cosmodynamics

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Tuesday, March 29, 2011

Cosmology 101: The End

Welcome back to the third, and last, installment of Cosmology 101. So far, we’ve covered the history of the universe up to the present moment. But what happens next? How will our universe end? And how can we be so sure that this is how the story unfolded?
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Full story at Universe Today.
Posted by Vanessa at 2:44 PM
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Labels: big bang, CMB, cosmology, dark energy, geometry, gravity, universe, WMAP

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