Framework for phase transitions between the Maxwell and Gibbs constructions
Constantinos Constantinou, Tianqi Zhao, Sophia Han, Madappa Prakash

TL;DR
This paper introduces a thermodynamically consistent framework to model phase transitions in neutron stars that interpolate between Maxwell and Gibbs constructions, enabling more accurate predictions of star properties.
Contribution
It develops a novel method combining local and global charge neutrality to describe intermediate phase transitions, bridging the gap between Maxwell and Gibbs models.
Findings
Smooth transformation of neutron star properties from Gibbs to Maxwell structures
Calculation of mass-radius curves and tidal deformabilities for intermediate models
Identification of a gap in g-mode frequencies at specific transition parameters
Abstract
By taking the nucleon-to-quark phase transition within a neutron star as an example, we present a thermodynamically consistent method to calculate the equation of state of ambient matter so that transitions that are intermediate to those of the familiar Maxwell and Gibbs constructions can be described. This method does not address the poorly known surface tension between the two phases microscopically (as, for example, in the calculation of the core pasta phases via the Wigner-Seitz approximation) but instead combines the local and global charge neutrality conditions characteristic of the Maxwell and Gibbs constructions, respectively. Overall charge neutrality is achieved by dividing the leptons to those that obey local charge neutrality (Maxwell) and those that maintain global charge neutrality (Gibbs). The equation of state is obtained by using equilibrium constraints derived from…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · High-pressure geophysics and materials · Geological and Geophysical Studies
