Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2009/iii/paper-60/1/solution

Use signature , , and unit-weight antisymmetrized gamma products. The massless Rarita-Schwinger field has the gauge freedom
since the antisymmetric annihilates . This gauge freedom is essential to remove the lower-spin components of the vector-spinor.
Put . Contracting the field equation with and using gives
Expanding the original three-gamma product then reduces its equation to
A gauge transformation changes by . Locally solve to impose gamma-trace gauge. The two equations become
Applying again gives . Nonzero propagating Fourier modes therefore have : the physical modes are massless.
For the massless Rarita-Schwinger polarization count, choose a nonzero future null momentum . The remaining gauge parameters satisfy . Transversality gives , and this residual gauge removes , hence also , because itself satisfies . Only remain, with
The kernel of on four-component spinors has complex dimension two, so there are exactly two independent polarization amplitudes.
To identify their helicities, the spinor rotation generator about the third axis in this convention is . Its two eigenvalues on that kernel are . If is such an eigenvector, then . Its transverse vector polarization is consequently for or for . These carry vector helicity or , respectively. Adding the vector and spinor angular momenta leaves
The unwanted opposite-sign vector-spinor combinations, which would have helicity , violate the gamma-trace constraint. For the gravitino of simple supergravity, its Majorana spinor reality condition identifies the negative-frequency antiparticle modes, giving two propagating degrees of freedom. If one instead chooses a complex Dirac vector-spinor, its independent antiparticle sector doubles the particle-plus-antiparticle count; the equation alone does not impose a Majorana condition.

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