Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-03-25
Astrophys.J. 578 (2002) 665
Astronomy and Astrophysics
Astrophysics
Version accepted for publication in ApJ (includes new section on polarization and tensor spectra). Fortran code for calculatio
Scientific paper
10.1086/342656
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 pre--computing the radiation temperature and gravitational potential transfer functions over a small sub--space 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 semi--analytic approximations which are highly accurate on all angular scales for which linear perturbation theory applies. A single power spectrum can be calculated in ~ 1 second on a desktop computer. We discuss applications to cosmological parameter estimation.
Kaplinghat Manoj
Knox Lloyd
Skordis Constantinos
No associations
LandOfFree
Rapid Calculation of Theoretical CMB Angular Power Spectra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Rapid Calculation of Theoretical CMB Angular Power Spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rapid Calculation of Theoretical CMB Angular Power Spectra will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-85842