A fast transition between a standard matter-like era and a late ΛCDM-like epoch generated by a single Unified Dark Matter component can explain the observed acceleration of the Universe. UDM models with a fast transition should be clearly distinguishable from ΛCDM (and alternatives) through observations. Here we focus on a particularly simple model and analyse its viability by studying features of the background model and properties of the adiabatic UDM perturbations. © Springer-Verlag Berlin Heidelberg 2014.
CITATION STYLE
Rozas-Fernández, A., Bruni, M., & Lazkoz, R. (2014). Phenomenology of Unified Dark Matter Models with Fast Transition. In Springer Proceedings in Mathematics and Statistics (Vol. 60, pp. 387–390). Springer New York LLC. https://doi.org/10.1007/978-3-642-40157-2_58
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