On the Computation of CMBR Anisotropies from Simulations of Topological Defects
arXiv: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.
16 pages, 2 figures from talk at ``Topological Defects in Cosmology'', Rome, October 1996