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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Antony Lewis

University of Sussex

A. Challinor

Université Paris-Sud

A. Lasenby

Centre National de la Recherche Scientifique

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The Astrophysical Journal

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

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

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Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

Complete treatment of CMB anisotropies in a FRW universe· 1998 · 175 citations
Why not consider closed universes?· 1995 · 57 citations
Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges· 1995 · 1,720 citations
Relativistic radiative transfer: moment formalisms· 1981 · 292 citations
Cosmic Microwave Background Anisotropies in the Cold Dark Matter Model: A Covariant and Gauge‐invariant Approach· 1999 · 120 citations

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

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