Testing the phase transition parameters inside neutron stars with the production of protons and lambdas in relativistic heavy-ion collisions. (arXiv:2211.04978v1 [nucl-th])
<a href="http://arxiv.org/find/nucl-th/1/au:+Li_A/0/1/0/all/0/1">Ang Li</a>, <a href="http://arxiv.org/find/nucl-th/1/au:+Yong_G/0/1/0/all/0/1">Gao-Chan Yong</a>, <a href="http://arxiv.org/find/nucl-th/1/au:+Zhang_Y/0/1/0/all/0/1">Ying-Xun Zhang</a>
We demonstrate the consistency of the quark deconfinement phase transition
parameters in the beta-stable neutron star matter and in the nearly symmetric
nuclear matter formed in heavy-ion collisions (HICs). We investigate the proton
and $Lambda$ flow in Au+Au collisions at 3 and 4.5 GeV/nucleon incident beam
energies with the pure hadron cascade version of a multi-phase transport model.
The phase transition in HICs and neutron stars is described based on a class of
hybrid equations of state from the quark mean-field model for the hadronic
phase and a constant-speed-of-sound parametrization for the high-density quark
phase. The measurements of the anisotropic proton flow at 3 GeV/nucleon by the
STAR collaboration favor a relatively low phase transition density lower than
$sim 2.5$ times saturation density indicated by the gravitational wave and
electromagnetic observations of neutron stars. And the proton flow data at the
higher energy of 4.5 GeV/nucleon can be used to effectively constrain the
softness of high-density quark matter equations of state. Finally, compared to
the proton flow, the $Lambda$ flow is found to be less sensitive and not
constraining to the equations of state.
We demonstrate the consistency of the quark deconfinement phase transition
parameters in the beta-stable neutron star matter and in the nearly symmetric
nuclear matter formed in heavy-ion collisions (HICs). We investigate the proton
and $Lambda$ flow in Au+Au collisions at 3 and 4.5 GeV/nucleon incident beam
energies with the pure hadron cascade version of a multi-phase transport model.
The phase transition in HICs and neutron stars is described based on a class of
hybrid equations of state from the quark mean-field model for the hadronic
phase and a constant-speed-of-sound parametrization for the high-density quark
phase. The measurements of the anisotropic proton flow at 3 GeV/nucleon by the
STAR collaboration favor a relatively low phase transition density lower than
$sim 2.5$ times saturation density indicated by the gravitational wave and
electromagnetic observations of neutron stars. And the proton flow data at the
higher energy of 4.5 GeV/nucleon can be used to effectively constrain the
softness of high-density quark matter equations of state. Finally, compared to
the proton flow, the $Lambda$ flow is found to be less sensitive and not
constraining to the equations of state.
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