Orbital Kondo effect modulated by off-diagonal orbital interference

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.