First-principles path integral Monte Carlo energies for the strongly coupled quantum Coulomb liquid in the white dwarf and neutron star crust regime, giving quantum heat capacities that can be much lower than classical estimates.
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Energy of Quantum Coulomb Liquid
First-principles path integral Monte Carlo energies for the strongly coupled quantum Coulomb liquid in the white dwarf and neutron star crust regime, giving quantum heat capacities that can be much lower than classical estimates.