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Beam Divergence

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Definition: a measure for how fast a laser beam expands far from its focus

The beam divergence of a laser beam is a measure for how fast the beam expands far from the beam waist, i.e., in the so-called far field. A low beam divergence can be important for applications such as pointing or free space optical communications. Beams with very small divergence, i.e., with approximately constant beam radius over significant propagation distances, are called collimated beams.

beam divergence

Figure 1: The half-angle divergence of a Gaussian laser beam is defined via the asymptotic variation of the beam radius (blue) along the beam direction. Note, however, that the divergence angle in the figure appears much larger than it actually is, since the scaling of the x and y axes is different.

Quantitative Definitions of Beam Divergence

Different quantitative definitions are used in the literature:

As an example, an FWHM beam divergence angle of 30° may be specified for the fast axis of a small edge-emitting laser diode. This corresponds to a 25.4° = 0.44 rad 1/e2 half-angle divergence, and it becomes apparent that for collimating such a beam without truncating it one would require a lens with a rather high numerical aperture of e.g. 0.6. Highly divergent (or convergent) beams also require carefully designed optics to avoid spherical aberrations.

Divergence of Gaussian Beams and Beams with Poor Beam Quality

For a diffraction-limited Gaussian beam, the 1/e2 beam divergence half-angle is λ / (π w0), where λ is the wavelength (in the medium) and w0 the beam radius at the beam waist. This is equation is based on the paraxial approximation, and is thus valid only for beams with moderately strong divergence.

A higher beam divergence for a given beam radius, i.e., a higher beam parameter product, is related to an inferior beam quality, which essentially means a lower potential for focusing the beam to a very small spot. If the beam quality is characterized with a certain M2 factor, the divergence half-angle is

beam divergence for non-ideal laser beam

Spatial Fourier Transforms

It can be helpful to use the spatial Fourier transform of the complex electric field of a laser beam as a function of the transverse coordinates (→ Fourier optics). Effectively this means that the beam is considered as a superposition of plane waves, and the Fourier transform indicates the amplitudes and phases of all plane wave components. For propagation in free space, only the phase values change.

The width (e.g. measured as the root-mean-squared (rms) width) of the spatial Fourier transform can be directly related to the beam divergence. This means that the beam divergence (and in fact the full beam propagation) can be calculated from the transverse complex amplitude profile of the beam at any position along the beam axis, assuming that the beam propagates in a homogeneous medium (e.g. in air).

Measurement of Beam Divergence

For the measurement of beam divergence, one usually measures the beam caustic, i.e., the beam radius at different positions, using e.g. a beam profiler.

It is also possible to derive the beam divergence from the complex amplitude profile of the beam in a single plane, as described above. Such data can be obtained e.g. with a Shack-Hartmann wavefront sensor.

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See also: beam radius, laser beams, collimated beams, beam parameter product, beam quality, beam pointing fluctuations, beam profilers, free space optical communications, Spotlight article 2007-07-11

Category: general optics


Dr. R. Paschotta

This encyclopedia is authored by Dr. Rüdiger Paschotta, the founder and executive of RP Photonics Consulting GmbH. Contact this distinguished expert in laser technology, nonlinear optics and fiber optics, and find out how his technical consulting services (e.g. product designs, problem solving, independent evaluations, or staff training) could become very valuable for your business!

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