Reproducibility despite exponential divergence in the Newtonian few-body problem
APA
Portegies Zwart, S. (2018). Reproducibility despite exponential divergence in the Newtonian few-body problem. Perimeter Institute. https://pirsa.org/18110058
MLA
Portegies Zwart, Simon. Reproducibility despite exponential divergence in the Newtonian few-body problem. Perimeter Institute, Nov. 14, 2018, https://pirsa.org/18110058
BibTex
@misc{ pirsa_PIRSA:18110058, doi = {10.48660/18110058}, url = {https://pirsa.org/18110058}, author = {Portegies Zwart, Simon}, keywords = {Other}, language = {en}, title = {Reproducibility despite exponential divergence in the Newtonian few-body problem}, publisher = {Perimeter Institute}, year = {2018}, month = {nov}, note = {PIRSA:18110058 see, \url{https://pirsa.org}} }
Energy and momentum are conserved in Newton's laws of gravitation.
Numerical integration of the equations of motion should comply to
these requirements in order to guarantee the correctness of a
solution, but this turns out to be insufficient. The steady growth of
numerical errors and the exponential divergence, renders numerical
solutions over more than a dynamical time-scale meaningless. Even
time reversibility is not a guarantee for finding the definitive
solution to the numerical few-body problem. As a consequence,
numerical N-body simulations produce questionable results. Using
brute force integrations to arbitrary numerical precision I will
demonstrate empirically that the statistics of an ensemble of resonant
3-body interactions is independent of the precision of the numerical
integration, and conclude that, although individual solutions using
common integration methods are unreliable, an ensemble of approximate
3-body solutions accurately represent the ensemble of true solutions.