2 Spin

In the previous section, we introduced the Dirac spinor as a solution to the Dirac equation. Now we will investigate this further and try to understand what the different components are.

2.1 Plane-Wave Solutions of the Dirac Equation

Let us try and solve the free Dirac equation in terms of plane waves. Since we expect both positive and negative energy solutions, we can make an ansatz

ψr(+)=e−i⁢p⋅x⁢ur⁢(p),ψr(−)=e+i⁢p⋅x⁢vr⁢(p).\displaystyle\psi_{r}^{(+)}={\rm e}^{-ip\cdot x}u_{r}(p)\,,\qquad\psi_{r}^{(-)% }={\rm e}^{+ip\cdot x}v_{r}(p)\,. (23)

This leads to two different momentum-space version of the Dirac equation

(γ⋅p−m)⁢ur⁢(p)=(−γ⋅p−m)⁢vr⁢(p)=0.\displaystyle(\gamma\cdot p-m)u_{r}(p)=(-\gamma\cdot p-m)v_{r}(p)=0\,. (24)

In the restframe of the particle where p=(m,0,0,0)p=(m,0,0,0), we have

(γ0−1)⁢u⁢(0)=(γ0+1)⁢v⁢(0)=0.\displaystyle(\gamma^{0}-1)u(0)=(\gamma^{0}+1)v(0)=0\,. (25)

We can find explicit answers for the spinors using the explicit representation of (16)

u1⁢(0)=𝒩⁢(1000),u2⁢(0)=𝒩⁢(0100),v1⁢(0)=𝒩⁢(0010),v2⁢(0)=𝒩⁢(0001).\displaystyle u_{1}(0)=\mathcal{N}\begin{pmatrix}1\\ 0\\ 0\\ 0\end{pmatrix}\,,\quad u_{2}(0)=\mathcal{N}\begin{pmatrix}0\\ 1\\ 0\\ 0\end{pmatrix}\,,\quad v_{1}(0)=\mathcal{N}\begin{pmatrix}0\\ 0\\ 1\\ 0\end{pmatrix}\,,\quad v_{2}(0)=\mathcal{N}\begin{pmatrix}0\\ 0\\ 0\\ 1\end{pmatrix}\,. (26)

Note that we have not one but two solution for each direction of pp. One can show that these correspond to the two spin directions. At this point the normalisation factor 𝒩\mathcal{N} is a free parameter. It turns out that 𝒩=2⁢m\mathcal{N}=\sqrt{2m} but it is possible to modify the following equations to accommodate another normalisation.

To turn these into solutions for u⁢(p)u(p), we could perform a Lorentz boost. Alternatively, we can note that

(γ⋅p−m)⁢(γ⋅p+m)=(p2−m2),\displaystyle(\gamma\cdot p-m)(\gamma\cdot p+m)=(p^{2}-m^{2})\,, (27)

to write

ur⁢(p)∝(γ⋅p+m)⁢ur⁢(0),vr⁢(p)∝(−γ⋅p+m)⁢vr⁢(0).\displaystyle u_{r}(p)\propto(\gamma\cdot p+m)u_{r}(0)\,,\qquad v_{r}(p)% \propto(-\gamma\cdot p+m)v_{r}(0)\,. (28)

This is a solution of the Dirac equation because we get zero if we left-multiply with γ⋅p−m\gamma\cdot p-m since p2=m2p^{2}=m^{2}. A suitable normalisation would be

ur⁢(p)=γ⋅p+m2⁢m⁢(m+p0)⁢ur⁢(0),vr⁢(p)=−γ⋅p+m2⁢m⁢(m+p0)⁢vr⁢(0),\displaystyle u_{r}(p)=\frac{\gamma\cdot p+m}{\sqrt{2m(m+p^{0})}}u_{r}(0)\,,% \qquad v_{r}(p)=\frac{-\gamma\cdot p+m}{\sqrt{2m(m+p^{0})}}v_{r}(0)\,, (29)

since it leads to be the “boost operator” to be normalised, i.e. for p→→0\vec{p}\to 0, the fraction has components of one.

2.2 Spin and helicity

Each of the two Dirac spinors has two linearly independent solutions which we claimed are the two possible spin states of a fermion. To verify this, we will try and define the spin operator that measures the spin of a fermion. In the particle’s rest frame, we had

u1=(1000)andu2=(0100).\displaystyle u_{1}=\begin{pmatrix}1\\ 0\\ 0\\ 0\end{pmatrix}\qquad\text{and}\qquad u_{2}=\begin{pmatrix}0\\ 1\\ 0\\ 0\end{pmatrix}\,. (30)

These have eigenvalues ±12\pm\frac{1}{2} under the matrix

12⁢(σz000)\displaystyle\frac{1}{2}\begin{pmatrix}\sigma_{z}&0\\ 0&0\end{pmatrix} (31)

Repeating the same for anti-particles, we have the spin operator

S→=12⁢(σ→00σ→).\displaystyle\vec{S}=\frac{1}{2}\begin{pmatrix}\vec{\sigma}&0\\ 0&\vec{\sigma}\end{pmatrix}\,. (32)

You can easily verify that S→2=3/4\vec{S}^{2}=3/4 as expected. We can therefore conclude that, at least in the rest frame, the top two components of ψ\psi describe a spin up (Sz=+1/2S_{z}=+1/2) and spin down (Sz=−1/2S_{z}=-1/2) state, respectively.

To generalise this to general p→\vec{p}, we can project the spin-operator along the direction of motion. This is called the helicity operator

h⁢(p→)=1|p→|⁢(σ→⋅p→00σ→⋅p→).\displaystyle h(\vec{p})=\frac{1}{|\vec{p}|}\begin{pmatrix}\vec{\sigma}\cdot% \vec{p}&0\\ 0&\vec{\sigma}\cdot\vec{p}\end{pmatrix}\,. (33)

This satisfies h⁢(p→)2=1h(\vec{p})^{2}=1 and therefore has eigenvalues ±1\pm 1.

2.3 Properties of spinors

To generate an equation for anti-particles, we first take the Hermitian conjugate of the Dirac equation and find

ψ†⁢(−i⁢γ0⁢∂←0−i⁢γi⁢∂←i−m)=0.\displaystyle\psi^{\dagger}(-i\gamma^{0}\overleftarrow{\partial}_{0}-i\gamma^{% i}\overleftarrow{\partial}_{i}-m)=0\,. (34)

Here we have used the fact that γ0⁣†=γ0\gamma^{0{\dagger}}=\gamma^{0} and γi⁣†=−γi\gamma^{i{\dagger}}=-\gamma^{i}. The arrow over the derivative means that it acts to the left rather than to the right. We can rearrange this slightly by multiplying from the right with γ0\gamma^{0} and defining ψ¯=ψ†⁢γ0\bar{\psi}=\psi^{\dagger}\gamma^{0}

ψ†⁢(−i⁢γ0⁢γ0⁢∂←0−i⁢γi⁢γ0⁢∂←i−m)=∗ψ†⁢(−i⁢γ0⁢γ0⁢∂←0+i⁢γ0⁢γi⁢∂←i−m)=ψ¯⁢(−i⁢γ⋅∂←−m)=0.\displaystyle\psi^{\dagger}(-i\gamma^{0}\gamma^{0}\overleftarrow{\partial}_{0}% -i\gamma^{i}\gamma^{0}\overleftarrow{\partial}_{i}-m)\stackrel{{\scriptstyle*}% }{{=}}\psi^{\dagger}(-i\gamma^{0}\gamma^{0}\overleftarrow{\partial}_{0}+i% \gamma^{0}\gamma^{i}\overleftarrow{\partial}_{i}-m)=\bar{\psi}(-i\gamma\cdot% \overleftarrow{\partial}-m)=0\,. (35)

At ∗*, we have used that {γ0,γi}=0\{\gamma^{0},\gamma^{i}\}=0. This can be understood by interpreting ψ¯\bar{\psi} as the wave function of an anti-particle.

One can show by explicit calculation that the choice of normalisation in (29) is orthonormal, i.e. that

ur⁢(p)†⁢γ0⁢us⁢(p)=u¯r⁢(p)⁢us⁢(p)=2⁢m⁢δr⁢s,vr⁢(p)†⁢γ0⁢vs⁢(p)=v¯r⁢(p)⁢vs⁢(p)=−2⁢m⁢δr⁢s,ur⁢(p)†⁢γ0⁢vs⁢(p)=u¯r⁢(p)⁢vs⁢(p)=vs⁢(p)†⁢γ0⁢ur⁢(p)=v¯s⁢(p)⁢ur⁢(p)=0.\displaystyle\begin{split}u_{r}(p)^{\dagger}\gamma^{0}u_{s}(p)&=\bar{u}_{r}(p)% u_{s}(p)=2m\delta_{rs}\,,\\ v_{r}(p)^{\dagger}\gamma^{0}v_{s}(p)&=\bar{v}_{r}(p)v_{s}(p)=-2m\delta_{rs}\,,% \\ \qquad u_{r}(p)^{\dagger}\gamma^{0}v_{s}(p)&=\bar{u}_{r}(p)v_{s}(p)=v_{s}(p)^{% \dagger}\gamma^{0}u_{r}(p)=\bar{v}_{s}(p)u_{r}(p)=0\,.\end{split} (36)

Further, we can show that (completeness relation)

∑r=1,2ur⁢(p)⁢u¯r⁢(p)=γ⋅p+mand∑r=1,2vr⁢(p)⁢v¯r⁢(p)=γ⋅p−m.\displaystyle\sum_{r=1,2}u_{r}(p)\bar{u}_{r}(p)=\gamma\cdot p+m\qquad\text{and% }\qquad\sum_{r=1,2}v_{r}(p)\bar{v}_{r}(p)=\gamma\cdot p-m\,. (37)

2.4 Lorentz transformation

We still need to define how ψ\psi changes under Lorentz transformation, similarly to what we did for ϕ\phi in (9) We define

ψ⁢(x)→ψ′⁢(x′)=ψ′⁢(Λ⁢x)=S⁢(Λ)⁢ψ⁢(x)\displaystyle\psi(x)\to\psi^{\prime}(x^{\prime})=\psi^{\prime}(\Lambda x)=S(% \Lambda)\psi(x) (38)

with a suitable matrix S⁢(Λ)S(\Lambda). Similarly for ψ¯\bar{\psi}

ψ¯⁢(x)→ψ¯′⁢(x′)=ψ¯⁢(x)⁢γ0⁢S⁢(Λ)†⁢γ0.\displaystyle\bar{\psi}(x)\to\bar{\psi}^{\prime}(x^{\prime})=\bar{\psi}(x)% \gamma^{0}S(\Lambda)^{\dagger}\gamma^{0}\,. (39)

SS is determined by requiring that the Dirac equation is Lorentz invariant. It is easy to see that if {γμ,γν}=gμ⁢ν\{\gamma^{\mu},\gamma^{\nu}\}=g^{\mu\nu} then also the matrices (γ′)μ=Λνμ⁢γν(\gamma^{\prime})^{\mu}=\Lambda^{\mu}_{\phantom{\mu}\nu}\gamma^{\nu} will. This means that they, too, are a representation of the Clifford algebra. One can now show that

(γ′)μ=Λνμ⁢γν=S⁢(Λ)−1⁢γμ⁢S⁢(Λ).\displaystyle(\gamma^{\prime})^{\mu}=\Lambda^{\mu}_{\phantom{\mu}\nu}\gamma^{% \nu}=S(\Lambda)^{-1}\gamma^{\mu}S(\Lambda)\,. (40)

This is called Pauli’s fundamental theorem. Therefore,

(i⁢∂μ′γμ−m)⁢ψ′⁢(x′)\displaystyle\big{(}i\partial^{\prime}_{\mu}\gamma^{\mu}-m\big{)}\psi^{\prime}% (x^{\prime}) =(i⁢Λμν⁢∂νγμ−m)⁢S⁢(Λ)⁢ψ⁢(x)\displaystyle=\Big{(}i\Lambda_{\mu}^{\phantom{\mu}\nu}\partial_{\nu}\gamma^{% \mu}-m\Big{)}S(\Lambda)\psi(x) (41)
=S⁢(Λ)⁢(i⁢Λμν⁢∂νS⁢(Λ)−1⁢γμ⁢S⁢(Λ)⏟(γ′)μ−m)⁢ψ⁢(x)\displaystyle=S(\Lambda)\Big{(}i\Lambda_{\mu}^{\phantom{\mu}\nu}\partial_{\nu}% \underbrace{S(\Lambda)^{-1}\gamma^{\mu}S(\Lambda)}_{(\gamma^{\prime})^{\mu}}-m% \Big{)}\psi(x) (42)
=S⁢(Λ)⁢(i⁢Λμν⁢Λρμ⁢∂νγρ−m)⁢ψ⁢(x)=S⁢(Λ)⁢(i⁢∂νγν−m)⁢ψ⁢(x)=0.\displaystyle=S(\Lambda)\Big{(}i\Lambda_{\mu}^{\phantom{\mu}\nu}\Lambda^{\mu}_% {\phantom{\mu}\rho}\partial_{\nu}\gamma^{\rho}-m\Big{)}\psi(x)=S(\Lambda)(i% \partial_{\nu}\gamma^{\nu}-m)\psi(x)=0\,. (43)

(40) is enough to fully specify the S⁢(Λ)S(\Lambda) matrix and we will not need an explicit form. It follows as well that

S†⁢(Λ)=γ0⁢S−1⁢γ0\displaystyle S^{\dagger}(\Lambda)=\gamma^{0}S^{-1}\gamma^{0} (44)

and therefore the transformation of ψ¯\bar{\psi} is also fine. The fact that S−1⁢(Λ)≠S†⁢(Λ)S^{-1}(\Lambda)\neq S^{\dagger}(\Lambda) is not surprising, and is due to the fact that the Lorentz group is non-compact, and therefore it does not admit unitary finite-dimensional representations.

It is very common to construct bi-linear products ψ¯⁢Γ⁢ψ\bar{\psi}\Gamma\psi with some 4×44\times 4 matrix Γ\Gamma. Since Γ\Gamma has 16=4216=4^{2} degrees of freedom, we need 16 linearly independent elements to form a basis out of which we can construct any Γ\Gamma. It turns out that it is possible to classify these 16 matrices very neatly by their behaviour under Lorentz transformations. We have

one scalar

The case of Γ=1\Gamma=1 transforms as

ψ¯⁢ψ→ψ¯⁢S−1⁢(Λ)⁢S⁢(Λ)⁢ψ=ψ¯⁢ψ.\displaystyle\bar{\psi}\psi\to\bar{\psi}S^{-1}(\Lambda)S(\Lambda)\psi=\bar{% \psi}\psi\,. (45)
four vectors

The cases of Γ=γμ\Gamma=\gamma^{\mu} correspond to four different basis entries that all transform the same way

ψ¯⁢γμ⁢ψ→ψ¯⁢S−1⁢(Λ)⁢γμ⁢S⁢(Λ)⁢ψ=Λνμ⁢(ψ¯⁢γν⁢ψ).\displaystyle\bar{\psi}\gamma^{\mu}\psi\to\bar{\psi}S^{-1}(\Lambda)\gamma^{\mu% }S(\Lambda)\psi=\Lambda^{\mu}_{\phantom{\mu}\nu}(\bar{\psi}\gamma^{\nu}\psi)\,. (46)
six tensors

By combining two γ\gamma matrices, we can construct more elements. Rather then setting Γ=γμ⁢γν\Gamma=\gamma^{\mu}\gamma^{\nu} which is not linearly independent due to (18), we instead choose

Σμ⁢ν=i4⁢[γμ,γν]\displaystyle\Sigma^{\mu\nu}=\frac{i}{4}[\gamma^{\mu},\gamma^{\nu}] (47)

as our six basis elements. These transform as follows

ψ¯⁢Σμ⁢ν⁢ψ→ψ¯⁢S−1⁢(Λ)⁢i4⁢[γμ,γν]⁢S⁢(Λ)⁢ψ=Λρμ⁢Λσν⁢(ψ¯⁢Σρ⁢σ⁢ψ).\displaystyle\bar{\psi}\Sigma^{\mu\nu}\psi\to\bar{\psi}S^{-1}(\Lambda)\frac{i}% {4}[\gamma^{\mu},\gamma^{\nu}]S(\Lambda)\psi=\Lambda^{\mu}_{\phantom{\mu}\rho}% \Lambda^{\nu}_{\phantom{\nu}\sigma}(\bar{\psi}\Sigma^{\rho\sigma}\psi)\,. (48)

To find the remaining five elements, we need to define one more matrix, in addition to our four normal γμ\gamma^{\mu}. Traditionally called γ5\gamma^{5},

γ5=i⁢γ0⁢γ1⁢γ2⁢γ3=i4!⁢εμ⁢ν⁢ρ⁢σ⁢γμ⁢γν⁢γρ⁢γσ=(0110).\displaystyle\gamma^{5}=i\gamma^{0}\gamma^{1}\gamma^{2}\gamma^{3}=\frac{i}{4!}% \varepsilon_{\mu\nu\rho\sigma}\gamma^{\mu}\gamma^{\nu}\gamma^{\rho}\gamma^{% \sigma}=\begin{pmatrix}0&1\\ 1&0\end{pmatrix}\,. (49)

The last equality here is again assuming the Dirac representation. Independent of the explicit representation, one can show that

(γ5)2=1,{γ5,γμ}=0,(γ5)†=γ5.\displaystyle(\gamma^{5})^{2}=1\,,\qquad\{\gamma^{5},\gamma^{\mu}\}=0\,,\qquad% (\gamma^{5})^{\dagger}=\gamma^{5}\,. (50)

Using it, we can define

one pseudo-scalar

The case of Γ=γ5\Gamma=\gamma^{5} transforms as

ψ¯⁢γ5⁢ψ\displaystyle\bar{\psi}\gamma^{5}\psi →ψ¯⁢S−1⁢(Λ)⁢i4!⁢εμ⁢ν⁢ρ⁢σ⁢γμ⁢γν⁢γρ⁢γσ⁢S⁢(Λ)⁢ψ\displaystyle\to\bar{\psi}S^{-1}(\Lambda)\frac{i}{4!}\varepsilon_{\mu\nu\rho% \sigma}\gamma^{\mu}\gamma^{\nu}\gamma^{\rho}\gamma^{\sigma}S(\Lambda)\psi (51)
=ψ¯⁢i4!⁢εμ⁢ν⁢ρ⁢σ⁢Λαμ⁢Λβν⁢Λγρ⁢Λδσ⁢γα⁢γβ⁢γγ⁢γδ⁢ψ\displaystyle=\bar{\psi}\frac{i}{4!}\varepsilon_{\mu\nu\rho\sigma}\Lambda^{\mu% }_{\phantom{\mu}\alpha}\Lambda^{\nu}_{\phantom{\nu}\beta}\Lambda^{\rho}_{% \phantom{\rho}\gamma}\Lambda^{\sigma}_{\phantom{\sigma}\delta}\gamma^{\alpha}% \gamma^{\beta}\gamma^{\gamma}\gamma^{\delta}\psi (52)
=∗(detΛ)⁢ψ¯⁢i⁢Λα0⁢Λβ1⁢Λγ2⁢Λδ3⁢γα⁢γβ⁢γγ⁢γδ⁢ψ=detΛ⁢ψ¯⁢γ5⁢ψ,\displaystyle\stackrel{{\scriptstyle*}}{{=}}(\det\Lambda)\ \bar{\psi}i\Lambda^% {0}_{\phantom{0}\alpha}\Lambda^{1}_{\phantom{1}\beta}\Lambda^{2}_{\phantom{2}% \gamma}\Lambda^{3}_{\phantom{3}\delta}\gamma^{\alpha}\gamma^{\beta}\gamma^{% \gamma}\gamma^{\delta}\psi=\det\Lambda\ \bar{\psi}\gamma^{5}\psi\,, (53)

where we have used at ∗* the fact that the determinant of a matrix can be written using the ε\varepsilon tensor.

four pseudo-vectors

The cases of Γ=γ5⁢γμ\Gamma=\gamma^{5}\gamma^{\mu} correspond to four different basis entries that all transform the same way

ψ¯⁢γ5⁢γμ⁢ψ→(detΛ)⁢Λνμ⁢(ψ¯⁢γ5⁢γν⁢ψ).\displaystyle\bar{\psi}\gamma^{5}\gamma^{\mu}\psi\to(\det\Lambda)\Lambda^{\mu}% _{\phantom{\mu}\nu}(\bar{\psi}\gamma^{5}\gamma^{\nu}\psi)\,. (54)

The presence of detΛ\det\Lambda in these last two classes gives these objects the pseudo prefix that means they swap sign for improper transformations.

The most common use of γ5\gamma^{5} is in the projectors PL=(1−γ5)/2P_{L}=(1-\gamma^{5})/2 and PR=(1+γ5)/2P_{R}=(1+\gamma^{5})/2. You can check explicitly that these behave like projectors (ie. P2=PP^{2}=P and PL⁢PR=0P_{L}P_{R}=0). When these act upon a Dirac spinor they project out either the component with “left-handed” chirality or with “right-handed” chirality. These projectors therefore appear when considering weak interactions, for example, as WW bosons only couple to left-handed particles. One has to take care when defining the handedness of antiparticles because

ψ¯L=ψL†⁢γ0=ψ†⁢PL⁢γ0=ψ†⁢γ0⁢PR=ψ¯⁢PR.\displaystyle\bar{\psi}_{L}=\psi^{\dagger}_{L}\gamma^{0}=\psi^{\dagger}P_{L}% \gamma^{0}=\psi^{\dagger}\gamma^{0}P_{R}=\bar{\psi}P_{R}\,. (55)

A left-handed anti-particle appears with a right-handed projection operator next to it and vice-versa.