Structure of neutron star crusts from new Skyrme effective interactions constrained by chiral effective field theory

Yeunhwan Lim, Jeremy W. Holt

Research output: Contribution to journalArticlepeer-review

38 Scopus citations

Abstract

We investigate the structure of neutron star crusts, including the crust-core boundary, based on new Skyrme mean field models constrained by the bulk-matter equation of state from chiral effective field theory and the ground-state energies of doubly-magic nuclei. Nuclear pasta phases are studied using both the liquid drop model as well as the Thomas-Fermi approximation. We compare the energy per nucleon for each geometry (spherical nuclei, cylindrical nuclei, nuclear slabs, cylindrical holes, and spherical holes) to obtain the ground state phase as a function of density. We find that the size of the Wigner-Seitz cell depends strongly on the model parameters, especially the coefficients of the density gradient interaction terms. We employ also the thermodynamic instability method to check the validity of the numerical solutions based on energy comparisons.

Original languageEnglish
Article number065805
JournalPhysical Review C
Volume95
Issue number6
DOIs
StatePublished - 30 Jun 2017

Fingerprint

Dive into the research topics of 'Structure of neutron star crusts from new Skyrme effective interactions constrained by chiral effective field theory'. Together they form a unique fingerprint.

Cite this