Laser Beam Expander Calculator

Calculate a two-lens beam expander's magnification, second-lens focal length, lens separation, and output divergence from the input/output beam diameters and lens focal length (M = D_out/D_in = f2/f1).

Quick Facts

Magnification
M = D_out / D_in = f2 / f1
The output-to-input beam diameter ratio equals the ratio of the two lens focal lengths.
Divergence scaling
θ_out = θ_in / M
An ideal afocal system conserves étendue (D × θ), so divergence shrinks as the beam grows.
Galilean spacing
L = f2 − f1
Diverging lens 1 + converging lens 2; compact, with no internal focal point.
Keplerian spacing
L = f1 + f2
Two converging lenses; the internal focus allows spatial filtering with a pinhole.

Your Results

Calculated
Beam Magnification
-
M = D_out / D_in = f2 / f1
Lens 2 Focal Length
-
f2 = M × f1
Lens Separation
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Galilean: L = f2 − f1 · Keplerian: L = f1 + f2
Output Beam Divergence
-
θ_out = θ_in / M

Ready

Enter beam diameters, the focal length of lens 1, and input divergence, then press Calculate.

Formula and Method for the Laser Beam Expander Calculator

A laser beam expander is a two-lens afocal (telescope-like) optical system that increases the diameter of a collimated input laser beam by a magnification factor M, while reducing the beam's angular divergence by that same factor. It is used to lower power density on downstream optics, shrink a laser's far-field spot at long range, or match a beam to the clear aperture of a telescope, scanner, or lens system. This calculator uses the standard thin-lens beam-expander relations M = D_out / D_in = f2 / f1, f2 = M × f1, and θ_out = θ_in / M, with lens spacing depending on whether the design is Galilean or Keplerian.

How the calculation works

Enter the input and output beam diameters — their ratio sets the required magnification, M = D_out / D_in. Enter the focal length of the first lens (f1); the calculator finds the focal length the second lens must have, f2 = M × f1, so both lenses share a common focal point and the system stays afocal (collimated in, collimated out). The lens separation follows from that shared focal point: L = f2 − f1 for a Galilean design (diverging lens 1, converging lens 2), or L = f1 + f2 for a Keplerian design (two converging lenses). Finally, because expanding a beam's diameter by M shrinks its divergence by the same factor — étendue is conserved by an ideal afocal system — the output full-angle divergence is θ_out = θ_in / M.

Galilean vs. Keplerian design

In a Galilean beam expander, lens 1 is diverging (negative focal length) and lens 2 is converging (positive focal length); the beam never comes to a real focus inside the housing, which keeps the assembly compact (L = f2 − f1) and avoids the intense focal spot that can ionize air or damage optics at high pulse energies. In a Keplerian beam expander, both lenses are converging and the beam passes through a real internal focus (L = f1 + f2); that design is longer overall, but the internal focus is a point where a pinhole spatial filter can remove diffraction rings and clean up the beam's intensity profile — a common step in high-quality laser systems.

Practical limits and common mistakes

This calculator uses paraxial (thin-lens) ray optics, which assumes small angles and lenses that are thin compared with their focal lengths — real multi-element expander lenses need slightly different spacing to correct for thickness and aberrations. Real laser beams are Gaussian, not uniform-diameter rays, so "diameter" should be measured the same way (commonly the 1/e² diameter) on both the input and output sides. Also remember that θ_out = θ_in / M is the theoretical, diffraction-limited reduction in divergence — a misaligned or aberrated expander can add divergence back, so treat the calculated value as a best-case target to verify with a beam profiler.

Frequently Asked Questions

What does a laser beam expander do and why use one?
A laser beam expander is a two-lens afocal system that increases a collimated beam's diameter from D_in to D_out while proportionally reducing its divergence angle. It is used to shrink a laser's far-field spot over long distances, to match a beam to an optic's clear aperture, and to lower power density on downstream lenses and mirrors.
How do I calculate the magnification of a beam expander?
Magnification equals the ratio of the output beam diameter to the input beam diameter, which also equals the ratio of the two lens focal lengths: M = D_out / D_in = f2 / f1. For example, a 2 mm input beam expanded to 10 mm gives M = 5, so a 25 mm first lens needs a 125 mm second lens.
What is the difference between a Galilean and a Keplerian beam expander?
A Galilean expander pairs a diverging (negative) first lens with a converging second lens, so the separation is L = f2 − f1; it is compact and has no internal focus, avoiding air breakdown at high laser power. A Keplerian expander uses two converging lenses with L = f1 + f2; the beam crosses an internal focus, which is longer overall but allows spatial filtering with a pinhole to clean the beam profile.
Why does the output beam diverge less than the input beam?
An ideal afocal system conserves étendue, so beam diameter times divergence angle stays roughly constant: D_in × θ_in ≈ D_out × θ_out. Because D_out = M × D_in, the output divergence is θ_out = θ_in / M — magnifying the beam 5× cuts its divergence to one-fifth.