4 Tabs · 12 Calculators

AMO Lab Calculators

Quick-reference calculators for everyday experimental AMO physics. Optics & beams, power & RF, atomic physics, trap & cavity — results update instantly.

Optics & Beam Calculations

Gaussian beam propagation, collimation, focusing, NA, telescope magnification.

Fiber → Collimated → Focused Spot

Given the fiber MFD and collimating lens focal length, computes the collimated beam radius and (optionally) the focused spot after a second lens.
w_col = f₁ · λ / (π · MFR) [optional] w_foc = f₂ · λ / (π · w_col) z_R = π w_foc² / λ
nm
µm
mm

mm

NA ↔ Gaussian Beam Waist

For a Gaussian beam, NA = λ/(πw₀). Also gives the Abbe resolution limit.
w₀ = λ / (π · NA) [Gaussian] d_Abbe = λ / (2 · NA) [Abbe resolution] NA = λ / (π · w₀)
nm

Rayleigh Range & Divergence

Gaussian beam propagation from waist w₀ and wavelength.
z_R = π w₀² / λ θ_div = λ / (π w₀) (far-field half-angle)
nm
µm

Beam Telescope Magnification

2-lens Galilean / Keplerian expander. Output beam waist and divergence.
M = f₂ / f₁ w₀_out = M · w₀_in θ_out = θ_in / M
mm
mm
mm

f-number → Spot Size

For a Gaussian beam: w₀ ≈ λf/(πw_in). For plane wave (overfilled): d_Airy = 2.44 λ (f/D).
w₀ = λ f / (π w_in) [Gaussian] d_Airy = 2.44 λ (f/D) [overfilled]
nm
mm
mm

Power, RF & AOM Calculators

mW / dBm, gain/loss chains, AOM Bragg angles, shot noise.

mW ↔ dBm Conversion

1 mW = 0 dBm. Used everywhere: AOM drivers, amplifiers, photodetectors, VCOs.
P [dBm] = 10 · log₁₀(P [mW]) P [mW] = 10^(P [dBm] / 10)
mW

dB Gain / Loss Chain

Enter input power and gains/losses in dB (negative = loss). E.g. AOM −10 dB, amplifier +30 dB.
P_out [dBm] = P_in [dBm] + Σ gains [dB]
dBm

AOM / AOD Deflection

Bragg diffraction angle for a given optical wavelength and AOM drive frequency.
Λ = v_s / f_AOM (acoustic wavelength) θ_B = λ_opt / (2Λ) (Bragg angle) θ_def = n·λ·f_AOM / v_s (n-th order)
nm
MHz

Shot Noise on Photodetector

Photon shot noise sets the quantum noise floor for a given detection bandwidth.
I_dc = η · e · P / (hν) i_shot = √(2 e I_dc BW) [A_rms] NEP = i_shot / R [W]
nm
µW
Hz

Atomic Physics Calculators

Recoil, Doppler, de Broglie, Zeeman, saturation intensity, Maxwell–Boltzmann velocities.

Photon Recoil

Recoil velocity & temperature from one photon kick. Sets the energy scale for laser cooling.
v_rec = ħk / m = h / (mλ) T_rec = m·v_rec² / k_B = (ħk)² / (m·k_B) E_rec/h = ħk² / (4πm) [kHz]
nm
amu

Doppler Shift

Frequency shift from atom/mirror velocity. Used to find which velocity class a detuned laser addresses.
Δf = v / λ (counter-propagating) v = Δf · λ
nm
m/s

Thermal de Broglie Wavelength

λ_dB ≫ inter-particle spacing → quantum degeneracy. Also for matter-wave interferometry.
λ_dB = h / √(2π m k_B T)
amu
µK

Zeeman Shift (Linear Regime)

Valid for |B| where Zeeman energy ≪ HF splitting (typically B ≪ few hundred Gauss for alkalis).
ΔE = g_F · m_F · μ_B · B Δf = ΔE / h [MHz]
(Cs F=4: +1/4)
G

Saturation Intensity

I_sat for a dipole-allowed transition. Above I_sat, the transition is power-broadened.
I_sat = π h c Γ / (3 λ³) (cycling transition) τ = 1 / (Γ/2π)
nm
MHz

Thermal Velocity Distribution

Maxwell–Boltzmann rms, most-probable, and mean speeds.
v_rms = √(3k_BT/m) v_prob = √(2k_BT/m) (most probable) v_mean = √(8k_BT/πm) (mean speed)
amu
µK

Trap & Cavity Calculators

Optical tweezer frequencies, Lamb–Dicke parameter, Fabry–Pérot cavity, mode matching.

Optical Tweezer Trap Frequencies

Harmonic approximation near the trap minimum. Radial and axial frequencies from trap depth and beam waist.
ω_r = √(4 U₀ / m w₀²) [radial] ω_z = √(2 U₀ / m z_R²) [axial] z_R = π w₀² / λ
mK
µm
amu
nm

Lamb–Dicke Parameter

η = k x_zpf. Resolved sideband cooling requires η ≪ 1. x_zpf = √(ħ/2mω) is the zero-point motion.
x_zpf = √(ħ / 2mω_trap) η = k · cos(θ) · x_zpf ⟨n⟩_min ≈ (Γ/2ω)² [RSB cooling limit]
nm
amu
kHz
°

Optical Cavity / Fabry–Pérot

FSR, finesse, linewidth, round-trip time. Used for laser locking, ULE cavities, transfer cavities.
FSR = c / (2nL) F = π√R / (1−R) δν = FSR / F (linewidth FWHM)
mm

Gaussian Mode Matching

Coupling efficiency into a fiber or cavity mode via overlap integral of two Gaussian modes.
η = (2w₁w₂/(w₁²+w₂²))² [Δz=0] Reduced by wavefront curvature for Δz≠0
µm
µm
µm
nm
References: Foot (2005) Atomic Physics · Grimm et al. (2000) Adv. At. Mol. Opt. Phys. 42 · Yariv (1989) Quantum Electronics · Saleh & Teich (2019) Fundamentals of Photonics · NIST CODATA 2018 constants.