 
 
| The diagram shows the CMB power spectrum using data from WMAP, CBI and ACBAR. Briefly explain exactly what the "CMB power spectrum" actually is and what the symbols l and Cl represent. | [3] | 
| Compare and contrast, carefully but without detailed mathematics, the growth of structure in a universe dominated by (i) non-baryonic cold dark matter, (ii) non-baryonic hot dark matter and (iii) baryonic matter. | [5] | 
(2005 Resit, part of Q8.)