Large-scale cosmic flows and moving dark energy
arXiv:0811.3606 · doi:10.1088/1475-7516/2009/03/015
Abstract
Large-scale matter bulk flows with respect to the cosmic microwave background have very recently been detected on scales 100 Mpc/h and 300 Mpc/h by using two different techniques showing an excellent agreement in the motion direction. However, the unexpectedly large measured amplitudes are difficult to understand within the context of standard LCDM cosmology. In this work we show that the existence of such a flow could be signaling the presence of moving dark energy at the time when photons decoupled from matter. We also comment on the relation between the direction of the CMB dipole and the preferred axis observed in the quadrupole in this scenario.
11 pages, 2 figures. New comments and references included. Final version to appear in JCAP
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- Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
- The Evolution of Our Local Cosmic Domain: Effective Causal Limits
- Cosmological anisotropy from non-comoving dark matter and dark energy
- A class of ghost-free theories in symmetric teleparallel geometry
- The Maxwell-Chern-Simons gravity and its cosmological implications
- Warm inflation with non-comoving scalar field and radiation fluid
- Backreaction mechanism in multifluid and extended cosmologies
- Horndeski in motion