Adaptively Refined Large-Eddy Simulations of Galaxy Clusters

Appendix I Color fields

There are two possibilities to implement a color field c in a fluid code. One can treat color like the density, i.e. the color variable obeys a conservation law like the density

tc+rj(vjc) =0. (I.1)

In this case c will exactly behave like density, if density and color have the same initial value.

On the other hand one can treat it like a specific quantity obeying a conservation law like

tρc+rj(vjρc) =0. (I.2)

In this case we see that if c is spatially constant at a time t0, i.e. c(t0)=c0, c(t0)rj=0, it will stay constant forever

tρc+rj(vjρc) =0
ct+vjcrj =0
ddtc =0
c =const.=c0