The first part of the post is a continuation of the previous post Arnold’s Mathematical Methods of Classical Mechanics: Exterior Differentiation. The second part is based upon my reading of Lecture 1 of Arnold’s PDE.

We left off with the computation of the principal linear part of the integral of the differential 1-form \omega = a(x_1, x_2)dx_1 along the boundary of the parallelogram, \partial \Pi, with edges \xi, \eta and vertex at 0 on the (x_1, x_2)-plane.

After some parameterization, we arrived at the step:

\int_{\partial \Pi} \omega = \int_0^1 [a(\xi t) - a(\xi t + \eta)]dx_1(\xi) - [a(\eta t) - a(\eta t + \xi)]dx_1(\eta)

Claim: a(\xi t + \eta) - a(\xi t) = \frac{\partial{a}}{\partial x_1} dx_1(\eta) + \frac{\partial{a}}{\partial x_2}dx_2(\eta) + O(\xi^2, \eta^2)

Why is this true? This is just the first-order Taylor expansion of a(x_1, x_2) at (0, 0).

Notice: the linear part \frac{\partial a}{\partial x_1} dx_1(\eta) + \frac{\partial a}{\partial x_2}dx_2(\eta) = \nabla(a) \cdot \eta. The \nabla(a) gives us the direction of greatest ascent for a(x_1, x_2) at each point (x_1, x_2). So, geometrically, this means that when our parallelogram is small enough, the increment of a(x_1, x_2) from \xi t to \xi t + \eta is given by the ‘amount of ascent’ in the \eta direction.

Algebraically, we have:

a(\xi t + \eta) - a(\xi t) = [a(\xi t) + \nabla(a) \cdot \eta + o(\xi^2, \eta^2)] - a(\xi t) = \nabla(a) \cdot \eta + o(\xi^2, \eta^2)

which is what we want.

Return to Arnold’s PDE

Recall the differential 1-form we were interested comes from the contact structure in J^1(\mathbb{R}^n, \mathbb{R}) \cong \mathbb{R}^{2n+1}:

\alpha = dy - p dx.

We now look at the 2-form \omega^2 = d\alpha that arises from the exterior differentiation of \alpha.

Example: in \mathbb{R}^3

The exterior differentiation would give us:

d \alpha = d1 \wedge dy + dz \wedge dx = 0 - dx \wedge dz = - dx \wedge dz

This 2-form gives the negative of the oriented area of the projection of a parallelogram in \mathbb{R}^3 onto the (x, z)-plane.

For general \mathbb{R}^{2n+1}:

Suppose the coordinates on \mathbb{R}^{2n+1} are given by x_1, ..., x_n, y, z_1, ..., z_n.

The exterior differentiation would give us:

d\alpha = \sum_{k=1}^n -dx_k \wedge dz_k.

This 2-form gives the sum of the oriented area of the projection of a parallelogram in \mathbb{R}^{2n+1} onto the (x_k, z_k)-planes.

Thinking about: Given two vectors \vec{u}, \vec{v} lying on a contact plane, what would d\alpha(\vec{u}, \vec{v} be?

Claim: The 2-form \omega^2 when restricted to the contact field is defined invariantly up to multiplication by a non-zero number at each point.

Proof: Let \tilde{\alpha} = f\alpha (i.e. f is a function of x, y, z.)

Then, d\tilde{\alpha} = d(f dy + \sum_{k=1}^n f z_k dx_k.

The RHS is equal to:

[df \wedge dy + f (d1) \wedge dy] + \sum_{k=1}^n (df \wedge z_k dx_k + f dz_k \wedge dx_k)

= df \wedge (dy + \sum_{k=1}^n z_k dx_k) + f \sum_{k=1}^n -dx_k \wedge dz_k

= df \wedge \alpha + f d \alpha.

Hence, when restricted to the field of contact planes, i.e. \alpha = 0, we have:

d\tilde{\alpha}|_{\alpha = 0} = df \wedge 0 + f d\alpha|_{\alpha = 0}

which is the same as

d\tilde{\alpha}|_{\alpha = 0} = f d \alpha|_{\alpha = 0}.

What does this mean geometrically?

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