(3+1)-dimensional relativistic hydrodynamical expansion of hot and dense   matter in ultra-relativistic nuclear collision
  A full (3+1)-dimensional calculation using the Lagrangian hydrodynamics is proposed for relativistic nuclear collisions. The calculation enables us to evaluate anisotropic flow of hadronic matter which appears in non-central and/or asymmetrical relativistic nuclear collisions. Applying hydrodynamical calculations to the deformed uranium collisions at AGS energy region, we discuss the nature of space-time structure and particle distributions in detail. 
Chiho Nonaka, Eiji Honda, Shin Muroya