Understand CMB Anisotropies & Interpret Figures

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Discussion Overview

The discussion focuses on understanding the Cosmic Microwave Background (CMB) anisotropies, specifically interpreting figures related to the C_l^{TT} parameter and the characteristics of the CMB power spectrum. Participants explore the implications of peak formations in the power spectrum and the significance of the multipole index l.

Discussion Character

  • Technical explanation
  • Conceptual clarification
  • Exploratory

Main Points Raised

  • One participant seeks clarification on the information extracted from CMB figures, particularly regarding the peak formations and the use of the multipole index l.
  • Another participant explains that the downward trend after the first peak is attributed to the transition of primordial plasma to gas, which causes blurriness at the surface of last scattering, impacting power at small angular scales.
  • The first peak is described as the "sound horizon," representing the distance sound waves could travel in the primordial plasma before the CMB was emitted.
  • Differences between even and odd peaks are attributed to the roles of normal and dark matter, with normal matter contributing to all peaks and dark matter contributing only to odd-numbered peaks.
  • The explanation includes that the ratio of odd-to-even peaks provides sensitive measurements of the normal matter to dark matter ratio.
  • It is noted that the multipole index l is used because the geometry of the sky resembles a sphere, and spherical harmonics are employed to analyze the power spectrum.

Areas of Agreement / Disagreement

Participants present various explanations and interpretations regarding the CMB power spectrum, but there is no clear consensus on all aspects of the discussion, particularly regarding the implications of the peak formations and the roles of different types of matter.

Contextual Notes

Some assumptions about the nature of the primordial plasma and the effects of dark matter on the peaks are not fully explored, leaving room for further clarification and discussion.

ChrisVer
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Can someone help me understand what information we extract from such kind of figure?

2000px-PowerSpectrumExt.svg.png


In fact the [itex]C_l^{TT}[/itex] parameter gives us information on the amplitude of the temperature fluctuations [itex]\Delta T/T[/itex]... However I don't understand why there is such a peak formation (1 very large, 2 smaller and 2 even smaller), or why this is given in terms of multipole index [itex]l[/itex].
 
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Some of the primary features on this graph:
1. The overall downward trend after the first peak is due to the fact that the primordial plasma took hundreds of thousands of years to transition to a gas. This has the impact of making the surface of last scattering (where the CMB photons came from) blurry. That blurriness is suppresses power at small angular scales. If it were not for this blurring effect, the CMB power spectrum would have very little overall increasing or decreasing trend.
2. The first peak is the "sound horizon". This is the distance that sound waves in the primordial plasma were able to travel from the time inflation ended to the time the CMB was emitted.
3. The difference in the even and odd peaks is due to dark matter. Within the primordial plasma, normal matter was able to bounce back out of gravity wells, while dark matter would just fall in. The first peak represents matter that just had enough time to fall into a gravitational potential well. The second peak is matter that had enough time to fall in and bounce back out. The third peak is matter that fell in, bounced out, then fell back in again. Normal matter contributes to all of the peaks, while dark matter only contributes to the odd-numbered peaks. This ratio of odd-to-even peaks is the most sensitive measurement we have of the ratio of normal matter to dark matter.

There are other things we can glean from the CMB power spectrum, but hopefully you can see why there is the overall trend here.

As for while it's given in terms of multipole index, this is because the sky has the geometry of the surface of a sphere, and the equivalent to Fourier transforms on the surface of a sphere are Spherical Hermonic transforms. In spherical harmonics, the power spectrum [itex]C_\ell[/itex] is the variance of all waves on the sky which have a wavelength on the sky of approximately [itex]\pi/\ell[/itex] radians across the surface of the sky.
 

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