2026-04-18T08:00:51Zhttps://recercat.cat/oai/request

oai:recercat.cat:2445/1219982025-12-05T16:47:11Zcom_2072_1057col_2072_478823col_2072_478917

Pasta-phase transitions in the inner crust of neutron stars Viñas Gausí, Xavier González Boquera, Claudia Sharma, B. K. Centelles Aixalà, Mario Transformacions de fase (Física estadística) Estels de neutrons Phase transformations (Statistical physics) Neutron stars 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. 2018-05-02T11:22:55Z 2018-05-02T11:22:55Z 2017 2018-05-02T11:22:55Z info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 1899-2358 https://hdl.handle.net/2445/121998 669454 eng https://doi.org/10.5506/APhysPolBSupp.10.259 Acta Physica Polonica B Proceedings Supplement, 2017, vol. 10, num. 1, p. 259-268 https://doi.org/10.5506/APhysPolBSupp.10.259 cc-by (c) Viñas Gausí, Xavier et al., 2017 http://creativecommons.org/licenses/by/3.0/es info:eu-repo/semantics/openAccess 10 p. application/pdf Jagiellonian University Articles publicats en revistes (Física Quàntica i Astrofísica)