[astro-ph/0207664] Stable clustering, the halo model and non
Posted: August 11 2006
This paper (the Smith et al HaloFit paper) says:
"our preliminary investigations show that the present formalism should cope naturally with spectra containing a realistic degree of baryonic features"
Does anyone know of any updates on this? esp is it OK to input a linear theory matter power spectrum containing baryon wiggles (e.g. from CMBFAST, CAMB etc) into HaloFit? (e.g. as implemented by "nonlinear_pk = F" in CAMB).
"our preliminary investigations show that the present formalism should cope naturally with spectra containing a realistic degree of baryonic features"
Does anyone know of any updates on this? esp is it OK to input a linear theory matter power spectrum containing baryon wiggles (e.g. from CMBFAST, CAMB etc) into HaloFit? (e.g. as implemented by "nonlinear_pk = F" in CAMB).