Abstract

The conformal anomaly for the electromagnetic field in the background gravitational field is obtained in the general covariant gauge with a gauge parameter. We have used the path integral method of Fujikawa with the zeta-regularization. The gauge dependence is observed in the coefficient of the DR term in the' anomaly; various contradicting values have been assigned to the coefficient of this term in the previous calculations on the basis of different regularization schemes in the Feynman gauge. We empha­ size that at the cost of the classical conformal invariance those terms can be eliminated altogether by adding a finite counterterm proportional to ,;g R2 to the Lagrangian. A calculational scheme with regularized Green functions was also examined, and it gives rise to the same results for the anomaly in the conventional Faddeev-Popov formalism as well as in the B-field formalism. The regularization of Green functions introduces an auxiliary mass parameter for each field and the W ard-Takahashi identities impose a condition among those mass parameters. In the framework of the zeta-function regularization, the gauge dependence of the DR term in the anomaly thus appears to be inevitable.

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