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Soft limits of $N$-point correlation functions, in which one wavenumber is much smaller than the others, play a special role in constraining the physics of inflation.
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A. H. Guth, The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems
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J. M. Maldacena, Non-Gaussian features of primordial fluctuations in single field inflationary models
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N. Kogo and E. Komatsu, Angular trispectrum of cmb temperature anisotropy from primordial non-gaussianity with the full radiation transfer function
2006
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L. Ackerman, S. M. Carroll, and M. B. Wise, Imprints of a Primordial Preferred Direction on the Microwave Background
2007
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2007
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2010
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2013
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2013
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2013
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2013
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2013
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2011
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J. Soda, Statistical Anisotropy from Anisotropic Inflation
2012
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2012
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2013
Cited alongside, same era.
A. Maleknejad, M. Sheikh-Jabbari, and J. Soda, Gauge Fields and Inflation
2013
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J. Kim and E. Komatsu, Limits on anisotropic inflation from the Planck data
2013
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2013
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2013
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2013
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S. Endlich, A. Nicolis, and J. Wang, Solid Inflation
2013
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