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Updated: Aug 27, 2025

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Quantum State Engineering of Light with Continuous-wave Optical Parametric Oscillators
Published on: May 30, 2014
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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.
The Review of Scientific Instruments
|October 1, 2022
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.
Area of Science:
- * Experimental physics
- * Astrophysics
- * Particle physics
Background:
- * Dark matter axion searches require highly sensitive detection systems.
- * Traveling wave parametric amplifiers offer potential for low-noise radio frequency (RF) amplification.
- * High Q microwave resonant cavities are essential for detecting axions.
Purpose of the Study:
- * To characterize an RF amplification chain for dark matter axion detection.
- * To evaluate the performance of a traveling wave parametric amplifier in this context.
- * To measure the system noise temperature at the cavity output port.
Main Methods:
- * Development and characterization of an RF amplification chain.
- * Coupling the amplification chain to a high Q microwave resonant cavity.
- * Implementation of a novel calibration scheme for system noise temperature measurement.
Main Results:
- * Successful characterization of the RF amplification chain.
- * Measurement of a system noise temperature (Tsys) of (3.3 ± 0.1) K at 10.77 GHz.
- * Validation of a novel calibration scheme enabling precise Tsys measurement at the cavity output.
Conclusions:
- * The developed RF amplification chain is suitable for dark matter axion searches.
- * The low system noise temperature achieved is a significant advancement for sensitive experiments.
- * The novel calibration technique enhances the reliability of noise temperature measurements.
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