Year: 2002
Type: article
Abstract: We have developed a fast method for predicting the angular power spectrum C l of the cosmic microwave background given cosmological parameters and a primordial power spectrum of perturbations. After precomputing the radiation temperature and gravitational potential transfer functions over a small subspace of the total model parameter space, the rest of the model space (six or more cosmological parameters and arbitrarily many primordial power spectrum parameters) is reached via rapid analytic and semianalytic approximations that are highly accurate on all angular scales for which linear perturbation theory applies. A single power spectrum can be calculated in ~1 s on a desktop computer. We discuss applications to cosmological parameter estimation.
Source: The Astrophysical Journal
DOI: 10.1086/342656
Institution: University of California, Davis
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W1978079086
