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Exotic nuclear phases in the inner crust of neutron stars in the light of Skyrme-Hartree-Fock theory

Piotr Magierski·Aurel Bulgac·Paul-Henri Heenen
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Abstract

The bottom part of the neutron star crust is investigated using the Skyrme-Hartree-Fock approach with the Coulomb interaction treated beyond the Wigner-Seitz approximation. A variety of nuclear phases is found to coexist in this region. Their stability and relative energies are governed by the Coulomb, surface and shell energies. We have also found that a substantial contribution is coming from the spin-orbit interaction.

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Piotr Magierski, Aurel Bulgac, Paul-Henri Heenen. 2002-12-21. Exotic nuclear phases in the inner crust of neutron stars in the light of Skyrme-Hartree-Fock theory. https://doi.org/10.1016/s0375-9474(03)00921-7

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