My research is on theoretical aspects of observational
cosmology including formation and evolution of galaxies,
galaxy clusters, and large-scale structure of the universe
based on the state-of-art numerical simulations. Current
reseach theme includes physical properties and detectability
of the missing baryons (aka dark baryons) in the present day
universe, kinematics and thermodynamics of the intracluster
medium, and the effects of the massive neutrinos on the
formation of the large-scale structure in the universe. I'm
also interested in and working on the technical aspects of the
high performance computing useful for the numerical
astrophysics.