Finsler geometric perspective on the bulk flow in the universe

Finsler geometric perspective on the bulk flow in the universe

Finsler geometric perspective on the bulk flow in the universe

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Finsler geometric perspective on the bulk flow in the universe   Astronomical observations showed that there may exist a bulk flow with peculiar velocities in the   universe, which contradicts with the CDM model. The bulk flow reveals that the observational   universe is anisotropic at large scales. In fact, a more reliable observation on the anisotropy of   spacetime comes from the CMB power spectra. The WMAP and Planck satellites both show that   there is a hemispherical power asymmetry at large-angular scales. In this paper, we propose a   “wind” scenario to the bulk flow (or the anisotropy of spacetime). Under the influence of the   “wind”, the spacetime metric could become a Finsler structure. By resolving the null geodesic   equation, we obtain the modified luminosity distance, which has a dipolar form at the leading   order. Thus, the “wind” describes well the bulk flow. In addition, we perform a least- 2 fit to the data of type Ia supernovae (SNe Ia) in t ...
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