:17.664503Z","submitted_at":"2005-04-02T21:44:44Z","title":"The inflationary prediction for primordial non-gaussianity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0504045","snapshot_observed_at":"2026-08-02T01:54:23.930281Z","title":"The Inflationary predic- tion for primordial non-Gaussianity,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.930281Z"},"links":{"cited_paper":"/paper/astro-ph/0504045","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:27de83c51fc75a7d55cf723880c460dcf914c51caccc77bc892d587834ae4650","observation_id":"fe65a7e0-b272-4b88-90bd-90833fe5708c","resolution":{"observed_at":"2026-08-02T01:54:23.930281Z","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":"2026-08-02T01:54:23.983381Z","title":"The Pri- mordial density perturbation in the curvaton sce- nario,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:23.983381Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:41e4794123729c47f779f7e811311ce5502e612b242af6d3b6b76f214d45ac38","observation_id":"c731f553-1b9f-46dc-b1cc-0cc718b09370","resolution":{"observed_at":"2026-08-02T01:54:23.983381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.0496","last_updated":"2010-03-03T19:05:30Z","snapshot_observed_at":"2026-08-10T21:39:55.752223Z","submitted_at":"2009-09-02T19:49:28Z","title":"Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.0496","snapshot_observed_at":"2026-08-02T01:54:24.035304Z","title":"Large non-Gaussianities with Intermediate Shapes from Quasi-Single Field Inflation,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.035304Z"},"links":{"cited_paper":"/paper/0909.0496","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:84f3e8a986164a04fda36aed9e73eaecf2786494d5544922681ae7ae4c42a45d","observation_id":"f05c4d94-ca51-44fe-812a-2bde24a50aec","resolution":{"observed_at":"2026-08-02T01:54:24.035304Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.0160","last_updated":"2012-07-03T16:05:01Z","snapshot_observed_at":"2026-08-12T06:39:39.428932Z","submitted_at":"2012-05-01T14:00:02Z","title":"Quasi-Single Field Inflation with Large Mass","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.0160","snapshot_observed_at":"2026-08-02T01:54:24.115731Z","title":"Quasi-Single Field In- flation with Large Mass,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.115731Z"},"links":{"cited_paper":"/paper/1205.0160","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:3ab2087a7ab37443bd100ccbb9c28777a5c8cf71b6e9a2710eb8975312f4e50e","observation_id":"444c6830-2e13-427a-a5f0-66a295e1fc6e","resolution":{"observed_at":"2026-08-02T01:54:24.115731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.3380","last_updated":"2010-04-24T15:03:29Z","snapshot_observed_at":"2026-08-13T04:42:22.763684Z","submitted_at":"2009-11-17T19:20:45Z","title":"Quasi-Single Field Inflation and Non-Gaussianities","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.3380","snapshot_observed_at":"2026-08-02T01:54:24.172439Z","title":"Quasi-Single Field Infla- tion and Non-Gaussianities,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.172439Z"},"links":{"cited_paper":"/paper/0911.3380","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:14c3bcf800b2ddca2f38dbf20425a47349e307dc69c53ce8f2763a7370d0cba1","observation_id":"5632bca8-2aa6-4679-8592-95e4f82a2bfd","resolution":{"observed_at":"2026-08-02T01:54:24.172439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.1624","last_updated":"2013-06-07T08:27:03Z","snapshot_observed_at":"2026-08-05T00:12:50.289415Z","submitted_at":"2012-11-07T17:59:24Z","title":"Effective field theory approach to quasi-single field inflation and effects of heavy fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.1624","snapshot_observed_at":"2026-08-02T01:54:24.201639Z","title":"Effec- tive field theory approach to quasi-single field infla- tion and effects of heavy fields,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.201639Z"},"links":{"cited_paper":"/paper/1211.1624","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:a07a08dea36ff7fdba44fe14fe4b47e56ae4b9b528aeda4b8e43953255a099e0","observation_id":"23e4f8a2-8824-4e89-ac1a-bbf7a873a80a","resolution":{"observed_at":"2026-08-02T01:54:24.201639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.08043","last_updated":"2015-03-27T12:21:32Z","snapshot_observed_at":"2026-08-13T00:18:01.919314Z","submitted_at":"2015-03-27T12:21:32Z","title":"Cosmological Collider Physics","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.08043","snapshot_observed_at":"2026-08-02T01:54:24.287904Z","title":"Cosmological Collider Physics,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.287904Z"},"links":{"cited_paper":"/paper/1503.08043","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:84212d4d6dab5536e666608883526cb85718bb144634f8bbb72166e0c9cfb0bd","observation_id":"770d305d-b802-4f10-8fcb-286733e5c3d5","resolution":{"observed_at":"2026-08-02T01:54:24.287904Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03735","last_updated":"2016-07-13T13:56:35Z","snapshot_observed_at":"2026-07-06T05:03:24.708864Z","submitted_at":"2016-07-13T13:56:35Z","title":"Non-Gaussianity as a Particle Detector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03735","snapshot_observed_at":"2026-08-02T01:54:24.354834Z","title":"Non- Gaussianity as a Particle Detector,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.354834Z"},"links":{"cited_paper":"/paper/1607.03735","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:b9239d8e1c235a058f19f946e464de1faf8415ed24e2f747793d65760559f85a","observation_id":"ad432fd5-a0b8-4361-a692-5295b1f98c2a","resolution":{"observed_at":"2026-08-02T01:54:24.354834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.06559","last_updated":"2016-12-17T20:46:24Z","snapshot_observed_at":"2026-07-06T05:15:25.173487Z","submitted_at":"2016-10-20T19:58:17Z","title":"Prospects for Cosmological Collider Physics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.06559","snapshot_observed_at":"2026-08-02T01:54:24.503218Z","title":"Prospects for Cosmological Collider Physics,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.503218Z"},"links":{"cited_paper":"/paper/1610.06559","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:24cb8d1844537e3d2d40a2ab04bb14ac859aa7339b42f0c40b2f038eaa056631","observation_id":"58b93ef5-ea29-4413-9a8f-0afeedaca494","resolution":{"observed_at":"2026-08-02T01:54:24.503218Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.06597","last_updated":"2017-06-30T08:40:24Z","snapshot_observed_at":"2026-07-06T05:15:25.173487Z","submitted_at":"2016-10-20T20:27:41Z","title":"Standard Model Background of the Cosmological Collider","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.06597","snapshot_observed_at":"2026-08-02T01:54:24.621753Z","title":"Standard Model Background of the Cosmological Collider,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.621753Z"},"links":{"cited_paper":"/paper/1610.06597","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:8fb6c167a002c16d2d390b763a1356facef01f7174e47dbccb312f4990327bbd","observation_id":"bb048ef1-85fe-4ed9-8b2d-d479735d408f","resolution":{"observed_at":"2026-08-02T01:54:24.621753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.09971","last_updated":"2017-12-18T21:33:16Z","snapshot_observed_at":"2026-08-01T22:39:08.424885Z","submitted_at":"2017-06-29T22:26:13Z","title":"Quasi Single Field Inflation in the non-perturbative regime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.09971","snapshot_observed_at":"2026-08-02T01:54:24.755190Z","title":"Quasi Single Field Inflation in the non-perturbative regime,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.755190Z"},"links":{"cited_paper":"/paper/1706.09971","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:aaa790aea97a532905c5ec822170c02526d1f9095dc0d9c6481a5d8b0028bdf4","observation_id":"4057272e-8a88-468c-ab8a-79204a42cadb","resolution":{"observed_at":"2026-08-02T01:54:24.755190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.03054","last_updated":"2017-11-21T02:08:35Z","snapshot_observed_at":"2026-08-13T05:05:34.342995Z","submitted_at":"2017-10-09T12:23:54Z","title":"Strongly Coupled Quasi-Single Field Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.03054","snapshot_observed_at":"2026-08-02T01:54:24.877924Z","title":"Strongly Coupled Quasi-Single Field Inflation,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.877924Z"},"links":{"cited_paper":"/paper/1710.03054","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:04c9dbf01ceecdfa1e3ab85fd85611d73367036c89e12b4ae1000bed4ea5c695","observation_id":"228fab8c-c89c-46d5-9e2e-7bcea160a32c","resolution":{"observed_at":"2026-08-02T01:54:24.877924Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.04459","last_updated":"2020-01-22T09:26:49Z","snapshot_observed_at":"2026-08-13T22:50:37.349999Z","submitted_at":"2019-11-11T18:56:23Z","title":"On the inflationary massive field with a curved field manifold","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.04459","snapshot_observed_at":"2026-08-02T01:54:24.976640Z","title":"On the inflationary massive field with a curved field manifold,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:24.976640Z"},"links":{"cited_paper":"/paper/1911.04459","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:91924676d2be53ad085ee239a9058d66a118cdc0086c2872fb324eccca4353f1","observation_id":"91082ce9-3e77-4533-941d-8d0c0c17783c","resolution":{"observed_at":"2026-08-02T01:54:24.976640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.13667","last_updated":"2021-04-12T10:14:21Z","snapshot_observed_at":"2026-08-12T01:21:37.126381Z","submitted_at":"2020-12-26T03:04:49Z","title":"Disentangling mass spectra of multiple fields in cosmological collider","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.13667","snapshot_observed_at":"2026-08-02T01:54:25.086052Z","title":"Disentangling mass spectra of multiple fields in cosmological collider,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.086052Z"},"links":{"cited_paper":"/paper/2012.13667","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:828230118447d9b8f6320eda2b67307a6e6a1bad164f6f7138187841dc84131f","observation_id":"61c28341-7440-4bd0-b06e-96d4342caaa4","resolution":{"observed_at":"2026-08-02T01:54:25.086052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.05710","last_updated":"2023-01-20T11:33:50Z","snapshot_observed_at":"2026-08-14T17:26:35.071203Z","submitted_at":"2021-12-10T18:06:46Z","title":"Inflationary flavor oscillations and the cosmic spectroscopy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.05710","snapshot_observed_at":"2026-08-02T01:54:25.211047Z","title":"Inflationary flavor oscillations and the cosmic spec- troscopy,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.211047Z"},"links":{"cited_paper":"/paper/2112.05710","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:5dd7825b14860ab13994a6a689d50657771968172b6b4a87ebd1d66e6222809f","observation_id":"d065c5c6-d238-4448-bb73-50657e246983","resolution":{"observed_at":"2026-08-02T01:54:25.211047Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2310.01494","last_updated":"2023-10-02T18:00:07Z","snapshot_observed_at":"2026-08-13T05:59:03.164696Z","submitted_at":"2023-10-02T18:00:07Z","title":"Light Scalars at the Cosmological Collider","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.01494","snapshot_observed_at":"2026-08-02T01:54:25.322791Z","title":"Light scalars at the cosmological collider,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.322791Z"},"links":{"cited_paper":"/paper/2310.01494","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:050dd074632983ab4746ce89d2b21d762723fb01da8cc82bc92c448a79bd3e5b","observation_id":"fa689df7-32c1-4d64-96a2-7266f83dc179","resolution":{"observed_at":"2026-08-02T01:54:25.322791Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.01894","last_updated":"2025-02-13T11:35:57Z","snapshot_observed_at":"2026-08-13T00:39:20.354641Z","submitted_at":"2024-04-02T12:35:29Z","title":"BOSS Constraints on Massive Particles during Inflation: The Cosmological Collider in Action","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.01894","snapshot_observed_at":"2026-08-02T01:54:25.454618Z","title":"BOSS constraints on massive particles during inflation: The cosmological collider in action,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.454618Z"},"links":{"cited_paper":"/paper/2404.01894","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:0a0f821922fe4fb77451f9536b4d119cdffbad51d62470acccd1925c3d89e427","observation_id":"301b109d-c5d5-4817-aa44-7686f9d48847","resolution":{"observed_at":"2026-08-02T01:54:25.454618Z","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":"2026-08-02T01:54:25.630014Z","title":"Massive inflationary am- plitudes: new representations and degenerate limits,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.630014Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:d53abca9e1b3dfc9b779bfbf565ebaf57cd44328d8f64656ba8a5546b249ae92","observation_id":"fad72202-f691-448b-8a55-c48ecb1889fa","resolution":{"observed_at":"2026-08-02T01:54:25.630014Z","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":"2026-08-02T01:54:25.751676Z","title":"Cosmo- logical Collider Searches beyond the Hubble Scale with Planck Data,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.751676Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:7e06cf33dc343e2a23a70fcf524b26b3e9504a5d5a7f5f819f14f7cc1d2236ad","observation_id":"f17319e6-bbc9-4a97-8552-46a048e59ff7","resolution":{"observed_at":"2026-08-02T01:54:25.751676Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2604.07434","last_updated":"2026-04-08T18:00:00Z","snapshot_observed_at":"2026-08-10T17:23:05.167232Z","submitted_at":"2026-04-08T18:00:00Z","title":"Scalars at the Cosmological Collider: Full Shapes of Tree Diagrams and Bispectrum Searches using Planck Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2604.07434","snapshot_observed_at":"2026-08-02T01:54:25.860626Z","title":"Scalars at the Cosmological Collider: Full Shapes of Tree Di- agrams and Bispectrum Searches using Planck Data,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.860626Z"},"links":{"cited_paper":"/paper/2604.07434","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:a68ae912affacb6e5bdc6f006f48a444d470fbd8b043279f38a55700fa64b2d0","observation_id":"ab2b5f6e-2f2e-4db0-b5ff-82f6cf0a485f","resolution":{"observed_at":"2026-08-02T01:54:25.860626Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2607.12010","last_updated":"2026-07-13T18:00:00Z","snapshot_observed_at":"2026-08-11T13:07:19.964733Z","submitted_at":"2026-07-13T18:00:00Z","title":"The Limitations of Cosmological Collider Analyses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2607.12010","snapshot_observed_at":"2026-08-02T01:54:25.947017Z","title":"The Limitations of Cosmological Col- lider Analyses,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:25.947017Z"},"links":{"cited_paper":"/paper/2607.12010","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:960f67aacdc1c4d5495a6a245a4edf8101cdb58dc0a5741b3905133dcd0c9b9f","observation_id":"a1128c7e-cf68-4242-810f-1023c063ffe9","resolution":{"observed_at":"2026-08-02T01:54:25.947017Z","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":"2026-08-02T01:54:26.112770Z","title":"Adiabatic and entropy perturbations from infla- tion,","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:26.112770Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:8e43da30b4ca1e73ad52cfe2c4dd51afecfce942b2b3bdcdbaa414bafaaa0e1a","observation_id":"915f00ac-444c-4379-bf5d-fd1c1c1c0a55","resolution":{"observed_at":"2026-08-02T01:54:26.112770Z","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":"2026-08-02T01:54:26.226716Z","title":"Scalar perturbations during multiple field slow-roll inflation,","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:26.226716Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:8f5edceb201d199d9983966032122d54c9866e3329ac665a664f24eb52e3b435","observation_id":"c460da0f-e2b6-4559-9662-e8ba744e5ef3","resolution":{"observed_at":"2026-08-02T01:54:26.226716Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0801.1085","last_updated":"2008-05-31T20:44:08Z","snapshot_observed_at":"2026-07-06T01:33:49.567180Z","submitted_at":"2008-01-07T18:06:07Z","title":"Perturbations in generalized multi-field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0801.1085","snapshot_observed_at":"2026-08-02T01:54:26.383206Z","title":"Perturbations in gen- eralized multi-field inflation,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:26.383206Z"},"links":{"cited_paper":"/paper/0801.1085","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:c04ee4859a7e1f2e01e2940b59a92f37b889b18b749979d8456b35a3300c4f63","observation_id":"f73271a5-f654-4f3f-b490-bd642c0d2332","resolution":{"observed_at":"2026-08-02T01:54:26.383206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0910.1853","last_updated":"2010-02-01T15:33:21Z","snapshot_observed_at":"2026-08-05T15:31:18.170612Z","submitted_at":"2009-10-12T19:22:42Z","title":"The Gelaton Scenario: Equilateral non-Gaussianity from multi-field dynamics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0910.1853","snapshot_observed_at":"2026-08-02T01:54:26.551316Z","title":"The Gelaton Scenario: Equilateral non-Gaussianity from multi-field dynam- ics,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:26.551316Z"},"links":{"cited_paper":"/paper/0910.1853","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:ee9a944129ab9a2ddfd04fdbb7c1da0e4509da2b0e0f4e5ab020fbe270c0892d","observation_id":"12a1ba09-5eab-4430-b633-dc7f8b5f1aa9","resolution":{"observed_at":"2026-08-02T01:54:26.551316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1010.3693","last_updated":"2011-05-26T02:12:27Z","snapshot_observed_at":"2026-08-13T04:42:23.283402Z","submitted_at":"2010-10-18T19:38:25Z","title":"Features of heavy physics in the CMB power spectrum","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1010.3693","snapshot_observed_at":"2026-08-02T01:54:26.719159Z","title":"Features of heavy physics in the CMB power spectrum,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:26.719159Z"},"links":{"cited_paper":"/paper/1010.3693","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:9df04aed27bf46a7efc57b3e0c825f0e850298ecebf45731d8fd96e9edc31c03","observation_id":"8ccae61a-a652-4be8-88e7-719f83a78948","resolution":{"observed_at":"2026-08-02T01:54:26.719159Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.5619","last_updated":"2013-05-30T00:20:13Z","snapshot_observed_at":"2026-08-03T21:30:55.824690Z","submitted_at":"2012-11-23T22:24:46Z","title":"Correlating features in the primordial spectra","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.5619","snapshot_observed_at":"2026-08-02T01:54:26.870561Z","title":"Correlating features in the primordial spectra,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:26.870561Z"},"links":{"cited_paper":"/paper/1211.5619","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:edd24d1d618321f1af9c9b4a5ff01c0e113edcc91709592b067607cbd5e6b5b2","observation_id":"632530a3-17ec-4dee-95b9-ec4ff2b59d3f","resolution":{"observed_at":"2026-08-02T01:54:26.870561Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1306.5680","last_updated":"2013-06-24T17:21:00Z","snapshot_observed_at":"2026-07-06T03:16:38.453054Z","submitted_at":"2013-06-24T17:21:00Z","title":"Oscillatory features in the curvature power spectrum after a sudden turn of the inflationary trajectory","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1306.5680","snapshot_observed_at":"2026-08-02T01:54:26.954961Z","title":"Oscillatory fea- tures in the curvature power spectrum after a sud- den turn of the inflationary trajectory,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:26.954961Z"},"links":{"cited_paper":"/paper/1306.5680","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:62160a2d79e10855ec445b6b086925bee378cf0d4d12cfb11498847cf1701c80","observation_id":"8c0568f5-b202-41fc-8b72-52201a658cb1","resolution":{"observed_at":"2026-08-02T01:54:26.954961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.2552","last_updated":"2015-10-16T14:47:17Z","snapshot_observed_at":"2026-08-13T14:58:48.141396Z","submitted_at":"2013-11-11T19:57:51Z","title":"Localized correlated features in the CMB power spectrum and primordial bispectrum from a transient reduction in the speed of sound","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.2552","snapshot_observed_at":"2026-08-02T01:54:27.064881Z","title":"Lo- calized correlated features in the CMB power spectrum and primordial bispectrum from a transient reduction in the speed of sound,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:27.064881Z"},"links":{"cited_paper":"/paper/1311.2552","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:f467f9b74b143f4414eeee7ec64b78db60a461f0bd6a4a9139710f9303a8beef","observation_id":"7675118a-a667-484e-b080-13a7c1156e55","resolution":{"observed_at":"2026-08-02T01:54:27.064881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.4257","last_updated":"2014-05-16T18:11:01Z","snapshot_observed_at":"2026-07-06T03:43:56.297161Z","submitted_at":"2014-05-16T18:11:01Z","title":"Combined features in the primordial spectra induced by a sudden turn in two-field DBI inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.4257","snapshot_observed_at":"2026-08-02T01:54:27.186754Z","title":"Combined fea- tures in the primordial spectra induced by a sudden turn in two-field DBI inflation,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:27.186754Z"},"links":{"cited_paper":"/paper/1405.4257","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:829a8997dcf2e34ef3611a5c41f364365da7b06576a1f7ae4e6d59bef657ee8e","observation_id":"f5d932d6-d523-4560-8de4-e5a12e7dafbc","resolution":{"observed_at":"2026-08-02T01:54:27.186754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1404.7522","last_updated":"2015-10-16T15:13:30Z","snapshot_observed_at":"2026-07-06T03:42:24.656546Z","submitted_at":"2014-04-29T20:45:06Z","title":"Inflation with moderately sharp features in the speed of sound: GSR and in-in formalism for power spectrum and bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1404.7522","snapshot_observed_at":"2026-08-02T01:54:27.446963Z","title":"Inflation with moderately sharp features in the speed of sound: Generalized slow roll and in-in formal- ism for power spectrum and bispectrum,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:27.446963Z"},"links":{"cited_paper":"/paper/1404.7522","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:c661cbb64120541a53e8c8980008ef14175fcc2a1323c920aeacefb07de0ff28","observation_id":"1f43bf6e-7c5f-4718-8faa-3d248e725208","resolution":{"observed_at":"2026-08-02T01:54:27.446963Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.08894","last_updated":"2015-08-29T00:26:43Z","snapshot_observed_at":"2026-07-06T04:22:21.682723Z","submitted_at":"2015-06-29T23:26:33Z","title":"Towards general patterns of features in multi-field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.08894","snapshot_observed_at":"2026-08-02T01:54:27.582713Z","title":"Towards general patterns of features in multi-field inflation,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:27.582713Z"},"links":{"cited_paper":"/paper/1506.08894","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:06f496dc71db16499db01da6db5ccb1c52d48461b868af79f0f470e9304ae85e","observation_id":"82760a19-a835-4923-9a0c-e4f59c2e875f","resolution":{"observed_at":"2026-08-02T01:54:27.582713Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.7110","last_updated":"2014-03-25T10:19:41Z","snapshot_observed_at":"2026-07-06T03:19:16.238811Z","submitted_at":"2013-07-26T17:34:51Z","title":"Primordial spectra from sudden turning trajectory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.7110","snapshot_observed_at":"2026-08-02T01:54:27.806152Z","title":"Primordial spectra from sudden turning trajectory,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:27.806152Z"},"links":{"cited_paper":"/paper/1307.7110","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:1fbc748b95cd287093954514dc19c2937d0b7728c7c80bde2b943a8161680689","observation_id":"fbe4f85d-0d26-49a3-8155-d8714fa5e48e","resolution":{"observed_at":"2026-08-02T01:54:27.806152Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.0161","last_updated":"2012-11-08T16:53:43Z","snapshot_observed_at":"2026-07-06T02:47:21.071404Z","submitted_at":"2012-05-01T14:02:35Z","title":"Curvature Perturbation Spectrum in Two-field Inflation with a Turning Trajectory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.0161","snapshot_observed_at":"2026-08-02T01:54:27.975789Z","title":"Curvature Perturbation Spectrum in Two-field Inflation with a Turning Trajectory,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:27.975789Z"},"links":{"cited_paper":"/paper/1205.0161","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:ad7b5b0c5f4a69a07c9bf58409b3eea4d2b53768b1bb7db935d85c52b65431e4","observation_id":"1535ed6d-bdae-4e91-b3fc-e16e99d5fe7c","resolution":{"observed_at":"2026-08-02T01:54:27.975789Z","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":"2026-08-02T01:54:28.146967Z","title":"Density perturbations and black hole formation in hybrid infla- tion,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:28.146967Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:be620b4c1256c5dee364c3207892185445e522578370d6b514d29bfa674eeb9b","observation_id":"e1f205f2-d39e-4d05-b9e8-2aa598725127","resolution":{"observed_at":"2026-08-02T01:54:28.146967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06106","last_updated":"2020-09-16T07:38:27Z","snapshot_observed_at":"2026-08-08T23:58:00.421591Z","submitted_at":"2020-04-13T17:59:59Z","title":"Seeding primordial black holes in multifield inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.06106","snapshot_observed_at":"2026-08-02T01:54:28.259624Z","title":"Seeding primordial black holes in multifield inflation,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:28.259624Z"},"links":{"cited_paper":"/paper/2004.06106","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:55530fcfec1c4811cd23e5257c6cf7461965ae304f65f7924e8be59a9f052d09","observation_id":"cfe0fc85-b2a9-49e2-9843-9c96eedb2ec5","resolution":{"observed_at":"2026-08-02T01:54:28.259624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.08369","last_updated":"2022-05-16T10:11:00Z","snapshot_observed_at":"2026-08-09T08:23:23.824701Z","submitted_at":"2020-04-16T17:57:17Z","title":"Turning in the landscape: a new mechanism for generating Primordial Black Holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.08369","snapshot_observed_at":"2026-08-02T01:54:28.442788Z","title":"Turning in the landscape: A new mechanism for generating primordial black holes,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:28.442788Z"},"links":{"cited_paper":"/paper/2004.08369","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:b44b1fdbd917ce56c74074d4c71aa4d682144f4997eba9a8e4d86fa97c894b86","observation_id":"7520fac4-527a-4cbc-b200-425cd14b9f79","resolution":{"observed_at":"2026-08-02T01:54:28.442788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.02895","last_updated":"2020-08-09T14:22:29Z","snapshot_observed_at":"2026-08-08T21:45:04.503013Z","submitted_at":"2020-05-06T15:15:39Z","title":"Generating PBHs and small-scale GWs in two-field models of inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.02895","snapshot_observed_at":"2026-08-02T01:54:28.551154Z","title":"Generating PBHs and small-scale GWs in two-field models of inflation,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:28.551154Z"},"links":{"cited_paper":"/paper/2005.02895","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:4d5a1b7b90d96d1b0f1230eea6d7c72cd0c9c8a4a2544b711b14030848492d0c","observation_id":"6441ae8c-eb1d-4c70-a59e-bc117bc3d26d","resolution":{"observed_at":"2026-08-02T01:54:28.551154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.12680","last_updated":"2023-12-21T05:33:10Z","snapshot_observed_at":"2026-08-13T17:09:20.299205Z","submitted_at":"2021-12-23T16:22:27Z","title":"Primordial Black Hole Formation in Non-Minimal Curvaton Scenario","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.12680","snapshot_observed_at":"2026-08-02T01:54:28.731834Z","title":"Primordial black hole formation in nonminimal curvaton scenarios,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:28.731834Z"},"links":{"cited_paper":"/paper/2112.12680","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:007d8a654391bf7904620f7c01a8c3f93cd474ac8bc453c9888ae5302670d41d","observation_id":"5e9270bb-eb33-46ac-a414-05049c607c1c","resolution":{"observed_at":"2026-08-02T01:54:28.731834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.03705","last_updated":"2021-05-25T20:01:49Z","snapshot_observed_at":"2026-08-02T06:36:34.489873Z","submitted_at":"2020-12-07T14:03:41Z","title":"On Primordial Black Holes from Rapid Turns in Two-field Models","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.03705","snapshot_observed_at":"2026-08-02T01:54:28.911413Z","title":"On Primordial Black Holes from Rapid Turns in Two-field Models,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:28.911413Z"},"links":{"cited_paper":"/paper/2012.03705","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:521af4b0c077800094f6c15c00352cc405b2cccf682f28eaf0efb011e00493eb","observation_id":"7933a70b-d68d-4478-ae0a-87cd05854222","resolution":{"observed_at":"2026-08-02T01:54:28.911413Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.04471","last_updated":"2022-09-29T16:24:18Z","snapshot_observed_at":"2026-08-13T15:47:34.454747Z","submitted_at":"2022-05-09T18:00:00Z","title":"Primordial Black Holes from Multifield Inflation with Nonminimal Couplings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.04471","snapshot_observed_at":"2026-08-02T01:54:29.046399Z","title":"Primordial black holes from multifield inflation with nonminimal couplings,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.046399Z"},"links":{"cited_paper":"/paper/2205.04471","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:7ae45e17699c20f3a30486f5332e08dea93c86fc8e99e45a20dfd779ecfd013e","observation_id":"01a9c8e5-a51f-4ced-a3c7-22966632e0e0","resolution":{"observed_at":"2026-08-02T01:54:29.046399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.13251","last_updated":"2025-04-17T18:00:01Z","snapshot_observed_at":"2026-08-07T16:01:20.235098Z","submitted_at":"2025-04-17T18:00:01Z","title":"Light Scalar Fields Foster Production of Primordial Black Holes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.13251","snapshot_observed_at":"2026-08-02T01:54:29.190715Z","title":"Light Scalar Fields Foster Production of Primordial Black Holes,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.190715Z"},"links":{"cited_paper":"/paper/2504.13251","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:f0aa790654a6c0fdf5f7feb40ac010f4ee8241dc4722acdcaf814524ba17e631","observation_id":"19f06a2c-13b5-416c-b4dd-68fe2112e3a6","resolution":{"observed_at":"2026-08-02T01:54:29.190715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.15605","last_updated":"2022-09-04T21:43:50Z","snapshot_observed_at":"2026-08-13T17:59:59.929528Z","submitted_at":"2022-03-29T14:13:45Z","title":"The effect of multiple features on the power spectrum in two-field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.15605","snapshot_observed_at":"2026-08-02T01:54:29.272913Z","title":"The effect of multiple features on the power spec- trum in two-field inflation,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.272913Z"},"links":{"cited_paper":"/paper/2203.15605","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:7f0b36a4668e235df92f07890b84ccdb466cbd7e00168ab5d3bc5e1b7bfc8a4f","observation_id":"77dcdf3b-db34-4ad5-afab-e592c10f4b9b","resolution":{"observed_at":"2026-08-02T01:54:29.272913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506056","last_updated":"2005-09-21T12:21:38Z","snapshot_observed_at":"2026-07-07T00:50:59.920722Z","submitted_at":"2005-06-02T12:10:52Z","title":"Primordial non-gaussianities from multiple-field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506056","snapshot_observed_at":"2026-08-02T01:54:29.360024Z","title":"Primordial non- Gaussianities from multiple-field inflation,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.360024Z"},"links":{"cited_paper":"/paper/astro-ph/0506056","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:dac1e5aa3c4c2fb155de0c00b20e8f4f55bd9f5d9c4458baed3583a6277b5f16","observation_id":"b376e4b6-bb6c-4580-afaa-364c5ee388fb","resolution":{"observed_at":"2026-08-02T01:54:29.360024Z","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":"2026-08-02T01:54:29.428909Z","title":"Large non-Gaussianity in multiple-field infla- tion,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.428909Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:c607d69efbec2ac69ef78188db3c1b803fd1d2f484d66bc541c03586feefd1e9","observation_id":"16c025a7-c4ab-4290-88d4-a3987f8825c6","resolution":{"observed_at":"2026-08-02T01:54:29.428909Z","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":"2026-08-02T01:54:29.514865Z","title":"Non-Gaussianities in two- field inflation,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.514865Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:6d19b277424dd3ed2512d96a718cf5aedb5a264428dd1ae69441abaa7785afaf","observation_id":"3fb8bbc8-cdda-4892-9f13-c73e1fc3203c","resolution":{"observed_at":"2026-08-02T01:54:29.514865Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0807.1101","last_updated":"2008-10-06T13:27:35Z","snapshot_observed_at":"2026-07-06T01:39:43.104039Z","submitted_at":"2008-07-07T20:04:58Z","title":"Conditions for large non-Gaussianity in two-field slow-roll inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0807.1101","snapshot_observed_at":"2026-08-02T01:54:29.597228Z","title":"Condi- tions for large non-Gaussianity in two-field slow-roll in- flation,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.597228Z"},"links":{"cited_paper":"/paper/0807.1101","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:3d4f369dc6aab4917ae67d890577b9376bc7921d7fe9b6c28b5c8cc315f6ac29","observation_id":"857ea66d-61ce-472a-bea7-c4876cbd0f73","resolution":{"observed_at":"2026-08-02T01:54:29.597228Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.12563","last_updated":"2018-11-06T17:54:13Z","snapshot_observed_at":"2026-08-08T05:18:07.976751Z","submitted_at":"2018-05-31T17:07:52Z","title":"Flattened non-Gaussianities from the effective field theory of inflation with imaginary speed of sound","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.12563","snapshot_observed_at":"2026-08-02T01:54:29.664363Z","title":"Flattened non- Gaussianities from the effective field theory of inflation with imaginary speed of sound,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.664363Z"},"links":{"cited_paper":"/paper/1805.12563","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:e1f578a6007107553a2786d780d667c0d7ae2e937a9b99845157bbbcf9be6795","observation_id":"1beb609b-b83c-4fb1-b158-a8310daac9d1","resolution":{"observed_at":"2026-08-02T01:54:29.664363Z","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":"2026-08-14T17:19:01.297760Z","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":"2026-08-02T01:54:29.742984Z","title":"Hyper-Non-Gaussianities in Inflation with Strongly Nongeodesic Motion,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.742984Z"},"links":{"cited_paper":"/paper/1902.03221","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:7098b6f47db4a425ff4bf8c25b196c9c915fb629ab7d3b4f3d260542a2c493aa","observation_id":"da097831-69f1-424c-b442-7e5f82c46f85","resolution":{"observed_at":"2026-08-02T01:54:29.742984Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.11316","last_updated":"2019-08-29T15:59:21Z","snapshot_observed_at":"2026-08-14T17:27:36.207279Z","submitted_at":"2019-08-29T15:59:21Z","title":"Mild Non-Gaussianities under Perturbative Control from Rapid-Turn Inflation Models","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.11316","snapshot_observed_at":"2026-08-02T01:54:29.818747Z","title":"Mild Non-Gaussianities under Perturbative Control from Rapid-Turn Inflation Models,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.818747Z"},"links":{"cited_paper":"/paper/1908.11316","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:cdddca76a05f51bbd1fcd16d0e32db8c48299bbf1fbda985c981f10b2354fcf8","observation_id":"9ca2f83d-afa3-4536-a032-58ec16ff64a3","resolution":{"observed_at":"2026-08-02T01:54:29.818747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10403","last_updated":"2020-02-09T18:04:22Z","snapshot_observed_at":"2026-08-14T16:02:54.138338Z","submitted_at":"2019-07-24T12:45:35Z","title":"Revisiting non-Gaussianity in multifield inflation with curved field space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10403","snapshot_observed_at":"2026-08-02T01:54:29.880100Z","title":"Revis- iting non-Gaussianity in multifield inflation with curved field space,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.880100Z"},"links":{"cited_paper":"/paper/1907.10403","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:961b0a020f50702f72547440f1e026d8f6c9eaed59e3f746950ea5c8f31eebcd","observation_id":"94d85f21-d6a4-4229-8813-d6587a25f08a","resolution":{"observed_at":"2026-08-02T01:54:29.880100Z","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":"2026-08-13T18:58:55.839905Z","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":"2026-08-02T01:54:29.935223Z","title":"Non- Gaussianity in rapid-turn multi-field inflation,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.935223Z"},"links":{"cited_paper":"/paper/2303.14156","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:51fda16f44c9546a5ecf1d90d11d894303960eede37a81752f0b46f5a9c32518","observation_id":"3346a9cd-963b-476c-ae0f-708f3e2ad949","resolution":{"observed_at":"2026-08-02T01:54:29.935223Z","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":"2026-08-02T01:54:29.983144Z","title":"Universal Non- Gaussian Signatures from Transient Instabilities,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:29.983144Z"},"links":{"citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:b332c4c66d9d382c066046b3a57b8310f9a0e69f4767139a738b03ab8492a3b5","observation_id":"b79cdac5-7d37-45e8-aea3-3ba0f9f004af","resolution":{"observed_at":"2026-08-02T01:54:29.983144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0704.0212","last_updated":"2007-07-13T19:45:32Z","snapshot_observed_at":"2026-07-06T01:25:48.402673Z","submitted_at":"2007-04-02T15:12:23Z","title":"Curvature and isocurvature perturbations in two-field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0704.0212","snapshot_observed_at":"2026-08-02T01:54:30.314692Z","title":"Curvature and isocurvature perturbations in two-field inflation,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:30.314692Z"},"links":{"cited_paper":"/paper/0704.0212","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:17208fedf3ed5324bbc3a7f5f7efc3147b9d58e9b23f8e77fd1e974db92fd568","observation_id":"ed1b821e-fa37-4d1c-83fb-1c82c6d5fe8b","resolution":{"observed_at":"2026-08-02T01:54:30.314692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.6163","last_updated":"2014-08-27T18:28:08Z","snapshot_observed_at":"2026-07-06T03:34:11.395413Z","submitted_at":"2014-01-23T20:55:31Z","title":"The effects of a fast-turning trajectory in multiple-field inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.6163","snapshot_observed_at":"2026-08-02T01:54:30.425785Z","title":"The effects of a fast-turning trajectory in multiple-field in- flation,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:30.425785Z"},"links":{"cited_paper":"/paper/1401.6163","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:64d26a499fd7d2e763316153346f5dd935d84b4f9e70e1caca2640164a90b08c","observation_id":"4fadd3d7-ad9f-40f1-9a97-ef1cfd8ef1e4","resolution":{"observed_at":"2026-08-02T01:54:30.425785Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-14T15:26:16.340562Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06956","snapshot_observed_at":"2026-08-02T01:54:30.518889Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:30.518889Z"},"links":{"cited_paper":"/paper/1908.06956","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:dc67b9acd85e483ffcc7ac29929178892a626316dc90760c95cde71bad2e6844","observation_id":"5d061c79-afd3-4d35-aeeb-bcb733a0a78b","resolution":{"observed_at":"2026-08-02T01:54:30.518889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.02761","last_updated":"2021-09-23T16:56:06Z","snapshot_observed_at":"2026-08-05T01:18:48.889560Z","submitted_at":"2020-12-04T18:27:25Z","title":"Oscillations in the stochastic gravitational wave background from sharp features and particle production during inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.02761","snapshot_observed_at":"2026-08-02T01:54:30.640953Z","title":"Oscillations in the stochastic gravitational wave back- ground from sharp features and particle production dur- ing inflation,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:30.640953Z"},"links":{"cited_paper":"/paper/2012.02761","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:9e3625f2d666c23982e15b70152ade4ee900a21a112d06a4d0bb09c854f71f54","observation_id":"384734c6-f8b3-4b1d-8c33-ee9660122224","resolution":{"observed_at":"2026-08-02T01:54:30.640953Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.09538","last_updated":"2022-02-09T10:13:27Z","snapshot_observed_at":"2026-08-13T17:50:27.955753Z","submitted_at":"2021-10-18T18:00:04Z","title":"Dark Matter from Entropy Perturbations in Curved Field Space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.09538","snapshot_observed_at":"2026-08-02T01:54:30.750477Z","title":"Dark matter from entropy perturbations in curved field space,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:30.750477Z"},"links":{"cited_paper":"/paper/2110.09538","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:cdb8c63e5020322f0334dd8628b151acfd50490f863386702bace879fbc9594e","observation_id":"2e13432c-715b-4244-82e5-9f5a6953ea59","resolution":{"observed_at":"2026-08-02T01:54:30.750477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08609","last_updated":"2017-04-18T15:32:51Z","snapshot_observed_at":"2026-07-06T05:05:18.656143Z","submitted_at":"2016-07-28T12:46:12Z","title":"Cumulative effects in inflation with ultra-light entropy modes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.08609","snapshot_observed_at":"2026-08-02T01:54:30.942258Z","title":"Cumulative effects in inflation with ultra-light entropy modes,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:30.942258Z"},"links":{"cited_paper":"/paper/1607.08609","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:ebfa7128292330948c9afa27ad1bb91883d67f1c405f857bbe05ee9086f8907e","observation_id":"d34bb537-e6e2-47df-8074-4786cc6c7390","resolution":{"observed_at":"2026-08-02T01:54:30.942258Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2603.03204","snapshot_observed_at":"2026-08-02T01:54:31.034762Z","title":"Ultra slow-turn inflation,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:31.034762Z"},"links":{"cited_paper":"/paper/2603.03204","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:46cf171db01dc89a349c88da4e71c3bb0a7920bb3e90d4d8e82467496ea8c534","observation_id":"937370d3-e9ee-49db-835f-e52e7dcbc8cf","resolution":{"observed_at":"2026-08-02T01:54:31.034762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.0363","last_updated":"2014-01-07T20:30:39Z","snapshot_observed_at":"2026-08-06T20:27:44.141907Z","submitted_at":"2013-04-01T14:29:46Z","title":"Multifield Inflation after Planck: The Case for Nonminimal Couplings","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.0363","snapshot_observed_at":"2026-08-02T01:54:31.126081Z","title":"Multifield Infla- tion after Planck: The Case for Nonminimal Cou- plings,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:31.126081Z"},"links":{"cited_paper":"/paper/1304.0363","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:0593aa7f8d71a1d1be0fed1bfbd7838dba9018bb3b9c34735ccec79b87b65b79","observation_id":"20d22aa3-0555-4ab4-bcb8-6f122ac579d9","resolution":{"observed_at":"2026-08-02T01:54:31.126081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.05125","last_updated":"2017-12-07T02:46:16Z","snapshot_observed_at":"2026-08-07T10:22:10.769742Z","submitted_at":"2017-07-17T12:53:24Z","title":"Primordial perturbations from inflation with a hyperbolic field-space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.05125","snapshot_observed_at":"2026-08-02T01:54:31.229754Z","title":"Primordial perturba- tions from inflation with a hyperbolic field-space,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:31.229754Z"},"links":{"cited_paper":"/paper/1707.05125","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:eea70839e3999ceb4d722a4802c0586558f725beb6c5c25d0d1262658b08494c","observation_id":"36573c54-9971-4e09-8d93-ec6ee0de0ff0","resolution":{"observed_at":"2026-08-02T01:54:31.229754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.05341","last_updated":"2019-04-22T04:02:23Z","snapshot_observed_at":"2026-07-06T07:02:12.971488Z","submitted_at":"2018-09-14T10:20:42Z","title":"Constraints on holographic multi-field inflation and models based on the Hamilton-Jacobi formalism","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.05341","snapshot_observed_at":"2026-08-02T01:54:31.393988Z","title":"Constraints on Holographic Multifield In- flation and Models Based on the Hamilton-Jacobi For- malism,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:31.393988Z"},"links":{"cited_paper":"/paper/1809.05341","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:a322868438c5b6e26bbd435bdaac76170c93de7955a64e8ffbefff0cc95e66de","observation_id":"0ea1f21d-ab65-40d3-ba1e-6baee651510d","resolution":{"observed_at":"2026-08-02T01:54:31.393988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12562","last_updated":"2019-10-17T02:21:17Z","snapshot_observed_at":"2026-08-14T16:24:20.985319Z","submitted_at":"2019-05-29T16:14:42Z","title":"Nonlinear Dynamics of Preheating after Multifield Inflation with Nonminimal Couplings","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12562","snapshot_observed_at":"2026-08-02T01:54:31.545564Z","title":"Nonlinear Dynamics of Preheat- ing after Multifield Inflation with Nonminimal Cou- plings,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:31.545564Z"},"links":{"cited_paper":"/paper/1905.12562","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:26ee3c860ce0bba6d3d5452e1b082b87fb5f0ec5db9313cc407e78e527b0223c","observation_id":"b0d6ca8b-6277-43a2-895d-6c484edf5b99","resolution":{"observed_at":"2026-08-02T01:54:31.545564Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.01281","last_updated":"2016-09-20T19:55:53Z","snapshot_observed_at":"2026-07-06T04:32:04.107898Z","submitted_at":"2015-10-05T18:50:13Z","title":"Geometrical Destabilization of Inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.01281","snapshot_observed_at":"2026-08-02T01:54:31.696955Z","title":"Geometrical Desta- bilization of Inflation,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:31.696955Z"},"links":{"cited_paper":"/paper/1510.01281","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:6e3b39977d86904425a3e441f0beb7faed6c9dc2fc31d970ebf75c5e46d999e3","observation_id":"4f332aa8-86fc-48e1-b27b-b3aa0c531c17","resolution":{"observed_at":"2026-08-02T01:54:31.696955Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.11279","last_updated":"2018-07-27T13:44:32Z","snapshot_observed_at":"2026-07-06T06:36:28.916734Z","submitted_at":"2018-04-30T15:37:04Z","title":"Primordial fluctuations and non-Gaussianities in sidetracked inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.11279","snapshot_observed_at":"2026-08-02T01:54:31.879041Z","title":"Primordial fluctuations and non-Gaussianities in sidetracked inflation,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:31.879041Z"},"links":{"cited_paper":"/paper/1804.11279","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:062bd792ea144d754866709f46f2eb6ff67889e647942ee1d35153ff772050fc","observation_id":"e9ee1b86-f45e-4702-a18e-aab22be74856","resolution":{"observed_at":"2026-08-02T01:54:31.879041Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.07495","last_updated":"2020-03-20T02:08:45Z","snapshot_observed_at":"2026-08-14T16:30:24.607089Z","submitted_at":"2019-05-17T22:35:46Z","title":"Multi-field Inflation in High-Slope Potentials","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.07495","snapshot_observed_at":"2026-08-02T01:54:32.017286Z","title":"Multi-field In- flation in High-Slope Potentials,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.017286Z"},"links":{"cited_paper":"/paper/1905.07495","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:7cd1cb683b7803e2ac793b7f6834267a6e917a1b332f38e78874ceff45c46e46","observation_id":"37b72122-38de-4c56-8ce6-263c22caa0c1","resolution":{"observed_at":"2026-08-02T01:54:32.017286Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.15933","last_updated":"2020-11-03T18:45:24Z","snapshot_observed_at":"2026-08-13T21:10:46.495000Z","submitted_at":"2020-10-29T20:47:24Z","title":"The Multi-Field, Rapid-Turn Inflationary Solution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.15933","snapshot_observed_at":"2026-08-02T01:54:32.079600Z","title":"The Multi- Field, Rapid-Turn Inflationary Solution,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.079600Z"},"links":{"cited_paper":"/paper/2010.15933","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:73cfcf8b8b49c2a3c70fc16558af9f34bc66dd69479cae9c04a5695c8a94b0ae","observation_id":"7f8c7acd-a752-48f9-86c8-4b2ae3f70133","resolution":{"observed_at":"2026-08-02T01:54:32.079600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.04090","last_updated":"2024-09-11T13:41:26Z","snapshot_observed_at":"2026-08-13T05:30:30.227942Z","submitted_at":"2023-11-07T16:00:25Z","title":"Enhanced power spectra from multi-field inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.04090","snapshot_observed_at":"2026-08-02T01:54:32.229496Z","title":"Enhanced power spectra from multi-field inflation,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.229496Z"},"links":{"cited_paper":"/paper/2311.04090","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:078d624beb4900f3030891ef1e3f17253081fe29713971cda291d38e16278f0e","observation_id":"afee496c-fa75-4432-a3fe-62e0def5a65d","resolution":{"observed_at":"2026-08-02T01:54:32.229496Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.11628","last_updated":"2024-09-05T08:39:56Z","snapshot_observed_at":"2026-08-13T00:04:15.062536Z","submitted_at":"2024-05-19T17:41:59Z","title":"Generalised conditions for rapid-turn inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.11628","snapshot_observed_at":"2026-08-02T01:54:32.369490Z","title":"Gener- alised conditions for rapid-turn inflation,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.369490Z"},"links":{"cited_paper":"/paper/2405.11628","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:f02c7df5a7c960eb8cfb71bc65425f28e04aacd065a82bbf49aac2a7815e7b97","observation_id":"91d2e9ce-2631-452c-872b-9c2536576e86","resolution":{"observed_at":"2026-08-02T01:54:32.369490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.11595","last_updated":"2024-09-05T07:45:46Z","snapshot_observed_at":"2026-08-13T00:04:16.755504Z","submitted_at":"2024-05-19T15:58:31Z","title":"On the Consistency of Rapid-Turn Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.11595","snapshot_observed_at":"2026-08-02T01:54:32.492984Z","title":"On the consistency of rapid-turn in- flation,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.492984Z"},"links":{"cited_paper":"/paper/2405.11595","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:8e93e688bb3489a2dc5654f7aae21f0d930cb83dda9abd996ee483967560563a","observation_id":"154aca21-4f6e-4f66-8999-3a11d373b2c7","resolution":{"observed_at":"2026-08-02T01:54:32.492984Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2606.18248","last_updated":"2026-07-21T14:36:20Z","snapshot_observed_at":"2026-08-12T20:08:05.318701Z","submitted_at":"2026-06-16T17:59:12Z","title":"Pushing the Primordial Frontier: Exact Linear Solutions in Multifield Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2606.18248","snapshot_observed_at":"2026-08-02T01:54:32.582062Z","title":"Pushing the Primordial Frontier: Exact Linear Solu- tions in Multifield Inflation,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.582062Z"},"links":{"cited_paper":"/paper/2606.18248","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:48653c22dbec4366f91b1d21060483e16052f15212377e4b28f15ef57942d2ac","observation_id":"488a24d6-7fb0-47f5-b821-591d9cd3020e","resolution":{"observed_at":"2026-08-02T01:54:32.582062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.4848","last_updated":"2012-05-07T14:21:49Z","snapshot_observed_at":"2026-07-06T02:41:38.149023Z","submitted_at":"2012-01-23T20:25:59Z","title":"On the importance of heavy fields during inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.4848","snapshot_observed_at":"2026-08-02T01:54:32.670361Z","title":"On the impor- tance of heavy fields during inflation,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.670361Z"},"links":{"cited_paper":"/paper/1201.4848","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:209588f8adfcd9dcb5508484b4b0debc8e5934d6ca0cf191ddf2c9ac4d49e9b4","observation_id":"1cdde501-bce6-43b3-b4f2-2767a5a1c530","resolution":{"observed_at":"2026-08-02T01:54:32.670361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.6342","last_updated":"2012-05-20T08:22:55Z","snapshot_observed_at":"2026-07-06T02:41:59.740159Z","submitted_at":"2012-01-30T20:34:02Z","title":"Effective theories of single field inflation when heavy fields matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.6342","snapshot_observed_at":"2026-08-02T01:54:32.755009Z","title":"Effective theories of single field infla- tion when heavy fields matter,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.755009Z"},"links":{"cited_paper":"/paper/1201.6342","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:e62a4ff5aab093ffb22ebddef727fb5ea7634cf994b4d396680bae35512ea1ec","observation_id":"da5154b7-e7fb-41c5-8eb9-75ce2fe653a3","resolution":{"observed_at":"2026-08-02T01:54:32.755009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.0710","last_updated":"2012-05-23T23:35:20Z","snapshot_observed_at":"2026-07-06T02:47:29.869838Z","submitted_at":"2012-05-03T13:42:58Z","title":"Heavy fields, reduced speeds of sound and decoupling during inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.0710","snapshot_observed_at":"2026-08-02T01:54:32.846382Z","title":"Heavy fields, reduced speeds of sound and decoupling during inflation,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.846382Z"},"links":{"cited_paper":"/paper/1205.0710","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:56da428d354870d86682302b79fb36667b3f9aee2c6ae4701c915f52a4d3a2cc","observation_id":"966adcfb-33d0-429b-af51-06dde0d1394c","resolution":{"observed_at":"2026-08-02T01:54:32.846382Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.13843","last_updated":"2025-03-12T23:30:40Z","snapshot_observed_at":"2026-08-12T22:20:39.547127Z","submitted_at":"2024-10-17T17:57:08Z","title":"Particle creation from non-geodesic trajectories in multifield inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.13843","snapshot_observed_at":"2026-08-02T01:54:32.941883Z","title":"Par- ticle creation from non-geodesic trajectories in multi- field inflation,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:32.941883Z"},"links":{"cited_paper":"/paper/2410.13843","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:7aedb8f798eb0e56c4fca7f5085f1929953439ca07d90226e582c00c590bb5b0","observation_id":"fb3a3a17-05e5-44fb-90bc-883079c64ff2","resolution":{"observed_at":"2026-08-02T01:54:32.941883Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.14664","last_updated":"2022-04-06T13:51:22Z","snapshot_observed_at":"2026-08-14T15:59:13.119387Z","submitted_at":"2021-11-29T16:22:33Z","title":"Primordial gravitational waves from excited states","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.14664","snapshot_observed_at":"2026-08-02T01:54:33.033479Z","title":"Primordial gravita- tional waves from excited states,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing","version":2},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-08-02T01:54:33.033479Z"},"links":{"cited_paper":"/paper/2111.14664","citing_paper":"/paper/2607.14529"},"observation_digest":"sha256:be5ffbce5b53b5fc67b10db9e63bc6d455b3ef41ce168f78124c56327cfd28f1","observation_id":"ee881bac-1978-41e8-bdd9-d03d3e65c703","resolution":{"observed_at":"2026-08-02T01:54:33.033479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.14529","last_updated":"2026-07-21T14:45:37Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-11T20:00:29.748380Z","submitted_at":"2026-07-16T03:30:36Z","title":"Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing"},"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":111},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 100 of 111 outbound references and 1 inbound Pith citation observation for arXiv:2607.14529."}