Faylali et al., International Journal of Advanced Engineering Technology E-ISSN 0976-3945 Research Paper MODELING OF OPTICAL PULSE PROPAGATION IN KERR AND RAMAN NONLINEAR DISPERSIVE MEDIA USING ADE-TLM METHOD H. El Faylali, M. Iben Yaich and M. Khaladi Address for Correspondence Electronic & Microwaves Group Faculty of Sciences, Abdelmalek Essaadi University P. O. Box: 2121, Tetuan 93000 Morocco ABSTRACT In this paper, we propose a simulation model of electromagnetic wave’s propagation, in media with different kinds of dispersions. This approach is based on the existing Auxiliary Differential Equation (ADE) technique in the context of the Transmission Line Matrix method with the symmetrical condensed node (SCN -TLM) and novel voltage sources. The proposed model, named ADE-TLM, gives a full solution of Maxwell’s equations and polarisation terms which describe the Lorentz linear dispersion, the nonlinear instantaneous Kerr and retarded Raman effects. KEYWORDS Auxiliary Differential Equation (ADE) technique, Finite-Difference Time Domain (FDTD), Transmission Line Matrix (TLM), dispersion, Kerr, Lorentz, Raman. I. INTRODUCTION Based on different techniques of discretization of own equations, several differential numerical time domain methods have efficiently simulated nonlinear dispersive media. These approaches include the linear and nonlinear properties and take into account physical complexity of media such as Kerr effects, Raman diffusion and/or photonic absorption. The Finite-Difference Time-Domain (FDTD) method and the numerical resolution of polarization and Maxwell’s equations are often used to characterize intrinsically nonlinear media, and to predict the behavior of propagated electromagnetic (EM) waves [1]-[3]. By incorporating judiciously the polarization vector and Maxwell's equations, The FDTD method based on the auxiliary differential equation (ADE) technique has effectively modeled the interaction of femtosecsond pulses in silica fibers [4],[5]. The Z-transform technique combined with the FDTD method, gave consistent results for the simulation of solitons in nonlinear dispersive media [6], [7]. In order to simulate the wave’s propagation in dispersive media with complex permittivity, methods based on the discrete convolution of the dispersion relation are presented in [8]. The nonlinear Schrödinger equation was applied to model the propagation of short optical pulses in Kerr media [9]. The Alternating-Direction Implicit Finite-Difference Time-Domain (ADI-FDTD) has been introduced as an unconditionally stable implicit method to solve the problems of EM radiation in nonlinear dispersive media [10]. Front of the variety of numerical techniques employed and the rigor of the proposed approaches and models developed by the FDTD method to simulate EM wave propagation in nonlinear media and predict their interactions, the TLM method provides further opportunities for proposals and development of new modeling tools and investigation despite of the numerous studies performed in this field [11]-[15]. In this paper, we increase the applicability of the TLM numerical method to model the linear and nonlinear dispersion properties. A novel algorithm based on the TLM method with condensed symmetrical node (SCN) and new voltage sources combined with the auxiliary differential equation ADE, is used to model the Lorentz dispersion, the Int J Adv Engg Tech/IV/III/July-Sept.,2013/01-04 nonlinear instantaneous Kerr and the retarded Raman effects in nanostructured nonlinear optical media. Numerical results that demonstrate the validity and efficiency of the proposed algorithm TLM-ADE as well as the nonlinear formulation of the electric field are presented. Excellent accordance is achieved between the ADE-TLM calculated and exact theoretical results for the reflection coefficient in Lorentz, Kerr and Raman media. II. THEORY In our proposed model, we reformulate the auxiliary differential equation (ADE) technique in the context of the TLM method. This approach allows the simulation of the propagation of optical pulses in linear Lorentz and nonlinear Kerr and Raman medias, by solving Maxwell's and polarization equations describing the effects of the media on the EM wave’s propagation. This approach is based on the time discretization applied to the components of the EM field and polarization vector by using centered differencing. A. Nonlinear Maxwell’s equations The Maxwell-Ampere equation for an EM wave propagating along the z-direction (i.e., E x component) in a dispersive nonlinear medium can be written as follows: ∂Ex (t) 1 ∂Px (t) = + ∇ΛH − x ∂t ε0ε∞ ∂t ( ) (1) Where ε 0 is the dielectric constant of free space, ε ∞ is the relative dielectric constant in the limit of infinite frequency and Px (t) = PL (t) + PNL (t) is the polarization term. The linear part PL (t) = PLorentz (t) describes the linear Lorentz dispersive properties of the medium and the nonlinear one PNL (t) = PKerr (t)+ PRaman (t) represents the instantaneous Kerr and retarded Raman effects. E x and Px are respectively the components, along the x-axis, of the electric field and polarization vectors. Using centered differencing scheme between time n+1 n steps t = (n + 1)∆l and t = n∆l , we can write the discretized equation for the electric and polarization fields in regular space Faylali et al., International Journal of Advanced Engineering Technology ( ∆x = ∆y = ∆z = ∆l ) χ0(3) being the third order nonlinear susceptibility and α , 0 ≤ α ≤ 1 , represents the relative strengths as follows: 1 n+ 1 ∆t 2 (Pxn+1 - Pxn )+ ∇ΛH ε0ε∞ ε 0ε ∞ x E nx +1 = E nx - (2) To develop a TLM model for the numerical treatment of these problems we need to transform the EM field parameters into circuit parameters that are related to transmission lines. Substituting in (2), the component E x by its electric equivalent Vx , we obtain the expression of the discretized ∆l n+1 electric voltage component Vx along the x-axis at ∆l ε 0ε ∞ (Pxn+1 - Pxn ) + 1 n+ ∆t∆l ∇ΛH 2 ε 0ε ∞ x (3) The proposed ADE-TLM algorithm, unifies all types of dispersion (of the second and the third order) of medias expressed by the polarization terms appearing in (3), in a single formula expressing the component of the electric voltage along the z-direction. In the sequel, we give the numerical expressions of the polarization of the second and the third order ( PL (t) and PNL (t) ) in terms of electric voltage. B. Second-order linear dispersion The Lorentz polarization as a function of electric voltage is governed by the following auxiliary differential equation: ∂2PLorentz (t) ∂P (t) +2δLorentz Lorentz 2 ∂t ∂t ε ε ( −ε ) 2 2 PLorentz (t) = 0 Lorentz ∞ ωLorentz V(t), +ωLorentz ∆l (4) frequency, δ Lorentz the damping factor and ε Lorentz the static permittivity caused by the Lorentz dispersion. By using centered differencing, the polarization of n+1 n+1 the Lorentz dispersion PLorentz at time step t obeys to the following difference equation: Vxn ∆l (5) Where a Lorentz = 2 2-ωLorentz ∆t 2 1 + δ Lorentz ∆t b Lorentz =c Lorentz = 1 − δ Lorentz ∆t 1 + δ Lorentz ∆t 2 ε 0 (ε Lorentz − ε ∞ )ωLorentz ∆t 2 1 + δ Lorentz ∆t C. Third-order nonlinear dispersion The polarization caused by the instantaneous Kerr nonlinearity is written, as function of the electric voltage by: PK err (t) = = ε 0 χ 0( 3 ) ∆l αε0χ ∆ l3 t V (t) ∫ -∞ (3) 0 α δ (t - t ' ) ∆ l2 V 2 (t ' )dt ' |V 2 (t)|V (t) IJAET/Vol. IV/ Issue II/April-June, 2013/ n+1 PKerr = αε 0 χ 0(3) |Vxn+1 |2 Vxn+1 (7) ∆l As a convolution, the polarization caused by the Raman effect may be writing as: 3 ε0 PRaman (t) = ∆l (3) V(t)χ Raman (t) * V 2 (t) ∆l 2 V 2 (t) (9) ∆l 2 Then we apply the Fourier transform to (9): 2 % ω ) = χ (3) (ω ) * ℑ V (t) S( Raman 2 ∆l (10) (3) S(t) = χ Raman (t) * Where S and χ denote the Fourier transforms of the corresponding time functions. The retarded response function is: 2 (3) (1 − α ) χ 0(3)ωRaman χ Raman (ω )= 2 ωRaman + 2 jωδ Raman − ω 2 (11) With τ 12 + τ 22 τ 12τ 22 ωRaman = Where ωLorentz is the Lorentz characteristic resonant n+1 n n-1 PLorentz = a Lorentz PLorentz + b Lorentz PLorentz + c Lorentz of the Kerr and Raman polarizations. Analogous to the Lorentz case, the polarization of n+1 n+1 the Kerr dispersion PKerr at time step t can be written as follows: (8) To solve (8), we introduce an auxiliary variable S(t) for the convolution: n+1 time step t : Vxn+1 =Vxn - E-ISSN 0976-3945 δ Raman = 1 τ2 Next insert (11) into (10), multiply by 2 2 ( ωRaman + 2 jωδ Raman − ω ) and transform to the time- ∂2 ∂ and ω 2 → − 2 to ∂t ∂t get the following auxiliary differential equation: domain functions by jω → 2 (1- α )χ 0(3)ωRaman ∂ 2 S(t) ∂S(t) 2 δ ω + 2 + S(t) = Vx2 (t) Raman Raman ∂t 2 ∂t ∆l 2 (12) The finite difference expression for the time n+1 derivative of (12) centered at time step t is then given by: c Sn+1 = a Raman Sn +b Raman Sn-1 + Raman Vxn 2 (13) ∆l 2 With 2 ∆t 2 2-ωRaman a Raman = 1 + δ Raman ∆t b Raman =c Raman = 1 − δ Raman ∆t 1 + δ Raman ∆t 2 (1 − α ) χ 0(3)ωRaman ∆t 2 1 + δ Raman ∆t n+1 Finally, the discretized Raman polarization PRaman (6) n+1 at time step t can be written as follows: Faylali et al., International Journal of Advanced Engineering Technology n+1 PRaman = ε0 Vxn+1Sn+1 (14) ∆l III. ADE-TLM ALGORITHM By substituting the terms of the polarization given by (5), (7) and (14) in (3), we can write the discretized nonlinear relation describing electrical n+1 voltage at time step t as: ∆l n+1 n (PLorentz -PLorentz ) ε0ε∞ Vxn+1 =Vxn + αχ 0(3) ∆l 2 ε ∞ (|V | Vxn+1 -|Vxn |2 Vxn ) - n+1 2 x 1 (Vxn Sn+1 + Vxn Sn ) ε∞ 1 n+ ∆t∆l ∇ΛH 2 ε 0ε∞ x E-ISSN 0976-3945 χ (3) = 7 ×10−2 (V/m)−2 , τ1 = 12.2fs , τ 2 = 32fs and α = 0.7 . The considered TLM mesh dimensions are (1, 1, 10000) ∆l with space step ∆l = 8 nm. The airnonlinear dispersive medium interface is located at z = 8∆l and excited by a unit amplitude pulse with a sinusoidal carrier frequency fc = 0.137×1015 Hz considering a hyperbolic secant envelope function with a characteristic time constant of 14.6fs. Fig. 1 shows the spatial evolution to the right of the short pulse propagation, after 8000, 16000 and 32000 iterations for a linear dispersive medium. Our results are in accordance with those presented in [1], [14] and [18]. (15) Writing the magnetic field components of (15) in terms of incident and reflected pulses [16]-[17], then applying the charge conservation principle for the symmetrical condensed node SCN with a capacitive stub of normalized admittance Yox (t) we obtain the following expression for the n+1 n+1 discretized electric voltage Vx at time step t : Vxn+1 + A 2 n+1 2 n+1 2 |Vx | Vx = A1 4+Yox V1i + V2i + V9i + V12i +Yox V13i + 0.5Vsx n+1 (16) Where A1 = ε ∞ + Sn+1 A2 = αχ0(3) Fig. 1. TLM results of the short pulse propagation after 8000, 16000 and 32000 time steps respectively in dispersive linear medium. Fig. 2 shows the spatial evolution to the right of the short pulse propagation, after 8000, 16000 and 32000 iterations for the Kerr and the Raman medium. Our results are in accordance with those presented in [1], [14] and [18]. ∆l2 Vsx and Yox are respectively the voltage source, and the normalized admittance terms in order to take into account, in the TLM mesh, linear and nonlinear dispersive properties and also Kerr effects and Raman interactions in the nonlinear medium. They are given by: ( ε ∞ + Sn+1 − A1 ) Vxn + 2A 2 |Vxn |2 Vxn Vsx = − n Vsx + 4 ∆l n+1 n − ε ( PLorentz -PLorentz ) 0 Yox = 4 ( ε ∞ + Sn+1 − 1) (17) n+1 (18) The ADE-TLM model with voltage sources is based on recursive calculation of normalized admittance made in (18) and the voltage sources expressed in (17). The obtained values are then inserted in (16). The solution of the last equation is then used in the calculation of reflected pulses and in the connection process along the TLM mesh nodes. IV. NUMERICAL RESULTS In order to show the efficiency of the new model ADE-TLM with voltage sources, we present spatial variations of electrical field propagation in a medium having a Lorentz linear dispersion characterized by the following [18]: ε s = 5.25 , ε ∞ = 2.25 , ωLorentz = 0.4 ×1015 rad/s and Fig. 2. TLM results of the short pulse propagation after 8000, 16000 and 32000 time steps respectively in dispersive nonlinear medium. Next, the air-nonlinear dispersive medium interface is exited by Gaussian unit amplitude pulse. The damping factor is δ Lorentz = 0.1ωLorentz . Fig. 3 compares the ADE-TLM calculated and exact theoretical results [19] for the magnitude of the reflection coefficient for Lorentz, Kerr and Raman media. δ Lorentz = 2 ×109 s−1 . Fig. 3. Comparison of the reflection coefficient magnitude for the Lorentz, Kerr and Raman media as predicted by exact analytical results and computed using ADE-TLM. 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