320Knowledge of transport properties of matter at high pressures and high temperatures is extremely impor tant. One of obvious examples of liquid at high pres sure and high temperature is Earth outer core which is supposed to be liquid. However, nowadays it is not possible to carry out any experiments at such extreme conditions. The extreme conditions region is also hard for theoretical investigations and simulation studies. Importantly, all theoretical models are developed for normal conditions, and we can never be sure that the same models are applicable at high pressure and tem perature. Basing on this speculation it becomes impor tant to carry out a systematic study of some simple model in wide range of pressures and temperatures in order to see the most important effects induced by pressure and temperature. Such investigation will give a solid base for studies of more complex and more realistic systems.In this work we choose a soft spheres system as a generic model for high pressure atomic systems. This system is defined by the interaction potential (1) where ε and σ are energy and length scales. This sys tem is convenient for our goals since its thermody namic quantities follow well known scaling laws [1][2][3][4][5]). An important consequence of this scaling is that the soft spheres phase diagram is one dimensional, and it is known at all temperatures. This allows us to carry out simulations up to very high temperatures and pres sures being sure that the system is in stable liquid phase. ¶ The article is published in the original.Obviously, soft sphere system is a toy model of a real liquid. However, at high pressures and tempera tures the behavior of substances is mostly governed by repulsive cores atoms. This makes soft spheres one of the simplest qualitative models of matter at extremely high temperatures and pressures.It is well known that the thermodynamic properties of the soft sphere system can be expressed in terms of a reduced parameter, γ = ρσ 3 (k B T/ε) -3/n , where ρ is the reduced number density (ρ = N/V, for N particles in volume V), k B is the Boltzmann constant and T is the temperature (Klein theorem [1-3]). It may be shown [1-5] that the following scaling laws are valid along the melting line (we skip the Boltzmann con stant in the formulas below for the sake of brevity):(2)where V 0 , T 0 , and P 0 are some arbitrary values of vol ume, temperature and pressure.The exponents in (2) and (3) were known before (see, for example, [3]). However, in [5] the method was developed which can be applied to any physical quantity of the form F = under the trans formation which preserves the form of Hamiltonian equations. This transformation conserves geometric relations on a phase trajectory, thereby preserving the scaling of the individual trajectories of each of the N particles and, hence, it conserves the multiphase nature of the whole system. The simplest example of a phase equilibrium curve is the two phase meltingMolecular dynamics computer simulation has been used to compute in wide pressure te...