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In the case of Higgs inflation, in which the inflaton has no couplings other than to standard model particles, some as-yet unknown mechanism would be required to preserve primordial isocurvature perturbations through reheating. Primordial isocurvature perturbations could more readily survive reheating in symmetric-coupling models if the inflaton coupled to some non standard model particles, such as cold dark matter particles.
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In the case of Higgs inflation, in which the inflaton has no couplings other than to standard model particles, some as-yet unknown mechanism would be required to preserve primordial isocurvature perturbations through reheating. Primordial isocurvature perturbations could more readily survive reheating in symmetric-coupling models if the inflaton coupled to some non standard model particles, such as cold dark matter particles.
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