16–20 Oct 2023
Kingscliff, NSW, Australia
Australia/Sydney timezone

Low-phase Noise Sapphire Oscillators with Improved Frequency Stability

19 Oct 2023, 09:00
30m
Kingscliff, NSW, Australia

Kingscliff, NSW, Australia

Mantra on Salt Beach Kingscliff, Tweed Coast Gunnamatta Avenue, Kingscliff NSW
Invited Oral Precision and Low Noise Signal Generation and Techniques Microwave Clocks and Oscillators

Speaker

Eugene N. Ivanov (Quantum Technologies and Dark Matter Labs, Department of Physics, University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia.)

Description

We show that low-phase noise and high-frequency stability can be simultaneously achieved in microwave sapphire oscillators. We describe the 9 GHz sapphire oscillator with interferometric signal processing, which was phase-locked to a stable RF reference by controlling microwave power dissipated in the sapphire resonator. The SSB phase noise of the oscillator was measured to be close to -170 dBc/Hz at Fourier frequency F = 10 kHz [1]. The fractional instability of the oscillator frequency was approximately 2x10^{-13} for integration times from 5 to 50 s.

The use of cryogenic sapphire resonators promises significant improvements in the phase noise performance of microwave oscillators [2]. Yet, serious attention must be paid to the noise mechanisms affecting the cryogenic resonators. The vibrations induced by cryocoolers and power-to-frequency conversion in the sapphire resonator are expected to be the leading causes of the oscillator's excess phase noise. In our recent experiments, we measured the power-to-frequency conversion of the cryogenic sapphire resonator as a function of Fourier frequency. We found that the resonator response to the fast variations of dissipated microwave power is similar to the transfer function of the 1st-order low-pass filter with corner frequency close to the resonator's loaded bandwidth [3]. The measurements were performed with three almost identical resonators cooled to 6 K and excited in the same whispering gallery mode with a resonant frequency near 11.2 GHz. Having measured the cryogenic sapphire resonator's power-to-frequency conversion, we predicted the phase noise spectrum of the cryogenic sapphire oscillator.
References
1. E. N. Ivanov and M. Tobar, “Low Phase Noise Sapphire Crystal Microwave Oscillators: Current Status”, IEEE Trans. on UFFC, v. 56, no.2, pp.263-269, 2009.
2. E. Ivanov and M. Tobar, “Noise Suppression with Cryogenic Resonators,” Microwave and Wireless Components Letters, vol. 31, Issue 4, pp. 405-408, April 2021, DOI: 10.1109/LMWC.2021.3059291, Print ISSN: 1531-1309, Online ISSN: 1558-1764
3. E. Ivanov and M. Tobar, “Power-to-Frequency Conversion in Cryogenic Sapphire Resonators,” Microwave and Wireless Components Letters, page(s): 1-4, Print ISSN: 2771-957X. Online ISSN: 2771-9588, Digital Object Identifier: 10.1109/LMWT.2023.3264975

Primary author

Eugene N. Ivanov (Quantum Technologies and Dark Matter Labs, Department of Physics, University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia.)

Co-author

Presentation materials