Experimental particle spectra can be successfully described by power-law tailed energy distributions characteristic to canonical equilibrium distributions associated to Rényi's or Tsallis' entropy formula -over a wide range of energies, colliding system sizes, and produced hadron sorts. In order to derive its evolution one needs a corresponding dynamical description of the system which results in such final state observables. The equations of relativistic fluid dynamics are obtained from a non-extensive Boltzmann equation consistent with Tsallis' non-extensive q-entropy formula. The transport coefficients like shear viscosity, bulk viscosity, and heat conductivity are evaluate based on a linearized collision integral. PACS. 24.10.Nz Hydrodynamic models -05.70.-a Entropy in thermodynamics -05.20.Dd Kinetic theory in statistical mechanics -47.75.+f Relativistic fluid dynamics 2 Non-extensive statistics, kinetic and fluid dynamical equations A non-extensive q-generalization of the Boltzmann-Gibbs (BG) entropy was proposed by C. Tsallis [19,26] based on