Dirac equations
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This article describes several equations named after Paul Dirac.
Contents |
The Maxwell-Dirac equation
[More info on this equation would be greatly appreciated. - Ed.]
This equation essentially reads

where y is a spinor field (solving a coupled massive Dirac equation), and D is the Dirac operator with connection A. We put y in
and A in
.
- Scaling is (s1,s2) = (n / 2 − 3 / 2,n / 2 − 1).
- When n = 1, there is GWP for small smooth data Chd1973
- When n = 3 there is LWP for (s1,s2) = (1,1) in the Coulomb gauge Bou1999, and for (s1,s2) = (1 / 2 + ,1 + ) in the Lorentz gauge Bou1996
- For (s1,s2) = (1,2) in the Coulomb gauge this is in Bou1996
- This has recently been improved by Selberg to (1 / 4 + ,1). Note that for technical reasons, lower-regularity results do not automatically imply higher ones when the regularity of one field (e.g. A) is kept fixed.
- LWP for smooth data was obtained in Grs1966
- GWP for small smooth data was obtained in Ge1991
- When n = 4, GWP for small smooth data is known (Psarelli?)
In the nonrelativistic limit this equation converges to a Maxwell-Poisson system for data in the energy space BecMauSb-p2; furthermore one has a local well-posedness result which grows logarithmically in the asymptotic parameter. Earlier work appears in MasNa2003.
Dirac-Klein-Gordon equation
[More info on this equation would be greatly appreciated. - Ed.]
This equation essentially reads

where ψ is a spinor field (solving a coupled massive Dirac equation), D is the Dirac operator and φ is a scalar (real) field. We put ψ in
and (φ,φt) in
.
The energy class is essentially (s1,s2) = (1 / 2,1), but the energy density is not positive. However, the L2 norm of y is also positive and conserved..
- Scaling is (s1,s2) = (d / 2 − 3 / 2,d / 2 − 1).
- When n = 1 there is GWP for (s1,s2) = (1,1) Chd1973, Bou2000 and LWP for (s1,s2) = (0,1 / 2) Bou2000.
- When n = 2 there are some LWP results in Bou2001
Nonlinear Dirac equation
This equation essentially reads
where ψ is a spinor field, m > 0 is the mass, λ is a complex parameter, γ is the zeroth Pauli matrix, and (,) is the spinor inner product.
- Scaling is sc = 1 (at least in the massless case m = 0).
- In R3, LWP is known for Hs when s > 1 EscVe1997
- This can be improved to LWP in H1 (and GWP for small H1 data) if an epsilon of additional regularity as assumed in the radial variable MacNkrNaOz-p; in particular one has GWP for radial H1 data.
- In R3, GWP is known for small Hs data when s > 1 MacNaOz-p2. Some results on the nonrelativistic limit of this equation are also obtained in that paper.

