Hi,
How is the output matter power spectrum normalized in CAMB? We have encountered discrepancies when trying to reproduce some paper plots. (In particular, the right plot in figure 7 of http://arxiv.org/pdf/astro-ph/0603494v2.pdf, in which the matter power spectrum is normalized by a factor (Omega_m(\tau))^-2. We don't understand this "choice" for normalization. Is it the standard one?)
Any help will be greatly appreciated.
Best,
Dan