We introduce the FLASH haloscope experiment and present its electronic read-out system, currently under development. FLASH searches for Dark Matter (DM) particles and High-Frequency Gravitational Waves (HFGWs) using two cryogenic resonant cavities to scan the radio frequency spectrum between 117 and 360 MHz, looking for signals as weak as 10-22 W. The signal read-out uses Microstrip Superconducting Quantum Interference Amplifiers (MSAs) as low-noise amplifiers and Software-Defined Radio (SDR) techniques to acquire, preprocess and reduce the physics signal to a format suitable for permanent storage and offline analysis.
@article{arxiv.2603.23846,
title = {The read-out electronics for the FLASH experiment},
author = {Luigi Calligaris and Claudio Puglia and Gianluca Lamanna},
journal= {arXiv preprint arXiv:2603.23846},
year = {2026}
}
Comments
Proceedings of the 2025 Topical Workshop on Electronics for Particle Physics (TWEPP2025), Rethymno, Greece, 6-10 October 2025