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The read-out electronics for the FLASH experiment

Luigi Calligaris, Claudio Puglia, Gianluca Lamanna

Abstract

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 readout 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 into a format suitable for permanent storage and offline analysis.

The read-out electronics for the FLASH experiment

Abstract

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 W. The signal readout 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 into a format suitable for permanent storage and offline analysis.
Paper Structure (12 sections, 2 equations, 3 figures, 1 table)

This paper contains 12 sections, 2 equations, 3 figures, 1 table.

Figures (3)

  • Figure 1: (top) Exploded view of the FLASH experiment, showing its main structural components. (bottom) Schematic of the readout chain for FLASH.
  • Figure 2: (left) Schematic of a composite ADC. (center) Schematic of a zero-IF receiver. (right) Representation of downconversion of a signal in frequency space.
  • Figure 3: Always give a caption.