Brans-Dicke Theory and Thermodynamical Laws on Apparent and Event
  Horizons
  In this work, we have described the Brans-Dicke theory of gravity and given a
particular solution by choosing a power law form of scalar field $\phi$ and
constant $\omega$. If we assume first law and entropy formula on apparent
horizon then we recover Friedmann equations. Next, assuming first law of
thermodynamics, the validity conditions of GSL on event horizon are presented.
Also without use first law, if we impose the entropy relation on the horizon,
then we also obtain the condition of validity of GSL on event horizon. The
validity of GSL completely depends on the model of BD scalar field solutions.
We have justified that on the apparent horizon the two process are equivalent,
but on the event horizon they are not equivalent. If first law is valid on the
event horizon then GSL may be satisfied in BD solution, but if first law is not
satisfied then GSL is not satisfied in BD solution. So first law always favours
GSL on event horizon. In our effective approach, the first law and GSL is
always satisfied in apparent horizon, which do not depend on BD theory of
gravity.
