We consider the effect of various particles on the cosmic expansion ra
te relative to that of the graviton. Effectively massless fermions, ga
uge bosons and conformally coupled scalars make only minuscule contrib
utions due to local conformal invariance. Minimally coupled scalars ca
n give much stronger contributions, but they are still sub-dominant to
those of gravitons on account of global conformal invariance. Unless
effectively massless scaler particles with very particular couplings e
xist, the leading effect on the expansion rate is furnished solely by
the graviton. An upper bound on the mass of such scalar particles is o
btained. (C) 1998 Elsevier Science B.V. All rights reserved.