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Anomalous Dimensions and Non-Gaussianity
We analyze the signatures of inflationary models that are coupled to strongly interacting field theories, a basic class of multifield models also motivated by their role in providing dynamically small scales. Near the squeezed limit of the bispectrum, we find a simple scaling behavior determined by...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2013
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1007/JHEP10(2013)171 http://cds.cern.ch/record/1504923 |
_version_ | 1780927230842503168 |
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author | Green, Daniel Lewandowski, Matthew Senatore, Leonardo Silverstein, Eva Zaldarriaga, Matias |
author_facet | Green, Daniel Lewandowski, Matthew Senatore, Leonardo Silverstein, Eva Zaldarriaga, Matias |
author_sort | Green, Daniel |
collection | CERN |
description | We analyze the signatures of inflationary models that are coupled to strongly interacting field theories, a basic class of multifield models also motivated by their role in providing dynamically small scales. Near the squeezed limit of the bispectrum, we find a simple scaling behavior determined by operator dimensions, which are constrained by the appropriate unitarity bounds. Specifically, we analyze two simple and calculable classes of examples: conformal field theories (CFTs), and large-N CFTs deformed by relevant time-dependent double-trace operators. Together these two classes of examples exhibit a wide range of scalings and shapes of the bispectrum, including nearly equilateral, orthogonal and local non-Gaussianity in different regimes. Along the way, we compare and contrast the shape and amplitude with previous results on weakly coupled fields coupled to inflation. This signature provides a precision test for strongly coupled sectors coupled to inflation via irrelevant operators suppressed by a high mass scale up to 1000 times the inflationary Hubble scale. |
id | cern-1504923 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2013 |
record_format | invenio |
spelling | cern-15049232023-03-14T18:24:30Zdoi:10.1007/JHEP10(2013)171http://cds.cern.ch/record/1504923engGreen, DanielLewandowski, MatthewSenatore, LeonardoSilverstein, EvaZaldarriaga, MatiasAnomalous Dimensions and Non-GaussianityParticle Physics - TheoryWe analyze the signatures of inflationary models that are coupled to strongly interacting field theories, a basic class of multifield models also motivated by their role in providing dynamically small scales. Near the squeezed limit of the bispectrum, we find a simple scaling behavior determined by operator dimensions, which are constrained by the appropriate unitarity bounds. Specifically, we analyze two simple and calculable classes of examples: conformal field theories (CFTs), and large-N CFTs deformed by relevant time-dependent double-trace operators. Together these two classes of examples exhibit a wide range of scalings and shapes of the bispectrum, including nearly equilateral, orthogonal and local non-Gaussianity in different regimes. Along the way, we compare and contrast the shape and amplitude with previous results on weakly coupled fields coupled to inflation. This signature provides a precision test for strongly coupled sectors coupled to inflation via irrelevant operators suppressed by a high mass scale up to 1000 times the inflationary Hubble scale.We analyze the signatures of inflationary models that are coupled to strongly interacting field theories, a basic class of multifield models also motivated by their role in providing dynamically small scales. Near the squeezed limit of the bispectrum, we find a simple scaling behavior determined by operator dimensions, which are constrained by the appropriate unitarity bounds. Specifically, we analyze two simple and calculable classes of examples: conformal field theories (CFTs), and large-N CFTs deformed by relevant time-dependent double-trace operators. Together these two classes of examples exhibit a wide range of scalings and shapes of the bispectrum, including nearly equilateral, orthogonal and local non-Gaussianity in different regimes. Along the way, we compare and contrast the shape and amplitude with previous results on weakly coupled fields coupled to inflation. This signature provides a precision test for strongly coupled sectors coupled to inflation via irrelevant operators suppressed by a high mass scale up to 1000 times the inflationary Hubble scale.arXiv:1301.2630SLAC-PUB-15334SU-ITP-12-42SLAC-PUB-15334SU-ITP-12-42oai:cds.cern.ch:15049232013-01-15 |
spellingShingle | Particle Physics - Theory Green, Daniel Lewandowski, Matthew Senatore, Leonardo Silverstein, Eva Zaldarriaga, Matias Anomalous Dimensions and Non-Gaussianity |
title | Anomalous Dimensions and Non-Gaussianity |
title_full | Anomalous Dimensions and Non-Gaussianity |
title_fullStr | Anomalous Dimensions and Non-Gaussianity |
title_full_unstemmed | Anomalous Dimensions and Non-Gaussianity |
title_short | Anomalous Dimensions and Non-Gaussianity |
title_sort | anomalous dimensions and non-gaussianity |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.1007/JHEP10(2013)171 http://cds.cern.ch/record/1504923 |
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