Sitnikov problem as a source of jets

TL;DR

This paper explores how the Sitnikov problem, involving two close binaries and a third small body, can explain astrophysical jets through rapid ejection mechanisms, with potential relativistic velocities.

Contribution

It introduces the Sitnikov problem as a novel dynamical mechanism for jet formation in astrophysics, linking celestial mechanics to high-velocity ejections.

Findings

Rapid ejection of small bodies from binaries can produce jets.

Relativistic velocities are achievable with suitable initial conditions.

Proposes a new dynamical explanation for astrophysical jets.

Abstract

Sitnikov problem, consisting two close binaries and a third small body is considered, leading to a rapid ejection of the small body from the binaries. This mechanism is proposed as an explanation of jets in many astrophysical systems. Choosing appropriate initial condition relativistic final velocities can be achieved.