Integrated Active Magnetic Probe in Silicon-on-Insulator Complementary Metal–Oxide–Semiconductor Technology

Abstract

We have investigated the isospin dependence of the neutron and proton 3 P F2 superfluidity in isospin-asymmetric nuclear matter within the framework of the Brueckner-Hartree-Fock approach and the BCS theory. We show that the 3 P F2 neutron and proton pairing gaps depend sensitively on isospin asymmetry of asymmetric nuclear matter. As the isospin asymmetry increases, the neutron 3 P F2 superfluidity becomes stronger and the peak value of the neutron 3 P F2 pairing gap increases rapidly. The isospin dependence of the proton 3 P F2 superfluidity is shown to be opposite to the neutron one. The proton 3 P F2 superfluidity becomes weaker at a higher asymmetry and it even vanishes at high enough asymmetries. At high asymmetries, the neutron 3 P F2 superfluidity turns out to be much stronger than the proton one, implying that the neutron 3 P F2 superfluidity is dominated in the highly asymmetric dense interior of neutron stars.