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A No-Truncation Approach to Cosmic Microwave Background Anisotropies

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arxiv astro-ph/0607076 v2 pith:WMGQXGKB submitted 2006-07-05 astro-ph gr-qchep-th

classification astro-phgr-qchep-th
keywords anisotropiesbackgroundcosmicmicrowaveapproachboltzmanncalculatingexpansion
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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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  1. Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics

    astro-ph.CO 2025-06 conditional novelty 6.0 of 10

    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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