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Discontinuous standard map dynamics Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015 6 August 2015 Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015 Discontinuous standard map dynamics

Discontinuous standard map dynamics - ICERM

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Page 1: Discontinuous standard map dynamics - ICERM

Discontinuous standard map dynamics

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf

Summer@ICERM 2015

6 August 2015

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 2: Discontinuous standard map dynamics - ICERM

Consider a kicked rotator

θ̈ = K∑n∈Z

δ(t − n) sin θ

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 3: Discontinuous standard map dynamics - ICERM

Consider a kicked rotator

θ̈ = K∑n∈Z

δ(t − n) sin θ

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 4: Discontinuous standard map dynamics - ICERM

θ̈ = K∑n∈Z

δ(t − n) sin θ

p = θ̇ is the angular momentum.

Integrate around t = n:

θn+1 = θn + pn (mod 2π)

pn+1 = pn + K sin θn+1

This is known as the Chirikov standard map.

Boundedness of momentum is understood using KAM theory.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 5: Discontinuous standard map dynamics - ICERM

θ̈ = K∑n∈Z

δ(t − n) sin θ

p = θ̇ is the angular momentum.

Integrate around t = n:

θn+1 = θn + pn (mod 2π)

pn+1 = pn + K sin θn+1

This is known as the Chirikov standard map.

Boundedness of momentum is understood using KAM theory.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 6: Discontinuous standard map dynamics - ICERM

θ̈ = K∑n∈Z

δ(t − n) sin θ

p = θ̇ is the angular momentum.

Integrate around t = n:

θn+1 = θn + pn (mod 2π)

pn+1 = pn + K sin θn+1

This is known as the Chirikov standard map.

Boundedness of momentum is understood using KAM theory.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 7: Discontinuous standard map dynamics - ICERM

θ̈ = K∑n∈Z

δ(t − n) sin θ

p = θ̇ is the angular momentum.

Integrate around t = n:

θn+1 = θn + pn (mod 2π)

pn+1 = pn + K sin θn+1

This is known as the Chirikov standard map.

Boundedness of momentum is understood using KAM theory.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 8: Discontinuous standard map dynamics - ICERM

Let’s replace the sine wave by a square wave and shift horizontally:

xn+1 = xn + αyn (mod 1)

yn+1 = yn + sgn

(xn+1 −

1

2

)

We’re interested in the dynamics of this function f on the cylinder[0, 1)× R.

KAM theory does not apply here because of the lack ofsmoothness.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 9: Discontinuous standard map dynamics - ICERM

Let’s replace the sine wave by a square wave and shift horizontally:

xn+1 = xn + αyn (mod 1)

yn+1 = yn + sgn

(xn+1 −

1

2

)

We’re interested in the dynamics of this function f on the cylinder[0, 1)× R.

KAM theory does not apply here because of the lack ofsmoothness.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 10: Discontinuous standard map dynamics - ICERM

Let’s replace the sine wave by a square wave and shift horizontally:

xn+1 = xn + αyn (mod 1)

yn+1 = yn + sgn

(xn+1 −

1

2

)

We’re interested in the dynamics of this function f on the cylinder[0, 1)× R.

KAM theory does not apply here because of the lack ofsmoothness.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 11: Discontinuous standard map dynamics - ICERM

f can be interpreted geometrically in several ways.

f is also related to the Fermi-Ulam model, introduced in 1961 byUlam as a variant of Fermi’s model of cosmic ray acceleration viamagnetic mirrors.

Understanding the dynamics of discontinuous maps of this kindcould be of interest.

Which orbits are unbounded? Why do they appear to grow slowly?

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 12: Discontinuous standard map dynamics - ICERM

f can be interpreted geometrically in several ways.

f is also related to the Fermi-Ulam model, introduced in 1961 byUlam as a variant of Fermi’s model of cosmic ray acceleration viamagnetic mirrors.

Understanding the dynamics of discontinuous maps of this kindcould be of interest.

Which orbits are unbounded? Why do they appear to grow slowly?

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 13: Discontinuous standard map dynamics - ICERM

f can be interpreted geometrically in several ways.

f is also related to the Fermi-Ulam model, introduced in 1961 byUlam as a variant of Fermi’s model of cosmic ray acceleration viamagnetic mirrors.

Understanding the dynamics of discontinuous maps of this kindcould be of interest.

Which orbits are unbounded? Why do they appear to grow slowly?

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 14: Discontinuous standard map dynamics - ICERM

Unbounded orbits?

A simple case occurs for α = 1:

xn+1 = xn + yn (mod 1), yn+1 = yn + sgn

(xn+1 −

1

2

)

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 15: Discontinuous standard map dynamics - ICERM

Unbounded orbits? A simple case occurs for α = 1:

xn+1 = xn + yn (mod 1), yn+1 = yn + sgn

(xn+1 −

1

2

)

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 16: Discontinuous standard map dynamics - ICERM

Unbounded orbits? A simple case occurs for α = 1:

xn+1 = xn + yn (mod 1), yn+1 = yn + sgn

(xn+1 −

1

2

)

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 17: Discontinuous standard map dynamics - ICERM

We’ll restrict to α, y0 ∈ Q. Reasons: More tractable, and maybeit’ll give insight into the case αy0 /∈ Q.

For now, consider α = 1/q and y0 = a/b.

For convenience, expand the cylinder:

x ′ = x +y

q(mod 1) x ′ = x + y (mod q)

y ′ = y + sgn

(x ′ − 1

2

)y ′ = y + sgn

(x ′ − q

2

)

Can also define f on the torus – glue y = 0 to y = q.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 18: Discontinuous standard map dynamics - ICERM

We’ll restrict to α, y0 ∈ Q. Reasons: More tractable, and maybeit’ll give insight into the case αy0 /∈ Q.

For now, consider α = 1/q and y0 = a/b.

For convenience, expand the cylinder:

x ′ = x +y

q(mod 1) x ′ = x + y (mod q)

y ′ = y + sgn

(x ′ − 1

2

)y ′ = y + sgn

(x ′ − q

2

)

Can also define f on the torus – glue y = 0 to y = q.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 19: Discontinuous standard map dynamics - ICERM

We’ll restrict to α, y0 ∈ Q. Reasons: More tractable, and maybeit’ll give insight into the case αy0 /∈ Q.

For now, consider α = 1/q and y0 = a/b.

For convenience, expand the cylinder:

x ′ = x +y

q(mod 1) x ′ = x + y (mod q)

y ′ = y + sgn

(x ′ − 1

2

)y ′ = y + sgn

(x ′ − q

2

)

Can also define f on the torus – glue y = 0 to y = q.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 20: Discontinuous standard map dynamics - ICERM

Invariant intervals (α = 1/q and y0 ∈ Z)The action of f is the same throughout certain intervals.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 21: Discontinuous standard map dynamics - ICERM

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 22: Discontinuous standard map dynamics - ICERM

Rotational symmetry

q = 36, x0 = 18 + 3.5 = 21.5, y0 = 0

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 23: Discontinuous standard map dynamics - ICERM

Rotational symmetry

Red orbit: x0 = 18− 3.5 = 14.5

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 24: Discontinuous standard map dynamics - ICERM

Rotational symmetry

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 25: Discontinuous standard map dynamics - ICERM

Consider y0 ∈ Z and α = 1/q.

Proposition

Suppose q is even. For (x0, y0) ∈ L, the orbit under f is bounded.

Proposition

Suppose q is odd. Then there exists a unique escaping orbit on LRunder f , and this orbit escapes to +∞.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 26: Discontinuous standard map dynamics - ICERM

Consider y0 ∈ Z and α = 1/q.

Proposition

Suppose q is even. For (x0, y0) ∈ L, the orbit under f is bounded.

Proposition

Suppose q is odd. Then there exists a unique escaping orbit on LRunder f , and this orbit escapes to +∞.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 27: Discontinuous standard map dynamics - ICERM

Can we find unbounded orbits for α = 1/q and y0 ∈ Q\Z?

For q ≡ 2 (mod 4), experiments indicated that y0 = 1/2 alwaysworks.

In fact, for q ≡ 2 (mod 4), the orbit under f of the point(r0, y0) = (q − 3, q+1

2 ) is unbounded. (Here r = x − 3/4)

Consider points at level y = q+12 + m.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 28: Discontinuous standard map dynamics - ICERM

Can we find unbounded orbits for α = 1/q and y0 ∈ Q\Z?

For q ≡ 2 (mod 4), experiments indicated that y0 = 1/2 alwaysworks.

In fact, for q ≡ 2 (mod 4), the orbit under f of the point(r0, y0) = (q − 3, q+1

2 ) is unbounded. (Here r = x − 3/4)

Consider points at level y = q+12 + m.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 29: Discontinuous standard map dynamics - ICERM

Can we find unbounded orbits for α = 1/q and y0 ∈ Q\Z?

For q ≡ 2 (mod 4), experiments indicated that y0 = 1/2 alwaysworks.

In fact, for q ≡ 2 (mod 4), the orbit under f of the point(r0, y0) = (q − 3, q+1

2 ) is unbounded. (Here r = x − 3/4)

Consider points at level y = q+12 + m.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 30: Discontinuous standard map dynamics - ICERM

Can we find unbounded orbits for α = 1/q and y0 ∈ Q\Z?

For q ≡ 2 (mod 4), experiments indicated that y0 = 1/2 alwaysworks.

In fact, for q ≡ 2 (mod 4), the orbit under f of the point(r0, y0) = (q − 3, q+1

2 ) is unbounded. (Here r = x − 3/4)

Consider points at level y = q+12 + m.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 31: Discontinuous standard map dynamics - ICERM

30 iterates with q = 18

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 32: Discontinuous standard map dynamics - ICERM

Consider points at level y = q+12 + m.

For m even we can only have r ≡ 3 (mod 4), and for m odd onlyr ≡ 2 (mod 4).

Starting at (r0, y0) = (q − 3, q+12 ), there are immediately two

consecutive increases.

There is no point at level y = q+12 + 2 from which there are two

consecutive decreases.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 33: Discontinuous standard map dynamics - ICERM

Consider points at level y = q+12 + m.

For m even we can only have r ≡ 3 (mod 4), and for m odd onlyr ≡ 2 (mod 4).

Starting at (r0, y0) = (q − 3, q+12 ), there are immediately two

consecutive increases.

There is no point at level y = q+12 + 2 from which there are two

consecutive decreases.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 34: Discontinuous standard map dynamics - ICERM

Conjecture

For every α = 1/q, there exists y0 = a/b such that there is anescaping orbit starting at some (x0, y0) ∈ LR .

We’ve shown this holds for q odd and q ≡ 2 (mod 4).

q 24 28 32 36 40 44 48 52 56 60

a 36 67 63 77 19 23 360 243 23 254

b 103 144 205 227 337 223 1043 1264 505 1379

For q ≡ 0 (mod 4), this table gives y0 = a/b with the smallest b.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 35: Discontinuous standard map dynamics - ICERM

Conjecture

For every α = 1/q, there exists y0 = a/b such that there is anescaping orbit starting at some (x0, y0) ∈ LR .

We’ve shown this holds for q odd and q ≡ 2 (mod 4).

q 24 28 32 36 40 44 48 52 56 60

a 36 67 63 77 19 23 360 243 23 254

b 103 144 205 227 337 223 1043 1264 505 1379

For q ≡ 0 (mod 4), this table gives y0 = a/b with the smallest b.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 36: Discontinuous standard map dynamics - ICERM

Conjecture

For every α = 1/q, there exists y0 = a/b such that there is anescaping orbit starting at some (x0, y0) ∈ LR .

We’ve shown this holds for q odd and q ≡ 2 (mod 4).

q 24 28 32 36 40 44 48 52 56 60

a 36 67 63 77 19 23 360 243 23 254

b 103 144 205 227 337 223 1043 1264 505 1379

For q ≡ 0 (mod 4), this table gives y0 = a/b with the smallest b.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 37: Discontinuous standard map dynamics - ICERM

Islands at y = q/n for n odd (y0 ∈ Z again)

The escaping orbit for q = 601.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 38: Discontinuous standard map dynamics - ICERM

First return map:

cm+1 = cm + ndm −(n − 1

2

)2

− r

dm+1 = dm − sgn(cm+1)

for all m ≥ 0, where r = q (mod n).

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 39: Discontinuous standard map dynamics - ICERM

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 40: Discontinuous standard map dynamics - ICERM

Asymptotics of the escaping orbit

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 41: Discontinuous standard map dynamics - ICERM

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 42: Discontinuous standard map dynamics - ICERM

L(q) > Cq log q

for some constant C > 0 and sufficiently large q.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 43: Discontinuous standard map dynamics - ICERM

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics

Page 44: Discontinuous standard map dynamics - ICERM

Acknowledgements and References

Many thanks to Maxim, Vadim, and Stefan for their guidance

M. Arnold and V. Zharnitsky. Communications in MathematicalPhysics 338, 501-521 (2015).

S. M. Ulam. Proceedings of the Fourth Berkeley Symposium onMathematical Statistics and Probability, Volume 3: Contributionsto Astronomy, Meteorology, and Physics, 315–320, University ofCalifornia Press, Berkeley, Calif., 1961.http://projecteuclid.org/euclid.bsmsp/1200512818.

Tom Dauer, Meg Doucette, and Shan-Conrad Wolf Summer@ICERM 2015

Discontinuous standard map dynamics