Hi, this may be a silly question. In the study of white dwarfs, why we change from the non-relativistic equation of state, P(ρ)=K.ρ^(5/3), to the relativistic case, P(ρ)=K'.ρ^(4/3), when there is an increase in the central density of the star, i.e., why the electrons, which compose the Fermi...