Let $U$ be a simply connected bounded open subset of $\mathbb{R}^n$.
Let $\Omega^k$ be the space of $k$-forms on $U$, and let $d_k: \Omega^k \to \Omega^{k+1}$ be the exterior derivative. Endow $U$ with a Riemannian metric and let $\delta_k: \Omega^k \to \Omega^{k-1}$ be the corresponding co-differential operator.
A 1-form $\omega \in \Omega^1$ is
- closed if $d_1{\omega} = 0 \in \Omega^2$, i.e. $\omega \in \ker{d_1}$
- exact if $\omega = d_0f$ for some $f \in \Omega^0$, i.e. $\omega \in \text{im}~{d_0}$
- co-closed if $\delta_1{\omega} = 0 \in \Omega^0$, i.e. $\omega \in \ker{\delta_1}$
- co-exact if $\omega = \delta_2{\beta}$ for some $\beta \in \Omega^2$, i.e. $\omega \in \text{im}~{\delta_2}$
Since $U$ is simply connected, by Poincaré lemma any 1-form is
- closed iff exact, and
- co-closed iff co-exact
Question: is it true that $\Omega^1$ admits the orthogonal direct sum decomposition $$\Omega^1 = \text{im}~{d_0} \oplus \text{im}~{\delta_2}$$
I think the answer is "no". If $\Omega^1$ was a finite dimensional vector space, then
$$ \begin{split} \Omega^{1} & = \ker{d_{1}} \oplus \left( \ker{d_{1}} \right)^{\perp} \\ & = \ker{d_{1}} \oplus \text{im}~{\delta_{2}} \\ & = \text{im}~{d_{0}} \oplus \text{im}~{\delta_{2}} \\ \end{split} $$ where
- the first equality is true by definition of direct sum and orthogonal complement, since $\ker{d_1}$ is a linear subspace;
- the second equality is true since $\delta_2$ is the adjoint of $d_1$;
- the last equality holds by Poincarè lemma.
But, $\Omega^1$ is a module over the algebra of smooth functions $C^{\infty}(U)$, so the above does not make sense - right?
Edit
Here is the proof that Hodge theorem holds true for a special Riemannian metric on the relative interior of the standard simplex.
$\newcommand{\rint}[1]{\mathring{#1}}$ $\newcommand{\X}{\mathcal{X}}$ $\newcommand{\R}{\mathbb{R}}$ $\newcommand{\d}{d}$ $\newcommand{\pull}[1]{#1^{*}}$ $\newcommand{\topspace}{\R^{n+1}_{>0}}$
Prop. There exists a Riemannian metric such that Hodge theorem holds true for the space of 1-forms on the relative interior of the standard simplex that are well-behaved on the boundary.
Proof.
Consider the relative interior of the standard $n$-dimensional simplex seen as an immersed submanifold of the positive orthant $\topspace$:
$$\rint{\X} = \{x \in \topspace: \sum_{i = 0}^n x_i = 1\} \hookrightarrow \topspace$$
Consider the standard Euclidean coordinates and endow $\topspace$ with the following Riemannian metric (known in the literature as Shahshahani metric [1, 2]): $$g(x) = \sum_{i, j = 0}^n \frac{\delta_{ij}}{x_i} \, dx^i \otimes dx^j$$ The matrix representation of this metric is $g(x) = \text{diag}(x_0, \dots, x_n)$.
Considering the following diffeomorphism of $\topspace$ onto itself: $$F: \topspace \to \topspace$$ $$F(x) = 2\sqrt{x}$$ $$F^{-1}(y) = \frac{y^2}{4}$$ This is known as Akin transformation [3].
The image of $\rint{\X}$ under $F$ is the portion of the sphere of radius $2$ lying in the positive orthant: $$\rint{C} := F(\rint{\X}) = \{y \in \topspace: \sum_{i = 0}^n y_i^2 = 4 \}$$ Furthermore it's easy to check that the pull-back of the metric $g$ along $F^{-1}$ is the Euclidean metric on $\topspace$. Hence, $F$ restricted to $\rint{\X}$ is an isometry $F|_{\rint{\X}}: \rint{\X} \to \rint{C}$ between $\rint{\X}$ that inherits the Shahshahani metric from the ambient space, and $\rint{C}$ that inherits the Euclidean metric from the ambient space.
Let now $V$ be a 1-form defined on a tubolar neighborhood $U$ of $\rint{\X}$ (in particular, well-behaved on the boundary of $\rint{\X}$), and let $v$ be the restriction of $V$ to $\rint{X}$. In Euclidean coordinates $V$ can be expressed as $$V(x) = \sum_{i = 0}^n V_i(x) \, dx^i$$ where $V_i$ are smooth functions on $U$. Let $\omega = (F^{-1})^*{V}$ be the pull-back of $v$ on $F(U)$. By an explicit computation $$\omega(y) = \sum_{i = 0}^n y_i \, (V_i \circ F^{-1})(y) \, dy^i$$ Since both $F$ and the $V_i$-s are well-behaved on the boundary of $\rint{\X}$, the 1-form $\omega$ is well-behaved on the closure $C$ of $\rint{C}$.
Then, by the Extension Lemma for Smooth Functions [4, Lemma 2.26], there exists a 1-form $\tilde{\omega}$ defined on the whole sphere $S$ of radius $2$ that agrees with $\omega|_C$ on $C$ and that is zero outside an arbitrarily small neighborhood of $C$.
The sphere is a closed (compact, no boundary) oriented manifold that inherits the Euclidean metric from the ambient space; thus Hodge theorem applies to the $1$-form $\tilde{\omega}$:
$$\tilde{\omega} = d{f} + \delta{\beta} + \gamma$$ with $f$ smooth function on $S$, $\beta$ 2-form on $S$, and $\gamma$ harmonic 1-form on $S$. Notice that if $n \geq 2$ then $S$ is simply connected and the harmonic component vanishes identically.
The restriction to $\rint{C}$ gives
$$ \begin{split} \tilde{\omega}|_{\rint{C}} = \omega|_{\rint{C}} & = \left( d\psi + \delta\beta + \gamma \right)|_{\rint{C}} \\ & = d{\left( \psi|_{\rint{C}} \right)} + \delta{\left( \beta|_{\rint{C}} \right)} + \gamma|_{\rint{C}} \end{split} $$ Pulling $\omega|_{\rint{C}}$ back to $\rint{\X}$ gives
$$ v = \pull{F}{\omega|_{\rint{C}}} = \pull{F} \Big( \d{\left( \psi|_{\rint{C}} \right)} + \delta{\left( \beta|_{\rint{C}} \right)} + \gamma|_{\rint{C}} \Big) $$
The exterior derivative always commutes with the pull-back, and the codifferential commutes with the pull-back via isometries, so
$$ v = \d\Big( \pull{F}(\psi|_{\rint{C}}) \Big) + \delta\Big( \pull{F}(\beta|_{\rint{C}}) \Big) + \pull{F} \left( \gamma|_{\rint{C}} \right) $$ where
- $\pull{F}(\psi|_{\rint{C}})$ is a smooth function on $\rint{\X}$
- $\pull{F}(\beta|_{\rint{C}})$ is a 2-form on $\rint{\X}$
- $\pull{F} \left( \gamma|_{\rint{C}} \right)$ is a harmonic 1-form on $\rint{\X}$
q.e.d.
- Shahshahani, S. A new mathematical framework for the study of linkage and selection. (American Mathematical Soc., 1979).
- Mertikopoulos, P. & Sandholm, W. H. Riemannian game dynamics. Journal of Economic Theory 177, 315–364 (2018).
- Sandholm, W. H. Population games and evolutionary dynamics. (MIT press, 2010).
- Lee, J. M. Introduction to Smooth Manifolds. (Springer-Verlag New York, 2012).
The decomposition you're looking for is referred to as the Hodge decomposition, and for forms over a compact oriented Riemannian manifold one has $\Omega^k(M)=\mathrm{im} d_{k-1}\oplus \mathrm{im} \delta_{k+1}\oplus \mathcal{H}^k$ where $\mathcal{H}^k$ is the space of harmonic $k$-forms.
In the non-compact case things are somewhat more subtle, since even though $d_k$ and $\delta_{k+1}$ are formally adjoint, they need not truely be adjoint in a more meaningful (functional analytic) sense.
Consider $U=(-1,1)\times (-1,1)\subset \mathbb{R}^2$. There is a diffeomorphism $\phi:U\to \mathbb{R}^2$ by $(x,y)\mapsto (\tan(\pi x/2, \tan(\pi y/2))$. Pulling back the standard Riemannian metric on $\mathbb{R}^2$ makes $\phi:U\to \mathbb{R}^2$ an orientation preserving isometry. The codifferential on $\Omega^2(\mathbb{R}^2)$ is $\delta=\star^{-1}d\star$, so if $\omega=fdx\wedge dy$ then $\delta\omega=\star^{-1}(\partial_x fdx+\partial_y f d_y)=\partial_xf dy-\partial_yfdx$. We have $d\delta\omega=(\partial_x^2f+\partial_y^2f)dx\wedge dy$, so if $f$ is chosen to be non-constant harmonic (i.e. the real part of an entire holomorphic function), $d\delta\omega=0$ and by the Poincare lemma, $\delta\omega=dg$ for some nonconstant $g\in C^\infty(\mathbb{R}^2)$. This of course means that $\mathrm{im\delta}\cap \mathrm{im d}\neq 0$ on $\mathbb{R}^2$. Since $U$ is isometric to $\mathbb{R}^2$, one sees that $\delta\phi^*\omega=d\phi^*g$, so the statement need not be true for sets which are bounded in $\mathbb{R}^n$.
As I have suggested, things are somewhat nicer in the compact case. Given $M$ a compact oriented Riemannian manifold without boundary, for $\omega\in \Omega^k(M)$ and $\alpha\in \Omega^{k+2}$ we have \begin{align}(d\omega,\delta\alpha)&=\int_Md\omega\wedge d\star\alpha\\ &=\int_M d(\omega\wedge d\star\alpha)-(-1)^{n-k-1}\omega\wedge dd\star \alpha\\ &=\int_M d(\omega\wedge d\star\alpha)\\ &=0\end{align} The final equality coming from Stokes' theorem. This means that $\mathrm{im}d_{k-1}$ is perpendicular to $\mathrm{im}\delta_{k+1}$ with respect to the inner product structure on $\Omega^k(M)$ induced by the metric. If the manifold has $H^1(M,\mathbb{R})=0$, the Hodge decomposition and DeRham's theorem tell us that $\Omega^1(M)=\mathrm{im} d_{k-1}\oplus \mathrm{im}\delta_{k+1}$.
EDIT: One has $\star^2\sigma=(-1)^{n(n-k)}\sigma$ so $\star^{-1}=\pm\star$, when restricted to $\Omega^k$ for fixed $k$, consistent with the convention.