In mathematics, a Clifford bundle is an algebra bundle whose fibers have the structure of a Clifford algebra and whose local trivializations respect the algebra structure. There is a natural Clifford bundle associated to any (pseudo) Riemannian manifold M which is called the Clifford bundle of M.
Let V be a (real or complex) vector space together with a symmetric bilinear form <·,·>. The Clifford algebra Cℓ(V) is a natural (unital associative) algebra generated by V subject only to the relation
v2=\langlev,v\rangle
Like other tensor operations, this construction can be carried out fiberwise on a smooth vector bundle. Let E be a smooth vector bundle over a smooth manifold M, and let g be a smooth symmetric bilinear form on E. The Clifford bundle of E is the fiber bundle whose fibers are the Clifford algebras generated by the fibers of E:
C\ell(E)=\coprodx\inC\ell(Ex,gx)
One is most often interested in the case where g is positive-definite or at least nondegenerate; that is, when (E, g) is a Riemannian or pseudo-Riemannian vector bundle. For concreteness, suppose that (E, g) is a Riemannian vector bundle. The Clifford bundle of E can be constructed as follows. Let CℓnR be the Clifford algebra generated by Rn with the Euclidean metric. The standard action of the orthogonal group O(n) on Rn induces a graded automorphism of CℓnR. The homomorphism
\rho:O(n)\toAut(C\ellnR)
\rho(A)(v1v2 … vk)=(Av1)(Av2) … (Avk)
C\ell(E)=F(E) x \rhoC\ellnR
C\ell(E)=C\ell0(E) ⊕ C\ell1(E).
If the vector bundle E is orientable then one can reduce the structure group of Cℓ(E) from O(n) to SO(n) in the natural manner.
If M is a Riemannian manifold with metric g, then the Clifford bundle of M is the Clifford bundle generated by the tangent bundle TM. One can also build a Clifford bundle out of the cotangent bundle T*M. The metric induces a natural isomorphism TM = T*M and therefore an isomorphism Cℓ(TM) = Cℓ(T*M).
There is a natural vector bundle isomorphism between the Clifford bundle of M and the exterior bundle of M:
C\ell(T*M)\congΛ(T*M).
The above isomorphism respects the grading in the sense that
\begin{align} C\ell0(T*M)&=Λeven(T*M)\\ C\ell1(T*M)&=Λodd(T*M). \end{align}
For a vector
v\inTxM
x\inM
\psi\inΛ(TxM)
v\psi=v\wedge\psi+v\lrcorner\psi
where the metric duality to change vector to the one form is used in the first term.
Then the exterior derivative
d
\delta
\nabla
\{ea\}
d=ea\wedge
\nabla | |
ea |
, \delta=-ea
\lrcorner\nabla | |
ea |
Using these definitions, the Dirac-Kähler operator[3] is defined by
D=ea
\nabla | |
ea |
=d-\delta
On a star domain the operator can be inverted using Poincaré lemma for exterior derivative and its Hodge star dual for coderivative.[4] Practical way of doing this is by homotopy and cohomotopy operators.[5]