Juliacon 2024

Time-reversible or symplectic methods are very useful for long-term integration of planetary systems with a constant step size. However, in the case of n-body problems involving close encounters, adaptive time-stepping is required. We present a SIMD-vectorized integrator for few-body problems which incorporates a robust time-reversible adaptivity mechanism that makes it highly performant for the long-term numerical integration of problems with close-encounters.