An approach for constructing a low-dissipation numerical method is described. The method is based on a combination of the operator-splitting method, Godunov method, and piecewise-parabolic method on the local stencil. Numerical method was tested on a standard suite of hydrodynamic test problems. In addition, the performance of the method is demonstrated on a global test problem showing the development of a spiral structure in a gravitationally unstable gaseous galactic disk. New high order accurate numerical method.New limiter-free, Galilean invariance, guaranteed non-decrease of the entropy numerical method.Numerical simulation of 2-4-7-arms spiral structure.
['Igor M. Kulikov', 'Eduard I. Vorobyov']
Using the PPML approach for constructing a low-dissipation, operator-splitting scheme for numerical simulations of hydrodynamic flows