Primordial Magnetic Field Effects on the CMB and Large-Scale Structure

Figure 13

Comparison of the best-fit computed total power spectrum with the observed CMB spectra. The orange region is from the best-fit parameter set, and the allowed region is from the constrained parameter set as given in Table 1. Red, black, blue, green, orange, and purple dots with error bars show WMAP 5 years, ACBAR 08, Boomerang, CBI, CAPMAP, and DASI data, respectively. Downward arrows for the error bars on this figure indicate that the data points are upper limits. Since the BB mode is not affected by the SZ effect, the upper curves and lower curves in this figure are defined by the constrained cosmological parameters of Table 1.