The non-adiabatic pressure in general scalar field systems
classification
🌌 astro-ph
keywords
perturbationfieldnon-adiabaticcurvaturepressurescalarsystemsaction
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We discuss the non-adiabatic or entropy perturbation, which controls the evolution of the curvature perturbation in the uniform density gauge, for a scalar field system minimally coupled to gravity with non-canonical action. We highlight the differences between the sound and the phase speed in these systems, and show that the non-adiabatic pressure perturbation vanishes in the single field case, resulting in the conservation of the curvature perturbation on large scales.
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