An ultralow phase noise 300 GHz wave based on optical frequency division via an integrated dissipative Kerr soliton comb

Tomohiro Tetsumoto; Tadao Nagatsuma; Martin E. Fermann; Gabriele Navickaite; Michael Geiselmann; Antoine Rolland

doi:10.1364/CLEO_SI.2021.STu2D.3

Conference on Lasers and Electro-Optics
OSA Technical Digest (Optica Publishing Group, 2021),
paper STu2D.3
•https://doi.org/10.1364/CLEO_SI.2021.STu2D.3

An ultralow phase noise 300 GHz wave based on optical frequency division via an integrated dissipative Kerr soliton comb

Tomohiro Tetsumoto, Tadao Nagatsuma, Martin E. Fermann, Gabriele Navickaite, Michael Geiselmann, and Antoine Rolland

CLEO: Science and Innovations 2021

San Jose, California United States
9–14 May 2021
ISBN: 978-1-943580-91-0

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Low Noise Optical and Microwave Sources (STu2D)

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T. Tetsumoto, T. Nagatsuma, M. E. Fermann, G. Navickaite, M. Geiselmann, and A. Rolland, "An ultralow phase noise 300 GHz wave based on optical frequency division via an integrated dissipative Kerr soliton comb," in Conference on Lasers and Electro-Optics, J. Kang, S. Tomasulo, I. Ilev, D. Müller, N. Litchinitser, S. Polyakov, V. Podolskiy, J. Nunn, C. Dorrer, T. Fortier, Q. Gan, and C. Saraceno, eds., OSA Technical Digest (Optica Publishing Group, 2021), paper STu2D.3.

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Abstract

We demonstrate low phase noise 300 GHz wave generation through optical frequency division using an integrated dissipative Kerr soliton. The obtained phase noise at 10 kHz Fourier frequency, measured with a devised system, is -100 dBc/Hz.

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