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Large-scale matter bulk flows with respect to the cosmic microwave backgroundhave very recently been detected on scales 100 Mpc/h and 300 Mpc/h by using twodifferent techniques showing an excellent agreement in the motion direction.However, the unexpectedly large measured amplitudes are difficult to understandwithin the context of standard LCDM cosmology. In this work we show that theexistence of such a flow could be signaling the presence of moving dark energyat the time when photons decoupled from matter. We also comment on the relationbetween the direction of the CMB dipole and the preferred axis observed in thequadrupole in this scenario.

Large-scale cosmic flows and moving dark energy