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Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: F λ ( z )= z n + λ z n , n ≥2 (why the case n = 2 is ) Mark Morabito Monica Moreno Rocha Kevin Pilgrim Elizabeth Russell Yakov Shapiro David Uminsky C R A Z Y

Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Page 1: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Dynamics of the family of complex maps

Paul BlanchardToni GarijoMatt HolzerU. HoomiforgotDan LookSebastian Marotta

with:€

Fλ (z) = zn +λ

zn, n ≥ 2

(why the case n = 2 is )

Mark MorabitoMonica Moreno RochaKevin PilgrimElizabeth RussellYakov ShapiroDavid Uminsky

CR AZ Y

Page 2: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (z) = z n +λ

z n

The case n > 2 is great because:

Page 3: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (z) = z n +λ

z n

The case n > 2 is great because:

There exists a McMullen domain around = 0 ....

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Parameter plane for n=3

λ

Page 4: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (z) = z n +λ

z n

The case n > 2 is great because:

... surrounded by infinitely many “Mandelpinski” necklaces...

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There exists a McMullen domain around = 0 ....

λ

Page 5: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (z) = z n +λ

z n

The case n > 2 is great because:

... surrounded by infinitely many “Mandelpinski” necklaces...

... and the Julia sets behave nicely as

λ → 0

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λ =.01

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λ =.0001

λ =.000001

There exists a McMullen domain around = 0 ....

λ

Page 6: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (z) = z n +λ

z n

There is no McMullen domain....

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The case n = 2 is crazy because:

Page 7: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (z) = z n +λ

z n

There is no McMullen domain....

... and no “Mandelpinski” necklaces...

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

QuickTime™ and aTIFF (LZW) decompressor

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The case n = 2 is crazy because:

Page 8: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (z) = z n +λ

z n

There is no McMullen domain....

... and the Julia sets “go crazy” as

λ → 0

... and no “Mandelpinski” necklaces...

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λ =−.000001

λ =−.0001

λ =−.01

The case n = 2 is crazy because:

Page 9: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Some definitions:

Julia set of

J = boundary of {orbits that escape to }

= closure {repelling periodic orbits}

= {chaotic set}

Fatou set

= complement of J

= predictable set

Fλ (z) = zn +λ

zn

Page 10: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Computation of J:

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Color points that escape toinfinity shades of red orange yellow green blue violet Black points do not escape.J = boundary of the black region.

λ =.08i

Fλ (z ) = z 3 +λ

z 3

Page 11: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

λ =.08i

is superattracting, so have immediate basin Bmapped n-to-1 to itself.

∞€

Fλ (z ) = z 3 +λ

z 3

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B

Page 12: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

is superattracting, so have immediate basin Bmapped n-to-1 to itself.

∞€

Fλ (z ) = z 3 +λ

z 3

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B

T

λ =.08i

0 is a pole, so havetrap door T mapped

n-to-1 to B.

Page 13: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

is superattracting, so have immediate basin Bmapped n-to-1 to itself.

∞€

Fλ (z ) = z 3 +λ

z 3

0 is a pole, so havetrap door T mapped

n-to-1 to B.

The Julia set has 2n-fold symmetry.

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B

T

λ =.08i

Page 14: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

Fλ (z ) = z 3 +λ

z 3

2n free critical points

cλ = λ1/2n

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λ =.08i

Page 15: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

2n free critical points

cλ = λ1/2n

Fλ (z ) = z 3 +λ

z 3

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λ =.08i

Page 16: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

2n free critical points

cλ = λ1/2n

Only 2 critical values

vλ = ±2 λ

Fλ (z ) = z 3 +λ

z 3

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λ =.08i

Page 17: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

2n free critical points

cλ = λ1/2n

Only 2 critical values

vλ = ±2 λ

Fλ (z ) = z 3 +λ

z 3

λ =.08i

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Page 18: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

2n free critical points

cλ = λ1/2n

Only 2 critical values

vλ = ±2 λ

Fλ (z ) = z 3 +λ

z 3

λ =.08i

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Page 19: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

2n free critical points

cλ = λ1/2n

Only 2 critical values

vλ = ±2 λ

But really only 1 freecritical orbit

Fλ (z ) = z 3 +λ

z 3

λ =.08i

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Page 20: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Easy computations:

2n free critical points

pλ = (−λ )1/2n

Only 2 critical values

vλ = ±2 λ

But really only 1 freecritical orbit

Fλ (z ) = z 3 +λ

z 3

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λ =.08iAnd 2n prepoles

cλ = λ1/2n

Page 21: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

The Escape Trichotomy

There are three possible ways that thecritical orbits can escape to infinity,

and each yields a different typeof Julia set.

(with D. Look & D Uminsky)

Page 22: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

The Escape Trichotomy

vλ∈

J ( Fλ

)

⇒B is a Cantor set

(with D. Look & D Uminsky)

Page 23: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

The Escape Trichotomy

vλ∈

J ( Fλ

)

⇒B

is a Cantor set

T

vλ∈ is a Cantor set of

simple closed curves

J ( Fλ

)

(McMullen)

(with D. Look & D Uminsky)

(n > 2)

Page 24: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

The Escape Trichotomy

vλ∈

J ( Fλ

)

⇒B

⇒€

is a Cantor set

T

vλ∈ is a Cantor set of

simple closed curves

J ( Fλ

)

k(v

λ) ∈ T

J ( Fλ

) is a Sierpinski curve

(McMullen)

(with D. Look & D Uminsky)

(n > 2)

In all other cases is a connected set, and if

J ( Fλ

)

Page 25: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

vλ∈

J ( Fλ

)

⇒BCase 1:

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parameter planewhen n = 3

is a Cantor set

Page 26: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

vλ∈

J ( Fλ

)

⇒BCase 1:

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are needed to see this picture.

parameter planewhen n = 3

λ

is a Cantor set

Page 27: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

vλ∈

J ( Fλ

)

⇒BCase 1:

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parameter planewhen n = 3

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J is a Cantor set

λ

is a Cantor set

Page 28: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

vλ∈

J ( Fλ

)

⇒BCase 1:

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parameter planewhen n = 3

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J is a Cantor set

λ

is a Cantor set

Page 29: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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parameter planewhen n = 3

Case 2: T

vλ∈

J ( Fλ

) is a Cantor set ofsimple closed curves

Page 30: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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parameter planewhen n = 3

λ

Case 2: T

vλ∈

J ( Fλ

) is a Cantor set ofsimple closed curves

Page 31: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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The central disk isthe McMullen domain

λ

Case 2: T

vλ∈ is a Cantor set of

simple closed curves

J ( Fλ

)

Page 32: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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parameter planewhen n = 3

λ

Case 2: T

vλ∈ is a Cantor set of

simple closed curves

J is a Cantor set of simple closed curves

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J ( Fλ

)

T

B

Page 33: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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parameter planewhen n = 3

λ

Case 2: T

vλ∈ is a Cantor set of

simple closed curves

J is a Cantor set of simple closed curves

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J ( Fλ

)

Page 34: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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parameter planewhen n = 3

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

) is a Sierpinski curve

Page 35: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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parameter planewhen n = 3

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

)

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A Sierpinski curve is a planarset homeomorphic to theSierpinski carpet fractal

is a Sierpinski curve

Page 36: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Sierpinski curves are important for two reasons:

1. There is a “topological characterization” of the carpet

2. A Sierpinski curve is a “universal plane continuum”

Page 37: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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The Sierpinski Carpet

Topological Characterization

Any planar set that is:1. compact2. connected3. locally connected4. nowhere dense5. any two complementary domains are bounded by simple closed curves that are pairwise disjoint is a Sierpinski curve.

Page 38: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Universal Plane Continuum

Any planar, one-dimensional, compact, connected set can be homeomorphically embedded in a Sierpinski curve.

For example....

Page 39: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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This set

Page 40: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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This set

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can be embedded inside

Page 41: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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parameter planewhen n = 3

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

) is a Sierpinski curve

Page 42: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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λ

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

) is a Sierpinski curve

A Sierpinski “hole”

Page 43: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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λ

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

)

A Sierpinski curve

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is a Sierpinski curve

A Sierpinski “hole”

Page 44: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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λ

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

)

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Fλ (vλ )

A Sierpinski curve

is a Sierpinski curve

A Sierpinski “hole”Escape time 3

Page 45: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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λ

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

)

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A Sierpinski curve

is a Sierpinski curve

Another Sierpinski “hole”

Page 46: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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λ

Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

)

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A Sierpinski curve

is a Sierpinski curve

Another Sierpinski “hole”

Fλ2(vλ )

Escape time 4

Page 47: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

)

λ

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A Sierpinski curve

is a Sierpinski curve

Another Sierpinski “hole”Escape time 7

Page 48: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Case 3:

Fλk(v λ ) ∈ T

J ( Fλ

)

λ

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A Sierpinski curve

is a Sierpinski curve

Another Sierpinski “hole”Escape time 5

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So to show that is homeomorphic to

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

Fatou set is the union of the preimages of B; all disjoint, open disks.

Page 52: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

Fatou set is the union of the preimages of B; all disjoint, open disks.

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

If J contains an open set, then J = C.

Page 54: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

If J contains an open set, then J = C.

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

No recurrent critical orbits and no parabolic points.

Page 56: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

No recurrent critical orbits and no parabolic points.

Page 57: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

J locally connected, so theboundaries are locally connected. Need to show they are s.c.c.’s. Can only meet at (preimages of) critical points, hence disjoint.

Page 58: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Need to show:

compactconnectednowhere denselocally connectedbounded by disjoint s.c.c.’s

So J is a Sierpinski curve.

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Remark: All Julia sets drawn from Sierpinski holes are homeomorphic, but only those in symmetrically locatedSierpinski holes have the same dynamics.

The maps on all these Julia sets are dynamically different.

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Remark: All Julia sets drawn from Sierpinski holes are homeomorphic, but only those in symmetrically locatedSierpinski holes have the same dynamics.

In fact, there are exactly (n-1)(2n)k-3 Sierpinski holes withescape time k, and (2n)k-3 different conjugacy classes (n odd).

The maps on all these Julia sets are dynamically different.

(with K.Pilgrim)

Page 61: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

1. The McMullen domain

2. Mandelpinski necklaces

3. Julia sets near 0

Topics

Page 62: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Part 1: The McMullen Domain

Page 63: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

What is the preimage of T?

First suppose

vλ∈ T:

Page 64: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

First suppose

What is the preimage of T?

vλ∈ T:

Can the preimage be 2n disjoint disks, each of which contains a critical point?

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Page 65: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

First suppose

What is the preimage of T?

vλ∈ T:

Can the preimage be 2n disjoint disks, each of which contains a critical point?

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are needed to see this picture.

No --- there would then be 4n preimages of any point in T, but the map has degree 2n.

Page 66: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

So some of the preimages of Tmust overlap, and by 2n-foldsymmetry, all must intersect.

Page 67: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

So some of the preimages of Tmust overlap, and by 2n-foldsymmetry, all must intersect.

By Riemann-Hurwitz, the preimage of T must then

be an annulus.

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Page 68: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

So here is the picture:

T

B

A

A is the annulus separating B and T

Page 69: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

So here is the picture:B

TA

A is the annulus separating B and T

XF maps X 2n-to-1

onto T

Page 70: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

So here is the picture:B

TA

A is the annulus separating B and T

X

A

A

0

1

F maps both A0

1and A as an n-to-1

covering onto A

F maps X 2n-to-1onto T

Page 71: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

B

TA

X

A

A

0

1

So mod(A0) = 1/n mod(A)

And mod(A1) = 1/n mod(A)

Page 72: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

B

TA

X

A

A

0

1

So mod(A0) = 1/n mod(A)

And mod(A1) = 1/n mod(A)

When n = 2,mod(A0) + mod(A1) =

mod(A)

Page 73: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

B

TA

X

A

A

0

1

So mod(A0) = 1/n mod(A)

And mod(A1) = 1/n mod(A)

When n = 2,mod(A0) + mod(A1) =

mod(A)

So there is no room for X, i.e., does

not lie in T

Page 74: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

vλ = ±2 λ

Fλ (vλ ) = 2nλn /2 +λ

2nλn /2 = 2nλn /2 +1

2nλ (n /2−1)

Why is there no McMullen domain when n = 2?

Here is another reason:

Page 75: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (vλ ) = 2nλn /2 +λ

2nλn /2 = 2nλn /2 +1

2nλ (n /2−1)

Why is there no McMullen domain when n = 2?

Here is another reason:

n > 2⇒ Fλ (vλ ) → ∞ as λ → 0

vλso lies in T when n > 2

vλ = ±2 λ

Page 76: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Why is there no McMullen domain when n = 2?

Here is another reason:

n > 2⇒ Fλ (vλ ) → ∞ as λ → 0

n = 2⇒ Fλ (vλ ) = 4λ +1

4€

vλso lies in T when n > 2

vλ = ±2 λ

Fλ (vλ ) = 2nλn /2 +λ

2nλn /2 = 2nλn /2 +1

2nλ (n /2−1)

Page 77: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Fλ (vλ ) = 2nλn /2 +λ

2nλn /2 = 2nλn /2 +1

2nλ (n /2−1)

Why is there no McMullen domain when n = 2?

Here is another reason:

n > 2⇒ Fλ (vλ ) → ∞ as λ → 0

so Fλ (vλ ) →1/ 4 as λ → 0(???)€

vλso lies in T when n > 2

vλ = ±2 λ

n = 2⇒ Fλ (vλ ) = 4λ +1

4

Page 78: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Part 2: Mandelpinski Necklaces

Page 79: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Parameter plane for n = 3

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A “Mandelpinski necklace” is a simple closed curve in the parameter plane that passes alternately through k centersof baby Mandelbrot sets and k centers of Sierpinski holes.

Page 80: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Parameter plane for n = 3

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are needed to see this picture.

A “Mandelpinski necklace” is a simple closed curve in the parameter plane that passes alternately through k centersof baby Mandelbrot sets and k centers of Sierpinski holes.

C1 passes through thecenters of 2 M-sets

and 2 S-holes

Page 81: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Parameter plane for n = 3

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

A “Mandelpinski necklace” is a simple closed curve in the parameter plane that passes alternately through k centersof baby Mandelbrot sets and k centers of Sierpinski holes.

Page 82: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Parameter plane for n = 3

A “Mandelpinski necklace” is a simple closed curve in the parameter plane that passes alternately through k centersof baby Mandelbrot sets and k centers of Sierpinski holes.

C2 passes through thecenters of 4 M-sets

and 4 S-holesQuickTime™ and a

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*

* only exception:2 centers of period 2 bulbs, not M-sets

Page 83: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

A “Mandelpinski necklace” is a simple closed curve in the parameter plane that passes alternately through k centersof baby Mandelbrot sets and k centers of Sierpinski holes.

C3 passes through thecenters of 10 M-sets

and 10 S-holes

Parameter plane for n = 3

Page 84: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

A “Mandelpinski necklace” is a simple closed curve in the parameter plane that passes alternately through k centersof baby Mandelbrot sets and k centers of Sierpinski holes.

C4 passes through thecenters of 28 M-sets

and 28 S-holes

Parameter plane for n = 3

Page 85: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

A “Mandelpinski necklace” is a simple closed curve in the parameter plane that passes alternately through k centersof baby Mandelbrot sets and k centers of Sierpinski holes.

C5 passes through thecenters of 82 M-sets

and 82 S-holesQuickTime™ and a

TIFF (LZW) decompressorare needed to see this picture.

Parameter plane for n = 3

Page 86: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Theorem: There exist closed curves Cj, surrounding the McMullen domain. Each Cj passes

alternately through (n-2)nj-1 +1 centers of baby Mandelbrot sets and centers of Sierpinski holes.€

j = 1,...,∞

Page 87: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

C14 passes through thecenters of 4,782,969 M-sets and S-holesQuickTime™ and a

TIFF (LZW) decompressorare needed to see this picture.

Parameter plane for n = 3

Theorem: There exist closed curves Cj, surrounding the McMullen domain. Each Cj passes

alternately through (n-2)nj-1 +1 centers of baby Mandelbrot sets and centers of Sierpinski holes.€

j = 1,...,∞

Page 88: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Parameter plane for n = 4

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C1: 3 holes and M-sets

Theorem: There exist closed curves Cj, surrounding the McMullen domain. Each Cj passes

alternately through (n-2)nj-1 +1 centers of baby Mandelbrot sets and centers of Sierpinski holes.€

j = 1,...,∞

Page 89: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Parameter plane for n = 4

C2: 9 holes and M-setsC3: 33 holes and M-setsQuickTime™ and a

TIFF (LZW) decompressorare needed to see this picture.

Theorem: There exist closed curves Cj, surrounding the McMullen domain. Each Cj passes

alternately through (n-2)nj-1 +1 centers of baby Mandelbrot sets and centers of Sierpinski holes.€

j = 1,...,∞

*

Page 90: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Easy computations:

Fλ (z ) = z 3 +λ

z 3

λ =.08i

All of the criticalpoints and prepoleslie on the “criticalcircle” : |z| = | |

λ 1/2n

γ0

γ0

Page 91: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Fλ (z ) = z 3 +λ

z 3

λ =.08i

All of the criticalpoints and prepoleslie on the “criticalcircle” : |z| = | |

λ 1/2n

γ0

γ0

which is mapped 2n-to-1onto the “critical value line”

connecting

±vλ €

−vλ

Easy computations:

Page 92: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Fλ (z ) = z 3 +λ

z 3

λ =.08i

γ0

Any other circle around 0is mapped n-to-1 to an ellipse

whose foci are

±2 λ

Easy computations:

−vλ

Page 93: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

Fλ (z ) = z 3 +λ

z 3

λ =.08i

γ0

±2 λ

Easy computations:

−vλ

Any other circle around 0is mapped n-to-1 to an ellipse

whose foci are

Page 94: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

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Fλ (z ) = z 3 +λ

z 3

λ =.08i

γ0

±2 λ

So the exterior of is mapped as an n-to-1 covering of the

exterior of the critical value line. €

γ0

Easy computations:

−vλ

Any other circle around 0is mapped n-to-1 to an ellipse

whose foci are

Page 95: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

Fλ (z ) = z 3 +λ

z 3

λ =.08i

γ0

±2 λ

So the exterior of is mapped as an n-to-1 covering of the

exterior of the critical value line. Same with the interior of . €

γ0

γ0

Easy computations:

−vλ

Any other circle around 0is mapped n-to-1 to an ellipse

whose foci are

Page 96: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Simplest case: C1

Assume that both sit on the critical circle.

±vλ

−vλ

γ0

(i.e., )

| vλ | = | cλ | = | pλ |

⇒ 2 | λ |1/2 = | λ |1/2n

Page 97: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Assume that both sit on the critical circle.

±vλ

−vλ

γ0

Simplest case: C1

⇒ 2 | λ |1/2 = | λ |1/2n

⇒ 22n | λ |n = | λ |

⇒ | λ | = 2−

2n

n−1 ⎛ ⎝

⎞ ⎠

Page 98: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Assume that both sit on the critical circle.

±vλ

This is the “dividing circle” in the parameter plane

Parameter plane n = 3

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r = 2-3

Simplest case: C1

⇒ 2 | λ |1/2 = | λ |1/2n

⇒ 22n | λ |n = | λ |

⇒ | λ | = 2−

2n

n−1 ⎛ ⎝

⎞ ⎠

Page 99: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

Assume that both sit on the critical circle.

±vλ

⇒ 2 | λ |1/2 = | λ |1/2n

⇒ 22n | λ |n = | λ |

This is the “dividing circle” in the parameter plane

Parameter plane n = 4

⇒ | λ | = 2−

2n

n−1 ⎛ ⎝

⎞ ⎠

r = 2-8/3

Simplest case: C1

Page 100: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Assume that lies on the dividing circle,so both sit on the critical circle.

±vλ

−vλ

γ0

λ

In this picture, is real and n = 3

λ

Simplest case: C1

Page 101: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Assume that lies on the dividing circle,so both sit on the critical circle.

±vλ

−vλ

γ0

As rotates around the dividing circle, rotates a half-turn, while and rotate1/2n of a turn. So each meets exactlyn - 1 prepoles and critical points.€

λ

±vλ

λ

pλ€

In this picture, is real and n = 3

λ

Simplest case: C1

Page 102: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Assume that lies on the dividing circle,so both sit on the critical circle.

±vλ

−vλ

γ0

As rotates around the dividing circle, rotates a half-turn, while and rotate1/2n of a turn. So each meets exactlyn - 1 prepoles and critical points.€

λ

±vλ

λ

pλ€

In this picture, is real and n = 3

λ

Simplest case: C1

So the dividing circle is C1

Page 103: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

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The dividing circle when n = 5

n-1 = 4 centers of Sierpinski holes;n-1 = 4 centers of baby Mandelbrot sets

Page 104: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Now assume that lies inside the critical circle:

±vλ

γ0€

−vλ

Page 105: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

γ0

Now assume that lies inside the critical circle:

±vλ

The exterior of is mapped n-to-1onto the exterior of the critical value ray, so there is a preimage mapped n-to-1 to , €

γ0

γ0

γ1

−vλ

Page 106: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Now assume that lies inside the critical circle:

±vλ

γ0€

−vλ

γ1

The exterior of is mapped n-to-1onto the exterior of the critical value ray, so there is a preimage mapped n-to-1 to , €

γ0

γ0

γ1

Page 107: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

then is mapped n-to-1 to ,

γ1

Now assume that lies inside the critical circle:

±vλ

γ2

γ0€

−vλ

γ1

γ2

The exterior of is mapped n-to-1onto the exterior of the critical value ray, so there is a preimage mapped n-to-1 to , €

γ0

γ0

γ1

Page 108: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

and on and onout to

∂B

Now assume that lies inside the critical circle:

±vλ

then is mapped n-to-1 to ,

γ1

γ0€

−vλ

γ1

γ2

B

The exterior of is mapped n-to-1onto the exterior of the critical value ray, so there is a preimage mapped n-to-1 to , €

γ0

γ0

γ1

γ2

Page 109: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

γ0 contains 2n critical points and 2n prepoles, so

γ1 contains 2n2 pre-critical points and pre-prepoles

γ0€

−vλ

γ1

Page 110: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

γ0 contains 2n critical points and 2n prepoles, so

γ1 contains 2n2 pre-critical points and pre-prepoles

γ0€

−vλ

γ1

γ2

B

γk contains 2nk+1 points thatmap to the critical pointsand pre-prepoles under

Fλk

Page 111: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

γ0€

−vλ

γk

As rotates by one turn, these 2nk+1 points on each rotate by 1/2nk+1 of a turn.

γk

λ

Page 112: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

γ0€

−vλ

γk

Fλ (vλ ) ≈λ

2nλn /2 =1

2nλ1−n /2

Since

the second iterate of the criticalpoints rotate by 1 - n/2 ofa turn

As rotates by one turn, these 2nk+1 points on each rotate by 1/2nk+1 of a turn.

γk

λ

Page 113: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

γ0€

−vλ

γk

Fλ (vλ ) ≈λ

2nλn /2 =1

2nλ1−n /2

Since

the second iterate of the criticalpoints rotate by 1 - n/2 ofa turn, so this point hitsexactly

(n / 2 −1)(2nk+1) +1 = (n − 2)nk+1 +1

preimages of the critical pointsand prepoles on

γk

As rotates by one turn, these 2nk+1 points on each rotate by 1/2nk+1 of a turn.

γk

λ

Page 114: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

There is a natural parametrization of each

γk

γkλ (θ )

The real proof involves the Schwarz Lemma:

γ0€

−vλ

γk

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are needed to see this picture.

γkλ (θ )

Page 115: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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are needed to see this picture.

There is a natural parametrization of each

γk

γkλ (θ )

The real proof involves the Schwarz Lemma:

γ0€

−vλ

γk

γkλ (θ )

Best to restrict to a “symmetry region” inside the dividingcircle, so that is well-defined.

γkλ (θ )

Page 116: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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γ0€

−vλ

γk

γkλ (θ )

Then we have a second map from the parameter plane to thedynamical plane, namely which is invertible on the symmetry sector

G(λ ) = Fλ (vλ )

G−1

Best to restrict to a “symmetry region” inside the dividingcircle, so that is well-defined.

γkλ (θ )

Page 117: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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γ0€

−vλ

γk

γkλ (θ )

Then we have a second map from the parameter plane to thedynamical plane, namely which is invertible on the symmetry sector

G(λ ) = Fλ (vλ )

G−1

G−1(γ kλ (θ ) )

a map from a “disk” to itself.

So consider the composition

Page 118: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

γ0€

−vλ

γk

γkλ (θ )

G−1

G−1(γ kλ (θ ) )

a map from a “disk” to itself.

So consider the composition

Schwarz implies that has a unique fixed point,i.e., a parameter for which the second iterate of the criticalpoint lands on the point , so this proves theexistence of the centers of the S-holes and M-sets.€

G−1(γ kλ (θ ) )

γkλ (θ )

Page 119: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Remarks: This proves the existence of centers of Sierpinski holes and Mandelbrot sets. Producingthe entire M-set involves polynomial-like maps;while the entire S-hole involves qc-surgery.

Page 120: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Part 3: Behavior of the Julia sets

Page 121: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

n = 2: When , the Julia set of is the unit circle. But, as , the Julia set of converges to the closed unit disk

λ → 0

λ =0

Part 3: Behavior of the Julia sets

Page 122: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

n > 2: J is always a Cantor set of “circles” when is small.

n = 2: When , the Julia set of is the unit circle. But, as , the Julia set of converges to the closed unit disk

λ → 0

λ =0

λ

Part 3: Behavior of the Julia sets

Page 123: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

n > 2: J is always a Cantor set of “circles” when is small.

n = 2: When , the Julia set of is the unit circle. But, as , the Julia set of converges to the closed unit disk

λ → 0

λ =0

Moreover, there is a such that there is always a“round” annulus of “thickness” between two of these circles in the Fatou set. So J does not converge to the unit disk when n > 2.

λ

δ > 0

δ

Part 3: Behavior of the Julia sets

Page 124: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

n = 2

Theorem: When n = 2, the Julia sets converge to the unit disk as

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λ → 0

Page 125: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Suppose the Julia sets do not converge to the unit disk D as

λ → 0

Sketch of the proof:

Page 126: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Suppose the Julia sets do not converge to the unit disk D as

λ → 0

Sketch of the proof:

Then there exists and a sequence such that, for each i,there is a point such that lies in the Fatou set.

Bδ (zi )

δ > 0

λi → 0

zi ∈D

Page 127: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Suppose the Julia sets do not converge to the unit disk D as

λ → 0

Sketch of the proof:

Then there exists and a sequence such that, for each i,there is a point such that lies in the Fatou set.

Bδ (zi )

λi → 0

zi ∈D

Bδ (z1)

Bδ (z2 )

Bδ (z3)

Bδ (z4 )

δ > 0

Page 128: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Suppose the Julia sets do not converge to the unit disk D as

λ → 0

Sketch of the proof:

Then there exists and a sequence such that, for each i,there is a point such that lies in the Fatou set.

Bδ (zi )

λi → 0

zi ∈D

The must accumulate on some nonzero point, say ,so we may assume that lies in the Fatou set for all i.

zi

z*

Bδ (z*)

Bδ (z1)

Bδ (z2 )

Bδ (z3)

Bδ (z4 )

δ > 0

Page 129: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Suppose the Julia sets do not converge to the unit disk D as

λ → 0

Sketch of the proof:

Then there exists and a sequence such that, for each i,there is a point such that lies in the Fatou set.

Bδ (zi )

λi → 0

zi ∈D

Bδ (z*)

The must accumulate on some nonzero point, say ,so we may assume that lies in the Fatou set for all i.

zi

z*

Bδ (z*)

δ > 0

Page 130: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Suppose the Julia sets do not converge to the unit disk D as

λ → 0

Sketch of the proof:

Then there exists and a sequence such that, for each i,there is a point such that lies in the Fatou set.

Bδ (zi )

λi → 0

zi ∈D

Bδ (z*)

The must accumulate on some nonzero point, say ,so we may assume that lies in the Fatou set for all i.

zi

z*

Bδ (z*)

But for large i, so stretchesinto an “annulus” that surrounds the origin, so thisdisconnects the Julia set.€

Fλ i ≈ z2

Fλ ik

Bδ (z*)€

Fλk

δ > 0

Page 131: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

So the Fatou components must become arbitrarily small:

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λ =−0.0001

λ =−0.0000001

Page 132: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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λ =.01

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λ =.0001

λ =.000001

n > 2: Note the “round” annuli in the Fatou set; there is alwayssuch an annulus of some fixed width for small.

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λ =.00000001

λ =.0000000001

| λ |

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λ =.000000000001

Page 133: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

T

B

| λ | small

⇒ T is tiny

A0

mod A0 = m is huge

Say n = 3:

Page 134: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

T

B

| λ | small

⇒ T is tiny

A0

mod A0 = m is hugeand the boundary of A0

is very close to S1

Say n = 3:

Page 135: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

T

B

| λ | small

⇒ T is tinymod A0 = m is hugeand the boundary of A0

is very close to S1

Say n = 3:

X1

A1

A1 and A1 mapped to A0;X1 is mapped to T

X1

A1

A1

~~

A0

mod A1 = mod A1 = mod X1 = m/3; A1 S1

∂~

Page 136: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

T

B

| λ | small

⇒ T is tinymod A0 = m is hugeand the boundary of A0

is very close to S1

Say n = 3:

X1

A1

A1 and A1 mapped to A0;X1 is mapped to T

X2

A1

A2

A2 is mapped to A1;X2 is mapped to X1

mod A2 = mod X2 = m/32; A2 S1

⇒mod A1 = mod A1 = mod X1 = m/3; A1 S1

~

~

Page 137: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

B

| λ | small

⇒ T is tinymod A0 = m is hugeand the boundary of A0

is very close to S1

Say n = 3:

A1 and A1 mapped to A0;X1 is mapped to T

Xk

Ak

Ak-1

M

Ak is mapped to Ak-1; Xk to Xk-1

mod A2 = mod X2 = m/32; A2 S1

⇒mod A1 = mod A1 = mod X1 = m/3; A1 S1

~

∂mod Ak = mod Xk = m/3k; Ak S1

A2 is mapped to A1;X2 is mapped to X1

~

N

Page 138: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

B

| λ | small

⇒ T is tinymod A0 = m is hugeand the boundary of A0

is very close to S1

Say n = 3:

Xk

Ak

Ak-1

1 mod Ak < 3

≤Eventually find k sothatand Ak S1

Page 139: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

B

| λ | small

⇒ T is tinymod A0 = m is hugeand the boundary of A0

is very close to S1

Say n = 3:

Xk

Ak

Ak-1

1 mod Ak < 3

≤Eventually find k sothatand Ak S1

⇒ Ak must contain a round annulus of modulus

(Ble, Douady, and Henriksen)

α −1/2 >1/2

Page 140: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

B

| λ | small

⇒ T is tinymod A0 = m is hugeand the boundary of A0

is very close to S1

Say n = 3:

Xk

Ak

Ak-1

⇒ Ak must contain a round annulus of modulus

(Ble, Douady, and Henriksen)

But does this annulus have definite “thickness?”

1 mod Ak < 3

≤Eventually find k sothatand Ak S1

α −1/2 >1/2

Page 141: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

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∂Ak in here

Page 142: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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∂Ak in here

=αmod Ak

says that the innerboundary of Ak

cannot be insideor outside ,so the round annulusin Ak is “thick”€

γ0

γ1

γ1

γ0

Ak

Page 143: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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∂Ak in here

μ1

μ0

Ak

Same argumentsays that Ak Xk

is twice as thick

∪ Xk

Page 144: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

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Xk

So Xk musthave definite thickness as well

Page 145: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Part 4: A major application

Page 146: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Here’s the parameter plane when n = 2:

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Page 147: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

Qu

ickTim

e™

an

d a

TIF

F (

LZ

W)

decom

pre

sso

rare

nee

de

d t

o s

ee t

his

pic

ture

.

Rotate it by 90 degrees:

and this object appears everywhere.....

Page 148: Dynamics of the family of complex maps Paul Blanchard Toni Garijo Matt Holzer U. Hoomiforgot Dan Look Sebastian Marotta with: (why the case n = 2 is )

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.