In a viscous Bianchi type-I metric of the Kasner form, it is well known tha
t it is not possible to describe an anisotropic physical model of the unive
rse, which satisfies the second law of thermodynamics and the dominant ener
gy condition in Einstein's theory of gravity. We examine this problem in sc
alar-tensor theories of gravity. In this theory we show that it is possible
to describe the growth of entropy, keeping the thermodynamics and the domi
nant energy condition.