APS March Meeting 2017
Volume 62, Number 4
Monday–Friday, March 13–17, 2017;
New Orleans, Louisiana
Session A29: Optical Frequency Combs - Generation, Metrology & Applications
8:00 AM–11:00 AM,
Monday, March 13, 2017
Room: 292
Sponsoring
Unit:
DLS
Abstract ID: BAPS.2017.MAR.A29.5
Abstract: A29.00005 : Optical Frequency Division for Low Noise RF to W Band Signal Generation
10:24 AM–11:00 AM
Preview Abstract
Abstract
Author:
Franklyn Quinlan
(National Institute of Standards and Technology)
Modern optical frequency references have extraordinary spectral purity, with
lasers stabilized to passive optical reference cavities reaching fractional
frequency instabilities below 10$^{\mathrm{-16}}$ at 1 second, and optical
atomic clocks approaching 10$^{\mathrm{-18}}$ at 10$^{\mathrm{4}}$ seconds.
Both the short- and long-term stability providing by ultrastable optical
references can find new utility after high fidelity conversion to the
electrical domain, including precision microwave spectroscopy, navigation
and radar systems, and an optical clock-based redefinition of the SI second.
Frequency division from an optical reference at 100s of THz to RF and
microwave frequencies is performed by phase locking an optical frequency
comb to the optical reference, followed by optical-to-electrical conversion
with a high-speed photodetector. This process generates RF and microwave
carriers at the harmonics of the repetition rate of the optical frequency
comb, all of which ideally maintain the fractional stability of the optical
reference. This talk will cover the performance of current and
next-generation optical references, as well as the current and required
performance of optical frequency combs and optical-to-electrical conversion
needed to support the exquisite performance available in the optical domain.
To date, 1 second instability \textless 10$^{\mathrm{-15}}$ at 10 GHz has
been demonstrated, limited by the optical reference. Optical-to-electrical
conversion has been shown to support state-of-the-art optical references,
with added noise at a level of 10$^{\mathrm{-17}}$ at 1 second, and
\textless 10$^{\mathrm{-19}}$ at 10$^{\mathrm{3}}$ seconds. Techniques to
extend the frequency range into the millimeter-wave domain while maintaining
10$^{\mathrm{-15}}$ fractional instability, as well as arbitrary frequency
generation with sub-millihertz precision tuning, will also be discussed.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2017.MAR.A29.5