MAGNETOROTATIONAL INSTABILITY IN A COLLISIONAL WEAKLY IONIZED PLASMA

被引:5
|
作者
Ren, Haijun [1 ]
Cao, Jintao [2 ,3 ]
Wu, Zhengwei [1 ]
机构
[1] Univ Sci & Technol China, CAS Key Lab Basic Plasma Phys, Hefei 230026, Peoples R China
[2] Chinese Acad Sci, Inst Phys, CAS Key Lab Soft Matter Phys, Beijing 100190, Peoples R China
[3] Chinese Acad Sci, Inst Phys, Beijing Natl Lab Condensed Matter Phys, Beijing 100190, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2012年 / 754卷 / 02期
基金
中国国家自然科学基金; 中国博士后科学基金;
关键词
accretion; accretion disks; instabilities; magnetic fields; protoplanetary disks; LOCAL SHEAR INSTABILITY; MAGNETIZED DISKS; PROTOPLANETARY DISKS; ACCRETION DISKS; LINEAR-ANALYSIS; TRANSPORT; STABILITY; TURBULENCE; EVOLUTION;
D O I
10.1088/0004-637X/754/2/128
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use a multi-fluid model to describe the dynamic behavior of electrons, ions, and neutrals in a weakly ionized three-component plasma and investigate the differentially rotational instability. Charged species and neutrals are supposed to have the same angular velocity to eliminate the equilibrium current and collisions in the unperturbed state. By taking into account collisions between electrons/ions and neutrals, we derive the analytical expression of the general local dispersion relation and examine the collision effect on the rotational instability in different limiting cases. Collisions on neutrals are neglected in the first case to obtain a simplified dispersion, in which collisions play an important role in the instability criteria. In the low-frequency region, the previous result in the magnetohydrodynamic model is reproduced. The collision effect in the high-frequency case for non-magnetized electrons is found to be similar to the low-frequency region, but can induce instability for both the negative and positive radial derivative of rotational frequency.
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