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

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© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Antony Lewis et al 2000 ApJ 538 473 DOI 10.1086/309179

0004-637X/538/2/473

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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10.1086/309179