Examples of applications of real-valued closed 1-forms in physics Closed 1-forms are well-studied in foliation topology, algebraic geometry, and theory of manifolds. What are examples of their most typical or most interesting applications in physics? 
I do not mean exact 1-forms (roughly speaking, functions -- not interesting). I am interested in examples of applications of real-valued closed 1-forms that that are not exact. 
My motivation is to mention several good examples in an introductory section of a mathematical paper on closed 1-forms to show their importance to physics, both classical and modern. So several good (typical, or interesting) examples suitable to be mentioned in such a section would do.
 A: Most notably, part of Maxwell's equations states that the Faraday 2-form is closed:
$$dF=0$$
From this we can infer from Poincare's lemma that there exists a 1-form $A$ such that $dA=F$. In some elementary treatments $F$ is considered to be an exact form. But when considering magnetic monopoles is it important to treat it as a closed form because of the "locally" clause in the Poincare lemma. 
A really trivial example is the following: let $g$ be an orthonormal metric. Then it is a closed 0-form
$$dg=0$$
This is merely the equation for the antisymmetry of the spin connection on a Riemannian manifold with orthonormal metric.
Cohomology is used quite extensively in a little sector of physics called String Theory. I'm sure you know how important closed forms are for that. A really important closed form is the Kahler form:
$$dJ=0$$
EDIT: Those weren't 1-forms. The curl operator is $\star d$. Thus a closed one-form is isomorphic to a vector that has zero curl! Some examples I can think of off the top of my head:
Take Faraday's law $\nabla\times\mathbf{E}+\dot{\mathbf{B}}=0$. Suppose the fields are static. Then $\dot{\mathbf{B}}=0$ and $\nabla\times\mathbf{E}=0$. If $\mathcal{E}=\mathbf{E}^\flat$
$$d\mathcal{E}=0$$
The same works for the Maxwell-Ampere law in a vacuum. Then the magnetic 1-form $\mathcal{B}=\mathbf{B}^\flat$ is closed
$$d\mathcal{B}=0$$
Suppose the integral of some force $\mathbf{F}$ is path-independent. Work is defined by
$$W_P=\int_P\mathbf{F}\cdot d\mathbf{x}$$
If $\mathcal{F}=\mathbf{F}^\flat$ then
$$W_P=\int_P\mathcal{F}$$
The difference of work along two different paths vanishes ($P'-P$ is a closed curve which is the boundary of a surface $S$)
$$W_{P'}-W_P=\int_{P'-P}\mathcal{F}=\int_S d\mathcal{F}=0$$
by Stokes' theorem. This implies for any conservative force
$$d\mathcal{F}=0$$
A: Many. Classical mechanics is essentially geometry. In the Hamiltonian formulation, the dynamics takes place on a cotangent bundle to a manifold, the configuration space $\Gamma$, known as the phase space $T^*\Gamma$. The tautological, or Poincaré 1-form $\theta$, leads through exterior derivative to the natural symplectic 2-form $\omega$ on the cotangent bundle $T^*\Gamma$, that is $\omega = \text d\theta$.
In Electrodynamics, the 4-potential $A$ can be viewed as a 1-form, and its exterior derivative $\text dA$ is the Faraday, or electromagnetic, tensor $F$, which describes both electric and magnetic fields and is linked to the 4-current 1-form $J$ through Maxwell's equations. For more on this subject see this answer.
For some other ideas in General Relativity see this other answer.
