Papers › Efficient Computation of CMB anisotropies in closed FRW models

Efficient Computation of CMB anisotropies in closed FRW models

10 Nov 1999arXiv:astro-ph/9911177links table onlyarchive 2025-07-28

Antony Lewis, Anthony Challinor, Anthony Lasenby

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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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alexzucca90/magcamb mentioned on GitHub report
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