Distance measurements to type Ia supernovae (SNe Ia) at cosmological distan
ces indicate that the Universe is accelerating and that a large fraction of
the critical energy density exists in a component with negative pressure.
Various hypotheses on the nature of this "dark energy" can be tested via th
eir prediction for the equation of state of this component. If the dark ene
rgy is due to a scalar field, its equation of state will in general vary wi
th time and is related to the potential of the held. We review the intrinsi
c degeneracies of luminosity distance measurements and compute the expected
accuracies that can be obtained for the equation of state parameter from a
realistic high statistic SNe Ia experiment. (C) 2001 Published by Elsevier
Science B.V.