arXiv · 0705.4426
Dynamics of Logamediate Inflation
Abstract
A computation of the inflationary observables n_{s} and r is made for `logamediate' inflation where the cosmological scale factor expands as $a=\exp (A(\ln t)^λ)$, and is compared to their predicted values in the intermediate inflationary theory, where $a=\exp (Bt^{f})$. Both versions prove to be consistent with observational measurements of the cosmic background radiation. It is shown that the dynamics of a single inflaton field can be mimicked by a system of several fields in an analogous manner to that created by the joint evolution of the fields in assisted power-law inflation.
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John D. Barrow, N. J. Nunes. 2007-07-23. Dynamics of Logamediate Inflation. https://doi.org/10.1103/physrevd.76.043501
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