Jeans self gravitational instability of strongly coupled quantum plasma

2014 ◽  
Vol 21 (7) ◽  
pp. 072104 ◽  
Author(s):  
Prerana Sharma ◽  
R. K. Chhajlani
2020 ◽  
Vol 58 (6) ◽  
pp. 781-788
Author(s):  
P. R. Dip ◽  
M. A. Hossen ◽  
M. Salahuddin ◽  
A. A. Mamun

2019 ◽  
Vol 99 (5) ◽  
Author(s):  
Zh. A. Moldabekov ◽  
H. Kählert ◽  
T. Dornheim ◽  
S. Groth ◽  
M. Bonitz ◽  
...  

2014 ◽  
Vol 81 (2) ◽  
Author(s):  
Prerana Sharma ◽  
R. K. Chhajlani

The Jeans self-gravitational instability is studied for dense quantum viscous plasma with Hall term and intrinsic magnetization generated by collective electron spin. The quantum magnetohydrodynamic model is employed to formulate the basic equations of the problem. The dispersion relation is obtained using the normal mode analysis, and further reduced for both transverse and longitudinal modes of propagation. The transverse mode of propagation is found to be unaffected by the Hall term but affected by quantum effect, viscosity, and magnetization parameters. The Jeans criterion of instability in the transverse direction is modified by Alfven velocity, magnetization parameter, and quantum effect. The non-gravitating magnetized mode is obtained in the longitudinal direction, which is modified by Hall parameter and is not affected by quantum term, whereas the gravitational mode is unaffected by the magnetization parameter but affected by viscosity and quantum parameters. It is observed that the Jeans condition of instability is affected by the quantum term. The growth rate of Jeans instability is plotted for various values of magnetization, quantum, and viscosity parameters of the quantum plasma medium.


2019 ◽  
Vol 57 (6) ◽  
pp. 813-820
Author(s):  
M. R. Hossen ◽  
S. A. Ema ◽  
A. A. Mamun

2017 ◽  
Vol 83 (2) ◽  
Author(s):  
Shraddha Argal ◽  
Anita Tiwari ◽  
R. P. Prajapati ◽  
P. K. Sharma

The present problem deals with the study of gravitational (Jeans) instability of magnetized, rotating, anisotropic plasmas considering quantum effects. The basic equations of the considered system are constructed using combined Chew–Goldberger–Low (CGL) fluid model and quantum magnetohydrodynamic (QMHD) fluid model. A dispersion relation is obtained using the normal mode technique which is discussed for transverse and longitudinal modes of propagation. It is found that a rotating quantum plasma influences the gravitational mode in transverse propagation but not in longitudinal propagation. The presence of rotation decreases the critical wavenumber and it has a stabilizing effect on the Jeans instability criterion of magnetized quantum plasma in transverse propagation. The firehose instability is unaffected due to the presence of uniform rotation and quantum corrections. We observe from the numerical analysis that region of instability and critical Jeans wavenumber are both decreased due to the presence of uniform rotation. The stabilizing influence of uniform rotation is observed for magnetized, rotating, anisotropic plasmas in the presence of quantum correction. In the case of a longitudinal mode of propagation we found the Jeans instability criterion is not affected by rotation. The quantum diffraction term has a stabilizing effect on the growth rate of the Jeans instability when the wave propagates along the direction of the magnetic field.


2012 ◽  
Vol 19 (7) ◽  
pp. 072123 ◽  
Author(s):  
Samiran Ghosh ◽  
Nikhil Chakrabarti ◽  
P. K. Shukla

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