| Very Early Universe |
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| 1. | Isotropy
– the universe looks the same in all |
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| directions,
again strictly true on large scales |
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| 2. | Small
Baryon/Anti-baryon asymmetry |
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| 3. | Close
to critical (Omega = 1) (will be HW) |
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| 4. | Initial
fluctuations to seed structure growth |
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