Determining the
spin angular momentum (SAM) of light is simple – SAM is related to the polarization state of the light: the AM is, per photon, in a left and right circularly polarized beam respectively. Thus the SAM can be measured by transforming the circular polarization of light into a p- or s-polarized state by means of a
wave plate and then using a
polarizing beam splitter that will transmit or reflect the state of light. As the state of OAM of light is unbounded, any integer value of
l is orthogonal to (independent from) all the others. Where a beam splitter could separate the two states of SAM, no device can separate the
N (if greater than 2) modes of OAM, and, clearly, the perfect detection of all
N potential states is required to finally resolve the issue of measuring OAM. Nevertheless, some methods have been investigated for the measurement of OAM. In practical scenarios, light beams carrying orbital angular momentum (OAM) are often not composed of a single pure mode due to distortions caused by atmospheric turbulence, optical misalignment, or scattering. These imperfections result in a superposition of multiple OAM modes within the beam. Measuring the OAM spectrum is essential to quantify the modal composition and assess the beam's quality, which is critical for applications such as optical communications, imaging, and quantum information processing. To determine the vortex mode spectrum, one common method involves decomposing the complex optical field into its constituent angular harmonics: For a scalar complex field expressed in polar coordinates, this decomposition is: u(\rho, \phi, z) = \frac{1}{\sqrt{2\pi}} \sum_{l=-\infty}^{\infty} a_l(\rho, z) \exp(i l \phi), where the summation runs over all integer OAM modes l. This decomposition requires knowledge of both the amplitude and phase of the field. While direct phase measurement is challenging,
phase retrieval algorithms — particularly single-beam multiple-image reconstruction (SBMIR) methods — enable reliable recovery of the phase profile from intensity measurements alone, achieving high resolution without auxiliary reference beams. The coefficients a_l(\rho, z), representing the amplitude of each mode, are obtained by projecting the field onto the corresponding angular harmonic: a_l(\rho, z) = \frac{1}{\sqrt{2\pi}} \int_{0}^{2\pi} u(\rho, \phi, z) \exp(-i l \phi)d\phi. The normalized intensity (or power) of each OAM mode l at a propagation distance z is then calculated by integrating the squared modulus of a_l over the radial coordinate \rho: P_l(z) = \frac{\int_{0}^{\infty} |a_l(\rho, z)|^2 \rho d\rho}{\sum_{l'=-\infty}^{\infty} \int_{0}^{\infty} |a_{l}(\rho, z)|^2 \rho d\rho}. Here, the denominator ensures normalization by the total power across all modes, making P_l(z) a dimensionless fraction between 0 and 1. This spectrum provides a direct measure of the beam's OAM purity and mode distribution.
Counting spiral fringes Beams carrying OAM have a helical phase structure. Interfering such a beam with a uniform plane wave reveals phase information about the input beam through analysis of the observed spiral fringes. In a
Mach–Zender interferometer, a helically phased source beam is made to interfere with a plane-wave
reference beam along a collinear path. Interference fringes will be observed in the plane of the beam waist and/or at the Rayleigh range. The path being collinear, these fringes are pure consequence of the relative phase structure of the source beam. Each fringe in the pattern corresponds to one step through: counting the fringes suffices to determine the value of
l.
Diffractive holographic filters Computer-generated holograms can be used to generate beams containing phase singularities, and these have now become a standard tool for the generation of beams carrying OAM. This generating method can be reversed: the hologram, coupled to a single-mode fiber of set entrance aperture, becomes a filter for OAM. This approach is widely used for the detection of OAM at the single-photon level. The phase of these optical elements results to be the superposition of several fork-holograms carrying topological charges selected in the set of values to be demultiplexed. The position of the channels in far-field can be controlled by multiplying each fork-hologram contribution to the corresponding
spatial frequency carrier.
Other methods Other methods to measure the OAM of light include the rotational
Doppler effect, systems based on a
Dove prism interferometer, the measure of the spin of trapped particles, the study of diffraction effects from apertures, and optical transformations. The latter use diffractive optical elements in order to unwrap the angular phase patterns of OAM modes into plane-wave phase patterns which can subsequently be resolved in the Fourier space. The resolution of such schemes can be improved by spiral transformations that extend the phase range of the output strip-shaped modes by the number of spirals in the input beamwidth. ==Applications==