Abstract
We propose an effective model to describe the backreaction on cosmological
observables induced by Laniakea, the gravitational supercluster hosting the
Milky Way, which was defined using peculiar velocity data from Cosmicflows-4
(CF4). The structure is well described by an ellipsoidal shape exhibiting
triaxial expansion, reasonably approximated by a constant expansion rate along
the principal axes. Our best fits suggest that the ellipsoid, after subtracting
the background expansion, contracts along the two smaller axes and expands
along the longest one, predicting an average expansion of $-1.1
~km/s/Mpc$. The different expansion rates within the region,
relative to the mean cosmological expansion, induce line-of-sight-dependent
corrections in the computation of luminosity distances. We apply these
corrections to two low-redshift datasets: the Pantheon+ catalog of type Ia
Supernovae (SN~Ia), and 63 measurements of Surface Brightness Fluctuations
(SBF) of early-type massive galaxies from the MASSIVE survey. We find
corrections on the distances of order $2-3\%$, resulting in a shift in the
inferred best-fit values of the Hubble constant $H_0$ of order $\Delta
H_0^SN~Ia0.5 ~km/s/Mpc$ and $\Delta
H_0^SBF1.1 ~km/s/Mpc$, seemingly worsening the
Hubble tension.
Description
[2311.00215] An effective description of Laniakea and its backreaction: Impact on Cosmology and the local determination of the Hubble constant
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