We show that if the beta functions of a field theory are given by the gradi
ent of a certain potential on the space of couplings, a gravitational backg
round in one more dimension can express the renormalization group (RG) flow
of the theory. The field theory beta functions and the gradient ow constra
int together reconstruct the second-order spacetime equations of motion. Th
e RG equation reduces to the conventional gravitational computation of the
spacetime quasilocal stress tensor, and a c-theorem holds true as a consequ
ence of the Raychaudhuri equation. Conversely, under certain conditions, if
the RG evolution of a field theory possesses a monotonic c-function, the f
low of couplings can be expressed in terms of a higher-dimensional gravitat
ional background.