Jeans instability in a viscoelastic fluid

被引:39
|
作者
Janaki, M. S. [1 ]
Chakrabarti, N. [1 ]
Banerjee, D. [1 ]
机构
[1] Saha Inst Nucl Phys, Kolkata 700064, W Bengal, India
关键词
DUSTY PLASMAS;
D O I
10.1063/1.3526685
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The well known Jeans instability is studied for a viscoelastic gravitational fluid using generalized hydrodynamic equations of motions. It is found that the threshold for the onset of instability appears at higher wavelengths in a viscoelastic medium. Elastic effects playing a role similar to thermal pressure are found to lower the growth rate of the gravitational instability. Such features may manifest themselves in matter constituting dense astrophysical objects. (C) 2011 American Institute of Physics. [doi: 10.1063/1.3526685]
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页数:5
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