Efficient Computation of CMB anisotropies in closed FRW models

arXiv · PDF · Open in the Atlas

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• alexzucca90/magcamb
• raphkou/camb
• raphkou/camb_edf
• santiagocasas/mgcamb
• sfu-cosmo/MagCosmoMC

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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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