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Pasta-phase transitions in the inner crust of neutron stars

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We perform calculations of nuclear pasta phases in the inner crust of neutron stars with the Thomas-Fermi method and the Compressible Liquid Drop Model using the Barcelona-Catania-Paris-Madrid (BCPM) energy density functional and several Skyrme forces. We compare the crust-core transition density estimated from the crust side with the predictions obtained from the core by using the thermodynamical and dynamical methods. Finally, the correlation between the crust-core transition density and the slope of the symmetry energy at saturation is briefly analyzed.

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Acta Physica Polonica B Proceedings Supplement, 2017, vol. 10, num. 1, p. 259-268

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cc-by (c) Viñas Gausí, Xavier et al., 2017

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Articles publicats en revistes (Física Quàntica i Astrofísica)

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Transformacions de fase (Física estadística)

# metadata.dc.title[].value
Pasta-phase transitions in the inner crust of neutron stars