2009
DOI: 10.1063/1.3227648
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The effect of dust size distribution on quantum dust acoustic wave

Abstract: Based on the quantum hydrodynamics theory, a proposed model for quantum dust acoustic waves (QDAWs) is presented including the dust size distribution (DSD) effect. A quantum version of Zakharov–Kuznetsov equation is derived adequate for describing QDAWs. Two different DSD functions are applied. The relevance of the wave velocity, amplitude, and width to the DSD is investigated numerically. The quantum effect changes only the soliton width. A brief conclusion is presented to the current findings and their relev… Show more

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Cited by 24 publications
(15 citation statements)
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“…Before going to the discussion, it should be mentioned here that our model is focused on quantum dusty plasmas of ultradense astrophysical objects (Ali and Shukla 2006;El-Taibany and Wadati 2007;El-Labany et al 2009b), in which the mass density is of order 10 6 g/cm 3 or more, like the case of white dwarfs or neutron stars, giving rise to k m ≈ 4 × 10 6 or more. Therefore, within the following numerical investigations, we will use (Ali and Shukla 2006;El-Taibany and Wadati 2007;El-Labany et al 2009b) r min = 10 −4 cm, k = 10 −6 , k z = 10 7 , k m = 4 × 10 6 , σ e ≈ 2, σ i ≈ 0.01, Fig. 1 Variation of phase shift with R for different values of the power law index β and r m = 10 −4 , k = 10 −6 , k z = 10 7 , k m = 4 × 10 6 n e0 = 5 × 10 23 cm −3 , n i0 = 2 × 10 24 cm −3 , H e ≈ 10 −1 , H i ≈ 10 −3 , and H d ≈ 10 −8 .…”
Section: Numerical Results and Discussionmentioning
confidence: 99%
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“…Before going to the discussion, it should be mentioned here that our model is focused on quantum dusty plasmas of ultradense astrophysical objects (Ali and Shukla 2006;El-Taibany and Wadati 2007;El-Labany et al 2009b), in which the mass density is of order 10 6 g/cm 3 or more, like the case of white dwarfs or neutron stars, giving rise to k m ≈ 4 × 10 6 or more. Therefore, within the following numerical investigations, we will use (Ali and Shukla 2006;El-Taibany and Wadati 2007;El-Labany et al 2009b) r min = 10 −4 cm, k = 10 −6 , k z = 10 7 , k m = 4 × 10 6 , σ e ≈ 2, σ i ≈ 0.01, Fig. 1 Variation of phase shift with R for different values of the power law index β and r m = 10 −4 , k = 10 −6 , k z = 10 7 , k m = 4 × 10 6 n e0 = 5 × 10 23 cm −3 , n i0 = 2 × 10 24 cm −3 , H e ≈ 10 −1 , H i ≈ 10 −3 , and H d ≈ 10 −8 .…”
Section: Numerical Results and Discussionmentioning
confidence: 99%
“…Z dj 0 is the number of electrons residing on the j th dust grain surface. The QDASWs dynamics can be described by the following normalized equations (El-Labany et al 2009b):…”
Section: Basic Equations and Head-on Collision Between Two Qdaswsmentioning
confidence: 99%
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