Query : 2007A&A...476...83M

2007A&A...476...83M - Astronomy and Astrophysics, volume 476, 83-88 (2007/12-2)

The actual Rees-Sciama effect from the local universe.


Abstract (from CDS):

Observations of the Cosmic Microwave Background (CMB) have revealed an unexpected quadrupole-octopole alignment along a preferred axis pointing toward the Virgo cluster. We here investigate whether this feature can be explained in the framework of the concordance model by secondary anisotropies produced by the non-linear evolution of the gravitational potential, the so-called Rees-Sciama (RS) effect. We focus on the effect caused by the local superclusters, which we calculate using a constrained high-resolution hydrodynamical simulation, based on the IRAS 1.2Jy all-sky galaxy redshift survey, which reproduces the main structures of our Universe out to a distance of 110Mpc from our Galaxy. The resulting RS effect peaks at low multipoles and has a minimum/maximum amplitude of -6.6µK/1.9µK. Even though its quadrupole is well aligned with the one measured for the CMB, its amplitude is not sufficient to explain the observed magnitude of the quadrupole/octopole alignment. To have an effect comparable to the actual CMB fluctuations, photons traversing the local cosmic structures would need to experience a five/ten times larger gravitational redshift than would be expected in a standard scenario with dark matter and Newtonian gravity. In addition, we analyze the WMAP-3 data with a linear matched filter in an attempt to determine an upper limit for the RS signal amplitude on large scales. We found that it is possible to infer a weak upper limit of 30µK for its maximum amplitude.

Abstract Copyright:

Journal keyword(s): cosmic microwave background

Simbad objects: 8

goto Full paper

goto View the references in ADS

Number of rows : 8
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
1 ACO 426 ClG 03 19 47.2 +41 30 47           ~ 2203 1
2 NAME Great Attractor SCG 10 32 -46.0           ~ 535 0
3 NAME Hydra I Cluster ClG 10 36 36.0 -27 31 04           ~ 826 1
4 NAME Virgo Cluster ClG 12 26 32.1 +12 43 24           ~ 6509 0
5 ACO 3526 ClG 12 48 51.8 -41 18 21           ~ 1045 2
6 NAME SHAPLEY-CENTAURUS CL SCG 13 06.0 -33 04           ~ 579 0
7 ACO 3637 ClG 19 16 59 -73 42.7           ~ 2 0
8 NAME Local Group GrG ~ ~           ~ 8155 0

To bookmark this query, right click on this link: simbad:objects in 2007A&A...476...83M and select 'bookmark this link' or equivalent in the popup menu


© Université de Strasbourg/CNRS

    • Contact