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• W3150819931 abstract "Magnetic impurities in a superconductor induce Yu-Shiba-Rusinov (YSR) states inside the superconducting gap, whose energy depends on the strength of the coupling to the impurity and on the density of states (DOS) at the Fermi level. We consider DOS exhibiting a logarithmic or a power-law divergence at the Fermi level due to Van Hove singularities (VHS) and high-order Van Hove singularities (HOVHS), respectively. We find that the energy of the YSR states has the same functional form as in the constant DOS scenario, with the effect of the singularity being an enhancement of the effective coupling constants. In particular, the critical magnetic coupling strength at which the Shiba transition occurs is always lowered by a factor $1/rho(Delta/E_{mathrm{c}}$), where $Delta$ is the superconducting gap, $E_{mathrm{c}}$ is the bandwidth, and $rho(E)$ is the factor in DOS which diverges at $E=0$ for a VHS or HOVHS. Further, since the critical magnetic coupling is significantly reduced, a new regime becomes accessible where the transition point is controlled by the non-magnetic coupling constant. Interestingly, the slope of the Shiba energy curve at the Shiba transition is independent of impurity parameters and purely reflects the band structure. Additionally, we find that our main conclusions remain valid even when the Fermi level is not precisely tuned to the Van Hove singularity, but instead lies on an energy range of order the superconducting gap. Our results show that tuning a superconducting material towards a VHS or HOVHS enhances the possibilities for engineering YSR states, and for characterizing the superconductor itself." @default.
• W3150819931 created "2021-04-13" @default.
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• W3150819931 date "2021-06-17" @default.
• W3150819931 modified "2023-10-18" @default.
• W3150819931 title "Effect of Van Hove singularities on Shiba states in two-dimensional<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mi>s</mml:mi></mml:math>-wave superconductors" @default.
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• W3150819931 doi "https://doi.org/10.1103/physrevb.103.214514" @default.
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