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Fluctuations in the Cosmic Microwave Background Radiation

1998
The study of the power-spectrum of spatial fluctuations in the Cosmic Microwave Background Radiation provides one of the most important means of confronting theories of the origin of the large-scale structure of the Universe with observation. The problem addressed in this chapter is how to relate the fluctuations in the dark and baryonic matter on the ...
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Cosmic Microwave Background Radiation Anisotropies in Brane Worlds

Physical Review Letters, 2003
We propose a new formulation to calculate the cosmic microwave background (CMB) spectrum in the Randall-Sundrum two-brane model based on recent progress in solving the bulk geometry using a low energy approximation. The evolution of the anisotropic stress imprinted on the brane by the 5D Weyl tensor is calculated.
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Fluctuations in Cosmic Microwave Background Radiation

2013
Cosmic microwave background (CMB) radiation is composed of photons which have decoupled from electrons in the epoch of the hydrogen and helium recombination at \(z = 1{,}089\) and it is observed as the perfectly black body radiation whose averaged temperature is 2.725 K. More precisely, however, the CMB involves tiny spatial fluctuations. Theoretically,
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3K: The Cosmic Microwave Background Radiation

American Journal of Physics, 1996
Bruce Partridge, Lyman Page
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The dipole anisotropy of the cosmic microwave background radiation

New Astronomy Reviews, 2002
Monique Signore
exaly  

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