For a free particle the Dirac matrices are constant and the momenta commute. Squaring the Hamiltonian cancels all mixed terms by their anticommutators:Applying another time derivative to the Dirac equation therefore givesfor every component. This is the Klein-Gordon equation. Its componentwise satisfaction is a necessary consequence of the first-order Dirac equation, not a converse selecting all spinor solutions of the squared equation.
HD2=c2p2+m2c4.
(c21∂t2−∇2+ℏ2m2c2)ψα=0
If Av=λv for A=αi or β, then A2=I implies λ2=1. The polynomial x2−1 has distinct roots, so such a matrix is diagonalizable andAnticommutation with another invertible Dirac matrix maps a +1 eigenspace to a −1 eigenspace, so both signs occur with equal multiplicities in a nontrivial representation. A Hermitian operator is appropriate for the physical Hamiltonian and additionally guarantees an orthonormal eigenbasis.
λ=+1 or −1.
For any one of the four anticommuting matrices A, choose another B. Since B−1=B and BAB=−A, cyclic invariance of the trace givesThereforeEquivalently, the paired positive and negative unit eigenvalues cancel. This argument does not depend on a particular matrix representation.
TrA=Tr(B−1AB)=Tr(−A).
Trαi=0,Trβ=0.
The zero trace and unit eigenvalues imply equal numbers of +1 and −1 eigenvalues, so N is even. A two-dimensional representation is impossible: all four matrices α1,α2,α3,β would be traceless 2×2 matrices. Anticommutation gives Tr(AB)=0 for distinct matrices, whereas Tr(A2)=2. They would therefore be four linearly independent members of the three-dimensional complex space of traceless 2×2 matrices, a contradiction.The usual irreducible 3+1 dimensional Dirac representation has N=4. Larger representations can contain multiple copies; the requested lower bound is not itself a proof of irreducibility.
N is even and N≥4.
In two spatial dimensions there are only two kinetic matrices and one mass matrix. The three Pauli matrices square to identity and anticommute pairwise, sois a two-component Dirac Hamiltonian with H2+12=c2(px2+py2)+m2c4. It therefore reproduces the stated first-order equation and its Klein-Gordon square. Requiring a fourth anticommuting matrix in three spatial dimensions is precisely what prevented this two-component construction above.
H2+1=cσxpx+cσypy+mc2σz
Printed angular-momentum qualification. Define the dimensionless spin si=−iεijkαjαk/4 and the physical orbital angular momentum ℓi=εijkxjpk, with [xi,pj]=iℏδij. ThenThe source prints Li=iℓi instead. Taken literally, it is anti-Hermitian, has incompatible units with the dimensionless spin when they are added, and givesIt cannot yield the requested usual angular-momentum algebra or conservation law. For a concrete counterexample set ℏ=1 and take a wave with momentum along z. Sincethe printed Ji=iℓi+si obeys [HD,Jx]=(1+i)cαypz=0.
[si,sj]=iεijksk,[ℓi,ℓj]=iℏεijkℓk,[ℓi,sj]=0.
[Li,Lj]=−ℏεijkLk,[Ji,Jj]=εijk(−ℏLk+isk).
[HD,ℓi]=−ic(α×p)i,[HD,si]=ic(α×p)i,
The physically consistent operator is Jphys=ℓ+ℏs. It satisfiesThe cancellation follows directly from the two mixed commutators above. In a spherical basis the free spinor can be labelled by energy, j=1/2,3/2,…, and mj=−j,…,j, together with a parity or equivalent Dirac angular label distinguishing the two orbital couplings ℓ=j±1/2. Alternatively one can choose a momentum and helicity basis. One cannot simultaneously assign all components of momentum and all angular labels as independent commuting observables.
[Jphys,i,Jphys,j]=iℏεijkJphys,k,[HD,Jphys,i]=0.
Use p=−iℏ∇ and regard e as the signed charge in the printed minimal coupling. Multiplying the first Dirac equation by cγ0 gives H=cα⋅π+βmc2+eΦ, with π=p−eA/c. Removing the rest-energy phase yieldsFor the alternative equation use its specified field conventions literally. They giveConsequently its Hamiltonian is cα⋅p+βmc2−κβΣ⋅B+(iκ/c)βα⋅E. The two shifted equations areThese electric-field factors depend on the source's convention Ei=cF0i; substituting a different Gaussian or SI definition without changing the equation would give incorrect powers of c.
iℏ∂tφ~iℏ∂tχ~=eΦφ~+cσ⋅πχ~,=cσ⋅πφ~+(eΦ−2mc2)χ~.
Fμνγμγν=c2α⋅E+2iΣ⋅B,Σ=diag(σ,σ).
iℏ∂tφ~iℏ∂tχ~=−κσ⋅Bφ~+(cσ⋅p+ciκσ⋅E)χ~,=(cσ⋅p−ciκσ⋅E)φ~+(−2mc2+κσ⋅B)χ~.
For kinetic and field energies small compared with mc2, the minimally coupled lower spinor is χ~≃(σ⋅π)φ~/(2mc). Inserting it into the upper equation and using [πi,πj]=i(eℏ/c)εijkBk gives the Pauli equationThe spin moment is eℏ/(2mc) multiplying σ, or gyromagnetic factor two relative to physical spin ℏσ/2.
iℏ∂tφ~=[2mπ2+eΦ−2mceℏσ⋅B]φ~.
For the alternative equation, elimination givesTo leading kinetic order and leading magnetic interaction this yieldsKeeping the source electric coupling during the same elimination writes the kinetic part more explicitly asThis product includes derivatives acting on the field and must not be treated as an ordinary scalar product of commuting variables. The parameter κ is the intrinsic magnetic-moment coefficient: the moment operator is κσ. As printed, the alternative equation has no minimal charge coupling, so it can describe a neutral particle carrying a magnetic moment. If a Pauli term were added to the charged equation instead, its coefficient would represent an additional, anomalous contribution to the charge-generated Dirac moment.
χ~≃2mc21(cσ⋅p−ciκσ⋅E)φ~.
iℏ∂tφ~=[2mp2−κσ⋅B]φ~+electric-gradient and spin-orbit terms suppressed by c−2.
2m1(σ⋅p+c2iκσ⋅E)(σ⋅p−c2iκσ⋅E).
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