arXiv:1502.04167·v2·Cosmology and Nongalactic Astrophysics
A new parameter in attractor single-field inflation
Jinn-Ouk Gong🇰🇷 · Misao Sasaki🇯🇵
Abstract
We revisit the notion of slow-roll in the context of general single-field inflation. As a generalization of slow-roll dynamics, we consider an inflaton in an attractor phase where the time derivative of is determined by a function of , . In other words, we consider the case when the number of -folds counted backward in time from the end of inflation is solely a function of , . In this case, it is found that we need a new independent parameter to properly describe the dynamics of the inflaton field in general, in addition to the standard parameters conventionally denoted by , , and . Two illustrative examples are presented to discuss the non-slow-roll dynamics of the inflaton field consistent with observations.
Comments: (v1) 11 pages; (v2) 12 pages, discussions improved including the running, to appear in Physics Letters B