QCD Phase Diagrams with Charge and Isospin Axes under Heavy-Ion Collision and Stellar Conditions. (arXiv:2004.03039v1 [nucl-th])
<a href="http://arxiv.org/find/nucl-th/1/au:+Aryal_K/0/1/0/all/0/1">K. Aryal</a>, <a href="http://arxiv.org/find/nucl-th/1/au:+Constantinou_C/0/1/0/all/0/1">C. Constantinou</a>, <a href="http://arxiv.org/find/nucl-th/1/au:+Farias_R/0/1/0/all/0/1">R. L. S. Farias</a>, <a href="http://arxiv.org/find/nucl-th/1/au:+Dexheimer%7D_V/0/1/0/all/0/1">V. Dexheimer}</a>
We investigate the phase transition from hadron to quark matter in the
general case without the assumption of chemical equilibrium with respect to
weak decays. The effects of net strangeness on charge and isospin fractions,
chemical potentials, and temperature are studied in the context of the Chiral
Mean Field (CMF) model that incorporates chiral symmetry restoration and
deconfinement. The extent to which these quantities are probed during
deconfinement in conditions expected to exist in protoneutron stars, binary
neutron-star mergers, and heavy-ion collisions is analyzed quantitatively via
the construction of 3-dimensional phase diagrams.
We investigate the phase transition from hadron to quark matter in the
general case without the assumption of chemical equilibrium with respect to
weak decays. The effects of net strangeness on charge and isospin fractions,
chemical potentials, and temperature are studied in the context of the Chiral
Mean Field (CMF) model that incorporates chiral symmetry restoration and
deconfinement. The extent to which these quantities are probed during
deconfinement in conditions expected to exist in protoneutron stars, binary
neutron-star mergers, and heavy-ion collisions is analyzed quantitatively via
the construction of 3-dimensional phase diagrams.
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