Stability of thin-shell interfaces inside compact stars
General Relativity and Quantum Cosmology
2015-01-07 v2 Solar and Stellar Astrophysics
Nuclear Theory
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.
Keywords
Cite
@article{arxiv.1412.1848,
title = {Stability of thin-shell interfaces inside compact stars},
author = {Jonas P. Pereira and Jaziel G. Coelho and Jorge A. Rueda},
journal= {arXiv preprint arXiv:1412.1848},
year = {2015}
}
Comments
matches version published in Physical Review D