MHD simulations of resistive viscous accretion disk around millisecond pulsar
High Energy Astrophysical Phenomena
2018-02-02 v1
Abstract
We perform MHD simulations of a thin resistive and viscous accretion disk around a neutron star with the surface dipolar magnetic field of 10 Gauss. The system evolution is followed during the interval of 500 millisecond pulsar rotations. Matter is accreted through a stable accretion column from the disk onto the star. We also show propagation of the stellar wind through the corona. Analysis of the mass accretion flux and torques on the star shows that the disk reaches the quasi-stationary state.
Keywords
Cite
@article{arxiv.1802.00261,
title = {MHD simulations of resistive viscous accretion disk around millisecond pulsar},
author = {M. Čemeljić and V. Parthasarathy and W. Kluźniak},
journal= {arXiv preprint arXiv:1802.00261},
year = {2018}
}
Comments
4 pages, published as a poster contribution to "International Conference Physics of Neutron Stars-2017. 50 years after." in St.Petersburg, Russia