Models of Strange Stars with a Crust and Strange Dwarfs

Abstract

Strange quark stars with a crust and strange dwarfs consisting of a compact strange quark core and an extended crust are investigated in terms of a bag model. The crust, which consists of atomic nuclei and degenerate electrons, has a limiting density of ρcr=ρdrip=4.3·1011 g/cm3. A series of configurations are calculated for two sets of bag model parameters and three different values of ρcr (109 g/cm3 ≤ ρcr ≤ ρdrip) to find the dependence of a star's mass M and radius R on the central density. Sequences of stars ranging from compact strange stars to extended strange dwarfs are constructed out of strange quark matter with a crust. The effect of the bag model parameters and limiting crust density ρcr on the parameters of the strange stars and strange dwarfs is examined. The strange dwarfs are compared with ordinary white dwarfs and observational differences between the two are pointed out.