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On the discrete Kuznetsov–Ma solutions for the defocusing Ablowitz-Ladik equation with large background amplitude

E. C. Boadi1, E. G. Charalampidis2,3, P. G. Kevrekidis4, N. J. Ossi1, B. Prinari1
(1 Department of Mathematics, State University of New York, Buffalo, NY 14260
2 Department of Mathematics and Statistics, San Diego State University, San Diego, CA 92182
3 Computational Science Research Center, San Diego State University, San Diego, CA 92182
4 Department of Mathematics and Statistics, University of Massachusetts, Amherst, MA 01003)
Abstract

The focus of this work is on a class of solutions of the defocusing Ablowitz-Ladik lattice on an arbitrarily large background which are discrete analogs of the Kuznetsov-Ma (KM) breathers of the focusing nonlinear Schrödinger equation. One such solution was obtained in 2019 as a byproduct of the Inverse Scattering Transform, and it was observed that the solution could be regular for certain choices of the soliton parameters, but its regularity was not analyzed in detail. This work provides a systematic investigation of the conditions on the background and on the spectral parameters that guarantee the KM solution to be non-singular on the lattice for all times. Furthermore, a novel KM-type breather solution is presented which is also regular on the lattice under the same conditions. We also employ Darboux transformations to obtain a multi-KM breather solution, and show that parameters choices exist for which a double KM breather solution is regular on the lattice. We analyze the features of these solutions, including their frequency which, when tending to 0, renders them proximal to rogue waveforms. Finally, numerical results on the stability and spatio-temporal dynamics of the single KM breathers are presented, showcasing the potential destabilization of the obtained states due to the modulational instability of their background.

1 Introduction

The Ablowitz-Ladik (AL) model:

idqndt=1h2(qn+12qn+qn1)σ|qn|2(qn+1+qn1),σ=±1,n,ti\frac{dq_{n}}{dt}=\frac{1}{h^{2}}(q_{n+1}-2q_{n}+q_{n-1})-\sigma|q_{n}|^{2}(q_{n+1}+q_{n-1}),\quad\sigma=\pm 1,\quad n\in\mathbb{Z},t\in\mathbb{R} (1)

was introduced in [2, 3] as an integrable spatial discretization of the focusing (σ=1\sigma=-1) and defocusing (σ=1\sigma=1) nonlinear Schrödinger (NLS) equation:

iqt=qxx2σ|q|2q,iq_{t}=q_{xx}-2\sigma|q|^{2}q,

to which they reduce as the lattice spacing h0h\to 0 with nhxnh\to x.

Besides being used as numerical schemes for their continuous counterparts, the AL equations describe the quantum correlation function of the XYXY-model of spins [21, 24]. When σ=1\sigma=-1, the equation plays a significant role in the study of anharmonic lattices [35] and lossless nonlinear electric lattices [27], and it is gauge equivalent to an integrable discretization of the Heisenberg spin chain [20]. Additionally, the focusing AL hierarchy describes the integrable motions of a discrete curve on the sphere [17]. Importantly, in addition to its intrinsic value, the AL model provides a springboard towards exploring solutions in the non-integrable, yet more widespread discrete variant of the nonlinear Schrödinger model, namely the so called discrete NLS equation [22]. Indeed, this has been leveraged for solitary wave dynamics in early works, such as, e.g., [11], but also for more complex structures including periodic and rogue waves, e.g., in the more recent work of [33]. This justifies a multi-faceted interest in the periodic (and rogue) wave solutions of the Ablowitz-Ladik model [5], from a theoretical point of view in their own right, but also from a computational and applications point of view, as well.

In this work we are interested in characterizing special solutions of the defocusing AL equation on a nontrivial background. Specifically, we will consider the equation:

idQndτ=Qn+1+Qn1+2r2Qn|Qn|2(Qn+1+Qn1),r2=Qo21>0i\frac{dQ_{n}}{d\tau}=Q_{n+1}+Q_{n-1}+2r^{2}Q_{n}-|Q_{n}|^{2}(Q_{n+1}+Q_{n-1}),\qquad r^{2}=Q_{o}^{2}-1>0 (2)

with boundary conditions:

limn±Qn(τ)=Q±Qoeiθ±Qo>1,θ±.\lim_{n\to\pm\infty}Q_{n}(\tau)=Q_{\pm}\equiv Q_{o}e^{i\theta_{\pm}}\qquad Q_{o}>1,\theta_{\pm}\in\mathbb{R}. (3)

Modulo a rescaling of dependent and independent variables (Qn=hqnQ_{n}=hq_{n} and τ=t/h2\tau=t/h^{-2}), the above equation is gauge-equivalent to Eq. (1) (the gauge transformation QnQn=e2iQo2τQ_{n}\to Q_{n}=e^{-2iQ_{o}^{2}\tau} has simply the effect of allowing for constant boundary conditions as n±n\to\pm\infty).

As mentioned above, the AL equations are integrable, and their initial-value problem can be solved by means of the Inverse Scattering Transform (IST). The IST for Eq. (2) was initially developed under the assumption that the background amplitude QoQ_{o} satisfies a “small norm” condition, 0<Qo<10<Q_{o}<1 [36, 14, 1]. This condition is actually not just a technical assumption: in [28] it was shown that the defocusing AL equation, which is modulationally stable for 0Qo<10\leq Q_{o}<1, becomes unstable if Qo>1Q_{o}>1, and exhibits discrete rogue wave solutions, some of which are regular for all times. This finding sparked renewed interest in the defocusing AL equation on a background. In [29] the IST was generalized to the case of arbitrarily large background Qo>1Q_{o}>1. As a by-product of the IST, explicit solutions were also obtained in [29], which are the discrete analog of the celebrated Kuznetsov–Ma [23, 26], Akhmediev [7, 8], Tajiri-Watanabe [34] and Peregrine solutions [30, 6, 5], and which mimic the corresponding solutions for the focusing AL equation [9, 10, 32, 31].

The recent work [15] further investigated the stability of background solutions of the AL equations in the periodic setting, confirming in particular that, unlike its continuous counterpart, in the defocusing case (ALAL_{-}, in the terminology of [15]) the background solution is unstable under a monochromatic perturbation of any wave number if the amplitude of the background is greater than 1. A discrete Kuznetsov-Ma (KM) breather solution was presented in [29], and it was observed that the solution could be regular for certain choices of the soliton parameters, but its regularity was not analyzed in detail.

The goal of the present work is to provide a systematic investigation of the conditions on the background and on the spectral parameters (discrete eigenvalue and associated norming constant) that guarantee the KM solution to be non-singular for all nn\in\mathbb{Z} and all τ\tau\in\mathbb{R}. Furthermore, a novel KM-type breather solution will be presented which is also regular on the lattice under the same conditions. We also employ the Darboux transformations derived in [15] to analyze Akhmediev breathers, and, by generalizing the construction to the case of KM breathers, we obtain multi-KM breather solutions. In particular, we show that parameters choices exist for which a double KM breather is regular on the lattice. Finally, we corroborate the analytical findings by numerical computations where for the obtained exact solutions, a spectral stability analysis is performed and dynamical evolution of the lattice model with such waveforms as initial data is explored. The latter will often lead to unbounded growth of the solution due to the manifestation of the modulational instability of its background.

Our presentation is structured as follows. First, we provide some relevant background of the model, including its Lax pair and associated discrete spectrum. We then move to the construction of the KM breathers, followed by an analysis of the conditions under which the relevant waveforms are regular. We then proceed to provide a construction of the solutions via Darboux transformations, before exploring the stability and direct numerical dynamics of the associated waveforms. We close with a discussion of the conclusions of our findings and some directions for future research.

2 Lax pair and discrete spectrum

The Lax pair for the AL system (2) is given by [2]:

vn+1=𝐋nvn,dvndτ=𝐌nvn,\displaystyle v_{n+1}=\mathbf{L}_{n}v_{n}\,,\qquad\frac{dv_{n}}{d\tau}=\mathbf{M}_{n}v_{n}\,, (4a)
𝐋n=𝐙+𝐐n,𝐙=(z001/z),𝐐n=(0QnQn0),\displaystyle\mathbf{L}_{n}=\mathbf{Z}+\mathbf{Q}_{n}\,,\qquad\mathbf{Z}=\left(\begin{array}[]{cc}z&0\\ 0&1/z\end{array}\right)\,,\qquad\mathbf{Q}_{n}=\left(\begin{array}[]{cc}0&Q_{n}\\ Q_{n}^{*}&0\end{array}\right)\,, (4f)
𝐌n=iσ3[𝐐n𝐐n1Qo2𝐈12(z1/z)2𝐈𝐐n𝐙1+𝐐n1𝐙],\displaystyle\mathbf{M}_{n}=i\sigma_{3}\left[\mathbf{Q}_{n}\mathbf{Q}_{n-1}-Q_{o}^{2}\mathbf{I}-\frac{1}{2}(z-1/z)^{2}\mathbf{I}-\mathbf{Q}_{n}\mathbf{Z}^{-1}+\mathbf{Q}_{n-1}\mathbf{Z}\right]\,, (4g)

where vnv_{n} is a 22-component vector, zz\in\mathbb{C} is the scattering parameter, and Qn(τ)Q_{n}(\tau) is the AL potential.

If Qn(τ)Q_{n}(\tau) satisfies (3) as n±n\to\pm\infty, the asymptotic behavior of the simultaneous solutions of the Lax pair is given by λn(ir)neiΩτ\lambda^{n}(ir)^{n}e^{i\Omega\tau} or λn(ir)neiΩτ\lambda^{-n}(ir)^{-n}e^{-i\Omega\tau}, where λ\lambda as a function of zz is defined by

ir(λ+1/λ)=z+1/z,r=Qo21+,ir(\lambda+1/\lambda)=z+1/z\,,\qquad r=\sqrt{Q_{o}^{2}-1}\in\mathbb{R}^{+}\,, (5)

and the dispersion relation is given by:

Ω(z)=i2r(z1/z)(λ1/λ)ir2λz(z21)(λ21).\Omega(z)=-\frac{i}{2}r(z-1/z)(\lambda-1/\lambda)\equiv-\frac{ir}{2\lambda z}(z^{2}-1)(\lambda^{2}-1)\,. (6)

Clearly, λ=λ(z)\lambda=\lambda(z) has branching, with 4 branch points on the imaginary axis located at:

z=i(r±Qo),z=i(r±Qo).z=i(r\pm Q_{o})\,,\qquad z=i(-r\pm Q_{o})\,. (7)

Note that rQo<1<rQo<0<Qor<1<Qo+r-r-Q_{o}<-1<r-Q_{o}<0<Q_{o}-r<1<Q_{o}+r, which specifies the order of the branch points.

Refer to caption
Refer to caption
Figure 1: Left: The choice of branch cut in the complex ξ\xi-plane, ξ=(z+1/z)/2ir\xi=(z+1/z)/2ir. Right: The 2-sheeted covering defined by λ=ξ+(ξ21)1/2\lambda=\xi+(\xi^{2}-1)^{1/2}.

It is convenient to introduce the variable ξ=(z+1/z)/2ir\xi=(z+1/z)/2ir, and define a 2-sheeted Riemann surface cut across the segment (1,1)(-1,1) on the real ξ\xi-axis, with local coordinates on each sheet given as in the left panel of Fig. 1:

ξ1=r1eiθ1,ξ+1=r2eiθ20θ1,θ2<2π\displaystyle\xi-1=r_{1}e^{i\theta_{1}}\,,\qquad\xi+1=r_{2}e^{i\theta_{2}}\qquad 0\leq\theta_{1},\theta_{2}<2\pi (8)
ξ=r~eiθ0θ<2π\displaystyle\xi=\tilde{r}e^{i\theta}\qquad 0\leq\theta<2\pi (9)

such that on Sheet I/II λ(z)=ξ±ξ21\lambda(z)=\xi\pm\sqrt{\xi^{2}-1}. The IST developed in [29] is formulated in terms of a uniformization variable

ζ(z)=λ(z)/z,\zeta(z)=\lambda(z)/z\,, (10)

for which one has

z2=ζirζ(irζ1),λ2=ζζirirζ1,zλ=ζirirζ1,z^{2}=\frac{\zeta-ir}{\zeta(ir\zeta-1)},\qquad\lambda^{2}=\zeta\frac{\zeta-ir}{ir\zeta-1},\qquad z\lambda=\frac{\zeta-ir}{ir\zeta-1}\,, (11)

showing that all these quantities, as well as all quantities which are even functions of λ\lambda and zz, are meromorphic functions of ζ\zeta. It is worth noticing that |λ2(ζ)|1|\lambda^{2}(\zeta)|\lessgtr 1 for ζD±\zeta\in D_{\pm}, where D±={ζ:|ζir|Qo}D_{\pm}=\left\{\zeta\in\mathbb{C}:\,|\zeta-ir|\lessgtr Q_{o}\right\}, and |λ(ζ)|2=1|\lambda(\zeta)|^{2}=1 for ζΣ\zeta\in\Sigma, where Σ={ζ:|ζir|=Qo}\Sigma=\left\{\zeta\in\mathbb{C}:\,|\zeta-ir|=Q_{o}\right\}. We refer the reader to [29] for the details about the IST, while noting that in Appendix B we provide a short errata to correct some typos and small inaccuracies in [29]. For the purposes of this work, it suffices to recall that the solitons/breathers of the AL equation are characterized by special values of the spectral parameter (zz, or ζ\zeta) for which bounded eigenfunctions of the Lax pair exist. In terms of the uniformization variable ζ\zeta such discrete eigenvalues appear in symmetric quartets: {ζk,ζk+irirζk+1,1/ζk,irζk1ζkir}\left\{\zeta_{k},\,\frac{\zeta_{k}^{*}+ir}{ir\zeta_{k}^{*}+1},\,-1/\zeta_{k}^{*},\,\frac{ir\zeta_{k}-1}{\zeta_{k}-ir}\right\}, with the first two in DD_{-} and the last two in D+D_{+}. It is convenient to then group the eigenvalues as follows:

{ζk,ζ¯k}k=12J,ζk=ζkJ+irirζkJ+1for k=J+1,,2J\left\{\zeta_{k},\bar{\zeta}_{k}\right\}_{k=1}^{2J}\,,\qquad\zeta_{k}=\frac{\zeta_{k-J}^{*}+ir}{ir\zeta_{k-J}^{*}+1}\quad\text{for }k=J+1,\dots,2J (12)

and ζ¯k=1/ζk\bar{\zeta}_{k}=-1/\zeta_{k}^{*} for k=1,,2Jk=1,\dots,2J. As is typical, the discrete eigenvalue specifies the velocity and amplitude of the corresponding soliton/breather. To each discrete eigenvalue ζ¯kD+\bar{\zeta}_{k}\in D_{+} is associated a norming constant C¯k\bar{C}_{k}:

Ck=(C¯k/ζ¯k2),Ck+J=(Q+)2(ζ¯kir)2C¯kk=1,,JC_{k}=-\left(\bar{C}_{k}/\bar{\zeta}_{k}^{2}\right)^{*},\qquad C_{k+J}=-\frac{(Q_{+}^{*})^{2}}{(\bar{\zeta}_{k}-ir)^{2}}\bar{C}_{k}\quad k=1,\dots,J (13)

which in turn characterizes the soliton/breather position and phase.

The general discrete breather solution of Eq. (2) on the nontrivial background (3) is given in Eq. (89) in [29], and it is an analog of the discrete Tajiri-Watanabe (TW) breather of the focusing AL equation obtained in [31]. The solution is given in terms of a discrete eigenvalue ζ¯1D+\bar{\zeta}_{1}\in D_{+} and its associated norming constant C¯1\bar{C}_{1}:

Qn(τ)=Q+{1+ir2Q+δ4(δ1+δ2)cosηi(δ1δ2)sinη+δ3eξcosh(ξξo)+αcos(ηηo)},Q_{n}(\tau)=Q_{+}\left\{1+\frac{ir}{2Q_{+}^{*}\sqrt{\delta_{4}}}\frac{(\delta_{1}^{*}+\delta_{2}^{*})\cos\eta-i(\delta_{1}^{*}-\delta_{2}^{*})\sin\eta+\delta_{3}^{*}e^{-\xi}}{\cosh{(\xi-\xi_{o})}+\alpha\cos(\eta-\eta_{o})}\right\}, (14)

where

δ1±δ2=C¯1ζ¯1ir1irζ¯1±C¯1Q+2ζ¯1(1+irζ¯1)2,δ3=|γ|2(ζ¯1ir)|ζ¯2ζ¯1|2(ζ¯1+ζ¯1)Q+(ζ1ir)(1+|ζ¯1|2)|λ¯121|2,\displaystyle\delta_{1}\pm\delta_{2}=\bar{C}_{1}\frac{\bar{\zeta}_{1}-ir}{1-ir\bar{\zeta}_{1}}\pm\bar{C}_{1}^{*}\frac{Q_{+}^{2}\bar{\zeta}_{1}^{*}}{(1+ir\bar{\zeta}_{1}^{*})^{2}}\,,\qquad\delta_{3}=-\frac{|\gamma|^{2}(\bar{\zeta}_{1}-ir)|\bar{\zeta}_{2}-\bar{\zeta}_{1}|^{2}(\bar{\zeta}_{1}+\bar{\zeta}_{1}^{*})}{Q_{+}^{*}(\zeta_{1}-ir)(1+|\bar{\zeta}_{1}|^{2})|\bar{\lambda}_{1}^{2}-1|^{2}}\,, (15a)
δ4=|γ|2|ζ¯1|2|ζ¯1ir|2(|1irζ¯1|2Qo2)2r2Qo2|λ¯121|2(1+|ζ¯1|2)2|1irζ¯1|2,γ=Q+C¯11irζ¯1,A~1+γ=γλ¯12λ¯121,\displaystyle\delta_{4}=\frac{|\gamma|^{2}|\bar{\zeta}_{1}|^{2}|\bar{\zeta}_{1}-ir|^{2}(|1-ir\bar{\zeta}_{1}|^{2}-Q_{o}^{2})^{2}}{r^{2}Q_{o}^{2}|\bar{\lambda}_{1}^{2}-1|^{2}(1+|\bar{\zeta}_{1}|^{2})^{2}|1-ir\bar{\zeta}_{1}|^{2}}\,,\qquad\gamma=\frac{Q_{+}^{*}\bar{C}_{1}}{1-ir\bar{\zeta}_{1}}\,,\qquad\tilde{A}_{1}+\gamma=\frac{\gamma\bar{\lambda}_{1}^{2}}{\bar{\lambda}_{1}^{2}-1}\,, (15b)
ξ=nlogρ+2(ImΩ¯1)τ,η=nϕ+2(ReΩ¯1)τ,\displaystyle\xi=n\log\rho+2(\mathop{\rm Im}\nolimits\bar{\Omega}_{1})\tau\,,\qquad\eta=n\phi+2(\mathop{\rm Re}\nolimits\bar{\Omega}_{1})\tau, (15c)
α=|A~1+γ|/δ4>1,\displaystyle\alpha=|\tilde{A}_{1}+\gamma|/\sqrt{\delta_{4}}>1\,, (15d)
ξo=logδ4,cosηo=Re(A~1+γ)|A~1+γ|,sinηo=Im(A~1+γ)|A~1+γ|,\displaystyle\xi_{o}=\log\sqrt{\delta_{4}}\,,\qquad\qquad\cos\eta_{o}=\frac{\mathop{\rm Re}\nolimits(\tilde{A}_{1}+\gamma)}{|\tilde{A}_{1}+\gamma|}\,,\qquad\sin\eta_{o}=-\frac{\mathop{\rm Im}\nolimits(\tilde{A}_{1}+\gamma)}{|\tilde{A}_{1}+\gamma|}\,, (15e)
Ω¯1Ω(ζ¯1)=r2(ζ¯12+2iζ¯1/r+1)(ζ¯122irζ¯1+1)2ζ¯1(ζ¯1ir)(1irζ¯1).\displaystyle\bar{\Omega}_{1}\equiv\Omega(\bar{\zeta}_{1})=\frac{r^{2}(\bar{\zeta}_{1}^{2}+2i\bar{\zeta}_{1}/r+1)(\bar{\zeta}_{1}^{2}-2ir\bar{\zeta}_{1}+1)}{2\bar{\zeta}_{1}(\bar{\zeta}_{1}-ir)(1-ir\bar{\zeta}_{1})}. (15f)

According to (11), λ2(ζ)=ζ(ζir)/(irζ1)\lambda^{2}(\zeta)=\zeta(\zeta-ir)/(ir\zeta-1) and

λ¯12=λ2(ζ¯1)=:eiϕ/ρ.\bar{\lambda}_{1}^{2}=\lambda^{2}(\bar{\zeta}_{1})=:e^{i\phi}/\rho. (16)

Also, ζ¯2=(ζ¯1+ir)/(irζ¯1+1)\bar{\zeta}_{2}=(\bar{\zeta}_{1}^{*}+ir)/(ir\bar{\zeta}_{1}^{*}+1) and ζ1=1/ζ¯1\zeta_{1}=-1/\bar{\zeta}_{1}^{*}, and we recall that |λ2(ζ)|<1|\lambda^{2}(\zeta)|<1 for any ζD+\zeta\in D_{+} (hence, ρ>1\rho>1). It is also important to point out that α>1\alpha>1 for any choice of the soliton parameters ζ¯1\bar{\zeta}_{1} and C¯1\bar{C}_{1}, which means that in general the TW solution is singular. This singularity, as well as ways to avoid it, is crucial for our considerations that follow next. We refer the reader to [29] for the details of the derivation of Eq. (14), while noting that we corrected a typo in the expressions for ξ,η\xi,\eta (see also Appendix B).

3 Kuznetsov-Ma (KM) breathers

The discrete analog of the Kuznetsov-Ma (KM) solutions is obtained when the discrete eigenvalue ζ¯1D+{0,r}\bar{\zeta}_{1}\in D_{+}\setminus\left\{0,r\right\} is purely imaginary, i.e., ζ¯1=iκ\bar{\zeta}_{1}=i\kappa with

κ(1+r2+r,1+r2+r){0,r},\kappa\in(-\sqrt{1+r^{2}}+r,\sqrt{1+r^{2}}+r)\setminus\left\{0,r\right\},

where we recall r=Qo21>0r=\sqrt{Q_{o}^{2}-1}>0. In this case, the parameter λ¯12=λ2(ζ¯1)\bar{\lambda}_{1}^{2}=\lambda^{2}(\bar{\zeta}_{1})\in\mathbb{R}, but note that it is not necessarily positive. Specifically, one has

λ¯12=κ(κr)1+rκ\bar{\lambda}_{1}^{2}=\frac{\kappa(\kappa-r)}{1+r\kappa} (17)

and one can check that 1/r<1+r2+r-1/r<-\sqrt{1+r^{2}}+r for any rr, therefore

λ¯12>0forr2+1+r<κ<0 and r<κ<r2+1+r\displaystyle\bar{\lambda}_{1}^{2}>0\quad\text{for}\quad-\sqrt{r^{2}+1}+r<\kappa<0\ \text{ and }\ r<\kappa<\sqrt{r^{2}+1}+r
λ¯12<0for0<κ<r.\displaystyle\bar{\lambda}_{1}^{2}<0\quad\text{for}\quad 0<\kappa<r\,.

In [29] the implicit assumption was made that λ¯12>0\bar{\lambda}_{1}^{2}>0, but in the parametrization λ¯12=eiϕ/ρ\bar{\lambda}_{1}^{2}=e^{i\phi}/\rho one needs to take ϕ=π\phi=\pi if λ¯12<0\bar{\lambda}_{1}^{2}<0, while indeed ϕ=0\phi=0 when λ¯12>0\bar{\lambda}_{1}^{2}>0. This will not affect the regularity of the solution (see below), but it will give rise to a different solution if one chooses values of r,κr,\kappa for which λ¯12<0\bar{\lambda}_{1}^{2}<0. Based on the above discussion, we have:

ρ=|1+κrκ(κr)|>1,\rho=\left|\frac{1+\kappa r}{\kappa(\kappa-r)}\right|>1\,, (18)

and

ϕ=0for 1+r2+r<κ<0orr<κ<r2+1+r\displaystyle\phi=0\qquad\text{for }-\sqrt{1+r^{2}}+r<\kappa<0\quad\text{or}\quad r<\kappa<\sqrt{r^{2}+1}+r (19)
ϕ=πfor0<κ<r.\displaystyle\phi=\pi\qquad\text{for}\qquad 0<\kappa<r. (20)

Now, considering (15) when ζ¯1=iκ\bar{\zeta}_{1}=i\kappa, one can immediately see that δ3=0\delta_{3}=0 and

Ω¯1=r(rκ2+2κr)(κ2+2rκ+1)2κ(κr)(1+κr)[corrected a typo in Eq. (94) in [29]].\bar{\Omega}_{1}=\frac{r(r\kappa^{2}+2\kappa-r)(-\kappa^{2}+2r\kappa+1)}{2\kappa(\kappa-r)(1+\kappa r)}\in\mathbb{R}\qquad\text{[corrected a typo in Eq.~(94) in \cite[cite]{[\@@bibref{Number}{OP2019}{}{}]}]}\,. (21)

The remaining coefficients (15) in the TW solution reduce to

δ4\displaystyle\delta_{4} =|C¯1|2κ2(κr)2(rκ2+2κr)2(1+κ2)2(1+κr)2(κ22κr1)2>0,\displaystyle=\frac{|\bar{C}_{1}|^{2}\kappa^{2}(\kappa-r)^{2}(r\kappa^{2}+2\kappa-r)^{2}}{(1+\kappa^{2})^{2}(1+\kappa r)^{2}(\kappa^{2}-2\kappa r-1)^{2}}>0, (22a)
δ1±δ2\displaystyle\delta_{1}\pm\delta_{2} =iC¯1κr1+κriC¯1Q+2κ(1+κr)2,\displaystyle=i\bar{C}_{1}\frac{\kappa-r}{1+\kappa r}\mp i\bar{C}_{1}^{*}Q_{+}^{2}\frac{\kappa}{(1+\kappa r)^{2}}, (22b)
A~1+γ\displaystyle\tilde{A}_{1}+\gamma =C¯1Q+κ(κr)(1+rκ)(κ22rκ1),\displaystyle=\bar{C}_{1}\frac{Q_{+}^{*}\kappa(\kappa-r)}{(1+r\kappa)(\kappa^{2}-2r\kappa-1)}, (22c)

and

ξ=nlogρ,η=nϕ+2Ω¯1τ,ξo=logδ4,\displaystyle\xi=n\log\rho\,,\qquad\eta=n\phi+2\bar{\Omega}_{1}\tau\,,\qquad\xi_{o}=\log\sqrt{\delta_{4}}, (23a)
α=|A~1+γ|δ4(1+κ2)1+r2|rκ2+2κr|>1,\displaystyle\alpha=\frac{|\tilde{A}_{1}+\gamma|}{\sqrt{\delta_{4}}}\equiv\frac{(1+\kappa^{2})\sqrt{1+r^{2}}}{|r\kappa^{2}+2\kappa-r|}>1, (23b)
cosηo=Re(A~1+γ)|A~1+γ|sgn(λ¯12)cos(χθ),sinηo=Im(A~1+γ)|A~1+γ|sgn(λ¯12)sin(χθ),\displaystyle\cos\eta_{o}=\frac{\mathop{\rm Re}\nolimits(\tilde{A}_{1}+\gamma)}{|\tilde{A}_{1}+\gamma|}\equiv-\mathrm{sgn}(\bar{\lambda}_{1}^{2})\cos(\chi-\theta)\,,\quad\sin\eta_{o}=-\frac{\mathop{\rm Im}\nolimits(\tilde{A}_{1}+\gamma)}{|\tilde{A}_{1}+\gamma|}\equiv\mathrm{sgn}(\bar{\lambda}_{1}^{2})\sin(\chi-\theta)\,, (23c)

where we have written the norming constant C¯1=ceiχ\bar{C}_{1}=c\,e^{i\chi}, c>0c>0, and the background as Q+=Qoeiθeiθ1+r2Q_{+}=Q_{o}\,e^{i\theta}\equiv e^{i\theta}\sqrt{1+r^{2}}, and to simplify the expressions of cosηo,sinηo\cos\eta_{o},\sin\eta_{o} we have taken into account that κ22rκ1<0\kappa^{2}-2r\kappa-1<0 for κ\kappa in the allowed range, and that the remaining factor in A~1+γ\tilde{A}_{1}+\gamma is simply λ¯12\bar{\lambda}_{1}^{2}. Note the additional term nϕn\phi in the expression (23a) of η\eta compared to [29], which, we reiterate, is only present if 0<κ<r0<\kappa<r.

For simplicity, we can assume below that θ+=0\theta_{+}=0, i.e., Q+=QoQ_{+}=Q_{o}, and also take the norming constant to be real and positive, i.e., χ=0\chi=0 and C¯1=c>0\bar{C}_{1}=c>0. Then, if r,κr,\kappa are chosen so that λ¯12>0\bar{\lambda}_{1}^{2}>0, ηo=π\eta_{o}=\pi and from (14) we obtain

Qn(τ)=Qo+ir2δ4(δ1+δ2)cos(2Ω¯1τ)i(δ1δ2)sin(2Ω¯1τ)cosh(nlogρξo)αcos(2Ω¯1τ).Q_{n}(\tau)=Q_{o}+\frac{ir}{2\sqrt{\delta_{4}}}\frac{\left(\delta_{1}^{*}+\delta_{2}^{*}\right)\cos{(2\bar{\Omega}_{1}\tau)}-i\left(\delta_{1}^{*}-\delta_{2}^{*}\right)\sin{(2\bar{\Omega}_{1}\tau)}}{\cosh(n\log\rho-\xi_{o})-\alpha\cos{(2\bar{\Omega}_{1}\tau)}}\,. (24)

Conversely, still assuming that the phases of Q+Q_{+} and C¯1\bar{C}_{1} are zero, if r,κr,\kappa are chosen so that λ¯12<0\bar{\lambda}_{1}^{2}<0, then ηo=0\eta_{o}=0, and (14) yields

Qn(τ)=Qo+ir(1)n2δ4(δ1+δ2)cos(2Ω¯1τ)i(δ1δ2)sin(2Ω¯1τ)cosh(nlogρξo)+(1)nαcos(2Ω¯1τ).Q_{n}(\tau)=Q_{o}+\frac{ir(-1)^{n}}{2\sqrt{\delta_{4}}}\frac{\left(\delta_{1}^{*}+\delta_{2}^{*}\right)\cos{(2\bar{\Omega}_{1}\tau)}-i\left(\delta_{1}^{*}-\delta_{2}^{*}\right)\sin{(2\bar{\Omega}_{1}\tau)}}{\cosh(n\log\rho-\xi_{o})+(-1)^{n}\alpha\cos{(2\bar{\Omega}_{1}\tau)}}\,. (25)

Eq. (24) was already obtained in [29], and we only corrected a typo. In the remainder of this work, we will refer to this solution as KM1. On the other hand, to the best of our knowledge Eq. (25) is a novel KM breather solution of the defocusing AL equation with background Qo>1Q_{o}>1, which we will refer to as KM2. Some prototypical case examples of both families of solutions are shown in Fig. 2. There, it can be seen that the examples of KM2 breathers, carrying the staggered spatial structure evident in Eq. (25), feature peaks that bear an alternating structure in time, contrary to what is observed for the KM1 breathers.

Refer to caption
Figure 2: Regular Kuznetsov-Ma solutions corresponding to (a) r=0.8r=0.8, κ=0.3\kappa=-0.3, c=1.23 (Period: 3.44946); (b) r=0.8r=0.8, κ=0.7\kappa=0.7, c=257.5c=257.5 (Period: 0.530412); (c) r=2r=2, κ=3.5\kappa=3.5, c=2.32339c=2.32339 (Period: 1.62646); (d) r=2r=2, κ=0.09\kappa=0.09, c=13.5884c=13.5884 (Period: 0.261321); (e) r=4r=4, κ=4.5\kappa=4.5, c=101.562c=101.562 (Period: 0.0466168). (a), (c), and (e) are KM1 solutions, i.e., given by (24), while (b) and (d) are KM2 solutions, i.e., corresponding to (25). To confirm that the solutions presented are correct, below each panel is a log-plot of the error maximized over nn\in\mathbb{Z} as a function of τ\tau.

4 Regularity conditions for the KM breathers

Note that α>1\alpha>1 for any κr\kappa\neq r [see Eq. (23b)], which means that the denominators in Eq. (24) and Eq. (25) will generically have zeros, and hence the solution will be singular unless, for a given rr (specified by QoQ_{o}), one can choose the soliton parameters κ\kappa and C¯1\bar{C}_{1} so that no integer falls in the interval where cosh(nlogρξo)α\cosh(n\log\rho-\xi_{o})\leq\alpha.

Indeed, the minimum value for the cosh\cosh term in the denominator is 1, and it is achieved when x=ξo/logρx=\xi_{o}/\log\rho, where ξo=logδ4\xi_{o}=\log\sqrt{\delta_{4}}. The interval where cosh\cosh is less than or equal to α\alpha is given by

(ξoarccoshα)/logρ<x<(ξo+arccoshα)/logρ,(\xi_{o}-\mathop{\rm arccosh}\nolimits\alpha)/\log\rho<x<(\xi_{o}+\mathop{\rm arccosh}\nolimits\alpha)/\log\rho, (26)

and the width of this interval is 2arccoshα/logρ2\mathop{\rm arccosh}\nolimits\alpha/\log\rho, which is independent of the norming constant C¯1\bar{C}_{1}, while the center of the interval, which is the center of the soliton, ξo/logρ\xi_{o}/\log\rho, is determined by |C¯1||\bar{C}_{1}| via δ4\delta_{4}.

A necessary condition in order for the above interval (26) not to contain any integer is that the width of the interval be strictly less than 1, and hence a necessary condition for regularity of the solution is that

f(r,κ):=arccosh[(1+κ2)1+r2|rκ2+2κr|]12log|1+κrκ(κr)|<0.f(r,\kappa):=\mathop{\rm arccosh}\nolimits\left[\frac{(1+\kappa^{2})\sqrt{1+r^{2}}}{|r\kappa^{2}+2\kappa-r|}\right]-\frac{1}{2}\log\left|\frac{1+\kappa r}{\kappa(\kappa-r)}\right|<0. (27)

The latter is an inequality for the two parameters r,κr,\kappa, and one can find pairs of values ro,κor_{o},\kappa_{o} with ro>0r_{o}>0 and ro2+1+r<κo<ro2+1+ro-\sqrt{r_{o}^{2}+1}+r<\kappa_{o}<\sqrt{r_{o}^{2}+1}+r_{o}, κo0,ro\kappa_{o}\neq 0,r_{o} for which this necessary condition for regularity is satisfied; see, in particular, the representation of the left panel of Fig. 3. Note that the set of loci of (r,κ)(r,\kappa) for which (27) is satisfied is certainly not empty, since logρ\log\rho in the second term is positive (recall ρ>1\rho>1), and it becomes arbitrarily large as κr\kappa\to r from either side. The contour plot of f(r,κ)f(r,\kappa) is shown on the left panel in Fig. 3. A stronger regularity condition, i.e., requiring the width of the interval where cosh(nlogρξo)α0\cosh(n\log\rho-\xi_{o})-\alpha\leq 0 to be smaller than 1/2, can be imposed to ensure a larger lower bound on the denominator of the solution. The corresponding contour plot is shown on the right panel in Fig. 3.

Refer to caption
Figure 3: (a) Contour plot of f(r,κ)=arccoshαlogρf(r,\kappa)=\mathop{\rm arccosh}\nolimits\alpha-\log\sqrt{\rho} as a function of rr (horizontal axis) and κ\kappa (vertical axis) for rr2+1<κ<r+r2+1r-\sqrt{r^{2}+1}<\kappa<r+\sqrt{r^{2}+1}. The blue shaded regions correspond to f(r,κ)<0f(r,\kappa)<0 (where the regularity condition is satisfied) and the red shaded regions correspond to f(r,κ)>0f(r,\kappa)>0 (where the regularity condition is not satisfied). The dashed red lines correspond to κ=0,(Qo1)/r,r\kappa=0,(Q_{o}-1)/r,r, where f(r,κ)f(r,\kappa) is singular. Note that if rr2+1<κ<0r-\sqrt{r^{2}+1}<\kappa<0 or r<κ<r+r2+1r<\kappa<r+\sqrt{r^{2}+1} the solution is a KM1, while if 0<κ<r0<\kappa<r the solution is a KM2. (b) Same for g(r,κ)=arccoshαlog(ρ)1/4g(r,\kappa)=\mathop{\rm arccosh}\nolimits\alpha-\log(\rho)^{1/4}. In order for the stronger regularity condition to be satisfied, (r,κ)(r,\kappa) should be chosen in the blue regions.

Once ro,κor_{o},\kappa_{o} are chosen to satisfy (27) so that the interval has width less than 1, we need to choose the center of the interval so that it does not contain any integer. We can fix n¯\bar{n}\in\mathbb{Z} arbitrarily, and place the center the soliton in the interval (n¯,n¯+1)(\bar{n},\bar{n}+1) by requiring:

n¯+Δ<ξologρ<n¯+1Δ,\bar{n}+\Delta<\frac{\xi_{o}}{\log\rho}<\bar{n}+1-\Delta, (28)

where the half width of the interval, Δ\Delta, is

Δ=arccoshαlogρ=arccosh[(1+κ2)1+r2|rκ2+2κr|1]log|1+κrκ(κr)|<12.\Delta=\frac{\mathop{\rm arccosh}\nolimits\alpha}{\log\rho}=\frac{\mathop{\rm arccosh}\nolimits\left[(1+\kappa^{2})\sqrt{1+r^{2}}|r\kappa^{2}+2\kappa-r|^{-1}\right]}{\log\left|\frac{1+\kappa r}{\kappa(\kappa-r)}\right|}<\frac{1}{2}. (29)

[Note the width of the above interval is exactly 12Δ>01-2\Delta>0.] The smaller the value of Δ\Delta, the further away from the singularities one can choose the closest integers, and therefore the smaller the value of Qn(τ)Q_{n}(\tau).

Recalling that ξo=logδ4\xi_{o}=\log\sqrt{\delta_{4}}, the inequality (28) can be written as

logρn¯+Δ<logδ4<logρn¯+1Δβρn¯+Δ<|C¯1|<βρn¯+1Δ,\log\rho^{\bar{n}+\Delta}<\log\sqrt{\delta_{4}}<\log\rho^{\bar{n}+1-\Delta}\quad\Leftrightarrow\quad\beta\rho^{\bar{n}+\Delta}<|\bar{C}_{1}|<\beta\rho^{\bar{n}+1-\Delta}, (30)

where we have used the definition of δ4\sqrt{\delta_{4}} in terms of C¯1\bar{C}_{1} and

β=|C¯1|δ4|(1+κ2)(1+κr)(κ22rκ1)κ(κr)(rκ2+2κr)|.\beta=\frac{|\bar{C}_{1}|}{\sqrt{\delta_{4}}}\equiv\left|\frac{(1+\kappa^{2})(1+\kappa r)(\kappa^{2}-2r\kappa-1)}{\kappa(\kappa-r)(r\kappa^{2}+2\kappa-r)}\right|\,. (31)

Any choice of c=|C¯1|c=|\bar{C}_{1}| in the above intervals guarantees that for the corresponding values of r,κr,\kappa the denominator of Qn(τ)Q_{n}(\tau) will not vanish at the integers. For instance, if one sets n¯=0\bar{n}=0, then n=0n=0 and n=1n=1 are the integers where the denominator will be the smallest, and one would want to choose cc in each range so that n=0n=0 and n=1n=1 are equidistant from the soliton center. Recall that the soliton center is ξo/logρ\xi_{o}/\log\rho, and the choice of cc in the above intervals guarantees that 0<Δ<ξo/logρ<1Δ<10<\Delta<\xi_{o}/\log\rho<1-\Delta<1. The plots in Fig. 4 show cosh(nlogρξo)α\cosh{(n\log\rho-\xi_{o})}-\alpha at the integer values n=0,1n=0,1. It is clear that the optimal choice for cc in each case is the value at the intersection of the two curves.

Refer to captionRefer to caption


Figure 4: Plots of cosh(nlogρξo)α\cosh{(n\log\rho-\xi_{o})}-\alpha at the integer vales n=0n=0 (blue) and n=1n=1 (orange) for r=1r=1 and κ=0.13\kappa=-0.13 (left), κ=0.06\kappa=0.06 (right) as functions of c=|C¯1|c=|\bar{C}_{1}| in the range of allowed values, i.e., 6.1c11.96.1\leq c\leq 11.9 (left) and 70c15670\leq c\leq 156. The optimal choice for cc in each case is at the intersection point, i.e., c~=8.52544\tilde{c}=8.52544 and c~=104.164\tilde{c}=104.164, respectively.

Note that for any fixed rr the frequency, Ω¯1\bar{\Omega}_{1}, and logρ\log\rho, which controls the width of the breather in each period, become singular at κ=0,r\kappa=0,r (cf Fig 5). As it is clear from the contour plots in Fig 3, solutions are regular in left and right neighborhoods of κ=0,r\kappa=0,r, but in order to obtain solutions whose frequency is not too large and width not too small, one wants to keep sufficiently far from those singular values. On the other hand, the further away one moves from κ=0,r\kappa=0,r in the intervals where the solution remains bounded for all nn\in\mathbb{Z}, the closer Δ\Delta is to its limiting value of 1/2, and correspondingly the larger the solution is going to be. So a careful balance is required in the choice of parameters in order to obtain more meaningful KM solutions which are regular for all nn\in\mathbb{Z}, τ\tau\in\mathbb{R}. In Table 1 we provide some such examples, for various values of r>0r>0. For the parameters in the Table, we have chosen n¯=0\bar{n}=0 for simplicity.

Refer to captionRefer to caption

Figure 5: Plots of Ω¯1\bar{\Omega}_{1} (left) and logρ\log\rho (right) as functions of κ(r2+1+r,r2+1+r)\kappa\in(-\sqrt{r^{2}+1}+r,\sqrt{r^{2}+1}+r) for r=2r=2.
Table 1: Soliton parameters for regular KM breathers
rr range for κ\kappa κ\kappa Δ\Delta Ω¯1\bar{\Omega}_{1} logρ\log\rho range for cc optimal cc infn|denom|\inf_{n\in\mathbb{Z}}|\text{denom}|
1/2 (-0.618, 0) -0.08 0.37 -3.37 3.0 [90, 193] 131.7418 0.67
(0, 0.0665) 0.05 0.44 4.53 3.8 [652,1005] 809.7477 0.64
(0.4196, 1/2) 0.44 0.44 -4.61 3.8 [780,1231] 980.1981 0.67
(1/2, 1.61803) 0.6 0.37 3.5 3.1 [130,287] 193.2707 0.71
0.8 (-0.480625, 0) -0.1 0.32 -4.0 2.3 [19,41] 27.6189 0.45
(0, 0.09407) 0.08 0.46 4.7 2.9 [125,159] 141.1548 0.24
(0.6565247, 0.8) 0.69 0.43 -5.3 3.0 [188,285] 231.2327 0.4
(0.8, 2.08062) 1.2 0.37 1.7 1.4 [9,13] 10.8274 0.12
1 (-0.414, 0) -0.13 0.31 -3.5 1.8 [7,11] 8.5254 0.26
(0, 0.10717) 0.1 0.48 4.75 2.5 [62,68] 65.008 0.08
(0.806396, 1) 0.82 0.48 -4.8 2.5 [102,115] 108.565 0.1
(1, 2.4) 1.5 0.32 2.0 0.8 [6.7, 9.9] 8.14424 0.1
5/2\sqrt{5}/2 (-0.38, 0) -0.14 0.30 -3.5 1.6 [3.8,7.1] 5.18209 0.2
(0, 0.113275) 0.1 0.46 5.4 2.4 [45,53] 48.7821 0.13
(0.892, 1.118) 0.9 0.48 -5 2.3 [80.84] 82.087 0.04
(1.118, 2.61803) 1.5 0.3 3.4 1.5 [12,21] 15.7055 0.2
2 (-0.236068, 0) -0.13 0.2 -5 1.0 [0.7,1.2] 0.9242 0.1
(0, 0.135249) 0.1 0.4 10.9 1.8 [10.3, 15.3] 12.5187 0.19
(1.46773, 2) 1.6 0.38 -11.4 1.9 [37,57] 45.8334 0.2
(2, 4.2) 3 0.2 4.2 0.8 [5.1,8.2] 6.4804 0.08
Table 2: Parameters for regular KM breathers. Recall that, for fixed rr, one needs to choose κ(r2+1r,r2+1+r){0,r}\kappa\in(-\sqrt{r^{2}+1}-r,\sqrt{r^{2}+1}+r)\setminus\left\{0,r\right\} in such a way that the regularity condition (29) holds. The interval for c=|C¯1|c=|\bar{C}_{1}| is then chosen so that (30) holds; for the values in this table, n¯=0\bar{n}=0. The estimate for the lower bound of the denominator is obtained by evaluating cosh(nlogρξo)α\cosh(n\log\rho-\xi_{o})-\alpha for the chosen r,κ,c=c~r,\kappa,c=\tilde{c} at n=0,1n=0,1. Finally, choices of 0<κ<r0<\kappa<r yield KM2 solutions, while for all other admissible values of κ\kappa a KM1 solution is obtained.

5 Darboux transformations for KM breathers

A Darboux transformation is meant to take a known solution of an integrable PDE or ODE into a new solution. In [15], the Darboux transformation for the focusing and defocusing AL equations (AL±, respectively) on a nontrivial background were obtained to derive and study the stability of periodic Akhmediev breather solutions. The construction of the Darboux matrix (DM) for the Lax pair (4a) follows the one proposed in [18, 25] for the case of rapidly decaying solutions (see also [13], where the Darboux transformation is used to obtain rogue wave solutions of the focusing AL equation superimposed to standing periodic waves). The DM Dn(z,τ)D_{n}(z,\tau) takes a fundamental solution Ψn[0](z,τ)\Psi_{n}^{[0]}(z,\tau) of the Lax pair (4a) with potential Qn[0](τ)Q_{n}^{[0]}(\tau) into a new fundamental solution Ψn(z,τ)=Dn(z,τ)Ψn[0]\Psi_{n}(z,\tau)=D_{n}(z,\tau)\Psi_{n}^{[0]} corresponding to a potential Qn(τ)Q_{n}(\tau). The requirement that both Ψn[0]\Psi_{n}^{[0]} and Ψn\Psi_{n} satisfy the equations in the Lax pair implies that the DM is

Dn+1Ln[0]=LnDn,dDndτ=MnDnDnMn[0].D_{n+1}L_{n}^{[0]}=L_{n}D_{n}\,,\qquad\frac{dD_{n}}{d\tau}=M_{n}D_{n}-D_{n}M_{n}^{[0]}\,. (32)

Furthermore, the symmetries of the Lax pair and of the boundary conditions require that

Dn(z,τ)=σ1Dn(1/z,τ)σ1,σ1=(0110).D_{n}(z,\tau)=\sigma_{1}D_{n}^{*}(1/z^{*},\tau)\sigma_{1}\,,\qquad\sigma_{1}=\begin{pmatrix}0&1\\ 1&0\end{pmatrix}.

The details of the construction of the DM are given in [15]; in Appendix B we report, in our notations, what is needed below in order to reproduce the KM solutions presented in Sec 3, as well as some examples of double KM breathers.

Below, we will apply the DM to the case of KM breathers. In order to compare the solutions in Sec 3 with the ones one can derive using the DM, we need to take into account that the latter is given in terms of the original spectral parameter zz (and λ(z)\lambda(z), as defined in (5)), while the former is expressed in terms of the uniform variable ζ\zeta (cf. Fig 6). For this reason, we start here by converting the purely imaginary discrete eigenvalues ζ¯j=iκjD+\bar{\zeta}_{j}=i\kappa_{j}\in D_{+} into the corresponding values for zjz_{j} and λj\lambda_{j}.

Refer to caption
Refer to caption
Refer to caption
Figure 6: Left: Sheet I of zz-plane, where λ=ξ+ξ21\lambda=\xi+\sqrt{\xi^{2}-1}. Center: Sheet II of zz-plane, where λ=ξξ21\lambda=\xi-\sqrt{\xi^{2}-1}. Right: ζ\zeta-plane; the dashed/solid red and blue circle |ζir|=Qo|\zeta-ir|=Q_{o} corresponds to the continuous spectrum (where |λ|=1|\lambda|=1), and the corresponding oriented contour Σ\Sigma identifies the regions D+D_{+} and DD_{-}. The points ζo±=i(r±Qo)\zeta_{o}^{\pm}=i(r\pm Q_{o}) are the images of the four branch points z=i(±r±Qo)z=i(\pm r\pm Q_{o}), and λo±=i(1Qo)/r\lambda_{o}^{\pm}=-i(1\mp Q_{o})/r; the dashed/solid purple circle C={ζ:|irζ1|=Qo}C=\left\{\zeta\in\mathbb{C}:|ir\zeta-1|=Q_{o}\right\} corresponds to |z|=1|z|=1.

Consider purely imaginary values of ζ=iκ\zeta=i\kappa, for all κ\kappa in the interval: (Qo+r,Qo+r){0,r}(-Q_{o}+r,Q_{o}+r)\setminus\left\{0,r\right\}. It follows from (11) that

z2=rκκ(rκ+1),λ2=κrκrκ+1,zλ=irκrκ+1i,z^{2}=\frac{r-\kappa}{\kappa(r\kappa+1)}\in\mathbb{R}\,,\qquad\lambda^{2}=-\kappa\frac{r-\kappa}{r\kappa+1}\in\mathbb{R}\,,\qquad z\lambda=i\frac{r-\kappa}{r\kappa+1}\in i\mathbb{R}\,,

showing that z2>0z^{2}>0 in the interval 0<κ<r0<\kappa<r where λ2<0\lambda^{2}<0, whereas z2<0z^{2}<0 for Qo+r<κ<0-Q_{o}+r<\kappa<0 and r<κ<r+1+r2r<\kappa<r+\sqrt{1+r^{2}} where λ2>0\lambda^{2}>0. This implies that when zz\in\mathbb{R} then λi\lambda\in i\mathbb{R} and vice versa. Note also that the third equation above allows one to determine the relative signs of zz and λ\lambda.

Specifically, we obtain the following.

For 0<κ<r0<\kappa<r:

z=±μ,λ=±iκμwith μ=rκκ(1+rκ)+.z=\pm\mu,\qquad\lambda=\pm i\kappa\mu\qquad\text{with }\mu=\sqrt{{\frac{r-\kappa}{\kappa(1+r\kappa)}}}\in\mathbb{R}^{+}\,. (33)

Since μ0+\mu\to 0^{+} as κr\kappa\to r^{-} and μ+\mu\to+\infty as κ0+\kappa\to 0^{+}, considering both signs in z=±μz=\pm\mu we see that the entire real zz-axis corresponds to the segment i[0,r]i[0,r] in the ζ\zeta-plane.

For Qo+r<κ<0-Q_{o}+r<\kappa<0:

z=±iμ,λ=±|κ|μwith μ=rκ|κ|(1+rκ)+.z=\pm i\mu\,,\qquad\lambda=\pm|\kappa|\mu\qquad\text{with }\mu=\sqrt{\frac{r-\kappa}{|\kappa|(1+r\kappa)}}\in\mathbb{R}^{+}. (34)

As κ(Qo+r)+\kappa\to(-Q_{o}+r)^{+}, one has μQo+r\mu\to Q_{o}+r, and μ+\mu\to+\infty as κ0\kappa\to 0^{-}, so in this case, considering both signs for z=±iμz=\pm i\mu, the segment i[Qo+r,0]i[-Q_{o}+r,0] in the ζ\zeta-plane corresponds to the semilines on the imaginary zz-axis: zi(,(Qo+r)]i[Qo+r,+)z\in i(-\infty,-(Q_{o}+r)]\cup i[Q_{o}+r,+\infty).

For r<κ<r+Qor<\kappa<r+Q_{o}:

z=±iμ,λ=κμwith μ=|rκ|κ(1+rκ)+.z=\pm i\mu\,,\qquad\lambda=\mp\kappa\mu\qquad\text{with }\mu=\sqrt{\frac{|r-\kappa|}{\kappa(1+r\kappa)}}\in\mathbb{R}^{+}. (35)

And since μQor\mu\to Q_{o}-r as κ(r+Qo)\kappa\to(r+Q_{o})^{-} and μ0\mu\to 0 as κr+\kappa\to r^{+}, it follows, again considering both signs in z=±iμz=\pm i\mu it follows that the segment i[r,r+Qo]i[r,r+Q_{o}] in the ζ\zeta-plane corresponds to segment i[Qo+r,Qor]i[-Q_{o}+r,Q_{o}-r] along the imaginary zz-axis.

For the purpose of the DM, one wants to parametrize both zz and λ\lambda above using one single parameter, and we can use the same parametrization for λ\lambda which was used for our KM breathers, namely:

λ=ρ1/2eiϕ/2elogρ+iϕ/2,λ±ne±iΩτ=exp[nlogρ(ImΩ)τ±inϕ2±i(ReΩ)τ],\lambda=\rho^{-1/2}e^{i\phi/2}\equiv e^{-\log\sqrt{\rho}+i\phi/2}\,,\qquad\lambda^{\pm n}e^{\pm i\Omega\tau}=\exp{\left[\mp n\log\sqrt{\rho}\mp(\mathop{\rm Im}\nolimits\Omega)\tau\pm i\frac{n\phi}{2}\pm i(\mathop{\rm Re}\nolimits\Omega)\tau\right]},

and further simplify the latter to:

λ±ne±iΩτ=exp[nlogρ±inϕ2±iΩτ]\lambda^{\pm n}e^{\pm i\Omega\tau}=\exp{\left[\mp n\log\sqrt{\rho}\pm i\frac{n\phi}{2}\pm i\Omega\tau\right]}

based on the fact that for KM breathers ρ>1\rho>1, ϕ/2=0,π,±π/2\phi/2=0,\pi,\pm\pi/2 depending on which of the above cases for κ\kappa we are considering, and also that ImΩ=0\mathop{\rm Im}\nolimits\Omega=0. As far as zz is concerned, that can be obtained from (5), and the appropriate sign chosen according to the cases indicated before. We need to establish the range of values of ρ>1\rho>1. This can be done by looking at each interval of values for κ\kappa below, determine what the corresponding interval of values for ρ\rho should be by solving (18) for ρ\rho in terms of κ\kappa. For any fixed rr, computing κρ\partial_{\kappa}\rho when 0<κ<r0<\kappa<r yields two stationary points, located at κ=(±Qo1)/r\kappa=(\pm Q_{o}-1)/r. These correspond to ζ=iκ\zeta=i\kappa coinciding with the points λo±\lambda_{o}^{\pm} (see Fig. 6); and κ=(Qo1)/r(0,r)\kappa=(Q_{o}-1)/r\in(0,r). In conclusion, for each given rr, one has:

min0<κ<rρ(r,κ)=ρ(r,(Qo1)/r)=r2(Qo1)2>1.\mathop{\rm min}\nolimits_{0<\kappa<r}\rho(r,\kappa)=\rho(r,(Q_{o}-1)/r)=\frac{r^{2}}{(Q_{o}-1)^{2}}>1. (36)

On the other hand, when Qo+r<κ<0-Q_{o}+r<\kappa<0 or r<κ<Qo+rr<\kappa<Q_{o}+r, one finds that κρ=(r2κ22κ+r)/κ2(κr)2\partial_{\kappa}\rho=(-r^{2}\kappa^{2}-2\kappa+r)/\kappa^{2}(\kappa-r)^{2}, with the same two stationary points κ=iλo±\kappa=-i\lambda_{o}^{\pm}. In these cases, however, the stationary points are both outside the ranges of values for κ\kappa, so ρ\rho is a monotonic function of κ\kappa. Furthermore, clearly ρ+\rho\to+\infty as either κ0\kappa\to 0^{-} or as κr\kappa\to r^{-}, while ρ1\rho\to 1 as κr±Qo\kappa\to r\pm Q_{o}, confirming that in both cases ρ\rho can take any value greater than 1.

0<κ<r0<\kappa<r:

The KM breathers in this case have λ\lambda purely imaginary and zz real, and z,iλz,-i\lambda with the same sign. Based on the fact that we expect |λ|<1|\lambda|<1 and taking, without loss of generality, λ\lambda in the upper half-plane, we have

λ=i/ρielogρz=rsinhlogρ±r2sinh2logρ1.\lambda=i/\sqrt{\rho}\equiv ie^{-\log\sqrt{\rho}}\quad\Leftrightarrow\quad z=r\sinh\log\sqrt{\rho}\pm\sqrt{r^{2}\sinh^{2}\log\sqrt{\rho}-1}. (37)

Now, it is not obvious that zz above is indeed real for any choice of ρ>1\rho>1; the condition that the argument of the square root be non-negative can be written as r2(ρ+1/ρ+2)4Qo20r^{2}(\rho+1/\rho+2)-4Q_{o}^{2}\geq 0, which, in turn is equivalent to

r2ρ22(1+Qo2)ρ+r20.r^{2}\rho^{2}-2(1+Q_{o}^{2})\rho+r^{2}\geq 0.

The roots of the above quadratic equation are ρ=(1±Qo)2/r2\rho=(1\pm Q_{o})^{2}/r^{2}, and the inequality is satisfied if either ρ(Qo1)2/r2\rho\leq(Q_{o}-1)^{2}/r^{2} or ρ(Qo+1)2/r2\rho\geq(Q_{o}+1)^{2}/r^{2} and the latter can be shown to coincide with the minimum value of ρ\rho in the interval 0<κ<r0<\kappa<r, as computed in (36), so indeed zz as given in (37) is real. Note that both choices for the sign of the square root in (37) would correspond to positive zz (equivalently, to positive iλz-i\lambda z), and therefore for a given ρ\rho greater or equal than the minimum value in (36), one could have two different KM breathers.

Qo+r<κ<0-Q_{o}+r<\kappa<0:

The KM breathers in this case have λ\lambda real and zz purely imaginary, and, as before, λ,iz\lambda,-iz have the same sign. Using similar parametrization as before:

λ=1/ρelogρz=ircoshlogρ+ir2cosh2logρ+1\lambda=1/\sqrt{\rho}\equiv e^{-\log\sqrt{\rho}}\quad\Leftrightarrow\quad z=ir\cosh\log\sqrt{\rho}+i\sqrt{r^{2}\cosh^{2}\log\sqrt{\rho}+1} (38)

and here the positive sign of the square root is the only one that ensures the correct sign of zz.

r<κ<Qo+rr<\kappa<Q_{o}+r:

The only difference with respect to the previous case is that iz-iz and λ\lambda should have opposite signs. If we want to keep zz in the upper half plane, then we should have

λ=elogρz=ircoshlogρ+ir2cosh2logρ+1\lambda=-e^{-\log\sqrt{\rho}}\quad\Leftrightarrow\quad z=-ir\cosh\log\sqrt{\rho}+i\sqrt{r^{2}\cosh^{2}\log\sqrt{\rho}+1} (39)

In all cases Ω\Omega, as a function of z,λz,\lambda is given in Eq. (6), which is actually independent of the signs since it depends on z2z^{2} and λ2\lambda^{2}.

In order to build the single KM and double KM breathers using the DM, we take Qn[0](τ)=QoQ_{n}^{[0]}(\tau)=Q_{o}, i.e, the background solution. In this case, one can take the fundamental matrix solution of the Lax pair to be

Ψn[0](ρ,τ)=(ir)n(λ(ρ)neiΩ(ρ)τQoir/λ(ρ)z(ρ)λ(ρ)neiΩ(ρ)τQoirλ(ρ)1/z(ρ)λ(ρ)neiΩ(ρ)τλ(ρ)neiΩ(ρ)τ),\Psi_{n}^{[0]}(\rho,\tau)=(ir)^{n}\begin{pmatrix}\lambda(\rho)^{n}e^{i\Omega(\rho)\tau}&\frac{Q_{o}}{ir/\lambda(\rho)-z(\rho)}\lambda(\rho)^{-n}e^{-i\Omega(\rho)\tau}\\ \frac{Q_{o}}{ir\lambda(\rho)-1/z(\rho)}\lambda(\rho)^{n}e^{i\Omega(\rho)\tau}&\lambda(\rho)^{-n}e^{-i\Omega(\rho)\tau}\end{pmatrix}, (40)

where λ(ρ)\lambda(\rho) and z(ρ)z(\rho) are given by (37), (38), or (39) depending on the desired range of values for κ\kappa; and Ω(ρ)\Omega(\rho) is defined by (6).

Following the construction of the Darboux transformation outlined in Appendix A, after simplification one can obtain explicit single KM solutions like those given in Section 3. These will depend on a single real parameter ρ1\rho_{1} that determines z1z(ρ1)z_{1}\equiv z(\rho_{1}), λ1λ(ρ1)\lambda_{1}\equiv\lambda(\rho_{1}), and Ω1Ω(ρ1)\Omega_{1}\equiv\Omega(\rho_{1}); as well as a complex proportionality constant γ1|γ1|eiφ\gamma_{1}\equiv|\gamma_{1}|e^{i\varphi} (defined in (56)) which plays the role of the norming constant.

First, by parametrizing z(ρ)z(\rho) and λ(ρ)\lambda(\rho) through either (38) or (39) (i.e. enforcing that z1=z1z_{1}=-z_{1}^{*} and λ1=λ1\lambda_{1}=\lambda_{1}^{*}), one can obtain the solution

Qn(τ)=Qo+r2(λ1λ11)B(AA1)cos(ηφ)i(A+A1)sin(ηφ)cosh(ξξo)+Bsin(ηφ),Q_{n}(\tau)=Q_{o}+\frac{r}{2}(\lambda_{1}-\lambda_{1}^{-1})B\frac{(A-A^{-1})\cos(\eta-\varphi)-i(A+A^{-1})\sin(\eta-\varphi)}{\cosh(\xi-\xi_{o})+B\sin(\eta-\varphi)}\,, (41)

where ξ=nlogρ1\xi=n\log\rho_{1}, η=2Ω1τ\eta=2\Omega_{1}\tau, and

A=Qoirλ1z11,B=(z1+z11)A|z1A2z11|ρ1,ξo=log|γ1|ρ1.A=\frac{Q_{o}}{ir\lambda_{1}-z_{1}^{-1}}\,,\;\;B=\frac{(z_{1}+z_{1}^{-1})A}{|z_{1}-A^{2}z_{1}^{-1}|\sqrt{\rho_{1}}}\,,\;\;\xi_{o}=-\log|\gamma_{1}|\sqrt{\rho_{1}}\,. (42)

If instead z(ρ)z(\rho) and λ(ρ)\lambda(\rho) are parametrized by (37) with either choice of the sign of the square root (i.e. z1=z1z_{1}=z_{1}^{*} and λ1=λ1\lambda_{1}=-\lambda_{1}^{*}), the solution is the KM2 breather, in the form

Qn(τ)=Qo+(1)nr2(λ1λ11)B(AA1)cos(ηφ)i(A+A1)sin(ηφ)cosh(ξξo)+(1)nBsin(ηφ).Q_{n}(\tau)=Q_{o}+(-1)^{n}\frac{r}{2}(\lambda_{1}-\lambda_{1}^{-1})B\frac{(A-A^{-1})\cos(\eta-\varphi)-i(A+A^{-1})\sin(\eta-\varphi)}{\cosh(\xi-\xi_{o})+(-1)^{n}B\sin(\eta-\varphi)}\,. (43)

For the purpose of comparing the solutions (41) and (43) with the previous forms (24) and (25), one can set the phase of γ1\gamma_{1} to be φ=π/2\varphi=\pi/2 (which is apparently equivalent to setting the phase of C¯1\bar{C}_{1} to zero as was done in Section 3). With this, (41) can be rewritten as

Qn(τ)=Qo+ir2(λ1λ11)B(A+A1)cosηi(AA1)sinηcosh(ξξo)Bcosη,Q_{n}(\tau)=Q_{o}+\frac{ir}{2}(\lambda_{1}-\lambda_{1}^{-1})B\frac{(A+A^{-1})\cos\eta-i(A-A^{-1})\sin\eta}{\cosh(\xi-\xi_{o})-B\cos\eta}\,, (44)

from which by comparison with (24) one can directly identify the coefficients in terms of the uniformization variable (parametrized by κ\kappa) with the parameters in terms of the original spectral parameter (parametrized by ρ1\rho_{1}) in the following way:

(λ1λ11)B(A±A1)δ1±δ2δ4,Bα.(\lambda_{1}-\lambda_{1}^{-1})B(A\pm A^{-1})\longleftrightarrow\frac{\delta_{1}^{*}\pm\delta_{2}^{*}}{\sqrt{\delta_{4}}}\,,\quad\quad B\longleftrightarrow\alpha\,. (45)

Finally, by comparing the two expressions for the center of the KM breather ξo\xi_{o}, one finds a way to relate the norming constant C¯1\bar{C}_{1} to the proportionality constant γ1\gamma_{1}; namely, |γ1|2ρ1=1/δ4|\gamma_{1}|^{2}\rho_{1}=1/\delta_{4} (recall that δ4\delta_{4} is proportional to |C¯1|2|\bar{C}_{1}|^{2}).

The parameter BB as defined above is real and could be positive or negative depending on the choice of parametrization. Regardless, it is true that |B|>1|B|>1 for any ρ1\rho_{1}, in which case the solutions above are generically singular. Following the same logic as in Section 4, we seek parameters ρ1\rho_{1} and γ1\gamma_{1} such that no integer lies in the interval where cosh(ξξo)|B|\cosh(\xi-\xi_{o})\leq|B|. A necessary condition for regularity that ensures that the width of this interval is less than 1 is

arccosh|B|12logρ1<0.\mathop{\rm arccosh}\nolimits|B|-\frac{1}{2}\log\rho_{1}<0\,. (46)

As before, it may be deemed to be useful to impose a stronger regularity condition, for example by replacing the 1/21/2 in (46) by 1/41/4 111However, as regards the practical manifestation of the instability, as illustrated in the next section, this was not found to modify the observed dynamics significantly.. Furthermore, we can center the solution between two lattice sites n¯\bar{n} and n¯+1\bar{n}+1 by choosing |γ1||\gamma_{1}| in the interval

ρ1Δn¯32<|γ1|<ρ1Δn¯12,Δ=arccosh|B|logρ1.\rho_{1}^{\Delta-\bar{n}-\frac{3}{2}}<|\gamma_{1}|<\rho_{1}^{-\Delta-\bar{n}-\frac{1}{2}}\,,\;\;\Delta=\frac{\mathop{\rm arccosh}\nolimits|B|}{\log\rho_{1}}\,. (47)

Additionally, the Darboux transformation can be used to construct a double KM solution according to the formulae provided in Appendix A. We remark that if two parameter sets {ρ1,γ1}\{\rho_{1},\gamma_{1}\} and {ρ2,γ2}\{\rho_{2},\gamma_{2}\} are chosen according to the regularity conditions (46) and (47) such that each set separately characterizes a well-behaved single KM solution, the resulting double KM solution is not guaranteed to remain regular (even with centers n¯1\bar{n}_{1} and n¯2\bar{n}_{2} chosen to be sufficiently separated). However, one can find combinations of parameters for which the double KM solution is well-behaved, examples of which are displayed in Fig. 7.

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Figure 7: (a) Double KM1 solution with r=2r=2 and z1z_{1} and z2z_{2} parametrized by (38), corresponding to ρ1=6\rho_{1}=6, γ1=104\gamma_{1}=10^{-4}, ρ2=3\rho_{2}=3, γ2=104\gamma_{2}=10^{4}. (b) Double KM2 solution with r=4r=4 and z1z_{1} and z2z_{2} parametrized by (37) with the positive sign, corresponding to ρ1=8\rho_{1}=8, γ1=104\gamma_{1}=10^{-4}, ρ2=12\rho_{2}=12, γ2=104\gamma_{2}=10^{4}. (c) Double KM1 solution with r=2r=2 and z1z_{1} and z2z_{2} parametrized by (38), corresponding to ρ1=2.2588611606273092\rho_{1}=2.2588611606273092, γ1=104\gamma_{1}=10^{-4}, ρ2=3.9647690662942265\rho_{2}=3.9647690662942265, γ2=104\gamma_{2}=10^{4}; chosen such that the period of the left wave is π/8\pi/8 and the period of the right wave is π/4\pi/4.

6 Instability & numerical blow-up

In this section, we study numerically and show respective results for a few representative cases of regular single KM breathers associated with Fig. 2. Specifically, we attempt herein to shed light on the spectral stability of KM breathers that are introduced in this work. In doing so, we obtain first the respective time-periodic yet numerically exact solution of Eq. (2) by using Newton’s method which is subsequently used in the variational equations towards deriving the monodromy matrix. The eigenvalues of the monodromy matrix are the Floquet multipliers which provide information about the stability of the pertinent structures, see [33] for the formulation of the stability analysis problem. Briefly, and as far as Newton’s method is concerned, time-periodic solutions of period Tb=π/Ω~1T_{b}=\pi/\tilde{\Omega}_{1}

Qn=m=kmkm𝒬n,me2imΩ~1τ,\displaystyle Q_{n}=\sum_{m=-k_{m}}^{k_{m}}{\cal Q}_{n,m}e^{2\mathrm{i}m\tilde{\Omega}_{1}\tau}, (48)

where 𝒬n,m{\cal Q}_{n,m} are the Fourier coefficients, and 2km+12k_{m}+1 are the total Fourier modes in time we consider. In this work, we use km=61k_{m}=61 and thus 123123 Fourier collocation points are used for the temporal discretization. Upon plugging Eq. (48) into Eq. (2) where periodic (in space) boundary conditions are imposed therein, we obtain a nonlinear algebraic system of equations for 𝒬n,m{\cal Q}_{n,m} that we solve with Newton’s method; see [33] for the formulation of the relevant root-finding problem and [12] for a recent yet relevant application of the method. We mention in passing that the initial guesses to the solver are provided directly by the exact solutions we aim to study, and Newton’s method converges in 1 iteration (within machine precision). However, we have noticed that the solver may need to perform more iterations, e.g., 3-4, to converge for the same number of Fourier collocation points employed. One such case is strongly reminiscent of Fig. 2(c) but with r=2r=2, κ=3\kappa=3, and c=6.48041c=6.48041 where the solver converged in 3 iterations (if km=81k_{m}=81, i.e., 163163 collocation points in time, the solver convergences in 1 iteration). There are also other cases, such as the one with r=4r=4, κ=8\kappa=8, and c=0.253c=0.253 where our nonlinear solver failed to converge entirely. This observation raises an important problem that merits a further yet separate investigation in developing suitable computational methods for identifying such periodic orbits. Regardless, and for the single KM solutions we present herein, we found that the use of 123123 collocation points in time together with a lattice of 100100 sites accurately resolves the time-translation mode 1+0i1+0\mathrm{i} within 10710810^{-7}-10^{-8} error.

Finally, we provide relevant dynamics of the KM solutions that are numerically obtained in order to explore the corresponding evolution of such states. For these direct numerical computations, we use the Burlisch-Stoer method [19] with 101410^{-14} relative and absolute errors for all time integrations (including those that are needed for the Floquet computations, i.e., variational problem). As a diagnostic in order to assess the accuracy of the dynamical results, we leverage the integrable structure of the AL model and, in particular, its bearing of an infinite number of associated conservation laws. The conserved quantities in the case of waveforms whose tails asymptotically vanish can be derived recursively using formulas (3.4.155) and (3.4.157) in [4], and simplified using the summation by parts formula (A.1.2). The conserved quantities for non-zero boundary conditions can be obtained by subtracting the boundary conditions to ensure all the series are convergent. Specifically, we have

Γ1=n=+{QnQn1Qo2},Γ¯1=n=+{Qn1QnQo2},\displaystyle\Gamma_{1}=\sum_{n=-\infty}^{+\infty}\left\{Q_{n}Q_{n-1}^{*}-Q_{o}^{2}\right\}\,,\qquad\bar{\Gamma}_{1}=\sum_{n=-\infty}^{+\infty}\left\{Q_{n-1}Q_{n}^{*}-Q_{o}^{2}\right\}, (49)
Γ2=n=+[QnQn2(1|Qn1|2)12(QnQn1)2Qo2+32Qo4],\displaystyle\Gamma_{2}=\sum_{n=-\infty}^{+\infty}\left[Q_{n}Q_{n-2}^{*}\left(1-|Q_{n-1}|^{2}\right)-\frac{1}{2}(Q_{n}Q_{n-1}^{*})^{2}-Q_{o}^{2}+\frac{3}{2}Q_{o}^{4}\right], (50)
Γ¯2=n=+[Qn2Qn(1|Qn1|2)12(Qn1Qn)2Qo2+32Qo4].\displaystyle\bar{\Gamma}_{2}=\sum_{n=-\infty}^{+\infty}\left[Q_{n-2}Q_{n}^{*}\left(1-|Q_{n-1}|^{2}\right)-\frac{1}{2}(Q_{n-1}Q_{n}^{*})^{2}-Q_{o}^{2}+\frac{3}{2}Q_{o}^{4}\right]. (51)

The IST also shows the following infinite product is conserved:

c=n=+|Qn|21Qo21.\displaystyle c_{\infty}=\prod_{n=-\infty}^{+\infty}\frac{|Q_{n}|^{2}-1}{Q_{o}^{2}-1}. (52)

Finally, from the expression of the Hamiltonian in the case of zero boundary conditions, once the nontrivial boundary conditions are subtracted out we obtain (cf. also [36]):

H=n=+{Qn(Qn+1+Qn1)2Qo2}+2n=+log|Qn|21Qo21.\displaystyle H=\sum_{n=-\infty}^{+\infty}\left\{Q_{n}^{*}\left(Q_{n+1}+Q_{n-1}\right)-2Q_{o}^{2}\right\}+2\sum_{n=-\infty}^{+\infty}\log\frac{|Q_{n}|^{2}-1}{Q_{o}^{2}-1}. (53)

with

H=Γ1+Γ¯1+2logc.H=\Gamma_{1}+\bar{\Gamma}_{1}+2\log c_{\infty}. (54)

It is worth pointing out that both the infinite product (52) and the related log series in (53) satisfy the necessary condition for convergence, since |Qn|Qo|Q_{n}|\to Q_{o} as n±n\to\pm\infty for both Qo<1Q_{o}<1 and Qo>1Q_{o}>1. In the case of zero boundary conditions, the defocusing AL lattice conserves the functional 𝒫=n=log(1|Qn|2)\mathcal{P}=\sum_{n=-\infty}^{\infty}\log(1-|Q_{n}|^{2}), and global existence is ensured if the initial condition satisfies Qn(0)<1||Q_{n}(0)||_{\infty}<1, but to the best of our knowledge the analog of this result has not yet been established in the case of nonzero boundary conditions even when 0<Qo<10<Q_{o}<1. For our exact solutions, we observe that when Qo>1Q_{o}>1, even though |Qn||Q_{n}| can dip below QoQ_{o} at some lattice sites, one has |Qn|>1|Q_{n}|>1 for all nn\in\mathbb{Z}. In this case, the terms in the infinite product (52) and the arguments of the logarithm in (53) are positive, and requiring QnQo1Q_{n}-Q_{o}\in\ell^{1} is sufficient to guarantee the convergence of both (52) and (53). It is interesting to add here that we have observed that in the course of the numerical evolution dynamics of such unstable solutions, round-off error may lead, through the resulting destabilization, to the indefinite growth of the modulus of particular nodes. As this happens, we have noticed that (pairwise) some sites drop below QoQ_{o} and indeed approach unit modulus, in a way that can be seen to conserve both the infinite product of (52) and the energy of (53). How this collapse dynamics manifests itself and its bearing on the AL lattice conservation laws are clearly topics meriting further investigation.

We now turn our focus on Fig. 8 which presents numerical results on the existence, stability and spatio-temporal dynamics in panels (a)-(d), (e)-(h), and (i)-(l), respectively. Those are complemented by the panels (m)-(p) which depict the relative error (with respect to t=0t=0) of the conserved quantities given by Eqs. (49), (51), (52), and (54), respectively (see the legend in panel (m)) all as a function of time. Moreover, the first, second, third, and fourth rows of Fig. 8 connect with the KM breathers of Figs. 2(e), (b), (c), and (d), respectively. The panels (a)-(d) showcase the spatial dependence of the amplitude QnQ_{n} of the numerically obtained solution (with blue open circles) against the respective exact solution (with red stars), see the legend in panel (a). Besides the expected matching between numerically exact and analytical solutions, we report that the ones shown in panels (a) and (c) of Fig. 8 bear two-site excitations, i.e., bond centered waveforms, whereas the ones of panels (b) and (d) correspond to site-centered solutions.

The respective results of the Floquet spectra of the solutions shown in (a)-(d) are presented in panels (e)-(h) where the Floquet multipliers λ=λr+iλi\lambda=\lambda_{r}+\mathrm{i}\lambda_{i} are depicted with blue filled circles. To understand the spectrum of the KM breathers, we complement the relevant spectra by including in each panel the Floquet multipliers (see, the legend in panel (e)) of the respective constant background (CW) solution in panels (e)-(h) with red open circles (see, the MI dispersion relation in [33], cf. Eqs. (10) and (14) therein with g=1g=1 and C=1C=-1). In all cases that we briefly report herein, all KM breathers are deemed spectrally unstable due to the presence of a band of real Floquet multipliers (i.e., with λi=0\lambda_{i}=0) where |λ|>1|\lambda|>1. However, the instabilities identified in these panels emanate from the instability of the background, that is, the CW is modulationally unstable here since the background amplitude in all cases we consider is greater than 11, i.e., Q0>1Q_{0}>1 [cf. [15]]. Indeed, executing the relevant computations in larger lattices, we have verified that the bands of associated instabilities become more dense as is expected due to the excitation of additional unstable wavenumbers therein. We find no additional unstable modes getting generated by the mounting of KM breathers atop the CW waveform at least for the cases we have studied numerically. This is in line with earlier results in both continuum [16] and discrete [33] problems of the discrete nonlinear Schrödinger type. It should be mentioned in passing that the breather itself slightly perturbs the Floquet multipliers of the CW solution, see, indicatively, panels (g) and (h). More importantly, we find that the site-centered solutions of panels (b) and (d) as well as the bond-centered one of panel (a) are less unstable compared to the bond-centered solution of panel (c) which itself involves a maximal growth rate of 𝒪(107)\mathcal{O}\left(10^{7}\right) and which is accordingly expected to be manifested over very short time scales. The stability trait of the KM breathers is reflected in the spatio-temporal evolution of the amplitude |Qn(τ)||Q_{n}(\tau)| in panels in (i)-(l). Here, we use the numerically exact solution as an initial conditions, and advance Eq. (2) forward in time until the integrator breaks down due to the (numerically induced) blow-up of the solutions.

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Figure 8: Summary of numerical results associated with the KM solutions of Fig. 2(e), (b), (c), and (d) shown here in the first, second, third, and fourth rows, respectively.  The panels (a)-(d) show the spatial distribution of numerically exact KM breathers with blue open circles (connected by solid line as a guide to the eye). For comparison, the exact solution is shown too with red stars (see, the legend in panel (a)). As expected, in all cases, the two are practically identical. The spectral stability results are summarized in panels (e)-(h) where the Floquet multipliers λ=λr+iλi\lambda=\lambda_{r}+\mathrm{i}\lambda_{i} are shown with blue filled circles against the MI prediction associated with the uniform background state shown with red open circles. Moreover, the spatio-temporal evolution of Qn(τ)Q_{n}(\tau) is depicted in (i)-(l) where the respective conserved quantities (in a semi-logarithmic scale) are shown in panels (m)-(p); see the legend and Eqs. (49), (51), (52), and (54), as well as the associated discussion in the text.

In line with our spectral stability calculations shown in panels (e)-(h), we observe that the waveforms of panels (i), (j), and (l) do breathe in time, and in a staggered or beating fashion without changing their structural characteristics until modulational instability (MI) gets triggered due to perturbations. For example, see the waveform shown in Fig. 8(i) close to the end of the time window, but also the one of Fig. 8(k) where MI gets manifested itself more quickly given the very large instability growth rate, causing the solution to not even return back after one period of time integration.

The perturbations mentioned above stem from not only round-off and local truncation errors of the integrator, but also from the error that gets introduced by the truncation of Eq. (48), i.e., in the computation of the initial condition as a fixed-point solution. For reference, we report the integration times [0,tf][0,t_{f}] of the respective cases with (i) tf=22.143Tb1.0322t_{f}=22.143T_{b}\approx 1.0322, (j) tf=18.4Tb9.7596t_{f}=18.4T_{b}\approx 9.7596, (k) tf=Tb1.6265t_{f}=T_{b}\approx 1.6265, and (l) tf=13Tb3.39720t_{f}=13T_{b}\approx 3.39720, respectively. It should be noted that the spatio-temporal dynamics of |Qn(τ)||Q_{n}(\tau)| shown in these panels are up to times where the solution has not blown up yet, i.e., up to times slightly before blow-up where the structures can still be visible. Despite the evolution of the KM breathers towards blow-up, we report that the conserved quantities introduced in Eqs. (49), (51), (52), and (54) are very well preserved with relative errors 𝒪(109)𝒪(1016)\mathcal{O}(10^{-9})-\mathcal{O}(10^{-16}).This happens even very close to blow-up times as this shown in panels (m)-(p) where the terminal times therein are up to and including those when the integrator breaks down. This is an additional indication of the fidelity of our numerical computations discussed in this section.

We speculate that what is happening here is that the relevant solutions are very proximal to ones featuring collapse dynamics, as discussed in the previous sections, given the relevant variation of parameters such as cc. The dynamical manifestation of the waveforms’ MI (often with a very large growth rate) due to its background rapidly leads to growth and opens a pathway towards exploring these proximal collapse-prone dynamical features of the model. Understanding these pathways towards collapse is naturally an interesting direction for further exploration. This is especially so since it’s worthwhile to bear in mind that the exact analytical solutions constructed herein have been designed to feature no collapse, and it is only the quite small perturbations of roundoff, integration local truncation error, and inexactness due to a finite mode truncation that lead to the observed blowup.

7 Concluding remarks

In the present work we have examined the existence (including the analytical form), stability and dynamics of an important, periodic-in-time class of solutions of the defocusing Ablowitz-Ladik lattice on an arbitrarily large background which are discrete analogs of the KM breathers of the focusing NLS equation. Specifically, we derived conditions on the background and on the spectral parameters that guarantee the exact KM solution to be non-singular on the lattice for all times. Furthermore, a novel KM-type breather solution is presented which is also regular on the lattice under suitable conditions. Furthermore, we employed Darboux transformations to obtain a multi-KM breather solution, and showed that parameters choices exist for which the newly obtained double KM breather to be regular on the lattice. Finally, we presented numerical results on the stability and spatio-temporal dynamics of the single KM breathers. The stability analysis manifested that these states were modulationally unstable due to the modulational instability of the background on top of which they existed, with their Floquet multipliers suitably modified (due to the nonlinear nature of the waveform), yet without novel instabilities introduced (similarly to what was found for the continuum NLS problem in [16]). Another important feature of the numerical computations was that small perturbations (introduced by roundoff and local truncation errors, or by the approximate nature of our numerical solution) led to the finite time blowup of the KM structures. The preservation of the model’s conservation laws strongly suggested that this feature was not a numerical artifact, but rather a real feature which merits further examination.

In a forthcoming work, a more systematic stability analysis will be carried out together with homotopic continuations of solutions presented herein towards the discrete nonlinear Schrödinger (DNLS) equation, and in the same spirit as in [33]. This may provide significant insights towards the existence of corresponding KM waveforms in the more experimentally relevant (within nonlinear optics) model of the discrete NLS equation [22]. Another interesting direction is to continue the waveforms (especially the novel ones discovered herein) towards smaller frequencies in order to acquire structures closer to the rogue waves that are known to exist in the AL model (see, e.g., [9]). Further such studies of rogue waves in both defocusing and focusing AL lattices and their non-integrable analogs are currently in progress and will be reported in future publications.

Acknowledgments

This work has been supported by the U.S. National Science Foundation under Grants No. DMS-2204782 (EGC), and DMS-2110030 and DMS-2204702 (PGK), and DMS-2406626 (BP). The authors also acknowledge the Isaac Newton Institute for Mathematical Sciences, Cambridge, UK, for support and hospitality during the satellite programme “Emergent phenomena in nonlinear dispersive waves” (supported by EPSRC grant EP/R014604/1), where work on this paper was undertaken. Finally, we would also like to thank Gino Biondini for his suggestions with one of the figures, and the anonymous referee for their useful comments which helped us improve the work.

Appendix A Construction of the Darboux matrix

The DM in [15] is assumed to be of the form

Dn[0,J](z,τ)=(zJ+l=1Jan(J2l)zJ2ll=1Jbn(J2l+1)zJ2l+1l=1J(bn(J2l+1))zJ+2l1zJ+l=1J(an(J2l))zJ+2l)D_{n}^{[0,J]}(z,\tau)=\begin{pmatrix}z^{J}+\sum_{l=1}^{J}a_{n}^{(J-2l)}z^{J-2l}&\sum_{l=1}^{J}b_{n}^{(J-2l+1)}z^{J-2l+1}\\ \sum_{l=1}^{J}\left(b_{n}^{(J-2l+1)}\right)^{*}z^{-J+2l-1}&z^{-J}+\sum_{l=1}^{J}\left(a_{n}^{(J-2l)}\right)^{*}z^{-J+2l}\end{pmatrix} (55)

where the symmetry has already been taken into account. The unknown quantities in the DM are then determined by requiring that the DM is singular at the discrete eigenvalues ±zj,±1/zj\pm z_{j},\pm 1/z_{j}^{*}, with

Dn[0,J](zj,τ)ϕn[0](zj,τ)=γjDn[0,J](zj,τ)ψn[0](zj,τ),D_{n}^{[0,J]}(z_{j},\tau)\phi_{n}^{[0]}(z_{j},\tau)=\gamma_{j}D_{n}^{[0,J]}(z_{j},\tau)\psi_{n}^{[0]}(z_{j},\tau)\,, (56)

where Ψn[0](z,τ)=(ϕn[0](z,τ),ψn[0](z,τ))\Psi_{n}^{[0]}(z,\tau)=\left(\phi_{n}^{[0]}(z,\tau),\psi_{n}^{[0]}(z,\tau)\right) is a fundamental analytic matrix solution of the Lax pair corresponding to the potential Qn[0](τ)Q_{n}^{[0]}(\tau), and γj\gamma_{j} are the proportionality constants that relate the column vectors at the discrete eigenvalue. Inserting the ansatz (55) into (56), one obtains

(zjJ+l=1Jan(J2l)zjJ2l)+(zjJ+l=1Jbn(J2l+1)zjJ2l+1)rj=0,\displaystyle\left(z_{j}^{J}+\sum_{l=1}^{J}a_{n}^{(J-2l)}z_{j}^{J-2l}\right)+\left(z_{j}^{J}+\sum_{l=1}^{J}b_{n}^{(J-2l+1)}z_{j}^{J-2l+1}\right)r_{j}=0, (57)
(1(zj)Jl=1Jan(J2l)(zj)J2l)+(l=1Jbn(J2l+1)(zj)J2l+1)1rj=0,\displaystyle\left(\frac{1}{(z_{j}^{*})^{J}}\sum_{l=1}^{J}\frac{a_{n}^{(J-2l)}}{(z_{j}^{*})^{J-2l}}\right)+\left(\sum_{l=1}^{J}\frac{b_{n}^{(J-2l+1)}}{(z_{j}^{*})^{J-2l+1}}\right)\frac{1}{r_{j}^{*}}=0, (58)

where

rj=ϕn[0],2(zj)γjψn[0],2(zj)ϕn[0],1(zj)γjψn[0],1(zj)r_{j}=\frac{\phi_{n}^{[0],2}(z_{j})-\gamma_{j}\psi_{n}^{[0],2}(z_{j})}{\phi_{n}^{[0],1}(z_{j})-\gamma_{j}\psi_{n}^{[0],1}(z_{j})}

and the superscript denotes the corresponding component of the vectors ϕn[0](zj,τ)\phi_{n}^{[0]}(z_{j},\tau), ψn[0](zj,τ)\psi_{n}^{[0]}(z_{j},\tau). If the number of singular points zjz_{j} is equal to the order JJ of the Darboux transformation, the above equations for j=1,,Jj=1,\dots,J define an linear system of 2J2J equations for the 2J2J unknowns an(l),bn(l)a_{n}^{(l)},b_{n}^{(l)} for l=1,,Jl=1,\dots,J. Finally, the solution Qn[J](τ)Q_{n}^{[J]}(\tau) can be obtained from Qn[0](τ)Q_{n}^{[0]}(\tau) using the first of (32), yielding

Qn[0,J](τ)=Qn[0](τ)an+1(J)(τ)+bn+1(J+1)(τ).Q_{n}^{[0,J]}(\tau)=Q_{n}^{[0]}(\tau)a_{n+1}^{(-J)}(\tau)+b_{n+1}^{(-J+1)}(\tau). (59)

The solutions of the above equations for the simplest cases, J=1J=1 and J=2J=2, are provided in [15]. Specifically, if J=1J=1:

an(1)(τ)=z1|r1|2/z1|r1|2z11/z1,bn(0)(τ)=r1|r1|2z11/z1(|z1|21/|z1|2),\displaystyle a_{n}^{(-1)}(\tau)=\frac{z_{1}-|r_{1}|^{2}/z_{1}^{*}}{|r_{1}|^{2}z_{1}^{*}-1/z_{1}}\,,\qquad b_{n}^{(0)}(\tau)=-\frac{r_{1}^{*}}{|r_{1}|^{2}z_{1}^{*}-1/z_{1}}\left(|z_{1}|^{2}-1/|z_{1}|^{2}\right), (60)

yielding

Qn[0,1](τ)=Qn[0](τ)an+1(1)(τ)+bn+1(0)(τ).Q_{n}^{[0,1]}(\tau)=Q_{n}^{[0]}(\tau)a_{n+1}^{(-1)}(\tau)+b_{n+1}^{(0)}(\tau)\,. (61)

Similarly, when J=2J=2 the DM elements are given by:

an(2)(τ)=Δa(2)Δ(2),bn(1)(τ)=Δb(2)Δ(2),a_{n}^{(-2)}(\tau)=\frac{\Delta_{a}^{(2)}}{\Delta^{(2)}}\,,\qquad b_{n}^{(-1)}(\tau)=\frac{\Delta_{b}^{(2)}}{\Delta^{(2)}}\,, (62)

where

Δ(2)=det(11/z12r1z1r1/z111/z22r2z2r2/z21(z1)21/(r1z1)z1/r11(z2)21/(r2z2)z2/r2)\Delta^{(2)}=\det\begin{pmatrix}1&1/z_{1}^{2}&r_{1}z_{1}&r_{1}/z_{1}\\ 1&1/z_{2}^{2}&r_{2}z_{2}&r_{2}/z_{2}\\ 1&(z_{1}^{*})^{2}&1/(r_{1}z_{1})^{*}&z_{1}^{*}/r_{1}^{*}\\ 1&(z_{2}^{*})^{2}&1/(r_{2}z_{2})^{*}&z_{2}^{*}/r_{2}^{*}\end{pmatrix}

Δa(2)\Delta_{a}^{(2)}, Δb(2)\Delta_{b}^{(2)} are obtained replacing the second and forth column, respectively, with the vector

(z12,z22,(z1)2,(z2)2)T,(-z_{1}^{2},-z_{2}^{2},-(z_{1}^{*})^{-2},-(z_{2}^{*})^{-2})^{T},

and the potential is reconstructed by means of Eq. (59), i.e.

Qn[0,2](τ)=Qn[0](τ)an+1(2)(τ)+bn+1(1)(τ).Q_{n}^{[0,2]}(\tau)=Q_{n}^{[0]}(\tau)a_{n+1}^{(-2)}(\tau)+b_{n+1}^{(-1)}(\tau)\,. (63)

Appendix B Errata for Ref. [29]

  1. 1.

    The first equation without number in Remark 1 should read

    |λ|21(|ζ|2+1)[|ζ|2+ir(ζζ)1]0|ζir|2Qo2|\lambda|^{2}\leq 1\quad\Leftrightarrow\quad(|\zeta|^{2}+1)\left[|\zeta|^{2}+ir(\zeta-\zeta^{*})-1\right]\leq 0\quad\Leftrightarrow\quad|\zeta-ir|^{2}\leq Q_{o}^{2}
  2. 2.

    The expression between Eq. (32b) and Eq. (33a) should read

    (Mn(τ,ζ)M¯n(τ,ζ))=(N¯n(τ,ζ)Nn(τ,ζ))Λneiσ3Ω(ζ)τT~(ζ)eiσ3Ω(ζ)τΛn(M_{n}(\tau,\zeta)\quad\bar{M}_{n}(\tau,\zeta))=(\bar{N}_{n}(\tau,\zeta)\quad N_{n}(\tau,\zeta))\Lambda^{n}e^{i\sigma_{3}\Omega{(\zeta)}\tau}\tilde{T}(\zeta)e^{-i\sigma_{3}\Omega{(\zeta)}\tau}\Lambda^{-n} (64)

    where T~=A(λ(ζ))T(z(ζ))A1(λ(ζ))\tilde{T}=A(\lambda(\zeta))T(z(\zeta))A^{-1}(\lambda(\zeta)) is defined as in [29] as

  3. 3.

    As a result, Eqs. (38c) and (38d) should respectively be

    β(ζ)=Q02Δn(τ)ir(ζ+1/ζ2ir)[ζ(ζir)irζ1]ne2iΩ(ζ)τWr(Mn(τ,ζ),N¯n(τ,ζ))\beta(\zeta)=-\dfrac{Q_{0}^{2}\Delta_{n}(\tau)}{ir(\zeta+1/\zeta-2ir)}\left[\dfrac{\zeta(\zeta-ir)}{ir\zeta-1}\right]^{n}e^{2i\Omega(\zeta)\tau}Wr(M_{n}(\tau,\zeta),\bar{N}_{n}(\tau,\zeta)) (65)
    β¯(ζ)=Q02Δn(τ)ir(ζ+1/ζ2ir)[ζ(ζir)irζ1]ne2iΩ(ζ)τWr(M¯n(τ,ζ),Nn(τ,ζ))\bar{\beta}(\zeta)=\dfrac{Q_{0}^{2}\Delta_{n}(\tau)}{ir(\zeta+1/\zeta-2ir)}\left[\dfrac{\zeta(\zeta-ir)}{ir\zeta-1}\right]^{-n}e^{-2i\Omega(\zeta)\tau}Wr(\bar{M}_{n}(\tau,\zeta),N_{n}(\tau,\zeta)) (66)
  4. 4.

    There is a typo in a sign in the exponents in Eqs. (63a) and (63b). The correct expression for (63a) and (63b) is respectively shown below

    Resζ=ζ¯kM¯n(τ,ζ)a¯(ζ)\displaystyle Res_{\zeta=\bar{\zeta}_{k}}\frac{\bar{M}_{n}(\tau,\zeta)}{\bar{a}(\zeta)} =C¯kλ2n(ζ¯k)e2iΩ(ζ¯k)τN¯n(τ,ζ¯k),C¯k=b¯kλ(ζ¯k)a¯(ζ¯k)\displaystyle=\bar{C}_{k}\lambda^{2n}(\bar{\zeta}_{k})e^{2i\Omega(\bar{\zeta}_{k})\tau}\bar{N}_{n}(\tau,\bar{\zeta}_{k}),\qquad\bar{C}_{k}=\frac{\bar{b}_{k}}{\lambda(\bar{\zeta}_{k})\bar{a}^{\prime}(\bar{\zeta}_{k})} (67)
    Resζ=ζkMn(τ,ζ)a(ζ)\displaystyle Res_{\zeta={\zeta}_{k}}\frac{{M}_{n}(\tau,\zeta)}{{a}(\zeta)} =Ckλ2n(ζk)e2iΩ(ζk)τNn(τ,ζk),C¯k=bkλ(ζk)a(ζk)\displaystyle={C}_{k}\lambda^{-2n}({\zeta}_{k})e^{-2i\Omega({\zeta}_{k})\tau}{N}_{n}(\tau,{\zeta}_{k}),\qquad\bar{C}_{k}=\frac{{b}_{k}\lambda({\zeta}_{k})}{{a}^{\prime}({\zeta}_{k})} (68)
  5. 5.

    Equation (63b) is used to obtain equations (68a) and so it contains a typo in a sign in the exponent. The correct expression for (68a) is

    N¯n(τ,ζ)=\displaystyle\bar{N}_{n}(\tau,\zeta)= (1/Δn(τ)(ζir)/Q+)+k=12J(ζir)(ζkir)(ζζk)Ckλ2n(ζk)e2iΩ(ζk)τNn(τ,ζk)\displaystyle\begin{pmatrix}1/\Delta_{n}(\tau)\\ (\zeta-ir)/Q_{+}\end{pmatrix}+\sum_{k=1}^{2J}\frac{(\zeta-ir)}{(\zeta_{k}-ir)(\zeta-\zeta_{k})}{C}_{k}\lambda^{-2n}({\zeta}_{k})e^{-2i\Omega({\zeta}_{k})\tau}{N}_{n}(\tau,{\zeta}_{k})
    12πiwΣ(ζir)(wζ)(wir)Ckλ2n(w)e2iΩ(w)τNn(τ,w)ρ(w)𝑑w\displaystyle-\frac{1}{2\pi i}\int_{w\in\Sigma}\frac{(\zeta-ir)}{(w-\zeta)(w-ir)}{C}_{k}\lambda^{-2n}({w})e^{-2i\Omega({w})\tau}{N}_{n}(\tau,w){\rho}(w)dw (69)
  6. 6.

    Similarly, Equation (63a) is used to obtain equations (68b), whose correct expression is

    Nn(τ,ζ)=\displaystyle{N}_{n}(\tau,\zeta)= ((1/ζir)/Q+1/Δn(τ))+k=12J(ζ+i/r)(ζ¯k+i/r)(ζζ¯k)C¯kλ2n(ζ¯k)e2iΩ(ζ¯k)τN¯n(τ,ζ¯k)\displaystyle\begin{pmatrix}(1/\zeta-ir)/Q_{+}^{*}\\ 1/\Delta_{n}(\tau)\end{pmatrix}+\sum_{k=1}^{2J}\frac{(\zeta+i/r)}{(\bar{\zeta}_{k}+i/r)(\zeta-\bar{\zeta}_{k})}\bar{C}_{k}\lambda^{2n}(\bar{\zeta}_{k})e^{2i\Omega(\bar{\zeta}_{k})\tau}\bar{N}_{n}(\tau,\bar{\zeta}_{k})
    +12πiwΣ(ζ+i/r)(wζ)(w+i/r)λ2n(w)e2iΩ(w)τN¯n(τ,w)ρ¯(w)𝑑w\displaystyle+\frac{1}{2\pi i}\int_{w\in\Sigma}\frac{(\zeta+i/r)}{(w-\zeta)(w+i/r)}\lambda^{2n}({w})e^{2i\Omega({w})\tau}\bar{N}_{n}(\tau,w)\bar{\rho}(w)dw (70)
  7. 7.

    Following the correction in (68b), Equations (69a) and (69b) are respectively corrected as

    1Δn(τ)=\displaystyle\frac{1}{\Delta_{n}(\tau)}= 1+Q+k=12J11irζ¯kC¯kλ2n(ζ¯k)e2iΩ(ζ¯k)τN¯n(1)(τ,ζ¯k)\displaystyle 1+Q_{+}^{*}\sum_{k=1}^{2J}\frac{1}{1-ir\bar{\zeta}_{k}}\bar{C}_{k}\lambda^{2n}(\bar{\zeta}_{k})e^{2i\Omega(\bar{\zeta}_{k})\tau}\bar{N}_{n}^{(1)}(\tau,\bar{\zeta}_{k})
    Q+2πiwΣ11irwλ2n(w)e2iΩ(w)τN¯n(1)(τ,w)ρ¯(w)𝑑w\displaystyle-\frac{Q_{+}^{*}}{2\pi i}\int_{w\in\Sigma}\frac{1}{1-irw}\lambda^{2n}({w})e^{2i\Omega({w})\tau}\bar{N}_{n}^{(1)}(\tau,w)\bar{\rho}(w)dw (71)
    Qn(τ)Δn(τ)=\displaystyle\frac{Q^{*}_{n}(\tau)}{\Delta_{n}(\tau)}= Q(τ)Δn(τ)+Q+k=12J1ζ¯k+i/rC¯kλ2n(ζ¯k)e2iΩ(ζ¯k)τN¯n(2)(τ,ζ¯k)\displaystyle\frac{Q^{*}(\tau)}{\Delta_{n}(\tau)}+Q_{+}^{*}\sum_{k=1}^{2J}\frac{1}{\bar{\zeta}_{k}+i/r}\bar{C}_{k}\lambda^{2n}(\bar{\zeta}_{k})e^{2i\Omega(\bar{\zeta}_{k})\tau}\bar{N}_{n}^{(2)}(\tau,\bar{\zeta}_{k})
    Q+2πiwΣ1w+i/rλ2n(w)e2iΩ(w)τN¯n(2)(τ,w)ρ¯(w)𝑑w\displaystyle-\frac{Q_{+}^{*}}{2\pi i}\int_{w\in\Sigma}\frac{1}{w+i/r}\lambda^{2n}({w})e^{2i\Omega({w})\tau}\bar{N}_{n}^{(2)}(\tau,w)\bar{\rho}(w)dw (72)
  8. 8.

    Consequently, equation (70) is corrected as

    Qn(τ)=Q+(1+k=12J(C¯kλ2n(ζ¯k)e2iΩ(ζ¯k)τN¯n(2)(τ,ζ¯k))/(ζ¯k+i/r)1+Q+k=12J(C¯kλ2n(ζ¯k)e2iΩ(ζ¯k)τN¯n(1)(τ,ζ¯k))/(1irζ¯k))Q^{*}_{n}(\tau)=Q^{*}_{+}\left(1+\frac{\sum_{k=1}^{2J}(\bar{C}_{k}\lambda^{2n}(\bar{\zeta}_{k})e^{2i\Omega(\bar{\zeta}_{k})\tau}\bar{N}_{n}^{(2)}(\tau,\bar{\zeta}_{k}))/({\bar{\zeta}_{k}+i/r})}{1+Q_{+}^{*}\sum_{k=1}^{2J}(\bar{C}_{k}\lambda^{2n}(\bar{\zeta}_{k})e^{2i\Omega(\bar{\zeta}_{k})\tau}\bar{N}_{n}^{(1)}(\tau,\bar{\zeta}_{k}))/({1-ir\bar{\zeta}_{k}})}\right) (73)
  9. 9.

    Eq. (87) should read

    ξ=nlogρ+2(ImΩ¯1)τ,η=nϕ+2(ReΩ¯1)τ.\xi=n\log\rho+2(\mathop{\rm Im}\nolimits\bar{\Omega}_{1})\tau\,,\qquad\eta=n\phi+2(\mathop{\rm Re}\nolimits\bar{\Omega}_{1})\tau\,. (74)
  10. 10.

    Equation (92) should read

    Ω¯1=iω,ω=2rQ02(Q0+rsinα)cosα2Q0(Q0+rsinα)1.\bar{\Omega}_{1}=i\omega,\quad\quad\omega=2rQ_{0}^{2}\frac{(Q_{0}+r\sin\alpha)\cos\alpha}{2Q_{0}(Q_{0}+r\sin\alpha)-1}. (75)

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