We show that a systematic study of the isospin dependence of the Equation of State of matter at densities of the order of 2-3 times nuclear matter saturation density can give important information concerning quark deconfinement.
Neutron-Rich matter and quark stars: Testing deconfinement with RNB facilities.
DRAGO, Alessandro;
2003
Abstract
We show that a systematic study of the isospin dependence of the Equation of State of matter at densities of the order of 2-3 times nuclear matter saturation density can give important information concerning quark deconfinement.File in questo prodotto:
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