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Dynamical Selection of the Primordial Density Fluctuation Amplitude

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arxiv 1008.4567 v2 pith:AMJK36T3 submitted 2010-08-26 hep-th astro-ph.CO

classification hep-thastro-ph.CO
keywords selectionamplitudedensitydynamicalmodelsobservedprimordialvalue
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In inflationary models, the predicted amplitude of primordial density perturbations Q is much larger than the observed value (~10^{-5}) for natural choices of parameters. To explain the requisite exponential fine-tuning, anthropic selection is often invoked, especially in cases where microphysics is expected to produce a complex energy landscape. By contrast, we find examples of ekpyrotic models based on heterotic M-theory for which dynamical selection naturally favors the observed value of Q.

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