Publications (3)0 Total impact
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ABSTRACT: Using Nambu$\otimes $spin space Keldysh Green's function approach, we present a nonequilibrium charge and spin pumping theory of a quantum dot in the mico-cavity coupled to two superconducting leads. It is found that the charge currents include two parts: The dissipationless supercurrent standing for the transfer of coherent Cooper pairs and the pumped quasi-particle current. The supercurrent exhibits a dynamic $0-\pi $ transition induced by the frequency and strength of the $\sigma_{-}$ polarized laser field. This dynamic transition is not affected by the strong Coulomb interaction. Especially, the spin current appears and is an even function of the phase difference between two superconductors when the frequency of the polarized laser field is larger than two times superconducting energy gap. Our theory serves as an extension to non-superconducting spintronics.
12/2006;
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ABSTRACT: We report the theoretical investigation of the orbital Kondo effect in an Aharonov-Bohm interferometer by slave-boson mean field approach. It is found that the present orbital Kondo effect can be tuned geometrically by the external magnetic flux. When the magnetic flux $\phi =(2n+1)\pi $, the off-diagonal self-energy vanishes and the orbital Kondo problem can be exactly mapped onto the usual spin Kondo model. For a general $\phi $, the presence of the off-diagonal orbital wave function interference will modify the height and width of the orbital Kondo peak, but not change the position of the orbital Kondo peak. We also give an analytic expression of the flux-dependent Kondo temperature and find it decreases monotonously as the magnetic flux $\phi $ goes from $(2n+1)\pi $ to $2n\pi $, which means the Kondo effect is suppressed by the off-diagonal orbital interference process and becomes more easily destroyed by the thermal fluctuation. The flux-dependence conductance is also presented.
12/2006;
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ABSTRACT: We report the theoretical investigation of the orbital Kondo effect in an Aharonov-Bohm interferometer by slave-boson mean field approach. It is found that the present orbital Kondo effect can be tuned geometrically by the external magnetic flux. When the magnetic flux φ=(2n+1)π, the off-diagonal self-energy vanishes and the orbital Kondo problem can be exactly mapped onto the usual spin Kondo model. For a general φ, the presence of the off-diagonal orbital wave function interference will modify the height and width of the orbital Kondo peak, but not change the position of the orbital Kondo peak. We also give an analytic expression of the flux-dependent Kondo temperature and find it decreases monotonously as the magnetic flux φ goes from (2n+1)π to 2nπ in both symmetry and asymmetry tunnel coupling cases. This means the Kondo effect is suppressed by the off-diagonal orbital interference process and becomes more easily destroyed by the thermal fluctuation. The flux-dependence conductance is also presented.
Phys. Rev. B. 75(15).