Figure 11From: GPU-enabled particle-particle particle-tree scheme for simulating dense stellar cluster system Time evolution of the core density (top) and the core radius (bottom). Thick and thin curves show the results of the \(\mathrm{P}^{3}\mathrm{T}\) and Hermite scheme, respectively. The curves for different runs are vertically shifted by a factor of 8 (top) and 2 (bottom).Back to article page