Ultra-Light Scalar Fields and the Growth of Structure in the Universe
Abstract
Ultra-light scalar fields, with masses of between m=10-33 eV and m=10-22 eV, can affect the growth of structure in the Universe. We identify the different regimes in the evolution of ultra-light scalar fields, how they affect the expansion rate of the universe and how they affect the growth rate of cosmological perturbations. We find a number of interesting effects, discuss how they might arise in realistic scenarios of the early universe and comment on how they might be observed.
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