О двумерном численном КГД моделировании спирально-вихревых структур в аккреционных газовых дисках

Институт прикладной математики им. М.В. Келдыша Российской академии наук , 2017. № 1.

Елизарова Т. Г., Злотник А.А., Истомина М. А.

We derive new axially symmetric stationary solutions to the barotropic Euler equations with a body force in the isentropic and isothermal cases. They are used as the initial distributions in the related non-stationary problem. Basing on a quasi-hydrodynamic approach, we perform numerical experiments on the development of small initial perturbations of the azimuthal velocity and the formation of large structures like the density "sleeves''. Splitting of the sleeves and decreasing of the gas angular momentum in the middle of the field are observed. Also the correctness of the shallow water approximation for describing the sleeve formation is confirmed. The designed algorithm is universal and allows one to perform various numerical experiments of interest in astrophysics on a personal computer.  

Keywords: баротропная квазигазодинамическая система уравнений, finite-difference schemes, численные эксперименты, barotropic quasi-gas dynamics system of equations, stationary solutions, numerical experiments, разностная схема, gas dynamic equations, уравнения газовой динамики, polar coordinates, accretion disk, полярные координаты, стационарные решения, аккреционный диск