•Losses and nonlinear effects –Introduction ECE 4006/5166 Guided Wave Optics Losses and nonlinearities Why related? • Loss gives ratio of output to input power per unit guide length • Nonlinearities limit input power. • The application (e.g. SNR at a receiver) sets minimum output power. All three, then, determine maximum link length. Primary loss mechanisms • Absorption (various sources) • Scattering (bulk = Rayleigh, surface) • Leakage (bending, coupling). Absorption mechanisms and Rayleigh scattering are covered in other classes. They cause exponential attenuation of the guided power just as they do for plane waves in homogenous media. I will thus focus on the new physics of surface scatter and bending loss. We will cover coupling loss later. Robert R. McLeod, University of Colorado 153 •Losses and nonlinear effects –Bend loss ECE 4006/5166 Guided Wave Optics Origins of bend loss Bend loss can be predicted from ray considerations (increased incidence angle on boundary) but not quantified. Straight waveguide Bent waveguide, radius R x θ z y r x z y The waves propagating in the curved space accumulate extra phase proportional to distance from the center of the waveguide. Ε ( x , y , z ) = E ( x, y ,0)e − jk0 δn ( x ) z Usual propagator Ε ( x , y , r θ ) = E ( x, y ,0)e − jk0 δn ( x ) r θ Equivalent in curved space Map to prev. coordinates = E ( x, y ,0)e − jk0 δn ( x ) ( R + x ) ( z / R ) − jk0 [δn ( x ) (1+ Rx ) ] z = E ( x, y ,0)e Equivalent index x x 0 0 δn ( x ) ncl nco δn ( x ) ( 1 + nco x R ) Thus we can simulate (and understand) curved waveguides via a scaled δn. Robert R. McLeod, University of Colorado Pollock and Lipson 6.1 154 •Losses and nonlinear effects –Bend loss ECE 4006/5166 Guided Wave Optics Propagating in curved spaces Conformal transform Consider a field in a 2D (x,z) plane described by [∇ 2 xz ] + k 02 n 2 ( x, z ) E (x, y ) = 0 This formally applies only TE propagation of a field Ez given a physical structure that is invariant in y. With minor modifications, it can describe TM propagation or waveguides with confinement in the y direction via the effective index approximation. Apply a conformal transformation to a new set of coordinates u (radial) and v (azimuthal). The proper transform is: W ≡ u + jv = R2 ln Which gives the new wave equation: {∇ 2 uv [ Z x + jz = R2 ln R2 R2 ]} 2 + k 02 e u R2 n ( x (u, v ), z (u, v )) E ( x, y ) = 0 Application: n (u ) = e u R2 n (ρ ) u ≈ 1 + + O (u 2 )n (ρ ) R which is the previous expression u = R2 ln ρ R2 v = θ R2 Robert R. McLeod, University of Colorado Heilblum & Harris, IEEE J. Q. E., VOL. QE-11, pp. 75-83, 1975 155 •Losses and nonlinear effects –Bend loss ECE 4006/5166 Guided Wave Optics BPM in straight guide Launch mode from slab waveguide solver. Mode travels > 3mm without significant chage. a = 5 [ µm] = λ0 = 1 [ µm] nco = 1.5 Neff δn = .001 N eff = 1.50068 |E| vs. x,z Robert R. McLeod, University of Colorado 156 •Losses and nonlinear effects –Bend loss ECE 4006/5166 Guided Wave Optics BPM in curved guide nclad (1 + xescape = R xescape R )=N N − nclad nclad Launch mode from slab waveguide solver. Mode at exit is leaky, lower total power and shifted towards larger radius xescape Neff Lossy Tail Radius of curvature, R 20 mm |E| vs. x,z . The plotting coordinate system has been warped to match the curvature of the space. The original propagation, however, is simply rectangular BPM with the index above. Robert R. McLeod, University of Colorado 157 •Losses and nonlinear effects –Bend loss ECE 4006/5166 Guided Wave Optics Loss due to curvature Derivation P (z ) = P (0)e −α z − 1 dP (z ) P (z ) dz − 1 PTail ≈ PTot Z Char α= Assume an exponential decay with z Solve for loss coefficient Approximate value, where ∞ PTail = 2 E ∫ (x )dx Power in tail, beyond escape radius x Escape ∞ PTot = ∫ E (x )dx 2 Total power in guide −∞ Z Char 2 2a ) ( = Characteristic diffraction length of mode 2λcl For simplicity, assume mode is unchanged (which will underestimate). Results for slabs and fibers: α = C1e − C R Slab 2 − 12 α = C3 R e − C R Fiber 4 where the constants depend only on waveguide geometry. The equations for the constants can be found in Pollock (Eq. 8.13 & 8.14) for the fiber case and Hunsperger (Eq. 5.3.12) for the slab case. Note that the dominate behavior is that loss increases exponentially with bending radius. Robert R. McLeod, University of Colorado Hunsperger, Sec 5.3 158 •Losses and nonlinear effects –Bend loss ECE 4006/5166 Guided Wave Optics Typical values Slab waveguide Putting the Hunsperger equation for a slab waveguide into normalized variables yields the following expression: C2 R C1 αλ0 = cos 2 (U ) exp (2W ) 2 a 2nclad W 1 + 21U sin (2U ) + W1 cos 2 (U ) λ0 [ ] R λ0 N − nclad exp − 4W a λ0 nclad Assume we desire a single mode guide with the minimum bend loss. This will occur for the largest N which will be at the cutoff for the second mode or V= π 2 ∴ a λ0 = 1 4 nco2 − ncl2 Taking nclad = 1.5 and solving for N0 at cutoff of m=1 in every case yields: Not physically reasonable. Violates assumptions? Robert R. McLeod, University of Colorado Not physically reasonable. Violates assumptions? Hunsperger 159 •Losses and nonlinear effects –Substrate coupling ECE 4006/5166 Guided Wave Optics Coupling to substrate wcore air Si dclad Si SiO2 SiO2 substrate thickness – coupling loss Robert R. McLeod, University of Colorado Wim Bogaerts, “Nanophotonic waveguides and photonic crystals in siliconon- insulator”, PhD Thesis, Ghent University, April 2004 160 •Losses and nonlinear effects –Edge scatter ECE 4006/5166 Guided Wave Optics Edge scatter SEM http://photonics.intec.ugent.be/download/ocs75.pdf Robert R. McLeod, University of Colorado F. P. Payne, J. P. R. Lacey, “A theoretical analysis of scattering loss from planar optical waveguides,” Optical and Quantum Electronics 26, 977-986 (1994) 161 •Losses and nonlinear effects –Edge scatter ECE 4006/5166 Guided Wave Optics Edge scatter Outline of derivation The field at the edge of the guide interacts with the rough edge which appears to be a random diffraction grating: −K = k −k inc The strength of the field at the guide edge. The strength of the effective grating. diff Bragg matching of the grating power spectrum to all possible scattering angles. By the Wiener-Khintchine the power spectrum is the Fourier transform of the auto-correlation of the roughness Various statistics could be chosen for this autocorrelation R(u), experiments suggest an exponential statistic is best: where Lc is the correlation length and σ is the standard deviation of the roughness. Moral: The loss will depend on the field at the edge, the index contrast of the edge, the standard deviation of the roughness and its correlation length. Robert R. McLeod, University of Colorado Size Influence on the Propagation Loss Induced by Sidewall Roughness in Ultrasmall SOI Waveguides, F. Grillot IEEE PHOTONICS TECHNOLOGY LETTERS, VOL. 16, NO. 7, JULY 2004 1661 162 •Losses and nonlinear effects –Edge scatter ECE 4006/5166 Guided Wave Optics Impact of sidewall roughness Numerical results Silica clad, H = 260 nm. Typical of raw RIE process Increasing confinement Single-mode Multi-mode Typical of RIE process followed by post-processing Increasing confinement Single-mode Robert R. McLeod, University of Colorado Multi-mode 163 •Losses and nonlinear effects –Intro to nonlinearities ECE 4006/5166 Guided Wave Optics Nonlinear optics Introduction In the temporal frequency domain, the general dielectric response of a material can be written as a vector Taylor series expansion of the polarization in the electric field as: r P (ωq ) r = ε 0 χ (ω q )E (ωq ) 1 Linear r r + ε 0 χ (ω q = ωm + ωn )E (ωm )E (ωn ) r r r 3 + ε 0 χ (ωq = ωm + ω n + ω p )E (ωm )E (ωn )E (ω p ) 2 2nd order 3rd order where sums are implied over all vector components and all frequencies, positive and negative, that obey the constraint of summing to ωq. χ is the “susceptibility” and is a tensor of order 2 for the linear case, 3 for second order etc. The linear susceptibility is usually lumped into the relative dielectric permittivity as εr = 1 + χ1. In the time domain, susceptibilities relate real electric fields to real polarization fields and are obviously real quantities. The Fourier transform of the susceptibilities can have real parts associated with nonresonant processes that do not exchange energy with the medium that are referred to as parametric processes imaginary parts associated with loss or gain of energy to the medium through material resonances that are referred to as nonparametric. The Kramers-Kronig relation and its analogs for the higher-order tensors requires that (for a local nonlinearity): χ n (ω q = ω1 + ω 2 + K + ω n ) = χ n (− ωq = −ω1 − ω2 − ... − ωn ) ∗ Robert R. McLeod, University of Colorado Photonic Devices, Jia-Ming Liu, Cambridge Press. Chapter 9. 164 •Losses and nonlinear effects –Intro to nonlinearities ECE 4006/5166 Guided Wave Optics Summary of second- and third-order processes Second order: Third order: Single primes (‘) indicate real part, double primes (“) imaginary part Robert R. McLeod, University of Colorado Photonic Devices, Jia-Ming Liu, Cambridge Press. Chapter 9. 165 •Losses and nonlinear effects –Intro to nonlinearities ECE 4006/5166 Guided Wave Optics Noether’s Theorem Real Domain Fourier Domain Translation invariance in time Conservation of energy E sin (ω t ) Time + hΩ δχ sin (Ωt ) − hΩ hω h (ω − Ω ) δP = ε 0δχE = 1 2 ε 0δχ {cos[(ω + Ω )t ] + cos[(ω − Ω )t ]} Translation invariance in space ( r r δχ sin K ⋅ r h (ω + Ω ) Conservation of momentum ) Space r + hK δP = 12 ε 0δχ r r r cos k + K ⋅ r + r r r cos k − K ⋅ r [( r r E sin k1 ⋅ r ( ) [( Robert R. McLeod, University of Colorado ) ] ) ] r r h k +K ( ) r hk r − hK r r h k −K ( ) 166 •Losses and nonlinear effects –Raman and Brillouin scattering ECE 4006/5166 Guided Wave Optics Spontaneous Rayleigh, Raman and Brillouin scattering Rayleigh scattering: elastic scattering of a photon. No energy exchange with medium so hωout = hωin Raman scattering: inelastic scattering of a photon from an “optical phonon” = an out-of-phase vibration of oppositely-charged atoms within a single crystal unit cell, creating an oscillating dipole that can interact with the EM field. These phonons are non-dispersive (any value of k is allowed for a particular frequency). If the phonon is created, energy is lost from the photon and thus it emerges with a lower frequency or Stokes shift, equal to ~14 THz for SiO2 hω out = hωin − hΩ phonon Maxwell-Boltzman statistics specify that, in equilibrium, most of the phonon states are unpopulated, so downward Stokes shift dominates. Anti-Stokes shift occurs when a phonon is destroyed: hωout = hωin + hΩ phonon Raman scattering is automatically phase-matched and the non-dispersive phonons allow any direction of scattering with the same frequency shift. Brillouin scattering: inelastic scattering of a photon from an “acoustic phonon” = an in-of-phase vibration of atoms within a single crystal unit cell in a long-range wave. These dispersive phonons result in a smaller frequency shift, typically 10 to 20 GHz for SiO2 that depends on scattering direction (maximum backwards). The physics is similar to the AO effect but here the photon creates the vibration. Scattering vanishes for the forward direction. Note: Stokes shift is also observed in fluorescence but is fundamentally different because it is only observed at fixed frequencies. The Stokes shift from scattering occurs at a phonon frequency offset from a broad range of input optical frequencies. Robert R. McLeod, University of Colorado 167 •Losses and nonlinear effects –Raman and Brillouin scattering ECE 4006/5166 Guided Wave Optics Acoustic vs. optical phonons Acoustic phonons have typical dispersion curve Ω = VA K. Optical nearly flat, so ~any K but always ~same Ω. Optical hω phonon = Acoustic This should probably be a/2. + charged atoms a - charged atoms Acoustic ka=0 Finite frequency at k=0 Optical Acoustic k a = 0.3 Optical 2π/K Density wave k a = 0.6 Acoustic Dipole wave Optical Robert R. McLeod, University of Colorado For animations of acoustic vs. optical phonons, see: http://fermi.la.asu.edu/ccli/applets/phonon/phonon.html 168 •Losses and nonlinear effects –Raman and Brillouin scattering ECE 4006/5166 Guided Wave Optics Spontaneous Brillouin scattering not allowed in forward direction Conservation of energy: A pump photon is destroyed causing a Stokes photon and an acoustic phonon to be created. ω pump = ω Stokes + Ω phonon Dispersion relations: Acoustic (not optical) phonons: ω pump r v v = c k pump , ω Stokes = c k Stokes , Ω phonon = V A K phonon Conservation of momentum: r v v k pump = k Stokes + K phonon In the forward direction: k pump = k Stokes + K phonon Assume pump is forward (k>0), Stokes and phonon k can be either + or r r . k pump k pump r r k Stokes K phonon r k Stokes k pump = k Stokes + K phonon ω pump = ω Stokes + r K phonon k pump = k Stokes − K phonon c Ω phonon VA Energy conservation not possible. ω pump = ω Stokes − c Ω phonon VA Energy conservation not possible. Optical phonon dispersion relation does permit forward Raman scattering. Robert R. McLeod, University of Colorado C.S. Wang ,” Vanishing of the forward first stokes line in stimulated Brillouin scattering “ Physics Letters A Volume 27, Issue 9, 23 September 1968, Pages 633-634 169 •Losses and nonlinear effects –Raman and Brillouin scattering ECE 4006/5166 Guided Wave Optics Spontaneous Brillouin scattering in other directions ky Assuming kpump ~ kStokes r k Stokes θ r r K phonon k pump kx θ 1 K phonon = k pump sin 2 2 θ 1 Ω phonon ω pump = sin cn 2 VA 2 Ω phonon = 2 n VA θ ω pump sin c 2 • This looks just like Bragg matching condition for an acoustooptic deflector. It essentially is – the acoustic wave is created by the scattering of the pump photon. • The frequency shift between the pump and the Stokes waves is dependent on the scattering angle, reaching a maximum of V Ω phonon = 2n A ω pump c in the backwards scattering case. The Raman frequency offset does not depend on scattering angle because all optical phonon K vectors (K < 0.3/a) have the same frequency. • The frequency shift is proportional to the optical frequency. In contrast, the Raman scattering frequency offset is constant with optical frequency. Robert R. McLeod, University of Colorado 170 •Losses and nonlinear effects –Raman and Brillouin scattering ECE 4006/5166 Guided Wave Optics Line shape of Raman and Brillouin processes χ (t ) ∝ e −γt sin (Ωt )u (t ) Time domain Ω Fourier transform in rotating wave aprox (ω − Ω ) + jγ Ω(ω − Ω ) Ωγ = −χ0 + j χ Re and Im parts 0 (ω − Ω )2 + γ 2 (ω − Ω )2 + γ 2 χ (ω ) ≈ − χ 0 Loss, γ > 0 Gain, γ < 0 2γ ω −Ω 2γ ω −Ω ω −Ω For Brillouin scattering in silica fiber, the counter-propagating frequency shift Ω/2π = 10 to 20 GHz and the bandwidth 2γ/2π = 50 to 100 MHz. Raman spectrum of silica is result of superposition of multiple resonances For Raman scattering in silica fiber, the frequency shift Ω/2π = 13.2 THz and the bandwidth 2γ/2π = ~10 THz. Robert R. McLeod, University of Colorado D. Hollenbeck and C. D. Cantrell, “Multiple-vibrational-mode model for fiber-optic Raman gain spectrum and response function”, J. Opt. Soc. Am. B 19 (12), 2886 (2002) 171