An Introduction to Symplectic Geometry and Some Applications

Clayton Shonkwiler

Colorado State University

shonkwiler.org

/rtg20

this talk!

Take-Home Message

Symplectic geometry can sound scary, but it turns out to be useful in some surprising contexts.

Symplecti-wha?

—Dusa McDuff & Dietmar Salamon

Introduction to Symplectic Topology

—Ana Cannas da Silva

Lectures on Symplectic Geometry

(\textcolor{12a4b6}{M},\textcolor{d9782d}{\omega})

A nice space, where multivariable calculus makes sense. Think spheres, tori, projective spaces, …

A rule for assigning a number to pairs of tangent vectors which transforms like (signed) area of the parallelogram they span.

\omega(v_1,v_2) = 1
\omega(v_1,v_2) = -1
v_1
v_1
v_2
v_2

Symplectic Manifold

Must be closed (think: divergence-free) and non-degenerate (doesn’t annihilate any vector).

Standard Example and Some Non-Examples

Example: \((\mathbb{R}^2,dx \wedge dy) = (\mathbb{C},\frac{i}{2}dz \wedge d\bar{z})\)

dx \wedge dy \left( \textcolor{12a4b6}{a \frac{\partial}{\partial x} + b \frac{\partial}{\partial y}}, \textcolor{d9782d}{c \frac{\partial }{\partial x} + d \frac{\partial}{\partial y}} \right) = ad - bc
(a,b) = a \vec{e}_1 + b \vec{e}_2 = a \frac{\partial}{\partial x} + b \frac{\partial}{\partial y}
(c,d) = c \vec{e}_1 + d \vec{e}_2 = c \frac{\partial}{\partial x} + d \frac{\partial}{\partial y}

Non-Example: \((\mathbb{R}^3, dx \wedge dy)\)

For any vector \(v\), \(dx \wedge dy\left(\frac{\partial}{\partial z}, v\right) = 0\), so \(dx \wedge dy\) is degenerate.

Non-Example: \((\mathbb{R}^4, dx_1 \wedge dy_1 + y_1 dx_2 \wedge dy_2)\)

Because of the coefficient \(y_1\), this is not closed (“not divergence-free”).

Examples

\((S^2,d\theta\wedge dz)\)

\((\mathbb{R}^2,dx \wedge dy) = (\mathbb{C},\frac{i}{2}dz \wedge d\bar{z})\)

\((S^2,\omega)\), where \(\omega_p(u,v) = (u \times v) \cdot p\)

\((\mathbb{R}^2,\omega)\) where \(\omega(u,v) = \langle i u, v \rangle \)

\((\mathbb{C}^n, \frac{i}{2} \sum dz_k \wedge d\overline{z}_k)\)

\((\mathbb{C}^{m \times n}, \omega)\) with \(\omega(X_1,X_2) = -\operatorname{Im} \operatorname{trace}(X_1^* X_2)\).

\((T^* \mathbb{R}^n,\sum dq_i \wedge dp_i)\)

phase space

position

momentum

What does this get you?

Volume

\(\omega^{\wedge n} = \omega \wedge \dots \wedge \omega\) is a volume form on \(M\), and induces a measure

m(U) := \int_U \omega^{\wedge n}

called Liouville measure on \(M\).

In particular, if \(M\) is compact, this can be normalized to give a probability measure.

Theorem [Archimedes]

\(\mathrm{d}\theta \wedge \mathrm{d}z\) is the standard area form on the unit sphere \(S^2\).

\int_{S^2} \mathrm{d}\theta \wedge \mathrm{d}z = \int_{-1}^1 \int_0^{2\pi} \mathrm{d}\theta\, \mathrm{d}z = 4\pi

A (Very) Classical Example

KoenB [   ] from Wikimedia Commons

Hamiltonian Mechanics

“Evolution of a physical system follows the symplectic gradient”

Functions and Symplectic Gradients

If \(H: M \to \mathbb{R}\) is smooth, then there exists a unique vector field \(X_H\) so that \({dH = \iota_{X_H}\omega}\), i.e.,

dH(\cdot) = \omega(X_H, \cdot)

(\(X_H\) is called the Hamiltonian vector field for \(H\), or sometimes the symplectic gradient of \(H\))

Example. \(H: (S^2, d\theta\wedge dz) \to \mathbb{R}\) given by \(H(\theta,z) = z\).

\(dH = dz = \iota_{\frac{\partial}{\partial \theta}}(d\theta\wedge dz)\), so \(X_H = \frac{\partial}{\partial \theta}\).

\(H\) is constant on orbits of \(X_H\):

\(\mathcal{L}_{X_H}(H) = dH(X_H)=\omega(X_H,X_H) = 0\)

Some Mechanics

Suppose we have a particle of mass \(m\) with position \(\vec{q} = (q_1,q_2,q_3)\).

Suppose the particle is subject to a potential \(V(\vec{q})\).

Newton’s Second Law: \(-\nabla V(\vec{q}) = m \frac{d^2 \vec{q}}{dt^2}\).

Momenta \(p_i := m \frac{dq_i}{dt}\).

\((\vec{q},\vec{p})\in T^*\mathbb{R}^3 \cong \mathbb{R}^6\); canonical symplectic form \(\omega = dq_1 \wedge dp_1 + dq_2 \wedge dp_2 + dq_3 \wedge dp_3\).

The Hamiltonian Formulation

Energy function (or Hamiltonian)

\(H(\vec{q},\vec{p}) := \frac{1}{2m}|\vec{p}|^2 + V(\vec{q})\).

\(dH = \sum\left(\frac{\partial H}{\partial p_i} dp_i + \frac{\partial H}{\partial q_i}dq_i\right)\),

\((\vec{q}(t),\vec{p}(t))\) is an integral curve for \(X_H\) if and only if

\(\frac{dq_i}{dt} = \frac{\partial H}{\partial p_i} = \frac{1}{m} p_i\)

\(\frac{dp_i}{dt} = -\frac{\partial H}{\partial q_i} = -\frac{\partial V}{\partial q_i}.\)

This is Newton’s Second Law written as a first-order system!

\(X_H = \sum\left(\frac{\partial H}{\partial p_i} \frac{\partial}{\partial q_i} - \frac{\partial H}{\partial q_i} \frac{\partial}{\partial p_i}\right)\).

Noether’s Theorem

“Every continuous symmetry has a corresponding conserved quantity”

Circle Actions

A circle action on \((M,\omega)\) determines a vector field \(X\) by

X(p) = \left.\frac{d}{dt}\right|_{t=0}e^{i t} \cdot p

\(S^1=U(1)\) acts on \((S^2,d\theta \wedge dz)\) by

e^{it} \cdot(\theta, z) = (\theta + t, z).

So \(X = \frac{\partial}{\partial \theta}\).

Symmetries and Conserved Quantities

Definition. A circle action on \((M,\omega)\) is Hamiltonian if there exists a map

\mu: M \to \mathbb{R}

so that \(d\mu = \iota_{X}\omega = \omega(X,\cdot)\), where \(X\) is the vector field generated by the circle action. In other words, \(X = X_\mu\).

\(X = \frac{\partial}{\partial \theta}\)

\(\mu(\theta,z) = z\)

\(\iota_X\omega = \iota_{\frac{\partial}{\partial \theta}} d\theta \wedge dz = dz \)

Extremely Deep Fact

Archimedes’ Theorem can be suitably generalized to any symplectic manifold with a Hamiltonian circle action (or, better yet, many commuting Hamiltonian circle actions).

 

 

See: Atiyah, Guillemin–Sternberg, Duistermaat–Heckman, and toric symplectic manifolds (and toric varieties)

Application to Polymers

In solution, linear polymers become crumpled:

Protonated P2VP

Roiter–Minko, J. Am. Chem. Soc. 127 (2005), 15688-15689

[CC BY-SA 3.0], from Wikimedia Commons

Modern polymer physics is based on the analogy between a polymer chain and a random walk.

Ring Polymers

Lots of Symmetries!

Continuous symmetry \(\Rightarrow\) conserved quantity

The space of equilateral \(n\)-gons has lots of symmetries...

A Generalized Archimedes Theorem

Theorem [with Cantarella]

The standard volume form on polygon space is 

\(\mathrm{d}\theta_1 \wedge \dots \wedge \mathrm{d}\theta_{n-3} \wedge \mathrm{d} r_1 \wedge \dots \wedge \mathrm{d}r_{n-3}\)

Corollary [with Cantarella, Duplantier, Uehara]

The first efficient, provably correct algorithm for sampling equilateral random polygons in \(\mathbb{R}^3\).

Application to Frame Theory

Signal: \(v \in \mathbb{C}^d\)

Design: \(f_1, \dots , f_n \in \mathbb{C}^d\)

Measurements: \(\langle f_1, v \rangle, \dots , \langle f_n, v \rangle \).

Parseval’s Theorem

If \(f_1, \dots , f_d \in \mathbb{C}^d\) is an orthonormal basis,

\(\|v\|^2 = \sum |\langle f_i, v \rangle |^2 = \|F^* v\|^2\)

for any \(v \in \mathbb{C}^d\).

Even better,

\(v = \sum \langle f_i, v \rangle f_i = FF^* v \).

If \(F = [f_1 \, f_2 \dots f_n]\), the measurement vector is \(F^*v\).

\(\Leftrightarrow FF^* = \mathrm{Id}_{d \times d}\)

Parseval frame

Fact: For any \(n \geq d\), there exist Parseval frames \(f_1, \dots , f_n \in \mathbb{C}^d\) so that \(\|f_i\|=\|f_j\|\) for all \( i,j\); these are the equal-norm Parseval frames (ENPs).

This is fragile! What if a measurement gets lost?

Group Actions on Frames

Some nice group actions on \(\mathbb{C}^{d \times n}\):

  1. \(U(d)\) acts on the left
  2. \(U(n)\) acts on the right
  3. \(U(1)^d\) acts on the left
  4. \(U(1)^n\) acts on the right
\mu_{U(d)}(F) = FF^*
\mu_{U(n)}(F) = -F^*F
\mu_{U(1)^d}\left(\begin{bmatrix} \rule[.8mm]{4mm}{.5px}\, f^1 \rule[.8mm]{4mm}{.5px}\\ \vdots \\ \rule[.8mm]{4mm}{.5px}\, f^d \rule[.8mm]{4mm}{.5px} \end{bmatrix}\right) = \left(\frac{1}{2}\|f^1\|^2 , \dots , \frac{1}{2}\|f^d\|^2\right)
\mu_{U(1)^n} \left(\begin{bmatrix} f_1 | \cdots | f_n \end{bmatrix}\right) = \left(-\frac{1}{2}\|f_1\|^2 , \dots , -\frac{1}{2}\|f_n\|^2\right)

Parseval frames

\(\mu_{U(d)}^{-1}(I_{d\times d})\)

equal-norm frames

\(\mu_{U(1)^N}^{-1}\left(-\frac{1}{2}r,\dots , -\frac{1}{2}r\right)\)

ENPs: \(\mu_{U(d)}^{-1}(I_{d \times d}) \cap \mu_{U(1)^n}^{-1}\left(-\frac{d}{2n}, \dots , -\frac{d}{2n}\right)\)

A Generalization of the Frame Homotopy Conjecture

Theorem [with Needham]

There is a continuous interpolation between any two frames \(f_1, \dots , f_n\) and \(g_1, \dots , g_n\) with \(FF^* = GG^*\) and \(\|f_i\| = \|g_i\|\) preserving these conditions.

Thank you!

Funding: Simons Foundation

References

The geometry of constrained random walks and an application to frame theory

Clayton Shonkwiler

2018 IEEE Statistical Signal Processing Workshop (SSP), 343–347

The symplectic geometry of closed equilateral random walks in 3-space

Jason Cantarella and Clayton Shonkwiler

Annals of Applied Probability 26 (2016), no. 1, 549–596

A fast direct sampling algorithm for equilateral closed polygons

Jason Cantarella, Bernard Duplantier, Clayton Shonkwiler, and Erica Uehara

Journal of Physics A: Mathematical and Theoretical 49 (2016), no. 27, 275202

An Introduction to Symplectic Geometry and Some Applications

By Clayton Shonkwiler

An Introduction to Symplectic Geometry and Some Applications

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