关于扫掠主导性吸积流的能量
天体物理学
2009-10-31 v1
摘要
我们使用平均场 MHD 讨论了光学薄、双温度、扫掠主导性吸积流(ADAFs)的能量。如果磁场是纠结的且大致各向同性的,磁化保存不足以维持磁场在与气体等分压状态。 In such a case, we expect a fraction of the energy generated by shear in the flow to be used to build up the magnetic field strength as the gas flows in; the remaining energy heats the particles. 我们认为严格等分压磁场与 a priori reasonable 粒子加热水平不相容;相反,ADAFs 中的等离子体 (定义为气压除以磁/涡旋压)很可能是 ;相应地,黏性参数 很可能是 。
关键词
引用
@article{arxiv.astro-ph/9810117,
title = {On the Energetics of Advection-Dominated Accretion Flows},
author = {Eliot Quataert and Ramesh Narayan},
journal= {arXiv preprint arXiv:astro-ph/9810117},
year = {2009}
}
备注
24 pages, ApJ submitted