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We consider a model of preheating where the coupling of the inflaton to the preheat field is modulated by an additional scalar field which is light during inflation.
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R. Micha and I. I. Tkachev, Relativistic turbulence: A Long way from preheating to equilibrium
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G. Dvali, A. Gruzinov, and M. Zaldarriaga, A new mechanism for generating density perturbations from inflation
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G. Dvali, A. Gruzinov, and M. Zaldarriaga, Cosmological perturbations from inhomogeneous reheating, freezeout, and mass domination
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M. Zaldarriaga, Non-Gaussianities in models with a varying inflaton decay rate
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A. V. Frolov, DEFROST: A New Code for Simulating Preheating after Inflation
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D. H. Lyth, K. A. Malik, and M. Sasaki, A General proof of the conservation of the curvature perturbation
2005
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H. Kurki-Suonio, V. Muhonen, and J. Valiviita, Correlated Primordial Perturbations in Light of CMB and LSS Data
2005
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M. Beltran, J. Garcia-Bellido, J. Lesgourgues, and M. Viel, Squeezing the window on isocurvature modes with the Lyman- alpha forest
2005
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M. Beltran, J. Garcia-Bellido, J. Lesgourgues, A. R. Liddle, and A. Slosar, Bayesian model selection and isocurvature perturbations
2005
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B. A. Bassett, S. Tsujikawa, and D. Wands, Inflation dynamics and reheating
2006
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D. I. Podolsky, G. N. Felder, L. Kofman, and M. Peloso, Equation of state and beginning of thermalization after preheating
2006
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2009
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A. Mazumdar and J. Rocher, Particle physics models of inflation and curvaton scenarios
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