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Free Dirac Spinors

Free Dirac solutions have two spin states in each frequency sector. Their explicit components are useful for currents and scattering, but normalization and momentum labels matter as much as the component formula. Covariant spin sums and equal-time Hilbert orthogonality use different conjugations and, for the negative-frequency sector, different momentum labels.

Required background. The Covariant Dirac Equation gives the algebraic constraints; Gamma-Matrix Conventions fixes the Dirac basis and adjoint. Helpful background. The Dirac Hamiltonian as an Operator constructs the energy projectors.

Use natural units ℏ=c=1\hbar=c=1, initially m>0m>0, and pμ=(Ep,p)p^\mu=(E_{\mathbf p},\mathbf p) with Ep=p2+m2>0E_{\mathbf p}=\sqrt{\mathbf p^2+m^2}>0. The two mode conventions are

ψ+(x)=us(p)e−ip⋅x,ψ−(x)=vs(p)e+ip⋅x.\begin{aligned} \psi_+(x)&=u_s(p)e^{-ip\cdot x},\\ \psi_-(x)&=v_s(p)e^{+ip\cdot x}. \end{aligned}

Thus uu obeys (p ⁣ ⁣ ⁣/−m)u=0(p\!\!\!/-m)u=0, while vv obeys (p ⁣ ⁣ ⁣/+m)v=0(p\!\!\!/+m)v=0. The vv mode has eigenvalues −Ep-E_{\mathbf p} and −p-\mathbf p under i∂ti\partial_t and −i∇-i\nabla. The label pp in v(p)v(p) remains future directed; it is not the mode’s canonical four-momentum.

For u=(ξ,ζ)Tu=(\xi,\zeta)^T, the Dirac-basis equations are

(E−m)ξ=(σ⋅p)ζ,(E+m)ζ=(σ⋅p)ξ.\begin{aligned} (E-m)\xi&=(\boldsymbol\sigma\cdot\mathbf p)\zeta,\\ (E+m)\zeta&=(\boldsymbol\sigma\cdot\mathbf p)\xi. \end{aligned}

Choose orthonormal two-spinors χs\chi_s and, independently, ηs\eta_s, with s=1,2s=1,2. A convenient covariant normalization is

us(p)=E+m(χsσ⋅pE+mχs),u_s(p)=\sqrt{E+m} \begin{pmatrix} \chi_s\\ \dfrac{\boldsymbol\sigma\cdot\mathbf p}{E+m}\chi_s \end{pmatrix}, vs(p)=E+m(σ⋅pE+mηsηs).v_s(p)=\sqrt{E+m} \begin{pmatrix} \dfrac{\boldsymbol\sigma\cdot\mathbf p}{E+m}\eta_s\\ \eta_s \end{pmatrix}.

The Pauli identity (σ⋅p)2=p2I(\boldsymbol\sigma\cdot\mathbf p)^2=\mathbf p^2I and E2−m2=p2E^2-m^2=\mathbf p^2 verify both equations directly. At rest us=2m(χs,0)Tu_s=\sqrt{2m}(\chi_s,0)^T and vs=2m(0,ηs)Tv_s=\sqrt{2m}(0,\eta_s)^T. Choosing fixed rest-spin labels and boosting them is one useful convention; helicity labels instead depend on the direction of momentum. No specific charge-conjugation phase relation between χs\chi_s and ηs\eta_s is required for these results.

Direct block multiplication gives

uˉr(p)us(p)=2mδrs,vˉr(p)vs(p)=−2mδrs,ur(p)†us(p)=2Eδrs,vr(p)†vs(p)=2Eδrs.\begin{aligned} \bar u_r(p)u_s(p)&=2m\delta_{rs},\\ \bar v_r(p)v_s(p)&=-2m\delta_{rs},\\ u_r(p)^\dagger u_s(p)&=2E\delta_{rs},\\ v_r(p)^\dagger v_s(p)&=2E\delta_{rs}. \end{aligned}

For example, u†u=(E+m)[1+p2/(E+m)2]=2Eu^\dagger u=(E+m)[1+\mathbf p^2/(E+m)^2]=2E, whereas the minus sign from γ0\gamma^0 gives uˉu=(E+m)[1−p2/(E+m)2]=2m\bar uu=(E+m)[1-\mathbf p^2/(E+m)^2]=2m. The negative sign of vˉv\bar vv is not a negative probability: the Hilbert density is v†v>0v^\dagger v>0.

For equal future-directed labels, uˉr(p)vs(p)=0\bar u_r(p)v_s(p)=0. However,

ur(p)†vs(p)=2χr†(σ⋅p)ηsu_r(p)^\dagger v_s(p)= 2\chi_r^\dagger(\boldsymbol\sigma\cdot\mathbf p)\eta_s

need not vanish. The two spinors do not belong to opposite eigenspaces of the same momentum-space Hamiltonian: v(p)v(p) belongs to the negative sector at canonical momentum −p-\mathbf p. The correct fixed-momentum orthogonality is

ur(p)†vs(−p)=0.u_r(p)^\dagger v_s(-\mathbf p)=0.

Here vs(−p)v_s(-\mathbf p) means vs(Ep,−p)v_s(E_{\mathbf p},-\mathbf p). This distinction is essential when normalizing Fourier wave packets.

Summing over the two spin states uses ∑sχsχs†=∑sηsηs†=I2\sum_s\chi_s\chi_s^\dagger=\sum_s\eta_s\eta_s^\dagger=I_2. The uu sum is ∑sus(p)uˉs(p)=p ⁣ ⁣ ⁣/+m\sum_su_s(p)\bar u_s(p)=p\!\!\!/+m, whose explicit blocks are

p ⁣ ⁣ ⁣/+m=((E+m)I2−σ⋅pσ⋅p−(E−m)I2).p\!\!\!/+m= \begin{pmatrix} (E+m)I_2&-\boldsymbol\sigma\cdot\mathbf p\\ \boldsymbol\sigma\cdot\mathbf p&-(E-m)I_2 \end{pmatrix}.

Similarly,

∑svs(p)vˉs(p)=p ⁣ ⁣ ⁣/−m.\sum_sv_s(p)\bar v_s(p)=p\!\!\!/-m.

These are basis-independent identities once the stated spinor normalization is fixed. They are not themselves unit-normalized orthogonal Hilbert projectors. Multiplying by γ0\gamma^0 and dividing by 2E2E gives

12E∑sus(p)us(p)†=P+(p),12E∑svs(−p)vs(−p)†=P−(p).\begin{aligned} \frac1{2E}\sum_su_s(p)u_s(p)^\dagger&=P_+(\mathbf p),\\ \frac1{2E}\sum_sv_s(-\mathbf p)v_s(-\mathbf p)^\dagger&=P_-(\mathbf p). \end{aligned}

Their sum is I4I_4. The scalar denominators 2m2m in covariant normalization and 2E2E in equal-time projectors have different roles.

With the present spinors, write a free square-integrable packet as

ψ(x)=∑s∫d3p(2π)3/22Ep Fs(p,x),Fs(p,x)=as(p)us(p)e−ip⋅x+bs(p)vs(p)e+ip⋅x.\begin{aligned} \psi(x) &=\sum_s\int\frac{d^3p}{(2\pi)^{3/2}\sqrt{2E_{\mathbf p}}} \,F_s(p,x),\\ F_s(p,x)&=a_s(\mathbf p)u_s(p)e^{-ip\cdot x}\\ &\quad+b_s(\mathbf p)v_s(p)e^{+ip\cdot x}. \end{aligned}

The spatial delta function in a mixed term enforces opposite labels; the orthogonality just derived then gives

∫d3x ψ†ψ=∑s∫d3p (∣as(p)∣2+∣bs(p)∣2).\int d^3x\,\psi^\dagger\psi =\sum_s\int d^3p\, \left(|a_s(\mathbf p)|^2+|b_s(\mathbf p)|^2\right).

Both signs enter positively. These coefficients describe a c-number one-particle equation; replacing them by field operators and assigning particle statistics is a further construction.

At m→0m\to0 with fixed nonzero p\mathbf p, the component formulas and the 2E2E Hilbert norms remain finite. The scalar bilinears uˉu\bar uu and vˉv\bar vv vanish, so a convention that divides spinors or projectors by mm has no direct massless continuation. For positive-frequency spinors choose (σ⋅p^)χλ=λχλ(\boldsymbol\sigma\cdot\widehat{\mathbf p})\chi_\lambda =\lambda\chi_\lambda, λ=±1\lambda=\pm1. Then uλ=E(χλ,λχλ)Tu_\lambda=\sqrt E(\chi_\lambda,\lambda\chi_\lambda)^T is an eigenvector of γ5\gamma^5 with eigenvalue λ\lambda and of helicity with eigenvalue λ/2\lambda/2. For massive spinors this equality of chirality and twice helicity no longer holds. Negative-frequency mode labels and physical antiparticle helicity require their own conjugation conventions.

  1. For p=pz^\mathbf p=p\widehat{\mathbf z} and χ=η=(1,0)T\chi=\eta=(1,0)^T, write u(p)u(p) and v(−p)v(-\mathbf p) and check their Hilbert orthogonality.
Solution

They are E+m(1,0,p/(E+m),0)T\sqrt{E+m}(1,0,p/(E+m),0)^T and E+m(−p/(E+m),0,1,0)T\sqrt{E+m}(-p/(E+m),0,1,0)^T. Their scalar product is −p+p=0-p+p=0. Using v(+p)v(+\mathbf p) would instead give 2p2p.

  1. Rescale uu to unit Hilbert norm. What becomes of uˉu\bar uu and the spin sum?
Solution

With w=u/2Ew=u/\sqrt{2E}, w†w=1w^\dagger w=1, wˉw=m/E\bar ww=m/E, and ∑swswˉs=(p ⁣ ⁣ ⁣/+m)/(2E)\sum_sw_s\bar w_s=(p\!\!\!/+m)/(2E). The energy factor is frame dependent; the invariant 2m2m convention has intentionally been changed.

  1. For m>0m>0, take the trace of the positive-frequency spin sum. Why does it match two spin states rather than four?
Solution

tr⁡(p ⁣ ⁣ ⁣/+m)=4m\operatorname{tr}(p\!\!\!/+m)=4m. On the other side, tr⁡(usuˉs)=uˉsus=2m\operatorname{tr}(u_s\bar u_s)=\bar u_su_s=2m for each of two states. A four-component spinor constrained to one on-shell energy sector has only two independent spin amplitudes.

  • J. D. Bjorken and S. D. Drell, Relativistic Quantum Mechanics, McGraw–Hill, 1964 — explicit free spinors; translate normalization before combining formulas.
  • C. Itzykson and J.-B. Zuber, Quantum Field Theory, McGraw–Hill, 1980 — covariant spinor normalization and completeness.
  • M. D. Schwartz, Quantum Field Theory and the Standard Model, Cambridge University Press, 2014, doi:10.1017/9781139540940 — spin sums and helicity.