August 1, 2000Open Access
Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models
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Abstract
We implement the efficient line of sight method to calculate the anisotropy and polarization of the cosmic microwave background for scalar and tensor modes in almost-Friedmann-Robertson-Walker models with positive spatial curvature. We present new results for the polarization power spectra in such models.
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Authors
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Antony Lewis
University of Sussex
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A. Challinor
Université Paris-Sud
A. Lasenby
Centre National de la Recherche Scientifique
Journals
The Astrophysical Journal
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