General heat kernel coefficients for massless free spin-3/2 Rarita-Schwinger field
arXiv:1709.08063 · doi:10.1142/S0217751X1850063X
Abstract
We review the general heat kernel method for the Dirac spinor field as an elementary example in any arbitrary background. We, then compute the first three Seeley-DeWitt coefficients for the massless free spin-3/2 Rarita-Schwinger field without imposing any limitations on the background geometry.
13 pages