Cosmic microwave background radiation

Results 151 to 160 of about 1,037 (174)

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The Cosmic Microwave Background Radiation

2022
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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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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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3K: The Cosmic Microwave Background Radiation

American Journal of Physics, 1996
Bruce Partridge, Lyman Page
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A search for primordial anisotropies in the cosmic microwave background radiation: first observations at 13.5 GHz with the Cosmic Anisotropy Telescope

Monthly Notices of the Royal Astronomical Society, 1995
G Yassin, P F Scott, G Pooley
exaly

Cosmic microwave background radiation

2015
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The dipole anisotropy of the cosmic microwave background radiation

New Astronomy Reviews, 2002
Monique Signore
exaly

COBE Measures Anisotropy in Cosmic Microwave Background Radiation

Physics Today, 1992
Barbara Goss Levi, Levi Barbara Goss
exaly

Testing for Non-Gaussianity on Cosmic Microwave Background Radiation: A Review

Statistical Science, 2004
Domenico Marinucci
exaly