August 1, 2000Open Access

Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models

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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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Lewis et al. (Tue,) studied this question.

synapsesocial.com/papers/69d6c86cfca0359822aa87e5 https://doi.org/https://doi.org/10.1086/309179

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Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models

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Cite This Study

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Discussion

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References and Citations

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