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Published November 20, 2024 | Published
Journal Article Open

Photonic millimeter-wave generation beyond the cavity thermal limit

Abstract

Next-generation communications, radar, and navigation systems will extend and exploit the higher bandwidth of the millimeter-wave domain for increased communication data rates as well as radar with higher sensitivity and increased spatial resolution. However, realizing these advantages will require the generation of millimeter-wave signals with low phase noise in simple and compact form-factors. Photonic integration addresses this challenge and provides a path toward simplified and portable, low-noise mm-wave generation. We leverage these advances by heterodyning two silicon photonic chip lasers, phase-locked to different axial modes of a miniature Fabry–Perot (F-P) cavity to demonstrate a simple framework for generating low-noise millimeter-waves. By reducing technical noise, we achieve common-mode rejection of the thermally driven Brownian noise such that the millimeter-wave phase noise surpasses that of the thermal limit of a single laser locked to the F-P cavity. This leads to a 118.1 GHz millimeter-wave signal with phase noise of −118dBc/Hz at 10 kHz offset, decreasing to −120dBc/Hz at 30 kHz offset. We achieve this with technologies that can be integrated into a platform less than ≈10mL. Our work overcomes fundamental thermal-mechanical noise limits intrinsic to integrated photonics, while illustrating advantages of the same for providing low-size, -weight, and -power (SWaP) mm-waves that will be enabling for multiple applications in communications and sensing.

Copyright and License

© 2024 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement.

Acknowledgement

W.G., I.K., K.J.V, J.E.B., F.Q., and S.A.D. conceived the experiment and supervised the project. W.G., I.K., and S.A.D. wrote the paper with input from all authors. W.G., I.K., and A.L. built the experiment and performed the mm-wave experiment. D.L., T.N., and Y.L. provided mm-wave reference sources and input regarding the cavity and cross-correlation measurements. M.L.K and C.A.M. built the cavity and provided information regarding the cavity. J.G., L.W., W.J., K.J.V, and J.E.B provided the lasers and spiral microresonators, as well as input regarding the operation of the lasers.

Funding

National Institute of Standards and Technology (80NM0018D0004); Defense Advanced Research Projects Agency GRYPHON program (HR0011-22-2-0009).

Conflict of Interest

The authors declare no conflicts of interest. Commercial equipment and trade names are identified for scientific clarity only and do not represent an endorsement by NIST.

Data Availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

Supplemental Material

Supplemental document (PDF).

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Additional details

Created:
November 26, 2024
Modified:
November 26, 2024