I'm reading "Lectures on black holes and the $AdS_3/CFT_2$ correspondence" by Kraus.
http://arxiv.org/abs/hep-th/0609074
I don't know how one can obtain Eq.7.12. My stupid question is how to obtain this equation. After this equation, it is stated that "one has to take care to consider only variations consistent with the equations of motion and the assumed boundary conditions". What are the variations consistent with the equations of motion and the assumed boundary conditions? What Krasu says is as follows.
To compute the bulk functional integral, we need to evaluate the bulk action for the solutions which contribute, including boundary counterterms if necessary. For an on-shell solution around the $AdS_{3}$ vacuum, one can evaluate the action at the $AdS_3$ vacuum by using the variation of the action with respect to the boundary metric $g^{(0)}$ and the gauge fields $A^{(0)}, \tilde A^{(0)}$
\begin{equation} \delta S= \int d^2x \sqrt{g}\,\left[ \frac12 T^{ij} \delta g_{ij}+\frac{i}{2\pi} J^{i} \delta A_{i} +\frac{i}{2\pi}\tilde J^{i} \delta \tilde A_{i} \right]~. \end{equation} where the superscript $(0)$ is omitted for brevity. Reexpressing this in complex coordinates of the boundary metric, we obtain:
\begin{equation} \delta S=4\pi i \left(T_{ww}\delta \tau+T_{\bar w\bar w}\delta \bar\tau +\frac{\tau_2}{\pi} J_{w}\delta A_{\bar w}+\frac{\tau_2}{\pi} \tilde J_{\bar w}\delta \tilde A_{w}\right)~. \end{equation}
One can integrate the above equation to get: \begin{eqnarray} \mathcal{S}(\tau) & = & - 2 \pi i \tau \big(L_{0} - \frac{c}{24} \big) + 2 \pi i \bar\tau \big(\tilde L_{0} - \frac{\tilde c}{24} \big) \cr && \; - \frac{i\pi}{2} k \big( \tau A_{w}^{2} + \bar \tau A_{\bar w}^{2} + 2 \bar \tau A_{w} A_{\bar w} \big) + \frac{i\pi}{2} \tilde k \big( \tau \tilde A_{w}^{2} + \bar\tau \tilde A_{\bar w}^{2} + 2 \tau \tilde A_{w} \tilde A_{\bar w} \big) \, . \end{eqnarray}
I would like to know the derivation of the last equation.
