  We report turbulence effects on magnetic reconnection in relativistic plasmas
using 3-dimensional relativistic resistive magnetohydrodynamics simulations. We
found reconnection rate became independent of the plasma resistivity due to
turbulence effects similarly to non-relativistic cases. We also found
compressible turbulence effects modified the turbulent reconnection rate
predicted in non-relativistic incompressible plasmas; The reconnection rate
saturates and even decays as the injected velocity approaches to the Alfv\'en
velocity. Our results indicate the compressibility cannot be neglected when
compressible component becomes about half of incompressible mode occurring when
the Alfv\'en Mach number reaches about $0.3$. The obtained maximum reconnection
rate is around $0.05$ to $0.1$, which will be able to reach around $0.1$ to
$0.2$ if injection scales are comparable to the sheet length.
