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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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