Can Non-Adiabatic Perturbations Arise After Single-Field Inflation?
classification
🌌 astro-ph
hep-phhep-th
keywords
ariseinflationnon-adiabaticperturbationscannotcosmologicalduringfield
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It is shown that non-adiabatic cosmological perturbations cannot arise during the period of reheating following inflation with a single scalar inflaton field.
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Cited by 1 Pith paper
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Generalized neutrino isocurvature
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