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$\mathcal{F}= \dfrac{\pi (R_1 R_2)^{1/4}}{1 - \sqrt{R_1 R_2}}$
$\tau_p = \dfrac{2L/c}{-\ln\sqrt{R_1 R_2} + L_i}$
$z_R = \dfrac{\pi w_0^2}{\lambda}$
Tune cavity length, mirror reflectivity, loss, and wavelength to compute FSR, finesse, Q-factor, and photon lifetime instantly. View the Airy transmission spectrum and Gaussian beam cross-section live.
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The Free Spectral Range (FSR) defines the spacing in frequency (or wavelength) between consecutive longitudinal modes of the resonator. It is fundamentally set by the time it takes light to complete one round trip.
$$\text{FSR}= \frac{c}{2nL}$$Where $c$ is the speed of light, $n$ is the refractive index of the medium (often ~1 for air), and $L$ is the physical cavity length. A shorter $L$ results in a larger FSR.
The Finesse ($\mathcal{F}$) quantifies the spectral sharpness or quality of the resonator. It is the ratio of the FSR to the linewidth of an individual resonance. It depends critically on the total round-trip loss.
$$\mathcal{F}= \dfrac{\pi (R_1 R_2)^{1/4}}{1 - \sqrt{R_1 R_2}}$$Where $R_1$ and $R_2$ are the mirror reflectivities (values between 0 and 1). Higher reflectivities lead to higher finesse, creating sharper, more selective resonances.
The Photon Lifetime ($\tau_p$) is the average time a photon spends inside the cavity before being lost due to transmission or absorption. It directly determines the resonance linewidth and is key for applications needing stored light.
$$\tau_p = \dfrac{2L/c}{-\ln\sqrt{R_1 R_2} + L_i}$$Here, $L_i$ is the fractional internal loss per round trip. The denominator is the total loss coefficient. A longer $\tau_p$ means a higher quality factor (Q-factor) and less energy loss per cycle.
Laser Oscillators: Every laser requires an optical resonator to provide feedback and amplify light at a specific frequency. The design parameters you adjust here—length, mirror reflectivity—directly control the laser's output wavelength, efficiency, and beam quality. For instance, a high-finesse cavity in a helium-neon laser produces a very pure, single-frequency red beam.
Optical Frequency Combs: These are precise "rulers" for light, used in atomic clocks and ultra-precise spectroscopy. They rely on a special type of ultra-high-finesse resonator (a micro-ring or Fabry-Pérot) to generate a spectrum of equally spaced, sharp lines. The FSR you calculate here becomes the comb's tooth spacing.
Interferometric Sensing: High-finesse optical cavities are used as extremely sensitive detectors. A common case is in gravitational wave observatories (LIGO), where tiny changes in cavity length, caused by a passing wave, shift the resonant frequency. The finesse determines how small a length change can be detected.
Telecommunications Filtering: Dense Wavelength Division Multiplexing (DWDM) systems use filters based on optical resonators to separate hundreds of closely spaced data channels. The FSR must be carefully designed to match the ITU channel grid, and the finesse determines the channel isolation and crosstalk.
First, pay attention to whether the reflectance R is expressed as a percentage or a decimal. In this tool, a reflectance of 0.99 means 99%. A common beginner's mistake is accidentally entering "0.99%" and then finding the calculation results are completely off. Next, the interpretation of the internal loss Li. This is the "intensity loss rate per round trip"; entering 0.01 means there is a 1% loss. If you confuse this with "transmittance" and enter a large value (e.g., 0.5), the photon lifetime will be calculated as anomalously short. In practice, even for ultra-precision mirrors, the world aims for Li values below 0.001 (0.1%).
Also, keep in mind that "the Gaussian beam profile is for the ideal case". The beam radius ω(z) shown by the tool assumes perfect spherical mirrors and perfect alignment. In reality, beam shape distorts due to mirror imperfections and slight misalignments. There's a pitfall where you might design something thinking "this size will fit" based on a simulation, but in the actual device, cavity length changes due to thermal expansion, causing the beam to widen and clip the mirror edge (= increased loss!). For example, using a resonator with L=1cm in an environment with ±5°C room temperature fluctuations can cause length changes on the order of several micrometers (depending on the material), potentially shifting the FSR and beam waist position.
Fabry-Pérot etalon for 1064 nm Nd:YAG laser: cavity length L=50 mm, R1=0.95, R2=0.99, insertion losses=0.5%, beam waist w0=200 μm. Computed FSR ≈ 3000 MHz (c/2L); finesse F ≈ 285; Q-factor ≈ 8.55×10⁸; photon lifetime τp ≈ 136 ns; Rayleigh range zR ≈ 1.18 mm; linewidth δν ≈ 1.17 kHz. These parameters suit narrowband filtering in Raman spectroscopy systems.