Viñas Gausí, XavierGonzález Boquera, ClaudiaSharma, B. K.Centelles Aixalà, Mario2018-05-022018-05-0220171899-2358https://hdl.handle.net/2445/121998We 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.10 p.application/pdfengcc-by (c) Viñas Gausí, Xavier et al., 2017http://creativecommons.org/licenses/by/3.0/esTransformacions de fase (Física estadística)Estels de neutronsPhase transformations (Statistical physics)Neutron starsinfo:eu-repo/semantics/article6694542018-05-02info:eu-repo/semantics/openAccess