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We generalize the Effective Field Theory of Inflation to include additional light scalar degrees of freedom that are in their vacuum at the time the modes of interest are crossing the horizon.
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M. Zaldarriaga, “Non-Gaussianities in models with a varying inflaton decay rate,” Phys. Rev. D 69
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M. Sasaki and E. D. Stewart, “A General Analytic Formula For The Spectral Index Of The Density Perturbations Produced During Inflation,” Prog. Theor. Phys. 95
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N. Arkani-Hamed, P. Creminelli, S. Mukohyama and M. Zaldarriaga, “Ghost Inflation,” JCAP 0404
2005
Cited alongside, same era.
P. Creminelli, M. A. Luty, A. Nicolis and L. Senatore, “Starting the universe: Stable violation of the null energy condition and non-standard cosmologies,” JHEP 0612
2006
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2006
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X. Chen, M. x. Huang, S. Kachru and G. Shiu, “Observational signatures and non-Gaussianities of general single field inflation,” JCAP 0701
2007
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F. Bernardeau and T. Brunier, “Non-Gaussianities in extended D-term inflation,” Phys. Rev. D 76
2007
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P. Creminelli, L. Senatore and M. Zaldarriaga, “Estimators for local non-Gaussianities,” JCAP 0703
2007
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2008
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2008
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D. Green, B. Horn, L. Senatore and E. Silverstein, “Trapped Inflation,” Phys. Rev. D 80
2009
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2009
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2009
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2010
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