Nonlinear Dynamics and Chaos
Nonlinear Dynamics and Chaos
2nd Edition
ISBN: 9780813349107
Author: Steven H. Strogatz
Publisher: PERSEUS D
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Chapter 6.8, Problem 11E
Interpretation Introduction

Interpretation:

For the complex vector field z˙ = zk, write the vector fields in both Cartesian and polar coordinates, and for the cases k=1,2,3,4, show that the origin is the only fixed point, and compute its index.

Concept Introduction:

The index of a closed curve C is an integer that measures the winding of the vector curve C is an integer that measures the winding of the vector field on C.

The index also provides information about a fixed point that might happen to lie inside the curve.

Index theory provides global information about the phase portrait

The index of the closed curve C can be defined as the net number of counterclockwise revolutions that are made by the vector field.

Expert Solution & Answer
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Answer to Problem 11E

Solution:

The vector field for z˙ = zk in both Cartesian and polar coordinates, for the case k = 1, the field is z˙ = x + iy and z˙ = re respectively, and for z˙ =(z¯)k in both Cartesian and polar coordinates, the field is z˙ = x-iy and z˙ = re-iθ respectively.

The vector field for z˙ = zk in both Cartesian and polar coordinates, for the case k = 2, the field is z˙ =x2-y2+2ixy and z˙ =r2e2iθ respectively, and for z˙ =(z¯)k in both Cartesian and polar coordinates, z˙ =x2-y2-2ixy and z˙ =r2e-2iθ respectively.

The vector field for z˙ = zk in both Cartesian and polar coordinates, for the case k = 3, the field is z˙=x3-3xy2+i(3x2y - y3) and z˙=r3e3iθ respectively, and for z˙ =(z¯)k in both Cartesian and polar coordinates, z˙=x3-xy2-i(3x2y-y3) and z˙ =r3e-3iθ respectively.

It is to be shown that origin is the only fixed point.

The vector fields will have k rotations on a loop enclosing the origin.

Explanation of Solution

Index theory provides global information about the phase portrait. The index of the closed curve C can be defined as the net number of counterclockwise revolutions that are made by the vector field. Mathematically, it can be expressed as:

Ic=1[ϕ]c

Here, Ic is the index of the closed curve, [ϕ]c is the net charge in ϕ around C.

Consider complex vector fields as,

z˙ = zk And z˙ = (z¯)k

Here, k is an integer and is greater than0. Also, z¯ = x -iy is the complex conjugate of z

Let, z= x + iy 

The Euler’s formula is given as,

cosθ + i sin θ = e

a)

Write the vector fields in both Cartesian and polar coordinates for different cases

Case 1)

k = 1

Solve for

Substitute, 1 for k in z˙ = zk,

z˙ = (z)1

Substitute, z= x + iy  and solve,

z˙ = x + iy

z˙ = r cosθ + i (r sinθ)

z˙ = r(cosθ + i sinθ)

Substitute, cosθ + i sin θ = e

z˙ = re

Here, r=x2+y2

And, θ = tan-1(yx)

Thus, the Cartesian and polar co-ordinate for this vector field is z˙ = x + iy and z˙ = re respectively.

Solve for z˙ =(z¯)k

Substitute, 1 for k in z˙ =(z¯)k

z˙ =(z¯)1

Substitute z¯ = x-iy

z˙ = x-iy

This is the Cartesian co-ordinate for this vector field.

Solve for polar coordinates.

Substitute, r cos θ for x, r sin θ for y in z˙ = x-iy and solve

z˙ = r cos θ- i(r sin θ)

z˙ = r(cos θ- isin θ)

Substitute, e-iθ=(cos θ- isin θ)

z˙ = re-iθ

Thus, the Cartesian and polar coordinates for this vector field are z˙ = x-iy and z˙ = re-iθ respectively.

Case 2)

k=2

Solve for z˙ = zk

z˙ = (z)2

Substitute, z= x + iy  and solve,

z˙ =(x+iy)2

z˙ =x2-y2+2ixy

This is the Cartesian co-ordinate for this vector field.

Solve for polar coordinates,

Substitute, rcosθ for x and rsinθ for y

z˙ =(r cosθ+i(sinθ))2

z˙ =r2(cosθ+isinθ)2

Substitute, cosθ + i sin θ = e

z˙ =r2e2iθ

Thus, the Cartesian and polar co-ordinate for this vector field are z˙ =x2-y2+2ixy and z˙ =r2e2iθ respectively.

Solve for z˙ =(z¯)k

Substitute 2 for k in z˙ =(z¯)k

z˙ =(z¯)2

Substitute z¯ = x-iy

z˙ =(x-iy)2

z˙ =x2-y2-2ixy

This is the Cartesian co-ordinate for this vector field.

Solve for polar coordinates.

Substitute, r cos θ for x, r sin θ for y in z˙ = x-iy and solve

z˙ =(rcosθ-i(rsinθ))2

z˙ =r2(cosθ - isinθ)2

Substitute, e-iθ=(cos θ- isin θ)

z˙ =r2e-2iθ

Thus, the Cartesian and polar coordinates for this vector field are z˙ =x2-y2-2ixy and z˙ =r2e-2iθ respectively.

Case 3)

k=3

Solve for z˙ = zk

z˙ = (z)3

Substitute, z= x + iy  and solve,

z˙ =(x+iy)3

z˙=x3-3xy2+i(3x2y - y3)

This is the Cartesian co-ordinate for this vector field.

Solve for polar coordinates,

Substitute, rcosθ for x and rsinθ for y

z˙ =(r cosθ+i(sinθ))3

z˙ =r3(cosθ+isinθ)3

Substitute, cosθ + i sin θ = e

Thus, the Cartesian and polar co-ordinate for this vector field are z˙=x3-3xy2+i(3x2y - y3) and z˙=r3e3iθ respectively.

Solve for z˙ =(z¯)k

Substitute, 3 for k in z˙ =(z¯)k

z˙ =(z¯)3

Substitute z¯ = x-iy

z˙=(x-iy)3

z˙=x3-xy2-i(3x2y-y3)

This is the Cartesian co-ordinate for this vector field.

Solve for polar coordinates.

Substitute, r cos θ for x, r sin θ for y in z˙ = x-iy and solve

z˙ =(rcosθ-i(rsinθ))3

z˙ =r3(cosθ - i sinθ)3

Substitute, e-iθ=(cos θ- isin θ)

z˙ =r3e-3iθ

Thus, the Cartesian and polar coordinates for this vector field are z˙=x3-xy2-i(3x2y-y3) and z˙ =r3e-3iθ respectively.

b)

It is to be shown that origin is the only fixed point

Take case 1 as k=1

Substitute, 0 for z˙ in the vector field z˙ =re

0=re

r=0

Substitute, 0 for z˙ in the vector field z˙ =re-iθ

0=re-iθ

r=0

The index can be calculated as,

Ic=1[ϕ]c

For the vector field z˙ =e kiθ, substitute for ϕ and take the limits from 0 to 2π

Ic=1[]0Ic=1k(2π-0)Ic=k

For the vector field z˙ =e- kiθ, substitute for ϕ and take the limits from 0 to 2π

Ic=1[-kθ]0Ic=1(-k)(2π-0)Ic= -k

c)

Let us generalize that this result for k>0, the index is calculated in the previous section comes out to be ±k in the vector fields zk and (z¯)k respectively. This implies that the vector fields will have k rotations on a loop enclosing the origin. Here, θ goes through a rotation of 2π due to the k in the term e±kiθ. Here, kiθ is causing counterclockwise rotation and - kiθ is causing clockwise rotation.

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Chapter 6 Solutions

Nonlinear Dynamics and Chaos

Ch. 6.1 - Prob. 11ECh. 6.1 - Prob. 12ECh. 6.1 - Prob. 13ECh. 6.1 - Prob. 14ECh. 6.2 - Prob. 1ECh. 6.2 - Prob. 2ECh. 6.3 - Prob. 1ECh. 6.3 - Prob. 2ECh. 6.3 - Prob. 3ECh. 6.3 - Prob. 4ECh. 6.3 - Prob. 5ECh. 6.3 - Prob. 6ECh. 6.3 - Prob. 7ECh. 6.3 - Prob. 8ECh. 6.3 - Prob. 9ECh. 6.3 - Prob. 10ECh. 6.3 - Prob. 11ECh. 6.3 - Prob. 12ECh. 6.3 - Prob. 13ECh. 6.3 - Prob. 14ECh. 6.3 - Prob. 15ECh. 6.3 - Prob. 16ECh. 6.3 - Prob. 17ECh. 6.4 - Prob. 1ECh. 6.4 - Prob. 2ECh. 6.4 - Prob. 3ECh. 6.4 - Prob. 4ECh. 6.4 - Prob. 5ECh. 6.4 - Prob. 6ECh. 6.4 - Prob. 7ECh. 6.4 - Prob. 8ECh. 6.4 - Prob. 9ECh. 6.4 - Prob. 10ECh. 6.4 - Prob. 11ECh. 6.5 - Prob. 1ECh. 6.5 - Prob. 2ECh. 6.5 - Prob. 3ECh. 6.5 - Prob. 4ECh. 6.5 - Prob. 5ECh. 6.5 - Prob. 6ECh. 6.5 - Prob. 7ECh. 6.5 - Prob. 8ECh. 6.5 - Prob. 9ECh. 6.5 - Prob. 10ECh. 6.5 - Prob. 11ECh. 6.5 - Prob. 12ECh. 6.5 - Prob. 13ECh. 6.5 - Prob. 14ECh. 6.5 - Prob. 15ECh. 6.5 - Prob. 16ECh. 6.5 - Prob. 17ECh. 6.5 - Prob. 18ECh. 6.5 - Prob. 19ECh. 6.5 - Prob. 20ECh. 6.6 - Prob. 1ECh. 6.6 - Prob. 2ECh. 6.6 - Prob. 3ECh. 6.6 - Prob. 4ECh. 6.6 - Prob. 5ECh. 6.6 - Prob. 6ECh. 6.6 - Prob. 7ECh. 6.6 - Prob. 8ECh. 6.6 - Prob. 9ECh. 6.6 - Prob. 10ECh. 6.6 - Prob. 11ECh. 6.7 - Prob. 1ECh. 6.7 - Prob. 2ECh. 6.7 - Prob. 3ECh. 6.7 - Prob. 4ECh. 6.7 - Prob. 5ECh. 6.8 - Prob. 1ECh. 6.8 - Prob. 2ECh. 6.8 - Prob. 3ECh. 6.8 - Prob. 4ECh. 6.8 - Prob. 5ECh. 6.8 - Prob. 6ECh. 6.8 - Prob. 7ECh. 6.8 - Prob. 8ECh. 6.8 - Prob. 9ECh. 6.8 - Prob. 10ECh. 6.8 - Prob. 11ECh. 6.8 - Prob. 12ECh. 6.8 - Prob. 13ECh. 6.8 - Prob. 14E
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