In theoretical physics, the Dirac–Kähler equation, also known as the Ivanenko–Landau–Kähler equation, is the geometric analogue of the Dirac equation that can be defined on any pseudo-Riemannian manifold using the Laplace–de Rham operator. In four-dimensional flat spacetime, it is equivalent to four copies of the Dirac equation that transform into each other under Lorentz transformations, although this is no longer true in curved spacetime. The geometric structure gives the equation a natural discretization that is equivalent to the staggered fermion formalism in lattice field theory, making Dirac–Kähler fermions the formal continuum limit of staggered fermions. The equation was discovered by Dmitri Ivanenko and Lev Landau in 1928[1] and later rediscovered by Erich Kähler in 1962.[2]
In four dimensional Euclidean spacetime a generic fields of differential forms
\Phi=\sumH\PhiH(x)dxH,
is written as a linear combination of sixteen basis forms indexed by
H
\{\mu1,...,\muh\}
\mu1< … <\muh
\PhiH(x)=
\Phi | |
\mu1...\muh |
(x)
dxH
dxH=
\mu1 | |
dx |
\wedge … \wedge
\muh | |
dx |
.
\star
d
\delta=-\stard\star
d-\delta
(d-\delta)2=\square
This equation is closely related to the usual Dirac equation, a connection which emerges from the close relation between the exterior algebra of differential forms and the Clifford algebra of which Dirac spinors are irreducible representations. For the basis elements to satisfy the Clifford algebra
\{dx\mu,dx\nu\}=2\delta\mu\nu
\vee
dx\mu\veedx\nu=dx\mu\wedgedx\nu+\delta\mu\nu.
Using this product, the action of the Laplace–de Rham operator on differential form basis elements is written as
(d-\delta)\Phi(x)=dx\mu\vee\partial\mu\Phi(x).
To acquire the Dirac equation, a change of basis must be performed, where the new basis can be packaged into a matrix
Zab
Zab=\sumH(-1)h(h-1)/2
T | |
(\gamma | |
ab |
dxH.
The matrix
Z
dx\mu\veeZ=
T | |
\gamma | |
\mu |
Z
a
\Phi=\sumab\Psi(x)abZab,
transforms the Dirac–Kähler equation into four sets of the Dirac equation indexed by
b
(\gamma\mu\partial\mu+m)\Psi(x)b=0.
dx\mu\vee\partial\mu → dx\mu\veeD\mu
(d-\delta+m)\Phi=iA\vee\Phi.
As before, this is also equivalent to four copies of the Dirac equation. In the abelian case
A=eA\mudx\mu
\Phi
There is a natural way in which to discretize the Dirac–Kähler equation using the correspondence between exterior algebra and simplicial complexes. In four dimensional space a lattice can be considered as a simplicial complex, whose simplexes are constructed using a basis of
h
(h) | |
C | |
x,H |
x
H
C(h)=\sumx,H\alphax,H
(h) | |
C | |
x,H |
.
The h-chains admit a boundary operator
\Delta
(h) | |
C | |
x,H |
\nabla
(h) | |
C | |
x,H |
h
\Phi(h)(C(h))
\hat\Delta
\hat\nabla
(\hat\Delta\Phi)(C)=\Phi(\DeltaC), (\hat\nabla\Phi)(C)=\Phi(\nablaC).
Under the correspondence between the exterior algebra and simplicial complexes, differential forms are equivalent to cochains, while the exterior derivative and codifferential correspond to the dual boundary and dual coboundary, respectively. Therefore, the Dirac–Kähler equation is written on simplicial complexes as[6]
(\hat\Delta-\hat\nabla+m)\Phi(C)=0.
The resulting discretized Dirac–Kähler fermion
\Phi(C)
As described previously, the Dirac–Kähler equation in flat spacetime is equivalent to four copies of the Dirac equation, despite being a set of equations for antisymmetric tensor fields. The ability of integer spin tensor fields to describe half integer spinor fields is explained by the fact that Lorentz transformations do not commute with the internal Dirac–Kähler
SO(2,4)
2n | |
2 |
2n-1 | |
2 |
In curved spacetime, the Dirac–Kähler equation no longer decomposes into four Dirac equations. Rather it is a modified Dirac equation acquired if the Dirac operator remained the square root of the Laplace operator, a property not shared by the Dirac equation in curved spacetime.[8] This comes at the expense of Lorentz invariance, although these effects are suppressed by powers of the Planck mass. The equation also differs in that its zero modes on a compact manifold are always guaranteed to exist whenever some of the Betti numbers vanish, being given by the harmonic forms, unlike for the Dirac equation which never has zero modes on a manifold with positive curvature.