Structure formation during phase transitions in strongly interacting matter

We investigate the properties of strangelets at finite temperature T, where an equivparticle model is adopted with both the linear confinement and leading-order perturbative interactions accounted for using density-dependent quark masses. The shell effects are examined by solving the Dirac equations for quarks in the mean-field approximation, which diminish with temperature as the occupation probability of each single-particle levels fixed by the Fermi-Dirac statistics, i.e., shell dampening. Consequently, instead of decreasing with temperature, the surface tension extracted from a liquid-drop formula increases with T until reaching its peak at T≈20–40 MeV with vanishing shell corrections, where the formula roughly reproduces the free energy per baryon of all strangelets. The curvature term, nevertheless, decreases with T despite the presence of shell effects. The neutron and proton emission rates are fixed microscopically according to the external nucleon gas densities that are in equilibrium with strangelets, which generally increase with T (≲50 MeV) for stable strangelets but decrease for those that are unstable against nucleon emission at T=0. The energy, free energy, entropy, charge-to-mass ratio, strangeness per baryon, and root-mean-square radius of β-stable strangelets obtained with various parameter sets are presented as well. The results indicated in this work are useful for understanding the products of binary compact star mergers and heavy-ion collisions. Published by the American Physical Society 2024

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Structure formation during phase transitions in strongly interacting matter

Cited by 7 publications

References 269 publications

Dynamics of dilute nuclear matter with light clusters and in-medium effects

Dynamics of dilute nuclear matter with light clusters and in-medium effects

Quarkyonic matter and quarkyonic stars in an extended relativistic mean field model

Strangelets at finite temperature: Nucleon emission rates, interface, and shell effects

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