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You are here: Science > Primary fluctuations
  Primary fluctuations
 
article What is the CMB and why is it useful
article Maps and spectra
article The physics behind what is observed
article The present lore: the minimal cosmological model
The physics of the CMB peaks
article The "initial conditions": The predictions from inflation
article Why peaks?
article The physics of CMB peaks - I. Influence of the baryon density
article The physics of CMB peaks - II. Influence of the Dark Matter density
article The physics of CMB peaks - III. Influence of what happens after recombination
What can be observed in the CMB fluctuations
article Matter content of the universe
 
    
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Primary fluctuations

This section presents the key ingredients that allow to understand the physics of CMB anisotropies.

Table of contents

- What is the CMB and why is it useful

- Maps and spectra

- The physics behind what is observed

- The present lore: the minimal cosmological model

More details are then given in the following headings:

- The physics of the CMB peaks

- What can be observed in the CMB fluctuations

- Back to Science

   
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