In the first part of this paper, we show that the semiclassical Einstein-La
ngevin equation, introduced in the framework of a stochastic generalization
of semiclassical gravity to describe the back reaction of matter stress-en
ergy fluctuations, can be formally derived from a functional method based o
n the influence functional of Feynman and Vernon. In the second part, we de
rive a number of results for background solutions of semiclassical gravity
consisting of stationary and conformally stationary spacetimes and scalar f
ields in thermal equilibrium states. For these cases, fluctuation-dissipati
on relations are derived. We also show that particle creation is related to
the vacuum stress-energy fluctuations and that it is enhanced by the prese
nce of stochastic metric fluctuations. [S0556-2821(99)02318-8].