{"as_of":"2026-08-15T06:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e50c28636eccc50c0dae2e35c34a6c8c1d8f63a2b30091aef846655d0b39dfac","coverage":[{"denominator":51,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":51,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T12:42:27.080091Z","state":"measured"},{"denominator":56,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":56,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T10:29:34.588642Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-03T22:49:02.627727Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","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":"2026-08-14T10:29:34.588642Z","title":"Achucarro, G","venue":null,"work_id":null,"year":1908},"citing_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},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T10:29:34.588642Z"},"links":{"cited_paper":"/paper/1908.06956","citing_paper":"/paper/1908.11316"},"observation_digest":"sha256:87916906769c6663021defedc6dea84c15372534727ea3380d1079a2b22c0401","observation_id":"9b221db6-f2b0-4b99-a5b2-b000bdbaa208","resolution":{"observed_at":"2026-08-14T10:29:34.588642Z","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":"2026-08-15T00:01:26.483298Z","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":"2026-08-02T19:14:22.642631Z","title":"Ach´ ucarro, G.A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.03204","last_updated":"2026-06-24T10:11:04Z","snapshot_observed_at":"2026-08-07T18:13:08.430083Z","submitted_at":"2026-03-03T17:57:50Z","title":"Ultra slow-turn inflation","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-02T19:14:22.642631Z"},"links":{"cited_paper":"/paper/1908.06956","citing_paper":"/paper/2603.03204"},"observation_digest":"sha256:8e24c87471c7272038b6ca830d0575ab6ec2be21894811ea4fb8d419545105db","observation_id":"b83c920c-cc48-48b8-8d18-0a2d9aa4139e","resolution":{"observed_at":"2026-08-02T19:14:22.642631Z","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":"2026-08-15T00:01:26.483298Z","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":"1908.06956","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.06956","snapshot_observed_at":"2026-07-03T22:49:02.627727Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity,","venue":null,"work_id":"1c21bb49-db83-453c-8e27-dbabd86f3577","year":2020},"citing_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":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-26T23:14:24.235897Z"},"links":{"cited_paper":"/paper/1908.06956","citing_paper":"/paper/2606.18248"},"observation_digest":"sha256:b2674d1617ab2c2730bed6d7e75eeb630aec46ec29e99ff55d7ab55267e3b46e","observation_id":"72ac499b-e8f0-47e2-bd7c-132580cf9e2a","resolution":{"observed_at":"2026-07-03T22:49:02.630842Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","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":"2026-08-02T11:07:11.804811Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity,","venue":null,"work_id":null,"year":2020},"citing_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},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-02T11:07:11.804811Z"},"links":{"cited_paper":"/paper/1908.06956","citing_paper":"/paper/2606.18248"},"observation_digest":"sha256:d956b88c04a2cd3a3efe06abe42c7d4ed127d8afe2f49b4f13d17e59af0aae6a","observation_id":"97374279-ed70-4211-b1f8-df02350b4feb","resolution":{"observed_at":"2026-08-02T11:07:11.804811Z","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":"2026-08-15T00:01:26.483298Z","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":"sha256:9f10d5b3dd30de0add23273605d72ea3fe86aa455b693c2c199d7f707c08aa3e","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"}}],"links":{"evidence":"/evidence","html":"/paper/1908.06956/citation-record","integrity":"/paper/1908.06956/integrity","json":"/paper/1908.06956/citation-record.json","paper":"/paper/1908.06956"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T12:42:27.797186Z","title":"ultra-light isocurvature","venue":null,"work_id":"8705e40d-a5bb-42b7-b559-d8324dc85bc4","year":null},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.870129Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:19e926949af69204de8bcb9e938b0ff515a5cbabbe20dc62150c5dba48b84ef9","observation_id":"3d07fe1a-571b-4c0a-8ec8-37ca4f46858f","resolution":{"observed_at":"2026-08-14T12:42:27.802154Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T12:42:27.782765Z","title":"The most readily available example is given by the choice G(s) = w2 0(3 − 2β2/s2)","venue":null,"work_id":"792dcbdd-4f0f-434e-a6e8-513a047bff65","year":null},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.875626Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:878b2eed1f3b090a93787ada36e7312d455462365a599b47df0e0e261971f7e5","observation_id":"745d9d22-bae7-43ca-bd0b-580b1618b687","resolution":{"observed_at":"2026-08-14T12:42:27.787303Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T12:42:27.769141Z","title":"ultra-light isocurvature","venue":null,"work_id":"1bbd1275-66ff-4d9a-bbd1-77a11d49717f","year":2020},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.879562Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:49e7712c307cc9a2ee0345febcbb2f0f55d04506adf77c7b5c64a303879f1186","observation_id":"04ddbadb-4966-4e54-9a98-31fe4b3271da","resolution":{"observed_at":"2026-08-14T12:42:27.773253Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.08609","last_updated":"2017-04-18T15:32:51Z","snapshot_observed_at":"2026-08-14T21:46:25.310134Z","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":"2026-08-14T12:42:26.885182Z","title":"Ach´ ucarro, V","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.885182Z"},"links":{"cited_paper":"/paper/1607.08609","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:ed28d0c6de336d81d1f874de5d23fb6c20c860d6341eaf6db598883097761e3f","observation_id":"e3abebc7-8e0f-4976-9984-877e4e4ae256","resolution":{"observed_at":"2026-08-14T12:42:26.885182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03657","last_updated":"2020-07-24T14:42:51Z","snapshot_observed_at":"2026-08-14T20:39:35.571812Z","submitted_at":"2019-01-11T17:22:42Z","title":"Shift-Symmetric Orbital Inflation: single field or multi-field?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.03657","snapshot_observed_at":"2026-08-14T12:42:26.889571Z","title":"Ach´ ucarro, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.889571Z"},"links":{"cited_paper":"/paper/1901.03657","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:864ce418020f3db967fc38c44608871660f0d19dbc8a4b1a2e1226914edd3858","observation_id":"76b9d493-2258-4e1b-8774-6c9aabbabf9e","resolution":{"observed_at":"2026-08-14T12:42:26.889571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0405103","last_updated":"2004-05-26T17:29:47Z","snapshot_observed_at":"2026-07-07T04:03:37.926682Z","submitted_at":"2004-05-12T13:14:51Z","title":"Non-Gaussian perturbations in hybrid inflation","version":2},"cited_work":{"arxiv_id":"hep-ph/0405103","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0405103","snapshot_observed_at":"2026-08-14T12:42:27.671425Z","title":"Non-Gaussian perturbations in hybrid inflation","venue":"hep-ph","work_id":"6a108392-72cb-499b-a434-b7e6fed9895d","year":2004},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.893832Z"},"links":{"cited_paper":"/paper/hep-ph/0405103","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:deccab0e714a96da45b58f06e10aeb86349314df0653f90328caee656979ae83","observation_id":"e821de60-e558-4fc8-8158-24994b04ab28","resolution":{"observed_at":"2026-08-14T12:42:27.677404Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"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":"2026-08-14T12:42:26.897494Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.897494Z"},"links":{"cited_paper":"/paper/astro-ph/0504045","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:0d3c6b9c7975f5f36db4c7fab77eceeb449ea27c448155e81a13f8e75f40db7e","observation_id":"72f5e0a3-9600-468c-bf1a-a41543d22861","resolution":{"observed_at":"2026-08-14T12:42:26.897494Z","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":"2026-08-14T12:42:26.900946Z","title":"Seery and J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.900946Z"},"links":{"cited_paper":"/paper/astro-ph/0506056","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:e56e252ae66215746a6c8028e63799298265d8cfd46e64dd6d2bbfacc4ef39c7","observation_id":"dfbec5db-bd6a-460e-8812-ea45337ef280","resolution":{"observed_at":"2026-08-14T12:42:26.900946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0506704","last_updated":"2006-05-05T15:11:44Z","snapshot_observed_at":"2026-07-07T00:51:43.193510Z","submitted_at":"2005-06-28T19:56:40Z","title":"Large non-Gaussianity in multiple-field inflation","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0506704","snapshot_observed_at":"2026-08-14T12:42:26.904693Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.904693Z"},"links":{"cited_paper":"/paper/astro-ph/0506704","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:89a7e9f2d80ef61bbcb7dee2b44f488e51c0cbe731092001858e40697231ac0f","observation_id":"07189507-9892-466e-95a5-ab446553239f","resolution":{"observed_at":"2026-08-14T12:42:26.904693Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510441","last_updated":"2005-12-01T12:55:40Z","snapshot_observed_at":"2026-08-12T22:13:39.190797Z","submitted_at":"2005-10-14T15:28:25Z","title":"Inflation models and observation","version":2},"cited_work":{"arxiv_id":"astro-ph/0510441","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0510441","snapshot_observed_at":"2026-08-14T12:42:27.615023Z","title":"Inflation models and observation","venue":"astro-ph","work_id":"d43e1134-c6aa-4b13-954f-35fd2dcfba8e","year":2005},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.908467Z"},"links":{"cited_paper":"/paper/astro-ph/0510441","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:ad3f57702ad1899312586bc007d8bcc63de9ad37d0ab19aa355baefbf3b6ac7d","observation_id":"9cc47e32-7024-45aa-be7d-44d84400a340","resolution":{"observed_at":"2026-08-14T12:42:27.619476Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0703012","last_updated":"2007-05-06T11:40:44Z","snapshot_observed_at":"2026-07-07T05:00:10.656873Z","submitted_at":"2007-03-02T18:14:26Z","title":"Non-Gaussianities in N-flation","version":3},"cited_work":{"arxiv_id":"hep-th/0703012","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0703012","snapshot_observed_at":"2026-08-14T12:42:27.597695Z","title":"Non-Gaussianities in N-flation","venue":"hep-th","work_id":"a80f952b-38ff-4300-82de-c5dfea715bb8","year":2007},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.912012Z"},"links":{"cited_paper":"/paper/hep-th/0703012","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:e77d94a99b843a2ee74b5397054167b97478e1d31e555bc4c6ef72aec1f0de79","observation_id":"2f8c1eb3-0efe-4067-9c89-c0c7815f9a4a","resolution":{"observed_at":"2026-08-14T12:42:27.602048Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0701247","last_updated":"2007-02-23T12:50:01Z","snapshot_observed_at":"2026-08-14T11:09:54.647669Z","submitted_at":"2007-01-09T19:08:57Z","title":"Spectral Running and Non-Gaussianity from Slow-Roll Inflation in Generalised Two--Field Models","version":2},"cited_work":{"arxiv_id":"astro-ph/0701247","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0701247","snapshot_observed_at":"2026-08-14T12:42:27.573158Z","title":"Spectral Running and Non-Gaussianity from Slow-Roll Inflation in Generalised Two--Field Models","venue":"astro-ph","work_id":"563027de-2f1d-4c22-a4c9-5c46375ec6dc","year":2007},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.915518Z"},"links":{"cited_paper":"/paper/astro-ph/0701247","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:6ef5a6a679f131527168091963c94872430086500c2d646847255675f3621474","observation_id":"263c60c1-6f8c-4cdd-b68a-7b6f7371df8e","resolution":{"observed_at":"2026-08-14T12:42:27.578075Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"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":"2026-08-14T12:42:26.919361Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.919361Z"},"links":{"cited_paper":"/paper/0807.1101","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:dee658b449a567ae4ec47cfb367b52c6bd1fe1680d4261a9a8b04d0d14d2f1ec","observation_id":"b64a0fdf-ab27-4876-babf-ddc4362cc4f0","resolution":{"observed_at":"2026-08-14T12:42:26.919361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0906.0767","last_updated":"2011-11-03T10:07:52Z","snapshot_observed_at":"2026-08-15T05:46:56.950330Z","submitted_at":"2009-06-04T12:39:59Z","title":"Non-Gaussianity beyond slow roll in multi-field inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0906.0767","snapshot_observed_at":"2026-08-14T12:42:26.923513Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.923513Z"},"links":{"cited_paper":"/paper/0906.0767","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:dd01372a4cf6515a87a09e585a358f201d39274a96a564a91e5b93746be9b976","observation_id":"cdfe307f-d16e-4c9e-8e53-d413b01122cc","resolution":{"observed_at":"2026-08-14T12:42:26.923513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0908.4269","last_updated":"2011-11-03T09:02:48Z","snapshot_observed_at":"2026-08-15T05:40:13.793397Z","submitted_at":"2009-08-31T18:46:20Z","title":"On Non-Gaussianities in Multi-Field Inflation (N fields): Bi- and Tri-spectra beyond Slow-Roll","version":3},"cited_work":{"arxiv_id":"0908.4269","doi":null,"metadata_source":"pith","pith_arxiv_id":"0908.4269","snapshot_observed_at":"2026-08-14T12:42:27.527010Z","title":"On Non-Gaussianities in Multi-Field Inflation (N fields): Bi- and Tri-spectra beyond Slow-Roll","venue":"hep-th","work_id":"825b7dd2-709e-4733-9f3d-5d04ba0185d5","year":2009},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.927856Z"},"links":{"cited_paper":"/paper/0908.4269","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:6a994105bec1eec455ff60536a69c2f9ed321289fd00a23a10d41b90f9ce5179","observation_id":"5f46997a-150e-494a-9c15-bfa5ca761552","resolution":{"observed_at":"2026-08-14T12:42:27.532560Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0909.0496","last_updated":"2010-03-03T19:05:30Z","snapshot_observed_at":"2026-08-15T05:40:00.337791Z","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":"2026-08-14T12:42:26.931942Z","title":"Chen and Y","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.931942Z"},"links":{"cited_paper":"/paper/0909.0496","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:53169226604a0e94eac650b99173343e44074e8ebad3d3c0674a04b69b58d7d9","observation_id":"dae1c626-3cb0-4fed-8ce4-4723ba75c97b","resolution":{"observed_at":"2026-08-14T12:42:26.931942Z","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":"2026-08-15T05:33:40.837974Z","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":"2026-08-14T12:42:26.935868Z","title":"Chen and Y","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.935868Z"},"links":{"cited_paper":"/paper/0911.3380","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:06e67e8207e3c51d4d56bb10ff2302bc38b3e6457996d9ee7354f75ceab31de3","observation_id":"6be7a031-b5ea-4fed-812f-cf72832c1e82","resolution":{"observed_at":"2026-08-14T12:42:26.935868Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1107.2270","last_updated":"2011-07-12T12:56:56Z","snapshot_observed_at":"2026-08-15T04:41:22.847668Z","submitted_at":"2011-07-12T12:56:56Z","title":"Evolution of non-Gaussianity in multi-scalar field models","version":1},"cited_work":{"arxiv_id":"1107.2270","doi":null,"metadata_source":"pith","pith_arxiv_id":"1107.2270","snapshot_observed_at":"2026-08-14T12:42:27.479663Z","title":"Evolution of non-Gaussianity in multi-scalar field models","venue":"astro-ph.CO","work_id":"6f9db094-1bf2-4bce-b554-e1f180e32b1b","year":2011},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.940313Z"},"links":{"cited_paper":"/paper/1107.2270","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:4875560fcedd80cc18b4d4fbbd77a79ccd0a5ebb0d5e30aeb111176cf47dca96","observation_id":"07df4e58-3b02-462d-88b2-65e988f189dc","resolution":{"observed_at":"2026-08-14T12:42:27.485273Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1107.4739","last_updated":"2011-07-24T09:15:22Z","snapshot_observed_at":"2026-08-15T04:40:07.209546Z","submitted_at":"2011-07-24T09:15:22Z","title":"Non-Gaussianity from the hybrid potential","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1107.4739","snapshot_observed_at":"2026-08-14T12:42:26.944741Z","title":"Mulryne, S","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.944741Z"},"links":{"cited_paper":"/paper/1107.4739","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:dc47a0fc33af6a3b9dfdbe9003a385e222d92b090ec58a48288f1c86b67ca259","observation_id":"5a48cac4-8d6c-4be5-bd8a-55421644d653","resolution":{"observed_at":"2026-08-14T12:42:26.944741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.0317","last_updated":"2012-10-02T12:11:46Z","snapshot_observed_at":"2026-08-15T00:54:42.834048Z","submitted_at":"2012-07-02T09:36:59Z","title":"A Statistical Approach to Multifield Inflation: Many-field Perturbations Beyond Slow Roll","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.0317","snapshot_observed_at":"2026-08-14T12:42:26.948710Z","title":"McAllister, S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.948710Z"},"links":{"cited_paper":"/paper/1207.0317","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:7f734eb2006969a0176633b458f5cfa98cc3857c0cd7f4754b0d8328d789a2a6","observation_id":"3131fa77-671f-4ebe-8194-625d6bc7c707","resolution":{"observed_at":"2026-08-14T12:42:26.948710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.1851","last_updated":"2012-11-27T12:33:03Z","snapshot_observed_at":"2026-08-15T00:44:08.143707Z","submitted_at":"2012-10-05T20:00:08Z","title":"General formula for the running of local fNL","version":2},"cited_work":{"arxiv_id":"1210.1851","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.1851","snapshot_observed_at":"2026-08-14T12:42:27.426503Z","title":"General formula for the running of local fNL","venue":"astro-ph.CO","work_id":"565f7d43-39f0-44e4-817c-a8d92bc91057","year":2012},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.952058Z"},"links":{"cited_paper":"/paper/1210.1851","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:29245c254ebd6bc067237d9987489433eecff55b70f09525301c85aeab3a2491","observation_id":"69df8c62-0552-4692-b16c-4de553a3228c","resolution":{"observed_at":"2026-08-14T12:42:27.431874Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1109.0292","last_updated":"2011-10-11T21:00:21Z","snapshot_observed_at":"2026-08-15T04:36:40.404246Z","submitted_at":"2011-09-01T20:02:27Z","title":"Signatures of Supersymmetry from the Early Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.0292","snapshot_observed_at":"2026-08-14T12:42:26.956518Z","title":"Baumann and D","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.956518Z"},"links":{"cited_paper":"/paper/1109.0292","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:14c437e254646f3656f9dcabf5f6208e75d73fda3f646129538009c3324b8725","observation_id":"eca24500-6a8d-4f53-93bc-e43efc3e6f71","resolution":{"observed_at":"2026-08-14T12:42:26.956518Z","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":"2026-08-14T22:54:41.272868Z","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":"2026-08-14T12:42:26.960392Z","title":"Arkani-Hamed and J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.960392Z"},"links":{"cited_paper":"/paper/1503.08043","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:01bff2fa43f902be3f9e70b82a828b21381f45f94fc47eb6ff9147eb0fa48c5b","observation_id":"1e952d94-7c96-4d24-aeac-64985c8a7e36","resolution":{"observed_at":"2026-08-14T12:42:26.960392Z","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":"2026-08-14T21:48:35.067063Z","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":"2026-08-14T12:42:26.964305Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.964305Z"},"links":{"cited_paper":"/paper/1607.03735","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:f11656edcfef13af5a5e91202c58142595566d6bbff3401a2eb47342e1ee7102","observation_id":"8aca6017-5b68-452f-b891-6917a0cd0f25","resolution":{"observed_at":"2026-08-14T12:42:26.964305Z","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":"2026-08-14T19:24:08.577400Z","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":"2026-08-14T12:42:26.968743Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.968743Z"},"links":{"cited_paper":"/paper/1804.07315","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:ada1d9c3d9678201cd901e1d4c300240576b0c3b03d1e120707bbccbd2bc9916","observation_id":"d2edd7ff-af0d-45c0-9120-9f8c8c9fbaed","resolution":{"observed_at":"2026-08-14T12:42:26.968743Z","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":"2026-08-14T19:04:05.134758Z","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":"2026-08-14T12:42:26.974910Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.974910Z"},"links":{"cited_paper":"/paper/1806.05202","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:fff0312ab30de2e31d3f05845d9b66e91b7607ca4be004d750ba29c5fa4e0a72","observation_id":"32869a2b-0937-4b31-8859-5329e7777654","resolution":{"observed_at":"2026-08-14T12:42:26.974910Z","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":"2026-08-14T19:20:31.844053Z","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":"2026-08-14T12:42:26.979346Z","title":"Garcia-Saenz, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.979346Z"},"links":{"cited_paper":"/paper/1804.11279","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:13ecd02049e9fa530b99a90ba8481624f974670af8e87906f037f04180e2612c","observation_id":"5f981d60-b37a-4dd8-9619-6c1dd1040cc9","resolution":{"observed_at":"2026-08-14T12:42:26.979346Z","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":"2026-08-14T12:42:26.983989Z","title":"Fumagalli, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.983989Z"},"links":{"cited_paper":"/paper/1902.03221","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:70ff1a91329359a5115c73d2b3826b55fb04cfeb5bc395fb6274f45ab3de2ba9","observation_id":"71a53a9e-ea7a-4df4-934b-9efc4953e551","resolution":{"observed_at":"2026-08-14T12:42:26.983989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.02020","last_updated":"2019-07-03T16:37:50Z","snapshot_observed_at":"2026-08-01T17:23:18.409994Z","submitted_at":"2019-07-03T16:37:50Z","title":"Orbital Inflation: inflating along an angular isometry of field space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.02020","snapshot_observed_at":"2026-08-14T12:42:26.988310Z","title":"Achcarro and Y","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.988310Z"},"links":{"cited_paper":"/paper/1907.02020","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:b91b8cdca96dabfbcef3a2deaf8acc3477fee62b074695c1c2623f64bca3fcc7","observation_id":"996d2499-a94a-458c-b3ac-c989e254ff5c","resolution":{"observed_at":"2026-08-14T12:42:26.988310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.02951","last_updated":"2019-07-04T12:09:44Z","snapshot_observed_at":"2026-08-14T16:08:49.224835Z","submitted_at":"2019-07-04T12:09:44Z","title":"A simple, exact, model of quasi-single field inflation","version":1},"cited_work":{"arxiv_id":"1907.02951","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.02951","snapshot_observed_at":"2026-08-14T12:42:27.299058Z","title":"A simple, exact, model of quasi-single field inflation","venue":"astro-ph.CO","work_id":"49386fb0-1b1d-41b1-aeee-f63f33e1efb4","year":2019},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.992737Z"},"links":{"cited_paper":"/paper/1907.02951","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:c5c9c1088c4724d05d72ccf88eab88f9d0929c7bbe10ac0039b346f6c96c626c","observation_id":"d203c8be-b7e6-4bf0-b338-f19536629a5a","resolution":{"observed_at":"2026-08-14T12:42:27.303298Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"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":"2026-08-14T12:42:26.997021Z","title":"Garcia-Saenz, L","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:26.997021Z"},"links":{"cited_paper":"/paper/1907.10403","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:92d4889fffbc7013aa51b56b319ab1bf6a41bac331a2424cfa58cc1b413f3f4a","observation_id":"821399e0-3ce7-4b80-8488-415195687ca0","resolution":{"observed_at":"2026-08-14T12:42:26.997021Z","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":"2026-08-14T12:42:27.000619Z","title":null,"venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.000619Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:8688fa786f89c9d05263b2af32e2d8343ff493f93befe279503a06a6f875bb0f","observation_id":"cd65d465-dab6-4a3c-961b-cf87c0079f00","resolution":{"observed_at":"2026-08-14T12:42:27.000619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T12:42:27.746879Z","title":null,"venue":null,"work_id":"e85fea89-d99c-4343-8a91-d6b043bc97b0","year":1980},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.004217Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:e335249ffa8792362f9470c883ec3a39b1c3cf41e151c118b7a2da61d742bfff","observation_id":"f489caf0-0842-4332-98b5-1e4dbe81f337","resolution":{"observed_at":"2026-08-14T12:42:27.752125Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T12:42:27.731286Z","title":null,"venue":null,"work_id":"0fba8833-3f82-4e74-a2d3-22c3f3160e80","year":1982},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.007947Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:6386fbaa4c628f86dd0f1ba6bd5d33666644fce398bb0c898501dd1d47110d67","observation_id":"2cf64675-8d8d-445f-96fd-3c11c6cb3dd9","resolution":{"observed_at":"2026-08-14T12:42:27.735817Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T12:42:27.011172Z","title":"Albrecht and P","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.011172Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:463210ce5f6b858092c21cccd39e7fce7edf9a1d3ab244a0cbde43d315773983","observation_id":"506733d9-6161-4f54-8b45-1fa9f38a635e","resolution":{"observed_at":"2026-08-14T12:42:27.011172Z","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":"2026-08-14T12:42:27.014423Z","title":null,"venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.014423Z"},"links":{"citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:64aa720c1923c325cdf20686ac84de45d01d5b296c28346ffb67205c358bbe34","observation_id":"0b77a7e9-37c0-4c66-95ae-9d233c4d2346","resolution":{"observed_at":"2026-08-14T12:42:27.014423Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0009131","last_updated":"2000-11-10T10:32:31Z","snapshot_observed_at":"2026-08-08T10:58:28.486634Z","submitted_at":"2000-09-08T08:34:53Z","title":"Adiabatic and entropy perturbations from inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0009131","snapshot_observed_at":"2026-08-14T12:42:27.018197Z","title":"Gordon, D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.018197Z"},"links":{"cited_paper":"/paper/astro-ph/0009131","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:2070e1a02ab01fc77374cda214b355352b0d5a91cd54610b88acd846a17b3a5a","observation_id":"c51c21ca-3b7d-4475-a8a8-75c9d3fec741","resolution":{"observed_at":"2026-08-14T12:42:27.018197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0011325","last_updated":"2000-12-13T12:34:44Z","snapshot_observed_at":"2026-07-07T03:50:36.913744Z","submitted_at":"2000-11-27T18:50:41Z","title":"Density perturbations arising from multiple field slow-roll inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0011325","snapshot_observed_at":"2026-08-14T12:42:27.022201Z","title":"Groot Nibbelink and B","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.022201Z"},"links":{"cited_paper":"/paper/hep-ph/0011325","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:d95ee7a5fb4064c0926427e37cd08544b991e7725aac87c8d15dfa0d28b5a1d9","observation_id":"324a3571-5950-4f80-96cc-4e8721609434","resolution":{"observed_at":"2026-08-14T12:42:27.022201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0107272","last_updated":"2002-03-22T17:59:54Z","snapshot_observed_at":"2026-07-07T03:53:09.825040Z","submitted_at":"2001-07-26T12:39:58Z","title":"Scalar perturbations during multiple-field slow-roll inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-ph/0107272","snapshot_observed_at":"2026-08-14T12:42:27.026716Z","title":"Groot Nibbelink and B","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.026716Z"},"links":{"cited_paper":"/paper/hep-ph/0107272","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:61b368ab56aafdf064de59e606f2f8258a91a9232cfe3280abfbfffd078d4a63","observation_id":"cbccc555-d13d-485a-ac8f-b54f90498cf8","resolution":{"observed_at":"2026-08-14T12:42:27.026716Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1005.3848","last_updated":"2011-05-25T21:11:33Z","snapshot_observed_at":"2026-08-15T05:18:31.183791Z","submitted_at":"2010-05-20T21:59:18Z","title":"Mass hierarchies and non-decoupling in multi-scalar field dynamics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1005.3848","snapshot_observed_at":"2026-08-14T12:42:27.030541Z","title":"Achucarro, J.-O","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.030541Z"},"links":{"cited_paper":"/paper/1005.3848","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:70a7fab18c1fe957a36062a5a2d8f702c78a64b8298c2fea3325842bdcd11178","observation_id":"5a2cd1ab-9d0e-4cf3-8808-bb072d343845","resolution":{"observed_at":"2026-08-14T12:42:27.030541Z","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":"2026-08-15T05:05:32.390160Z","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":"2026-08-14T12:42:27.034524Z","title":"Achucarro, J.-O","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.034524Z"},"links":{"cited_paper":"/paper/1010.3693","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:7a0ae111bc4085cd2d9e2e05854fda303cc17550c31b76acf5025dc8c9d3663d","observation_id":"a602765f-4b04-4da0-816b-2d543b1be9bb","resolution":{"observed_at":"2026-08-14T12:42:27.034524Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.5174","last_updated":"2011-12-21T21:12:46Z","snapshot_observed_at":"2026-08-15T04:24:46.778276Z","submitted_at":"2011-12-21T21:12:46Z","title":"Spontaneous Symmetry Probing","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.5174","snapshot_observed_at":"2026-08-14T12:42:27.039478Z","title":"Nicolis and F","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.039478Z"},"links":{"cited_paper":"/paper/1112.5174","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:0e6805bdbcfe9b79fcbf4299789297f96c05a3a09277db55be0f5f758829e697","observation_id":"a7b065ed-3c98-4c0f-96c9-fa3215a011eb","resolution":{"observed_at":"2026-08-14T12:42:27.039478Z","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":"2026-08-14T12:42:27.043721Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.043721Z"},"links":{"cited_paper":"/paper/astro-ph/0210603","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:23c36cefb00384deed06a8682d1817490b28ade777cef0e859f41b2588aff57f","observation_id":"19ddc83a-26de-43d3-be9b-8d90111f7baa","resolution":{"observed_at":"2026-08-14T12:42:27.043721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0407059","last_updated":"2004-10-19T15:07:58Z","snapshot_observed_at":"2026-07-07T00:43:25.239869Z","submitted_at":"2004-07-02T20:01:02Z","title":"Single field consistency relation for the 3-point function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0407059","snapshot_observed_at":"2026-08-14T12:42:27.048500Z","title":"Creminelli and M","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.048500Z"},"links":{"cited_paper":"/paper/astro-ph/0407059","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:3fa3b4226a83f05033dbcda771d7306db5b95802f85875148ac357d0963a7359","observation_id":"438cbd56-1ed6-4718-8f37-d2fad8a950a5","resolution":{"observed_at":"2026-08-14T12:42:27.048500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0295","last_updated":"2008-03-05T15:13:42Z","snapshot_observed_at":"2026-07-06T01:33:44.168354Z","submitted_at":"2007-09-04T19:05:06Z","title":"On the consistency relation of the 3-point function in single field inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.0295","snapshot_observed_at":"2026-08-14T12:42:27.053504Z","title":"Cheung, A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.053504Z"},"links":{"cited_paper":"/paper/0709.0295","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:e73fdb86ad803f6aa8b7e0738f0d533ffcc3762a9c89f57216ce10a33701824e","observation_id":"39966d0b-21fe-419e-81aa-e47886153d7c","resolution":{"observed_at":"2026-08-14T12:42:27.053504Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02680","last_updated":"2018-05-14T15:09:53Z","snapshot_observed_at":"2026-08-14T20:15:58.037616Z","submitted_at":"2017-11-07T19:00:37Z","title":"A generalized non-Gaussian consistency relation for single field inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.02680","snapshot_observed_at":"2026-08-14T12:42:27.057671Z","title":"Bravo, S","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.057671Z"},"links":{"cited_paper":"/paper/1711.02680","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:24a50c018b57024a2dec9065a551a24f840a1ca212bf6be58b6c223960b9c82b","observation_id":"c67c7d78-bc7e-40af-9d9c-73c49e3bf7f2","resolution":{"observed_at":"2026-08-14T12:42:27.057671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.08775","last_updated":"2018-08-25T14:57:45Z","snapshot_observed_at":"2026-08-14T19:12:22.585354Z","submitted_at":"2018-05-22T17:59:22Z","title":"Spectral distortion anisotropies from single-field inflation","version":2},"cited_work":{"arxiv_id":"1805.08775","doi":null,"metadata_source":"pith","pith_arxiv_id":"1805.08775","snapshot_observed_at":"2026-08-14T12:42:27.161918Z","title":"Spectral distortion anisotropies from single-field inflation","venue":"astro-ph.CO","work_id":"3f8132d0-2351-459d-8e75-84d3f2547e3a","year":2018},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.062573Z"},"links":{"cited_paper":"/paper/1805.08775","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:ef54dc29f426479b9f3945db4794777f5d7a93e08c1d4962acc033848870b410","observation_id":"6b5366e1-61db-4544-977f-f39ab8393aba","resolution":{"observed_at":"2026-08-14T12:42:27.168879Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"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"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.09478","last_updated":"2018-04-09T17:36:26Z","snapshot_observed_at":"2026-08-14T20:10:03.365642Z","submitted_at":"2017-11-26T22:40:19Z","title":"Universality of multi-field $\\alpha$-attractors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.09478","snapshot_observed_at":"2026-08-14T12:42:27.066734Z","title":"Ach´ ucarro, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.066734Z"},"links":{"cited_paper":"/paper/1711.09478","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:7e847ebf3c16e15428e32d00fbf6abde3f8367fb9c04c9d609c5d4cdeb926195","observation_id":"983d00cc-39ac-4c8d-9b44-b65b27557a1d","resolution":{"observed_at":"2026-08-14T12:42:27.066734Z","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":"2026-08-14T18:28:26.625716Z","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":"2026-08-14T12:42:27.071685Z","title":"Ach´ ucarro, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.071685Z"},"links":{"cited_paper":"/paper/1809.05341","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:1318e861f3aad32c367ddd8f8f479005ff7c816d720c4c4c8100492d9815ae49","observation_id":"f62e72e8-95ce-4b62-b1f8-417a3dea8f80","resolution":{"observed_at":"2026-08-14T12:42:27.071685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1101.4809","last_updated":"2012-01-14T10:57:36Z","snapshot_observed_at":"2026-08-15T04:56:41.981603Z","submitted_at":"2011-01-25T13:28:54Z","title":"A covariant approach to general field space metric in multi-field inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1101.4809","snapshot_observed_at":"2026-08-14T12:42:27.076175Z","title":"Gong and T","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.076175Z"},"links":{"cited_paper":"/paper/1101.4809","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:e07aacfe76b43a86e4a6e0ecaad6990104a94e6f2ef57e043afc43c68e832a79","observation_id":"cf5e3466-138b-4aae-a0e2-e836e08f9afb","resolution":{"observed_at":"2026-08-14T12:42:27.076175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.06971","last_updated":"2016-08-03T07:17:57Z","snapshot_observed_at":"2026-08-14T21:51:54.970036Z","submitted_at":"2016-06-20T21:11:22Z","title":"Multi-field inflation and cosmological perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.06971","snapshot_observed_at":"2026-08-14T12:42:27.080091Z","title":"Gong, Int","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T12:42:27.080091Z"},"links":{"cited_paper":"/paper/1606.06971","citing_paper":"/paper/1908.06956"},"observation_digest":"sha256:a5cbcf737e28add36fa2f6ff57dfe95bc97c7895092bcc69c6a661f21644732b","observation_id":"ffa48554-68a3-4ca5-ac56-82a643d4af7e","resolution":{"observed_at":"2026-08-14T12:42:27.080091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.06956","last_updated":"2019-08-19T17:47:22Z","latest_version":1,"primary_category":"hep-th","snapshot_observed_at":"2026-08-15T00:01:26.483298Z","submitted_at":"2019-08-19T17:47:22Z","title":"Origin of ultra-light fields during inflation and their suppressed non-Gaussianity"},"reference_resolution":{"displayed":51,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":39,"verified_exact":8,"verified_fuzzy":3},"total_outbound_references":51},"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 15 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 5 inbound Pith citation observations for arXiv:1908.06956."}