Abstract

A method for calculating the asymptotic expansion coefficients of the heat kernel associated with a fermion of spin in an arbitrary-dimensional Riemann - Cartan spacetime is presented. It is shown that the first two coefficients in our approach agree with those given by using the proper time and the normal coordinate methods. In a four-dimensional massless fermion model, the explicit expression of the coefficients is given in the form of separating torsions from the curvature and the covariant differentiation.

Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call