| Other
issues |
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| • | Can also solve
for velocity perturbations and |
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| solve for
peculiar velocities as a function of |
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| epoch. |
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| • | Need to
address the relativistic case since the |
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| perturbations
begin in the radiation-dominated |
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| epoch and we
need to know how they grow. |
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| • | A key result
from the analysis is that in the |
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| radiation-dominated
universe growth is |
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| relatively
fast: |
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| • | Slows down a
lot at low z (why?). |
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