摘要The quantum hydrodynamic model is employed to investigate the effects of gravitational potential on multi-component dusty plasmas. The effects of Fermi temperature ratios of ions to electrons (TFi/TFe) and positrons to electrons (TFp/TFe) have been calculated and presented graphically. It is observed that an increase in the Fermi temperature ratios of ions to electrons and positrons to electrons stabilizes the Jeans instability as the mode phase speed increases with these ratios. In the absence of the statistical effects due to Fermi pressure, the dispersion is weak. The stability criteria are calculated for each case separately.
Abstract:The quantum hydrodynamic model is employed to investigate the effects of gravitational potential on multi-component dusty plasmas. The effects of Fermi temperature ratios of ions to electrons (TFi/TFe) and positrons to electrons (TFp/TFe) have been calculated and presented graphically. It is observed that an increase in the Fermi temperature ratios of ions to electrons and positrons to electrons stabilizes the Jeans instability as the mode phase speed increases with these ratios. In the absence of the statistical effects due to Fermi pressure, the dispersion is weak. The stability criteria are calculated for each case separately.
S. Ali Shan;**;A. Mushtaq
. Role of Jeans Instability in Multi-Component Quantum Plasmas in the Presence of Fermi Pressure[J]. 中国物理快报, 2011, 28(7): 75204-075204.
S. Ali Shan, **, A. Mushtaq
. Role of Jeans Instability in Multi-Component Quantum Plasmas in the Presence of Fermi Pressure. Chin. Phys. Lett., 2011, 28(7): 75204-075204.
[1] Ali S and Shukla P K 2007 Eur. Phys. J. D 41 319
[2] Shukla P K and Mamun A A 2002 Introduction to Dusty Plasma Physics (Bristol: Institute of Physics)
[3] Haas F, Manfredi G and Feix M R 2000 Phys. Rev. E 62 2763
[4] Shukla P K and Ali S 2005 Phys. Plasmas 12 114502
[5] El-Taibanya W F and Miki Wadatib 2007 Phys. Plasmas 14 042302
[6] Bingham R and Tsytovich V N 2001 Astron. Astrophys. 376 43
[7] Shukla P K and Stenflo L 2006 Phys. Lett. A 355 378
[8] Masood W, Salimullah M and Shah H A 2008 Phys. Lett. A 372 6757
[9] Mushtaq A 2007 Phys. Plasmas 14 113701
[10] Pandey B P, Avinash K and Dwivedi C B 1994 Phys. Rev. E 49 5599
[11] Kolb E W and Turner M S 1990 The Early Universe (Reading MA: Addison-Wesley) p 342
[12] Landau L D and Lifshitz E M 1980 Statistical Physics (Oxford: Butterworth-Heinemann) part 1
[13] Haas F, Garcia L G, Goedert J and Manfredi G 2003 Phys. Plasmas 10 3858
[14] Shukla N, Shukla P K, Brodin G and Stenflo L 2008 Phys. Plasmas 15 044503
[15] Ali S and Shukla P K 2006 Phys. Plasmas 13 022313
[16] Tajima T and Shibata K 1997 Plasma Astrophysics (New York: Addison Wesley)
[17] Ditmire T, Tisch J W G and Springate E et al 1997 Nature 386 54
Ditmire T, Tisch J W G and Springate E et al 1997 Phys. Rev. Lett. 78 2732
[18] Liu C S and Tripathi V K 2003 Phys. Plasmas 10 4085
[19] Mourou G A, Barty C P J and Perry M D 1998 Phys. Today 51 22