Strange Quark Stars with a Rotating Superfluid Core

摘要: The generation of a magnetic field and its distribution inside rotating bare strange quark star are discussed. It is shown that the difference between angular velocities superfluid superconducting core Ωs normal electron plasma Ω n increases because spin-down this leads to field. in found for stationary value ∆Ω=Ω s - = const . shell continuous along star’s axis rotation has same B q , while it dipole outside star. In all parts determined entirely by total moment M also proportional ΔW, some models compact stars can vary from 1031-1034 G·cm3.