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Testing the Phase Transition Parameters Inside Neutron Stars with the Production of Protons and Lambdas in Relativistic Heavy-ion Collisions by Ang Li; Gao-Chan Yong; Ying-Xun Zhang is a Physics and Astronomy article available to read on EtoBox.

What is Testing the Phase Transition Parameters Inside Neutron Stars with the Production of Protons and Lambdas in Relativistic Heavy-ion Collisions about?

We demonstrate the consistency of the quark deconfinement phase transition parameters in the betastable neutron star matter and in the nearly symmetric nuclear matter formed in heavy-ion collisions (HICs). We investigate the proton and Λ flow in Au þ Au collisions at 3 and 4.5 GeV=nucleon incident beam energies with the pure hadron cascade version of a multiphase transport model. The phase transition in HICs and neutron stars is described based on a class of hybrid equations of state from the quark meanfield 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 ∼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 highdensity quark matter equations of state. Finally, compared to the proton flow, the Λ flow is found to be less sensitive and not constraining to the equations of state.

Who reads Testing the Phase Transition Parameters Inside Neutron Stars with the Production of Protons and Lambdas in Relativistic Heavy-ion Collisions?

It is typically read by researchers, students, and practitioners in Physics and Astronomy.

Author
Ang Li; Gao-Chan Yong; Ying-Xun Zhang
Publisher
American Physical Society (APS)
Published
2023
Language
EN
Field
Physics and Astronomy (Physical Sciences)

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