English

Testing the Flux-based statistical prediction of the Three-Body Problem

Earth and Planetary Astrophysics 2021-07-14 v1 Solar and Stellar Astrophysics Chaotic Dynamics

Abstract

We present an extensive comparison between the statistical properties of non-hierarchical three-body systems and the corresponding three-body theoretical predictions. We perform and analyze 1 million realizations for each different initial condition considering equal and unequal mass three-body systems to provide high accuracy statistics. We measure 4 quantities characterizing the statistical distribution of ergodic disintegrations: escape probability of each body, the characteristic exponent for escapes by a narrow margin, predicted absorptivity as a function of binary energy and binary angular momentum, and, finally, the lifetime distribution. The escape probabilities are shown to be in agreement down to the 1% level with the emissivity-blind, flux-based theoretical prediction. This represents a leap in accuracy compared to previous three-body statistical theories. The characteristic exponent at the threshold for marginally unbound escapes is an emissivity-independent flux-based prediction, and the measured values are found to agree well with the prediction. We interpret both tests as strong evidence for the flux-based three-body statistical formalism. The predicted absorptivity and lifetime distributions are measured to enable future tests of statistical theories.

Keywords

Cite

@article{arxiv.2101.03661,
  title  = {Testing the Flux-based statistical prediction of the Three-Body Problem},
  author = {Viraj Manwadkar and Barak Kol and Alessandro A. Trani and Nathan W. C. Leigh},
  journal= {arXiv preprint arXiv:2101.03661},
  year   = {2021}
}

Comments

17 pages, 11 figures