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Dark solitons and their bound states in a nonlinear fiber with second- and fourth-order dispersion

Peng Gao1 pgao@gscaep.ac.cn    Li-Zheng Lv2    Xin Li3 1Graduate School, China Academy of Engineering Physics, Beijing 100193, China 2School of Physics, Xi’an Jiaotong University, Xi’an 710049, China 3School of Science, Beijing University of Posts and Telecommunications, Beijing 100876, China
Abstract

We study the excitations of dark solitons in a nonlinear optical fiber with the second- and fourth-order dispersion, and find the emergence of striped dark solitons (SDSs) and some multi-dark-soliton bound states. The SDSs can exhibit time-domain oscillating structures on a plane wave, and they have two types: the ones with or without the total phase step, while the multi-dark-soliton bound states exhibit different numbers of amplitude humps. By the modified linear stability analysis, we regard the SDSs as the results of the competition between periodicity and localization, and analytically give their existence condition, oscillation frequency, and propagation stability, which show good agreements with numerical results. We also provide a possible interpretation of the formation of the existing striped bright solitons (SBSs), and find that SBS will become the pure-quartic soliton when its periodicity and localization keep balance. Our results provide the theoretical support for the experimental observation of striped solitons in nonlinear fibers, and our method can also guide the discovery of striped solitons in other physical systems.

I Introduction

Periodicity and localization are two fundamental but distinct characteristics of nonlinear waves. The periodicity is a commonality of all waves and dominates various wave phenomena Hecht-book ; Cronin-2009 , while the (self-induced) localization dominates the formation of nonlinear localized waves Kivshar-book ; Onorato-2013 ; Dudley-2014 . As a widespread kind of nonlinear localized wave, soliton has been attracting lots of attentions and has wide applications by virtue of its property of stable propagation Mollenauer-1980 ; Weiner-1988 ; Agrawal-book ; Kevrekidis-book ; Haus-1996 ; McDonald-2014 . Soliton can produce periodicity-dominated phenomena like interference Snyder-1997 ; Kumar-2009 ; Zhao-2016 and diffraction Xiong-2023 ; Gao-2023 , and it also has localization-dominated phenomena like self-bound propagation and elastic collision Zabusky-1965 ; Stegeman-1999 . In the previous studies, the periodicity and localization of a soliton were always treated separately, and little attention has been paid to their combined effects. However, in nonlinear fibers with the fourth-order dispersion (FOD), the bright solitons with oscillating tails Akhmediev-1994 ; Buryak-1995 ; Blanco-2016 ; Tam-2019 and even stripe structures Zakharov-1998 ; Tam-2020 were discovered. They exhibit both of noticeable periodicity and localization, and therefore can be considered as the results of competition between the two characteristics. As we know, the modified linear stability analysis (MLSA) method has been used to predict the quantitative dynamics of nonlinear waves, including their periodicity and localization Gao-2020 ; Gao-2021 . Therefore, it provides the possibility to figure out the formation mechanism of striped solitons under the FOD and furthermore find more kinds of solitons in this system.

In this paper, we study the excitations of dark solitons in a nonlinear optical fiber with the second-order dispersion and FOD. We find that striped dark solitons (SDSs) and their bound states exist in this system, which exhibit more kinds of structures than the striped bright solitons Zakharov-1998 ; Tam-2020 and the multi-soliton bound states Buryak-1995 . The single-soliton state of SDS contains two types, i.e., the ones with or without the total phase step, while the multi-dark-soliton bound states have different numbers of amplitude humps in the time-domain distribution. By the MLSA method, a SDS is considered as the result of the competition between periodicity and localization, and furthermore we quantitatively give its existence condition and oscillation frequency. Based on the derived oscillation frequency, we analyze the modulation instability (MI) of plane-wave background of SDS and give its stability condition. Besides, we apply the MLSA to the SBSs to provide a possible interpretation of their formation, and find that the pure-quartic soliton is a special kind of SBS when its periodicity and localization keep balance.

II Model and the existence condition of striped solitons

In the slow-varying envelope approximation, the propagation of a linearly polarized light in a single-mode nonlinear fiber can be described by the following nonlinear Schrödinger equation with the second-order dispersion and FOD Agrawal-book ,

iAZβ222AT2+β4244AT4+γ|A|2A=0,\displaystyle i\frac{\partial A}{\partial Z}-\frac{\beta^{\prime}_{2}}{2}\frac{\partial^{2}A}{\partial T^{2}}+\frac{\beta^{\prime}_{4}}{24}\frac{\partial^{4}A}{\partial T^{4}}+\gamma|A|^{2}A=0, (1)

where A(T,Z)A(T,Z) represents the slowly varying complex envelope of optical field, and ZZ, TT are the evolution distance and retarded time. β2\beta^{\prime}_{2}, β4\beta^{\prime}_{4}, and γ\gamma are the coefficients of second-order dispersion, FOD, and Kerr nonlinearity, respectively. By the transformation A=P0ψA=\sqrt{P_{0}}\psi, Z=UzzZ=U_{z}z, and T=UttT=U_{t}t, the model (1) can be transformed into a dimensionless model,

iψzβ222ψt2+β4244ψt4+|ψ|2ψ=0,\displaystyle i\frac{\partial\psi}{\partial z}-\frac{\beta_{2}}{2}\frac{\partial^{2}\psi}{\partial t^{2}}+\frac{\beta_{4}}{24}\frac{\partial^{4}\psi}{\partial t^{4}}+|\psi|^{2}\psi=0, (2)

where β2=β2Uz/Ut2\beta_{2}=\beta^{\prime}_{2}U_{z}/U_{t}^{2}, β4=β4Uz/Ut4\beta_{4}=\beta^{\prime}_{4}U_{z}/U_{t}^{4}, and P0P_{0} is the background value of the incident light power. The two quantities, UzU_{z} and UtU_{t}, respectively have the units of space and time. In Ref. Runge-2020 , to generate a pure-quartic soliton in a fiber laser, the parameters were set as β2=21.4ps2/km\beta^{\prime}_{2}=21.4\,{\rm ps^{2}/km}, β4=80ps4/km\beta^{\prime}_{4}=-80\,{\rm ps^{4}/km}, γ=1.6/W/km\gamma=1.6\,{\rm/W/km}, and P0=0.37WP_{0}=0.37\,{\rm W}. When setting Uz=1/γP0=1.69kmU_{z}=1/\gamma P_{0}=1.69\,{\rm km} and Ut=6psU_{t}=6\,{\rm ps}, one can obtain the dimensionless parameters, β2=1\beta_{2}=1 and β4=0.13\beta_{4}=-0.13. In our work, the range of β2\beta_{2} and β4\beta_{4} will be extended to generate more kinds of solitons.

In the model (2), some solitons and multi-soliton states have been studied Karlsson-1994 ; Piche-1996 ; Akhmediev-1994 ; Buryak-1995 ; Blanco-2016 ; Tam-2019 ; Zakharov-1998 ; Tam-2020 , including their existence conditions, stability, and even analytical solutions. All of these solitons belong to bright solitons, which have no plane waves as their background waves. In our work, the solitons we mainly concern about are the dark solitons, which exist on the plane-wave background, and therefore are essentially different from the bright solitons. According to our analysis, the existence condition of solitons in the model (2) is shown in Fig. 1. The solitons with different structures correspond to different regions in the β2\beta_{2}-β4\beta_{4} plane. The details are as follows.

  • The horizontal line: when β4=0\beta_{4}=0, the model (2) becomes the standard nonlinear Schödinger model, where only the traditional dark (β2>0\beta_{2}>0) or bright (β2<0\beta_{2}<0) solitons can exist.

  • The region of SDS: when β4>3β22/4β\beta_{4}>{3\beta_{2}^{2}}/{4\beta}, the SDSs exist and their periodicity gets stronger with β2\beta_{2} decreasing [see Eq. (17)].

  • The region of DS: when β43β22/4β\beta_{4}\leq{3\beta_{2}^{2}}/{4\beta} and β2>0\beta_{2}>0, the traditional dark soliton exists, which has no stripe.

  • The region of SBS: when β4<3β22/2β\beta_{4}<-{3\beta_{2}^{2}}/{2\beta}, the SBSs exist and their periodicity gets stronger with β2\beta_{2} increasing [see Eq. (27)]. The solitons presented in Refs. Akhmediev-1994 ; Buryak-1995 ; Blanco-2016 ; Tam-2019 ; Zakharov-1998 ; Tam-2020 are in this region. In particular, it becomes the so-called pure-quartic soliton when β2=0\beta_{2}=0 Blanco-2016 .

  • The region of BS: when β4<3β22/2β\beta_{4}<-{3\beta_{2}^{2}}/{2\beta} and β2<0\beta_{2}<0, the traditional bright soliton exists, which has no stripe. The solitons presented in Refs. Karlsson-1994 ; Piche-1996 are in this region.

In the above conditions, β(>0)\beta(>0) denotes the propagation constant of solitons. In other regions of the β2\beta_{2}-β4\beta_{4} plane, no soliton exists. We define the quantity φ\varphi by φ=tan1(ωs/ηs)\varphi=\tan^{-1}({\omega_{s}}/{\eta_{s}}) in the range from 0 to π/2\pi/2 to describe the strength of a wave’s stripe characteristic. ωs\omega_{s} and ηs\eta_{s} are respectively the parameters determining the periodicity and localization of a wave, whose expressions can be seen in Eqs. (16) and (26) for SDS and SBS, respectively. With φ\varphi increasing, the wave’s periodicity gets stronger and the wave’s localization gets weaker. The striped solitons with different shapes can be regarded as the results of the competition between periodicity and localization in different proportions. In particular, for a pure-quartic soliton Blanco-2016 , the two parameters ωs\omega_{s} and ηs\eta_{s} are equal, which indicates that its periodicity and localization keep balance.

In the next two sections, we will separately study SDS and SBS, including their existence condition, stripe characteristic, and formation mechanism.

Refer to caption
Figure 1: (Color online) Existence condition of solitons under different second-order dispersion β2\beta_{2} and FOD β4\beta_{4}. They contain the regions of SDS (striped dark soliton), DS (the traditional dark soliton), SBS (the striped bright soliton), and BS (the traditional bright soliton). The boundary of SDS region has the expression β4=3β22/4β\beta_{4}=3\beta_{2}^{2}/4\beta, and the boundary of SBS region is β4=3β22/2β\beta_{4}=-3\beta_{2}^{2}/2\beta, where β\beta is the propagation constant of solitons. The color scale describes the strength φ\varphi of a soliton’s periodicity relative to its localization in the range from 0 to π/2\pi/2. The black dashed line denotes the case of β2=0\beta_{2}=0, where a pure-quartic soliton can exist. In all cases, the propagation constant is set as β=1\beta=1.
Refer to caption
Figure 2: (Color online) The dark solitons with (upper row) or without (lower row) the total phase step. Distributions of the wave functions ψ\psi of dark solitons (red dashed curves) and their amplitude |ψ||\psi| (blue solid curves), when the second-order dispersion β2\beta_{2} is (a) 1-1, (b) 0.8-0.8, (c) 0.3-0.3, (d) 0, and (e) 1.5. The insets are their corresponding amplitude evolution plots, where the horizontal lines are the spatial dividers between the solitons and the spontaneous oscillations induced by MI. Other parameters are set as β4=1\beta_{4}=1 and β=1\beta=1.

III SDS

III.1 Single-soliton state

At first, let us focus on the single-soliton states of SDSs and their counterparts without the total phase step. The term “the total phase step” is used to describe the phase difference of plane wave between the two sides of dark solitons, which is the key characteristic of dark solitons. It is known that the model (2) has the plane-wave solution,

ψ0=a0eiβz,\displaystyle\psi_{0}=a_{0}e^{i\beta z}, (3)

where the amplitude a0a_{0} and the propagation constant β\beta have the relationship β=a02\beta=a_{0}^{2}. In this section, we set a0=1a_{0}=1 so that β=1\beta=1. Considering that it is quite difficult to analytically solve Eq. (2), we numerically solve it by the biconjugate gradient method Press-book . This numerical method has been successfully applied to obtain dark solitons or vertices in different models of Bose-Einstein condensates Winiecki-1999 ; Edmonds-2016 . By the method, when β4=1\beta_{4}=1, we obtain the numerical solutions of dark solitons under different β2\beta_{2} and show them in Fig. 2. When β2=1\beta_{2}=-1, we find two kinds of fundamental SDSs, which has or does not have the total phase step (i.e., the key characteristic of dark solitons), and we show them at the top or bottom of Fig. 2 (a), respectively. Both of them have some stripes and oscillating tails, but their structures are different.

Later, we set their wave functions as the initial states to numerically integrate the model (2), by the split-step Fourier method Yang-book . The evolution results are shown as the insets in Fig. 2 (a). The SDS with the total phase step stably propagates for seven unit distance. At its final evolution stage, some new waves can be seen. Because the plane-wave background is unstable under the perturbation of dark solitons, these waves are generally induced by the modulation instability (MI), which will be analyzed in detail below. The similar result is also obtained for the SDS without the total phase step, which propagates stably for six unit distance.

For some larger values of β2\beta_{2}, the results are shown in Figs. 2 (b), (c), (d), and (e). With the increase of β2\beta_{2}, the SDS has less stripes but can propagate for a longer distance, especially when β2>0\beta_{2}>0. Note that the SDS without the total phase step can be regarded as two separated dark solitons when β2=1.5\beta_{2}=1.5, as shown in Fig. 2 (e). It indicates that, when the SDS does not exist, the dark soliton without the total phase step does not exist.

III.2 Analysis of existence condition and oscillation frequency

For the bright solitons in the model (2), the asymptotic analysis has been used to obtain their existence condition and oscillation characteristic Akhmediev-1994 ; Buryak-1995 ; Tam-2020 ; Zakharov-1998 . However, considering that the dark solitons have plane-wave backgrounds, the asymptotic analysis cannot be applied directly to them. As shown in Fig. 2, SDSs have the background waves, and meanwhile they have both of periodicity and localization. For such a nonlinear wave, the MLSA method can quantitatively give its dynamical characteristics and guide its generation Gao-2020 ; Gao-2021 . Thus, we will apply this method to analyze the existence condition and characteristics of fundamental SDSs. It starts with the ansatz solution of a perturbed plane wave,

ψp=ψ0(1+u),\displaystyle\psi_{p}=\psi_{0}(1+u), (4)

where the plane wave ψ0\psi_{0} has the expression (3), and uu denotes a perturbation exerted on it. Substituting Eq. (4) into the model (2) and linearizing it about uu, we can obtain

iuzβ222ut2+β4244ut4+β(u+u)=0,\displaystyle i\frac{\partial u}{\partial z}-\frac{\beta_{2}}{2}\frac{\partial^{2}u}{\partial t^{2}}+\frac{\beta_{4}}{24}\frac{\partial^{4}u}{\partial t^{4}}+\beta(u+u^{*})=0, (5)

where uu^{*} denotes the complex conjugation of uu, and we have β=a02\beta=a_{0}^{2}. If the ansatz u=eλtu=e^{\lambda t} is applied to Eq. (5) according to Refs. Akhmediev-1994 ; Tam-2020 ; Zakharov-1998 , the term uu^{*} in Eq. (5) will be neglected and the results of dark solitons will be the same as the ones of bright solitons. It will cause that the derived existence region and oscillation frequency of SDSs don’t agree with the numerical results of Figs. 2 and 3 (b).

Therefore, to take the term uu^{*} into consideration, we assume the perturbation as the linear superposition of two conjugating components,

u=Aep(t,z)+Bep(t,z),\displaystyle u=Ae^{p(t,z)}+Be^{p^{*}(t,z)}, (6)

where AA and BB are the amplitudes of the two components, and p(t,z)p(t,z) is a complex function. This ansatz is a key setting of the MLSA method. Substituting Eq. (6) into the perturbation’s model (5) and only considering the parts of ep(t,z)e^{p(t,z)}, one can obtain two linear equations of AA and BB^{*}. They can be written as the following form,

i[M+βββMβ][AB]=pz[AB],\displaystyle i\begin{bmatrix}-M+\beta&\beta\\ -\beta&M-\beta\end{bmatrix}\begin{bmatrix}A\\ B^{*}\end{bmatrix}=p_{z}\begin{bmatrix}A\\ B^{*}\end{bmatrix}, (7)

where

M=\displaystyle M= β22pttβ424pt4β48ptt2β46ptpttt\displaystyle\frac{\beta_{2}}{2}p_{tt}-\frac{\beta_{4}}{24}p_{t}^{4}-\frac{\beta_{4}}{8}p_{tt}^{2}-\frac{\beta_{4}}{6}p_{t}p_{ttt}
β424pttttpt2(β22+β44ptt).\displaystyle-\frac{\beta_{4}}{24}p_{tttt}-p_{t}^{2}(-\frac{\beta_{2}}{2}+\frac{\beta_{4}}{4}p_{tt}). (8)

In the above expressions, ptp_{t} and pzp_{z} denote the partial derivative of p(t,z)p(t,z) about tt and zz, respectively. The function pzp_{z} can be obtained by solving the eigenvalue of the left-hand matrix in Eq. (7):

pz=\displaystyle p_{z}= ±M(2βM).\displaystyle\pm\sqrt{M(2\beta-M)}. (9)

There are two modes, where the eigenvalues pzp_{z} are the opposite of each other. The mode with a positive eigenvalue is focused on here.

Now, our main aim is to find the condition that the shape of the perturbation remains unchanged in the propagating process, which is just the existence condition of SDS. We consider the function p(t,z)p(t,z) has the following form at the initial distance,

p(t,z=0)=iωt+ln[sech(ηt)],\displaystyle p(t,z=0)=i\omega t+\ln[{\rm sech}(\eta t)], (10)

where ω\omega and η\eta are the perturbation’s frequency and steepness, determining its periodicity and localization, respectively. The localized function with the sech form is set because it has the following limit value,

pt(±)=limt±pt=iωη.\displaystyle p_{t}^{(\pm)}=\lim_{t\rightarrow\pm\infty}p_{t}=i\omega\mp\eta. (11)

By this approximation, the function pt(t,z)p_{t}(t,z) can be successfully transformed into a complex constant, and therefore offers great convenience for our analysis. Moreover, this approximation can be conveniently applied to the function pzp_{z}. Considering that the cases of t±t\rightarrow\pm\infty have the same results, we take the case of tt\rightarrow-\infty as an example and can obtain

pz()=\displaystyle p_{z}^{(-)}= M()(2βM()),\displaystyle\sqrt{M^{(-)}(2\beta-M^{(-)})}, (12)

where

M()=\displaystyle M^{(-)}= (iω+η)2[β22β424(iω+η)2].\displaystyle(i\omega+\eta)^{2}[\frac{\beta_{2}}{2}-\frac{\beta_{4}}{24}(i\omega+\eta)^{2}]. (13)

It describes the propagation characteristics of the perturbation. To be specific, the perturbation’s propagation constant and growing rate relative to the plane wave are respectively

K=Im[pz()],G=Re[pz()].\displaystyle K={\rm Im}[p_{z}^{(-)}],\quad G={\rm Re}[p_{z}^{(-)}]. (14)

Then, the velocity of its localized envelope and stripes are

Ven=G/η,Vst=K/ω.\displaystyle V_{\rm en}=G/\eta,\quad V_{\rm st}=K/\omega. (15)

From the insets of Fig. 2, we know that a SDS has a zero-velocity localized envelope and some zero-velocity stripes, which indicates Ven=0V_{\rm en}=0 and Vst=0V_{\rm st}=0. In Fig. 3 (a), when β2=0.5\beta_{2}=-0.5, β4=1\beta_{4}=1, and β=1\beta=1, we show the curves of Ven=0V_{\rm en}=0 and Vst=0V_{\rm st}=0 in the ω\omega-η\eta plane. The coordinate of their intersection point (ωs,ηs)(\omega_{s},\eta_{s}) is just the oscillation frequency and steepness of SDS, and the expressions are

ωs=Re[3β2+23ββ4β4],ηs=Re[3β2+23ββ4β4].\displaystyle\omega_{s}={\rm Re}[\sqrt{\frac{-3\beta_{2}+2\sqrt{3\beta\beta_{4}}}{\beta_{4}}}],\;\eta_{s}={\rm Re}[\sqrt{\frac{3\beta_{2}+2\sqrt{3\beta\beta_{4}}}{\beta_{4}}}]. (16)

Thus, the parameters need to satisfy ωs0\omega_{s}\neq 0 and ηs0\eta_{s}\neq 0 for the existence of SDS, namely

β4>3β22/4β,\displaystyle\beta_{4}>{3\beta_{2}^{2}}/{4\beta}, (17)

as shown in Fig. 1. Besides, one can find that they have the relationship,

ωs2+ηs2=43ββ4,ωs2ηs2=6β2β4.\displaystyle\omega_{s}^{2}+\eta_{s}^{2}=\frac{4\sqrt{3\beta}}{\sqrt{\beta_{4}}},\quad\omega_{s}^{2}-\eta_{s}^{2}=-\frac{6\beta_{2}}{\beta_{4}}. (18)

The former is independent of β2\beta_{2}, and the latter is independent of β\beta. Thus, the point (ωs,ηs)(\omega_{s},\eta_{s}) always locates on a circle when β4\beta_{4} and β\beta are fixed, and it moves towards the positive axis of η\eta with β2\beta_{2} increasing, as shown in Fig. 3 (a). More interestingly, this point is just an exceptional point of the eigenvalue pzp_{z}, which is related to the non-Hermiticity of the matrix in Eq. (7). By calculating the contour integral of its argument, one can obtain that its winding number is π\pi Ding-2022 . In eigenvalue problems, an exceptional point is a singularity where the two eigenvalues coalesce and each of them undergoes the transition from a real value to a complex. With the development of non-Hermitian physics, the exceptional point plays an important role in various systems, like optics, photonics, and Bose–Einstein condensates Miri-2019 ; El-Ganainy-2018 . However, for the relationship between SDS and exceptional point, a deeper understanding needs further investigations. Next, to verify the effectiveness of our prediction, the dependence of ωs\omega_{s} on β2\beta_{2} is studied. When β4=1\beta_{4}=1 and β=1\beta=1, we numerically measure the oscillation frequency of SDSs under different values of β2\beta_{2} and show them by the red dots in Fig. 3 (b). One can see that ωs\omega_{s} gradually decreases into 0 with β2\beta_{2} increasing. To obtain them, we measure the time interval between the first and second peaks on the right side of SDS as its time period TsT_{s}, and then the oscillation frequency can be calculated by ωs=2π/Ts\omega_{s}=2\pi/T_{s}, as shown in the upper row of Fig. 2 (a). On the other hand, we also show the analytic prediction from the MLSA method by the black curve. There are good agreements between the two results.

Refer to caption
Figure 3: (Color online) (a) Phase of the propagating function pz(t,z)p_{z}(t,z) under different ω\omega and η\eta, when β2=0.5\beta_{2}=-0.5, β4=1\beta_{4}=1, and β=1\beta=1. The black solid and dashed curves denote Ven=0V_{\rm en}=0 and Vst=0V_{\rm st}=0, respectively. The white point with the coordinate (ωs,ηs)(\omega_{s},\eta_{s}) is an exceptional point of arg(pz)\arg(p_{z}) function. The yellow curve with an arrow is the trajectory of this point with β2\beta_{2} increasing. (b) Dependence of SDS’s oscillation frequency ωs\omega_{s} on β2\beta_{2}, when β4=1\beta_{4}=1. The red dots and the black curve are respectively the results from numerical evolution and the MLSA method. (c) Dependence of the gain value GG on ω\omega, when β2=1\beta_{2}=-1 (upper) or β2=0.3\beta_{2}=-0.3 (lower). The strong or weak MI is defined by whether ωs\omega_{s} locates in the MI band or not. (d) Distribution of MI (modulation instability) and MS (modulation stability) on the β2\beta_{2}-β4\beta_{4} plane. The color scale describes the value of g(ωs)g(\omega_{s}), i.e., Eq. (III.3).
Refer to caption
Figure 4: (Color online) The multi-dark-soliton bound states. The upper row is the distribution of their wave functions ψ\psi (red dashed curves) and amplitude |ψ||\psi| (blue solid curves), when β2=0\beta_{2}=0, β4=1\beta_{4}=1, and β=1\beta=1. The lower row is their corresponding amplitude evolution.

III.3 Analysis of propagation stability

Another problem worthy of consideration is the propagation stability of SDSs. From the insets of Fig. 2, one can see that some spontaneous oscillations emerge in the propagating process of SDSs. It is a widespread phenomenon in the nonlinear systems with MI, and therefore prompts us to analyze the MI in the model (2). As we know, different types of perturbations can produce different phenomena under the influence of MI. Generally speaking, a purely periodic perturbation can generate Akhmediev breathers Dudley-2014 ; Dudley-2009 ; a purely localized one can generate a rogue wave Zhao-2016-JOSAB or Kuznetsov-Ma breather Duan-2019 , and induce the spontaneous oscillations in a triangular region El-1993 ; Biondini-2016 . (The word "purely" in front of "perturbation" is used to distinguish them with a periodic-localized perturbation.) A SDS at the initial distance can be seen as a periodic-localized perturbation on a plane wave, so we need to separately consider the influence of MI on its periodic and localized components. For its periodic component, we know that the traditional growing rate gg can be obtained by the modified growing rate GG when η=0\eta=0, namely

g(ω)\displaystyle g(\omega) =|G(ω,η=0)|\displaystyle=|G(\omega,\eta=0)|
=|ωRe[(β22+β424ω2)(2β+β22ω2+β424ω4)]|.\displaystyle=\Big{|}\omega\;{\rm Re}\Big{[}\sqrt{-(\frac{\beta_{2}}{2}+\frac{\beta_{4}}{24}\omega^{2})(2\beta+\frac{\beta_{2}}{2}\omega^{2}+\frac{\beta_{4}}{24}\omega^{4}})\Big{]}\Big{|}. (19)

If the SDS’s oscillation frequency ωs\omega_{s} locates in the MI band, its periodicity will intensively impact the stability of plane wave, whose corresponding MI distribution is shown as the upper plot in Fig. 3 (c). Thus, we calculate the growing rate when ω=ωs\omega=\omega_{s} by

g(ωs)\displaystyle g(\omega_{s}) =18β43β2+2ββ4\displaystyle=\frac{1}{8\beta_{4}}\sqrt{-\sqrt{3}\beta_{2}+2\sqrt{\beta\beta_{4}}}
×3β2(9β22+68ββ4)+2ββ4(9β22+20ββ4),\displaystyle\times\sqrt{\sqrt{3}\beta_{2}(-9\beta_{2}^{2}+68\beta\beta_{4})+2\sqrt{\beta\beta_{4}}(9\beta_{2}^{2}+20\beta\beta_{4})}, (20)

to describe the MI growing rate induced by the periodicity of SDSs. Because it can produce MI phenomena faster than the localization component, we call the periodicity-induced MI "strong MI", and accordingly we call the localization-induced MI "weak MI". The typical distribution of growing rate of weak MI is shown as the lower plot in Fig. 3 (c). In Fig. 3 (d), we illustrate the phase diagram of strong MI, weak MI, and modulation stability (MS) on the β2\beta_{2}-β4\beta_{4} plane, and the growing rate of strong MI is presented by the color scale. The strong MI corresponds to the region of β2<0\beta_{2}<0 and 3β224β<β4<27β224β\frac{3\beta_{2}^{2}}{4\beta}<\beta_{4}<\frac{27\beta_{2}^{2}}{4\beta}, and the weak MI is in the region of β2<0\beta_{2}<0 and β4>27β224β\beta_{4}>\frac{27\beta_{2}^{2}}{4\beta}. When β4=1\beta_{4}=1, the strong and weak MI respectively need the conditions of 2/3<β2<2/9-2/\sqrt{3}<\beta_{2}<-2/9 and β2>2/9\beta_{2}>-2/9. It is consistent with the evolution plots in Fig. 2, where the SDS is more and more stable with β2\beta_{2} increasing.

III.4 Multi-soliton bound state

In this subsection, we focus on the multi-dark-soliton bound states. In Ref. Buryak-1995 , the bound states of several bright solitons under the FOD have been found, and their existence condition and stability were analyzed. Here, we will find the bound states of dark solitons by the biconjugate gradient method Press-book . When β2=0\beta_{2}=0, β4=1\beta_{4}=1, and β=1\beta=1, the distributions of wave functions of the multi-dark-soliton bound states are shown as the upper row in Fig. 4. There are many kinds of bound states, which have different number of amplitude humps, such as (a) two small humps, (b) six small humps, (c) two big humps, (d) six big humps, and (e) two small and two big humps. The bound states include but are not limited to these five kinds, and their counterparts without the total phase step also exist but are not shown in this paper. Next, we study their numerical evolution to test their propagation stability, which are shown as the lower row in Fig. 4. These bound states can always propagate for a long distance, and no MI phenomenon emerges.

We stress that the “dispersion waves” in Figs. 2 (a-c) are the manifestation of the MI of plane-wave backgrounds, which is induced by the unstable frequency sideband from the periodicity of dark solitons. As shown in Fig. 3 (a), the MI can be strong, weak, or absent in different cases, and therefore the dark solitons can propagate for a short or long distance under the influence of MI. Considering that they could be observed in the optical fibers with different length, our calculations about dark solitons can provide the theoretical guidance for their observations. Particularly, when β40\beta_{4}\geq 0, the dark solitons and their bound states are stable and propagate for a long distance, as shown in Figs. 2 (d,e) and 4. In addition, the traditional linear stability analysis can also be used to obtain the linear equation (5) and the classical dispersion law (19). However, they can give us only the MI condition of a perturbed plane wave, but cannot give anything about striped solitons. This is the reason why we use the MLSA method to analyze the SDSs.

Refer to caption
Figure 5: (Color online) (a) Distribution of the SBS’s wave function ψ\psi (red dashed curves) and its amplitude |ψ||\psi| (blue solid curves), when β2=0\beta_{2}=0, β4=1\beta_{4}=-1 and β=1\beta=1. (b) Same as (a) except for β2=0.75\beta_{2}=0.75. (c) In the ω\omega-η\eta plane, the characteristic parameters (ωs,ηs)(\omega_{s},\eta_{s}) is the intersection point between the curves of Ven=0V_{\rm en}=0 (black solid curve) and different β\beta value. The blue solid, purple dashed, and red solid curves denote β=1\beta=1, 3/83/8, and 1/81/8, respectively. The parameters are β2=0.5\beta_{2}=0.5 and β4=1\beta_{4}=-1. (d) Dependence of SBS’s oscillation frequency ωs\omega_{s} on β2\beta_{2}, when β4=1\beta_{4}=1 and β=1\beta=1. The red dots and the black solid curve are respectively the results of numerical solutions and the MLSA method [see Eq. (26)].

IV SBS

As we know, the bright soliton with stripe structures in the model (2) has been studied in Refs. Zakharov-1998 ; Tam-2020 , including their existence condition and oscillation frequency. Here, we will study them by the MLSA method and then provide a possible interpretation of their formation mechanism.

Firstly, by the biconjugate gradient method, we show the distribution of wave functions of SBS in Fig. 5 (a) when β2=0\beta_{2}=0, β4=1\beta_{4}=-1, where the propagation constant is β=1\beta=1. A bright soliton with oscillating tails can be seen, which is just the so-called pure-quartic soliton Blanco-2016 . Then, when we change β2\beta_{2} to 0.750.75, a bright soliton with many stripes appears in Fig. 5 (b). Unlike the SDS, the SBS has on background of plane wave. Thus, our calculation of MLSA directly starts with the perturbation,

ψp=u=Aep(t,z)+Bep(t,z),\displaystyle\psi_{p}=u=Ae^{p(t,z)}+Be^{p^{*}(t,z)}, (21)

where the function p(t,z)p(t,z) still has the form of Eq. (10) at the initial distance. Then, substituting Eq. (21) into the model (2) and considering that the perturbation has a small amplitude, one can obtain

pz=\displaystyle p_{z}= i{pt2[β22+β424(pt2+ptt)]\displaystyle i\{p_{t}^{2}[-\frac{\beta_{2}}{2}+\frac{\beta_{4}}{24}(p_{t}^{2}+p_{tt})]
+ptt(β22+β48ptt)+β46ptpttt+β424ptttt}.\displaystyle+p_{tt}(-\frac{\beta_{2}}{2}+\frac{\beta_{4}}{8}p_{tt})+\frac{\beta_{4}}{6}p_{t}p_{ttt}+\frac{\beta_{4}}{24}p_{tttt}\}. (22)

After taking the limitations of tt\rightarrow-\infty, the propagation function becomes

pz()=i(iω+η)2[β22+β424(iω+η)2].\displaystyle p_{z}^{(-)}=i(i\omega+\eta)^{2}[-\frac{\beta_{2}}{2}+\frac{\beta_{4}}{24}(i\omega+\eta)^{2}]. (23)

It indicates that the propagation constant of this wave is

β=Im[pz()]=β22(η2ω2)+β424[(η2ω2)24ω2η2].\displaystyle\beta={\rm Im}[p_{z}^{(-)}]=-\frac{\beta_{2}}{2}(\eta^{2}-\omega^{2})+\frac{\beta_{4}}{24}[(\eta^{2}-\omega^{2})^{2}-4\omega^{2}\eta^{2}]. (24)

It is worth noting that the formation mechanism of stripes in SDS and SBS is different. For SDS, the stripes originate from the interaction between a perturbation and a zero-velocity plane wave; for SBS, the stripes are caused by the interaction between two components with opposite frequencies. Thus, the velocity of stripes in SBS is not equal to Vst=K/ωV_{\rm st}=K/\omega. Nevertheless, the formation of localized envelopes is not related to the background wave, so VenV_{\rm en} can still describe the velocity of localized envelopes in SBS. Its expression is

Ven=G/η=Re[pz()]/η=ω[β2+β46(ω2η2)].\displaystyle V_{\rm en}=G/\eta={\rm Re}[p_{z}^{(-)}]/\eta=\omega[\beta_{2}+\frac{\beta_{4}}{6}(\omega^{2}-\eta^{2})]. (25)

For a certain propagation constant β\beta, by solving Ven=0V_{\rm en}=0 and Eq. (24), we can obtain that the oscillation frequency and steepness of SBS,

ωs=Re[3β2+6ββ4β4],ηs=Re[3β2+6ββ4β4].\displaystyle\omega_{s}={\rm Re}[\sqrt{\frac{3\beta_{2}+\sqrt{-6\beta\beta_{4}}}{-\beta_{4}}}],\;\eta_{s}={\rm Re}[\sqrt{\frac{-3\beta_{2}+\sqrt{-6\beta\beta_{4}}}{-\beta_{4}}}]. (26)

As shown in Fig. 5 (c), the point (ωs,ηs)(\omega_{s},\eta_{s}) is the intersection of the black curve (Ven=0V_{\rm en}=0) and the blue curve (β=1\beta=1), when β2=0.5\beta_{2}=0.5 and β4=1\beta_{4}=-1. We also depict the curves of β=3/8\beta=3/8 and β=1/8\beta=1/8: the former is the critical case where the intersection exists just right, and the latter has no intersection with the curve of Ven=0V_{\rm en}=0. It indicates that the SBS cannot exist when β<3/8\beta<3/8, and we also obtain the same result in our numerical simulations. Then, considering that ωs0\omega_{s}\neq 0 and ηs0\eta_{s}\neq 0, we can obtain that the existence condition of SBS is

β4<3β22/2β,\displaystyle\beta_{4}<-{3\beta_{2}^{2}}/{2\beta}, (27)

as shown in Fig. 1. We also show the oscillation frequency of SDS under different sets of β2\beta_{2} in Fig. 5 (d), when β4=1\beta_{4}=1 and β=1\beta=1. Our analytical prediction (26) shows a good agreement with the numerical result.

Refer to caption
Figure 6: (Color online) (a) Dependence of VenV_{\rm en} on β4\beta_{4} when ω=2.1678\omega=2.1678, η=0.4466\eta=0.4466, and β2=0.75\beta_{2}=0.75. The insets are the amplitude evolution of the initial state (28) when β4=2\beta_{4}=-2, 1-1, and 0.5-0.5. (b) Dependence of VenV_{\rm en} on ω\omega when η=0.4466\eta=0.4466, β2=0.75\beta_{2}=0.75, and β4=1\beta_{4}=-1. The insets are the amplitude evolution of the initial state (28) when ω=1\omega=1, 2.16782.1678, and 33.
Table 1: Characteristics of several nonlinear waves
   Periodicity
(ωs\omega_{s})
   Localization
(ηs\eta_{s})
Proportion (ωs/ηs\omega_{s}/\eta_{s}) Characteristic quantity (φ\varphi)
Traditional soliton No (ωs=0\omega_{s}=0) Yes (ηs>0\eta_{s}>0) 0 0
Striped soliton Yes (ωs>0\omega_{s}>0) Yes (ηs>0\eta_{s}>0) (0,+)(0,+\infty) (0,π/2)(0,{\pi}/{2})
Pure-quartic soliton Yes (ωs>0\omega_{s}>0) Yes (ηs>0\eta_{s}>0) 11 π/4{\pi}/{4}
Periodic wave Yes (ωs>0\omega_{s}>0) No (ηs=0\eta_{s}=0) ++\infty π/2{\pi}/{2}

Our derived existence condition (27) and oscillation frequency (26) of SBSs agree well with the results given by Ref. Tam-2020 . It indicates that for SBSs, the MLSA method are equivalent to the direct asymptotic analysis, due to the absence of plane-wave background. Nevertheless, besides of the above results, the MLSA method can also provide the interpretation for the formation mechanism of SBSs. It is known that the wave function (21) has two components with opposite frequencies. When both of their localized envelopes have the zero velocity, i.e., Ven=0V_{\rm en}=0, a SBS will be generated. It means that the formation of a SBS is the result of synchronous propagation of the two components. To confirm this guess, for a wave function with frequency ω\omega and steepness η\eta, we show the dependence of VenV_{\rm en} on β4\beta_{4} in Fig. 6 (a), when ω=2.1678\omega=2.1678, η=0.4466\eta=0.4466, and β2=0.75\beta_{2}=0.75. When β4=1\beta_{4}=-1, we have Ven=0V_{\rm en}=0. The initial state has the form of

ψ(t,0)=acos(ωt)sech(ηt),\displaystyle\psi(t,0)=a\cos(\omega t){\rm sech}(\eta t), (28)

where the amplitude aa is set as 0.60.6 according to the numerical solution of the SBS in this case. Its amplitude evolution plot is shown in the middle inset of Fig. 6 (a), where a SBS is generated. When β4=2\beta_{4}=-2, we have Ven<0V_{\rm en}<0. Its corresponding evolution plot is shown in the left insets of Fig. 6 (a), where the two components move towards opposite directions. Also, the similar result can be obtained in the case of β4=0.5\beta_{4}=-0.5, as shown in the right inset. It indicates that one cannot find SBS in the absence of FOD, because the velocity of localized envelopes is not zero in this case.

Similarly, we also show the dependence of VenV_{\rm en} on ω\omega in Fig. 6 (b), when η=0.4466\eta=0.4466, β2=0.75\beta_{2}=0.75, and β4=1\beta_{4}=-1. The evolution plots in the cases of ω=1\omega=1, 2.16782.1678, and 33 are shown as the insets in Fig. 6. Only in the case of ω=2.1678\omega=2.1678, the SBS can be generated. In the cases of ω2.1678\omega\neq 2.1678, the two components propagate towards opposite directions.

Finally, we summarize the characteristics of different nonlinear waves in Tab. 1. They contains the traditional solitons, the striped solitons, the pure-quartic solitons, and periodic waves. We recall that the quantity φ\varphi is defined by φ=tan1(ωs/ηs)\varphi=\tan^{-1}({\omega_{s}}/{\eta_{s}}) to describe the strength of a wave’s periodicity relative to its localization, and ωs\omega_{s} and ηs\eta_{s} are the parameters determining the periodicity and localization of a wave, respectively. A traditional soliton has the localization but no the periodicity (i.e., ωs=0\omega_{s}=0 and ηs>0\eta_{s}>0), while a periodic wave has the periodicity but no the localization (i.e., ωs>0\omega_{s}>0 and ηs=0\eta_{s}=0). A striped soliton has both of the periodicity and localization, and therefore it corresponds to ωs>0\omega_{s}>0 and ηs>0\eta_{s}>0. The pure-quartic soliton is a particular case of the striped solitons when the periodicity and localization achieve a balance, i.e., ωs=ηs\omega_{s}=\eta_{s}, so its proportion of periodicity and localization is ωs/ηs=1\omega_{s}/\eta_{s}=1 and the characteristic quantity is φ=π/4\varphi=\pi/4.

V Conclusion

In summary, the excitations of dark solitons in a nonlinear fiber with the second-order dispersion and FOD are investigated. In this system, we find the SDSs, their counterparts without the total phase step, and some multi-dark-soliton bound states. With the help of the MLSA method, we quantitatively analyze the periodicity and localization of the SDSs under different coefficients of second-order dispersion and FOD. Their oscillation frequency is successfully predicted and the corresponding MI is analyzed, which can make the propagation of SDSs unstable. For the SBSs, though their major characteristics have been studied in the previous works Zakharov-1998 ; Tam-2020 , we provide a new possible perspective to understand their formation mechanism. Our method and results can provide the theoretical guidance for the generations and manipulations of striped solitons in nonlinear fibers, and furthermore bring more possibility for their applications in soliton communications and optical measurements. Considering that stripe solitons have been also found in spinor Bose-Einstein condensates Achilleos-2013 ; Xu-2013 ; Zhao-2020 ; Yang-2021 , we expect that our method can be applied in these systems and help with the observation of matter-wave striped solitons. We also note that the competition between periodicity and localization of a soliton is similar to the well-known wave-particle duality to some extent. Understanding the similarity between them is a challenging but might be important task, which is worthy of future’s study.

Acknowledgement

The authors thank Prof. Jie Liu for his helpful discussion. This work was supported by NSAF (No.U2330401) and National Natural Science Foundation of China (No. 12247110).

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