Assessing the Hierarchical Hamiltonian Splitting Integrator for Collisionless N -Body Simulations

ABSTRACT The large dynamic range in some astrophysical N-body problems led to the use of adaptive multi-time-steps; however, the search for optimal strategies is still challenging. We numerically quantify the performance of the hierarchical Hamiltonian Splitting (HHS) integrator for collisionless simulations using a direct summation code. We compare HHS with the constant global time-step leapfrog integrator, and with the adaptive one (AKDK). We find that HHS is approximately reversible, whereas AKDK is not. Therefore, it is possible to find a combination of parameters such that the energy drift is considerably milder for HHS, resulting in a better performance. We conclude that HHS is an attractive alternative to AKDK, and it is certainly advantageous for direct summation and P3M codes. Also, we find advantages with GADGET4 (Tree/FMM) HHS implementation that are worth exploring further.

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Bibliographic Details
Main Authors: Aguilar-Argüello,G., Valenzuela,O., Velázquez,H., Clemente,J. C., Trelles,J. A.
Format: Digital revista
Language:English
Published: Universidad Nacional Autónoma de México, Instituto de Astronomía 2022
Online Access:http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012022000200197
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