Evolution of f<sub>NL</sub> to the adiabatic limit
Joseph Elliston; David J. Mulryne; David Seery; Reza Tavakol
Журнал:
Journal of Cosmology and Astroparticle Physics
Дата:
2011-11-01
Аннотация:
We study inflationary perturbations in multiple-field models, for which ζ typically evolves until all isocurvature modes decay — the “adiabatic limit”. We use numerical methods to explore the sensitivity of the local-shape bispectrum to the process by which this limit is achieved, finding an appreciable dependence on model-specific data such as the time at which slow-roll breaks down or the timescale of reheating. In models with a sum-separable potential where the isocurvature modes decay before the end of the slow-roll phase we give an analytic criterion for the asymptotic value of f<sub>NL</sub> to be large. Other examples can be constructed using a waterfall field to terminate inflation while f<sub>NL</sub> is transiently large, caused by descent from a ridge or convergence into a valley. We show that these two types of evolution are distinguished by the sign of the bispectrum, and give approximate expressions for the peak f<sub>NL</sub>.
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