Magnetic landscape of NbTiN superconducting resonators under radio-frequency excitation

TL;DR

This study visualizes magnetic flux penetration in NbTiN superconducting resonators under RF excitation, revealing how flux avalanches affect device performance and providing insights to enhance their stability.

Contribution

First direct visualization of flux avalanches in superconducting resonators under RF excitation, linking flux events to resonance shifts and advancing understanding of magnetic effects.

Findings

Flux avalanches weakly depend on RF intensity within linear regime

Magnetic flux bursts influence RF transmission and resonance frequency

Flux events correlate with specific shifts in resonance frequency

Abstract

Planar superconducting resonators are essential components in quantum circuits and highly sensitive sensors. However, their performance is often compromised by magnetic flux penetration, as the interaction of flux quanta and the induced radio-frequency (RF) currents in the superconducting thin film leads to significant energy dissipation. At low operating temperatures, this issue is aggravated as thermomagnetic instabilities can trigger the sudden propagation of magnetic flux avalanches. An important open question is whether the RF excitation itself stimulates the nucleation and propagation of magnetic flux avalanches in the superconducting thin film. The literature remains inconclusive on this point, partly due to the lack of compelling evidence for this phenomenon. In this work, we address this issue by unprecedented direct visualization of magnetic flux penetration through Faraday rotation imaging under simultaneous RF excitation. We demonstrate that the avalanche activity exhibits a weak dependence on the RF intensity for RF excitations within the linear Campbell regime. However, magnetic flux bursts clearly influence the RF transmission properties of the device. Furthermore, it is possible to unambiguously associate a particular avalanche event with a jump in resonance frequency. This enables us to identify the loci of most deleterious events and understand the distinct origins of upward and downward frequency shifts. These observations are supported by electromagnetic simulations in which local changes of the kinetic inductance mimic flux avalanches and confirm the invasive character of the MOI technique. The insights gained from this study aim to contribute to the broader understanding of the magnetic resilience of superconducting resonators, with the goal of improving their efficiency and stability.