Was the Universe Not Perfectly Homogeneous at Photon-Decoupling?

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SUMMARY

The discussion centers on the implications of Cosmic Microwave Background (CMB) fluctuations regarding the universe's homogeneity and isotropy at photon-decoupling. Participants assert that the CMB fluctuations, attributed to varying dark matter densities, indicate a lack of homogeneity rather than perfect isotropy. It is concluded that while the universe is statistically homogeneous and isotropic on large scales, small-scale fluctuations reveal complexities that challenge this notion. The relationship between inhomogeneity and anisotropy is emphasized, with the consensus that CMB anisotropy is primarily due to inhomogeneous matter distribution.

PREREQUISITES
  • Understanding of Cosmic Microwave Background (CMB) theory
  • Familiarity with concepts of homogeneity and isotropy in cosmology
  • Knowledge of dark matter and its role in cosmic structure
  • Basic mathematical principles related to spatial and angular dispersion
NEXT STEPS
  • Research the implications of CMB fluctuations on cosmological models
  • Study the role of dark matter in the formation of cosmic structures
  • Explore mathematical frameworks for analyzing homogeneity and isotropy
  • Investigate current methods for measuring CMB inhomogeneity
USEFUL FOR

Astronomers, cosmologists, and physics students interested in the early universe, CMB analysis, and the fundamental properties of cosmic structures.

Niles
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Hi guys

Please take a look at this familiar picture: http://www.astr.ua.edu/keel/galaxies/wmap_map.jpg

Does this imply that the universe was not perfectly homogeneous or that it was anisotropic at the time of photon-decoupling?

Since the CMB-fluctuations are because of the different dark-matter densities, I would say that it is because of lack of homogenity. Am I corret?
 
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Strictly speaking, it is neither homogeneous nor isotropic.
The Universe is (more or less) statistically homogeneous and statistically isotropic averaged over all small scale fluctuations of density, temperature, velocity and grav.potential.
Those fluctuations are actually small - only about 1 part in 100,000 (they are enhanced for the picture).
 
But if to be very correct, the fluctuation are because of different densities in matter, so it must be lack of homogeneity?
 
It's a matter or your personal preference.
Spatial dispersion is usually being related to inhomogeneity,
angular dispersion - to anisotropy. Thus people usually prefer to say that anisotropy of CMB is caused by inhomogeneity of matter. You can say, as well, that inhomogeneity of CMB is caused by anisotropy of matter. Unfortunately, we cannot experimentally prove the second case, since we cannot travel in space far enough to measure CMB inhomogeneity.
Mathematically:
Inhomogeneous=>anisotropic, isotropic in every point => homogeneous.
 
Excellent, thanks!
 

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