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We study the sensitivity of cosmological observables to the reheating phase following inflation driven by many scalar fields.
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A. M. Green and K. A. Malik, Primordial black hole production due to preheating
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S. Dodelson and L. Hui, A Horizon ratio bound for inflationary fluctuations
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A. R. Liddle and S. M. Leach, How long before the end of inflation were observable perturbations produced?
2003
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D. H. Lyth, C. Ungarelli, and D. Wands, The Primordial density perturbation in the curvaton scenario
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J. M. Maldacena, Non-Gaussian features of primordial fluctuations in single field inflationary models
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J. Elliston, D. J. Mulryne, D. Seery, and R. Tavakol, Evolution of fNL to the adiabatic limit
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S. Weinberg, Can non-adiabatic perturbations arise after single-field inflation?
2004
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S. Weinberg, Must cosmological perturbations remain non-adiabatic after multi-field inflation?
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P. Creminelli and M. Zaldarriaga, Single field consistency relation for the 3-point function
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K. Enqvist, A. Jokinen, A. Mazumdar, T. Multamäki, and A. Väihkönen, Non-Gaussianity from preheating
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J. Fonseca and D. Wands, Primordial non-Gaussianity from mixed inflaton-curvaton perturbations
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J. Martin, C. Ringeval, and V. Vennin, Observing Inflationary Reheating
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2015
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V. Vennin, K. Koyama, and D. Wands, Encyclopædia curvatonis
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M. Drewes, What can the CMB tell about the microphysics of cosmic reheating?
2016
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J. Martin, C. Ringeval, and V. Vennin, Information Gain on Reheating: the One Bit Milestone
2016
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