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Old December 22nd 12, 12:03 AM posted to sci.astro
Steve Willner
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Default It seems that as Dark Energy increases, Dark Matter decreases as time goes on

SW Dark matter is just matter. Its exact nature is
SW unknown except that most of it is non-baryonic.

In article ,
dlzc writes:
Based on what is this conclusion reached?


Originally on abundances of light nuclides:
http://astro.berkeley.edu/~mwhite/darkmatter/bbn.html

Nowadays I think CMB fluctuations provide tighter constraints:
http://map.gsfc.nasa.gov/resources/camb_tool/index.html

I don't understand the rest of the post.

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