Comparative Study of Two-Valley Models for Space Charge Wave Propagation in GaAs Semiconductor Films

Author(s):  
V. Grimalsky ◽  
A. Garcia ◽  
E. Gutierrez
1984 ◽  
Vol 27 (7) ◽  
pp. 1808 ◽  
Author(s):  
D. L. Fenstermacher ◽  
C. E. Seyler

1985 ◽  
Vol 28 (1) ◽  
pp. 358-365 ◽  
Author(s):  
A. Anselmo ◽  
G. Kerslick ◽  
J. A. Nation ◽  
G. Providakes

1976 ◽  
Vol 47 (10) ◽  
pp. 4464-4466 ◽  
Author(s):  
R. A. Mahaffey ◽  
D. B. Batchelor ◽  
A. W. Trivelpiece

1977 ◽  
Vol 64 (1) ◽  
pp. 53-55 ◽  
Author(s):  
Toshitaka Idehara ◽  
Kuni Nakajima ◽  
Yoshio Ishida

2019 ◽  
Vol 97 (6) ◽  
pp. 651-655
Author(s):  
Myoung-Jae Lee ◽  
Young-Dae Jung

The dispersion characteristics and the resonant instability mode of the space-charge wave are investigated in a streaming Lorentzian dusty plasma column by using the normal mode analysis. The result shows that the non-thermal character of the Lorentzian cylindrical dusty plasma enhances the unstable property of the space-charge wave due to the beam–plasma interaction. It is found that the resonant growth rates of the space-charge wave increase with an increase of the harmonic-order of the root of the Bessel function. It is also found that the influence of the self-gravitation enhances the resonant growth rate of the space-charge wave of the Lorentzian cylindrical dusty plasma. In addition, it is found the resonant growth rate decreases with an increase of the radius of the dusty plasma column. The variation of the resonant instability mode due to the non-thermal character and geometric effects is also discussed.


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