Stability of thin-shell interfaces inside compact stars [CL]

We use the thin-shell Darmois-Israel formalism to model and assess the stability of the interfaces separating phases, e.g. the core and the crust, within compact stars. We exemplify this treatment in the simplest case of an incompressible star, in constant pressure phase transitions, and in the case of strange quark stars with crust.

Read this paper on arXiv…

J. Pereira, J. Coelho and J. Rueda
Mon, 8 Dec 14

Comments: To appear in Phys. Rev. D