We discuss a new numerical method for solving the relativistic hydrody
namic equations based upon the basis-spline collocation approach. Anal
ytical and numerical results are compared for several problems, includ
ing one-dimensional expansions and collisions for which analytical sol
utions exist. Our methods, which may be easily and massively paralleli
zed, are shown to give numerical results which agree to within a few p
ercent of the analytic solutions. We discuss the relevance of the v =
z/t scaling solutions for the one-dimensional problem when applied to
relativistic heavy-ion collisions. Finally, we discuss applications to
three-dimensional problems, and present results for a typical three-d
imensional expansion.