# Quench spot detection for superconducting accelerator cavities via flow visualization in superfluid helium-4

## TL;DR

This paper introduces a novel method for detecting quench spots on superconducting accelerator cavities by visualizing heat transfer in superfluid helium-4 using tracer lines, offering improved localization over existing techniques.

## Contribution

The study presents a new visualization technique using He$_2^*$ tracer lines to detect quench spots, demonstrating feasibility with a proof-of-concept experiment and analyzing heat transfer mechanisms.

## Key findings

- Tracer line deformation accurately locates heater within a few hundred microns
- Heat transfer in He II involves only a small fraction of the input energy
- Cavitation zone formation near the heater explains long-standing experimental puzzles

## Abstract

Superconducting ratio-frequency (SRF) cavities, cooled by superfluid helium-4 (He II), are key components in modern particle accelerators. Quenches in SRF cavities caused by Joule heating from local surface defects can severely limit the maximum achievable accelerating field. Existing methods for quench spot detection include temperature mapping and second-sound triangulation. These methods are useful but all have known limitations. Here we describe a new method for surface quench spot detection by visualizing the heat transfer in He II via tracking He$_2^*$ molecular tracer lines. A proof-of-concept experiment has been conducted, in which a miniature heater mounted on a plate was pulsed on to simulate a surface quench spot. A He$_2^*$ tracer line created nearby the heater deforms due to the counterflow heat transfer in He II. By analyzing the tracer-line deformation, we can well reproduce the heater location within a few hundred microns, which clearly demonstrates the feasibility of this new technology. Our analysis also reveals that the heat content transported in He II is only a small fraction of the total input heat energy. We show that the remaining energy is essentially consumed in the formation of a cavitation zone near the heater. By estimating the size of this cavitation zone, we discuss how the existence of the cavitation zone may explain a decades-long puzzle observed in many second-sound triangulation experiments.