Electromagnetically Induced Flows in Water

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1 Electromagnetically Induced Flows in Water Michiel de Reus 8 maart 213 () Electromagnetically Induced Flows 1 / 56

2 Outline 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 2 / 56

3 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 3 / 56

4 Introduction Optical trapping consist of: Focussed laser beam is applied in fluid. Small particles are trapped by electromagnetic force. () Electromagnetically Induced Flows 4 / 56

5 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 5 / 56

6 Maxwell equations The macroscopic Maxwell equations in vacuum: E H + ε t H E + µ t = J, = K. Compatibility relations E = and H =. E(x, t), (time domain) electric field, H(x, t), (time domain) magnetic field, J(x, t), total electric current density, K(x, t), total magnetic current density. () Electromagnetically Induced Flows 6 / 56

7 Electric current density The current density consists of three terms: J p, polarization current, J f, free (conduction) current, J ext, external current. Induced current is given by J ind = J p + J f. The induced currents depend on E, so J ind = J ind (E). So-called constitutive relations. The external current is independent of E and H. () Electromagnetically Induced Flows 7 / 56

8 Induced currents Linear polarization, instantaneous response: J p = ε χ e E t, with χ e the electric susceptibility. Free current is proportional to the electric field (Ohm s law): with σ the electric conductivity. J f = σe, () Electromagnetically Induced Flows 8 / 56

9 Maxwell equations in (rigid) matter Substitution results in: H + ε E t + σe = Jext, E + µ H t Electric permittivity given by: ε = (1 + χ e )ε. =. () Electromagnetically Induced Flows 9 / 56

10 Maxwell equations in fluids Fluid in motion: movement w.r.t. the reference frame. Induced currents because of charges moving: J rel = (µ ε µ ε )v H, K rel = (µ ε µ ε )v E, v 1, effect will be neglected. () Electromagnetically Induced Flows 1 / 56

11 Energy equation (1) Define the electromagnetic energy density as u em = 1 ( ε E 2 + µ H 2), 2 and the Poynting vector as S = E H. Then from the Maxwell equations one can derive: t u em = S E J H K. () Electromagnetically Induced Flows 11 / 56

12 Energy equation (2) For linear polarization we had: This results in: J = (ε ε ) E t + σe. t u em = S 1 2 (ε ε ) t E 2 σ E 2. The polarization term in general oscillates. The conduction term is strictly negative, so acts as an energy sink. () Electromagnetically Induced Flows 12 / 56

13 Momentum equation Likewise we can derive the momentum equation: f = S t + T. Here T is the Maxwell stress tensor given by T = µ H H + ε E E 1 2 µ H 2 I 1 2 ε E 2 I. The force density is given by: f = ( E)E + ( H)H + µ J H ε K E. () Electromagnetically Induced Flows 13 / 56

14 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 14 / 56

15 Monochromatic source External current density of only one frequency: J ext (x, t) = J ext (x) cos(ωt + δ). Resulting fields are also time-harmonic: with a possible phase-shift. E(x, t) = Ẽ(x) cos(ωt + δ 1 ), H(x, t) = H(x) cos(ωt + δ 2 ), () Electromagnetically Induced Flows 15 / 56

16 Complex fields (1) Notice that we can write: Like-wise for the fields: J ext (x, t) = Re {Ĵext (x)e ıωt}. E(x, t) = Re {Ê(x)e ıωt }, H(x, t) = Re {Ĥ(x)e ıωt }. The phase-shifts are absorbed in Ĵ ext, Ê and Ĥ. () Electromagnetically Induced Flows 16 / 56

17 Complex fields (2) Time derivatives become complex multiplications: {Ê(x)e } { t Re ıωt = Re ıωê(x)e ıωt}. Substitution in the Maxwell equations results in: {[ ] Re Ĥ(x) ıωε Ê(x) e ıωt} { = Re Ĵ(x)e ıωt}, {[ ] Re Ê(x) ıωµ Ĥ(x) e ıωt} =, () Electromagnetically Induced Flows 17 / 56

18 Complex polarization (1) Linear polarization, J p = ε χ e E t is non-physical. Better form, temporal dependency, localized in space: J p = ε f (τ) E (x, t τ) dτ. t The complex form is given by: [ ] } J p = Re { ıωε f (τ)e ıωτ dτ Ê(x)e ıωt. () Electromagnetically Induced Flows 18 / 56

19 Complex polarization (2) The complex permittivity is defined as ˆε = ε + ıε. The real part gives the polarization current: ε (ω) = ε f (τ)e ıωτ dτ. The imaginary part gives the free current: ε (ω) = σ(ω) ω. () Electromagnetically Induced Flows 19 / 56

20 Complex Maxwell equations (1) The (complex) induced current is then given by: Ĵ ind = ıω(ˆε ε )Ê. Substitution in the Maxwell equations results in: {[ ] Re Ĥ(x) ıωˆεê(x) e ıωt} { = Re Ĵ ext (x)e ıωt}, {[ ] Re Ê(x) ıωµ Ĥ(x) e ıωt} =. The two separate induced currents form one complex term. () Electromagnetically Induced Flows 2 / 56

21 Complex Maxwell equations (2) Finally, drop the real parts, and strip off e ıωt. The resulting complex Maxwell equations are: Ĥ(x) ıωˆεê(x) = Ĵ ext (x), Ê(x) ıωµ Ĥ(x) =. The compatibility relations are: Ĥ = and Ê =. The equations no longer depend on the time variable t. () Electromagnetically Induced Flows 21 / 56

22 Time Averaging (1) The frequencies are extremely large compared to all the movement in the liquid: f = Hz for λ = 1.2 µm. The quantities are time-averaged: f (x, t) = 1 T T 2 T 2 Re {ˆf (x)e ıωt} dt. f (x, t) can be replaced by other quantities. () Electromagnetically Induced Flows 22 / 56

23 Time Averaging (2) The results for different quantities are: E(x, t) =, E(x, t) E(x, t) = 1 } {Ê(x) 2 Re Ê (x), S(x, t) = E(x, t) H(x, t) = 1 } {Ê(x) 2 Re Ĥ (x), [E(x, t) E(x, t)] =. t () Electromagnetically Induced Flows 23 / 56

24 Time-averaged energy equation (1) The time-averaged energy equation is given by: t u em = S E J. Using the time-harmonic representation, we have: Ĵ = ıω(ˆε ε )Ê. Also we define the complex Poynting vector Ŝ = 1 2Ê Ĥ. () Electromagnetically Induced Flows 24 / 56

25 Time-averaged energy equation (2) Substitution of the time-averaged expressions results in: } = Re {Ŝ 1 2 ωε Ê Ê. } We have Re {Ŝ the time-averaged energy flux. The second term shows the time-averaged dissipation: q em = 1 2 ωε Ê Ê. The electromagnetic energy is transformed to heat. () Electromagnetically Induced Flows 25 / 56

26 Time-averaged Lorentz force (1) The time-averaged Lorentz force is given by f = µ J H. Using again the relation Ĵ = ıω(ˆε ε )Ê, the time-averaged result is f = 1 { } 2 µ Re ıω(ˆε ε )Ê Ĥ, } }] = ωµ [ε Re {Ŝ + (ε ε )Im {Ŝ. () Electromagnetically Induced Flows 26 / 56

27 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 27 / 56

28 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 28 / 56

29 GB: properties Properties of the Gaussian beam model: Widely used to model laser beams, analytical solution available, Transforms easily through lens systems, only the parameters change, Gaussian decay (e cr 2 ) in axial direction, Only an approximation, does not satisfy the Maxwell equations. () Electromagnetically Induced Flows 29 / 56

30 GB: derivation (1) The Maxwell equations are rewritten in terms of a vector potential Â. The potential is assumed to have the form: With: Â(x, y, z) = ψ(x, y)e ıˆkzŷ. z the propagation direction, y the polarization direction, ˆk the (complex) wave number, ˆε = ε c 2 ω 2 ˆk 2. () Electromagnetically Induced Flows 3 / 56

31 GB: derivation (2) ψ is expanded around ŝ 2 = The zero order term is used: ψ = w ( w(z) exp ıˆk ρ 2 2R(z) ρ is the axial distance x 2 + y 2. ( ) 2 λ. 2πw ˆn Expected accuracy of order O( ŝ 2 ). ρ2 w(z) 2 ıα ρ 2 ) k w(z) 2 ıζ(z). () Electromagnetically Induced Flows 31 / 56

32 GB: electric field Electric field has two components: E pol = E exp(ıˆkz)ψ, ( E prop = E exp ıˆkz ) ψ [ 1 R(z) 2ı ˆkw(z) 2 + 2α kˆkw(z) 2 ] y, () Electromagnetically Induced Flows 32 / 56

33 GB: accuracy 1 1 n = 32 n = 64 n = 96 1 n = 128 O( s 2 ) n = 32 n = 64 n = 96 n = 128 O( s 2 ) res gb 1 1 res f s s Figuur: Residual of the Maxwell equations and moment equation. Accurate to order O( ŝ 2 ). We have.15 < ŝ <.4. () Electromagnetically Induced Flows 33 / 56

34 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 34 / 56

35 Gaussian dipole array The goal is to: Create a source that does satisfy the Maxwell equations, that resembles a Gaussian beam (focussing, exponential radial decay). The idea is to combine a lot of simple, exact solutions for perfect dipoles. () Electromagnetically Induced Flows 35 / 56

36 Perfect dipole (1) The perfect dipole is a simple point source. The external current density is given by: with Ĵ ext (x, t) = δ(x x s )I cos(ωt ϕ)ˆd, δ(x x s ) localizes the source at x s. ˆd is the orientation of the point source. Using Green s functions we can derive an analytic expression for the electric and magnetic field for the dipole. () Electromagnetically Induced Flows 36 / 56

37 Perfect dipole (2) Fields resulting from the dipole: [ ( 1 Ê = ıωµ I g(r) ˆd (ˆd ˆr)ˆr + Ĥ = I g(r) ( ıˆk 1 r ) ˆr ˆd. ˆk 2 r 2 ı ˆkr ) ( ) ] 3(ˆd ˆr)ˆr ˆd, The Green s function is given by g(r) = 1 4πr eıˆkr, r = x x s. () Electromagnetically Induced Flows 37 / 56

38 External current density The external current density is prescribed such that: It is zero everywhere outside the source plane, The source plane is divided in a rectangular grid, For each grid point Ĵ ext is proportional to Ê gb. The field in the domain is calculated using the Green s function. () Electromagnetically Induced Flows 38 / 56

Resulting field y y y y 1 λ = 1.2 µm, yz plane, gb λ = 1.2 µm, yz plane, dipole 1 5 5 1 5 1 z λ = 2.4 µm, yz plane, gb 5 1 z λ = 2.

39 Resulting field y y y y 1 λ = 1.2 µm, yz plane, gb λ = 1.2 µm, yz plane, dipole z λ = 2.4 µm, yz plane, gb 5 1 z λ = 2.4 µm, yz plane, dipole z 5 1 z This methods results in: Similar fields for small wavelengths. Deviations for larger wavelengths: larger ŝ value. Constant I : Numerically normalized incoming power. () Electromagnetically Induced Flows 39 / 56

40 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 4 / 56

41 Basis of the NS equations. The equations are based on: Conservation of mass and incompressibility: continuity equation, v =. Conservation of momentum: Navier-Stokes equations, including f em. Boussinesq approximation: Gravity driven buoyancy effects in NS equations. Conservation of energy: temperature equation with source term q em. () Electromagnetically Induced Flows 41 / 56

42 Incompressible Navier Stokes equations. For the simulations we have used the equations: i v i =, ρ v j j v i = i p + gyδ i2 2 ρ + µ 2 j v i + f em i, ρ c p v i i T = k 2 i T + q em, Steady-state equations, with p = p + ρgy the modified pressure, ρ = ρ (1 β(t T )). f em the electromagnetic force density, q em the electromagnetic heat dissipation. () Electromagnetically Induced Flows 42 / 56

43 Solving algorithm: SIMPLE (1) Semi-Implicit Method for Pressure Linked Equations. Not that simple: Pressure and velocity are coupled, Non-linear system. Each equation is solved separately. This is iterated until solution is reached. Differentiation is discretized using central differences, Integrations are discretized using a midpoint rule. () Electromagnetically Induced Flows 43 / 56

44 Solving algorithm: SIMPLE (2) The iterative procedure is given by: u i+1 is solved by using p i and u i (to handle the non-linearity), T i+1 is solved using u i+1, ρ i+1 is solved using T i+1, p i+1 is solved using u i+1 and ρ i+1. u i+1 is corrected using p i+1 to satisfy the continuity equation. Repeated until tolerance is met. () Electromagnetically Induced Flows 44 / 56

45 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 45 / 56

46 Frequencies in water 1.5 δ ε rel ε rel λ [µm] Four wavelengths are selected, One small one, 1.2µm, no losses, One larger one, 2.4µm, almost no losses, Two larger ones, 2.8µm and 3.2µm, with larger losses. () Electromagnetically Induced Flows 46 / 56

47 Intensities y y y y x x x x y y y y 1 λ = 1.2 µm, xy plane 1 λ = 1.2 µm, xz plane 1 λ = 1.2 µm, yz plane x λ = 2.4 µm, xy plane z λ = 2.4 µm, xz plane z λ = 2.4 µm, yz plane x λ = 2.8 µm, xy plane z λ = 2.8 µm, xz plane z λ = 2.8 µm, yz plane x λ = 3.2 µm, xy plane 5 1 z λ = 3.2 µm, xz plane z λ = 3.2 µm, yz plane x 5 1 z 5 1 z Figuur: Intensities for the four different wavelenghts, using the dipole array method. () Electromagnetically Induced Flows 47 / 56

48 Force density (1) y y y y 6.5 x 1 6 λ = x 1 6 λ = x 6 x x 1 6 λ = x 6 x x 1 6 λ = x x x x 1 Figuur: Force density in plane perpendicular to propagation. Polarization direction: Away from the centre, Perpendicular direction: Towards the centre () Electromagnetically Induced Flows 48 / 56

49 Force density (2) x x y y 6.5 x 1 6 λ = 1.2 x 1 6 λ = z x x λ = z x x λ = z 4 5 x z 4 5 x 1 Figuur: Force density for 1.2µm and 2.4µm, z direction. No component in propagation direction. () Electromagnetically Induced Flows 49 / 56

50 Force density (3) x x y y 6.5 x 1 6 λ = x 1 6 λ = z 3 4 x z 3 4 x x 1 6 λ = x 1 6 λ = z 3 4 x z 3 4 x 1 Figuur: Force density for 2.8µm and 3.2µm, z direction. Relatively large component in propagation direction. () Electromagnetically Induced Flows 5 / 56

51 Resulting velocity y y y y 1 x 1 5 λ = x 1 5 λ = x 1 x 1 1 x 1 5 λ = x 1 x 1 1 x 1 5 λ = x 1 x 1.5 x 1 x 1 Velocity in the xy-plane, at the point of focus. Streamlines indicate circular motion for small wavelengths. () Electromagnetically Induced Flows 51 / 56

52 Temperature rise For P = 1mW, maximum temperature rise is given by: wavelength Energy absorbed max. T 1.2 µm µm µm µm For P = 5mW, maximum temperature rise is given by: wavelength max. T 1.2 µm µm 95.2 The Boussinesq approximation is only valid for small increases. () Electromagnetically Induced Flows 52 / 56

53 1 Introduction 2 Maxwell equations Complex Maxwell equations 3 Gaussian sources Gaussian beam Gaussian dipole array 4 Incompressible Navier Stokes equations 5 Simulations 6 Conclusion and future research () Electromagnetically Induced Flows 53 / 56

54 Conclusion Some conclusions drawn from the simulations: The dipole array is an adequate alternative for the GB, No losses: Force density leads to loops, Losses: Complicated flows, large component in propagation direction. Temperature increase is too large, Boussinesq not valid, Use of compressible Navier-Stokes to capture total flow. () Electromagnetically Induced Flows 54 / 56

55 Further research More work needs to be done at: Establishing whether the correct force is used. Use compressible NS to capture effect due to heat. Temperature dependent viscosity. Experimental set-up, to capture characteristic flow. Investigate possible back-action by fluid on fields. () Electromagnetically Induced Flows 55 / 56

56 Electromagnetically Induced Flows in Water Michiel de Reus 8 maart 213 () Electromagnetically Induced Flows 56 / 56

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