# Pinning effects on hot-electron vortex flow instability in   superconducting films

**Authors:** Valerij A. Shklovskij

arXiv: 1704.04168 · 2017-05-23

## TL;DR

This paper theoretically investigates how pinning affects the hot-electron vortex flow instability in superconducting films under magnetic fields, revealing monotonic and non-monotonic behaviors of critical parameters and their dependence on pinning potential.

## Contribution

It extends previous models by including pinning effects, deriving magnetic field dependencies of critical parameters, and explaining experimental observations of vortex velocity behavior.

## Key findings

- Critical parameters depend on pinning potential type.
- Vortex velocity can change its magnetic field dependence sign.
- Instability temperature is approximately 5/6 of T_c, independent of B.

## Abstract

The hot-electron vortex flow instability in superconducting films in magnetic field $B$ at substrate temperature $T_0 \ll T_c$ is theoretically considered in the presence of pinning. The magnetic field dependence of the instability critical parameters (electric field $E^\ast$, current density $j^\ast$, resistivity $\rho^\ast$, power density $P^\ast$ and vortex velocity $v^\ast$) is derived for a cosine and a saw-tooth washboard pinning potential and compared with the results obtained earlier by M.\,Kunchur [Phys. Rev. Lett. \textbf{89} (2002) 137005] in the absence of pinning. It is shown that the $B$-behavior of $E^\ast$, $j^\ast$ and $\rho^\ast$ is monotonic in $B$, whereas the $B$-dependence of $v^\ast$ is quite different, namely $dv^\ast/dB$ may change its sign twice with decreasing $B$ as it was observed in some experiments. The simplest heat balance equation for electrons in low-$T_c$ superconducting films in the two-fluid approach is considered. It allows one to show that the instability critical temperature $T^\ast \approx 5T_c/6$ at $T_0 < T^\ast/2$ with $T^\ast$ independent of $B$.

## Full text

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## Figures

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## References

44 references — full list in the complete paper: https://tomesphere.com/paper/1704.04168/full.md

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Source: https://tomesphere.com/paper/1704.04168