Simulating radially outward winds within a turbulent gas clump
Abstract
By using the particle-based code Gadget2, we follow the evolution of a gas clump, in which a gravitational collapse is initially induced. The particles representing the gas clump have initially a velocity according to a turbulent spectrum built in a Fourier space of 64 grid elements. In a very early stage of evolution of the clump, a set of gas particles representing the wind, suddenly move outwards from the clump's center. We consider only two kinds of winds, namely: one with spherical symmetry and a second one being a bipolar collimated jet. In order to assess the dynamical change in the clump due to interaction with the winds, we show iso-velocity and iso-density plots for all our simulations.
Cite
@article{arxiv.1603.08956,
title = {Simulating radially outward winds within a turbulent gas clump},
author = {Guillermo Arreaga-Garcia and Silvio Oreste Topa},
journal= {arXiv preprint arXiv:1603.08956},
year = {2016}
}
Comments
To appear in book entitled "Recent Advances in High Performance Computer applications", I. Gitler and J. Klapp (Eds.), 2016, Communications in Computer and Information Science (CCIS), Springer