The Walecka model is extended to the neutron star matter, and in it s mean field approximation, the properties of neutron star matter consisted of proton, neutron and electron in uniform strong magnetic fields are studied.

The Kaon condensation in neutron star matter is calculated in the framework of the density dependent relativistic mean-field theory.

The proton and neutron 1S 0 pairing gaps in β-stable neutron star matter have been studied by using the isospin dependent Brueckner-Hartree-Fock approach and the BCS theory.

Neutron ~3PF_2 superfluidity in neutron matter and the effect of microscopic three-body force;

This paper studies the ground state properties of the relativistic neutron matter with variation-al method, by adopting the Hamiltonian of relativistic form, relativistic meson exchange potential, variational function of ψ=FΦ form and a specific correlation function, the single particle s energy and the equation of neutron matter state are calculated,and the results are improved remarkably.

Changes and Clinical Significances of Middle Molecular Substances Levels in the Plasma of Patients with Pregnancy Induced Hypertension;

The changes of middle molecular substances(MMS)content in plasma of rabbitsfollowing abdominal surgery have been assayed by an improved ultra violet ray absorptionmethod.

Clinical study of "Shenshuaikang" to clear middle molecular substance;

Clinical evaluation of the removal of median-molecular solutes in high permeability dialysis;