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Efficient Computation of CMB anisotropies in closed FRW 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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Showing 60 of 157 Pith papers that cite this
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Multi-Agent System for Cosmological Parameter Analysis
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