Using monomer-resolved molecular dynamics simulations and theoretical argum
ents based on the radial dependence of the osmotic pressure in the interior
of a star, we systematically investigate the effective interactions betwee
n hard, colloidal particles and star polymers in a good solvent. The releva
nt parameters are the size ratio q between the stars and the colloids, as w
ell as the number of polymeric arms f (functionality) attached to the commo
n centre of the star. By covering a wide range of q's ranging from zero (st
ar against a flat wall) up to about 0.75, we establish analytical forms for
the star-colloid interaction which are in excellent agreement with simulat
ion results. A modified expression for the star-star interaction for low fu
nctionalities, f less than or similar to 10 is also introduced.