López Maroto, Antonio2023-06-202023-06-2020060094-243x10.1063/1.2409093https://hdl.handle.net/20.500.14352/52050© 2006 American Institute of Physics. International Conference on the Dark Side of the Universe (2nd. 2006. Madrid, Spain). This work has been partially supported by DGICYT (Spain) under project numbers FPA 2004-02602 and FPA 2005-02327.If dark energy can be described as a perfect fluid, then, apart from its equation of state relating energy density and pressure, we should also especify the corresponding rest frame. Since dark energy is typically decoupled from the rest of components of the universe, in principle such a frame could be different from that of matter and radiation. In this work we consider the potential observable effects of the motion of dark energy and the possibility to measure the dark energy velocity relative to matter. In particular we consider the modification of the usual interpretation of the CMB dipole and its implications for the determination of matter bulk flows on very large scales. We also comment on the possible origin of a dark energy flow and its evolution in different models.engjournal articlehttp://dx.doi.org/10.1063/1.2409093http://aip.scitation.orgrestricted access53Galaxy clustersVelocity-fieldAnisotropyUniverseMotionsFlowFísica-Modelos matemáticos