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Models of inflation based on axions, which owe their popularity to the robustness against UV corrections, have also a very distinct class of signatures.
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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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N. Barnaby and J. M. Cline, “Predictions for non-Gaussianity from Nonlocal Inflation,” JCAP 0806
2007
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X. Chen, R. Easther and E. A. Lim, “Large non-Gaussianities in single field inflation,” JCAP 0706
2007
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N. Barnaby and J. M. Cline, “non-Gaussian and nonscale-invariant perturbations from tachyonic preheating in hybrid inflation,” Phys. Rev. D 73
2007
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2007
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R. Holman and A. J. Tolley, “Enhanced Non-Gaussianity from Excited Initial States,” JCAP 0805
2008
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2009
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2009
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2009
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2009
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N. Barnaby, J. R. Bond, Z. Huang and L. Kofman, “Preheating After Modular Inflation,” JCAP 0912
2009
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2010
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2010
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2010
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2010
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2010
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J. Braden, L. Kofman and N. Barnaby, “Reheating the Universe After Multi-Field Inflation,” JCAP 1007
2010
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