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DIA and DA solitary waves in adiabatic dusty plasmas

Published online by Cambridge University Press:  01 June 2009

A. A. MAMUN ,
N. JAHAN  and
P. K. SHUKLA
A. A. MAMUN
Affiliation:
Department of Physics, Jahangirnagar University, Savar, Dhaka-1342, Bangladesh ([email protected])
N. JAHAN
Affiliation:
Department of Physics, Jahangirnagar University, Savar, Dhaka-1342, Bangladesh ([email protected])
P. K. SHUKLA
Affiliation:
Fakultät für Physik und Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany
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Abstract

We consider an adiabatic dusty plasma containing adiabatic inertialess electrons, adiabatic ions, and adiabatic negatively charged dust. The basic features of the dust–ion-acoustic (DIA) as well as the dust-acoustic (DA) solitary waves (SWs) in such an adiabatic dusty plasma are investigated using the reductive perturbation method, which is valid for small amplitude SWs, and by the pseudo-potential approach which is valid for arbitrary amplitude SWs. The combined effects of the adiabaticity of electrons/ions and negatively charged static/mobile dust on the basic features (polarity, speed, amplitude and width) of small as well as arbitrary amplitude DIA and DA SWs are examined explicitly. It is found that the combined effects of the adiabaticity of electrons/ions and negatively charged static/mobile dust significantly modify the basic features (polarity, speed, amplitude and width) of the DIA and DA SWs. The implications of our results in space and laboratory dusty plasmas are discussed briefly.

Type
Papers
Information
Journal of Plasma Physics , Volume 75 , Issue 3 , June 2009 , pp. 413 - 431
Copyright
Copyright © Cambridge University Press 2008

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References

[1]Goertz, C. K. 1989 Rev. Geophys. 27, 271.Google Scholar
[2]Mendis, D. A. and Rosenberg, M. 1994 Annu. Rev. Astron. Astrophys. 32, 419.CrossRefGoogle Scholar
[3]Verheest, F. 2000 Waves in Dusty Plasmas. Dordrecht: Kluwer.Google Scholar
[4]Shukla, P. K. and Mamun, A. A. 2002 Introduction to Dusty Plasma Physics. Bristol: Institute of Physics.Google Scholar
[5]Ishihara, O. 2007 J. Phys. D 40, R121.Google Scholar
[6]Selwyn, G. S. 1993 Jpn. J. Appl. Phys. 32, 3068.CrossRefGoogle Scholar
[7]Winter, J. 1998 Plasma Phys. Control. Fusion 340, 1201.Google Scholar
[8]Shukla, P. K. and Silin, V. P. 1992 Phys. Scripta 45, 508.CrossRefGoogle Scholar
[9]Barkan, A., D'Angelo, N. and Merlino, R. L. 1996 Planet. Space Sci. 44, 239.CrossRefGoogle Scholar
[10]Rao, N. N., Shukla, P. K. and Yu, M. Y. 1990 Planet. Space Sci. 38, 543.Google Scholar
[11]Barkan, A., Merlino, R. L. and D'Angelo, N. 1995 Phys. Plasmas 2, 3563.CrossRefGoogle Scholar
[12]Bharuthram, R. and Shukla, P. K. 1992 Planet. Space Sci. 40, 973.Google Scholar
[13]Nakamura, Y., Bailung, H. and Shukla, P. K. 1999 Phys. Rev. Lett. 83, 1602.Google Scholar
[14]Nakamura, Y. and Sharma, A. 2001 Phys. Plasmas 8, 3921.Google Scholar
[15]Mamun, A. A. and Shukla, P. K. 2002 Phys. Plasmas 9, 1470.Google Scholar
[16]Mamun, A. A. and Shukla, P. K. 2002 IEEE Trans. Plasma Sci. 30, 720.Google Scholar
[17]Shukla, P. K. and Mamun, A. A. 2003 New J. Phys. 5, 17.1.Google Scholar
[18]Mamun, A. A. and Shukla, P. K. 2005 Plasma Phys. Contr. Fusion 47, A1–49.Google Scholar
[19]Mamun, A. A., Shukla, P. K. and Cairns, R. A. 1996 Phys. Plasmas 3, 702.CrossRefGoogle Scholar
[20]Ma, J. X. and Liu, J. 1997 Phys. Plasmas 4, 253.Google Scholar
[21]Mamun, A. A. 1999 Astrophys. Space Sci. 268, 443.Google Scholar
[22]Mamun, A. A. and Shukla, P. K. 2001 Phys. Lett. A 290, 173.Google Scholar
[23]Mamun, A. A. and Shukla, P. K. 2002 Phys. Scripta T98, 107.Google Scholar
[24]Roychoudhury, R. and Mukkerjee, S. 1997 Phys. Plasmas 4, 2305.Google Scholar
[25]Mendoza-Briceño, C. A. et al. 2000 Planet. Space Sci. 48, 599.Google Scholar
[26]Gill, T. S., Kaur, H. and Saini, N. S. 2004 J. Plasma Phys. 70, 481.CrossRefGoogle Scholar
[27]Sayed, F. and Mamun, A. A. 2007 Phys. Plasmas 14, 014502.Google Scholar
[28]Cairns, R. A. et al. 1995 Geophys. Res. Lett. 22, 2709.Google Scholar
[29]Nishihara, K. and Tajiri, M. 1981 J. Phys. Soc. Japan 50, 4047.Google Scholar
[30]Mamun, A. A. 2008 Phys. Lett. A 372, 1490.Google Scholar
[31]Mamun, A. A. 2008 Phys. Lett. A 372, 884.CrossRefGoogle Scholar
[32]Bernstein, I. B., Greene, J. M. and Kruskal, M. D. 1957 Phys. Rev. 108, 546.CrossRefGoogle Scholar
[33]Washimi, H. and Taniuti, T. 1966 Phys. Rev. Lett. 17, 996.Google Scholar