Skip to main content
U.S. flag

An official website of the United States government

Official websites use .gov
A .gov website belongs to an official government organization in the United States.

Secure .gov websites use HTTPS
A lock ( ) or https:// means you’ve safely connected to the .gov website. Share sensitive information only on official, secure websites.

Scientists Greatly Expand the Frequencies Generated by a Miniature Optical Ruler

Wider range of a frequency comb on a chip may lead to better detectors of greenhouse gases and enhance global navigation systems.

Like a vocal coach who extends the octave range of an opera singer, researchers at the National Institute of Standards and Technology (NIST) have expanded by nearly two-thirds the frequency range over which a chip-scale device can generate and measure the oscillations of light waves with exquisite accuracy. The expanded range of the system, known as a microring resonator frequency comb, or microcomb, could lead to better sensors of greenhouse gases and may also improve global navigation systems.

Gregory Moille and his colleagues at NIST, including team leader Kartik Srinivasan, along with collaborators at the Joint Quantum Institute (a NIST-University of Maryland research partnership) and the University of Maryland, reported their findings in the December 14, 2021 issue of Nature Communications.

A frequency comb acts like the optical version of a ruler. Just as a ruler, divided into hundreds of tick marks spaced a known distance apart, measures an object of unknown length, a frequency comb features hundreds of different ultrasharp, uniformly spaced frequency spikes to precisely measure light of an unknown frequency (The tool is so named because the frequency spikes resemble the teeth of a comb.)

Expanding a Microring Resonator Frequency Comb
Expanding a Microring Resonator Frequency Comb
By using two lasers instead of one, NIST researchers have developed a method for nearly doubling the range of the frequency comb generated by a microring resonator. Credit: S. Kelley/NIST

Over the past two decades, scientists at NIST and other research institutions have shown that microcombs can play an important role in building highly accurate optical clocks, calibrating detectors that analyze starlight to search for planets beyond the solar system, and detecting trace gases in the environment.

One type of microcomb extensively studied at NIST consists of a miniature, rectangular waveguide--a channel that confines light waves--coupled to a ring-shaped resonator about 50 micrometers (millionths of a meter) in diameter. Laser light injected into the waveguide enters the microring resonator and races around the ring.

Ordinarily, the circulating light begins to vary in amplitude and can form different patterns. However, by carefully adjusting the laser, the light within the microring forms a soliton--a solitary wave pulse that preserves its shape as it moves around the ring.

Each time the soliton completes one roundtrip around the microring, a portion of the pulse splits off and enters the waveguide. Soon, an entire train of wave pulses fills the waveguide, with each wave separated in time from its neighbor by the same fixed interval—the time it took for the soliton to complete one lap around the microring. The train of wave pulses in the waveguide corresponds to a single set of evenly spaced frequencies and forms the teeth of the frequency comb. The number and amplitude of the teeth are primarily determined by the size and composition of the ring and the power and frequency of the laser.

Recently, the NIST scientists wondered what would happen if they produced a microcomb using two lasers, each generating a different frequency of light, instead of just one. They found that through a complex series of interactions with the soliton light circulating in the microring resonator, the second laser induced two new sets of teeth, or evenly spaced frequencies, that are replicas of the original set of teeth but shifted to higher and lower frequencies. The lower frequency set lies in the infrared part of the spectrum, while the other is at a much higher frequency, close to visible light. The comb also retains its original teeth, at near-infrared frequencies.

The extended range of the microcomb enables a host of applications at different frequencies. The system is the first time that researchers have produced a stable microcomb that ties together such a wide range of frequencies of light, Srinivasan said.

In addition, the team discovered that by varying the frequency of the second laser, the new sets of teeth could be easily shifted to higher or lower frequencies independent of the shape or composition of the microring resonator. This makes the system extremely versatile.

The feat may enable a single microcomb to measure the characteristic vibrations of atoms and molecules, including pollutants, that both emit and absorb light over a broad range of frequencies, thus enhancing the sensitivity of detectors.

The broader coverage could also help subsequent efforts to stabilize the microcomb, so that its tick marks remain fixed rather than wander slightly from their original set of colors. The enhanced stability may spur the development of portable optical atomic clocks accurate enough to be employed outside the laboratory, leading to more accurate and precise navigation systems, said Moille.


Paper: Gregory Moille, Edgar F. Perez, Jordan R. Stone, Ashutosh Rao, Xiyuan Lu, Tahmid Sami Rahman, Yanne K. Chembo & Kartik Srinivasan. Ultra-broadband Kerr microcomb through soliton spectral translation. Nature Communications volume 12, Article number: 7275, Published online in the December 14, 2021 issue. DOI: https://doi.org/10.1038/s41467-021-27469-0

Released February 23, 2022, Updated March 8, 2022