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So far, w ith rectangular coordinates, the Laplacian Operator is given by two de rivatives with respect to x plus two derivatives with respect to y:" } }{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 15 " \+ " }{XPPEDIT 18 0 "Delta;" "6#%&DeltaG" }{TEXT 286 1 "u" }{TEXT -1 3 " = " }{XPPEDIT 18 0 "diff(u,`$`(x,2));" "6#-%%diffG6$%\"uG-%\"$G 6$%\"xG\"\"#" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "diff(u,`$`(y,2));" "6# -%%diffG6$%\"uG-%\"$G6$%\"yG\"\"#" }{TEXT -1 1 "." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 79 "It would be no surprise h ow to write this in three dimensions, instead of two. " }}{PARA 0 "" 0 "" {TEXT -1 2 " " }}{PARA 0 "" 0 "" {TEXT -1 285 " If the origi ns of the problem to be considered is on a disk, or annulus, or cylind er, it is often better to think of the problem in polar coordinates. A way to think of the change is to remember that in order to change bet ween rectangular and polar coordinates, use this identity:" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 10 " " } {TEXT 287 1 "x" }{TEXT -1 9 " = r cos(" }{XPPEDIT 18 0 "theta;" "6#%&t hetaG" }{TEXT -1 6 ") and " }{TEXT 288 1 "y" }{TEXT -1 9 " = r sin(" } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 3 "). " }}{PARA 0 "" 0 " " {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 18 "In that case, r = " } {XPPEDIT 18 0 "sqrt(x^2+y^2);" "6#-%%sqrtG6#,&*$%\"xG\"\"#\"\"\"*$%\"y GF)F*" }{TEXT -1 6 " and " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" } {TEXT -1 10 " = arctan(" }{TEXT 289 3 "y/x" }{TEXT -1 2 ")." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 75 " For exampl e take these examples. We take r = 2 and use five different " } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 " 's." }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 43 "r:=2; theta:=[-3*Pi/4,-Pi/2,0,Pi/4,3*Pi/4 ];" }}}{PARA 0 "" 0 "" {TEXT -1 85 "We compute the sequence or points \+ [ r cos(t), r sin(t) ] where t is one of the above " }{XPPEDIT 18 0 "t heta;" "6#%&thetaG" }{TEXT -1 4 " 's." }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 34 "map(t->[r*cos(t),r*sin(t)],theta);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}{PARA 0 "" 0 "" {TEXT -1 0 "" }} {PARA 0 "" 0 "" {TEXT -1 66 " We now do it the other way. We pick \+ points and make r 's and " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" } {TEXT -1 5 " 's. " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 534 " (A part of the problem here is that arctan(-1/1) an d arctan(1/(-1)) look the same to the arctangent function. Yet the poi nts [-1, 1] and [1, -1] are in different quadrants. Thus, we either ha ve to be careful in our programming, or hope that Maple has a routine \+ to do this. It does. The program computes the angle associated with a \+ complex number a + b I. Thus, we change the point [ x, y] to the compl ex number x + y I and use Maple's built in program. You might enjoy ma king a program that does not use Maple's built in scheme.)" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 50 " Here, we give points and compute r and theta. " }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 42 "pts:=[[-1,-1],[0,-1],[1,-1],[1,1],[-1,1]];" }}} {EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 55 "r:=(x,y)->sqrt(x^2+y^2);\nth eta:=(x,y)->argument(x+I*y);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 75 "seq(r(pts[i][1],pts[i][2]),i=1..5);\nseq(theta(pts[j][1],pts[j][ 2]),j=1..5);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}{PARA 0 "" 0 "" {TEXT -1 0 "" } }{PARA 0 "" 0 "" {TEXT -1 0 "" }}{SECT 0 {PARA 3 "" 0 "" {TEXT 297 39 "Laplace's Equation in Polar Coordinates" }}{PARA 0 "" 0 "" {TEXT -1 87 "We want to establish Laplace's equation in polar coordinates. To d o this, suppose that " }{TEXT 260 1 "u" }{TEXT -1 1 "(" }{TEXT 261 1 " x" }{TEXT -1 2 ", " }{TEXT 262 1 "y" }{TEXT -1 39 ") satisfies Laplace 's equation. Define " }{TEXT 263 1 "v" }{TEXT -1 4 "(r, " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 5 ") as " }{TEXT 264 1 "u" } {TEXT -1 7 "(r cos(" }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 9 "), r sin(" }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 25 ")). We \+ use the fact that " }{XPPEDIT 18 0 "Delta;" "6#%&DeltaG" }{TEXT -1 1 " " }{TEXT 265 1 "u" }{TEXT -1 17 " = 0 to show that" }}{PARA 0 "" 0 " " {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 28 " \+ " }{XPPEDIT 18 0 "diff(r*diff(v(r,theta),r),r)/r+diff(v(r,theta), `$`(theta,2))/(r^2);" "6#,&*&-%%diffG6$*&%\"rG\"\"\"-F&6$-%\"vG6$F)%&t hetaGF)F*F)F*F)!\"\"F**&-F&6$-F.6$F)F0-%\"$G6$F0\"\"#F**$F)F:F1F*" } {TEXT -1 6 " = 0" }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 43 "v:=(r, theta)->u(r*cos(theta),r*sin(theta));" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 64 "diff(r*diff(v(r,theta),r),r)/r+diff(v(r,theta),theta, theta)/r^2:" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 12 "simplify(%); " }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}{PARA 0 "" 0 "" {TEXT -1 30 " We see that this last is " }{XPPEDIT 18 0 "Delta;" " 6#%&DeltaG" }{TEXT -1 1 " " }{TEXT 266 1 "u" }{TEXT -1 7 "(r cos(" } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 9 "), r sin(" }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 134 ")). The assumption is that t his is zero. Thus, we know a form for the Laplacian Operator in polar \+ coordinates. Here are some examples." }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 71 "LO:=v->diff(r*diff(v(r,theta),r),r)/r+diff(v(r,theta) ,theta,theta)/r^2;" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 34 "v:=(r ,theta)->r*sin(theta);\nLO(v);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 38 "v:=(r,theta)->r^n*cos(n*theta);\nLO(v);" }}}{EXCHG {PARA 0 "> \+ " 0 "" {MPLTEXT 1 0 0 "" }}}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 " " 0 "" {TEXT -1 231 " What are the type problems we can solve with this realization of the Laplacian Operator? You could guess this is a typical problem. You can even guess a solution.\n Suppose we have a disk with radius 1. We seek the surface " }{TEXT 267 1 "u" }{TEXT -1 16 " which satisfies" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 43 " " } {XPPEDIT 18 0 "Delta;" "6#%&DeltaG" }{TEXT 268 1 "u" }{TEXT -1 18 "=0 \+ for 0< r < 1, -" }{XPPEDIT 18 0 "Pi;" "6#%#PiG" }{TEXT -1 5 " < " } {XPPEDIT 18 0 "theta" "6#%&thetaG" }{TEXT -1 4 " < " }{XPPEDIT 18 0 " Pi;" "6#%#PiG" }{TEXT -1 2 " ." }}{PARA 0 "" 0 "" {TEXT -1 52 " \+ with u(1," }{XPPEDIT 18 0 "theta" "6#%&thetaG" }{TEXT -1 8 ") = cos(" }{XPPEDIT 18 0 "theta" "6#%&thetaG " }{TEXT -1 7 ") for -" }{XPPEDIT 18 0 "Pi;" "6#%#PiG" }{TEXT -1 5 " \+ < " }{XPPEDIT 18 0 "theta" "6#%&thetaG" }{TEXT -1 4 " < " }{XPPEDIT 18 0 "Pi;" "6#%#PiG" }{TEXT -1 2 " ." }}{PARA 0 "" 0 "" {TEXT -1 18 "W hat do you guess?" }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 27 "u:=(r,t heta)->r*cos(theta);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 6 "LO(u );" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 11 "u(1,theta);" }}} {PARA 0 "" 0 "" {TEXT -1 31 "Here is a graph of the surface." }} {EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 112 "cylinderplot([r,theta,u(r,t heta)],r=0..1,theta=0..2*Pi,\n axes=boxed,orientation=[-125,75] , shading=zhue);" }}}{EXCHG }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 190 "We might be lucky to guess at solutions, but lik ely will not be. Thus, we need to develop techniques for solving probl ems on a disk with radius c. We seek bounded solutions for the equatio ns" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 15 " \+ " }{XPPEDIT 18 0 "Delta;" "6#%&DeltaG" }{TEXT 269 1 "u" } {TEXT -1 15 " = 0 with u(c, " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" } {TEXT -1 6 ") = f(" }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 " ), " }{XPPEDIT 18 0 "-Pi;" "6#,$%#PiG!\"\"" }{TEXT -1 3 " < " } {XPPEDIT 18 0 "theta <= Pi;" "6#1%&thetaG%#PiG" }{TEXT -1 2 " ." }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 20 "Note that the ray " }{XPPEDIT 18 0 "theta = Pi;" "6#/%&thetaG%#PiG" }{TEXT -1 12 " is not a " }{TEXT 259 8 "boundary" }{TEXT -1 111 " in the sa me sense as the circle r = c is. To be sure that we do not have false \+ boundary problems, we ask that " }}{PARA 0 "" 0 "" {TEXT -1 18 " \+ " }{TEXT 270 1 "u" }{TEXT -1 4 "(r, " }{XPPEDIT 18 0 "Pi; " "6#%#PiG" }{TEXT -1 4 ") = " }{TEXT 271 1 "u" }{TEXT -1 4 "(r, " } {XPPEDIT 18 0 "-Pi;" "6#,$%#PiG!\"\"" }{TEXT -1 6 ") and " }{XPPEDIT 18 0 "diff(u,theta);" "6#-%%diffG6$%\"uG%&thetaG" }{TEXT -1 5 " (r, " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 ") = " }{XPPEDIT 18 0 "diff(u,theta);" "6#-%%diffG6$%\"uG%&thetaG" }{TEXT -1 7 " (r, - " } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 3 "). " }}{PARA 0 "" 0 " " {TEXT -1 71 "These are natural boundary conditions of the problem we have described." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{SECT 0 {PARA 259 "" 0 "" {TEXT -1 68 "Separation of Variables for Laplace's Equation in Polar Coordinates." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 " " {TEXT -1 129 " In these notes to this point, our first guess for how to solve such a problem has been to separate variables in the equ ation" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 21 " " }{XPPEDIT 18 0 "diff(r*diff(v(r,theta),r),r)/r+ diff(v(r,theta),`$`(theta,2))/(r^2);" "6#,&*&-%%diffG6$*&%\"rG\"\"\"-F &6$-%\"vG6$F)%&thetaGF)F*F)F*F)!\"\"F**&-F&6$-F.6$F)F0-%\"$G6$F0\"\"#F **$F)F:F1F*" }{TEXT -1 8 " = 0, " }}{PARA 0 "" 0 "" {TEXT -1 6 "to g et" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 9 " \+ " }{XPPEDIT 18 0 "1/r;" "6#*&\"\"\"F$%\"rG!\"\"" }{TEXT -1 11 " ( r R ') ' " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 5 " + " } {XPPEDIT 18 0 "1/(r^2);" "6#*&\"\"\"F$*$%\"rG\"\"#!\"\"" }{TEXT -1 3 " R " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 8 " '' = 0." }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 12 "Multiply \+ by " }{XPPEDIT 18 0 "r^2;" "6#*$%\"rG\"\"#" }{TEXT -1 14 ", divide by \+ R " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 8 " to get" }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 10 " \+ " }{XPPEDIT 18 0 "1/R;" "6#*&\"\"\"F$%\"RG!\"\"" }{TEXT -1 16 " r (r \+ R ') ' + " }{XPPEDIT 18 0 "1/theta;" "6#*&\"\"\"F$%&thetaG!\"\"" } {TEXT -1 1 " " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 10 " '' \+ = 0." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 25 "Boundary conditions are " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" } {TEXT -1 4 " (- " }{XPPEDIT 18 0 "pi;" "6#%#piG" }{TEXT -1 4 ") = " } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 3 " ( " }{XPPEDIT 18 0 " pi;" "6#%#piG" }{TEXT -1 2 ")," }}{PARA 0 "" 0 "" {TEXT -1 40 " \+ " }{XPPEDIT 18 0 "theta;" "6#%&thetaG " }{TEXT -1 5 " '(- " }{XPPEDIT 18 0 "pi;" "6#%#piG" }{TEXT -1 4 ") = \+ " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 " '( " }{XPPEDIT 18 0 "pi;" "6#%#piG" }{TEXT -1 2 ")." }}{PARA 0 "" 0 "" {TEXT -1 34 "T he two differential equations are" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }} {PARA 0 "" 0 "" {TEXT -1 5 " " }{XPPEDIT 18 0 "theta;" "6#%&thetaG " }{TEXT -1 6 " '' + " }{XPPEDIT 18 0 "lambda^2*theta;" "6#*&%'lambdaG \"\"#%&thetaG\"\"\"" }{TEXT -1 6 " = 0, " }{XPPEDIT 18 0 "theta;" "6#% &thetaG" }{TEXT -1 4 " (- " }{XPPEDIT 18 0 "pi;" "6#%#piG" }{TEXT -1 4 ") = " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 3 " ( " } {XPPEDIT 18 0 "pi;" "6#%#piG" }{TEXT -1 7 "), and " }{XPPEDIT 18 0 "th eta;" "6#%&thetaG" }{TEXT -1 5 " '(- " }{XPPEDIT 18 0 "pi;" "6#%#piG" }{TEXT -1 4 ") = " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 " \+ '( " }{XPPEDIT 18 0 "pi;" "6#%#piG" }{TEXT -1 2 ")." }}{PARA 0 "" 0 " " {TEXT -1 3 "and" }}{PARA 0 "" 0 "" {TEXT -1 18 " r( rR ') ' - " }{XPPEDIT 18 0 "lambda^2;" "6#*$%'lambdaG\"\"#" }{TEXT -1 7 " R = 0." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 77 "The sol utions for the first equation, with eigenvalues and eigenfunctions are " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 5 " \+ " }{XPPEDIT 18 0 "lambda;" "6#%'lambdaG" }{TEXT -1 9 " = 0, " } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 5 " = 1." }}{PARA 0 "" 0 "" {TEXT -1 5 " " }{XPPEDIT 18 0 "-lambda^2;" "6#,$*$%'lambdaG\" \"#!\"\"" }{TEXT -1 3 " = " }{XPPEDIT 18 0 "-n^2;" "6#,$*$%\"nG\"\"#! \"\"" }{TEXT -1 5 ", " }{XPPEDIT 18 0 "Theta;" "6#%&ThetaG" }{TEXT -1 1 "(" }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 10 ") = cos(n \+ " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 13 ") or sin(n " } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 2 ")." }}{PARA 0 "" 0 " " {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 28 "The second equation is \+ now " }{XPPEDIT 18 0 "r^2;" "6#*$%\"rG\"\"#" }{TEXT -1 16 " R '' + r \+ R ' - " }{XPPEDIT 18 0 "n^2;" "6#*$%\"nG\"\"#" }{TEXT -1 6 "R = 0." }} {PARA 0 "" 0 "" {TEXT -1 32 "Solutions for this equation are " }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 37 " R(r) = 1 or ln(r) in case n = 0," }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 15 "and, otherwise," }}{PARA 0 "" 0 "" {TEXT -1 17 " R(r) = " }{XPPEDIT 18 0 "r^n;" "6#)%\"rG%\"nG" }{TEXT -1 6 " or " }{XPPEDIT 18 0 "r^(-n);" "6#)%\"rG,$%\"nG!\"\"" }{TEXT -1 2 " .\n" }}{PARA 0 "" 0 "" {TEXT -1 69 "Here's how you might remember the \+ solution for this equation in case " }{TEXT 298 5 "n = 0" }{TEXT -1 4 " or " }{XPPEDIT 18 0 "n <> 0;" "6#0%\"nG\"\"!" }{TEXT -1 1 "." }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{EXCHG }{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 14 "unassign('r');" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 91 "n:=0;\nde := r^2*diff(R(r),r,r)+r*diff(R(r),r)-n^2*R(r)=0;\nds olve(de, R(r)); \nunassign('n');" }}}{EXCHG }{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 49 "de := r^2*diff(R(r),r,r)+r*diff(R(r),r)-n^2*R(r);" }} }{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 11 "dsolve(de);" }}}{EXCHG } {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 68 "As a resu lt, we can make the general solution for this problem with " } {XPPEDIT 18 0 "0 <= r;" "6#1\"\"!%\"rG" }{TEXT -1 1 "." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 10 " v(r, " } {XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 ") = " }{XPPEDIT 18 0 "a[0];" "6#&%\"aG6#\"\"!" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(a[n]*r ^n*cos(n*theta),n);" "6#-%$sumG6$*(&%\"aG6#%\"nG\"\"\")%\"rGF*F+-%$cos G6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(b[n]*r^ n*sin(n*theta),n);" "6#-%$sumG6$*(&%\"bG6#%\"nG\"\"\")%\"rGF*F+-%$sinG 6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 1 "." }}}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 103 "We have changed the problem to one \+ that can be solved by Fourier Series Techniques. Here is an example." }}{PARA 0 "" 0 "" {TEXT -1 1 " " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }} {SECT 0 {PARA 3 "" 0 "" {TEXT 272 11 "Example 1: " }{XPPEDIT 273 0 "De lta;" "6#%&DeltaG" }{TEXT 274 12 "u = 0, u(1, " }{XPPEDIT 275 0 "theta ;" "6#%&thetaG" }{TEXT 276 5 " ) = " }{XPPEDIT 277 0 "sin(theta)^2;" " 6#*$-%$sinG6#%&thetaG\"\"#" }}{PARA 0 "" 0 "" {TEXT -1 8 "We solve" }} {PARA 0 "" 0 "" {TEXT -1 15 " " }{XPPEDIT 18 0 "Delta;" "6#%&DeltaG" }{TEXT -1 12 "u = 0, u(1, " }{XPPEDIT 18 0 "theta;" "6#%& thetaG" }{TEXT -1 5 " ) = " }{XPPEDIT 18 0 "sin(theta)^2;" "6#*$-%$sin G6#%&thetaG\"\"#" }{TEXT -1 5 " for " }{XPPEDIT 18 0 "theta;" "6#%&the taG" }{TEXT -1 23 " in the interval [0, 2 " }{XPPEDIT 18 0 "Pi;" "6#%# PiG" }{TEXT -1 3 " ]." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 39 "First, we draw the boundary conditions:" }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 120 "spacecurve([cos(theta),sin(theta), sin(theta)^2],theta=-Pi..Pi,\n color=BLACK,orientation=[35, 65],axes=NORMAL);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 29 "We have t he general solution " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 " " {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 5 " " }{TEXT 290 1 "u" }{TEXT -1 4 "(r, " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 ") = " }{XPPEDIT 18 0 "a[0];" "6#&%\"aG6#\"\"!" }{TEXT -1 3 " + " } {XPPEDIT 18 0 "sum(a[n]*r^n*cos(n*theta),n);" "6#-%$sumG6$*(&%\"aG6#% \"nG\"\"\")%\"rGF*F+-%$cosG6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 3 " + " } {XPPEDIT 18 0 "sum(b[n]*r^n*sin(n*theta),n);" "6#-%$sumG6$*(&%\"bG6#% \"nG\"\"\")%\"rGF*F+-%$sinG6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 1 "." }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 19 ". If r = \+ 1, we have" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 11 " (" }{XPPEDIT 18 0 "sin(theta)^2;" "6#*$-%$sinG6#%&the taG\"\"#" }{TEXT -1 3 " = " }{XPPEDIT 18 0 "a[0];" "6#&%\"aG6#\"\"!" } {TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(a[n]*1^n*cos(n*theta),n);" "6#-%$ sumG6$*(&%\"aG6#%\"nG\"\"\")F+F*F+-%$cosG6#*&F*F+%&thetaGF+F+F*" } {TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(b[n]*1^n*sin(n*theta),n);" "6#-%$ sumG6$*(&%\"bG6#%\"nG\"\"\")F+F*F+-%$sinG6#*&F*F+%&thetaGF+F+F*" } {TEXT -1 1 "." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 110 "We have only to compute the coefficients. This is a job \+ for Fourier Series. Or, maybe you remember some trig. " }}{PARA 0 "" 0 "" {TEXT -1 15 " " }{XPPEDIT 18 0 "sin(theta)^2;" "6#* $-%$sinG6#%&thetaG\"\"#" }{TEXT -1 3 " = " }{XPPEDIT 18 0 "(1-cos(2*th eta))/2;" "6#*&,&\"\"\"F%-%$cosG6#*&\"\"#F%%&thetaGF%!\"\"F%F*F," } {TEXT -1 2 " " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 6 "Thus, " }{XPPEDIT 18 0 "a[0];" "6#&%\"aG6#\"\"!" }{TEXT -1 9 " = 1/2, " }{XPPEDIT 18 0 "a[2];" "6#&%\"aG6#\"\"#" }{TEXT -1 27 " = -1/2, and all the other " }{TEXT 291 1 "a" }{TEXT -1 38 " 's ar e zero. The implication is that " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 35 "u:=(r,theta)->1/2-r^2*cos(2*theta);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 129 "cylinderplot([r,theta,u(r,theta)],r=0..1,theta=0..2* Pi,\n orientation=[40,40],axes=NORMAL, shading=zhue, numpoint s=1000);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}}{PARA 0 " " 0 "" {TEXT -1 0 "" }}{SECT 0 {PARA 3 "" 0 "" {TEXT 278 12 "Example 2 , " }{XPPEDIT 279 0 "Delta;" "6#%&DeltaG" }{TEXT 280 12 "u = 0, u(1, \+ " }{XPPEDIT 281 0 "theta;" "6#%&thetaG" }{TEXT 282 5 " ) = " } {XPPEDIT 283 0 "theta^3*(Pi^2-theta^2);" "6#*&%&thetaG\"\"$,&*$%#PiG\" \"#\"\"\"*$F$F)!\"\"F*" }}{PARA 0 "" 0 "" {TEXT -1 8 "We solve" }} {PARA 0 "" 0 "" {TEXT -1 15 " " }{XPPEDIT 18 0 "Delta;" "6#%&DeltaG" }{TEXT 292 1 "u" }{TEXT -1 11 " = 0, u(1, " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 5 " ) = " }{XPPEDIT 18 0 "theta^3*(P i^2-theta^2);" "6#*&%&thetaG\"\"$,&*$%#PiG\"\"#\"\"\"*$F$F)!\"\"F*" } {TEXT -1 5 " for " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 23 " in the interval [0, 2 " }{XPPEDIT 18 0 "Pi;" "6#%#PiG" }{TEXT -1 3 " \+ ]." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 39 "Fir st, we draw the boundary conditions:" }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 130 "spacecurve([cos(theta),sin(theta),theta^3*(Pi^2-thet a^2)],theta=-Pi..Pi,\n color=BLACK,orientation=[10,55],axes =NORMAL);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}{PARA 0 " " 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 29 "We have the genera l solution " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 5 " " }{TEXT 293 1 "u" }{TEXT -1 4 "(r, " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" }{TEXT -1 4 ") = " } {XPPEDIT 18 0 "a[0];" "6#&%\"aG6#\"\"!" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(a[n]*r^n*cos(n*theta),n);" "6#-%$sumG6$*(&%\"aG6#%\"nG\"\"\" )%\"rGF*F+-%$cosG6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(b[n]*r^n*sin(n*theta),n);" "6#-%$sumG6$*(&%\"bG6#%\"nG\"\"\" )%\"rGF*F+-%$sinG6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 1 "." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 19 ". If r = 1, we have " }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 10 " \+ " }{XPPEDIT 18 0 "theta^3*(Pi^2-theta^2);" "6#*&%&thetaG\"\"$,&*$ %#PiG\"\"#\"\"\"*$F$F)!\"\"F*" }{TEXT -1 3 " = " }{XPPEDIT 18 0 "a[0]; " "6#&%\"aG6#\"\"!" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(a[n]*1^n*cos (n*theta),n);" "6#-%$sumG6$*(&%\"aG6#%\"nG\"\"\")F+F*F+-%$cosG6#*&F*F+ %&thetaGF+F+F*" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(b[n]*1^n*sin(n*t heta),n);" "6#-%$sumG6$*(&%\"bG6#%\"nG\"\"\")F+F*F+-%$sinG6#*&F*F+%&th etaGF+F+F*" }{TEXT -1 1 "." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 123 "We compute coefficients. It seems to be of no va lue to list the numerical output of these integrals, so we suppress ou tput." }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 80 "a[0]:=int(theta^3*(Pi^2-theta^2),theta=-Pi..Pi)/\n \+ int(1,theta=-Pi..Pi):" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 147 "for n from 1 to 10 do\n a[n]:=int(theta^3*(Pi^2-theta^2)*cos( n*theta),theta=-Pi..Pi)/\n int(cos(n*theta)^2,theta=-Pi..Pi): \nend do:\nn:='n':" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 147 "for \+ n from 1 to 10 do\n b[n]:=int(theta^3*(Pi^2-theta^2)*sin(n*theta),th eta=-Pi..Pi)/\n int(sin(n*theta)^2,theta=-Pi..Pi):\nend do:\n n:='n':" }}}{PARA 0 "" 0 "" {TEXT -1 16 "Here, we define " }{TEXT 294 1 "u" }{TEXT -1 1 "." }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 95 "u:=( r,theta)->a[0]+sum(a[n]*r^n*cos(n*theta)+b[n]*r^n*sin(n*theta),\n \+ n=1..10);" }}}{PARA 0 "" 0 "" {TEXT -1 116 "Here is a gra ph of the surface. Compare this \"rubber sheet\" with the space curve \+ given at the start of this problem." }}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 129 "cylinderplot([r,theta,u(r,theta)],r=0..1,theta=0..2* Pi,\n orientation=[10,55],axes=NORMAL, shading=zhue, numpoint s=1000);" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 0 "" }}}}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 104 "In summary, Laplace's Equation on a disk can be solved i n a manner consistent with what has come before:" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 16 " " }{TEXT 295 1 "u" }{TEXT -1 4 "(r, " }{XPPEDIT 18 0 "theta;" "6#%&thetaG" } {TEXT -1 4 ") = " }{XPPEDIT 18 0 "a[0];" "6#&%\"aG6#\"\"!" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(a[n]*r^n*cos(n*theta),n);" "6#-%$sumG6$*(& %\"aG6#%\"nG\"\"\")%\"rGF*F+-%$cosG6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 3 " + " }{XPPEDIT 18 0 "sum(b[n]*r^n*sin(n*theta),n);" "6#-%$sumG6$*(& %\"bG6#%\"nG\"\"\")%\"rGF*F+-%$sinG6#*&F*F+%&thetaGF+F+F*" }{TEXT -1 2 " ," }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 10 " where " }{XPPEDIT 18 0 "a[0];" "6#&%\"aG6#\"\"!" }{TEXT -1 3 " = \+ " }{XPPEDIT 18 0 "int(f(t),t = -Pi .. Pi)/(2*Pi);" "6#*&-%$intG6$-%\"f G6#%\"tG/F*;,$%#PiG!\"\"F.\"\"\"*&\"\"#F0F.F0F/" }{TEXT -1 2 " ," }} {PARA 0 "" 0 "" {TEXT -1 15 " " }{XPPEDIT 18 0 "a[n];" " 6#&%\"aG6#%\"nG" }{TEXT -1 3 " = " }{XPPEDIT 18 0 "int(f(t)*cos(n*t),t = -Pi .. Pi)/(Pi*c^n);" "6#*&-%$intG6$*&-%\"fG6#%\"tG\"\"\"-%$cosG6#* &%\"nGF,F+F,F,/F+;,$%#PiG!\"\"F5F,*&F5F,)%\"cGF1F,F6" }{TEXT -1 2 " , " }}{PARA 0 "" 0 "" {TEXT -1 3 "and" }}{PARA 0 "" 0 "" {TEXT -1 15 " \+ " }{XPPEDIT 18 0 "b[n];" "6#&%\"bG6#%\"nG" }{TEXT -1 3 " \+ = " }{XPPEDIT 18 0 "int(f(t)*sin(n*t),t = -Pi .. Pi)/(Pi*c^n);" "6#*&- %$intG6$*&-%\"fG6#%\"tG\"\"\"-%$sinG6#*&%\"nGF,F+F,F,/F+;,$%#PiG!\"\"F 5F,*&F5F,)%\"cGF1F,F6" }{TEXT -1 2 " ," }}{PARA 0 "" 0 "" {TEXT -1 6 " where " }{TEXT 296 1 "c" }{TEXT -1 27 " is the radius of the disk." }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 50 "EMAIL: he rod@math.gatech.edu or jherod@tds.net" }}{PARA 0 "" 0 "" {TEXT -1 38 "URL: http://www.math.gatech.edu/~herod" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 258 "" 0 "" {TEXT -1 36 "Copyright \251 2003 by Jame s V. Herod" }}{PARA 258 "" 0 "" {TEXT -1 19 "All rights reserved" }} {PARA 0 "" 0 "" {TEXT -1 0 "" }}{PARA 0 "" 0 "" {TEXT -1 0 "" }}} {MARK "0 0 0" 0 }{VIEWOPTS 1 1 0 1 1 1803 1 1 1 1 }{PAGENUMBERS 1 1 2 33 1 1 }