Original Articles |
|
|
|
|
Effect of Thermionic Emission on Dust-Acoustic Solitons in a Dust-Electron Plasma |
REN Li-Wen;WANG Zheng-Xiong;LIU Yue;WANG Xiao-Gang |
State Key Laboratory of Materials Modification by Laser, Electron and Ion Beams Department of Physics, Dalian University of Technology, Dalian 116024 |
|
Cite this article: |
REN Li-Wen, WANG Zheng-Xiong, LIU Yue et al 2007 Chin. Phys. Lett. 24 767-770 |
|
|
Abstract The effects of thermionic emission on dust-acoustic solitons with a very small but finite amplitude in a dust--electron plasma are studied using the reductive perturbation technique. The self-consistent variation of dust charge is taken into account. It is shown that the thermionic emission could significantly increase the dust positive charge. The dependences of the phase velocity, amplitude, and width of such solitons on the dust temperature and the dust work function of dust material are plotted and discussed.
|
Keywords:
52.27.Lw
52.35.Fp
52.35.Sb
|
|
Received: 28 September 2006
Published: 08 February 2007
|
|
PACS: |
52.27.Lw
|
(Dusty or complex plasmas; plasma crystals)
|
|
52.35.Fp
|
(Electrostatic waves and oscillations (e.g., ion-acoustic waves))
|
|
52.35.Sb
|
(Solitons; BGK modes)
|
|
|
|
|
[1] Rao N N, Shukla P K, and Yu M Y 1990 Planet. Space Sci. 38 543 [2] Barkan A, Merlino R L and Angelo N D 1995 Phys. Plasmas 2 3563 [3] Luo Q Z, Angelo N D and Merlino R L 1999 Phys. Plasmas 6 3455 [4] Nakamura Y, Bailung H and Shukla P K 1999 Phys. Rev. Lett. 83 1602 [5] Thomas H, Morfill G and Tsytovich V N 2003 Plasma Phys. Rep. 29 895 [6] Popel S I, Yu M Y and Tsytovich V N 1966 Phys. Plasmas 3 4313 [7] Vladimirov S V and Nambu M 1995 Phys. Rev. E 52 R2172. [8] Fortov V E, Petrov O F, Molotkov V I, Poustylnik M Y, Torchinsky VM, Khrapak A G and Chernyshev A V 2004 Phys. Rev. E 69 016402 [9] Samsonov D, Zhdanov S K, Quinn R A, Popel S I and Morfill G E 2004 Phys. Rev. Lett. 92 255004 [10] Singh S and Dahiya R P 1990 Phys. Fluids B 2 901 [11] Bai D X, Wang Z X and Wang X G 2004 Chin. Phys. Lett. 21 125 [12] Verheest F, Cattaert T and Hellberg M A 2005 Phys. Plasmas 12 082308 [13] Bharuthram R and Shukla P K 1992 Planet. Space Sci. 40973 [14] Chen Y H and Yu M Y 1994 Phys. Plasmas 1 1868 [15] Ma J and Liu J 1997 Phys. Plasmas 4 253 [16] Ivlev A and Morfill G 2001 Phys. Rev. E 63 026412 [17] Popel S I, Golub A P, Losseva T V, Ivlev A V, Khrapak S A andMorfill G 2003 Phys. Rev. E 67 056402 [18] Mahmood S and Saleem H 2003 Phys. Plasmas 10 47 [19] Xie B S, He K and Huang Z Q 1998 Phys. Lett. A 247 403 [20] Ghosh S, Sarkar S, Khan M and Gupta M R 2000 Phys. Plasmas 7 3594 [21] Xue J K 2004 Phys. Lett. A 330 390 [22] Duan W S 2001 Phys. Plasmas 8 3583 [23] Ghosh S 2005 Phys. Plasmas 12 094504 [24] Rosenberg M, Mendis D A and Sheehan D P 1999 IEEE Trans.Plasma Sci. 24 239 [25] Rosenberg M and Shukla P K 2001 IEEE Trans. PlasmasSci. 29 202 [26] Wu H C and Xie B S 2005 Phys. Plasmas 12 064503 [27] Delzanno G L, Lapenta G and Rosenberg M 2004 Phys. Rev.Lett. 92 035002 [28] Shukla P K 2001 Phys. Plasmas 8 1791 [29] Whipple E C 1981 Rep. Prog. Phys. 44 1198 [30] Ostrikov K N, Yu M Y and Stenflo L 2000 Phys. Rev. E 61 782 [31] Allen J E 2000 Phys. Rev. E 61 7249 [32] Havnes O, Tr\o im J, Blix T et al 1996 J. Geophys. Res. 101 10839 [33] Tsytovich V N, Nefedov A P, Fortov V E, Petrov O F and Morfill G E2003 Phys. Plasmas 10 2633 [34] Wang Z X, Liu Y, Liu J Y and Wang X G 2005 Phys. Plasmas 12 014505 [35] Vaulina O S, Nefedov A P, Petrov O F, and Fortov V E 2002 Phys. Rev. Lett. 88 035001 [36] Sorasio G, Mendis D A and Rosenberg M 2001 Planet. SpaceSci. 49 1257 [37] Sodha M and Guha S 1971 Adv. Plasma Phys. 4 219 [38] Shukla P K and Mamun A 2002 Introduction to Dusty PlasmaPhysics (London: IOPP) [39] Washimi H and Taniuti T 1966 Phys. Rev. Lett. 17 996 |
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|