Quadrupolar matter-wave soliton in two-dimensional free space

Jia-Sheng Huang , Xun-Da Jiang , Huai-Yu Chen , Zhi-Wei Fan , Wei Pang , Yong-Yao Li

Front. Phys. ›› 2015, Vol. 10 ›› Issue (4) : 100507

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Front. Phys. ›› 2015, Vol. 10 ›› Issue (4) :100507 DOI: 10.1007/s11467-015-0501-1
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Quadrupolar matter-wave soliton in two-dimensional free space
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Abstract

We study two-dimensional (2D) matter-wave solitons in the mean-field models formed by electric quadrupole particles with long-range quadrupole–quadrupole interaction (QQI) in 2D free space. The existence of 2D matter-wave solitons in the free space was predicted using the 2D Gross–Pitaevskii Equation (GPE). We find that the QQI solitons have a higher mass (smaller size and higher intensity) and stronger anisotropy than the dipole–dipole interaction (DDI) solitons under the same environmental parameters. Anisotropic soliton–soliton interaction between two identical QQI solitons in 2D free space is studied. Moreover, stable anisotropic dipole solitons are observed, to our knowledge, for the first time in 2D free space under anisotropic nonlocal cubic nonlinearity.

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Keywords

2D matter-wave solitons / quadrupole–quadrupole interaction / anisotropy soliton–soliton interaction / dipole solitons

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Jia-Sheng Huang, Xun-Da Jiang, Huai-Yu Chen, Zhi-Wei Fan, Wei Pang, Yong-Yao Li. Quadrupolar matter-wave soliton in two-dimensional free space. Front. Phys., 2015, 10 (4) : 100507 DOI:10.1007/s11467-015-0501-1

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1 Introduction

The Bose–Einstein condensate (BEC), which is a macroscopic quantum state of matter, was theoretically predicted by Bose and Einstein 90 years ago [1]. In the past few decades, scientists have performed much theoretical and experimental research in the field of BECs after a BEC was first observed in dilute alkali gases. Rich phenomena have been revealed in the studies of BEC, such as solitons [2, 3], vortex formation [4, 5], Josephson oscillation [6, 7], chaos [8], and symmetry breaking [9–12]. The matter-wave soliton was also experimentally observed in ultra-cold atom gases [13, 14], and with the development of Feshbach resonance [15–17], it plays a crucial role in the research on solitons [18–21].

As is well known, stable two-dimensional (2D) matter-wave solitons are more significant than one-dimensional (1D) solitons in terms of both theoretical interest and potential for applications, which makes them crucial in the study of matter-wave solitons. It is also well known that cubic nonlinearity is the most common type of nonlinearity in nature, and the modulation instability in such nonlinearity leads to the collapse of solitons in 2D free space [22]. There are two methods to overcome this instability and obtain a stable 2D soliton in the cubic nonlinear material. The first involves the introduction of a periodical potential through structures such as 2D waveguide arrays or optical lattices [23, 24]. The periodical potential introduces new features, such as lattice solitons [26–28], lattice gap solitons [29], and lattice vortex solitons [30, 24, 31]. However, it also breaks the translation symmetry and rotational symmetry of the system, limiting the mobility of the solitons. The other method involves introducing long-range interactions. For example, isotropic long-range Van der Waals interactions between Rydberg atoms in ultra-cold boson gases [33, 34], anisotropic long-range dipole–dipole interactions (DDI) in dipolar condensates [35–40], etc. Introducing long-range interaction can not only stabilize 2D matter-wave solitons but also enhance the mobility and soliton–soliton interactions for solitons in free space.

Recently, we studied matter-wave solitons supported by anisotropic long-range quadrupole–quadrupole interaction (QQI) inter-site interactions in quadrupolar condensates [43]. In that work, we built stable 2D matter-wave solitons maintained by long-range QQI in a deep 2D optical lattice. However, realizing stable solitons with QQI in 2D free space is more challenging. In the present study, we propose a model to produce stable solitons in 2D free space and systematically study their interactions. Moreover, under the actions of QQI, stable 2D dipole solitons are observed. To our knowledge, in the background of anisotropic nonlocal nonlinearity, such solitons have not been reported in the literature.

The objective of this work is to study the shapes and interactions of 2D matter-wave solitons in BECs formed by quadrupole particles in 2D free space. The model describing this system is derived in Section 2. Numerical results of fundamental solitons and their interactions as well as dipolar solitons and their properties are systematically studied in Section 3. The paper is concluded in Section 4.

2 The model

2.1 The system induced by QQI

Two types of quadrupoles exist: electric quadrupoles and magnetic quadrupoles. Because magnetic quadrupolar BECs have been proved unsuitable to support 2D bright solitons in free space [43], we only consider electric quadrupolar BECs in this work. The electric quadrupoles are built as tightly bound pairs of dipoles and anti-dipoles, which are directed perpendicular to the systems’ plane (x,y), i.e., along the z axis. Its strength is a linearly growing function of x. Such an external electric field can be stimulated by a tapered capacitor, as shown in Fig. 1. These electric quadrupoles can be described by a symmetric traceless tensor Qα⁢β(α,β=x,y,z) with Σα⁢Qα⁢α≡0 [44]; therefore, in the setting of Fig. 1, they have the following components in this notation:

(1)Qx⁢y=Qy⁢x≡Q;Qz⁢z=Qz⁢x=Qx⁢z=Qy⁢z=0,

where the quadrupole moment is defined as

(2)Q=3⁢d⁢ε,

±d are the dipolar moments of the bound dipoles and anti-dipoles, and ε is the distance between them.

Between two quadrupoles in the planar configuration considered here, the potential of the interaction can be derived from the general formula for the QQI potential as

(3)UQ⁢Q(e⁢l⁢e⁢c⁢t⁢r)⁢(r,θ)=43⁢Q2⁢r−5⁢(1−5⁢cos2⁡θ),

where r is the distance between the quadrupoles while θ is the angle between the vector connecting the quadrupoles and the line connecting the dipole and anti-dipole inside the quadrupole.

The mean-field dynamics of solitons in this setting is described by the underlying 2D Gross–Pitaevskii Equation (GPE) [42]:

(4)i⁢∂ψ∂t=−12⁢(∂2∂x2+∂2∂y2)⁢ψ+g⁢|ψ|2⁢ψ+κ⁢ψ⁢(r)⁢∫dr′⁢K⁢(r−r′)⁢|ψ⁢(r′)|2,

where r≡{x,y} is the position of the quadrupole, g is the local nonlinear parameter of the system (g<0 indicates contact self-attraction while g>0 indicates contact self-repulsion), and κ is the strength of nonlocal nonlinearity. In this work, κ is fixed as κ≡1. The kernel in the integral term, which provides the QQI interaction between the particles, is defined as

(5)KQ⁢Q⁢(r−r′)=1−5⁢cos2⁡θ[b2+(r−r′)2]5/2,

where b, which is fixed to 0.2 in the following discussion, is the regularization scale provided by the thickness of the confined layer in the z direction. If we replace this kernel by

(6)KD⁢D⁢(r−r′)=1−3⁢cos2⁡θ[b2+(r−r′)2]3/2,

Equation (4) can be applied to describe the mean-field dynamics of 2D dipolar matter-wave solitons [38, 39].

We assume the solitons have the form

(7)ψ⁢(r,t)=ϕ⁢(r)⁢e−i⁢μ⁢t,

where ϕ⁢(r) is the stationary form of the soliton solution and μ is its chemical potential. The total norm is defined by

(8)N=∫|ϕ⁢(r)|2⁢dr.

In the following sections, the solitons are numerically studied. For the stationary solution, the numerical method we use is imaginary-time propagation (ITP) [47–49], while for the dynamical real-time evolution, the numerical method we use is the split-step Fourier transformation [50]. In order to study the formation of solitons solely from the anisotropic nonlocal nonlinearity, we fix the local nonlinear parameter g≡0 in this paper. This treatment can be physically achieved via Feshbach resonance [15–17].

3 Numerical results

3.1 Anisotropic fundamental soliton

Figure 2 shows typical examples of stable fundamental matter-wave solitons maintained by QQI and DDI based on Eq. (4) with kernels (5) and (6), respectively. Their total norm is N=1.5. This figure shows that the QQI solitons feature stronger anisotropy and their occupied area is far smaller than that of the DDI solitons, which makes their intensity higher than that of the DDI solitons.

To quantify the solitons between the DDI and QQI further, we define their effective area Aeff and structural anisotropy η between the horizontal (“Aeffx”) and vertical (“Aeffy”) directions as follows:

(9)Aeff=(∬⁢|ψ|2⁢d⁢x⁢d⁢y)2∬⁢|ψ|4⁢d⁢x⁢d⁢y,

(10)η=|Aeffx−Aeffy|Aeffx+Aeffy,

where

(11)Aeffx=[∫|ψ⁢(x,0)|2⁢dx]2∫|ψ⁢(x,0)|4⁢dx,Aeffy=[∫|ψ⁢(0,y)|2⁢dy]2∫|ψ⁢(0,y)|4⁢dy.

Figure 3 shows a comparison of these two characters [Eqs. (9) and (10)] as well as μ versus N for two types of solitons. In Figs. 3(a) and (b), the area and degree of anisotropy (i.e., Aeff and η) of both types of solitons decreases and increases, respectively, with increasing N; however, the area of the QQI solitons is two orders smaller than that of the DDI solitons for the same magnitude of N, and the degree of anisotropy of the QQI solitons is approximately twice that of the DDI solitons for the same N. In Fig. 3(c), both solitons satisfy d⁢μ/d⁢N<0, i.e., the Vakhitov–Kolokolov criterion, which is a well-known necessary stable condition for modes supported by attractive nonlinearities [45, 46]. For the magnitude of μ, the QQI solitons are more than two orders smaller than the DDI solitons for the same N.

These phenomena can be explained by the difference between the two kernels in Eqs. (5) and (6). The denominators of these two kernels are ∼1/r5 and ∼1/r3, respectively. Therefore, QQI features more compactly nonlocal effect than DDI, causing the QQI solitons to be heavier (smaller size and higher intensity) than the DDI solitons. Moreover, in the numerators of both kernels, the coefficient before cos2⁡θ for QQI is 5, while that for DDI is 3, causing the QQI solitons to have an anisotropy that is approximately twice that of the DDI solitons. Furthermore, the threshold for forming a soliton in the QQI case is smaller than that in the DDI case, and the QQI case has a wider stability area than the DDI case.

3.2 Anisotropic soliton–soliton interaction

In this subsection, we study for the anisotropic interaction between the QQI solitons through the real-time evolution of Eq. (4) from an initial condition, which is constructed by two identical solitons placed at a pair of zero-point symmetric positions defined by

(12)ψ⁢(r,t=0)=ϕ⁢(x+x0,y+y0)+ϕ⁢(x−x0,y−y0).

According to kernel (5), when the angle θ satisfies 1−5⁢cos2⁡θ=0 (i.e., θ≈63.44∘ or 116.56°), the QQI is zero; therefore, these two typical angles form the borders between the repulsive and attractive QQI. Figure 4 shows the interaction map of the zero-symmetric soliton pair starting from (12) in the x0–y0 plane. Because the QQI interaction is a long-range interaction, the two solitons automatically interact with each other when placed inside the plane. Generally, there are two types of interactions between the solitons: attraction and repulsion. The soliton will set into mobility through these two types of interactions without any kicks acting on them. As shown in Fig. 4, if the center of the solitons were initially placed in the yellow areas, the interaction between them is attractive; the two solitons move toward each other and eventually merge into a single one. Typical examples of such dynamics are displayed in Figs. 5(a1)–(a3). In contrast, in the blue areas, the two solitons are repelled away from each other because of repulsive interaction; typical examples of such dynamics are displayed in Figs. 5(b1)–(b3). If the center of the solitons is initially placed in the white (blank) area, the soliton pair shows no obvious interaction within t=100×Aeffx2, which implies that the distance between them is sufficiently high for the interactions between them to be negligible.

The red dashed lines in Fig. 4 are the theoretical boundaries of attractive and repulsive interaction, along which the interaction of QQI is equal to zero. As predicted by kernel (5), the borders between blue and yellow areas approximately coincide with the red dashed lines. An interesting phenomenon is that the soliton pair features attraction in the area of 63.44∘<θ<116.56∘ when −0.094<y0<0.094. Typical examples of such dynamics are displayed in Figs. 5(c1)–(c3). In this case, the attraction results from the thin and long profile of the soliton along the horizontal direction. When the two solitons are placed sufficiently close (i.e., |y0|<0.094), such attraction overcomes the repulsion. However, this attraction decays more quickly than the repulsion when the distance between the soliton pair is increased, causing the soliton pair to have repulsive interaction after |y0|>0.094. Another interesting phenomenon is that the soliton pair rotates before merging or bouncing away, when the solitons are launched close to the two dashed lines. Because the solitons have a finite size, some part of the soliton crosses the border and extends to the other side, resulting in the combined action of repulsion and attraction between the soliton pair. Such combined action creates a torque between the solitons, resulting in the rotational motion between them. Figures 6 and 7 show typical examples of such dynamics. In Fig. 6, two solitons are rotating with mutual attraction when the center of the solitons is arranged diagonally in the yellow region close to the dashed line. In Fig. 7, two solitons are rotating with mutually repulsion when the center of the solitons is arranged diagonally in the blue region close to the dashed line.

3.3 Anisotropic dipole soliton

Dipole matter-wave solitons are also observed in this model. It is found that the dipole soliton is stable when N>0.18. A typical example of such solitons is displayed in Fig. 8. Figure 8(d1) demonstrates that the width of this type of solitons decreases with increasing N. Figure 8(d2) shows that the μ–N relation of this kind of solitons satisfies d⁢μ/d⁢N<0, the Vakhitov–Kolokolov criterion.

When N<0.18, the dipole soliton decays to a moving fundamental soliton. A typical example of this process is shown in Fig. 9. In this process, the intensity distribution of the soliton becomes asymmetric with one part absorbing into another part [See Figs. 9(a) and (b)], and then it finally becomes a moving fundamental soliton [See Fig. 9(c)]. This phenomenon can be explained as follows: unlike the fundamental solitons, dipole solitons are in an excited state, and their formation requires stronger nonlinearity. If the nonlinearity is not sufficient, the dipole soliton decays to a fundamental one, which does not require as much nonlinearity [51]. To our knowledge, in 2D free space, this is the first observation of such solitons under anisotropic nonlocal cubic nonlinearity.

4 Conclusion

We studied two-dimensional matter-wave solitons formed by electric quadrupole particles in mean-field models with long-range quadrupole–quadrupole interaction between particles in 2D free space. The quadrupoles have two straightforward settings: electric quadrupole and magnetic quadrupole. This work was based on electric quadrupolar particles. We applied the 2D Gross–Pitaevskii Equation with the long-range QQI term under the mean-field approximation to describe the dynamics of the solitons. Shapes, stability, and anisotropy of the fundamental and dipolar matter-wave solitons were investigated in 2D free space. The anisotropic soliton–soliton interaction between the fundamental solitons was systematically studied, and the distribution map of soliton–soliton interaction was plotted. Through a comparison between the QQI and DDI cases, we found that the QQI solitons have a higher mass (smaller size and higher intensity) and stronger anisotropy than the DDI solitons under the same environmental parameters. Moreover, a stable anisotropic dipole soliton is observed for the first time in 2D free space under anisotropic nonlocal cubic nonlinearity.

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