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BIG BANG EXPANSION SCENARIOS
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[[Big Bang|
BIG BANG
]]
EXPANSION SCENARIOS
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The Universe is (1) open, (2) closed, or (3), flat, depending on whether the ratio of its
+
[[
The Universe
]]
is (1) open, (2) closed, or (3), flat, depending on whether the
[[
ratio
]]
of its
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actual density to the "critical density", called omega, is <1, >1, or precisely equal
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actual
[[
density
]]
to the "critical density", called omega, is <1, >1, or precisely equal
to 1. The "critical density" of the Universe is the density above which the Universe
to 1. The "critical density" of the Universe is the density above which the Universe
would go on expanding forever.
would go on expanding forever.
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