General heat kernel coefficients for massless free spin-3/2 Rarita-Schwinger field

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

References in corpus (2)

• Logarithmic Corrections to Extremal Black Hole Entropy from Quantum Entropy Function
• Generalized mirror symmetry and trace anomalies

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