Hadron-Qualiton Model for the Internal Structure of a Neutron Star and Gravitating Skyrme Theory for Dark Matter/Dark Energy

摘要

We propose the potential strong effects of perturbative (namely, the quark matter) and non-perturbative (namely, the Skyrme soliton) QCD, the theory of the strong interaction, on astrophysicsand cosmology, which is not yet well understood, to explore the internal structure of the neutronstar and to understand the nature of dark matter and dark energy.