Bending of Light in Quantum Gravity
  We consider the scattering of lightlike matter in the presence of a heavy scalar object (such as the Sun or a Schwarzschild black hole). By treating general relativity as an effective field theory we directly compute the nonanalytic components of the one-loop gravitational amplitude for the scattering of massless scalars or photons from an external massive scalar field. These results allow a semiclassical computation of the bending angle for light rays grazing the Sun, including long-range $\hbar$ contributions. We discuss implications of this computation, in particular the violation of some classical formulations of the equivalence principle. 
N. E. J. Bjerrum-Bohr, John F. Donoghue, Barry R. Holstein, Ludovic   Plant\'e and Pierre Vanhove
hep-th gr-qc hep-ph