# Regularization of $\delta$ function and Chiral anomaly in gravity

Mark Srednicki's QFT book presents a regularization of the $$\delta$$ function in calculating the chiral anomaly (see section 77 of the book). This regularization reads $$$$\delta (x-y)=\lim_{M \rightarrow \infty}\int \frac{d^4k}{(2\pi)^4} e^{(i\gamma ^{\mu}D_{\mu})^2/M^2}\circ e^{-ik(x-y)},$$$$ where $$D_{\mu}=\partial_{\mu}-igA_{\mu}$$.

Now I am trying to applying this method to calculate the chiral anomaly of a massless fermion in a gravity field but without gauge field. The action in the gravitational field is $$$$S=\int d^4x \sqrt{g}\bar{\Psi}i\gamma^{\mu}D_{\mu}\Psi,$$$$ where $$D_{\mu}$$ now is $$\partial_{\mu}+\frac{1}{2}\omega_{\mu}^{ab}\sigma_{ab}$$. Under a chiral transformation $$$$\Psi'(x)=e^{-i\alpha(x)\gamma^5}\Psi(x)=\int d^4y ~\delta(x-y)e^{-i\alpha(y)\gamma^5}\Psi(y),$$$$ one gets the shift of the path integral measure: $$$$\mathcal{D \Psi'}\mathcal{D}{\bar{\Psi}'}=\mathcal{D \Psi}\mathcal{D}{\bar{\Psi}}\exp\bigg\{2i\int d^4x \alpha(x) Tr[\delta (x-x) \gamma^5]\bigg\}.$$$$ At this step, I still regularize $$\delta$$ function as \begin{aligned} \delta (x-y)&=\lim_{M \rightarrow \infty}\int \frac{d^4k}{(2\pi)^4} e^{(i\gamma ^{\mu}D_{\mu})^2/M^2}\circ e^{-ik(x-y)}\\ &=\lim_{M \rightarrow \infty}\int \frac{d^4k}{(2\pi)^4}e^{-ik(x-y)}\circ e^{-(\gamma ^{\mu}D_{\mu}-ik_{\mu}\gamma^{\mu})^2/M^2}. \end{aligned} We can expand the square as $$$$(\gamma ^{\mu}D_{\mu}-ik_{\mu}\gamma^{\mu})^2=\frac{1}{\sqrt{g}}D_{\mu}\sqrt{g}g^{\mu \nu}D_{\nu}-\frac{R}{4}+\{\gamma ^{\mu}D_{\mu},-ik_{\mu}\gamma^{\mu}\}-k^2.$$$$ Here, I cannot continue. Could someone please correct me? I have already known the result is a quadratic expression in terms of Riemann tensor and its dual. So I guess the square should produce something like $$[D_{\mu},D_{\nu}]=R^{ab}_{\mu \nu}\sigma_{ab}/2$$, together with the $$\gamma^5$$ put in the trace, the result can be recovered.

It's just very tedious algebra. Expand the exponential function as a power series. Commute all the derivatives to the right where they die against "1", and keep all the terms that can possibly survive the large $$M$$ limit after doing the $$k$$ integral (this requires going to higher orders than you might expect) and then do the gamma matrix traces.