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

In summary, the conversation discusses the temperature fluctuations of the CMB and whether they have an inversion symmetry about the mean. The participants also question if the Fourier transforms of the hotter and cooler regions are similar and if the fluctuations map would still be plausible if the colors were inverted. One participant notes that since these are fluctuations about the average, there cannot be an upward fluctuation without a downward fluctuation. They also mention that the answer to the inversion symmetry question is not obvious and would require further analysis.
  • #1
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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  • #2
Since these are fluctuations about the average, you can't have an upward fluctuation without a downward fluctuation. Right?
 
  • #3
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.
 

1. What are CMB fluctuations?

CMB fluctuations refer to small variations in the temperature of the cosmic microwave background (CMB) radiation, which is the leftover radiation from the Big Bang. These fluctuations are thought to be caused by quantum mechanical fluctuations in the early universe.

2. How are CMB fluctuations measured?

CMB fluctuations are measured using specialized telescopes and detectors, such as the Planck satellite and the Atacama Cosmology Telescope. These instruments measure the temperature of the CMB radiation at different points in the sky and create a map of the fluctuations.

3. What is the significance of the symmetry between hot and cold spots in the CMB?

The symmetry between hot and cold spots in the CMB is important because it provides evidence for the inflationary theory of the universe. Inflation is a period of rapid expansion in the early universe that is thought to have smoothed out any irregularities, resulting in the observed symmetry in the CMB.

4. How do CMB fluctuations support the Big Bang theory?

CMB fluctuations provide strong evidence for the Big Bang theory because they are predicted by the theory and have been observed by multiple experiments. The existence of these fluctuations is consistent with the idea that the universe began as a hot, dense state and has been expanding and cooling ever since.

5. What can we learn from studying CMB fluctuations?

Studying CMB fluctuations can provide valuable insights into the early universe and the fundamental laws of physics. By analyzing the patterns and statistics of these fluctuations, scientists can test and refine our understanding of the universe's origins and evolution. CMB fluctuations also provide information about the distribution of matter and energy in the universe, which can help us better understand the structure and composition of the universe.

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