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Planning Future Space Measurements of the CMB
Published online by Cambridge University Press: 25 May 2016
Extract
A central problem in cosmology is the building and testing of a full and detailed theory for the formation of (large-scale) structures in the Universe. It is widely believed that the observed structures today grew by gravitational instability out of very small density perturbations. Such perturbations should have left imprints as small temperature anisotropies in the cosmic microwave background (CMB) radiation.
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- Part II: Contributed Papers
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- Copyright © Kluwer 1996
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