Testing the flux-based statistical prediction of the three-body problem

Viraj Manwadkar*, Barak Kol, Alessandro A. Trani, Nathan W.C. Leigh

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

28 Scopus citations

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 analyse 1 million realizations for each different initial condition considering equal and unequal mass three-body systems to provide high-accuracy statistics. We measure four 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 per cent 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.

Original languageEnglish
Pages (from-to)692-708
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume506
Issue number1
DOIs
StatePublished - Sep 2021

Bibliographical note

Publisher Copyright:
© 2021 The Author(s)

Keywords

  • celestial mechanics
  • chaos
  • gravitation
  • planets and satellites: dynamical evolution and stability

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