CMB fluctuations related to dark matter and normal matter?

AI Thread Summary
The discussion highlights the relationship between cosmic microwave background (CMB) fluctuations and the presence of dark and normal matter. It notes that the CMB power spectrum exhibits strong oscillations in the multipole moment range of l=500-850, which cannot be explained by either dark matter or normal matter alone. A mixture of both types of matter is necessary to produce these oscillations, while using only one leads to a rapid fall-off in the spectrum. The conversation references external resources for further information on this topic. Understanding this interplay is crucial for comprehending the universe's composition and structure.
bcrowell
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I came across this http://scienceblogs.com/startswithabang/2010/11/the_simplest_argument_for_dark.php cutesy pop-sci-ish explanation of how we know there's dark matter. If you scroll about 1/3 of the way down, it shows plots of the CMB's power spectrum as a function of multipole moment, l. (Note that the observed plot and the theoretical plots have mismatched x axes.) The observed spectrum has strong oscillations in the region of l=500-850. If you assume only dark matter, or only normal matter, then you don't get these strong oscillations; you mainly get a rapid fall-off. Why is it that you need a mixture of dark matter and normal matter to get the strong oscillations, but if you assume only one or the other you get a rapid fall-off?
 
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Thanks, pervect! I'll have to spend some time studying that.
 
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