Dust mass variation rates as a function of time in the fiducial G10LG simulation for various dust processes: dust growth by gas accretion (‘acc’, black), dust destruction by thermal sputtering (‘spu’, red), by supernovae (‘SNII−’, pink), or by astration (‘ast’, purple), dust released by supernovae (‘SNII+’, orange) or stellar winds (‘SW’, green), and dust mass transfer between small and large grains by coagulation (‘coa’, blue) and vice versa by shattering (‘sha’, cyan).