Next Generation Ta-STJ Sensor Arrays for BSM Physics Searches
Joseph P. T. Templet, Spencer Fretwell, Andrew Marino, Robin Cantor, Ad Hall, Connor Bray, Caitlyn Stone-Whitehead, Inwook Kim, Francisco Ponce, Wouter Van De Pontseele, Kyle G. Leach, Stephan Friedrich
TL;DR
The paper addresses calibration artifacts in BeEST Be-7 recoil spectroscopy using superconducting tunnel junctions. It identifies resistive crosstalk from shared ground wiring and substrate-absorption of calibration photons as the main sources of systematic errors and demonstrates design and operation changes to mitigate them. By implementing per-pixel ground wires and employing a more stable, collimated UV laser, the BeEST collaboration achieved robust energy resolution in the $1$–$2$ eV range below $100$ eV and suppressed the phase-III calibration artifacts, enabling more reliable searches for BSM neutrinos in Phase-IV and related experiments like SALER at FRIB. These improvements have clear practical impact for precision recoil spectroscopy and rare-process studies using STJ sensors, with potential for further gains through improved laser collimation.
Abstract
The Beryllium Electron capture in Superconducting Tunnel junctions (BeEST) experiment uses superconducting tunnel junction (STJ) sensors to search for physics beyond the standard model (BSM) with recoil spectroscopy of the $\mathbf{^7}$Be EC decay into $\mathbf{^7}$Li. A pulsed UV laser is used to calibrate the STJs throughout the experiment with $\sim$20 meV precision. Phase-III of the BeEST experiment revealed a systematic calibration discrepancy between STJs. We found these artifacts to be caused by resistive crosstalk and by intensity variations of the calibration laser. For phase-IV of the BeEST experiment, we have removed the crosstalk by designing the STJ array so that each pixel has its own ground wire. We now also use a more stable UV laser for calibration. The new STJ arrays were fabricated at STAR Cryoelectronics and tested at LLNL and FRIB. They have the same high energy resolution of $\sim$1\textendash2~eV in the energy range of interest below 100~eV as before, and they no longer exhibit the earlier calibration artifacts. We discuss the design changes and the STJ array performance for the next phase of the BeEST experiment.
