Let (M,g)(M,g) be an oriented nn-dimensional . The metric and determine an on kk-forms and a volume form vol⁡g\operatorname{vol}_g. The Hodge star operator is the unique linear isomorphism

∗:Ωk(M)⟶Ωn−k(M)*:\Omega^k(M)\longrightarrow\Omega^{n-k}(M)

such that, for all real kk-forms α,β\alpha,\beta,

α∧∗β=⟨α,β⟩g vol⁡g.\alpha\wedge *\beta=\langle\alpha,\beta\rangle_g\,\operatorname{vol}_g.

It is defined pointwise and varies smoothly with gg. Thus the star combines the , the metric, and orientation into an operator complementary in degree.

Characterizing identities

On real kk-forms in the Riemannian convention,

∗(∗α)=(−1)k(n−k)α.*(*\alpha)=(-1)^{k(n-k)}\alpha.

The star is a pointwise isometry, and ∗1=vol⁡g*1=\operatorname{vol}_g, while ∗vol⁡g=1*\operatorname{vol}_g=1. These identities follow directly in an oriented orthonormal coframe and characterize the signs used here.

The star also converts the into its , up to a degree- and dimension-dependent sign. This is the basic mechanism behind the and harmonic-form theory.

Computation in an orthonormal coframe

If e1,…,ene^1,\ldots,e^n is a positively oriented orthonormal coframe and I=(i1<⋯<ik)I=(i_1<\cdots<i_k), then ∗eI*e^I is the uniquely signed complementary wedge eIce^{I^c} for which

eI∧∗eI=e1∧⋯∧en.e^I\wedge *e^I=e^1\wedge\cdots\wedge e^n.

For the standard orientation of R3\mathbb R^3, for example, ∗dx=dy∧dz*dx=dy\wedge dz, ∗dy=dz∧dx*dy=dz\wedge dx, and ∗dz=dx∧dy*dz=dx\wedge dy.

Conventions and scope
References
  1. Shigeyuki Morita, Geometry of Differential Forms, Translations of Mathematical Monographs 201, American Mathematical Society, 2001. Publisher record. Relevant: “Laplacian and harmonic forms.”
  2. Raymond O. Wells Jr., Differential Analysis on Complex Manifolds, 3rd ed., Graduate Texts in Mathematics 65, Springer, 2008. Publisher record. Relevant: Chapter III, “Differential Geometry,” Hermitian exterior algebra and the Hodge star.