Why is the CMB power spectrum often plotted as l(l+1) C_l and not only C_L ?

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SUMMARY

The Cosmic Microwave Background (CMB) power spectrum is typically plotted as $$\ell(\ell+1)C_\ell$$ rather than just $$C_\ell$$ to accurately represent the power per unit logarithmic interval in $$\ell$$. This method highlights the plateau observed at low $$\ell$$ values, which corresponds to scale invariance expected at large angular scales. The relationship between $$\ell(\ell+1)$$ and the power spectrum provides a clearer visualization of the underlying physics and the distribution of power across different scales.

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Anne-Sylvie
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Hello everybody, (sorry for the eventual Engrish)

I can't find any convincing answer for the following question :

Why do we always (or often) plot the CMB power spectrum in this way :
jb.man.ac.uk/research/cosmos/vsa/images/CMB_power_spectrum.gif

I mean the y-axis is $$C_\ell \ell (\ell+1)$$ and not only $$C_\ell. $$ Why ?

Thanks for your answer. I already heard that its because of we want show the plateau at low l. But if it is the answer, why is the plateau proportional to $$\ell (\ell +1) ?$$

Thanks :)
 
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From http://relativity.livingreviews.org/open?pubNo=lrr-1998-11&page=articlesu14.html
The reason for plotting \ell \left( \ell + 1 \right) C_\ell is that it approximately equals the power per unit logarithmic interval in \ell.

If a log scale is used for \ell, scale invariance is a flat line. Scale invariance is expected at large angular scales (low \ell), hence the plateau.
 
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