Generalized Slow-roll Inflation in Non-minimally Coupled Theories
A. Savas Arapoglu

TL;DR
This paper develops and compares two methods for deriving slow-roll inflation equations in non-minimally coupled scalar field theories, finding that conformal transformation yields more precise spectral index calculations.
Contribution
It introduces a second method using conformal transformation to derive slow-roll equations in non-minimal coupling, improving accuracy over direct generalization.
Findings
The conformal transformation method provides more precise spectral index calculations.
Comparison shows differences between the two methods in slow-roll inflation modeling.
The paper advances understanding of inflation in non-minimally coupled theories.
Abstract
The slow-roll field equations for the case of non-minimally coupled scalar fields are obtained in two ways: first using the direct generalization of slow-roll conditions in the minimal coupling case to non-minimal one; and, second, conformal transforming the slow-roll field equations in the Einstein frame to the Jordan frame and then applying the generalized slow-roll conditions. We compare the difference of two methods in calculation of the spectral index, , for a model example. The second method seems to be more precise.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena
