Numerical simulations of thin accretion discs with PLUTO
High Energy Astrophysical Phenomena
2014-12-30 v1
Abstract
Our goal is to perform global simulations of thin accretion discs around compact bodies like neutron stars with dipolar magnetic profile and black holes by exploiting the facilities provided by state-of-the-art grid-based, high resolution shock capturing (HRSC) and finite volume codes. We have used the Godunov-type code PLUTO to simulate a thin disc around a compact object prescribed with a pseudo-Newtonian potential in a purely hydrodynamical (HD) regime, with numerical viscosity as a first step towards achieving our goal as mentioned above.
Keywords
Cite
@article{arxiv.1412.8037,
title = {Numerical simulations of thin accretion discs with PLUTO},
author = {Varadarajan Parthasarathy and Wlodek Kluzniak},
journal= {arXiv preprint arXiv:1412.8037},
year = {2014}
}
Comments
10 pages, 7 figures, accepted to Proceedings of RAGtime