タイトル：The CR-Hydro simulation for modeling of the SNRs
In recent years, the various things about the SuperNova Remnants(SNRs) have become clear by the multi-wavelength observations. Especially, the most interesting thing is that SNRs could produce the galactic Cosmic-Rays(CRs) via Diffusive Shock Acceleration(DSA). To get the self-consistent model that can explain the observation properties, We are now developing the hydrodynamic code coupling with CR-prodution. In this talk, I will shortly talk about SNRs and CRs, then present my current condition.