Particle heating in advection-dominated accretion flows

被引：0
|
作者：
Quataert, E [1 ]
机构：
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
来源：
HIGH ENERGY PROCESSES IN ACCRETING BLACK HOLES | 1999年 / 161卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
I review particle heating by MHD turbulence in collisionless plasmas appropriate to advection-dominated accretion flows. These considerations suggest that the preferential turbulent heating of protons assumed by theoretical models is only achieved for relatively subthermal magnetic fields.
引用
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页码：404 / 409
页数：6
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