A No-Truncation Approach to Cosmic Microwave Background Anisotropies

Details A No-Truncation Approach to Cosmic Microwave Background Anisotropies A No-Truncation Approach to Cosmic Microwave Background Anisotropies

2006-07-05

arxiv.org/abs/astro-ph/0607076v2

Phys.Rev. D74 (2006) 063517

Astronomy and Astrophysics

Astrophysics

16 pages. Figure added, some typographical errors corrected

Scientific paper

10.1103/PhysRevD.74.063517

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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