http://arxiv.org/abs/1412.1848
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.
J. Pereira, J. Coelho and J. Rueda
Mon, 8 Dec 14
19/61
Comments: To appear in Phys. Rev. D