Solar-system tests of the inflation model with a Weyl term
  Recently, there has been an interest in inflation and modified gravity with a
Weyl term added to the general-relativistic action (N. Derulle, M. Sasaki, Y.
Sendouda and A. Youssef, JCAP, 3, 040 (2011)). In this paper we study empirical
constraint on this modified gravity from solar-system experiments/observations.
We first derive linearized equation of motion in the weak field limit and solve
it for isolated system in the slow motion limit. We then use it to derive the
light propagation equations, and obtain the relativistic Shapiro time delay and
the light deflection in one-body central problem. Applying these results to the
solar-system measurements, we obtain constraints on the Weyl term parameter
{\gamma}_W; the most stringent constraint, which comes from the Cassini
relativistic time delay experiment, is for {\gamma}_W to be less than 0.0015
AU^2, or |{\gamma}_W|^(1/2) less than 0.039 AU (19 s). Analysis of precision
laboratory gravity experiments put further limit on the Weyl term parameter
{\gamma}_W to below the laboratory scale.
