  Relativistic and non-relativistic fluid equations can exhibit finite time
singular solutions including density singularities appearing in collapse or
compression systems and gradient singularities in shock waves. However, only
the non-relativistic fluid equations have been shown to exhibit finite-time
velocity singularities, v tending to infinity in this regime. As this limit
violates the cosmic speed limit v<c, where c is the speed of light, it is
unclear how velocity singularity source terms in the non-relativistic equations
are modified in the relativistic equations. This paper uses a driven system to
demonstrate that singular points within the relativistic fluid equations can
generate finite time relativistic velocity singularities v tending to c.
