{"as_of":"2026-08-17T00:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1053e1f3a6faf0b4b5233099e96c502e61e5e3fe5a1d3189a5423f541f8612ed","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":"2026-08-12T17:29:14.902162Z","state":"measured"},{"denominator":54,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":54,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T14:56:15.568195Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-07T23:07:27.410883Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12699","snapshot_observed_at":"2026-08-09T14:56:15.568195Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.01632","last_updated":"2025-05-26T14:04:07Z","snapshot_observed_at":"2026-08-13T18:28:06.459387Z","submitted_at":"2025-02-03T18:58:27Z","title":"Curvature perturbations from vacuum transition during inflation","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-09T14:56:15.568195Z"},"links":{"cited_paper":"/paper/2411.12699","citing_paper":"/paper/2502.01632"},"observation_digest":"sha256:af33641883cf3fdd32f93d4e5bbe17bd62bb3361237803da4ca36abae06cb456","observation_id":"f237eb8b-4dfb-42ea-9aff-c4ff1a105b07","resolution":{"observed_at":"2026-08-09T14:56:15.568195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"cited_work":{"arxiv_id":"2411.12699","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.12699","snapshot_observed_at":"2026-08-07T23:07:27.410883Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","venue":"hep-ph","work_id":"3570ae3a-59d1-44c2-be39-5d2150d90cd5","year":2024},"citing_paper":{"arxiv_id":"2502.08986","last_updated":"2025-03-17T16:54:28Z","snapshot_observed_at":"2026-08-16T21:25:50.821458Z","submitted_at":"2025-02-13T05:48:58Z","title":"Gauss-Bonnet-induced symmetry breaking/restoration during inflation","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T23:07:26.968909Z"},"links":{"cited_paper":"/paper/2411.12699","citing_paper":"/paper/2502.08986"},"observation_digest":"sha256:4fc7d2a54963e6a323e36c1a0a03bf9a773df9d08a9e74f43e467513dbbceafd","observation_id":"a9da14f4-a762-4568-bb76-a37d94fb7df1","resolution":{"observed_at":"2026-08-07T23:07:27.415949Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12699","snapshot_observed_at":"2026-08-03T04:21:37.834323Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.05501","last_updated":"2026-03-13T12:11:09Z","snapshot_observed_at":"2026-08-15T23:44:28.307901Z","submitted_at":"2026-02-05T10:03:23Z","title":"Simulating first-order phase transition during inflation","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-03T04:21:37.834323Z"},"links":{"cited_paper":"/paper/2411.12699","citing_paper":"/paper/2602.05501"},"observation_digest":"sha256:fe4763453d548a0d46a7bc366e16431d669a869fc8a8525db04b99cb2cfa9663","observation_id":"70be0d45-501f-4159-a3b1-c18d87fb0447","resolution":{"observed_at":"2026-08-03T04:21:37.834323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2411.12699/citation-record","integrity":"/paper/2411.12699/integrity","json":"/paper/2411.12699/citation-record.json","paper":"/paper/2411.12699"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T17:29:16.127730Z","title":"Spectrum of relict gravitational radiation and the early state of the universe,","venue":null,"work_id":"24ee527d-a5cf-45f4-bb5f-e13e644e97ca","year":1979},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.583372Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:2080e802e13043059430ebdc9f377fc7fea53d0a7bc52c64335a516fbe6788e7","observation_id":"4450ebb1-017c-4e12-a834-043a86fd51d3","resolution":{"observed_at":"2026-08-12T17:29:16.133465Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T17:29:14.590362Z","title":"A new type of isotropic cosmological models without singularity,","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.590362Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:e9152b55c92119a65f30c3182de34eff359cbe9a2171735ff93165d8b9545762","observation_id":"cc69d5ac-10a9-48bd-9960-75feaf06c0e7","resolution":{"observed_at":"2026-08-12T17:29:14.590362Z","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":"2026-08-12T17:29:16.109266Z","title":"Dynamics of the Universe and Spontaneous Symmetry Breaking,","venue":null,"work_id":"296756b8-fd5f-4749-8772-67063fd0f83d","year":1980},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.595400Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:d27ea7fd6721e6df30cb8abde5a6734974482ddb87b51e4893ea294536035e2b","observation_id":"1e7e37c5-2cce-42f0-9755-706a3c58773e","resolution":{"observed_at":"2026-08-12T17:29:16.115481Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T17:29:16.089860Z","title":"First-order phase transition of a vacuum and the expansion of the Universe,","venue":null,"work_id":"d898b153-e8de-4e2b-89f8-0e2c1a0caca8","year":1981},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.602691Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:6a2ed3c65cbb6d1a0fc39719b86d1597902573f6c845ae8ea89ba48e33ac0626","observation_id":"778c335a-77b7-4e65-9022-a74268d57f06","resolution":{"observed_at":"2026-08-12T17:29:16.096993Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T17:29:14.609406Z","title":"The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.609406Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:d63182afc44092bae34698d554378151288a750b133f66fdbfacb6119dc204c0","observation_id":"7b81017b-8ffd-410f-bb1e-566937be0eb9","resolution":{"observed_at":"2026-08-12T17:29:14.609406Z","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":"2026-08-12T17:29:16.055008Z","title":"A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems,","venue":null,"work_id":"2418645a-e73e-4ee5-ac75-edeb84a3221e","year":1982},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.615273Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:f1cc2af9ccf86fe7ae9f8fad8a5f8ff653521da47b1e7d76090815af1140f949","observation_id":"525ad42d-c003-4049-9c3e-034d84691d3b","resolution":{"observed_at":"2026-08-12T17:29:16.061378Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T17:29:14.620998Z","title":"Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking,","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.620998Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:079e84ec6d49f38a2e3b982cf1276b0739c4f8cef8309196796576c2650b0317","observation_id":"d4c96dbe-aab3-4a49-8c01-8668f8a6a15a","resolution":{"observed_at":"2026-08-12T17:29:14.620998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2009.12381","last_updated":"2021-10-15T04:25:41Z","snapshot_observed_at":"2026-08-15T00:54:28.771078Z","submitted_at":"2020-09-25T18:00:13Z","title":"A unique gravitational wave signal from phase transition during inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2009.12381","snapshot_observed_at":"2026-08-12T17:29:14.626085Z","title":"A unique gravitational wave signal from phase transition during inflation*,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.626085Z"},"links":{"cited_paper":"/paper/2009.12381","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:f0f83026b3e691d06a24db250477b8619d7ec02793c4b8e34e2bd085801295ec","observation_id":"1946a6f5-5725-478b-9d33-f5a0f9a87011","resolution":{"observed_at":"2026-08-12T17:29:14.626085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.05171","last_updated":"2022-06-09T21:23:56Z","snapshot_observed_at":"2026-08-16T17:39:36.461074Z","submitted_at":"2022-01-13T19:00:17Z","title":"Gravitational Waves from an Inflation Triggered First-Order Phase Transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.05171","snapshot_observed_at":"2026-08-12T17:29:14.631573Z","title":"Gravitational waves from an inflation triggered first-order phase transition,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.631573Z"},"links":{"cited_paper":"/paper/2201.05171","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:0a9eb2a8d68c00fd273165ffd9c8d8e7e2078bd24fe46a51601afdc4ec76cefb","observation_id":"90da05e1-65ab-49fc-9a4f-674d70712e2c","resolution":{"observed_at":"2026-08-12T17:29:14.631573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.05833","last_updated":"2024-09-09T17:38:52Z","snapshot_observed_at":"2026-08-16T13:20:02.632279Z","submitted_at":"2024-09-09T17:38:52Z","title":"A model for inflaton induced baryogenesis and its phenomenological consequences","version":1},"cited_work":{"arxiv_id":"2409.05833","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.05833","snapshot_observed_at":"2026-08-12T17:29:15.875662Z","title":"A model for inflaton induced baryogenesis and its phenomenological consequences","venue":"astro-ph.CO","work_id":"0c42881f-74e7-4fa6-a2b9-05c446134e54","year":2024},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.638298Z"},"links":{"cited_paper":"/paper/2409.05833","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:38419e66e6d987374c1d146af5dff14382d6e6803003bdbe1cefc8525d029a71","observation_id":"a4d29993-31f8-4ad0-b970-1dc917ca3fc5","resolution":{"observed_at":"2026-08-12T17:29:15.881924Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.09428","last_updated":"2024-06-10T08:38:14Z","snapshot_observed_at":"2026-08-16T15:39:23.785277Z","submitted_at":"2023-04-19T05:56:22Z","title":"BCS in the Sky: Signatures of Inflationary Fermion Condensation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.09428","snapshot_observed_at":"2026-08-12T17:29:14.646671Z","title":"BCS in the sky: signatures of inflationary fermion condensation,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.646671Z"},"links":{"cited_paper":"/paper/2304.09428","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:e9c60b50448fa5b035f919d40330572a76e2f1785a867198a267d88fe3d04342","observation_id":"98543c38-046b-4c3e-8ef5-b17eaa021e3b","resolution":{"observed_at":"2026-08-12T17:29:14.646671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.05665","last_updated":"2021-02-10T19:00:00Z","snapshot_observed_at":"2026-08-16T18:46:23.654356Z","submitted_at":"2021-02-10T19:00:00Z","title":"Non-Gaussian Stochastic Gravitational Waves from Phase Transitions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.05665","snapshot_observed_at":"2026-08-12T17:29:14.651494Z","title":"Non-Gaussian stochastic gravitational waves from phase transitions,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.651494Z"},"links":{"cited_paper":"/paper/2102.05665","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:055d2994e36d692d37c1f5bef1bc106152e6a5631123b92087d7b9468663661c","observation_id":"29bdeec2-ddd3-461d-bcd0-084a7ada22b8","resolution":{"observed_at":"2026-08-12T17:29:14.651494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.09301","last_updated":"2022-11-17T02:28:04Z","snapshot_observed_at":"2026-08-16T16:15:31.243653Z","submitted_at":"2022-11-17T02:28:04Z","title":"Large Primordial Fluctuations in Gravitational Waves from Phase Transitions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.09301","snapshot_observed_at":"2026-08-12T17:29:14.656578Z","title":"Large primordial fluctuations in gravitational waves from phase transitions,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.656578Z"},"links":{"cited_paper":"/paper/2211.09301","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:dc9a82af7c68630fe0f939abbc0deff8eb4e116e1afccde904604a9a3a8e0289","observation_id":"c1cd1ba9-becd-45f8-b539-0093be6fb968","resolution":{"observed_at":"2026-08-12T17:29:14.656578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.04482","last_updated":"2022-05-09T18:00:05Z","snapshot_observed_at":"2026-08-16T17:01:32.500333Z","submitted_at":"2022-05-09T18:00:05Z","title":"Primordial Clocks within Stochastic Gravitational Wave Anisotropies","version":1},"cited_work":{"arxiv_id":"2205.04482","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.04482","snapshot_observed_at":"2026-08-12T17:29:15.776614Z","title":"Primordial Clocks within Stochastic Gravitational Wave Anisotropies","venue":"astro-ph.CO","work_id":"f3421e2f-aa3a-494d-bdcf-e228e8c628dc","year":2022},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.662365Z"},"links":{"cited_paper":"/paper/2205.04482","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:ae51882f88a1cebe0340633e1eb967a807b65fd4e63fb58b4b9a6ed54bcb97e7","observation_id":"7a206ef3-412c-4a8a-8d0e-8c2d4703ee6d","resolution":{"observed_at":"2026-08-12T17:29:15.782316Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+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":"2026-08-12T17:29:14.668830Z","title":"Phase transition during inflation and the gravitational wave signal at pulsar timing arrays,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.668830Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:63708c9ef8cbf125461aa17cd5cc073c5d754e489ae1526e4820abe9cefd4fbf","observation_id":"380895b1-51cd-4a7c-9d59-508e80d833a6","resolution":{"observed_at":"2026-08-12T17:29:14.668830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16216","last_updated":"2023-06-28T13:51:04Z","snapshot_observed_at":"2026-08-08T13:18:07.452026Z","submitted_at":"2023-06-28T13:51:04Z","title":"Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16216","snapshot_observed_at":"2026-08-12T17:29:14.674916Z","title":"Searching for the Nano-Hertz Stochastic Gravitational Wave Background with the Chinese Pulsar Timing Array Data Release I,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.674916Z"},"links":{"cited_paper":"/paper/2306.16216","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:944cbb13dd485f72f14175494b5157ca72c5af893606cf66f45b2185369efd4f","observation_id":"abefbe22-d22d-4259-bed9-9c44c60a5737","resolution":{"observed_at":"2026-08-12T17:29:14.674916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16213","last_updated":"2023-06-28T13:51:01Z","snapshot_observed_at":"2026-08-13T16:50:10.214371Z","submitted_at":"2023-06-28T13:51:01Z","title":"The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16213","snapshot_observed_at":"2026-08-12T17:29:14.681943Z","title":"The NANOGrav 15 yr Data Set: Evidence for a Gravitational-wave Background,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.681943Z"},"links":{"cited_paper":"/paper/2306.16213","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:7f0a45ab8ee661c203aec0e43195a203f3e3f73c3006a428eb3f5449bf8e4b11","observation_id":"94dc3e56-6148-4d7c-ac78-7f979093ca6b","resolution":{"observed_at":"2026-08-12T17:29:14.681943Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16214","last_updated":"2023-06-28T13:51:02Z","snapshot_observed_at":"2026-08-15T04:04:48.616971Z","submitted_at":"2023-06-28T13:51:02Z","title":"The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16214","snapshot_observed_at":"2026-08-12T17:29:14.687913Z","title":"The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.687913Z"},"links":{"cited_paper":"/paper/2306.16214","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:5992379a610dfeb52fecf90604e7f3a542a0760dd71cd7726799464633c9e7a5","observation_id":"8409c527-6301-4f3c-a101-9aa679c4f2f6","resolution":{"observed_at":"2026-08-12T17:29:14.687913Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.16215","last_updated":"2023-06-28T13:51:03Z","snapshot_observed_at":"2026-08-12T23:01:24.461267Z","submitted_at":"2023-06-28T13:51:03Z","title":"Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.16215","snapshot_observed_at":"2026-08-12T17:29:14.695512Z","title":"Search for an Isotropic Gravitational-wave Background with the Parkes Pulsar Timing Array,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.695512Z"},"links":{"cited_paper":"/paper/2306.16215","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:1bbd2a4c249de198ef047653f4be29b038703c695b36beec82740e241ff8ad9f","observation_id":"7512d427-2205-4ad4-83b0-0732bdefcc1e","resolution":{"observed_at":"2026-08-12T17:29:14.695512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.07972","last_updated":"2022-12-22T19:44:37Z","snapshot_observed_at":"2026-08-16T17:14:23.907629Z","submitted_at":"2022-03-15T15:01:12Z","title":"Detection of Early-Universe Gravitational Wave Signatures and Fundamental Physics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.07972","snapshot_observed_at":"2026-08-12T17:29:14.703189Z","title":"Detection of early-universe gravitational-wave signatures and fundamental physics,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.703189Z"},"links":{"cited_paper":"/paper/2203.07972","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:b24fb5e260d496d722f1d8a4caaaade2f4310c3218527effd54c4d8f63053de1","observation_id":"779f7238-af8a-40e9-8b6b-6858181d8fee","resolution":{"observed_at":"2026-08-12T17:29:14.703189Z","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":"2026-08-12T17:29:14.710449Z","title":"Multi-field inflation and cosmological perturbations,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.710449Z"},"links":{"cited_paper":"/paper/1606.06971","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:4e358b0fbc4d4f1bdf4b5a74e2fd93a075cc2f0221b63f4eb7c06cf2eda2754d","observation_id":"e031261f-324e-407b-b9fc-3e58329c6df8","resolution":{"observed_at":"2026-08-12T17:29:14.710449Z","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":"2026-08-12T17:29:14.717670Z","title":"Planck 2018 results. IX. Constraints on primordial non-Gaussianity,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.717670Z"},"links":{"cited_paper":"/paper/1905.05697","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:c38096961db3734d52b39962462dc908cf50e70c3b34b20e52a0dfc3c2c13061","observation_id":"7b663177-3e8a-4338-bc22-e57c78c5ea38","resolution":{"observed_at":"2026-08-12T17:29:14.717670Z","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":"2026-08-12T17:29:14.725641Z","title":"Euclid. I. Overview of the Euclid mission,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.725641Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:02c2ce2ca5c4f3c5ae9fe77308b0fb68ca43eb328f1caa65e4b1cdc00c62dbba","observation_id":"dc58962d-5b3f-4520-a009-44ea3692d901","resolution":{"observed_at":"2026-08-12T17:29:14.725641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-08-12T17:29:14.731700Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.731700Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:84f7c97d7b49272336527d75d38d46538b7d9f0fffb0ef19b0a5b860d6d965f8","observation_id":"342b2141-6ac7-4fa3-af02-737c8a4ba97b","resolution":{"observed_at":"2026-08-12T17:29:14.731700Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.4872","last_updated":"2015-03-25T23:27:43Z","snapshot_observed_at":"2026-08-14T23:07:27.492198Z","submitted_at":"2014-12-16T03:59:10Z","title":"Cosmology with the SPHEREX All-Sky Spectral Survey","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.4872","snapshot_observed_at":"2026-08-12T17:29:14.737331Z","title":"Cosmology with the SPHEREX All-Sky Spectral Survey,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.737331Z"},"links":{"cited_paper":"/paper/1412.4872","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:feb8a394784d88053632f5b4fb162c10d256495ba623a887df0477b70d69c836","observation_id":"66e219ce-c0f8-4837-a89d-6214bf02fb17","resolution":{"observed_at":"2026-08-12T17:29:14.737331Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.0310","last_updated":"2012-11-01T21:23:33Z","snapshot_observed_at":"2026-08-15T00:40:45.653070Z","submitted_at":"2012-11-01T21:23:33Z","title":"Large Synoptic Survey Telescope: Dark Energy Science Collaboration","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.0310","snapshot_observed_at":"2026-08-12T17:29:14.743767Z","title":"Large Synoptic Survey Telescope: Dark Energy Science Collaboration,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.743767Z"},"links":{"cited_paper":"/paper/1211.0310","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:2b73917215705ed988d22d7e1f4b02203bfed2bffba03c4e523299bfce3c31e1","observation_id":"7334af65-5e84-4802-8be2-95aa5ae25fe1","resolution":{"observed_at":"2026-08-12T17:29:14.743767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1206.0737","last_updated":"2013-07-30T05:39:14Z","snapshot_observed_at":"2026-08-15T00:57:58.158375Z","submitted_at":"2012-06-04T20:00:02Z","title":"Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.0737","snapshot_observed_at":"2026-08-12T17:29:14.751112Z","title":"Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.751112Z"},"links":{"cited_paper":"/paper/1206.0737","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:ae335779ef87db8390580aebb2deadb43cf0e7308e4130d424ad5d7f9c0a74dc","observation_id":"97e1d3e2-10b5-48af-8d04-c06e5a1fee0a","resolution":{"observed_at":"2026-08-12T17:29:14.751112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.05271","last_updated":"2020-04-11T00:35:56Z","snapshot_observed_at":"2026-08-13T23:02:39.216802Z","submitted_at":"2020-04-11T00:35:56Z","title":"Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.05271","snapshot_observed_at":"2026-08-12T17:29:14.761032Z","title":"Cosmology with the Roman Space Telescope – multiprobe strategies,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.761032Z"},"links":{"cited_paper":"/paper/2004.05271","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:b6c026fcf95223dfdb2a01dbb41546e4557cbed4cdec3ff0b67283ec5b93cd51","observation_id":"892a6a2d-41a3-4f10-b892-4739c20ed9d0","resolution":{"observed_at":"2026-08-12T17:29:14.761032Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.04322","last_updated":"2022-09-09T14:25:02Z","snapshot_observed_at":"2026-08-16T16:33:38.880098Z","submitted_at":"2022-09-09T14:25:02Z","title":"The MegaMapper: A Stage-5 Spectroscopic Instrument Concept for the Study of Inflation and Dark Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.04322","snapshot_observed_at":"2026-08-12T17:29:14.767013Z","title":"The MegaMapper: A Stage-5 Spectroscopic Instrument Concept for the Study of Inflation and Dark Energy,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.767013Z"},"links":{"cited_paper":"/paper/2209.04322","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:729288b30f6ff3880086660f43b47cbe12fa239462d5d60fccd899417b7f9cbe","observation_id":"fcc88e27-1e74-4814-b9c7-3ec951189343","resolution":{"observed_at":"2026-08-12T17:29:14.767013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.00070","last_updated":"2019-08-30T20:58:20Z","snapshot_observed_at":"2026-08-14T12:04:40.082123Z","submitted_at":"2019-08-30T20:58:20Z","title":"ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.00070","snapshot_observed_at":"2026-08-12T17:29:14.773747Z","title":"ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System,","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.773747Z"},"links":{"cited_paper":"/paper/1909.00070","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:01bb24ad2a8d0a47bde8173f6bf16d4c376ee94781998310ada24f0b9537e9a0","observation_id":"dbd9b494-b55f-4467-9855-523a31bfd50b","resolution":{"observed_at":"2026-08-12T17:29:14.773747Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.07864","last_updated":"2022-03-15T13:13:02Z","snapshot_observed_at":"2026-08-16T17:14:26.775017Z","submitted_at":"2022-03-15T13:13:02Z","title":"Snowmass2021 Cosmic Frontier White Paper: 21cm Radiation as a Probe of Physics Across Cosmic Ages","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.07864","snapshot_observed_at":"2026-08-12T17:29:14.779853Z","title":"Snowmass2021 Cosmic Frontier White Paper: 21cm Radiation as a Probe of Physics Across Cosmic Ages,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.779853Z"},"links":{"cited_paper":"/paper/2203.07864","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:f07b967ed031e8ea9ffb61a0a9a3ef7de2cdbd55d14570df3533c41d7265d9c8","observation_id":"3b965d40-cc40-49e6-bda1-51baa617d6f4","resolution":{"observed_at":"2026-08-12T17:29:14.779853Z","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":"2026-08-12T17:29:14.785100Z","title":"Non-Gaussian features of primordial fluctuations in single field inflationary models,","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.785100Z"},"links":{"cited_paper":"/paper/astro-ph/0210603","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:8d6d7c3fe86085560454d5767df2d8deb626c7a1c83823c2256f9ee241e2d4d4","observation_id":"a189fb2b-727b-4917-92c1-122368ff03d0","resolution":{"observed_at":"2026-08-12T17:29:14.785100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-ph/0011104","last_updated":"2001-04-06T02:49:48Z","snapshot_observed_at":"2026-08-14T06:45:31.305309Z","submitted_at":"2000-11-08T09:02:27Z","title":"Natural Chaotic Inflation in Supergravity and Leptogenesis","version":2},"cited_work":{"arxiv_id":"hep-ph/0011104","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-ph/0011104","snapshot_observed_at":"2026-08-12T17:29:15.271412Z","title":"Natural Chaotic Inflation in Supergravity and Leptogenesis","venue":"hep-ph","work_id":"16d84258-d52f-4421-a56e-a8122c513225","year":2000},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.791927Z"},"links":{"cited_paper":"/paper/hep-ph/0011104","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:38d10c372d749502615b8ddb5023df9e4511a3ecde1452c4afad97b609cbef5b","observation_id":"c6bc0598-815b-4676-8985-3d349de1979b","resolution":{"observed_at":"2026-08-12T17:29:15.279564Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0602178","last_updated":"2006-03-31T22:47:25Z","snapshot_observed_at":"2026-07-07T04:56:41.885342Z","submitted_at":"2006-02-20T20:30:07Z","title":"Causality, Analyticity and an IR Obstruction to UV Completion","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0602178","snapshot_observed_at":"2026-08-12T17:29:14.798590Z","title":"Causality, analyticity and an IR obstruction to UV completion,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.798590Z"},"links":{"cited_paper":"/paper/hep-th/0602178","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:6b47496d15d68dbfc958561cdb1855712c7101a334b26bcb5a877d082f98cd9d","observation_id":"43ec2d88-1567-4298-9013-2d7419dcbe9f","resolution":{"observed_at":"2026-08-12T17:29:14.798590Z","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":"2026-08-14T23:38:02.952876Z","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":"2026-08-12T17:29:14.804365Z","title":"Baumann and L","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.804365Z"},"links":{"cited_paper":"/paper/1404.2601","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:c38251887425e641bf5c5a6db3fc85684bc9a7385ea876f8812d29f512d8a0c1","observation_id":"75073256-00b8-4a4f-8a30-c6d9939a37b1","resolution":{"observed_at":"2026-08-12T17:29:14.804365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00864","last_updated":"2018-06-27T01:11:37Z","snapshot_observed_at":"2026-08-16T08:23:15.023072Z","submitted_at":"2017-11-02T18:00:26Z","title":"The String Landscape, the Swampland, and the Missing Corner","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00864","snapshot_observed_at":"2026-08-12T17:29:14.810077Z","title":"The String Landscape, the Swampland, and the Missing Corner,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.810077Z"},"links":{"cited_paper":"/paper/1711.00864","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:d43c61375ed62bd5a52445d48b5242f69c476d824d1c8fb1f5f2138b9664d726","observation_id":"7df739c8-3061-4257-9fa0-228810ad12ee","resolution":{"observed_at":"2026-08-12T17:29:14.810077Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.08380","last_updated":"2023-06-15T16:13:35Z","snapshot_observed_at":"2026-08-16T17:26:59.715574Z","submitted_at":"2022-01-20T18:59:27Z","title":"The Weak Gravity Conjecture: A Review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.08380","snapshot_observed_at":"2026-08-12T17:29:14.815674Z","title":"Weak gravity conjecture,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.815674Z"},"links":{"cited_paper":"/paper/2201.08380","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:b64ef597d441e37cdb2479725590a9f1f9f984c467fc69b9bb6f80de5b6e681a","observation_id":"c9e9a58c-52bd-4f37-b93c-faa32556fb5b","resolution":{"observed_at":"2026-08-12T17:29:14.815674Z","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":"2026-08-12T17:29:16.024115Z","title":"Cosmological Consequences of a First Order Phase Transition in the SU(5) Grand Unified Model,","venue":null,"work_id":"fc38e6e8-827b-4da9-bb20-e974474fd8d7","year":1981},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.821224Z"},"links":{"citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:7971603f3a3e86c23f7433f3bcc7332b6803d97b97ed748f0398948094a6ba92","observation_id":"073b18c6-414b-4ad5-b4aa-d881d4424d68","resolution":{"observed_at":"2026-08-12T17:29:16.030224Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.14857","last_updated":"2022-09-07T00:44:34Z","snapshot_observed_at":"2026-08-16T16:35:40.394469Z","submitted_at":"2022-08-31T13:39:59Z","title":"Superheavy Dark Matter Production from Symmetry Restoration First-Order Phase Transition During Inflation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.14857","snapshot_observed_at":"2026-08-12T17:29:14.826312Z","title":"Superheavy dark matter production from a symmetry-restoring first-order phase transition during inflation,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.826312Z"},"links":{"cited_paper":"/paper/2208.14857","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:65b48f22e6d02e1b998e1b965e6856850ce1c3054b859f2d7924652ef60a0e71","observation_id":"72e61489-f3e3-46c2-ba70-db6b6fab166a","resolution":{"observed_at":"2026-08-12T17:29:14.826312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.4189","last_updated":"2011-09-19T23:50:00Z","snapshot_observed_at":"2026-08-15T04:34:47.916842Z","submitted_at":"2011-09-19T23:50:00Z","title":"CosmoTransitions: Computing Cosmological Phase Transition Temperatures and Bubble Profiles with Multiple Fields","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.4189","snapshot_observed_at":"2026-08-12T17:29:14.831598Z","title":"CosmoTransitions: Computing Cosmological Phase Transition Temperatures and Bubble Profiles with Multiple Fields,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.831598Z"},"links":{"cited_paper":"/paper/1109.4189","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:6979e7a5a6a77603d5edb07e626850fc6bd9d1db3e8305cdb81d72b1c61ca834","observation_id":"4eaba06f-15c5-4ada-94c4-dd5ffff7f567","resolution":{"observed_at":"2026-08-12T17:29:14.831598Z","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":"2026-08-12T17:29:14.837126Z","title":"A covariant approach to general field space metric in multi-field inflation,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.837126Z"},"links":{"cited_paper":"/paper/1101.4809","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:fd1bb978f0fbbb309697c5a0b4ee085a571d346d1df9b781deac4fd5a909b6b0","observation_id":"617dd11c-4dac-4a87-b81a-dba168e387ec","resolution":{"observed_at":"2026-08-12T17:29:14.837126Z","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":"2026-08-15T04:20:50.879939Z","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":"2026-08-12T17:29:14.843458Z","title":"Effective theories of single field inflation when heavy fields matter,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.843458Z"},"links":{"cited_paper":"/paper/1201.6342","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:5db7df2f768737e1e7f1fb55f7be5d44f9e191251a001a98057d6ad5325043e6","observation_id":"4a5300b5-9d6c-452a-9fb6-11552c14030e","resolution":{"observed_at":"2026-08-12T17:29:14.843458Z","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":"2026-08-12T17:29:14.849882Z","title":"Quantum contributions to cosmological correlations,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.849882Z"},"links":{"cited_paper":"/paper/hep-th/0506236","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:6f8862a8b6232e49eee667cda3901d50726ccb53a5db3544273d3971b67a698e","observation_id":"9c4fed6e-719d-408b-831c-b5336c0cb5a1","resolution":{"observed_at":"2026-08-12T17:29:14.849882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0605244","last_updated":"2006-06-22T00:11:54Z","snapshot_observed_at":"2026-08-14T16:11:27.054753Z","submitted_at":"2006-05-24T22:10:18Z","title":"Quantum Contributions to Cosmological Correlations II: Can These Corrections Become Large?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0605244","snapshot_observed_at":"2026-08-12T17:29:14.855663Z","title":"Quantum contributions to cosmological correlations. II. Can these corrections become large?,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.855663Z"},"links":{"cited_paper":"/paper/hep-th/0605244","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:cc28f6a18581a0c3c3f5a997c52ff295d1c77d0ec192d6fa933162a638a20616","observation_id":"0858291d-6b3d-42be-84e3-a646ef60d804","resolution":{"observed_at":"2026-08-12T17:29:14.855663Z","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":"2026-08-14T21:09:20.351315Z","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":"2026-08-12T17:29:14.863353Z","title":"Schwinger-Keldysh Diagrammatics for Primordial Perturbations,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.863353Z"},"links":{"cited_paper":"/paper/1703.10166","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:84dab4d2900b68ea09fe96de03f38ed922819048b46641bea4049c6c40057d1e","observation_id":"f24c23a7-ecd7-4044-9a11-450fd5d6bb4e","resolution":{"observed_at":"2026-08-12T17:29:14.863353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507053","last_updated":"2005-12-12T00:01:13Z","snapshot_observed_at":"2026-08-15T02:06:53.044825Z","submitted_at":"2005-07-03T19:17:52Z","title":"Running Non-Gaussianities in DBI Inflation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0507053","snapshot_observed_at":"2026-08-12T17:29:14.871990Z","title":"Running non-Gaussianities in DBI inflation,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.871990Z"},"links":{"cited_paper":"/paper/astro-ph/0507053","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:ab479717c5334ebf036ca5d09a83bef348a34b3de13a00ce6d3dcf10979554fb","observation_id":"3cea4731-cd46-4d01-887a-0dc9a2c112f8","resolution":{"observed_at":"2026-08-12T17:29:14.871990Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.2040","last_updated":"2009-09-28T23:12:21Z","snapshot_observed_at":"2026-08-15T05:39:18.959888Z","submitted_at":"2009-09-11T14:23:59Z","title":"Scale Dependent Local Non-Gaussianity from Loops","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.2040","snapshot_observed_at":"2026-08-12T17:29:14.878037Z","title":"Scale Dependent Local Non-Gaussianity from Loops,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.878037Z"},"links":{"cited_paper":"/paper/0909.2040","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:c526e3b6f30d1769833971668dc8020653b0120eda7be43f463441a4dccb8f30","observation_id":"a3023f62-a3e4-4a5b-8b6e-4f9530cce6bc","resolution":{"observed_at":"2026-08-12T17:29:14.878037Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.2780","last_updated":"2010-06-13T16:39:22Z","snapshot_observed_at":"2026-08-15T05:33:49.367157Z","submitted_at":"2009-11-16T16:02:53Z","title":"Scale dependence of local f_NL","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.2780","snapshot_observed_at":"2026-08-12T17:29:14.883804Z","title":"Scale dependence of local f NL,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.883804Z"},"links":{"cited_paper":"/paper/0911.2780","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:1a157393898ce99a64c6cbd18862595215e267b3463c85d912831b3f9c5df5c1","observation_id":"96be451b-c3c0-4c3f-8cff-cd1707c9471b","resolution":{"observed_at":"2026-08-12T17:29:14.883804Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.02361","last_updated":"2023-04-05T10:54:39Z","snapshot_observed_at":"2026-08-16T15:42:35.810047Z","submitted_at":"2023-04-05T10:54:39Z","title":"Gravitational Waves Produced by Domain Walls During Inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.02361","snapshot_observed_at":"2026-08-12T17:29:14.891756Z","title":"Gravitational waves produced by domain walls during inflation,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.891756Z"},"links":{"cited_paper":"/paper/2304.02361","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:e9619a9f7125f07a1ada7a64706491330101a497a423d500cd055c486461e6e6","observation_id":"c29c9fcc-40be-4cfd-90e1-0d07681c36a3","resolution":{"observed_at":"2026-08-12T17:29:14.891756Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1506.04152","last_updated":"2015-10-08T17:15:55Z","snapshot_observed_at":"2026-08-14T22:44:37.621287Z","submitted_at":"2015-06-12T20:00:51Z","title":"Primordial non-gaussianity from the bispectrum of 21-cm fluctuations in the dark ages","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1506.04152","snapshot_observed_at":"2026-08-12T17:29:14.896801Z","title":"Primordial non-gaussianity from the bispectrum of 21-cm fluctuations in the dark ages,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.896801Z"},"links":{"cited_paper":"/paper/1506.04152","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:9bde390a144f7e4043cfcfa158986cc950dd35b9832f3300c008f06637515443","observation_id":"b7b27b55-e1c4-4e89-864f-75be956de4fb","resolution":{"observed_at":"2026-08-12T17:29:14.896801Z","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":"2026-08-14T21:34:16.605571Z","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":"2026-08-12T17:29:14.902162Z","title":"Prospects for Cosmological Collider Physics,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T17:29:14.902162Z"},"links":{"cited_paper":"/paper/1610.06559","citing_paper":"/paper/2411.12699"},"observation_digest":"sha256:24bdda3e40f69add235d31f7e38d1d47d27f5df7d8a9b3c260fad3697afe0c02","observation_id":"74253f84-9638-4d39-b974-825713908df1","resolution":{"observed_at":"2026-08-12T17:29:14.902162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2411.12699","last_updated":"2024-11-19T18:06:26Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-16T05:49:14.150070Z","submitted_at":"2024-11-19T18:06:26Z","title":"Large non-Gaussianities corresponding to first-order phase transitions during inflation"},"reference_resolution":{"displayed":51,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":43,"verified_exact":3,"verified_fuzzy":5},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 3 inbound Pith citation observations for arXiv:2411.12699."}