Code to perform collisionless N-body simulations.
Code to perform collisionless N-body simulations. Supports cosmological simulations with periodic boundary conditions in comoving coordinates and simulations of isolated stellar systems. Includes hydrodynamics via Smooth Particle Hydrodynamics (SPH). Uses a Barnes-Hut tree for gravity with hexadecapole expansion and Ewald summation for periodic forces. Timestepping via leapfrog integrator with individual timesteps. Uses Charm++ dynamic load balancing for massively parallel systems. Uses the Tipsy file format for I/O.
Platforms, integrations, and language support vary by plan and region. Confirm final requirements with the vendor.
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Compliance claims are normalized from current vendor documentation and independently reviewed by SOTA2.