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On the Computation of CMBR Anisotropies from Simulations of Topological Defects

Albert Stebbins, Scott Dodelson

astro-pharXiv:astro-ph/9705177

Abstract

Techniques for computing the CMBR anisotropy from simulations of topological defects are discussed with an eye to getting as much information from a simulation as possible. Here we consider the practical details of which sums and multiplications to do and how many terms there are.

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