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Secondary 'Smile'-gap in the density of states of a diffusive Josephson junction for a wide range of contact types

Authors :
Reutlinger, J.
Glazman, L.
Nazarov, Yu. V.
Belzig, W.
Source :
Phys. Rev. B 90, 014521 (2014)
Publication Year :
2014

Abstract

The superconducting proximity effect leads to strong modifications of the local density of states in diffusive or chaotic cavity Josephson junctions, which displays a phase-dependent energy gap around the Fermi energy. The so-called minigap of the order of the Thouless energy $E_{\mathrm{Th}}$ is related to the inverse dwell time in the diffusive region in the limit $E_{\mathrm{Th}}\ll\Delta$, where $\Delta$ is the superconducting energy gap. In the opposite limit of a large Thouless energy $E_{\mathrm{Th}}\gg\Delta$, a small new feature has recently attracted attention, namely, the appearance of a further secondary gap, which is around two orders of magnitude smaller compared to the usual superconducting gap. It appears in a chaotic cavity just below the superconducting gap edge $\Delta$ and vanishes for some value of the phase difference between the superconductors. We extend previous theory restricted to a normal cavity connected to two superconductors through ballistic contacts to a wider range of contact types. We show that the existence of the secondary gap is not limited to ballistic contacts, but is a more general property of such systems. Furthermore, we derive a criterion which directly relates the existence of a secondary gap to the presence of small transmission eigenvalues of the contacts. For generic continuous distributions of transmission eigenvalues of the contacts, no secondary gap exists, although we observe a singular behavior of the density of states at $\Delta$. Finally, we provide a simple one-dimensional scattering model which is able to explain the characteristic "smile" shape of the secondary gap.<br />Comment: 12 pages, 12 figures

Details

Database :
arXiv
Journal :
Phys. Rev. B 90, 014521 (2014)
Publication Type :
Report
Accession number :
edsarx.1406.6797
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevB.90.014521