The cosmological bulk flow: consistency with $Λ$CDM and $z\approx 0$ constraints on $σ_8$ and $γ$

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Two added figures. Emphasizes the robustness of the new method, ASCE, to the choice of the prior. Emphasizes the agreement of

Scientific paper

We derive estimates for the cosmological bulk flow from the SFI++ Tully-Fisher (TF) catalog. For a sphere of radius $40 \hmpc$ centered on the MW, we derive a bulk flow of $333 \pm 38\kms $ towards Galactic $ (l,b)=(276^\circ,14^\circ)$ within a $3^\circ$ $1\sigma$ error. Within a $ 100\hmpc$ we get $ 257\pm 44\kms$ towards $(l,b)=(279^\circ, 10^\circ)$ within a $6^\circ$ error. These directions are at a $40^\circ$ with the Supergalactic plane, close to the apex of the motion of the Local Group of galaxies after the Virgocentric infall correction. Our findings are consistent with the $\Lambda$CDM model with the latest WMAP best fit cosmological parameters. But the bulk flow allows independent constraints. For WMAP inferred Hubble parameter $h=0.71$ and baryonic mean density parameter $\Omega_b=0.0449$, the constraint from the bulk flow on the matter density $\Omega_m$, the normalization of the density fluctuations, $\sigma_8$, and the growth index, $\gamma$, can be expressed as $\sigma_8\Omega_m^{\gamma-0.55}(\Omega_m/0.266)^{0.28}=0.86\pm 0.11$ (for $\Omega_m\approx 0.266$). Fixing $\sigma_8=0.8$ and $\Omega_m=0.266$ as favored by WMAP, we get $\gamma=0.495\pm 0.096$. The constraint derived here rules out popular DGP models at more than the 99% confidence level. Our results are based on a method termed \ace\ (All Space Constrained Estimate) which reconstructs the bulk flow from an all space three dimensional peculiar velocity field constrained to match the TF measurements. At large distances \ace\ generates a robust bulk flow from the SFI++ that is insensitive to the assumed prior. For comparison, a standard straightforward maximum likelihood estimate leads to very similar results.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The cosmological bulk flow: consistency with $Λ$CDM and $z\approx 0$ constraints on $σ_8$ and $γ$ does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The cosmological bulk flow: consistency with $Λ$CDM and $z\approx 0$ constraints on $σ_8$ and $γ$, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The cosmological bulk flow: consistency with $Λ$CDM and $z\approx 0$ constraints on $σ_8$ and $γ$ will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-266158

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.