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A No-Truncation Approach to Cosmic Microwave Background Anisotropies
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We offer a method of calculating the source term in the line-of-sight integral for cosmic microwave background anisotropies without using a truncated partial-wave expansion in the Boltzmann hierarchy.
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Cited by 1 Pith paper
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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics
CLASSIER computes cosmological perturbation spectra with non-cold relics using iterated integral equations and non-uniform fast Fourier transforms, matching a converged Boltzmann hierarchy to <0.01% in the matter powe...
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