On the Evolution and Gravitational Collapse of a Toroidal Vortex
Astrophysics
2015-06-24 v1
Abstract
The evolution and collapse of a gaseous toroidal vortex under the action of self-gravitation are considered using the Hamiltonian mechanics approach. It is shown that evolution occurs in three main stages separated by characteristic time scales. First, a compression along the small radius to a quasi-equilibrium state takes place, followed by a slower compression along the large radius to a more stable compact vortex object. In the latter stage, the possibility of effective scattering and ejection of particles along the vortex axis (jet formation) is detected. As a result, mass, energy, and momentum losses take place, and the vortex collapses.
Cite
@article{arxiv.astro-ph/0407320,
title = {On the Evolution and Gravitational Collapse of a Toroidal Vortex},
author = {K. Yu. Bliokh and V. M. Kontorovich},
journal= {arXiv preprint arXiv:astro-ph/0407320},
year = {2015}
}
Comments
11 pages, 3 figures