A note on inflationary scenario with non-minimal coupling
Abhishek Basak, Jitesh R. Bhatt

TL;DR
This paper analyzes first-order perturbations in a non-minimally coupled inflationary model, demonstrating that under slow-roll conditions, results align with adiabatic assumptions and previous findings on spectral index and coupling bounds.
Contribution
It shows that non-adiabatic perturbations in non-minimally coupled inflation can be approximated as adiabatic under slow-roll, confirming earlier results with a different approach.
Findings
Spectral index results match previous adiabatic-based calculations.
Bounds on non-minimal coupling parameter are consistent with earlier work.
Perturbation theory simplifies under slow-roll assumptions.
Abstract
We consider first order perturbation theory for a non-minimally coupled inflaton field without assuming an adiabatic equation of state. In general perturbations in non-minimally coupled theory may be non-adiabatic. However under the slow-roll assumptions the perturbation theory may look like adiabatic one. We show in the frame-work of perturbation theory, that our results of spectral index and bound on no-minimal coupling parameter agree with the results obtained using the adiabatic equation of state by the earlier authors.
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Geophysics and Gravity Measurements
