Microwave Signature of the Emerging Abrikosov Lattice Above $H_{c2}$
Hang Zhou, Zhanghai Chen, A. A. Varlamov, Andreas Glatz, Yuriy Yerin
TL;DR
This work predicts a microwave-scale electromagnetic signature of emergent Abrikosov vortex precursors in the normal state above the upper critical field $H_{c2}$, arising from quantum fluctuations of fluctuating Cooper pairs. By developing a microscopic diagrammatic framework in a magnetic field and exploiting the Lowest Landau Level limit near $H_{c2}$, the authors show that the ac conductivity acquires a pronounced imaginary component at a characteristic frequency $\omega_{QF} \sim \hbar^{-1} \Delta (H-H_{c2})/H_{c2}$, much smaller than the superconducting energy scale. The dominant fluctuation contributions come from the Aslamazov-Larkin and anomalous Maki–Thompson processes, while DOS-related diagrams largely cancel, yielding a measurable inductive signature in the microwave range (e.g., ~0.1–1 GHz for Nb). This provides a practical route to detect vortex-formation precursors via microwave spectroscopy, offering a direct probe of quantum fluctuations in type-II superconductors. The results bridge fluctuation theory with high-frequency experiments, suggesting concrete experimental tests in Nb-based films using modern microwave resonators.
Abstract
The emergence of the Abrikosov lattice in the normal phase of type-II superconducting films when the magnetic field approaches the critical field $H_{c2}$ from above was predicted in Ref.~\cite{GVV2011}. In the quantum fluctuation regime \cite{GL2001} it is characterized by the formation of relatively large (with sizes of order $ξ_{\mathrm{QF}} \sim ξ_{\mathrm{BCS}}\sqrt{H_{c2}/(H-H_{c2})}$) ``long lived'' (lifetime of order $τ_{\mathrm{QF}} \sim \hbar Δ^{-1} H_{c2}/(H-H_{c2})$) clusters of rotating fluctuation Cooper pairs - signatures of developing Abrikosov vortices. We demonstrate that these fluctuation-induced vortex clusters, previously considered unobservable due to their ultrafast dynamics and weak (only logarithmically singular) contribution to the dc-conductivity, can in fact be detected through their distinct electromagnetic signature. By analyzing the high-frequency electromagnetic response of these rotating fluctuation Cooper pairs above the second critical field in superconducting film, we predict a pronounced and measurable enhancement in the imaginary part of the ac-conductivity arising directly from quantum fluctuations. This enhancement is expected to occur at characteristic frequencies $ω_{QF} \sim \hbar^{-1}Δ(H-H_{c2})/H_{c2}$, which are well below the superconducting threshold at $2\hbar^{-1}Δ$, where a similar increase in imaginary conductivity occurs in the superconducting phase. For niobium, a prototypical type II superconductor, $ω_{QF}$ lies in the experimentally accessible microwave range, making the effect directly testable with modern microwave spectroscopy.
