Comparing sharp and smooth transitions of the second slow-roll parameter in single-field inflation
Jason Kristiano, Jun'ichi Yokoyama

TL;DR
This paper compares sharp and smooth transitions of the second slow-roll parameter in single-field inflation, analyzing their effects on curvature perturbations and non-Gaussianities, with implications for the validity of the Wands duality.
Contribution
It introduces a detailed comparison of sharp versus smooth transitions of the second slow-roll parameter and their impact on the bispectrum and loop corrections in inflation.
Findings
Wands duality condition determines vanishing of certain corrections.
Sharp transitions cause large one-loop corrections at the transition.
Smooth transitions maintain smaller, controlled corrections.
Abstract
In single-field inflation, violation of the slow-roll approximation can lead to growth of curvature perturbation outside the horizon. This violation is characterized by a period with a large negative value of the second slow-roll parameter. At an early time, inflation must satisfy the slow-roll approximation, so the large-scale curvature perturbation can explain the cosmic microwave background fluctuations. At intermediate time, it is viable to have a theory that violates the slow-roll approximation, which implies amplification of the curvature perturbation on small scales. Specifically, we consider ultraslow-roll inflation as the intermediate period. At late time, inflation should go back to the slow roll period so that it can end. This means that there are two transitions of the second slow-roll parameter. In this paper, we compare two different possibilities for the second…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Cosmology and Gravitation Theories
