Low-noise microwave generation with an air-gap optical reference cavity

Author:

Liu Yifan12ORCID,Lee Dahyeon12ORCID,Nakamura Takuma12ORCID,Jin Naijun3,Cheng Haotian3ORCID,Kelleher Megan L.12ORCID,McLemore Charles A.12ORCID,Kudelin Igor12,Groman William12ORCID,Diddams Scott A.124ORCID,Rakich Peter T.3,Quinlan Franklyn24ORCID

Affiliation:

1. Department of Physics, University of Colorado Boulder 1 , Boulder, Colorado 80309, USA

2. Time and Frequency Division, National Institute of Standards and Technology 2 , Boulder, Colorado 80305, USA

3. Department of Applied Physics, Yale University 3 , New Haven, Connecticut 06520, USA

4. Electrical, Computer and Energy Engineering, University of Colorado Boulder 4 , Boulder, Colorado 80309, USA

Abstract

We demonstrate a high finesse, microfabricated mirror-based, air-gap cavity with volume less than 1 ml, constructed in an array, that can support low-noise microwave generation through optical frequency division. We use the air-gap cavity in conjunction with a 10 nm bandwidth mode-locked laser to generate low phase noise 10 GHz microwaves, exhibiting a phase noise of −95 and −142 dBc/Hz at 100 Hz and 10 kHz offset frequencies, respectively. This is accomplished using the 2-point lock optical frequency division method, where we exploit 40 dB common-mode rejection of two lasers separated by 1.29 THz and locked to the same air-gap cavity. If used with an octave spanning comb, the air-gap cavity is capable of supporting 10 GHz phase noise below −160 dBc/Hz at 10 kHz offset, a level significantly lower than electronic synthesizers. These results show how extremely small optical reference cavities, operated without the benefit of vacuum enclosures or thermal insulation, can, nonetheless, support state-of-the-art microwave phase noise in compact and portable systems.

Funder

National Institute of Standards and Technology

Defense Advanced Research Projects Agency

Publisher

AIP Publishing

Subject

Computer Networks and Communications,Atomic and Molecular Physics, and Optics

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