Hadron-quark mixed phase in neutron stars
arXiv:nucl-th/0209091 · doi:10.1016/S0375-9474(03)00739-5
Abstract
Possibility of structured mixed phase at first order phase transitions is examined by taking into account of charge screening and surface effects. Hadron-quark phase transition in dense neutron star interiors is considered as a concrete example.
Talk given at the 7th International Symposium on "Nuclei in the Cosmos", July 8-12,2002
References in corpus (8)
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