Hodge theory
In mathematics, Hodge theory is the study of the consequences for the algebraic topology of a smooth manifold M of the partial differential equation theory of generalised Laplacian operators associated to a Riemannian metric on M. It was developed by W. V. D. Hodge in the 1930s as an extension of De Rham cohomology, and has major applications on three levels:
- Riemannian manifolds
- KÃÂähler manifolds
- algebraic geometry of complex projective varieties.
An abstract definition of Hodge structure is now given: for a real vector space W, a Hodge structure on W is a direct sum decomposition of
- Wp,q
- Wq,p.
- Hk(V'')
- Hp,q.
- Bk = dim Hk(V) = Σ hp,q'',
- hp,q = dim Hp,q.
This grading comes initially from the theory of harmonic forms, that are privileged representatives in a de Rham cohomology class picked out by the Hodge Laplacian (generalising harmonic functions, which must be locally constant on compact manifolds by their maximum principle). In later work (Dolbeaut) it was shown that the Hodge decomposition above can also be found by means of the sheaf cohomology groups
- Hp(V,Ωq)
- Ωq
In the case of singularities, the Hodge structure has to be modified to a mixed Hodge structure, where what survives is a filtration rather than a direct sum decomposition. This case is much used, for example in monodromy questions.
See also:
- Hodge conjecture
- Variation of Hodge structure
- Hodge cycle
- Yoga of weights (algebraic geometry)