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• |
3He
and D abundances strongly
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constrain the
baryon density. 4He is set
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by different
physics, essentially
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thermodynamics,
fixed by neutron to
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proton
ratio. Not so for D, etc., which are
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set by
reaction sequence before T falls
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too much. In a high density universe,
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there is time
for everything to become
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4He,
giving a low D abundance. Opposite
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case for low
density.
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