Stability of strange star crusts and strangelets

We construct strangelets, taking into account electrostatic effects, including Debye screening, and arbitrary surface tension sigma of the interface between vacuum and quark matter. We find that there is a critical surface tension sigma(crit) below which large strangelets are unstable to fragmentation and below which quark star surfaces will fragment into a crystalline crust made of charged strangelets immersed in an electron gas. We derive a model-independent relationship between sigma(crit) and two parameters that characterize any quark matter equation of state. For reasonable model equations of state, we find sigma(crit) typically of order a few MeV/fm(2). If sigma <=sigma(crit), the size-distribution of strangelets in cosmic rays could feature a peak corresponding to the stable strangelets that we construct.