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Ultra-Light Scalar Fields and the Growth of Structure in the Universe

Published 17 Sep 2010 in hep-ph and astro-ph.CO | (1009.3501v1)

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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