Nonlinear optics is the field of studying systems that can generate new frequencies (De Angelis 2021). In optics, this often looks like sending light of a specific frequency (ω) into a material and observing different frequencies exiting the
material. The polarization (P ) of the material can be described by a Taylor Expansion
P = ε0χ1E + ε0χ2E2 + ε0χ3E3 + ...
This relationship between the polarization and electric field determines the materials optical response to the incident light (Pedrotti et al. 2017). When a material behaves nonlinearly, the optical properties of the material, like the refractive index, can no longer be approximated as linear but become functions of the incident light's electric field (E). The nonlinear third order term produces nonlinear effects such as frequency mixing. Frequency mixing occurs when two or more frequency beams interact in the medium and produce new frequencies of 2ω1, 2ω2, ω1 + ω2, ω1 − ω2, and so on (Pedrotti et al. 2017).
It was well known in the scientific community that materials had nonlinear properties and that our description of linear behavior in materials was an approximation valid only at low light intensities. The existence of nonlinear behavior was interesting, but unexplored due to the lack of a light source with a strong enough intensity to produce these optical nonlinearities. This all changed with the invention of the laser in 1960. In 1961, Franken demonstrated second-harmonic generation for the first time using a red laser and crystalline quartz, which served as the beginning of the study of nonlinear optics (Franken et al. 1961).
Light and matter interactions are so short lived that it was difficult to stimulate efficient nonlinear optical effects. Optical waveguides, a common example of which is the optical fiber (Stolen et al. 1974), helped solve this problem by directing a light wave by total internal reflection. This greatly increased the interaction time between the light and the waveguide material. A ring resonator is an optical instrument that contains at least one straight waveguide and a ring waveguide very close together. These waveguides are commonly made of silicon due to silicon's high refractive index contrast (Bogaerts et al. 2012). When light is sent into this structure, the light travels from the straight waveguide into the ring via evanescent coupling (Mansuripur 2009). If the light is sent in at the correct wavelength, the ring will be in resonance, allowing for light intensity to grow inside the ring, instead of over an inconveniently long length of waveguide. Because the resonance of the ring is wavelength specific, any frequencies that were generated due to the nonlinear behavior of the material will not remain in resonance in the ring and instead will couple back out to the straight waveguide.
We began with ring of radius r = 3.1 um made of linear silicon nitride with a refractive index of
n = 2.11. The basic steps taken to optimize ring resonator design to see nonlinearity are:
The material of the ring resonator was then changed to nonlinear silicon nitride. A χ3 Raman Kerr material was added to the Ansys Lumerical material database with values of χ3 = 4.83686e-21 m2/V2, α = 0.957 , ωRaman = 7e+13 Hz, and δRaman = 3.125e+13 Hz. The α value controls the relative weighting between the Kerr and Raman terms. The ωRaman term is the non-linear Raman angular frequency and the δRaman term is the linewidth of the resonance. The χ3 and ωRaman values for silicon nitride are known and used, but the α and δRaman values for silicon were used.
To increase the Q factor, the radius of the ring was increased from r = 3.1 um to r = 6.0 um. This decreased bend loss in the ring, which increased the Q factor. In order to reach critical coupling, which is when 100% of incident light is coupled to the ring, the gap between the straight waveguide and the ring was increased in steps of 50 nm until the depth of the resonance dips reached a maximum, at a gap width of 0.45 um.
These nonlinear effects can create an optical frequency comb. The incredibly accurate and evenly spaced generated frequency peaks form a comb shape which can be used to measure light with extreme precision and accuracy. These optical frequency combs are helping in the search for exoplanets, improving technology for radio astronomy, and improving distance measurements in lidar. The next hurdle for frequency combs is shrinking them to microchip size, something that microring resonators could make possible.2,3
[1] C. Krückel, A. Fülöp, T. Klintberg, J. Bengtsson, P. Andrekson, and V. Torres-Company, "Linear and nonlinear characterization of low-stress high-confinement silicon-rich nitride waveguides," Opt. Express 23, 25827-25837 (2015).
[2] R. McCracken, J. Charsley, and D. Reid, "A decade of astrocombs: recent advances in frequency combs for astronomy [Invited]," Opt. Express 25, 15058-15078 (2017).
[3] Optical frequency combs. NIST. (2022, April 5). https://www.nist.gov/topics/physics/optical-frequency-combs
My name is Emma VanderKooi and I am a rising junior at Wheaton College as a Physics major and Math minor. I am interested in astrophysics and astronomy, and in addition to classes I enjoy working as Lead TA of my school's observatory! This summer I worked with Dr. Hooman Mohseni's lab at Northwestern University's McCormick School of Engineering to simulate nonlinear optical behavior in silicon nitride ring resonators. Apart from doing research, I love watching soccer, reading, and spending time with my friends and family!
Contact: emma.vanderkooi@my.wheaton.edu or LinkedIn