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Supernovae (SN) explosions are thought to be an important source of dust ingalaxies. At the same time strong shocks from SNe are known as an efficientmechanism of dust destruction via thermal and kinetic sputtering. A criticallyimportant question of how these two hypotheses of SNe activity control the dustbudget in galaxies is still not quite clearly understood. In this paper weaddress this question within 3D multi-fluid hydrodynamical simulations,treating separately the SNe injected dust and the dust pre-existed in ambientinterstellar gas. We focus primarily on how the injected and the pre-existingdust is destroyed by shock waves and hot gas in the SN bubble depending on thedensity of ambient gas. Within our model we estimate an upper limit of theSN-produced dust mass which can be supplied into interstellar medium. For a SNprogenitor mass of 30 $M_\odot$ and the ejected dust mass $M_d=1~M_\odot$ weconstrain the dust mass that can be delivered into the ISM as $\geq0.13~M_\odot$, provided that the SN has injected large dust particles with$a\geq 0.1~\mu$m.

Dust evolution in a supernova interacting with the ISM