Fluctuations of the CMB, symmetry between the hot and cold?

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SUMMARY

The discussion centers on the analysis of temperature fluctuations in the Cosmic Microwave Background (CMB) and their potential inversion symmetry about the mean. Participants explore the implications of applying Fourier transforms to regions of the CMB that are hotter and cooler than the mean, questioning whether these transforms exhibit similar statistical properties. The conversation highlights the necessity of examining correlations rather than relying solely on visual assessments or power spectra to determine symmetry. A participant's experiment using the Windows Paint app to invert colors on a fluctuation map raises questions about the perceptibility of such changes.

PREREQUISITES
  • Understanding of Cosmic Microwave Background (CMB) temperature fluctuations
  • Knowledge of Fourier transforms and their applications in signal processing
  • Familiarity with statistical analysis methods in cosmology
  • Basic skills in image processing software, such as Windows Paint
NEXT STEPS
  • Research the statistical properties of Fourier transforms in cosmological data analysis
  • Study correlation techniques used to analyze CMB fluctuations
  • Explore inversion symmetry in physical systems and its implications
  • Examine advanced image processing techniques for analyzing CMB maps
USEFUL FOR

Astronomers, cosmologists, graduate students in physics, and researchers interested in the analysis of Cosmic Microwave Background data and its implications for understanding the universe.

Spinnor
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Consider any of the latest maps of the temperature fluctuations of the CMB. Such a map can be considered a 2 dimensional topographical map of the surface of a sphere, high points hotter, low points cooler. Consider the contours that divide such a map into the two regions, fluctuations hotter then the mean and fluctuations colder then the mean.

If we now take a Fourier transform of only the region hotter then mean and compare that with the Fourier transform of the region cooler then the mean are those Fourier transforms very similar, do they have the same statistics if that question makes sense? Do the temperature fluctuations of the CMB considered as a surface have an inversion symmetry about the mean?

Or put another way, if some graduate student inverted the colors on a fluctuation map would anyone notice, would we still have a plausible fluctuations map (exclude the great void)?

I have taken such a map and with Windows Paint app inverted the colors, seems similar, see attached.

Thanks for any help!
 

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Since these are fluctuations about the average, you can't have an upward fluctuation without a downward fluctuation. Right?
 
Spinnor said:
Do the temperature fluctuations of the CMB considered as a surface have an inversion symmetry about the mean?
Interesting question. I don't think the answer is obvious. There's none apparent to the eyeball, and it would not be revealed in the usual power spectrum. You'd need to look at correlations. I suspect that if there is an asymmetry, at some level the cold fluctuations would be more sharply peaked.
 

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