Publication Type:

Journal Article

Source:

Acta Physica Polonica B, Proceedings Supplement, Jagellonian University, Volume 10, Number 1, p.259-268 (2017)

URL:

https://www.scopus.com/inward/record.uri?eid=2-s2.0-85017355473&doi=10.5506%2fAPhysPolBSupp.10.259&partnerID=40&md5=4ac43c928bd7fdc1cb2d67330de6ffdd

Keywords:

Compressibility of liquids, Compressible liquid, Energy density, Neutron stars, Phase transitions, Skyrme-forces, Stars, Symmetry energies, Thermodynamical, Thomas-Fermi method, Transition density

Abstract:

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.

Notes:

cited By 0

Cite this Research Publication

X. Viñas, Gonzalez-Boquera, C., Sharma, B. K., and Centelles, M., “Pasta-phase transitions in the inner crust of neutron stars”, Acta Physica Polonica B, Proceedings Supplement, vol. 10, pp. 259-268, 2017.

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