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Introduction Nonlinear Maxwells Equations Direct and Inverse Problems for Nonlinear Time-harmonic Maxwells Equations T ING Z HOU Northeastern University IAS Workshop on Inverse Problems, Imaging and PDE joint work with Y. Assylbekov T


  1. Introduction Nonlinear Maxwell’s Equations Direct and Inverse Problems for Nonlinear Time-harmonic Maxwell’s Equations T ING Z HOU Northeastern University IAS Workshop on Inverse Problems, Imaging and PDE joint work with Y. Assylbekov T ING Z HOU Northeastern University HKUST

  2. Introduction Nonlinear Maxwell’s Equations Outline Introduction 1 Nonlinear Maxwell’s Equations 2 Kerr-type Nonlinearity Construction of CGO solutions Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) T ING Z HOU Northeastern University HKUST

  3. Introduction Nonlinear Maxwell’s Equations Calderón’s Problem Electrical Impedance Tomography: Recover electric conductivity of an object from voltage-to-current measurements on the boundary. Posed by Alberto Calderón (1980). Voltage-to-current measurements are modeled by the Dirichlet-to-Neumann-map Λ σ : f �→ σ∂ ν u | ∂ Ω where u solves ∇ · ( σ ∇ u ) = 0 in Ω , u | ∂ Ω = f . Inverse Problem: Determine σ from Λ σ . T ING Z HOU Northeastern University HKUST

  4. Introduction Nonlinear Maxwell’s Equations Inverse Problem for Maxwell’s equations Consider the time-harmonic Maxwell’s equations with a fixed (non-resonance) frequency ω > 0 Ω ⊂ R 3 . ∇ × E = i ωµ H ∇ × H = − i ωε E and in E , H : Ω → C 3 electric and magnetic fields; ε, µ ∈ L ∞ (Ω; C ) electromagnetic parameters with Re ( ε ) ≥ ε 0 > 0 and Re ( µ ) ≥ µ 0 > 0; Electromagnetic measurements on ∂ Ω are modeled by the admittance map Λ ε,µ : ν × E | ∂ Ω �→ ν × H | ∂ Ω . Inverse Problem: Determine ε and µ from Λ ε,µ . T ING Z HOU Northeastern University HKUST

  5. Introduction Nonlinear Maxwell’s Equations Uniquness Results Conductivity equation: Calderón (1980) for the linearized inverse problem; Kohn-Vogelius (1985) for piecewise real-analytic conductivities; Sylvester-Uhlmann (1987) for smooth conductivities ( n ≥ 3); Nachman (1996) for n = 2; Maxwell’s equations: Somersalo-Isaacson-Cheney (1992) for the linearized inverse problem; Ola-Päivärinta-Somersalo (1993); Ola-Somersalo (1996) simplified proof; T ING Z HOU Northeastern University HKUST

  6. Introduction Nonlinear Maxwell’s Equations Nonlinear Conductivity Equations Consider nonlinear conductivity equation Ω ⊂ R n . div ( σ ( x , u , ∇ u ) ∇ u ) = 0 in p ) : Ω × R × R n → R is positive nonlinear conductivity; σ ( x , z ,� Measurements on ∂ Ω are given by the nonlinear DN map Λ σ : f �→ σ ( x , u , ∇ u ) ∂ ν u | ∂ Ω , where u solves the above equation with u | ∂ Ω = f . Inverse Problem: Recover σ from Λ σ . T ING Z HOU Northeastern University HKUST

  7. Introduction Nonlinear Maxwell’s Equations Linearization Approach Due to [Sun] (1996) following [Isakov-Sylvester] (1994). If σ = σ ( x , u ) , then for a fixed λ ∈ R . t → 0 t − 1 (Λ σ ( λ + tf ) − Λ σ ( λ )) = Λ σ λ ( f ) , σ λ ( x ) := σ ( x , λ ) lim in an appropriate norm. Then the uniqueness problem for the nonlinear equation is reduced to the uniqueness in the linear case: Λ σ 1 = Λ σ 2 ⇒ Λ σ λ 1 = Λ σ λ for all λ ∈ R ⇒ σ 1 = σ 2 . 2 T ING Z HOU Northeastern University HKUST

  8. Introduction Nonlinear Maxwell’s Equations Other Uniqueness Results for Nonlinear Conductivity For certain σ = σ ( x , ∇ u ) : [Hervas-Sun] (2002) for constant coefficient nonlinear terms and n = 2; [Kang-Nakamura] (2002) for n � σ ( x , ∇ u ) ∇ u γ ( x ) ∇ u + c ij ( x ) ∂ i u ∂ j u + R ( x , ∇ u ) . replaced by i , j = 1 ( ∗ Higher Order Linearization. ) For p -Laplacian type equations: σ = γ ( x ) |∇ u | p − 2 with 1 < p < ∞ . ( ∗ Linearization is not helpful. ) [Salo-Guo-Kar] (2016) under monotonicity condition if n = 2; under monotonicity condition for γ close to constant if n ≥ 3. T ING Z HOU Northeastern University HKUST

  9. Introduction Nonlinear Maxwell’s Equations Other Nonlinear Equations Inverse Problems were considered for other nonlinear models: Semilinear parabolic: Isakov (1993); Semilinear elliptic: Isakov-Sylvester (1994), Isakov-Nachman (1995); Elasticity: Sun-Nakamura (1994) for St. Venant-Kirchhoff model; Hyperbolic: Lorenzi-Paparoni (1990), Denisov (2007), Nakamura-Vashisth (2017). ** Comparing to the inverse problem of determining spacetime using nonlinear wave interactions. T ING Z HOU Northeastern University HKUST

  10. Kerr-type Nonlinearity Introduction Construction of CGO solutions Nonlinear Maxwell’s Equations Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) Outline Introduction 1 Nonlinear Maxwell’s Equations 2 Kerr-type Nonlinearity Construction of CGO solutions Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) T ING Z HOU Northeastern University HKUST

  11. Kerr-type Nonlinearity Introduction Construction of CGO solutions Nonlinear Maxwell’s Equations Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) Nonlinear Optics No charge and current density: ∇ × E = − ∂ t B , ∇ × H = ∂ t D , div D = 0 , div B = 0 in Ω × R . E ( t , x ) and H ( t , x ) are electric and magnetic fields; D is the electric displacement and B is the magnetic induction: D = ε E + P NL ( E ) , B = µ H + M NL ( H ); ( ∗ High energy lasers can modify the optical properties of the medium ). ε, µ ∈ L ∞ (Ω; C ) are scalar electromagnetic parameters with Re ( ε ) ≥ ε 0 > 0 and Re ( µ ) ≥ µ 0 > 0 ; P NL and M NL nonlinear polarization and magnetization. T ING Z HOU Northeastern University HKUST

  12. Kerr-type Nonlinearity Introduction Construction of CGO solutions Nonlinear Maxwell’s Equations Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) Nonlinearity In nonlinear optics, the polarization P ( t ) = χ ( 1 ) E + P NL ( E ) P NL = χ ( 2 ) E 2 + χ ( 3 ) E 3 + · · · := P ( 2 ) + P ( 3 ) + · · · ∗ χ ( j ) — j -th order nonlinear susceptibility. Second-order polarization (Noncentrosymmetric media): incident wave E = Ee − i ω t + c . c . generates P ( 2 ) ( t ) = 2 χ ( 2 ) EE + χ ( 2 ) E 2 e − i 2 ω t + c . c . Second harmonic generation Third-order polarization: incident wave E = E 1 e − i ω 1 t + E 2 e − i ω 2 t + E 3 e − i ω 3 t + c . c . generates polarization with terms of frequencies 3 ω 1 , 3 ω 2 , 3 ω 3 , ± ω 1 ± ω 2 ± ω 3 , 2 ω 1 + ω 2 , . . . . Sum- and difference-frequency generation. T ING Z HOU Northeastern University HKUST

  13. Kerr-type Nonlinearity Introduction Construction of CGO solutions Nonlinear Maxwell’s Equations Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) Nonlinearity Lossy media: complex valued. Equivalence to time-domain ME: � ∞ � ∞ P ( 2 ) = R ( 2 ) ( τ 1 , τ 2 ) E ( t − τ 1 ) E ( t − τ 2 ) d τ 1 d τ 2 . 0 0 Using Fourier transform, � ∞ � ∞ R ( 2 ) ( τ 1 , τ 2 ) e i ω ( τ 1 + τ 2 ) d τ 1 d τ 2 . χ ( 2 ) ( ω 1 , ω 2 ; ω 1 + ω 2 ) = 0 0 T ING Z HOU Northeastern University HKUST

  14. Kerr-type Nonlinearity Introduction Construction of CGO solutions Nonlinear Maxwell’s Equations Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) Kerr-type Nonlinear Media We are interested in time-harmonic electromagnetic fields with frequency ω > 0: E ( x , t ) = E ( x ) e − i ω t + E ( x ) e i ω t , H ( x , t ) = H ( x ) e − i ω t + H ( x ) e i ω t . A model of nonlinear media of Kerr type: � � T � x , 1 |E ( x , t ) | 2 dt E ( x , t ) = a ( x ) | E ( x ) | 2 E ( x , t ) P NL ( x , E ( x , t )) = χ e T 0 � � T � x , 1 |H ( x , t ) | 2 dt H ( x , t ) = b ( x ) | H ( x ) | 2 H ( x , t ) . M NL ( x , H ( x , t )) = χ m T 0 Kerr-type electric polarization: third order susceptibility χ ( 3 ) e ( ω, ω, ω ; ω ) = a ( x ) common in nonlinear optics; Kerr-type magnetization: χ ( 3 ) m ( ω, ω, ω ; ω ) = b ( x ) appears in certain metamaterials; T ING Z HOU Northeastern University HKUST

  15. Kerr-type Nonlinearity Introduction Construction of CGO solutions Nonlinear Maxwell’s Equations Continue the proof for the case of Kerr-type nonlinearity Second Harmonic Generation (SHG) Maxwell’s Equations with the Kerr-type Nonlinearity This leads to the nonlinear time-harmonic Maxwell’s equations � ∇ × E = i ωµ H + i ω b | H | 2 H Ω ⊂ R 3 . in ∇ × H = − i ωε E − i ω a | E | 2 E . Electromagnetic measurements on ∂ Ω are modeled by the admittance map Λ ω ε,µ, a , b : ν × E | ∂ Ω �→ ν × H | ∂ Ω . Inverse Problem: Determine ε, µ, a , b from Λ ω ε,µ, a , b . T ING Z HOU Northeastern University HKUST

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