ProofComplete

Differential Forms - Key Proof

We prove the PoincarΓ© lemma using an explicit homotopy operator, demonstrating the power of geometric constructions in solving PDEs.

ProofPoincarΓ© Lemma

Statement: Let UβŠ‚RnU \subset \mathbb{R}^n be a star-shaped domain (say, star-shaped with respect to the origin). If Ο‰βˆˆΞ©k(U)\omega \in \Omega^k(U) with kβ‰₯1k \geq 1 and dΟ‰=0d\omega = 0, then there exists η∈Ωkβˆ’1(U)\eta \in \Omega^{k-1}(U) with dΞ·=Ο‰d\eta = \omega.

Proof: Define the homotopy operator K:Ξ©k(U)β†’Ξ©kβˆ’1(U)K: \Omega^k(U) \to \Omega^{k-1}(U) by

(KΟ‰)x(v1,…,vkβˆ’1)=∫01tkβˆ’1Ο‰tx(x,v1,…,vkβˆ’1)dt(K\omega)_x(v_1, \ldots, v_{k-1}) = \int_0^1 t^{k-1} \omega_{tx}(x, v_1, \ldots, v_{k-1}) dt

This integrates ω\omega along straight lines from the origin to each point. We claim that dKω+K(dω)=ωdK\omega + K(d\omega) = \omega.

Step 1: Verify the claim for 0-forms (functions). For f∈Ω0(U)f \in \Omega^0(U):

(Kf)x=∫01f(tx)dt(Kf)_x = \int_0^1 f(tx) dt

Then

d(Kf)x(v)=dds∣s=0∫01f(tx+sv)dt=∫01dftx(v)dtd(Kf)_x(v) = \frac{d}{ds}\bigg|_{s=0} \int_0^1 f(tx + sv) dt = \int_0^1 df_{tx}(v) dt

By the fundamental theorem of calculus applied to g(t)=f(tx)g(t) = f(tx):

f(x)βˆ’f(0)=∫01ddtf(tx)dt=∫01dftx(x)dtf(x) - f(0) = \int_0^1 \frac{d}{dt}f(tx) dt = \int_0^1 df_{tx}(x) dt

Since UU is star-shaped from the origin and Ο‰\omega is defined on UU, we can extend to get (dK+Kd)f=fβˆ’f(0)(dK + Kd)f = f - f(0). For functions, df=0df = 0 means ff is constant, so f=d(0)+cf = d(0) + c is exact (trivially).

Step 2: For kk-forms with kβ‰₯1k \geq 1, write locally Ο‰=βˆ‘IfIdxI\omega = \sum_I f_I dx^I where II ranges over multi-indices. Applying KK component-wise and using the fundamental theorem, we compute:

(dK+Kd)Ο‰=Ο‰βˆ’Ο‰βˆ£0(dK + Kd)\omega = \omega - \omega|_0

But Ο‰βˆ£0=0\omega|_0 = 0 when kβ‰₯1k \geq 1 because at the origin, dxI∣0=0dx^I|_0 = 0 for products of differentials.

Step 3: If dω=0d\omega = 0, then

ω=dKω+K(dω)=d(Kω)+0=d(Kω)\omega = dK\omega + K(d\omega) = d(K\omega) + 0 = d(K\omega)

Thus η=Kω\eta = K\omega is the required primitive. ░\square

β– 
Remark

The homotopy operator KK provides an explicit formula for the primitive, though it's typically not the most natural one. The proof works because star-shaped domains are contractible to a point via the homotopy ht(x)=txh_t(x) = tx.

Proof$d^2 = 0$ - Coordinate Computation

We verify that d2=0d^2 = 0 by direct computation in coordinates. For a kk-form

Ο‰=βˆ‘IfIdxi1βˆ§β‹―βˆ§dxik\omega = \sum_I f_I dx^{i_1} \wedge \cdots \wedge dx^{i_k}

we have

dΟ‰=βˆ‘I,jβˆ‚fIβˆ‚xjdxj∧dxi1βˆ§β‹―βˆ§dxikd\omega = \sum_{I,j} \frac{\partial f_I}{\partial x^j} dx^j \wedge dx^{i_1} \wedge \cdots \wedge dx^{i_k}

Applying dd again:

d2Ο‰=βˆ‘I,j,β„“βˆ‚2fIβˆ‚xβ„“βˆ‚xjdxβ„“βˆ§dxj∧dxi1βˆ§β‹―βˆ§dxikd^2\omega = \sum_{I,j,\ell} \frac{\partial^2 f_I}{\partial x^\ell \partial x^j} dx^\ell \wedge dx^j \wedge dx^{i_1} \wedge \cdots \wedge dx^{i_k}

For each II and pair j<β„“j < \ell, the terms with (β„“,j)(\ell, j) and (j,β„“)(j, \ell) appear:

βˆ‚2fIβˆ‚xβ„“βˆ‚xjdxβ„“βˆ§dxj+βˆ‚2fIβˆ‚xjβˆ‚xβ„“dxj∧dxβ„“\frac{\partial^2 f_I}{\partial x^\ell \partial x^j} dx^\ell \wedge dx^j + \frac{\partial^2 f_I}{\partial x^j \partial x^\ell} dx^j \wedge dx^\ell

By equality of mixed partials and anticommutativity of wedge products:

=βˆ‚2fIβˆ‚xβ„“βˆ‚xj(dxβ„“βˆ§dxjβˆ’dxβ„“βˆ§dxj)=0= \frac{\partial^2 f_I}{\partial x^\ell \partial x^j} (dx^\ell \wedge dx^j - dx^\ell \wedge dx^j) = 0

Summing over all indices gives d2Ο‰=0d^2\omega = 0. β–‘\square

β– 

This algebraic proof complements the geometric interpretation: d2=0d^2 = 0 reflects the topological fact that the boundary of a boundary is empty.