advanced30 min studyLesson 218 in Physics

Gaussian beams and Rayleigh range

Connect an explicitly defined Gaussian intensity radius to diffraction spreading, conserved power, wavefront curvature, and the Gouy phase.

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What you’ll understand

  • Distinguish the 1/e field radius from the 1/e² intensity radius and diameter.
  • Calculate Rayleigh range, divergence, and peak irradiance.
  • Explain why a planar waist does not imply an indefinitely parallel beam.

A laser beam cannot be both transversely confined and exactly parallel everywhere in free space. Its finite waist requires a spread of transverse plane-wave directions, and those directions accumulate different phases on propagation. The fundamental Gaussian beam is an analytic paraxial solution that makes this spreading especially simple. Its usefulness depends on stating precisely what the quoted beam radius means and on separating the envelope width from the curvature of the optical phase.

Define the radius before using a beam formula

Use the intensity profile with radial dependence exp⁡(−2r2/w2)\exp(-2r^2/w^2). The radius ww is therefore the distance where intensity falls to 1/e21/e^2 of its on-axis value, while the electric-field amplitude falls to 1/e1/e. The quoted beam diameter in this convention is 2w2w. A radius based on half maximum or on 1/e1/e intensity is a different number, so substituting it into the same Rayleigh-range formula creates a systematic error.

Integrate the intensity over circular rings to normalize it to total power. The result fixes peak irradiance as inversely proportional to squared radius. The Gaussian has no sharp edge: approximately 86.5 percent of its total power lies inside radius ww, and some remains outside every finite circle. An aperture with radius equal to the quoted beam radius therefore clips appreciable power and generally perturbs the subsequent ideal Gaussian propagation.

I(r,z)=2Pπw2(z)exp⁡ ⁣[−2r2w2(z)],P(<R)=P(1−e−2R2/w2(z))I(r,z)=\frac{2P}{\pi w^2(z)}\exp\!\left[-\frac{2r^2}{w^2(z)}\right],\qquad P(<R)=P\left(1-e^{-2R^2/w^2(z)}\right)
P is total power in watts, I is irradiance in W/m², and r, R, w are lengths in metres. This is the circular fundamental Gaussian intensity profile in a lossless homogeneous medium; w is a radius, not a diameter.↔ Scroll wide equations horizontally.

The waist sets the propagation scale

For a waist of radius w0w_0 at z=0z=0, the Rayleigh range is πw02/λ\pi w_0^2/\lambda, using wavelength in the uniform medium. At one Rayleigh range, the squared beam radius doubles, so the radius grows by a factor of square root two and the peak irradiance halves. The full confocal parameter is twice the Rayleigh range. These three related quantities should not be interchanged merely because all are sometimes described informally as a focal depth.

Far beyond the Rayleigh range, the radius grows approximately linearly with distance. The resulting divergence half-angle is λ/(πw0)\lambda/(\pi w_0) in radians for an ideal fundamental Gaussian. Reducing waist radius therefore increases divergence; making a tighter focus does not make a more parallel outgoing beam. This result assumes paraxial angles and an ideal mode. A nonideal beam can have a larger beam-parameter product and requires a carefully defined beam-quality treatment.

zR=πw02λ,w(z)=w01+(zzR)2,θdiv≃λπw0z_R=\frac{\pi w_0^2}{\lambda},\qquad w(z)=w_0\sqrt{1+\left(\frac{z}{z_R}\right)^2},\qquad \theta_{\mathrm{div}}\simeq\frac{\lambda}{\pi w_0}
zR, z, w0, w, lambda are in metres, and theta_div is the far-field radius divergence half-angle in radians. These formulas assume a circular fundamental Gaussian beam in a homogeneous lossless medium with w0 large enough for paraxial propagation.↔ Scroll wide equations horizontally.

Envelope width and phase curvature are different

The phase fronts are planar at the waist, even though the beam subsequently expands. Their curvature radius is R(z)=z[1+(zR/z)2]R(z)=z[1+(z_R/z)^2] away from the waist, with infinite-radius limit at zero. In the negative-time phasor convention, the field phase contains kz+kr2/(2R)−ψkz+kr^2/(2R)-\psi, where ψ=arctan⁡(z/zR)\psi=\arctan(z/z_R) is the Gouy phase. The amplitude factor decreases as w0/ww_0/w, preserving integrated power as the cross-sectional area grows.

The Gouy contribution changes by pi between the distant incoming and outgoing sides of an ideal fundamental focus. It is a phase shift relative to an unconfined plane-wave reference, not an extra path length that all rays simply travel. Confusing a Gaussian envelope with a Gaussian intensity also causes errors: squaring the field doubles the exponent. Check that the radius convention, phase convention, and power normalization agree before combining formulas from different references.

A millimetre-scale infrared waist

An ideal Gaussian beam in vacuum has wavelength 1.0 μm1.0\,\mathrm{\mu m}, power 10 mW10\,\mathrm{mW}, and waist radius w0=1.0 mmw_0=1.0\,\mathrm{mm} in the 1/e² intensity convention. Find its Rayleigh range, radius one Rayleigh range away, and peak irradiance at the waist and there.

  1. The Rayleigh range is π(10−3)2/(10−6)=π m≃3.14 m\pi(10^{-3})^2/(10^{-6})=\pi\,\mathrm m\simeq3.14\,\mathrm m. The large waist-to-wavelength ratio supports a small paraxial divergence.

  2. At z=zRz=z_R, the radius is 2w0=1.414 mm\sqrt2w_0=1.414\,\mathrm{mm}. This is a radius; the corresponding diameter is 2.828 mm2.828\,\mathrm{mm}, which should not be inserted as w in the intensity formula.

  3. At the waist, I(0,0)=2(0.010)/[π(10−3)2]≃6.37×103 W/m2I(0,0)=2(0.010)/[\pi(10^{-3})^2]\simeq6.37\times10^3\,\mathrm{W/m^2}. Doubling squared radius at zR halves this peak to 3.18×103 W/m23.18\times10^3\,\mathrm{W/m^2} while total power remains 10 mW.

The result

The Rayleigh range is 3.14 m; at that distance the radius is 1.414 mm and the peak irradiance is half its 6.37 kW/m² waist value.

Explore the model

Interactive lab

Interactive lab · function

Squared-width growth as a parabola

For each run, Reset and set BOTH Coefficient a=1 and Position x. Compare x=1 and x=2, predicting y=1 and y=4. Interpret x as z/zR and y as the dimensionless squared-width excess w²/w0²−1. The instrument plots y=ax², its tangent, and signed area, not a Gaussian field or optical power.

Squared-width growth as a parabolaThis lab uses only y = ax². Playback traces the curve within the fixed integration interval from 0 to x; it does not estimate numerical error or change the chosen point. Current readings: y at chosen x: 0.608; Tangent slope · 2ax: 1.35; Signed area · ax³/3: 0.182. All parameters are adjustable with the labeled controls below.−2.4−1.201.22.4−9−4.504.59xy(x, ax²)
y = ax²TangentSigned integral
y at chosen x
0.608
Tangent slope · 2ax
1.35
Signed area · ax³/3
0.182
t = 0 s

This lab uses only y = ax². Playback traces the curve within the fixed integration interval from 0 to x; it does not estimate numerical error or change the chosen point. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.

Look forThe parabola tests the squared-width law only. Its tangent and area are mathematical readouts and are not Gaussian-beam divergence or transmitted power.

Check your understanding

A quoted fundamental Gaussian waist diameter is 2 mm in the 1/e² intensity convention. What value belongs in zR=πw0²/λ?

Try it yourself

An ideal vacuum Gaussian at 500 nm500\,\mathrm{nm} has waist radius 50 μm50\,\mathrm{\mu m}. Estimate its far-field divergence half-angle and the fraction of power inside one local beam radius. Does halving the waist halve the divergence?

Take a moment to make a prediction or work it out on paper. Open a hint when you need one.

Give me a hint

Use the wavelength and waist radius in the same units. Integrate the normalized circular intensity or use the enclosed-power formula with R=w.

Compare with the solution

The half-angle is 500×10−9/[π(50×10−6)]=3.18×10−3 rad500\times10^{-9}/[\pi(50\times10^{-6})]=3.18\times10^{-3}\,\mathrm{rad}, or about 3.18 mrad. Inside one local radius the fraction is 1−e−2≃0.86471-e^{-2}\simeq0.8647, independent of propagation distance for the ideal Gaussian. Halving the waist instead doubles the divergence to about 6.37 mrad and reduces the Rayleigh range by a factor of four. The small numerical angles remain consistent with the paraxial approximation, although real clipping or aberration can invalidate the ideal-mode description.

Take it with you

  • The conventional Gaussian radius is simultaneously a 1/e field and 1/e² intensity radius.
  • A smaller waist gives a shorter Rayleigh range and larger divergence.
  • Integrated power is conserved while peak irradiance falls as the beam spreads.

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