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Homogeneity
– matter is uniformly spread across
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the
universe on large scales
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Isotropy
– the universe looks the same in all
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directions,
again strictly true on large scales
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Universality
– laws of physics apply everywhere in
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the
universe (being challenged!)
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These lead to the “cosmological principle” which says
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that any observer in any galaxy in the universe should see
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essentially the same features of the universe.
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