A Fabry–Pérot interferometer (also called Fabry–Pérot resonator) is a linear optical resonator (or cavity) which consists of two highly reflecting mirrors (with some small transmissivity) and is often used as a high-resolution optical spectrometer. One exploits the fact that the transmission through such a resonator exhibits sharp resonances and is very small between those.
The spelling Fabry–Perot (without accent) is also frequently seen. Alfred Perot spelled his name with the accent, but the French civil register didn't.
The following explanations, assuming a lossless symmetric high-finesse Fabry–Pérot, help to understand its operation principles:
- A substantial circulating optical power in the resonator is possible only if the input wave has an optical frequency close to one of the resonance frequencies of the resonator.
- In resonance, the contribution of the input wave leaking through the input mirror adds constructively to the circulating wave. And, there is destructive interference for the reflected field: the input field reflected at the input mirror is canceled by the field leaking out of the resonator. Therefore, there is effectively no reflection in resonance.
- In anti-resonance, the circulating field is quite weak, and most radiation is reflected at the input mirror. The weak field leaking out of the resonator towards the input source adds constructively to the reflected field.
The resonance frequencies can often be tuned by changing the cavity length (mirror distance) with a piezo actuator. When the voltage applied to the piezo is periodically varied, e.g. with a triangular temporal shape, and the transmitted power versus time is monitored with a photodetector and an oscilloscope, the latter can directly display the optical spectrum of the incident light, provided that the spectral width is smaller than the free spectral range and the scan is slow enough to reach a quasi-stationary state of the resonator.
The following animated diagrams show how the reflected and transmitted complex amplitudes involve when the residence condition is tuned.
Both mirrors are assumed to have a reflectance of 80%. In this symmetric situation, total transmission and zero reflection are obtained in resonance.
In this asymmetric situation, the reflection does no more go to zero in resonance.
The analysis becomes more complicated if the incident light field has power in multiple spatial modes, since each of those may have a different round-trip phase shift related to the Gouy phase shift. That leads to different resonant frequencies for those peaks. In effect, the resonance peaks may be washed out, or (in cases with high finesse) one may even see multiple resonances in the transmission curve.
Strictly, a Fabry–Pérot interferometer by definition consists of two planar mirrors, but the term is frequently also used for resonators with curved mirrors. From a theoretical viewpoint, plane–plane optical resonators are special in the sense that their resonator modes extend up to the edges of the mirrors and experience some diffraction losses. However, Fabry–Pérot interferometers are usually used with input beams of much smaller diameter, which are actually not really matched to the resonator modes. For the usually small mirror spacings, where diffraction within a round trip is weak, this deviation is not very important.
Normally, Fabry–Pérot interferometers are devices with free-space light propagation between the mirrors. However, the term is sometimes also used for devices containing in a waveguide. For example, Fabry–Pérot lasers are laser diodes containing an active (amplifying) waveguide with some kind of mirrors at the ends.
A typical application of a Fabry–Pérot interferometer is to check whether a laser operates on a single resonator mode or on multiple modes. High-finesse Fabry–Pérot interferometers are also used as reference cavities and for spectral analysis.
For optical spectrum analysis, the Fabry–Pérot interferometer is often made short enough to achieve a sufficiently large free spectral range; the bandwidth of the resonances is then the free spectral range divided by the finesse. Due to the high reflectivities, the finesse can be high (well above 1000, and with supermirrors even much higher). For a given finesse, the wavelength resolution can be improved by increasing the mirror distance, but only at the cost of reducing the free spectral range, i.e., the range within which unique spectral assignment is possible.
|||C. Fabry and A. Pérot, “Théorie et applications d’une nouvelle méthode de spectroscopie interférentielle”, Ann. de Chim. et de Phys. 16 (7), 115 (1899)|
|||J. Stone and D. Marcuse, “Ultrahigh finesse fiber Fabry–Pérot interferometers”, J. Lightwave Technol. 4 (4), 382 (1986), DOI:10.1109/JLT.1986.1074739|
|||E. D. Palik, H. Boukari, and R. W. Gammon, “Experimental study of the effect of surface defects on the finesse and contrast of a Fabry–Perot interferometer”, Appl. Opt. 35 (1), 38 (1996), DOI:10.1364/AO.35.000038|
|||M. Suter and P. Dietiker, “Calculation of the finesse of an ideal Fabry–Perot resonator”, Appl. Opt. 53 (30), 7004 (2014), DOI:10.1364/AO.53.007004|
|||N. Ismail et al., “Fabry-Pérot resonator: spectral line shapes, generic and related Airy distributions, linewidths, finesses, and performance at low or frequency dependent reflectivity”, Opt. Express 24 (15), 16366 (2016), DOI:10.1364/OE.24.016366|
|||C Saavedra et al., “Tunable fiber Fabry–Perot cavities with high passive stability”, Opt. Express 29 (2), 974 (2021), DOI:10.1364/OE.412273|
|||D. Martin-Sanchez et al., “ABCD transfer matrix model of Gaussian beam propagation in Fabry-Perot etalons”, Opt. Express 30 (26), 46404 (2022), DOI:10.1364/OE.477563|
|||A. E. Siegman, Lasers, University Science Books, Mill Valley, CA (1986)|
|||J. M. Vaughan, The Fabry-Pérot Interferometer: History, Theory, Practice and Applications, CRC Press (1989)|
|||R. Paschotta, Photonics Spotlight article: The resonator mystery|
See also: Fabry–Perot laser diodes, standing-wave resonators, interferometers, spectrometers, etalons, Gires–Tournois interferometers, supermirrors, optical resonators, resonator modes, mode matching, reference cavities, free spectral range, finesse
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