Clusters of Galaxies in a Weyl Geometric Approach to Gravity

Figure 6

Comparison of dark/transparent/phantom mass halos for Coma in NFW, WST, and TeVeS models, free parameters of halos for NFW and TeVeS ( with neutrino core) adapted to mass data (black error bars) at . Red error bar indicates variability of NFW halo values at  kpc (fitting the NFW profile inside the margins of empirical error bars at ); blue error bars give model errors of WST model at and .