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The amplitude of primordial curvature perturbations is enhanced when a radiation bath at a temperature T>H is sustained during inflation by dissipative particle production, which is particularly significant when a non-trivial statistical ensemble of inflaton fluctuations is also maintained.
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This model overcomes the concerns raised by thermal corrections when m χ ≪ T m_{\chi}\ll T as initially discussed in A. Berera, M. Gleiser and R. O. Ramos, Phys. Rev. D 58
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