Introduction
Our galaxy, the Milky Way, belongs to a supercluster of galaxies known as Laniakea. The main goal of this project is to estimate its gravitational backreaction or, in other words, to understand how (if at all) the latter influences our Cosmological inference. We propose a toy model where Laniakea is described as a triaxially expanding homogeneous ellipsoid, with constant expansion rate along the principal axes. To build the model we use the CF4 reconstruction of the peculiar velocity field in the local Universe, and the recently update definition of Laniakea obtained from it. In this page you will find some of our results from this paper, and some supplementary material, including interactive plots, which did not fit there. I Hope you enjoy them!
Toy Model
Best fit Ellipsoid
The Ellipsoid which best fits Laniakea Surface:
Radial Velocities
The reconstructed radial peculiar velocity field inside Laniakea, computed with respect to the centre of our best fit ellipsoid:
Theoretical prediction
The quadrupolar prediction for the radial peculiar velocity field inside Laniakea predicted by the triaxial anisotropic expansion:
Residuals
The residuals, in units of standard deviations, between the reconstructed radial peculiar velocity field and the theoretical prediction for a constant dispersion of 170 km/s :