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arXiv · 1908.01600

Energy of Quantum Coulomb Liquid

D. A. Baiko
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Abstract

Using Metropolis method to compute path integrals, the energy of quantum strongly-coupled Coulomb liquid ($1 \leq \Gamma \leq 175$) composed of distinguishable atomic nuclei and uniform incompressible electron background is calculated from first principles. The range of considered temperatures and densities represents fully-ionized layers of white dwarfs and neutron stars. In particular, the results allow one to determine reliably the heat capacity of ions in dense fluid stellar matter, which is a crucial ingredient for modelling thermal evolution of compact degenerate stars.

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D. A. Baiko. 2019-08-05. Energy of Quantum Coulomb Liquid. https://doi.org/10.1093/mnras/stz2041

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