In theories of modified gravity with the chameleon screening mechanism, the strength of the fifth force depends on environment. This induces an environment dependence of structure formation, which differs from Λ-cold-dark-matter (ΛCDM). We show that these differences could be captured by the marked correlation function. With the galaxy correlation functions and number densities calibrated to match between f(R) and ΛCDM models in simulations, we show that the marked correlation functions by using either the local galaxy number density or halo mass as the marks encode extra information, which can be used to test these theories. We discuss possible applications of these statistics in observations.
|Number of pages||6|
|Journal||Monthly Notices of the Royal Astronomical Society|
|Early online date||21 May 2018|
|Publication status||Published - 1 Aug 2018|
- Cosmology: theory
- Dark energy
- Large-scale structure of Universe