arXiv · 1412.1848
Stability of thin-shell interfaces inside compact stars
Abstract
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 the relevance and non-triviality of 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.
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Jonas P. Pereira, Jaziel G. Coelho, Jorge A. Rueda. 2015-01-05. Stability of thin-shell interfaces inside compact stars. https://doi.org/10.1103/physrevd.90.123011
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