Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature
Year: 2025
Type: article
Abstract: The characteristics of the hadron-to-quark first-order phase transition differ depending on whether charge neutrality is locally or globally fulfilled. In $\ensuremath{\beta}$-equilibrated matter, these two possibilities correspond to the Maxwell and Gibbs constructions. Recently, we presented a new framework in which a continuously varying parameter allows one to describe a first-order phase transition in intermediate scenarios to the two extremes of fully local and fully global charge neutrality. In this work, we extend the previous framework to finite temperatures and out-of-$\ensuremath{\beta}$ equilibrium conditions, making it available for simulations of core-collapse supernovae and binary neutron star mergers. We investigate its impact on key thermodynamic quantities across a range of baryon densities, temperatures, and electron fractions. We find that when matter is not in $\ensuremath{\beta}$ equilibrium, the pressure in the mixed phase is not constant even for the case of fully local charge neutrality. Moreover, we compute the thermal index using three different approaches, demonstrating that the finite-temperature extension of an equation of state using a constant thermal index can be ill defined when applied to the mixed phase.
DOI: 10.1103/8l3m-tdlc
Institutions: Istituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And Applications, European Centre for Theoretical Studies in Nuclear Physics and Related Areas, University of Ferrara, Istituto Nazionale di Fisica Nucleare, Sezione di Ferrara, University of Washington, Ohio University, University of California, Berkeley, Shanghai Jiao Tong University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W4416088467
