Halos and Voids in f(R) Gravity
  In this paper, we study the distribution of dark matter halos and voids using
high resolution simulations in f(R) gravity models with the chameleon mechanism
to screen the fifth force in dense environment. For dark matter halos, we show
that the semi-analytic thin shell condition, with a suitably-defined
environment, provides a good approximation to describe the mass and
environmental dependence of the screening of the fifth force in halos. Due to
stronger gravity, there are far more massive halos and large voids in f(R)
models compared with the \Lambda CDM model. The numbers of voids with an
effective radius of 15Mpc/h are twice and four times as many as those in
\Lambda CDM for f(R) models with |f_{R0}|=1e-5 and 1e-4 respectively. This
provides a new means to test the models using the upcoming observational data.
We also find that halos inside voids are all unscreened in our simulations,
which are ideal objects for the gravity test.
