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Check your starting knowledge

Supersymmetry adds a new kind of symmetry to field theory. You can begin without knowing superspace, complex geometry, localization, or conformal field theory. The useful starting tools are more familiar: varying an action, following a gauge transformation, evaluating a Gaussian integral, and multiplying matrices.

Try the four questions below before opening their solutions. A missed sign is a reason to revisit one calculation, not to postpone the entire course. Each solution includes a short refresher that you can use immediately. Afterward, begin with what a supercharge does.

Work in four-dimensional Minkowski space with metric ημν=diag⁡(1,−1,−1,−1)\eta_{\mu\nu}=\operatorname{diag}(1,-1,-1,-1) and units ℏ=c=1\hbar=c=1. A complex scalar field has Lagrangian density

L=∂μϕ∗∂μϕ−m2ϕ∗ϕ.\mathcal L=\partial_\mu\phi^*\partial^\mu\phi-m^2\phi^*\phi.

Under a constant phase rotation, δϕ=iαϕ\delta\phi=i\alpha\phi and δϕ∗=−iαϕ∗\delta\phi^*=-i\alpha\phi^*. Derive the Noether current in the convention

δL=jμ∂μα\delta\mathcal L=j^\mu\partial_\mu\alpha

when α\alpha is temporarily allowed to depend on position. Check conservation on the equations of motion. Is the current real?

Hint

The terms proportional to α\alpha cancel. Keep the terms in which the derivative acts on α\alpha.

Complete solution

The differentiated field variation is

δ(∂μϕ)=iα∂μϕ+i(∂μα)ϕ,\delta(\partial_\mu\phi)=i\alpha\partial_\mu\phi +i(\partial_\mu\alpha)\phi,

with the complex-conjugate formula for ϕ∗\phi^*. Substitution gives

δL=i(ϕ∂μϕ∗−ϕ∗∂μϕ)∂μα.\delta\mathcal L =i\bigl(\phi\partial^\mu\phi^*-\phi^*\partial^\mu\phi\bigr) \partial_\mu\alpha.

Thus our specified current is

jμ=i(ϕ∂μϕ∗−ϕ∗∂μϕ).j^\mu=i\bigl(\phi\partial^\mu\phi^*-\phi^*\partial^\mu\phi\bigr).

Taking the divergence cancels the products of first derivatives:

∂μjμ=i(ϕ□ϕ∗−ϕ∗□ϕ)=0,\partial_\mu j^\mu =i\bigl(\phi\Box\phi^*-\phi^*\Box\phi\bigr)=0,

because (□+m2)ϕ=0(\Box+m^2)\phi=0 and its conjugate hold. Complex conjugation reverses the sign of both ii and the bracket, so (jμ)∗=jμ(j^\mu)^*=j^\mu. In mass units [ϕ]=1[\phi]=1 and [∂μ]=1[\partial_\mu]=1, giving [jμ]=3[j^\mu]=3 and a dimensionless integrated charge ∫d3x j0\int d^3x\,j^0.

Choosing δϕ=−iαϕ\delta\phi=-i\alpha\phi instead would reverse the current. A current sign cannot be compared between sources without also comparing the transformation convention.

For fields φa\varphi_a, integrating by parts gives

δS=∫ddx[(∂L∂φa−∂μ∂L∂(∂μφa))δφa+∂μ(∂L∂(∂μφa)δφa)].\delta S=\int d^dx\left[ \left(\frac{\partial\mathcal L}{\partial\varphi_a} -\partial_\mu\frac{\partial\mathcal L}{\partial(\partial_\mu\varphi_a)}\right) \delta\varphi_a +\partial_\mu\left( \frac{\partial\mathcal L}{\partial(\partial_\mu\varphi_a)} \delta\varphi_a\right)\right].

Here repeated field labels are summed. Treat ϕ\phi and ϕ∗\phi^* as independent variables while varying, then impose their physical conjugation relation. Stationarity for arbitrary compactly supported variations gives the Euler–Lagrange equations. Localizing a symmetry parameter isolates the current without guessing it. Return to the current question and identify exactly where the equations of motion were needed.

Let a scalar of charge qq transform as ϕ′=eiqα(x)ϕ\phi'=e^{iq\alpha(x)}\phi. Define

Dμϕ=(∂μ−iqAμ)ϕ,Aμ′=Aμ+∂μα.D_\mu\phi=(\partial_\mu-iqA_\mu)\phi, \qquad A_\mu'=A_\mu+\partial_\mu\alpha.

Show that Dμ′ϕ′=eiqαDμϕD_\mu'\phi'=e^{iq\alpha}D_\mu\phi. Then calculate [Dμ,Dν]ϕ[D_\mu,D_\nu]\phi. We have absorbed the gauge coupling into AμA_\mu here; it is not an additional missing factor.

Hint

Differentiate the exponential before using the transformation of AμA_\mu. In the commutator, terms with two derivatives and terms quadratic in the Abelian connection cancel.

Complete solution

The product rule gives

Dμ′ϕ′=(∂μ−iqAμ−iq∂μα)(eiqαϕ)=eiqα[iq(∂μα)ϕ+∂μϕ−iqAμϕ−iq(∂μα)ϕ]=eiqαDμϕ.\begin{aligned} D_\mu'\phi' &=(\partial_\mu-iqA_\mu-iq\partial_\mu\alpha) (e^{iq\alpha}\phi)\\ &=e^{iq\alpha}\bigl[ iq(\partial_\mu\alpha)\phi+\partial_\mu\phi -iqA_\mu\phi-iq(\partial_\mu\alpha)\phi\bigr]\\ &=e^{iq\alpha}D_\mu\phi. \end{aligned}

Expanding both orders of covariant differentiation leaves

[Dμ,Dν]ϕ=−iqFμνϕ,Fμν=∂μAν−∂νAμ.[D_\mu,D_\nu]\phi=-iqF_{\mu\nu}\phi, \qquad F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu.

The curvature FμνF_{\mu\nu} is unchanged by Aμ↦Aμ+∂μαA_\mu\mapsto A_\mu+\partial_\mu\alpha for smooth α\alpha, since mixed partial derivatives commute. When q=0q=0, both formulas reduce to ordinary differentiation. This check would catch an unpaired sign change in the definition of DμD_\mu.

A position-dependent change of basis produces an extra derivative of that basis. A connection cancels this extra term so that the derivative transforms in the same way as the original field. The gauge field above is the simplest example. In GR, the Christoffel connection plays a related role for coordinate components; a spin connection does so for spinors in a local frame. You will learn the spinor construction when it is needed. For now, reproduce the cancellation above with a constant α\alpha and then with a varying one.

Let a>0a>0 be real, and define

Z(a,J)=∫−∞∞dx exp⁡(−a2x2+Jx)Z(a,J)=\int_{-\infty}^{\infty}dx\, \exp\left(-\frac a2x^2+Jx\right)

for real JJ. Evaluate Z(a,J)Z(a,J) and the normalized moment

⟨x2⟩a=∫dx x2e−ax2/2∫dx e−ax2/2.\langle x^2\rangle_a= \frac{\int dx\,x^2e^{-ax^2/2}}{\int dx\,e^{-ax^2/2}}.

Why does the condition a>0a>0 matter?

Hint

Complete the square. Obtain the moment either by differentiating twice with respect to JJ, or once with respect to aa.

Complete solution

Completing the square yields

−a2x2+Jx=−a2(x−Ja)2+J22a.-\frac a2x^2+Jx =-\frac a2\left(x-\frac Ja\right)^2+\frac{J^2}{2a}.

A real shift of the integration variable and the elementary Gaussian integral therefore give

Z(a,J)=2πa eJ2/(2a).Z(a,J)=\sqrt{\frac{2\pi}{a}}\, e^{J^2/(2a)}.

Since ∂J2Z(a,J)∣J=0\partial_J^2Z(a,J)|_{J=0} inserts x2x^2, division by Z(a,0)Z(a,0) gives ⟨x2⟩a=1/a\langle x^2\rangle_a=1/a. Independently,

−2∂alog⁡Z(a,0)=1a-2\partial_a\log Z(a,0)=\frac1a

gives the same answer. Positivity of aa ensures decay at both ends of the real contour. At a=0a=0 the zero-source integral has infinite volume; for a<0a<0 its integrand grows exponentially. Neither case is covered by the formula as a convergent real integral.

If xx has units, the exponent requires [a]=[x]−2[a]=[x]^{-2} and [J]=[x]−1[J]=[x]^{-1}. Thus 1/a1/a has precisely the units of x2x^2.

To fix the normalization without memorization, square I=∫Re−x2/2dxI=\int_{\mathbb R}e^{-x^2/2}dx. The resulting two-dimensional integral in polar coordinates is I2=2π∫0∞re−r2/2dr=2πI^2=2\pi\int_0^\infty r e^{-r^2/2}dr=2\pi. Positivity gives I=2πI=\sqrt{2\pi}. Rescaling x↦x/ax\mapsto x/\sqrt a supplies the factor a−1/2a^{-1/2}. Return to the Gaussian question and check the power of aa before doing any differentiation.

Consider the Pauli matrices

σ1=(0110),σ2=(0−ii0),σ3=(100−1).\sigma_1=\begin{pmatrix}0&1\\1&0\end{pmatrix}, \quad \sigma_2=\begin{pmatrix}0&-i\\i&0\end{pmatrix}, \quad \sigma_3=\begin{pmatrix}1&0\\0&-1\end{pmatrix}.

Compute σ1σ2\sigma_1\sigma_2 and σ2σ1\sigma_2\sigma_1. For an ordinary complex two-component column u=(a,b)Tu=(a,b)^T, compute u†σ3uu^\dagger\sigma_3u. No anticommuting variables are involved in this question.

Hint

Use row-by-column multiplication. The dagger combines complex conjugation and transpose.

Complete solution

Multiplication gives

σ1σ2=(i00−i)=iσ3,σ2σ1=−iσ3.\sigma_1\sigma_2 =\begin{pmatrix}i&0\\0&-i\end{pmatrix}=i\sigma_3, \qquad \sigma_2\sigma_1=-i\sigma_3.

Thus {σ1,σ2}=0\{\sigma_1,\sigma_2\}=0, whereas [σ1,σ2]=2iσ3[\sigma_1,\sigma_2]=2i\sigma_3. Braces mean AB+BAAB+BA and brackets mean AB−BAAB-BA here. Replacing one bracket with the other changes the algebra.

Since u†=(a∗,b∗)u^\dagger=(a^*,b^*),

u†σ3u=∣a∣2−∣b∣2,u^\dagger\sigma_3u=|a|^2-|b|^2,

which is real but can have either sign. The reality follows from σ3†=σ3\sigma_3^\dagger=\sigma_3; Hermiticity alone does not imply positivity. For u=(1,0)Tu=(1,0)^T the answer is 11, while for u=(0,1)Tu=(0,1)^T it is −1-1.

At this stage a two-component spinor is a column on which rotation matrices act; the details of its Lorentz transformation will be introduced separately for each dimension. Do not infer a conjugation rule merely from the number of components. Bilal’s Introduction to Supersymmetry, section 2.2 provides an optional four-dimensional introduction. Its dotted and undotted notation is not required to solve the matrix question.

If these calculations are comfortable, go directly to the first lesson. If one was unfamiliar, use its refresher and repeat that calculation with a changed input: reverse the phase convention, set q=0q=0, replace aa by 2a2a, or choose another column uu. A useful self-check explains why the answer changes, rather than only producing a new number.

The next new tool is Grassmann calculus. It changes how odd quantities reorder and differentiate. Ordinary matrix noncommutativity and Grassmann anticommutation are different ideas; the course will keep them distinct.