|<<< | >>> | Feedback|
The ideal place to find suppliers for photonics products: high-quality information, simple and fast, and respects your privacy!
4 suppliers for Gires-Tournois interferometers are listed.
You are not yet listed? Get your entry!
Ask RP Photonics for advice on how to design a Gires–Tournois interferometer or a different kind of dispersion-compensating device.
Definition: linear optical resonators used for introducing chromatic dispersion
A Gires–Tournois interferometer is an optical standing-wave resonator similar to Fabry–Pérot interferometer, which however is operated in reflection and designed for generating chromatic dispersion. The front mirror is partially reflective, whereas the back mirror has a high reflectivity. If no losses occur in the resonator, the power reflectivity is unity at all wavelengths, but the phase of the reflected light is frequency-dependent due to the resonance effect, causing chromatic dispersion. The phase change of reflected light and the dispersion (including group delay dispersion and higher-order dispersion) change periodically with optical frequency, if material dispersion is negligible. There is no second-order dispersion exactly on-resonance or anti-resonance, and positive or negative dispersion between these points.
Ideally, the GTI is operated near a maximum or minimum of the GDD, and the usable bandwidth is some fraction (e.g. one-tenth) of the free spectral range, which is inversely proportional to the resonator length. In the time domain, this means that the pulse duration needs to be well above the round-trip time of the GTI. The maximum magnitude of GDD scales with the square of the resonator length.
Tunable dispersion can be obtained with a variable air gap between the mirrors, which however must be carefully stabilized to avoid unwanted drifts. More stable but in general not tunable GDD can be generated with monolithic designs, based e.g. on thin films of dielectric media such as TiO2 and SiO2, particularly for use in femtosecond lasers.
The main drawbacks of the GTI are the fundamentally limited bandwidth (proportional to the square root of the given magnitude of GDD) and the limited amount of control of higher-order dispersion. Dispersive mirrors with significantly broader optical bandwidth can be designed as chirped mirrors.
|||F. Gires and P. Tournois, “Interferometre utilisable pour la compression d'impulsions lumineuses modulees en frequence”, C. R. Acad. Sci. Paris 258, 6112 (1964)|
|||B. Golubovic et al., “Double Gires–Tournois interferometer negative-dispersion mirrors for use in tunable mode-locked lasers”, Opt. Lett. 25 (4), 275 (2000)|
|||Analysis of a GTI with the RP Coating software|
See also: interferometers, Fabry–Perot interferometers, chromatic dispersion, dispersion compensation, dispersive mirrors, optical resonators
and other articles in the categories photonic devices, light pulses, optical resonators
How do you rate this article?
If you like this article, share it with your friends and colleagues, e.g. via social media: