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| | B2 |
 | | Rather than detailing the zoo of proposed structure formation models, only the adiabatic inflationary model will be considered here (this choice of model is motivated by the fact that it fits the observed temperature anisotropies better than the others). |
 | | Adiabatic models further stipulate that while the overall density of the universe varied, the fraction of the material in any particular form (neutrinos, photons, baryons, cold dark matter, etc.) was initially a constant throughout space. |
 | | Therefore, in the adiabatic inflationary scenario, a well defined pattern of initial perturbations was created in the first fraction of a second after the big bang. |
| quiet.uchicago.edu /capmap/b2.htm (218 words) |
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