The study of N =2 supersymmetric (SUSY) extensions of nonlinear evolution equations has been largely studied in the past [1,2,3,4,5,6,7,8] in terms of integrability conditions and solutions. Such extensions are given as a Grassmann-valued partial differential equation with one dependent variable A(x,t;θ₁,θ₂)which is assumed to be bosonic to get nontrivial extensions. The independent variables are given as a set of even (commuting) space x and time t variables and a set of odd (anticommuting) variables variables θ₁, θ₂. Since the odd variables satisfy , the dependent variable A admits the following finite Taylor expansion

where u and v are bosonic complex valued functions and ξ₁ and ξ₂ are fermionic complex valued functions. In this paper, we show that some of these extensions can be related to a linear partial differential equation (PDE) by assuming that A is a chiral superfield [9]. Proving the integrability of an equation by linearization has been largely studied in the classical case [10,11] and has found new developments in the N=1 formalism [12]. We propose a similar development in the N=2 formalism. In N=2 SUSY, we consider a pair of supercovariant derivatives defined as

which satisfy the anticommutation relations and {D₁,D₂} = 0. We consider also the complex supercovariant derivatives

which satisfy {D_±,D_±}=0 and . In terms of the complex Grassmann variables , the derivatives Equation (3) admits the following representation

and the superfield A given in Equation (1) writes

The fermionic complex valued functions ρ_± are defined as .

Chiral superfields are superfields of type Equation (5) satisfying D₊A=0. In terms of components, we get

or equivalently ξ₂ = iξ₁ and v= -iu_x.

In the subsequent sections, we produce solutions of N=2 SUSY extensions of the Korteweg–de Vries [1] (SKdV_α), modified Korteweg–de Vries [6] (SmKdV) and Burgers [5] (SB) equations from a chiral superfield point of view. In this instance, the equations, in terms of the complex covariant derivatives Equation (3), reads, respectively, as

where [X,Y]=XY - YX is the commutator. In Equation (7), α is an arbitrary parameter but we will consider only the integrable cases [1] where α = −2,1,4.

In this paper, we start by presenting a general reduction procedure of these equations using chiral superfields (Section II). We thus treat SKdV_-2 and SmKdV together and construct classical N super soliton solutions [4,7,8,13] and an infinite set of similarity solutions [7]. In Section IV, we demonstrate the existence of special N super soliton solutions, called virtual solitons [5], for the SUSY extensions of the KdV equation with α=1,4 and the Burgers equation using a related linear partial differential equation. The last section is devoted to a N=4 extension of the KdV equation [6] in an attempt to construct a general N super virtual soliton solution.

Here, we propose a general approach for the construction of chiral solutions of SUSY extensions. This approach avoids treating SUSY extensions in terms of components of the bosonic field A given in Equation (1). Assuming D₊A = 0, we get the chiral property {D₊,D_-}A = D₊D_-A = A_x and the Equations (7–9) reduce to

Note that these equations may be evidently treated as classical [14] PDE's, but remains SUSY extensions due to the Grassmannian dependence of the bosonic field A.

The absence of the Grassmannian variables θ₊ and θ_- derivatives in Equations (10–12) indicates that the odd sectors of chiral solutions should be free from fermionic constraint. This property is in accordance with the integrability of these extensions due to arbitrary bosonization of the fermionic components [15] of the bosonic superfield A.

From the classical case, we know that the methods of resolution of all these equations are similar. The same could be said for the SUSY case. Indeed, if we assume the introduction of a potential à such that A = Ã_x in Equation (10) and after one integration with respect to x, we get

where the constant of integration is set to zero. The same is done on Equation (12) and leads to

We thus observe that the Equations (11,13,14) are now on an equal footing, i.e., the order of the equation in x is equal to the number of appearance of ∂_x in the nonlinear terms. This is standard in Hirota formalism. The choice α = -2 in Equation (13) gives, up to a slight change of variable, the SmKdV Equation (11). This means that the known [7] N super soliton solutions and similarity solutions of SKdV_-2 will lead to similar types of solutions for the SmKdV Equation (11).

Now setting

in Equation (13), we obtain

The above equation reduces to the linear dispersive equation [14]

for the special and only values α=1 with β₁=i and α=4 with . For α=-2, Equation (16) writes

which does not linearize but can be bilinearized taking β_-2=i. It is discussed in the next Section.

A similar change of variable as in Equation (15) but with Ã= β_B log H_B and in Equation (14) is assumed and leads to the linear Schrödinger Equation

It is well known [13,14,15,16,17,18,19] that we can generate via the Hirota bilinear formalism N soliton and similarity solutions in the classical case and in SUSY N=1 extensions. Recently, the formalism was adapted to N=2 extensions [4,7,8] by splitting the equation into two N=1 equations, one fermionic and one bosonic. Our approach consists of treating the equation as a N=2 extension without splitting it, but imposing chirality conditions.

Equation (11) can be bilinearized using the Hirota derivative defined as

Indeed, we take à as in Equation (15) with β_-2=i and , where are bosonic chiral superfields for i=1,2. Equation (11) leads to the set of bilinear equations

This set is analogous to the corresponding bilinear equations in the classical mKdV equation [14] but we deal with superfields τ₁ and τ₂.

In order to get chiral solutions, we have to solve the set of bilinear equations with the additional chiral property D₊τ_i = 0 for i=1,2. It will lead to new solutions of the SmKdV equation which are related to our recent contribution [7].

In this section, we exhibit N super soliton solutions, called N super virtual solitons, for the three equations SKdV₁, SKdV₄ and SB. Virtual solitons are soliton-like solutions which exhibit no phase shifts in nonlinear interactions. In terms of classical N soliton solutions [3,4,5,7,14,16,19], this is equivalent to say that the interaction coefficients A_ij between soliton i and soliton j are zero, . They manifest as traveling wave solutions for negative time t«0 and decrease spontaneously at time t=0 to split into a N soliton profile which exhibit no phase shifts. It is often said that the traveling wave solution was charged with N-1 soliton, called virtual solitons [5].

Using the change of variable Equation (15) for the unknown bosonic field Ã, we have seen that the bosonic field H_α must be a chiral superfield and solve the linear dispersive Equation (17) when α=1 and α=4. For the Burgers equation, the bosonic field H_B had to be chiral and solves Equation (19).

It is easy to show that they admit the following solution

where the bosonic superfields Ψ_i are given as

The frequencies ω(κ_i) are such that ω(κ_i)= - κ_i³ for SKdV_α and ω(κ_i)=- κ_i² for SB. It looks like a typical KdV type soliton solution where all the interaction coefficients A_ij are set to zero.

We see that the virtual soliton solutions of the SKdV₁ and SKdV₄ equations are completely similar due to the form of à which differs only by the constant value of β_α. The expression of the original bosonic field is obtained from

where β=β_α for the SKdV_α equation and β=β_B for the SB equation. Thus, we can give the explicit forms of the superfield components u and ρ_-. Indeed, we have

where η_i=κ_ix+ ω(κ_i)t and the bosonic functions f_i(x,t) are defined as

In Figure 3, we may enjoy the three virtual soliton solution Im(u) of the SKdV₁ Equation for and α_i = 1 in Equation (36) and t= 0,10,20. In Figure 4, we observe the behavior of the function v where v = - iu_x, and α_i=1 in Equation (36) and t=20,0,20. For the same special values, Figure 5 gives the density plots of the bosonic functions f₁, f₂ and f₃ as given in Equation (40).

The SUSY N=4 KdV equation, as proposed by Popowicz in [6], reads

where Г is a bosonic superfield and the complex supercovariant derivatives are defined as

where for i=1,2,3,4. Using the relations {D_i,D_j}=2δ_ij∂_x, where δ_ij is the Kronecker delta, we have that the supercovariant derivatives Equation (42) satisfy the anticommutation rules

where μ,v ∈ {+,-}. Equation (41) can easily be viewed as a generalization of a N=2 equation. Indeed, setting θ₃=θ₄=0 and in Equation (41), we retrieve the SmKdV Equation (8).

To construct virtual solitons of N=2 SUSY extensions, we have considered chiral superfields. Here, we propose a generalization of this concept. Indeed, we impose the following constraints on the superfield Г

A bosonic superfield Ξ satisfying the chiral conditions Equation (44) has the following general form

where u=u(x,t) and w=w(x,t) are complex valued bosonic functions and ξ=ξ(x,t) and η=η(x,t) are complex valued fermionic functions. The Grassmann variables in Equation (45) are defined as and . Now, using the chirality conditions Equation (44), we have and Equation (41) reduces to the classical nonlinear PDE

Equation (46) is, up to a slight change of variable, similar to Equation (13) for the integrable cases α=1,4. Indeed, we retrieve Equation (13) for α=1,4by casting in Equation (46).

The above equation can be linearized into the linear dispersive Equation (17) by the change of variable

Thus to obtain solutions of Equation (41), the superfield must satisfy the constraints

A solution to this system is

where φ is a N=4 chiral bosonic superfield of the form

with and λ₁ is an even constant. This result can thus be generalized to give a N super virtual soliton solution of the SUSY N=4 KdV Equation (41) by taking

where the superfields φ_i are defined as in Equation (50) for i=1,…,N.

It is interesting to note that by setting in Equation (50), one recovers the superfields Equation (24).

In this paper, we have studied special solutions of supersymmetric extensions of the Burgers, KdV and mKdV equations in a unified way and using a chirality of the superfield A.

We have recovered interacting super soliton solutions (often called KdV type solitons) and an infinite set of rational similarity solutions. To produce such rational solutions, we have used an SUSY extension of the Yablonskii–Vorob'ev polynomials. We have introduce a new representation of the τ-functions to solve the bilinear equations. These τ-functions are N=2 extensions of classical τ-functions of the mKdV equation. Till now, in the literature, only N=1 extensions of the τ-functions were given.

We have shown the existence of non-interacting super soliton solutions, called virtual solitons, for the Burgers and SKdV_α (α=1,4). These special solutions are a direct generalization of the solutions obtained in a recent contribution [5] where N super virtual solitons have been found by setting to zero the fermionic contributions ξ₁ and ξ₂ in the bosonic superfield A given as in Equation (1). We retrieve those solutions by setting ς_i= 0 in the exponent terms Equation (37). Thus the chirality property, exposed in this paper, has produced a nontrivial fermionic sector for a N super virtual soliton. Furthermore, to obtain such solutions we have related the SUSY equations to linear PDE's showing the true origin of those special solutions.

A N=4 extension of the KdV equation has been shown to produce a N super virtual soliton solution. The study of N=4 extensions is quite new to us and we hope in the future to produce a N super soliton solution with interaction terms.