Modelling and research of dynamical ejection scenario of runaway stars from stellar clusters.
Note: Correct work of this code depends on paths. Some data, such as simulations parameters, was transferred to the programs using Linux terminal
This files can simulate N-body system by solving differential equations with Euler method; plot the dependence of each interaction outcome probability on semi-major axis (branching ratio)
This file plots final graphs (branching ratios) for each mass of objects
This file generates conditions for a current simulation
This file receives initial conditions from the previous file; counts simulations
This file shows object motion and energy graphs during simulation
My poster devoted to this science work, which I presented at the All-Russian Scientific Conference Scientists of the Future and took third place