1. Skyrme crystals, nuclear matter and compact stars
- Author
-
Christoph Adam, Alberto García Martín-Caro, Miguel Huidobro, and Andrzej Wereszczynski
- Subjects
High Energy Physics - Theory ,Physics and Astronomy (miscellaneous) ,Nuclear Theory ,General Mathematics ,FOS: Physical sciences ,Skyrme model ,neutron stars ,Nuclear Theory (nucl-th) ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,High Energy Physics - Theory (hep-th) ,Skyrme crystals ,Chemistry (miscellaneous) ,nuclear matter ,Computer Science (miscellaneous) - Abstract
A general review of the crystalline solutions of the generalized Skyrme model and their application to the study of cold nuclear matter at finite density and the Equation of State (EOS) of neutron stars is presented. For the relevant range of densities, the ground state of the Skyrme model in the three torus is shown to correspond to configurations with different symmetries, with a sequence of phase transitions between such configurations. The effects of nonzero finite isospin asymmetry are taken into account by the canonical quantization of isospin collective coordinates, and some thermodynamical and nuclear observables (such as the symmetry energy) are computed as a function of the density. We also explore the extension of the model to accommodate strange degrees of freedom, and find a first order transition for the condensation of kaons in the Skyrme crystal background in a thermodynamically consistent, non-perturbative way. Finally, an approximate EOS of dense matter is constructed by fitting the free parameters of the model to some nuclear observables close to saturation density, which are particularly relevant for the description of nuclear matter. The resulting neutron star mass-radius curves already reasonably satisfy current astrophysical constraints., 54 pages, 28 figures, review
- Published
- 2023