Dusty plasma is normal electron-ion plasma with an added highly charged element of small micron or sub-micron-sized extremely massive charged gritty (dust grains). Shukla and Silin, (1992) have theoretically shown the low-frequency dust-ion-acoustic waves in a dusty plasma system. Barkan et al. (1995) have experimentally verified the existence of dust-ion-acoustic wave in dusty plasma. These waves differ from usual ion-acoustic waves (Lonngren, 1983) due to the conservation of equilibrium charge density ne0e+nd0Zde−ni0e = 0, and the strong inequality, ne0 ≪ ni0, where ns0 is the particle number density of the species s with s = e (i) d for electrons (ions) dust, Zd is the figure of electrons residing onto the dust grain side, and e is the magnitude of an electronic charge. DIA waves linear properties are now prudent understood (Shukla and Mamun, 2002; Barkan et al., 1996; and Shukla and Rosenberg, 1999). 

The nonlinear structures related with the DIA waves are particularly solitary waves (Bharuthram and Shukla, 1992; Nakamura and Sharma, 2001); shock waves (Nakamura et al., 1999; Luo, 2000; and Mamun and Shukla, 2002), etc. These waves have also had a great deal of interest to understand the localized electrostatic perturbations in galactic space (Geortz, 1989; Fortov, 2005), and laboratory dusty plasmas (Shukla and Mamun, 2002; Nakamura and Sharma, 2001, and Barkan et al., 1996). 

Dusty plasmas create a fully modern interdisciplinary area with direct link to astrophysics, nanoscience, fluid mechanics, and material science as specified through experimental, theoretical, analytical, and arithmetical studies. All of these works (Shukla and Mamun, 2002; Bharuthram and Shukla, 1992; Nakamura and Sharma, 2001; Nakamura et al., 1999; Luo, 1995; Mamun, 2009) are limited to planar (1D) geometry and are subjected to some critical value. 

A few works have also been done on finite amplitude DIA solitons and shock structures (Luo, 1995), where K-dV or Burgers equations are used, which are not valid because, the latter gives infinitely large amplitude structures which break down the validity of the reductive perturbation method) for a parametric regime corresponding to A = 0 or A ∼ 0 (where A is the coefficient of the nonlinear term of the K-dV or Burgers equation) (Luo, 1995). 

Here, A ∼ 0 means A is not equal to 0, but A is around 0. In our present work, we have been able to show the bright and dark solitons for a large region of multi-ion dusty plasma system in an adiabatic state.

The manuscript is prepared as follows; the model equations are given in Sec. 2, the K-dV equation is derived in Sec. 3, the mK-dV equation is derived in Sec. 4, then results and discussion are given in Sec. 5, and conclusion is given in Sec. 6.

Model Equations

The dynamics of the one-dimensional multi-ion DIA waves are governed by:

where ns is the number density with s = n(i)e(d) of negative ion (positive ion) electron (stationary dust), us is the fluid speed of s, mj is the positive (when j = i) or negative (when j = n) ion mass, Z_d is the number of electron occupy on the dust grain side, e = magnitude of the electron-charge (q), ϕ is the electrostatic wave potential; n_s0, (n_j0), and nd0 are the equilibrium value of n_s, (n_j), and nd respectively i.e. n_s, (n_j), and nd are the number density normalized by n_s0, (n_j0), and n_d0 respectively, p_i is the pressure of species i, γ is an adiabatic index, x is the space variable, and t is the time variable.

K-dV Equation

For the DIA K-dV equation we introduce the stretched coordinates:

Where, Vp is the wave phase speed (ω/k), and ϵ is a smallness parameter (0 < ϵ < 1). 

To get the dispersion relation, we expand ns, us, ps, and ϕ with s be the charged species like positive and negative ion, electron in power series of ϵ, to their equilibrium and perturbed parts,

Where ns(1) , us(1) , ps(1) , and ψ(1) are the perturbed part of ns, us, ps, and ψ respectively.

Combining above equations, we get -

Where,

, and

Equation (12) represents linear dispersion relation. 

The next higher order of ϵ can be simplified as an equation of the form:

Where,

Equation (13) is known as K-dV equation. We get stationary localized solution of (13) by introducing a transformation ξ = ζ −U_0τ; 

Where the amplitude ψm and the width δ are given by respectively.

Fig 1: Bright and dark K-dV solitons.

Equation (14) is the solution of K-dV equation. This represents a solitary wave. We observed that the Fig 1 shows the existence of bright and dark K-dV solitons with mass number density (µ).

mK-dV Equation

For the third order calculation a new set of stretched coordinates is applied:

Using (15) we can find the same values of ni ⁽¹⁾, nn⁽¹⁾, ne⁽¹⁾, u i⁽¹⁾, ue⁽¹⁾, un⁽¹⁾, pi⁽¹⁾, pe⁽¹⁾, pn⁽¹⁾, and Vp as like as that in K-dV.

To the next order approximation of ϵ, we obtain a set of equations, which, after using the values ni ⁽¹⁾, nn⁽¹⁾, ne⁽¹⁾, and Vp, can be simplified and applying the condition, ψ ≠ 0 (so, its coefficient is zero), we get,

For the next higher order of ϵ, we obtain an equation: 

Where, 

Where,

and 

Equation (17) is known as mK-dV equation. The stationary localized solution of (17), obtained by introducing a transformation ξ = ζ −U_0τ, is, therefore, directly given by 

Where the amplitude ψm and the width δ are given by ψm =√6U₀/αβ, and δ = 1/ψm√γ. where the amplitude ψm and the width ∆ are given by ψm =√6U₀/αβ, ∆ = 1/(√γψm), and γ = α/6.

Fig 2: Bright mK-dV soliton.

Fig 2 gives the existence of mK-dV solitons. We get only one type of solitons, bright solitons.

Dust ion acoustic K-dV and mK-dVsolitons have been investigated in a multi-ion dusty plasma system where we observed;

1. The positive and negative K-dVsolitons are observed.
2. The width and amplitude of the K-dVsolitons varies with polaritychanges.
3. Existence of positive mK-dVsolitons is observed.

Present investigation are valid for tiny amplitude DIA K-dV, and mK-dV solitons. The first K-dV equation has been derived which gave both bright and dark solitons but for a very limited region. Though we have considered positive and negative ions, Maxwells electrons, and arbitrarily charged stationary dust, our model is applicable for small amplitude waves only.

We are so much acknowledged to Prof. Dr. Md. Kamal-Al- Hassan and Asst. Prof. Dr. Farah Deeba for their guidance to this research.

The authors declare that they have no competing interests with respect to the research.