Optics Communications 249 (2005) 117–128 www.elsevier.com/locate/optcom Coupled periodic waves with opposite dispersions in a nonlinear optical fiber S.C. Tsang a, K. Nakkeeran b b,* , Boris A. Malomed c, K.W. Chow a a Department of Mechanical Engineering, University of Hong Kong, Pokfulam Road, Hong Kong Photonics Research Center, Department of Electronic and Information Engineering, The Hong Kong Polytechnic University, Hung Hom, Kowloon, Hong Kong c Department of Interdisciplinary Studies, School of Electrical Engineering, Faculty of Engineering, Tel Aviv University, Tel Aviv 69978, Israel Received 13 September 2004; received in revised form 17 December 2004; accepted 20 December 2004 Abstract Using the HirotaÕs method and elliptic h-functions, we obtain three families of exact periodic (cnoidal) wave solutions for two nonlinear Schrödinger (NLS) equations coupled by XPM (cross-phase-modulation) terms, with a ratio r of the XPM and SPM (self-phase-modulation) coefficients. Unlike the previous works, we obtain the solutions for the case when the coefficients of the group-velocity-dispersion (GVD) in the coupled equations have opposite signs. In the limit of the infinite period, the solutions with r > 1 carry over into inverted bound states of bright and dark solitons in the normal- and anomalous-GVD modes (known as ‘‘symbiotic solitons’’), while the infinite-period solution with r < 1 is an uninverted bound state (also an unstable one). The case of r = 2 is of direct interest to fiber-optic telecommunications, as it corresponds to a scheme with a pulse stream in an anomalous-GVD payload channel stabilized by a concomitant strong periodic signal in a mate normal-GVD channel. The case of arbitrary r may be implemented in a dual-core waveguide. To understand the stability of the coupled waves, we first analytically explore the modulational stability of CW (constant-amplitude) solutions, concluding that they may be completely stable for r P 1, provided that the absolute value of the GVD coefficient is smaller in the anomalous-GVD mode than in the normal-GVD one, and certain auxiliary conditions on the amplitudes are met. The stability of the exact cnoidal-wave solutions is tested in direct simulations. We infer that, while, strictly speaking, in the practically significant case of r = 2 all the solutions are unstable, in many cases the instability may be strongly attenuated, rendering the above-mentioned paired channels scheme usable. In particular, the instability is milder for a smaller period of the wave pattern, and/or if the anomalous * Corresponding author. Tel.: +852 2766 6197; fax: +852 2362 8439. E-mail addresses: [email protected] (K. Nakkeeran), [email protected] (B.A. Malomed), [email protected] (K.W. Chow). 0030-4018/$ - see front matter Ó 2004 Elsevier B.V. All rights reserved. doi:10.1016/j.optcom.2004.12.042 118 S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 GVD is weaker than the normal GVD in the mate channel. When the instability sets in, it first initiates quasi-reversible modulations, and only at a later stage the wave pattern decays into a ‘‘turbulent’’ state. Ó 2004 Elsevier B.V. All rights reserved. PACS: 42.81.Dp; 42.65.Tg; 05.45.Yv Keywords: Optical fiber; Coupled nonlinear Schrödinger (NLS) equations; Periodic solutions; Hirota method 1. Introduction Exact solutions to the nonlinear Schrödinger (NLS) equation, and coupled systems of such equations, in the form of periodic arrays of pulses, which are frequently called ‘‘cnoidal waves’’ (because they are based on elliptic functions like cn), play an important role in the analysis of the data transmission in fiber-optic telecommunications links. It has been demonstrated, theoretically and experimentally, that such arrays may be created using the modulational instability of the continuous-wave (CW) signal [1–3], or from a dual-frequency pump [4,5], or directly (without the use of a CW input) by a high-repetition-rate pulse-generating fiber-ring laser (see, e.g., [6]). Search for exact solutions to coupled (generally speaking, nonintegrable) systems of NLS equations is also a mathematical problem of considerable interest in its own right [7–11]. A crucially important parameter of a datatransmitting channel in the optical fiber is its group-velocity-dispersion (GVD) coefficient, which depends on the carrier wavelength k [12,13]. In particular, in the dispersion-shifted fiber, the transparency window (which is centered at k = 1540 nm in all silica fibers) includes a zero-dispersion point (ZDP) k0 (in fact, k0 in the dispersion-shifted fiber is very close to 1540 nm), at which the GVD coefficient changes its sign from positive (normal GVD) at k < k0 to negative (anomalous GVD) at k > k0 (in fibers of other types, the ZDP is shifted to smaller values of k, usually falling between 1300 and 1500 nm). The negative-GVD region, k > k0, is employed for the data transmission in the returnto-zero (RZ), or quasi-soliton, format, in which a bit of data is carried by an isolated light pulse (with the zero field between them, hence the term RZ). In this case, which is of major importance to the applications [12,13], the bandpass in the normal-GVD region remains idle, as normal GVD cannot support quasi-soliton pulses in nonlinear optical fibers. In Ref. [14] it was proposed to employ the normal-GVD band, k < k0, for service channels, which carry strictly periodic signals. Such a signal cannot transmit any information; instead, it is intended to stabilize the concomitant array of RZ pulses in the payload channels set at k > k0. In the usual on-off realization of the binary code with the RZ signals, the most important stability requirement is to prevent the pulse from leaving a prescribed temporal slot (which would compromise ‘‘ons’’ and ‘‘offs’’). A trend of the pulse to jitter, i.e., random walk off the prescribed temporal position, is due to its interaction with the optical noise created by amplifiers (the Gordon–Haus effect), as well as the nonlinearity-mediated interaction of the pulse with adjacent ones in its own channel, and collisions with pulses belonging to channels carried by other wavelengths, in the wavelength-division-multiplexed (WDM) regime [15]. Suppression of the random walk is thus the most important condition securing the use of the fiber-optic links for long-haul telecommunications in the quasi-soliton regime. A new approach proposed for this purpose in Ref. [14] was based on the fact that the idle channel servicing its payload mate may be chosen so that both have equal group velocities (this is possible just because both channels are chosen on the opposite sides of the ZDP), hence the pulses in the latter channel must be immobile relative to the periodic signal in the support channel. Further, if the periodic signal is stable by itself and strong enough, it induces, through the XPM (cross-phase-modulation) nonlinear interaction, an effective potential acting on the pulse in the payload channel. Accordingly, the pulse tends to be trapped in a local well belonging to the periodic potential. This should help one S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 to suppress the pulseÕs random walk, provided that the trapping potential well is deep enough. In fact, this stabilization scheme may turn out to be simpler and more efficient than other known ones (such as the use of guiding bandpass filters [12,15]). Besides the applications, a possibility of direct experimental observation of stabilized cnoidal waves in the anomalous-GVD channel, as suggested by the results reported in this work, is a physically interesting result in its own right. An important circumstance which makes the use of the proposed scheme relevant is that the cnoidal wave in the normal-GVD NLS equation may indeed be dynamically stable, unlike the anomalous-GVD one [16,17], hence it can be employed as a support structure (the stability of cnoidalwave solutions in the single-channel models with various nonlinearities was recently reviewed in [18], and a relevant issue of the cnoidal-wave stability in the dispersion-management scheme was considered in Ref. [19]). The same concept of pairing a payload channel with an idle one carrying a periodic support structure may, in principle, be realized in terms of two waves with one wavelength and orthogonal polarizations. In this context, periodic coupled-cnoidalwave solutions were studied in Ref. [11]. However, the realization based on the pair of different wavelengths with equal group velocities, taken on the opposite sides of the ZDP, is much more practical, therefore in the present work we chiefly focus on the latter case. The actual difference between the two models is in the size of the XPM/SPM ratio r, see Eqs. (1) and (2) below: it is 2/3 for the orthogonal linear polarizations, and 2 for the different carrier wavelengths (or orthogonal circular polarizations). In fact, any value of r may be realized not in ordinary fibers, but rather in a dual-core waveguide with different carrier wavelengths in the two cores: obviously, r depends on the proximity between them. In particular, a promising medium to realize such a structure is a photonic-crystal fiber, with two parallel holes made in it (fabrication of such a system has already been reported [20]). As it was already mentioned, a strictly periodic signal in the payload channel cannot trans- 119 mit information. Nevertheless, the promising application outlined above makes it a relevant problem to find the broadest possible family of exact solutions for coupled periodic (cnoidal) waves in the XPM-coupled NLS equations describing the pair of the payload and service channels, with opposite signs of the GVD coefficients in them, and to test stability of such solutions. This problem, which is the subject of the present work, is practically important, as it helps to understand whether the scheme of the stabilization of the payload channel by the concomitant periodic signal in the service channel is itself completely stable. On the other hand, this problem is also novel in terms of the mathematical analysis of the coupled NLS equations, as all the previously reported families of exact periodic solutions were only found for systems of equations with the equal signs of the GVD coefficients. In Section 2 of this paper, we produce three families of such exact solutions in the system with opposite signs of the GVD in the XPMcoupled NLS equations. Two families are found for r > 1, and one for r < 1. In Section 3, we address stability of the solutions. To get a general idea of the stability in this type of the model, we first consider the modulational stability of CW (constant-amplitude) solutions, which can be done in a complete analytical form. We find that they may be stable in the case of r P 1, provided that the absolute value of the dispersion coefficient is larger in the normal-GVD channel than in the anomalous-GVD one, and certain auxiliary conditions on the amplitudes are met. Then, we summarize results for the stability of the cnoidal-wave solutions, obtained by dint of direct simulations. It is concluded that, in the physically important case of r = 2 (as well as for r < 1) the cnoidal waves are never strictly stable, which is not surprising, as all the cnoidal waves are unstable in the single NLS equation with anomalous GVD. Nevertheless, it is possible to identify a parameter region where the instability is very weak, so that the region is of direct interest to applications. A general trend is that the coupled cnoidal waves are less unstable when the absolute value of the dispersion 120 S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 coefficient in the anomalous-GVD channel is small in comparison with the respective coefficient in its normal-GVD counterpart, and the period of the cnoidal waves is smaller (in the limit case of the infinite period, the coupled cnoidal waves with r > 1 carry over into a known exact solution for coupled ‘‘symbiotic’’ solitons, which is strongly unstable; the infinite-period limit for r < 1 is another unstable bound state of bright and dark solitons). In the case when the instability is tangible, it may be of two different types. Moderate instability manifests itself as onset of quasi-regular modulations of the coupled waves; on the other hand, strong instability results in direct transition to a spatiotemporal chaos. Results obtained from these simulations are summarized in Section 3. 2. Exact solutions for the coupled waves 2.1. Cnoidal waves The system of the normalized XPM-coupled NLS equations describing the interaction of electromagnetic waves with local amplitudes A and B in the idle and payload channels in a fiber-optic telecommunications link, or in a dual-core waveguide (in both cases, two different carrier wavelengths are implied), is 2 2 iAz d1 Att þ jAj þ rjBj A ¼ 0; ð1Þ 2 2 iBz þ d2 Btt þ jBj þ rjAj B ¼ 0; ð2Þ where z and t are, as usual, the propagation distance and ‘‘local time’’ [12,13], 2d1 and 2d2 are the GVD coefficients (in accordance with what said above, we consider the case when both d1 and d2, defined as in Eqs. (1) and (2), are positive), and the SPM (self-phase-modulation) nonlinearity coefficient is normalized to be 1, then r > 0 is the relative XPM coefficient. As said above, the case of r = 2 is of major interest to applications, but we will display exact solutions for arbitrary r > 0. We also assume, as explained above, that the channels governed by Eqs. (1) and (2) have the same group velocity, therefore group-veloc- ity-difference terms do not appear in Eqs. (1) and (2). The latter condition implies the symmetric choice of the two carrier waves relative to the ZDP, then the case of d1 = d2 is the most natural one, although unequal values of d1 and d2 are relevant too. The system (1) and (2) is definitely nonintegrable, except for the ManakovÕs case [21], r = 1 (which does not apply to optical fibers). Nevertheless, a vast class of exact cnoidal-wave solutions can be found, using the HirotaÕs method [22] and special relations between the elliptic h-functions, as explained in detail in Refs. [23,24]. Note that, in all the previous works, this method (as well as other techniques employed to generate exact periodic-wave solutions [7,8]) was applied to the case when the GVD coefficients in the coupled NLS equations had the same sign. Here, we apply the HirotaÕs method to Eqs. (1) and (2), where these signs are opposite. First, we address the case of r > 1, which is most important for applications (because it includes r = 2, i.e., the value relevant to fiber optics). Skipping details of manipulations with the h-functions, which follow the pattern of [11], we display a final form of the solutions found in this case. Two families of the exact periodic waves correspond to the signs + and in the following expressions: rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðrd2 þ d1 Þ ð Þ 2 1=4 ðÞ A ðz; tÞ ¼ exp iQ1 z r 1 k r2 1 " # 2 1=4 1k dnðrt; k Þ ð3Þ 1=4 ; dnðrt; k Þ 1 k2 B ðÞ rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðd2 þ rd1 Þ ðz; tÞ ¼ exp r r2 1 2 k snðrt; k Þcnðrt; k Þ ; dnðrt; k Þ ð Þ iQ2 z ð4Þ where the propagation constants are pffiffiffiffiffiffiffiffiffiffiffiffiffi pffiffiffiffiffiffiffiffiffiffiffiffiffi 2r2 1 k 2 ð Þ 2 2 2 Q1 ¼ r d1 2 k 2 1 k þ 2 pffiffiffiffiffiffiffiffiffiffiffiffiffi r 1 1 rd2 1 k 2 þ pffiffiffiffiffiffiffiffiffiffiffiffi2ffi 2 1k pffiffiffiffiffiffiffiffiffiffiffiffiffi 1 2 2 ffiffiffiffiffiffiffiffiffiffiffiffi ffi p þ d1 r 1k þ 2 ; ð5Þ 1 k2 S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 ð Þ Q2 pffiffiffiffiffiffiffiffiffiffiffiffiffi pffiffiffiffiffiffiffiffiffiffiffiffiffi 2r2 1 k 2 1 2 2 d2 ¼ 1 k þ pffiffiffiffiffiffiffiffiffiffiffiffi2ffi 2r r2 1 1 k pffiffiffiffiffiffiffiffiffiffiffiffiffi 1 þ rd1 1 k 2 þ pffiffiffiffiffiffiffiffiffiffiffiffi2ffi 2 ; ð6Þ 1k sn, cn and dn being the standard JacobiÕs elliptic functions with the modulus k (0 < k < 1). The solutions depend on two arbitrary constants, k and r, but the latter one is actually a trivial parameter, as it accounts for the obvious scaling invariance of the underlying Eqs. (1) and (2). The period of the solutions of both types is T ¼ 2KðkÞ=r; ð7Þ where K is the complete elliptic integral of the first kind [23]. These solutions disappear at the point r = 1, which corresponds to the integrability in the ManakovÕs sense [21]. In the case of r < 1, the above expressions are meaningless, as they are imaginary, while, by definition, the magnitude of the amplitude must be real. However, another exact solution family can be found in this case: rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðrd2 þ d1 Þ A ¼ rk expðiQ1 zÞ snðrt; kÞ; ð8Þ 1 r2 rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðrd1 þ d2 Þ B ¼ r expðiQ2 zÞ dnðrt; kÞ; ð9Þ 1 r2 Q1 ¼ r2 d1 ð1 k 2 Þ þ 2r2 ðd1 þ rd2 Þ ; 1 r2 ð10Þ 2rr2 ðd1 þ rd2 Þ : ð11Þ 1 r2 We note that, for both cases r 6 1, the above solutions remain valid in the case when either d1 or d2 vanishes, i.e., one of the two channels is chosen exactly at the ZDP. This special case was not considered in previous works [7–11]. Q2 ¼ r2 d2 ð2 k 2 Þ þ 2.2. The limit case: solitons In the case of k = 0, which corresponds to the smallest period (7), T = p/r, the solutions take a trivial CW form: Eqs. (3) and (4) yield A = const, B = 0, and Eqs. (8) and (9) yield A = 0, B = const. It is obvious that the former CW state is stable 121 (any CW solution is modulationally stable in the single-component normal-GVD model), and latter is not, as it has a CW state in the anomalous-GVD subsystem. In the opposite limit, k = 1, the period (7) diverges, and the solutions (3) and (4) turn into an inverted bound pair of the bright and dark solitons in the normal-GVD and anomalous-GVD channels, respectively rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðrd2 þ d1 Þ ð Þ iQ1 z sechðrtÞ; A ¼ e r r2 1 rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðd2 þ rd1 Þ tanhðrtÞ; ð12Þ BðÞ ¼ eiQ2 z r r2 1 r2 2rd2 þ ð1 þ r2 Þd1 ; 1 2r2 Q2 ¼ 2 ðd2 þ rd1 Þ: r 1 Q1 ¼ r2 ð13Þ In fact, it is a known solution in the form of the socalled ‘‘symbiotic soliton’’, which has bright and dark components in the subsystems with the positive and negative GVD, despite the fact that such solitons cannot exist in isolation [25] (uninverted bound states, with the bright and dark solitons in the anomalous-GVD and normal-GVD components, do not exist for r > 1). The symbiotic soliton is strongly unstable, as the finite-amplitude background of the dark soliton in the anomalous-GVD equation is subject to the modulational instability. In the same limit of k ! 1, the solution (3) and (4) corresponding to r < 1 goes over into a ‘‘normal’’ (uninverted) bound state of dark and bright solitons in the normal- and anomalous-GVD components, respectively (dn ! sech, sn ! tanh): rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðrd2 þ d1 Þ A ¼ r expðiQ1 zÞ tanhðrtÞ; 1 r2 rffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi 2ðrd1 þ d2 Þ B ¼ r expðiQ2 zÞ sechðrtÞ; ð14Þ 1 r2 Q1 ¼ 2r2 ðd1 þ rd2 Þ ; 1 r2 Q2 ¼ r2 d2 þ 2rr2 ðd1 þ rd2 Þ : 1 r2 ð15Þ It is obvious that this bound state is also unstable, although for a reason completely different 122 S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 from that in the case of the symbiotic soliton (12). Indeed, while both bright and dark uninverted solitons are stable in isolation, their interaction is repulsive (as the XPM-mediated interaction between the two fields is attractive, the bright soliton is effectively repelled by the hole representing the dark soliton in the mate channel). Obviously, a bound state of the solitons may only be unstable in the case of repulsion between them. resulting dispersion equation for the perturbation propagation constant X is ½X2 d1 p2 ðd1 p2 þ 2A20 Þ½X2 d2 p2 ðd2 p2 2B20 Þ þ 4r2 d1 d2 A20 B20 p4 ¼ 0: The stability condition is that both roots for X2 determined by Eq. (18) must be real and positive for all real p. For the biquadratic equation in the form of (X2)2 + b(X2) + c = 0, the latter condition amounts to the set of inequalities b2 4c > 0; 3. Stability of the solutions In the previous section, it was concluded that the exact solution (3) and (4) for r > 1 is unstable in the limiting case of k ! 1, and stable in the limit of k ! 0. The solution (8) and (9) for r < 1 is unstable in both limits. In the general case, 0 < k < 1, the stability can be tested by direct simulations of perturbed periodic-wave solutions. Results of the test are reported in the next subsection. Before proceeding to that, it is relevant to study the modulational stability of the full family of CW solutions in the present model, as this issue has never been considered before for XPM-coupled equations with opposite signs of the dispersion, and exact analytical results for this relatively simple problem may be a clue to the understanding of stability of the cnoidal waves in the same system. The CW solutions with arbitrary amplitudes A0 and B0 are Að0Þ ¼ A0 exp½iðA20 þ rB20 Þz; ð16Þ A perturbed solution is taken in the form A ¼ Að0Þ ðzÞð1 þ ar þ iai Þ; B ¼ Bð0Þ ðzÞð1 þ br þ ibi Þ; b < 0; c > 0: ð19Þ For Eq. (18), these conditions take the form, respectively, pffiffiffiffiffiffiffiffiffi 2 A20 d1 þ B20 d2 2A0 B0 r d1 d2 þ ðd21 d22 Þp2 > 0; 3.1. Continuous-wave states Bð0Þ ¼ B0 exp½iðrA20 þ B20 Þz: ð18Þ ð17Þ where ar,i(z,t) and br,i(z,t) are infinitesimal real and imaginary parts of the perturbation. After the substitution of Eqs. (17) and (16) in Eqs. (1), (2) and subsequent linearization, eigenmodes are looked for as exp[i(pt Xz)] with arbitrary real p. The ð20Þ 2ðd1 A20 d2 B20 Þ þ ðd21 þ d22 Þp2 > 0; ð21Þ 4A20 B20 ðr2 1Þ þ 2ðd2 A20 d1 B20 Þp2 þ d1 d2 p4 > 0: ð22Þ Straightforward analysis of these inequalities demonstrates that the CW solutions with A0B0 6¼ 0 may be stable only if r P 1 and d1 P d2. If the latter conditions hold, the stability region of the CW solutions is A0 P max B0 sffiffiffiffiffi (sffiffiffiffiffi ) pffiffiffiffiffiffiffiffiffiffiffiffiffi d2 pffiffiffiffiffiffiffiffiffiffiffiffiffi d1 2 2 r r 1 ; rþ r 1 : d2 d1 ð23Þ The purport of this result is that, if the amplitude A0 of the solution in the normal-GVD channel, which by itself is modulationally stable, is sufficiently large as compared to the amplitude B0 in the anomalous-GVD channel, the CW as a whole is stable. Further, consideration of Eq. (23) demonstrates that, for any r P 1, the minimum value of the ratio A0/B0 admitting the stability is exactly p(A 0/B0)min = 1, which is attained at ffiffiffiffiffiffiffiffiffiffiffiffiffi 2 d1 =d2 ¼ ðr þ r2 1Þ . 3.2. Cnoidal waves For the numerical analysis of the stability of the exact periodic-wave solutions, simulations of the S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 perturbed solutions were performed by means of the Hopscotch method, which amounts to marching forward in z using both implicit and explicit schemes. It is known that the method itself is definitely stable [26]. Initial conditions were taken, at z = 0, in the form prt 2prt A0 ðtÞ ¼ Að0Þ ðz ¼ 0; tÞ þ 1 sin þ 2 sin ; KðkÞ KðkÞ B0 ðtÞ ¼ Bð0Þ ðz ¼ 0; tÞ; ð24Þ where A(0)(z,t) and B(0)(z,t) are the exact solution (3) and (4) or (8) and (9), and 1,2 are small amplitudes of the perturbation. Recall that the period of the unperturbed solutions is given by the expression (7), therefore the form of the initial perturbation in Eq. (24) implies that it is taken as a combination of the fundamental and second harmonics of the underlying solution. Additional numerical simulations demonstrate that inclusion of higher-order harmonics in the perturbation does not essentially alter the results. Note also that the initial perturbation is added only to the A-component of the solution; more extensive simulations show that a perturbation added to the Bcomponent does not lead to essentially new effects. The results turn out to be nearly the same for the perturbation of both solutions, (3), (4) and (8), (9), 123 therefore the conclusions are illustrated below by plots obtained for the former one. Extensive simulations have not revealed any strictly stable solution, although it is difficult to perform an exhaustive scan of the entire solution family. However, the propagation distance after which the instability sets in, as observed in the direct simulations, strongly depends on the solutionÕs parameter k (i.e., on the period (7) of the cnoidal solution): the instability of the cnoidal waves (3) and (4) with r > 1 gets strongly suppressed with the decrease of k, making the solution a ‘‘practically stable’’ one (see details below), and, accordingly, rendering the system appropriate for the applications to fiber-optic telecommunications. This feature can be easily understood, as these exact solutions are definitely unstable if k = 1, and stable if k = 0, see above. Note that, as the period T decreases with k, see Eq. (7), while the bit-rate, provided by the scheme in which the normalGVD channel is employed as the one supporting the pulse stream in its anomalous-GVD channel, is 1/T, the case of smaller k and, accordingly, smaller T is of major interest to the applications. To illustrate the dependence of the instability on the period, in Figs. 1(a) and (b) we compare typical results of the simulations of Eqs. (1) and (2) for the cases of k = 0.5 and k = 0.9, in the most relevant model, with r = 2 and d1 = d2 = 1. Note Fig. 1. Results of direct simulations of Eqs. (1) and (2) with r = 2, d1 = d2 = 1 and the initial condition (24), in which the unperturbed solution is the one A(+), B(+) from Eqs. (3) and (4), and the perturbation amplitudes are 1 = 0.1 and 2 = 0. The other parameters are r = 1, and k = 0.5 (a) or k = 0.9 (b). In this and subsequent figures, only the evolution of the field jA(z,t)j is displayed, as the field jB(z,t)j demonstrates a very similar behavior. 124 S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 that the respective periods of the unperturbed solution are 3.37 and 4.56, according to Eq. (7). In the case of k = 0.5, the instability, after it sets in at z . 50, first gives rise to quasi-reversible modulations of the wave pattern, and only at z . 150 the pattern suffers destruction, which leaves the system in an apparently chaotic state. On the contrary to that, in the case of k = 0.9 the instability immediately destroys the wave patterns at a much earlier stage, z . 20. To realize the actual meaning of these critical values of the normalized transmission distance, it is necessary to express them in units of the dispersion length of the periodic wave, which is Z disp ’ T 2 =ð4pd2 Þ; ð25Þ (recall T is the waveÕs period). Thus, in the case shown in Fig. 1(a), the instability commences at z 50Zdisp, while in the case of Fig. 1(b) it starts at z 10Zdisp. In the fiber-optic telecommunication networks, the dispersion length of RZ signals may typically be in the range of 300 km [15], which shows that the instability-free propagation distance suggested by Fig. 1(a) is quite appropriate for the applications. Next, we test how the stability is affected by variation of the relative strength of the normal and anomalous GVD in the two channels, d1/d2. Generally, the cnoidal wave pattern gets more stable with the increase of d1/d2, as is illustrated by Fig. 2. This is natural, as the cnoidal-wave solution in the single NLS equation may be completely stable only in the case of the normal GVD. Accordingly, the decrease of d1/d2 makes the pattern less stable, although not dramatically (which suggests the robustness of the proposed scheme for the applications), as is shown in Fig. 3. The trend to the stabilization of the solution with the growth of d1/d2 is strongly suggested too by the analytical conditions (23) for the CW solutions, as they demonstrate that the stability threshold gets lower with the increase of d1/d2, as long as it remains than ðd1 =d2 Þmax ¼ ffiffiffiffiffiffiffiffiffiffiffiffiffi 2 smaller p ðr r2 1Þ . In particular, (d1/d2)max 14 for r = 2, which includes the cases of d1/d2 = 2 and d1/d2 = 0.5, that are displayed in Figs. 2 and 3. The onset and development of the instability should, obviously, depend on the amplitude of the perturbation. To illustrate that dependence, in Fig. 4 we display the situations which are observed if the initial amplitude of the perturbation is taken, respectively, as (a) 10%, (b) 30%, and (c) twice that in Fig. 1(a). From here, it is observed that the weakest initial perturbation (1 = 0.01, Fig. 4(a)) generates no visible instability within the propagation distance simulated, and the perturbation which is somewhat stronger (1 = 0.03, Fig. 4(b)) gives rise only to quasi-reversible modulations, that set in at the latest stage of the evolution. The really strong perturbation (1 = 0.2, Fig. 4(c)) initiates the instability at the value of z not much smaller than that in the case which was shown above in Fig. 1(a), but in this case, the instability immediately causes complete destruc- Fig. 2. The same as in Fig. 1, but with d2 = 0.5 (the anomalous GVD twice as weak as the normal GVD). S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 125 Fig. 3. The same as in Fig. 1, but for d2 = 2 (the anomalous GVD twice as strong as the normal GVD). Fig. 4. The same as in Fig. 1(a), but for different amplitudes of the initial perturbation: 1 = 0.01 (a), 1 = 0.03 (b), and 1 = 0.2 (c). tion of the pattern and transition to a ‘‘turbulent’’ state. We also studied the effect of adding the secondharmonic component to the initial perturbation, i.e., 2 6¼ 0 in Eq. (24). If the perturbation is weak, for instance, 1 = 2 = 0.01 or 0.03 (cf. Figs. 4(a) and (b)), the extra disturbance does not produce any noticeable effect. However, in the case of a stronger initial disturbance, such as that with 1 = 2 = 0.1 or 0.2 (cf. Figs. 1(a) and 4(c)), the 126 S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 Fig. 5. The same as in Fig. 1(a), but for the initial perturbation (24) that includes the second-harmonic component, so that 1 = 2 = 0.1 (a), 1 = 2 = 0.2 (b). additional component in the perturbation naturally makes the transition to chaos quicker, as is shown in Fig. 5. The stability of the exact cnoidal-wave solutions (8), (9) corresponding to r < 1 was explored too. An inference is that these solutions are more unstable than their counterparts with r > 1, which is quite natural, as all the CW solutions with r < 1 are unstable, and the limiting case of the solutions (8), (9) corresponding to k = 0 is unstable too. A typical example is shown, for r = 2/3 (recall this value corresponds to the interaction between orthogonal linear polarizations of light), in Fig. 6. Comparing with the case displayed above in Fig. 1 for the same parameters, except that r = 2, one concludes that, in the present case, the initial pattern gets completely destroyed and replaced Fig. 6. The same as in Fig. 1(a), but with r = 2/3. by a turbulent state already by z = 40, while in the pattern corresponding to r = 2 survived unperturbed up to z = 50, and then persisted at least up to z = 150 in a periodically modulated state. 4. Conclusion In this work, using the technique based on the HirotaÕs method and elliptic theta-functions, we have constructed three families of exact coupled periodic (cnoidal) waves for XPM-coupled NLS equations, with the XPM/SPM ratio r. Two families were found for r > 1, and one for r < 1. Unlike all the previous works on this topic, we have obtained the solutions for the case when the groupvelocity-dispersion (GVD) coefficients in the two equations have opposite signs (including the case when the GVD vanishes in one equation). The model with r = 2 has direct interest to fiber-optic telecommunications, where it pertains to a scheme with a pulse stream in an anomalous-GVD payload channel stabilized by a strong periodic signal in a mate normal-GVD channel. The model with smaller values of r may be realized as a dual-core waveguide with different carrier wavelengths launched into the cores, an especially promising realization being the one with two parallel cores embedded in a photonic-crystal fiber. To attack the stability problem, we have first explored, in an analytical form, the modulational stability of the two-component CW solutions. A S.C. Tsang et al. / Optics Communications 249 (2005) 117–128 stability domain was identified, with the main inference that the CW state may be stable if its normal-GVD amplitude is sufficiently large in comparison with the anomalous-GVD one. In addition, necessary stability conditions for the CW states are r > 1, and a demand that the absolute value of the anomalous-GVD coefficient must be smaller than its normal-GVD counterpart. The stability of the exact periodic solutions was tested by means of direct simulations. It was concluded that, although all the coupled-cnoidal-wave patterns are, strictly speaking, unstable, a parameter region with a very weak instability can be found in the model with r = 2, making the above-mentioned dual-channel scheme appropriate for the applications to fiber-optics telecommunications. The instability is milder when the period of the wave pattern is smaller, and/or the anomalous GVD is weaker than the normal GVD in the mate channel. When the instability sets in, it may first take the form of quasi-reversible modulations, and only at a later stage will the wave pattern be completely destroyed. In agreement with what is suggested by the analytical results for the stability of the CW solutions, the cnoidal waves are much more unstable for r < 1. The analysis presented in this work calls for an extension, as the analytical cnoidal-wave solutions are, obviously, not the most generic periodic ones. In particular, it was shown above that, in the limit of k ! 0 (i.e., for the smallest period), the solutions go over into particular CW solutions with the vanishing amplitude in either of the two XPM-coupled modes. On the other hand, it was also shown, in the analytical form, that general CW solutions have two nonzero amplitudes, and a part of such solutions is modulationally stable. Thus, a natural issue is to find the most generic periodic-wave solutions that would abut, in the limit similar to k ! 0, upon the general CW states; in particular, the periodic solutions that carry over, in this limit, into the stable CW solutions, may themselves have a chance to be truly stable. 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