{VERSION 3 0 "SUN SPARC SOLARIS" "3.0" } {USTYLETAB {CSTYLE "Maple Input" -1 0 "Courier" 0 1 255 0 0 1 0 1 0 0 1 0 0 0 0 }{CSTYLE "2D Math" -1 2 "Times" 0 1 0 0 0 0 0 0 2 0 0 0 0 0 0 }{CSTYLE "2D Output" 2 20 "" 0 1 0 0 255 1 0 0 0 0 0 0 0 0 0 } {PSTYLE "Normal" -1 0 1 {CSTYLE "" -1 -1 "" 0 1 0 0 0 0 0 0 0 0 0 0 0 0 0 }0 0 0 -1 -1 -1 0 0 0 0 0 0 -1 0 }{PSTYLE "Maple Output" 0 11 1 {CSTYLE "" -1 -1 "" 0 1 0 0 0 0 0 0 0 0 0 0 0 0 0 }3 3 0 -1 -1 -1 0 0 0 0 0 0 -1 0 }{PSTYLE "" 11 12 1 {CSTYLE "" -1 -1 "" 0 1 0 0 0 0 0 0 0 0 0 0 0 0 0 }1 0 0 -1 -1 -1 0 0 0 0 0 0 -1 0 }{PSTYLE "Title" 0 18 1 {CSTYLE "" -1 -1 "" 1 18 0 0 0 0 0 1 1 0 0 0 0 0 0 }3 0 0 -1 12 12 0 0 0 0 0 0 19 0 }} {SECT 0 {EXCHG {PARA 18 "" 0 "" {TEXT -1 20 "Chapter 5, Problem 8" }}} {EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 89 "restart : eqn := diff(diff(x (t),t),t) + 9*x(t) - eps*(gamma*cos(t) - beta*x(t) + x(t)^3);" }} {PARA 11 "" 1 "" {XPPMATH 20 "6#>%$eqnG,(-%%diffG6$-%\"xG6#%\"tG-%\"$G 6$F,\"\"#\"\"\"F)\"\"**&%$epsGF1,(*&%&gammaGF1-%$cosGF+F1F1*&%%betaGF1 F)F1!\"\"*$)F)\"\"$\"\"\"F1F1F<" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 56 "eqn := subs(x(t) = x0(t) + eps*x1(t) + eps^2*x2(t),eqn):" }}} {EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 25 "expr := coeff(eqn,eps,0);" } }{PARA 11 "" 1 "" {XPPMATH 20 "6#>%%exprG,&-%%diffG6$-%#x0G6#%\"tG-%\" $G6$F,\"\"#\"\"\"F)\"\"*" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 35 "x0(t) := a0*cos(3*t) + b0*sin(3*t);" }}{PARA 11 "" 1 "" {XPPMATH 20 " 6#>-%#x0G6#%\"tG,&*&%#a0G\"\"\"-%$cosG6#,$F'\"\"$F+F+*&%#b0GF+-%$sinGF .F+F+" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 39 "expr := combine(co eff(eqn,eps,1),trig);" }}{PARA 12 "" 1 "" {XPPMATH 20 "6#>%%exprG,<-%% diffG6$-%#x1G6#%\"tG-%\"$G6$F,\"\"#\"\"\"F)\"\"**&%&gammaGF1-%$cosGF+F 1!\"\"*(%%betaGF1%#a0GF1-F66#,$F,\"\"$F1F1*(F9\"\"\"%#b0GF1-%$sinGFF@-F66#,$F,F2F1#F7\"\"%*&FEF@F;F@#!\"$FJ*()F:F0F@FAF@-FCFGF1F L*(FOF@FAF@FBF@FL*(F:F@F;F@)FAF0F@FL*(F:F@FSF@FFF@#F>FJ*&)FAF>F@FPF@#F 1FJ*&FWF@FBF@FL" }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 52 "Now find the s ecular terms from the O(eps) equation." }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 29 "eqn1 := coeff(expr,cos(3*t));" }}{PARA 11 "" 1 "" {XPPMATH 20 "6#>%%eqn1G,(*&%%betaG\"\"\"%#a0GF(F(*$)F)\"\"$\"\"\"#!\"$ \"\"%*&F)F-)%#b0G\"\"#F-F." }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 29 "eqn2 := coeff(expr,sin(3*t));" }}{PARA 11 "" 1 "" {XPPMATH 20 "6#> %%eqn2G,(*&%%betaG\"\"\"%#b0GF(F(*&)%#a0G\"\"#\"\"\"F)F.#!\"$\"\"%*$)F )\"\"$F.F/" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 31 "solve(\{eqn1= 0,eqn2=0\},\{a0,b0\});" }}{PARA 12 "" 1 "" {XPPMATH 20 "6&<$/%#b0G\"\" !/%#a0GF&<$/F(,$-%'RootOfG6#,&%%betaG!\"\"*$)%#_ZG\"\"#\"\"\"\"\"$F5F$ <$/F%F+F'<$/F%F%/F(-F-6#,(F2F7F0!\"%*$)F%F5F6F7" }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 97 "So there are two constraints coming from the O(eps) \+ secular terms. One is (a0,b0) = (0,0). The" }}{PARA 0 "" 0 "" {TEXT -1 100 "other is a0^2 + b0^2 = 4/3 beta. This means that the \+ amplitude of the O(1) solution is fixed, but" }}{PARA 0 "" 0 "" {TEXT -1 101 "the phase is free. So we go back and take x0(t) = 2 sqrt(beta /3) cos(3 t + phi_0) where phi_0 is the" }}{PARA 0 "" 0 "" {TEXT -1 29 "additional degree of freedom." }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 41 "x0(t) := 2*sqrt(beta/3)*cos(3*t + phi_0);" }}{PARA 11 "" 1 "" {XPPMATH 20 "6#>-%#x0G6#%\"tG,$*(-%%sqrtG6#\"\"$\"\"\"-F+6# %%betaGF.-%$cosG6#,&F'F-%&phi_0G\"\"\"F7#\"\"#F-" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 39 "expr := combine(coeff(eqn,eps,1),trig);" }} {PARA 11 "" 1 "" {XPPMATH 20 "6#>%%exprG,*-%%diffG6$-%#x1G6#%\"tG-%\"$ G6$F,\"\"#\"\"\"F)\"\"**&%&gammaGF1-%$cosGF+F1!\"\"*(-%%sqrtG6#\"\"$\" \"\")%%betaG#F " 0 "" {MPLTEXT 1 0 21 "dsolve(expr=0,x1(t));" }}{PARA 12 "" 1 "" {XPPMATH 20 "6#/-%#x1G6#%\"tG,**&,**&%&gammaG\"\"\"-%$cosG6#,$F'\"\"%F -#F-\"#C*&F,\"\"\"-F/6#,$F'\"\"#F-#F-\"#7*(-%%sqrtG6#\"\"$F6)%%betaG#F AF:F6-F/6#,&F'F<%&phi_0GFAF-#F-\"$C$*(F>F6FBF6-F/6#,&F'\"\"'FHFAF-#!\" \"\"$i\"F--F/6#,$F'FAF-F-*&,**&F,F6-%$sinGF8F-F;*&F,F6-FZF0F-F3*(F>F6F BF6-FZFMF-#F-FR*(F>F6FBF6-FZFFF-FIF--FZFTF-F-*&%$_C1GF-FSF6F-*&%$_C2GF -F\\oF6F-" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 16 "x1(t) := rhs(% ):" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 37 "x1(t) := subs(\{_C1=a 1,_C2=b1\},x1(t));" }}{PARA 12 "" 1 "" {XPPMATH 20 "6#>-%#x1G6#%\"tG,* *&,**&%&gammaG\"\"\"-%$cosG6#,$F'\"\"%F-#F-\"#C*&F,\"\"\"-F/6#,$F'\"\" #F-#F-\"#7*(-%%sqrtG6#\"\"$F6)%%betaG#FAF:F6-F/6#,&F'F<%&phi_0GFAF-#F- \"$C$*(F>F6FBF6-F/6#,&F'\"\"'FHFAF-#!\"\"\"$i\"F--F/6#,$F'FAF-F-*&,**& F,F6-%$sinGF8F-F;*&F,F6-FZF0F-F3*(F>F6FBF6-FZFMF-#F-FR*(F>F6FBF6-FZFFF -FIF--FZFTF-F-*&%#a1GF-FSF6F-*&%#b1GF-F\\oF6F-" }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 66 "We now look for the O(eps^2) secular terms to determ ine a1 and b1." }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 39 "expr := c ombine(coeff(eqn,eps,2),trig);" }}{PARA 12 "" 1 "" {XPPMATH 20 "6#>%%e xprG,>-%%diffG6$-%#x2G6#%\"tG-%\"$G6$F,\"\"#\"\"\"F)\"\"**(%%betaGF1%& gammaGF1-%$cosGF+F1#!\"\"\"\")*()F4#\"\"&F0\"\"\"-%%sqrtG6#\"\"$F?-F76 #,&F,F2%&phi_0GFCF1#F1\"$C$*(F4F?%#a1GF1-F76#,$F,FCF1F9*(F4F?%#b1GF1-% $sinGFMF1F9*(F4F?F5F?-F76#,&F,F>FGF0F1F8*(F4F?F5F?-F76#,&F,\"\"(FGF0F1 F8*(FF1FH*(F4F?FK F?-F76#,&F,FCFGF0F1F9*(F4F?FKF?-F76#,&F,F2FGF0F1F9*(F4F?FPF?-FRFeoF1F9 *(F4F?FPF?-FRFaoF1F1" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 46 "RHS := expr - diff(diff(x2(t),t),t) - 9*x2(t);" }}{PARA 12 "" 1 "" {XPPMATH 20 "6#>%$RHSG,:*(%%betaG\"\"\"%&gammaGF(-%$cosG6#%\"tGF(#!\" \"\"\")*()F'#\"\"&\"\"#\"\"\"-%%sqrtG6#\"\"$F6-F+6#,&F-\"\"*%&phi_0GF: F(#F(\"$C$*(F'F6%#a1GF(-F+6#,$F-F:F(F/*(F'F6%#b1GF(-%$sinGFEF(F/*(F'F6 F)F6-F+6#,&F-F4F?F5F(F.*(F'F6F)F6-F+6#,&F-\"\"(F?F5F(F.*(F2F6F7F6-F+6# ,&F-F:F?F(F(F@*(F2F6F7F6-F+6#,&F-\"#:F?F4F(F@*(F'F6FCF6-F+6#,&F-F:F?F5 F(F/*(F'F6FCF6-F+6#,&F-F>F?F5F(F/*(F'F6FHF6-FJF]oF(F/*(F'F6FHF6-FJFinF (F(" }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 120 "Now I have to be careful, if I ask for coeff(test,cos(3*t)), then it won't give me all the 3-mo de stuff. I want to make" }}{PARA 0 "" 0 "" {TEXT -1 117 "sure that R HS of \"d^2/dt^2 x2 + 9 x2 = RHS\" is orthogonal to cos(3t) and sin(3 t). So I take the inner product below" }}{PARA 0 "" 0 "" {TEXT -1 51 "and then demand that the two coefficients are zero." }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 0 "" }{MPLTEXT 1 0 53 "eqn1 := combine(int(RHS*cos( 3*t),t=0..2*Pi)/Pi,trig);" }}{PARA 11 "" 1 "" {XPPMATH 20 "6#>%%eqn1G, **(%%betaG\"\"\"%#a1GF(-%$cosG6#,$%&phi_0G\"\"#F(!\"\"*&F'\"\"\"F)F2F0 *()F'#\"\"&F/F2-%%sqrtG6#\"\"$F2-F+6#F.F(#F(\"$C$*(F'F2%#b1GF(-%$sinGF ,F(F(" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 53 "eqn2 := combine(in t(RHS*sin(3*t),t=0..2*Pi)/Pi,trig);" }}{PARA 11 "" 1 "" {XPPMATH 20 "6 #>%%eqn2G,**(%%betaG\"\"\"%#a1GF(-%$sinG6#,$%&phi_0G\"\"#F(F(*&F'\"\" \"%#b1GF(!\"\"*(F'F1F2F1-%$cosGF,F(F(*()F'#\"\"&F/F1-%%sqrtG6#\"\"$F1- F+6#F.F(#F3\"$C$" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 39 "sols := solve(\{eqn1=0,eqn2=0\},\{a1,b1\});" }}{PARA 11 "" 1 "" {XPPMATH 20 " 6#>%%solsG<$/%#b1G,$*&,&*(%%betaG\"\"\"%#a1GF--%$cosG6#%&phi_0GF-\"$[' *&)F,#\"\"&\"\"#\"\"\"-%%sqrtG6#\"\"$F9!\"\"F9*&F,\"\"\"-%$sinGF1\"\" \"!\"\"#F-F3/F.F." }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 101 "Okay, so I' m getting that a1 is free and b1 is determined by a1. Which is the sa me as we had before." }}{PARA 0 "" 0 "" {TEXT -1 97 "Although we don't have a1^2 + b1^2 = const, which we did have for a0 and b0. (That's w hy I could" }}{PARA 0 "" 0 "" {TEXT -1 46 "put the freedom in a0 and b 0 in a phase shift." }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 19 "b1 : = rhs(sols[1]);" }}{PARA 11 "" 1 "" {XPPMATH 20 "6#>%#b1G,$*&,&*(%%bet aG\"\"\"%#a1GF*-%$cosG6#%&phi_0GF*\"$['*&)F)#\"\"&\"\"#\"\"\"-%%sqrtG6 #\"\"$F6!\"\"F6*&F)\"\"\"-%$sinGF.\"\"\"!\"\"#F*F0" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 24 "combine(a1^2+b1^2,trig);" }}{PARA 11 "" 1 " " {XPPMATH 20 "6#*&,(*&)%%betaG\"\"#\"\"\")%#a1GF(F)!'o*R\"**)F'#\"\"( F(F)F+\"\"\"-%$cosG6#%&phi_0GF1-%%sqrtG6#\"\"$F)\"$K%*$)F'\"\"&F)!\"\" F),&*$F&F)!&%)*p*&F&F)-F36#,$F5F(F1\"&%)*p!\"\"" }}}{EXCHG {PARA 0 "> \+ " 0 "" {MPLTEXT 1 0 29 "x1(t) := combine(x1(t),trig);" }}{PARA 12 "" 1 "" {XPPMATH 20 "6#>-%#x1G6#%\"tG,$*&,.*(%%betaG\"\"\"%&gammaGF--%$si nG6#,&F'F-%&phi_0GF-F-\"#\")*(F,\"\"\"F.F6-F06#,&F'F-F3!\"\"F-!#\")*() F,#\"\"&\"\"#F6-%%sqrtG6#\"\"$F6-F06#,&F'\"\"*F3\"\"%F-!\"#*(F=F6FAF6- F06#,&F'FHF3F@F-F@*(F,F6%#a1GF--F06#,&F'FDF3F-F-\"%'H\"*(-F06#,$F'FDF- F=F6FAF6FJF6*&F,\"\"\"-F06#F3\"\"\"!\"\"#F-FT" }}}{EXCHG {PARA 0 "> " 0 "" {MPLTEXT 1 0 26 "x(t) := x0(t) + eps*x1(t);" }}{PARA 12 "" 1 "" {XPPMATH 20 "6#>-%\"xG6#%\"tG,&*(-%%sqrtG6#\"\"$\"\"\"-F+6#%%betaGF.-% $cosG6#,&F'F-%&phi_0G\"\"\"F7#\"\"#F-*&*&%$epsGF7,.*(F1F7%&gammaGF7-%$ sinG6#,&F'F7F6F7F7\"#\")*(F1F.F?F.-FA6#,&F'F7F6!\"\"F7!#\")*()F1#\"\"& F9F.F*F.-FA6#,&F'\"\"*F6\"\"%F7!\"#*(FLF.F*F.-FA6#,&F'FRF6F9F7F9*(F1F. %#a1GF7-FAF4F7\"%'H\"*(-FA6#,$F'F-F7FLF.F*F.FTF7F.*&F1\"\"\"-FA6#F6\" \"\"!\"\"#F7Ffn" }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 115 "Note that eve n if you had assumed that at the O(1) level the solution had a0 = 2 s qrt(beta/3) and b0 = 0, then you" }}{PARA 0 "" 0 "" {TEXT -1 84 "still get a degree of freedom at the O(eps) level from the O(eps^2) secular terms..." }{MPLTEXT 1 0 0 "" }}}{EXCHG {PARA 0 "" 0 "" {TEXT -1 0 "" }}}}{MARK "28 1 0" 84 }{VIEWOPTS 1 1 0 1 1 1803 }