Observing the Evolution of the Universe
How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the universe. Through detailed measurements one may address everything from the physics of the birth of the universe to the...
المؤلفون الرئيسيون: | , , , , , , , , , , , , , , , , , , , , , , , , |
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التنسيق: | Journal article |
منشور في: |
2009
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