Recent data point in the direction of a cosmological constant dominated uni
verse. We investigate the role of supersymmetric QCD with N-f<N-c as a poss
ible candidate for a dynamical cosmological constant("quintes sence"). When
N-f>1, the multiscalar dynamics is fully taken into account, showing that
a certain degree of flavor symmetry in the initial conditions is necessary
in order to attain the required late-time "tracking" attractor behavior. A
possible solution to the problem of long-range interactions of gravitationa
l strength is proposed. Finally we show how, as a consequence of the intera
ction with the standard model fields, the early cosmological evolution of t
he scalar fields may be dramatically altered, and the approach to the track
ing behavior may become much more efficient.