Efficient Computation of CMB anisotropies in closed FRW 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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Publication date Created: 10 November 1999

Publication date Updated: 2000-06-01

Article

DOI: 10.1086/309179

ArXiV ID: astro-ph/9911177

SO-VID: fb7db69f-f27e-4b0d-bf38-c0a6feeb0e33

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Journal reference Astrophys.J.538:473-476,2000

Comments 4 pages, 1 figure. Corrected/updated references. Accepted by ApJ. For the F90 source code see http://www.mrao.cam.ac.uk/~aml1005/cmb/

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