astrophysics
Simulating gravitational dynamics of star clusters with varying initial conditions using leapfrog integration of Newtonian gravity with softened potentials. Reports energy conservation, bound fraction, ejected bodies, and virial ratio.
Simulating gravitational dynamics of star clusters with varying initial conditions using leapfrog integration of Newtonian gravity with softened potentials. Reports energy conservation, bound fraction, ejected bodies, and virial ratio.