Symmetry, Volume 16, Issue 9
2024 September - 158 articles
Cover Story: The equation of state is a fundamental property of nuclear matter governing the size and radius of neutron stars, and the dynamics of neutron star mergers. In addition to astrophysical observations, experiments with heavy-ion collisions at relativistic beam energies have contributed to constrain the parameters of the equation-of-state for symmetric and neutron-rich matter at high density, which exists in the core of neutron stars. The article reviews the status of the experimental research in the laboratory and outlines future prospects. View this paper - Issues are regarded as officially published after their release is announced to the table of contents alert mailing list .
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