The Russo–Susskind–Thorlacius model or RST model in short is a modification of the CGHS model to take care of conformal anomalies and render it analytically soluble. In the CGHS model, if we include Faddeev–Popov ghosts to gauge-fix diffeomorphisms in the conformal gauge, they contribute an anomaly of −24. Each matter field contributes an anomaly of 1. So, unless N=24, we will have gravitational anomalies. To the CGHS action
S CGHS = 1 2 π ∫ d 2 x − g { e − 2 ϕ [ R + 4 ( ∇ ϕ ) 2 + 4 λ 2 ] − ∑ i = 1 N 1 2 ( ∇ f i ) 2 } {\displaystyle S_{\text{CGHS}}={\frac {1}{2\pi }}\int d^{2}x\,{\sqrt {-g}}\left\{e^{-2\phi }\left[R+4\left(\nabla \phi \right)^{2}+4\lambda ^{2}\right]-\sum _{i=1}^{N}{\frac {1}{2}}\left(\nabla f_{i}\right)^{2}\right\}} , the following term
S RST = − κ 8 π ∫ d 2 x − g [ R 1 ∇ 2 R − 2 ϕ R ] {\displaystyle S_{\text{RST}}=-{\frac {\kappa }{8\pi }}\int d^{2}x\,{\sqrt {-g}}\left[R{\frac {1}{\nabla ^{2}}}R-2\phi R\right]}
is added, where κ is either ( N − 24 ) / 12 {\displaystyle (N-24)/12} or N / 12 {\displaystyle N/12} depending upon whether ghosts are considered. The nonlocal term leads to nonlocality. In the conformal gauge,
S RST = − κ π ∫ d x + d x − [ ∂ + ρ ∂ − ρ + ϕ ∂ + ∂ − ρ ] {\displaystyle S_{\text{RST}}=-{\frac {\kappa }{\pi }}\int dx^{+}\,dx^{-}\left[\partial _{+}\rho \partial _{-}\rho +\phi \partial _{+}\partial _{-}\rho \right]} . It might appear as if the theory is local in the conformal gauge, but this overlooks the fact that the Raychaudhuri equations are still nonlocal.
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