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Planning Future Space Measurements of the CMB

Published online by Cambridge University Press:  25 May 2016

J.L. Puget ,
N. Aghanim ,
R. Gispert ,
F.R. Bouchet  and
E. Hivon
J.L. Puget
Affiliation:
Institut d'Astrophysique Spatiale, Orsay, France
N. Aghanim
Affiliation:
Institut d'Astrophysique Spatiale, Orsay, France
R. Gispert
Affiliation:
Institut d'Astrophysique Spatiale, Orsay, France
F.R. Bouchet
Affiliation:
Institut d'Astrophysique, Paris, France
E. Hivon
Affiliation:
Institut d'Astrophysique, Paris, France

Extract

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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.

Type
Part II: Contributed Papers
Information
Symposium - International Astronomical Union , Volume 168: Examining the Big Bang and the Diffuse Background Radiations , 1996 , pp. 447 - 452
Copyright
Copyright © Kluwer 1996