Abstract
The Fabry-Perot interferometer (Fig. 1.1) is perhaps the most deceptively simple setup in optics. In an idealised form it consists of two spherical or plane partially reflective surfaces facing each other and separated by a fixed or variable distance.
These are some of the things that hydrogen atoms do, given fifteen billion years of cosmic evolution.
—Carl Sagan.
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Notes
- 1.
The Fabry-Perot interferometer was conceived as a parallel plate interferometer. It was not until the late 1950’s that interferometry using spherical surfaces was introduced.
- 2.
Perot A and Fabry Ch 1899, Sur l’application de phénomènes d’interférence à la solution de divers problèmes de spectroscopie et de mètrologie. ‘Bull. Astronomique 16:5−32’.
- 3.
Fabry Ch and Perot A 1899, Théorie et applications d’une nouvelle méthode de spectroscopie interférentielle, Ann. Chim. Phys. 16:115−44.
- 4.
Perot A and Fabry Ch 1899, Méthodes interférentielles pour la mesure des grandes épaisseurs et la comparaison des longueurs d’onde, Ann. Chim. Phys. 16:289−338.
- 5.
Fabry Ch and Perot A 1897, Sur les franges des lames minces argentées et leur application à la mesure de petites épaisseurs d’air, Ann. Chim. Phis. 12:459−501.
- 6.
Perot A and Fabry Ch 1901, Sur un nouveau modèle d’interféromètre, Ann. Chim. Phys. 22.
- 7.
Connes P 1958, L’étalon Fabry-Perot sphérique, J. Phys. Radium 19:262−9.
- 8.
Metrology is the science of measurement, encompassing several fields across physics, mathematics and chemistry. It deals with the establishment of units of measurement, as well as the development of the measurement methods and standards of measurement.
- 9.
Gouy L G 1890, Sur une propriete nouvelle des ondes lumineuses, C. R. Acad. Sci. Paris 110:1251.
- 10.
For a variable with zero mean \((\Delta x)^2 = \left\langle x^2\right\rangle \).
- 11.
We can recast other parameters in terms of q(z). For example, \(w^2(z) = \frac{\lambda }{\pi } \frac{\left| q(z) \right| ^2}{\mathrm {Im}\left[ q(z) \right] } \), \( R(z) = \frac{\left| q(z) \right| ^2}{ \mathrm {Re}\left[ q(z) \right] } \), \( \zeta (z) = \arctan \left( \frac{\mathrm {Re}\left[ q(z) \right] }{\mathrm {Im}\left[ q(z) \right] } \right) \), \( w_0^2 = \frac{\lambda }{\pi } \mathrm {Im}\left[ q(z) \right] \).
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Álvarez, M.D. (2019). Introduction to Optical Cavities, Atomic Clocks, Cold Atoms and Gravitational Waves. In: Optical Cavities for Optical Atomic Clocks, Atom Interferometry and Gravitational-Wave Detection. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-20863-9_1
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