In this paper, a new hydrodynamics code to simulate astrophysical flows on Intel Xeon Phi
KNL and Intel Xeon Scalable processors is presented. A new vector high-order accuracy …

Aims. The initial stages of planet formation may start concurrently with the formation of a gas-
dust protoplanetary disk. This makes the study of the earliest stages of protoplanetary disk …

A new code to simulate special relativistic hydrodynamic flows on supercomputer
architectures with distributed memory is described. The code is based on a combination of …

In this paper, a new approach to vectorization of algorithms of computational fluid dynamics
to simulate the dynamics of astrophysical objects is presented. A co-design of a …

A new parallel code based on models of special relativistic hydrodynamics is presented for
describing interacting flows. A new highly accurate numerical method is considered and …

A construction of the original HLL method for solving problems of relativistic hydrodynamics
by using a piecewise-parabolic reconstruction of the physical variables is described. The …

The Rusanov solver for solving hydrodynamic equations is one of the most robust schemes
in the class of Riemann solvers. For special relativistic hydrodynamics, the robustness …

Aims. Our aim is to derive a fast and accurate method for computing the gravitational
potential of astrophysical objects with high contrasts in density, for which nested or adaptive …

Based on the theory of dynamic adaptive chemistry and dynamic cell clustering, a 3D model
for fuel combustion in the cylinder is constructed to study the fast calculation algorithm to …

The rapid growth of supercomputer technologies became a driver for the development of
natural sciences. Most of the discoveries in astronomy, in physics of elementary particles, in …