A haloscope amplification chain based on a traveling wave parametric amplifier.

Caterina Braggio1, Giulio Cappelli2, Giovanni Carugno3

  • 1Dip. di Fisica e Astronomia, Università di Padova, 35100 Padova, Italy.

Summary

We characterized a radio frequency (RF) amplification chain for dark matter axion searches. The system achieved a low system noise temperature of 3.3 K, crucial for sensitive detection experiments.

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