Chaos Theory: A Journey from Kepler to Fractals
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I
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Department of Physics
University of Wisconsin - Madison
Presented to Physics 311
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,
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on October 31, 2014
undefinedA
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H
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y
n
Kepler (1605)
n
Newton (1687)
n
Poincare (1890)
n
Lorenz (1963)
K
e
p
l
e
r
(
1
6
0
5
)
n
Tycho Brahe
n
3 laws of planetary motion
n
Elliptical orbits
N
e
w
t
o
n
(
1
6
8
7
)
n
Invented calculus
n
Derived 3 laws of motion
F = ma
n
Proposed law of gravity
F
=
Gm
1
1
m
2
/
r
2
n
Explained Kepler’s laws
n
Got headaches (3 body problem)
P
o
i
n
c
a
r
e
(
1
8
9
0
)
n
200 years later!
n
King Oscar (Sweden, 1887)
n
Prize won – 200 pages
n
No analytic solution exists!
n
Sensitive dependence on initial
conditions (Lyapunov exponent)
n
Chaos! (Li & Yorke, 1975)
3
-
B
o
d
y
P
r
o
b
l
e
m
C
h
a
o
s
n
Sensitive dependence on initial
conditions (positive Lyapunov exp)
n
Aperiodic (never repeats)
n
Topologically mixing
n
Dense periodic orbits
S
i
m
p
l
e
P
e
n
d
u
l
u
m
F = ma
-mg
sin
x
=
md
2
x/dt
2
dx/dt = v
dv/dt = -g
sin
x
dv/dt
=
-x
(for
g
= 1,
x
<< 1)
Dynamical system
Flow in 2-D phase space
P
h
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s
e
S
p
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c
e
P
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t
f
o
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P
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a
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r
e
s
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P
e
n
d
u
l
u
m
F
l
o
w
n
Stable (O) & unstable (X) equilibria
n
Linear and nonlinear regions
n
Conservative / time-reversible
n
Trajectories cannot intersect
P
e
n
d
u
l
u
m
w
i
t
h
F
r
i
c
t
i
o
n
dx/dt = v
dv/dt = -
sin
x – bv
F
e
a
t
u
r
e
s
o
f
P
e
n
d
u
l
u
m
F
l
o
w
n
Dissipative (cf: conservative)
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Attractors (cf: repellors)
n
Poincare-Bendixson theorem
n
No chaos in 2-D autonomous system
D
a
m
p
e
d
D
r
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v
e
n
P
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d
u
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u
m
dx/dt = v
dv/dt = -
sin
x – bv +
sin
t
2-D
3-D
nonautonomous
autonomous
dx/dt = v
dv/dt = -
sin
x – bv +
sin
z
dz/dt =
N
e
w
F
e
a
t
u
r
e
s
i
n
3
-
D
F
l
o
w
s
n
More complicated trajectories
n
Limit cycles (2-D attractors)
n
Strange attractors (fractals)
n
Chaos!
S
t
r
e
t
c
h
i
n
g
a
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d
F
o
l
d
i
n
g
C
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C
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c
u
i
t
E
q
u
a
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i
o
n
s
f
o
r
C
h
a
o
t
i
c
C
i
r
c
u
i
t
dx/dt = y
dy/dt = z
dz/dt = az – by + c
(sgn
x
– x
)
Jerk system
Period doubling route to chaos
B
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I sometimes work on
publishable research with
bright undergraduates who are
crack computer programmers
with an interest in chaos. If
interested, contact me
.
R
e
f
e
r
e
n
c
e
s
n
http://sprott.physics.wisc.edu/
lectures/phys311.pptx
(this talk)
n
http://sprott.physics.wisc.edu/chaost
sa/
(my chaos textbook)
n
sprott@physics.wisc.edu
(contact
me)
P
r
o
p
s
n
Hard copy of slides
n
Driven chaotic pendulum
n
Ball point pen
n
Silly putty
n
Chaotic circuit / speaker
Workshop on Self-Organization
Entire presentation available on WWW
Delve into the fascinating world of chaos theory, tracing its evolution from the seminal works of Kepler and Newton to the complexities of Poincare's findings and modern chaos concepts. Discover the dynamics of chaotic systems like the simple pendulum and understand the implications of sensitive dependence on initial conditions. Explore how chaos theory has revolutionized our understanding of nonlinear systems and their behavior.
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Presentation Transcript
Introduction to Chaos Clint Sprott Department of Physics University of Wisconsin - Madison Presented to Physics 311 at University of Wisconsin in Madison, WI on October 31, 2014
Abbreviated History n Kepler (1605) n Newton (1687) n Poincare (1890) n Lorenz (1963)
Kepler (1605) n Tycho Brahe n 3 laws of planetary motion n Elliptical orbits
Newton (1687) n Invented calculus n Derived 3 laws of motion F = ma n Proposed law of gravity F = Gm1m2/r2 n Explained Kepler s laws n Got headaches (3 body problem)
Poincare (1890) n 200 years later! n King Oscar (Sweden, 1887) n Prize won 200 pages n No analytic solution exists! n Sensitive dependence on initial conditions (Lyapunov exponent) n Chaos! (Li & Yorke, 1975)
Chaos n Sensitive dependence on initial conditions (positive Lyapunov exp) n Aperiodic (never repeats) n Topologically mixing n Dense periodic orbits
Simple Pendulum F = ma -mg sin x = md2x/dt2 dx/dt = v dv/dt = -g sin x dv/dt = -x (for g = 1, x << 1) Dynamical system Flow in 2-D phase space
Features of Pendulum Flow n Stable (O) & unstable (X) equilibria n Linear and nonlinear regions n Conservative / time-reversible n Trajectories cannot intersect
Pendulum with Friction dx/dt = v dv/dt = -sin x bv
Features of Pendulum Flow n Dissipative (cf: conservative) n Attractors (cf: repellors) n Poincare-Bendixson theorem n No chaos in 2-D autonomous system
Damped Driven Pendulum dx/dt = v dv/dt = -sin x bv + sin t 2-D nonautonomous dx/dt = v dv/dt = -sin x bv + sin z dz/dt = 3-D autonomous
New Features in 3-D Flows n More complicated trajectories n Limit cycles (2-D attractors) n Strange attractors (fractals) n Chaos!
Equations for Chaotic Circuit dx/dt = y dy/dt = z dz/dt = az by + c(sgn x x) Jerk system Period doubling route to chaos
Bifurcation Diagram for Chaotic Circuit
Invitation I sometimes work on publishable research with bright undergraduates who are crack computer programmers with an interest in chaos. If interested, contact me.
References n http://sprott.physics.wisc.edu/ lectures/phys311.pptx (this talk) n http://sprott.physics.wisc.edu/chaost sa/ (my chaos textbook) n sprott@physics.wisc.edu (contact me)
