Faraday’s Cage Acoustic and Electric Faraday Cages P. A. Martin Colorado School of Mines “Everybody knows Faraday’s cage or metal-lined room, into which he went with electroscopes, birds, frogs, and other instruments, arranged that the outside should receive violent flashes, and detected nothing inside.” Oliver Lodge, 1890 Acknowledgment: D. P. Hewett (Oxford) Faraday’s Cage: how does it work? A quick gives A Faraday cage’s operation depends on the fact that an external static electrical field will cause the electrical charges within the cage’s conducting material to redistribute themselves so as to cancel the field’s effects in the cage’s interior. Faraday’s Cage: how does it work? A quick gives A Faraday cage’s operation depends on the fact that an external static electrical field will cause the electrical charges within the cage’s conducting material to redistribute themselves so as to cancel the field’s effects in the cage’s interior. This is the classic explanation for a closed conductor – but what is the effect of the holes, the gaps between the wires in the cage? We consider such problems for electrostatics (∇2 V = 0) and for acoustics (∇2 u + k 2 u = 0). First, we need a model . . . Hertz’s “Mouse-Mill”: a Ring of Parallel Wires Hertz’s “Mouse-Mill”: a Ring of Parallel Wires b Terminology and figure taken from 1890 paper by O. Lodge. Also reprinted in his 1892 book: Terminology and figure taken from 1890 paper by O. Lodge. Also reprinted in his 1892 book: O N wires equally spaced around a circle of radius b, the “ring”. Hertz’s “Mouse-Mill”: a Ring of Parallel Wires Solution for Complete Ring: Acoustics I b Terminology and figure taken from 1890 paper by O. Lodge. Also reprinted in his 1892 book: I x = r cos θ, O N wires equally spaced around a circle of radius b, the “ring”. Does the solution for this problem converge to solution for the ring as N → ∞? If so, what is the rate of convergence? Solve Helmholtz equation, ∇2 u + k 2 u = 0, for u(r , θ) outside a circle (the “ring”) of radius b ∞ X ikx Solution: u(r , θ) = e + cn Hn (kr )einθ n=−∞ Hn = Hankel function I First term is incident wave I Summation gives effect of the ring: for “soft” ring u=0 on circle r = b cn = −i n [Jn (kb)]/[Hn (kb)], Jn = Bessel function Does the solution for the cage, with N wires equally spaced around the ring, approach the solution for a single ring as N → ∞? b O Maxwell’s Infinite Grating: ∇2 V = 0 Electrostatic Solution for Complete Ring I Solve Laplace’s equation, ∇2 V = 0, for V (x, y) outside a circle (the “ring”) of radius b p b2 y Solution: V (x, y) = y − 2 , r = x 2 + y 2 r First term is uniform field at infinity I Second term is effect of the conducting ring, I I V =0 Note exponential decay. on circle r = b W = AV + C is another solution. Adjust constants A and C so that Does the solution for the cage, with N wires equally spaced around the ring, approach the solution for a single ring as N → ∞? b I W has the desired behaviour as Y →∞ I W ' 0 on small circles (wires) at Y = 0, X = 2nπ. O There are classical results for an infinite straight row of wires . . . Acoustic Scattering by N Scatterers e−iωt , 354 Phys. perspect. This is example of an inverse method. Philip L. Taylor and William J. Fickinger Leslie L. Foldy (1919–2001) (∇2 + k 2 )u I N sound-soft scatterers in 2D, I For N circles, this problem can be solved exactly using multipole methods, but we are interested in N 1. I 1 log 1 − 2eY cos X + e 2Y 2 Y − e−Y cos X , Y → +∞ V ∼ −eY cos X , Y → −∞ V = =0 Born László Földi in Czechoslovakia. Emigrated to USA, 1920 I BS in Physics, Case Western Reserve University, Cleveland, Ohio, 1941 I MS, Wisconsin, with Léon Brillouin, 1942 We use Foldy’s method. For one scatterer at the origin, basic assumption is that we can represent the total field as u(r) = uinc (r) + guinc (0)H0 (k |r|) (1) (1) I I 1942–1945: New York uinc = incident field H0 = H0 = Hankel function. g = scattering coefficient. For circular scatterer, radius a, can take g = −[J0 (ka)]/[H0 (ka)]. I I PhD, Princeton, 1948, with Oppenheimer The assumption (1) says the scattering is isotropic. It is justified for small soft (u = 0 on boundary) scatterers. I Then, back to Case for entire career Fig. 5. Leslie Foldy (1919–2001) in 1974. Credit: Courtesy of Frank Cverna. P.L. Taylor & W.J. Fickinger, Physics in Perspective 9 (2007) 346–356 lege to be his colleagues at Case Western Reserve University, where he remained for Foldy in New York (1942–1945) Foldy’s Method (1945) I Underwater Sound Laboratory, Division of War Research, Columbia University I 64th floor, Empire State Building [J. B. Keller also there] I Problem: understand transmission of sound through submarine wakes, and echoes received from wakes Scattering by N identical small objects (cylinders, wires). Assume each scatters isotropically: u(r) = uinc (r) + Cylinders centred at r = rj . The “exciting field” for n th cylinder is incident field + field scattered by all the other cylinders: Scattering by a Ring of Identical Small Scatterers n th scatterer at θ = nh, where h = 2π/N is angular spacing I b Foldy linear system is N X Cn−j Aj = fn , j=1 C0 = −g −1 , I θ O Aj H0 (k|r − rj |), Solution Recall system: N X Cj = H0 (2kb| sin (jπ/N)|), j 6= 0 mod N The system matrix is a circulant matrix: we can solve for Aj using discrete Fourier transforms . . . n = 1, 2, . . . , N j=1 N X Aj φ mj j=1 [Cj+mN = Cj , all m], Cn−j Aj = fn , Discrete Fourier transform: Ãm = n = 1, 2, . . . , N where fn = −uinc (rn ), Cj is N-periodic N X (3) Evaluate (3) at r = rn . As An = gun (rn ) for self-consistency, we get linear N × N system for Aj . Solve. Then put these numbers in (2) to get u(r). We apply this method to a ring of scatterers . . . Saturday 28 July 1945 I (2) j=1 j6=n Bubbly liquids behind ◦◦ ◦◦ ◦ Scatterers at rn , n = 1, 2, . . . , N. Aj H0 (k|r − rj |) j=1 un (r) = uinc (r) + I N X Solution: N 1X Am = Ãj φ−mj N φ = e2πi/N j=1 Ãn = f̃n /C̃n At centre of the ring: u(0) = uinc (0) + Ã0 H0 (kb) The far-field pattern is also expressible in terms of Ãn Dependence on N: f̃n Recall: Ãn = f̃n /C̃n . Trapezoidal Rule I Start with f̃n . Basic formula. Z Incident plane wave, uinc (r) = eikx = eikr cos θ . As fj = −uinc (rj ), f̃n = N X nj fj φ = − j=1 N X 2π 0 e ikb cos (jh) e Let h = 2π/N. N−1 X h h F (θ) dθ ' F (0) + h F (jh) + F (2π) 2 2 j=1 injh I j=1 When F (0) = F (2π), Z where h = 2π/N and φ = eih . 0 RHS looks like (repeated) trapezoidal rule: N X f̃n =h F (jh), N j=1 2π 1 F (θ) = − eikb cos θ einθ 2π I F (θ) dθ ' h N X F (jh) j=1 When F is 2π-periodic and smooth, the error goes down exponentially fast as N increases. L.N. Trefethen and J.A.C. Weideman, The exponentially convergent trapezoidal rule. SIAM Review 56 (2014) 385–458. Dependence on N: f̃n Dependence on N: f̃n Incident plane wave, uinc (r) = eikx = eikr cos θ . As fj = −uinc (rj ), f̃n = N X nj fj φ = − j=1 N X e ikb cos (jh) e injh j=1 f̃n = j=1 where h = 2π/N and φ = eih . RHS looks like (repeated) trapezoidal rule: N X f̃n F (jh), =h N Incident plane wave, uinc (r) = eikx = eikr cos θ . As fj = −uinc (rj ), 1 F (θ) = − eikb cos θ einθ 2π N X nj fj φ = − j=1 N X eikb cos (jh) einjh j=1 where h = 2π/N and φ = eih . RHS looks like (repeated) trapezoidal rule: N X f̃n F (jh), =h N j=1 F (θ) = − 1 ikb cos θ inθ e e 2π As F (θ) is entire 2π-periodic function of θ, the trapezoidal rule converges exponentially fast, f̃n ∼ N Z 0 2π F (θ) dθ = −i n Jn (kb), N → ∞. Dependence on N: C̃n Recall: Ãn = f̃n /C̃n . N−1 X 1 C̃n =h v (jh) − , N gN j=1 Dependence on N: C̃n Next, C̃n : Recall: Next, C̃n : N−1 X 1 C̃n =h v (jh) − , N gN einθ v (θ) = H0 (2kb | sin (θ/2)|) 2π v (θ) is 2π-periodic but there are log singularities at θ = 0, 2π. The sum looks like the trapezoidal rule in which the endpoint contributions have been “ignored”. Ãn = f̃n /C̃n . j=1 v (θ) = einθ H0 (2kb | sin (θ/2)|) 2π v (θ) is 2π-periodic but there are log singularities at θ = 0, 2π. The sum looks like the trapezoidal rule in which the endpoint contributions have been “ignored”. Fortunately (for me), the convergence of such quadrature rules has been studied. A theorem of A. Sidi (2004) shows that the sum converges to Z 0 2π v (θ) dθ = Jn (kb) Hn (kb), but the error is O(N −1 log N): it’s a very poor quadrature rule! In fact, Sidi gives an asymptotic expansion for the error: the error estimate is sharp. Dependence on N: Ãn I I I For fixed n, − in log N Ãn = +O , Hn (kb) N Concluding Remarks I The slow convergence with N is surprising (to me). It contrasts with the exponential convergence with distance seen with Maxwell’s grating. I We have made similar calculations for potential problems (Laplace’s equation). This required a (new?) static version of Foldy’s method. I Extension to sound-hard scatterers would require a modified form of Foldy’s method, with dipole contributions. I Direct extension to three dimensions is not possible because there is no analogous circulant structure. I Reference: Proc. Roy. Soc. A 470 (2014) I Related work by Chapman, Hewett & Trefethen, using very different methods, on potential problems. Finally: Ãn = f̃n /C̃n . N → ∞. The leading-order term shows that we recover the expected far-field pattern for scattering by a sound-soft circle of radius b. The total field at the centre of the ring vanishes slowly, as N −1 log N.