Advanced Techniques for Calculating Electric Potentials

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Explore specialized methods including Laplace's equation, the method of images, separation of variables, and multipole expansion for calculating electric potentials. Learn about boundary conditions, uniqueness theorems, harmonic functions, and numerical relaxation methods for solving Laplace's equation. Dive into one-dimensional Laplace's equation and discover the method of relaxation through a numerical example.

  • Electric Potentials
  • Laplaces Equation
  • Boundary Conditions
  • Harmonic Functions
  • Numerical Methods

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  1. Chapter 3 Special Techniques for Calculating Potential 3.1 Laplace s Equation 3.2 The Method of Images 3.3 Separation of Variables 3.4 Multipole Expansion

  2. 3.1 Laplaces Equation 3.1.1 Introduction 3.1.2 Laplace s Equation in One Dimension 3.1.3 Laplace s Equation in Two Dimensions 3.1.4 Laplace s Equation in Three Dimensions 3.1.5 Boundary Conditions and Uniqueness Theorems 3.1.6 Conducts and the Second Uniqueness Theorem

  3. 3.1.1 Introduction The primary task of electrostatics is to study the interaction (force) of a given stationary charges. = since F q E test 1 R R = ( ) E d 4 2 0 this integrals can be difficult (unless there is symmetry) x y z E E x E y E z = + + + we usually calculate 1 4 = 1 R = ( ) V d 0 E V This integral is often too tough to handle analytically.

  4. 3.1.1 In differential form Eq.(2.21): Poisson s eq. 2 = V 0 to solve a differential eq. we need boundary conditions. In case of = 0, Poisson s eq. reduces to 2 Laplace s eq = 0 V T q 1 h 1 h 2 or = = 0 ( ) V A i q k i i i k 2 2 2 V x V y V z + + = 0 2 2 2 The solutions of Laplace s eq are called harmonic function.

  5. 3.1.2 Laplaces Equation in One Dimension 2 0 V mx b dx m, bare to be determined by B.C.s ( 1) 4 ( 5) 0 5 V x b = = = V=4 V=0 d V = = + 2 = = = V x 1 m e.q., = + 5 V x x 1 5 1. V(x)is the average of V(x + R)and V(x - R), for any R: 2 1 = + + ( ) ( ) ( ) V x V x R V x R 2. Laplace s equation tolerates no local maxima or minima.

  6. 3.1.2 (2) Method of relaxation: A numerical method to solve Laplace equation. Starting V at the boundary and guess V on a grid of interior points. Reassign each point with the average of its nearest neighbors. Repeat this process till they converge.

  7. 3.1.2 (3) The example of relaxation n 0 1 2 3 4 5 6 7 8 9 10 V(x=0)V(x=1)V(x=2)V(x=3)V(x=4) 4 0 0 4 2 0 4 2 1 4 1 4 4 4 4 4 4 4 16 2 16 1 0 0 0 1 0 0 0 0 0 0 0 0 0 0 0 2 1 1 2 2 1 2 1 1 2 1 2 3 2 3 2 1 4 3 2 3 4 4 3 2 1 4 7 4 3 8 7 2 1 8 7 4 7 8 7 2 1 8 15 8 7 16 5 2 1 16 15 8 15 16 15 4 3 2 1 0

  8. 3.1.3 Laplaces Equation in Two Dimensions A partial differential eq. : 2 V x 2 V y + = 0 2 2 There is no general solution. The solution will be given in 3.3. We discuss certain general properties for now. 1. The value of V at a point (x, y)is the average of those around the point. 1 ( , ) 2 circle R = V x y Vdl 2. V has no local maxima or minima; all extreme occur at the boundaries. 3. The method of relaxation can be applied.

  9. 3.1.4 Laplaces Equation in Three Dimensions 1. The value of V at point P is the average value of V over a spherical surface of radius R centered at P: 1 ( ) 4 R 2 2 2 1 , 2 4 rr 2 2 2 0 4 4 R 2 2 1 2 4 2 rR ( ) ( 0 4 2 rR = V p Vda 2 sphere q = = + cos V r R rR 0 1 2 q 1 2 = + d d [ 2 cos ] sin V r R rR R ave q = + cos ) R r R rR 0 0 q q r 1 1 = + = = r R r at the center of the sphere V 4 0 The same for a collection of q by the superposition principle. 2. As a consequence, V can have no local maxima or minima; the extreme values of V must occur at the boundaries. 3. The method of relaxation can be applied.

  10. 3.1.5 Boundary Conditions and Uniqueness Theorems in 1D, one end the other end = + V mx b Vb Va V is uniquely determined by its value at the boundary. First uniqueness theorem : the solution to Laplace s equation in some region is uniquely determined, if the value of V is specified on all their surfaces; the outer boundary could be at infinity, where V is ordinarily taken to be zero.

  11. 3.1.5 Proof: Suppose V1, V2are solutions 2 1 0 V = 2 = = 0 V 2? V V 2 1 = V V V 3 1 2 2 2 2 = = 0 V V V 3 1 2 = = at boundary. at boundary 0 V V V 1 2 3 V3 = 0 everywhere hence V1 = V2everywhere

  12. 3.1.5 The first uniqueness theorem applies to regions with charge. 2 Proof. 2 = = V V 1 2 0 0 = V V V 3 1 2 2 2 2 = = + = 0 V V V 3 1 2 0 0 at boundary. = = = 0 V V V V 3 1 2 i e V = 0, . ., V 1 2 3 Corollary : The potential in some region is uniquely determined if (a) the charge density throughout the region, and (b) the value of V on all boundaries, are specified.

  13. 3.1.6 Conductors and the Second Uniqueness Theorem Second uniqueness theorem: In a region containing conductors and filled with a specified charge density , the electric field is uniquely determined if the total charge on each conductor is given. (The region as a whole can be bounded by another conductor, or else unbounded.) Proof: E E Suppose both and are satisfied. 1 1 E = 1 2 1 = E 2 0 0 and 1 1 E da = = , Q E da Q 1 1 2 2 i i 0 0 ith conducting surface ith conducting surface , tot Q 1 1 E da = = E da Q 1 2 tot 0 0 outer bourndary outer bourndary

  14. 3.1.6 = E E E define 3 1 2 = = = = ( ) 0 E E E E E 3 1 2 1 2 0 0 = E da = 0 E da E da 3 1 2 for V3 is a constant over each conducting surface = + 2 3 = ( ) ( ) ( ) 3 3 V E V E E V E 3 3 3 3 2 3 volume = = = ( ) E d 3 3 V E d 3 3 V E da surface 0 = V E da 3 3 surface = = i. e., 0 E E E 3 1 2

  15. 3.2 The Method of Images 3.2.1 The Classical Image Problem 3.2.2 The Induced Surface Charge 3.2.3 Force and Energy 3.2.4 Other Image Problems

  16. 3.2.1 The Classical Image Problem B.C. ( ) = = 1. 0 0 V z 2 2 2 2 + + 2. 0 V for x y z d What is V (z>0) ? The first uniqueness theorem guarantees that there is only one solution. If we can get one any means, that is the only answer.

  17. 3.2.1 = = = E E E z E = = Trick : z Only care z > 0 0 x y 0 at z or E z < 0 is not of concern 0 V(z=0) = const = 0 ( ) 0 E z = 0 in original problem for z 0 1 q q = + ( , , ) V x y z 4 2 2 ( ) ( ) 2 2 2 2 + + + + + 0 x y z d x y z d

  18. 3.2.2 The Induced Surface Charge Q E da = 0 at z Eq.(2.49) 0 V z = A 0 = = E A E z z = 0 z 0 0 V z = = = z z E V 0 1 q q = 4 z 2 2 ( ) ( ) 2 2 2 2 + + + + + x y z d x y z d = 0 z

  19. 3.2.2 1 2 1 2 + 2( ) 2( ) z d z d q = 3 2 3 2 4 2 2 2 2 2 2 + + + + + ( ) ( ) x y z d x y z d = 0 z qd qd = = 3/2 3/2 2 2 2 2 2 + + + 2 2 x y d r d total induced surface charge 2 0 qd = = Q da rdrd 3/2 0 2 2 + 2 r d 1 = = qd q 0 Q=-q 1/2 2 2 + r d

  20. 3.2.3 Force and Energy The charge q is attracted toward the plane. The force of attraction is ( ) ( ) 0 d d 2 q q 1 1 q = = z z F 2 2 ( ) 4 4 2 d 0 With 2 point charges and no conducting plane, the energy is 2 1 2 i = = + + ( ) = W i i qV p Eq.(2.36) i 1 1 2 1 1 q q ( ) q ( ) q 4 4 d d 2 ( ) 0 0 d d 2 1 q = ( ) 4 2 d 0

  21. 3.2.3 (2) For point charge q and the conducting plane at z = 0 the energy is half of the energy given at above, because the field exist only at z 0 ,and is zero at z < 0 ; that is 2 1 q = or W ( ) 4 4 d 0 2 1 q d d = F dl = W dz = ( ) dl dlz 2 ( ) 4 2 z 0 2 2 1 1 q q d = = ( ) 4 4 4 4 z d 0 0

  22. 3.2.4 Other Image Problems Stationary distribution of charge 1q 1q 2 q 2 q 3 q 3 q

  23. 3.2.4 (2) Conducting sphere of radius R R a 2 = q q Image charge R a = at b 1 q r r q 1 2 ( ) = + , V r r r 2 2 = + 2 cos r a ra 4 0 1 2 1 q q 2 2 = + = + 2 cos r b rb 4 rr as rr bs 0 1 q q = + a r r b 4 0 s r s r r b

  24. 3.2.4 (3) 1 q q ( ) = + = , 0 V R a R R b 4 0 s r s R r b 2 a R R b R a = = b q R q b b R R a = = = q q q 2 1 1 qq q Ra = = F Force ( ) 2 2 ( ) 4 4 a b 2 2 0 0 a R [Note : how about conducting circular cylinder?]

  25. 3.3 Separation of Variables 3.3.0 Fourier series and Fourier transform 3.3.1 Cartesian Coordinate 3.3.2 Spherical Coordinate

  26. 3.3.0 Fourier series and Fourier transform Basic set of unit vectors in a certain coordinate can express any vector uniquely in the space represented by the coordinate. e.g. z V y V x V i V V z y x i 1 = V V V , , N = = + + in 3D. Cartesian Coordinate. i , , x y z are unique because are orthogonal. j i x y z i j 0 1 = = i j Completeness: a set of function ( ) x is complete. fn ( ) x ( ) x n = ( ) x = if for any function f C f f n n 1 Orthogonal: a set of functions is orthogonal if f a n n = m m ( ) x ( ) x b for for = =const 0 f dx n m

  27. 3.3.0 (2) A complete and orthogonal set of functions forms a basic set of functions. e.g. ( ) ( ) = odd = = 0 if if k k n n sin sin kx kx sin sin kx nx dx ( ) even ( ) = cos cos kx kx = = 0 if if k k n n cos cos kx nx dx = sin cos 0 kx nx dx , k n N sin(nx) is a basic set of functions for any odd function. cos(nx) is a basic set of functions for any even function. sin(nx) and cos(nx) are a basic set of functions for any functions.

  28. 3.3.0 (3) for any ( ) x ( ) x f ( ) x ( ) ( ) x ( ) f f x + ( ) x ( ) x even [coskx] f f x , ( ) x = f g ; odd even = h 2 2 ( ) x = + g h odd [sinkx] Fourier transform and Fourier series ( 0 n = = ) ( ) f x = + (*) sin cos A nx B nx n n 1 1 1 ( ) x ( ) x ( ) sin A f nx dx n = , 2 , 1 n ( ) = cos B f nx dx n ( ) x = = 0 B f dx A 0 0 2

  29. 3.3.0 (4) Proof ( ) * sin = ( ) kx dx ( ) f x sin kxdx ( ) ( ) + sin cos sin A nx B nx kx dx n n = 0 n = ( ) ( ) sin sin A nx kx dx n = 0 n A = if 0 k k 1 ( ) f x ( ) = sin A kx dx k 0

  30. 3.3.0 (5) ( ) * cos = ( ) kx dx ( ) f x ( ) cos kx dx ( ) ( ) kx dx + sin cos cos A nx B nx n n = 0 n B0 2 for k = 0 Bk for k = 1, 2, = = cos cos B nx kx dx n = 0 n 1 ( ) f x ( ) = cos B nx dx n 1 ( ) f x dx = B 0 2

  31. 3.3.1 Cartesian Coordinate Use the method of separation of variables to solve the Laplace s eq. Example 3 = = ( ) 0 0 V y = = ( ) 0 V y = = ( ) 0 ( ) V x V y 0 ( V x ) 0 Find the potential inside this slot ? 2 2 V V + = 0 Laplace s eq. 2 2 x y set = ( , ) ( ) ( ) V x y X x Y y 2 2 X Y + = 0 Y X 2 2 x y

  32. 3.3.1 (2) 2 2 1 X 1 Y X Y + = 0 2 2 x y depedent depedent ( ) f x x only ( ) g y y only f and g are constant 2 1 Y dy d Y 2 1 X d X = = ( ) g y C = = ( ) f x C 2 2 1 2 dx , are constant ( ) g y = C C 1 ( ) f x 2 + + = = = set 2 0 C C C C k 1 2 0 1 2 2 2 d Y dy d X 2 so 2 = = 2 k X k Y 2 dx = + = + kx kx ( ) , ( ) sin cos X x Ae Be Y y C ky D ky + ( ) Ae Be kx kx = + ( , ) ( sin cos ) V x y C ky D ky

  33. 3.3.1 (3) = ) , y = B.C. (iv) ( ) 0 0, 0 V x A k e kx + ( V x ( sin cos ) C ky D ky B.C. (i) = = Ce kx = ( ( , ) V x y 0) 0 0 V y D ky = sin B.C. (ii) = = = = ( ) 0 sin 0 1,2,3 V y k k kx The principle of superposition = sin Ce ky ( , ) V x y = 1 k = = ( ) 0 = ( ) kx V x 0y V C e B.C. (iii) sin ky ( ) 0y V A fourier series for odd function k = 1 k 2 = ( )sin y C V ky dy 0 k 0

  34. 3.3.1 (4) = = ( ) V y V const ant For 0 0 2 V 0 = sin C ky dy k 0 = 0 if k even 2 k V 0 = (1 cos = ) k 40 V k = if k odd 4 2 V V 1 k sin sinh y 1 k 0 0 = = ( , ) V x y sin tan ( ) e ky x 1,3,5, = k

  35. 3.4 Multipole Expansion 3.4.1 Approximate Potentials at Large distances 3.4.2 The Monopole and Dipole Terms 3.4.3 Origin of Coordinates in Multipole Expansions 3.4.4 The Electric Field of a Dipole

  36. 3.4.1 Approximate Potentials at Large distances Example 3.10 A dipole (Fig 3.27). Find the approximate potential at points far from the dipole. 1 4 0 + r r r 2 2 2 4 r r 2(1 cos ) r 1 1 1 1 2 2 r r r r q q = ( ) ( ) V p d 2 2 2 = + ( ) cos r rd 2 d d = + (1 cos ) r d r d r d d (1 cos ) (1 cos ) r 1 r + 1 r - d ( ) cos 2 r qd 1 cos 2 r ( ) V p 4 0

  37. 3.4.1 Example 3.10 For an arbitrary localized charge distribution. Find a systematic expansion of the potential? 1 1 ( ) 4 r r = V p d 0 2 2 2 = + 2 cos r r rr r r r 2 2 = [1 ( ) + 2( )cos ] r r r r r r r = + = 1 ( )( 2cos ) r

  38. 3.4.1(2) 1 2 1 r 1 r 1 r 1 2 3 8 5 2 3 = + = + + (1 ) (1 ) 16 1 r 1 2 3 8 5 r r r r r r r r r 2 2 3 3 = + + [1 ( )( r 2cos ) ( ) ( r 2cos ) ( ) ( r 2cos ) ] 16 1 r 3 2 1 2 5 2 3 2 r r r 2 2 3 3 = + + + + [1 ( )cos r = ( ) ( cos r ) ( ) ( cos r cos ) ] 1 r r n ( ) r (cos ) P d n = 0 n 1 n 1 n = ( ) ( ) r (cos ) V r P d n + ( 1) 4 r 0 = 0 n 1 1 r 1 2 r 1 3 r 3 2 1 2 2 ( ) ( cos r = + + + [ cos ) ] d r d d 4 0 Monopole term Dipole term Quadrupole term Multipole expansion

  39. 3.4.2 The Monopole and Dipole Terms monopole 4 mon 1 Q r dominates if r >> 1 = ( ) p V 0 1 1 2 r = r r cos r = ( ) p cos V r d dipole dip 4 0 1 1 2 r = r r d 4 0 P dipole moment (vector) p r 1 = ( ) p V dip 2 4 r n 0 = = p r d q r i i = 1 i A physical dipole is consist of a pair of equal and opposite charge, q p qr qr + = = + = ( ) q r r qd

  40. 3.4.3 Origin of Coordinates in Multipole Expansions = p r d = ( ) r d d = r d d d = p dQ = = 0 Q p p if

  41. 3.4.4 The Electric Field of a Dipole A pure dipole cos P r P ( , ) r = = V dip 2 2 4 4 r r 0 0 2 cos P V r = = E r 3 4 r 0 sin P 1 r V = = E 3 4 r 0 1 V = = 0 E sin r P ( , ) r = + r (2cos sin ) E dip 3 4 r 0

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