Abstract
The study of the mechanical effects of light, including angular momentum, has a long history. The recent rapid growth of interest, however, can be traced to the observation that the Laguerre–Gaussian modes, familiar from laser physics, carry a well-defined quantity of orbital angular momentum [1]. To be specific, the mode u LG pℓ (Eq. (12.21)) propagating in the z-direction, with azimuthal dependence exp(iℓø), carries a z-component of orbital angular momentum of ℓħ per photon. This idea is strongly suggested by the powerful analogy between paraxial optics and the Schrödinger equation, together with the operator corresponding to the z-component of orbital angular momentum L z = -iħ∂/∂ø [2]. A convincing demonstration follows from an analysis of the Poynting vector and the associated angular momentum density [1, 3] as briefly described in Section 12.2.
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Barnett, S.M., Zambrini, R. (2007). Orbital Angular Momentum of Light. In: Kolobov, M.I. (eds) Quantum Imaging. Springer, New York, NY. https://doi.org/10.1007/0-387-33988-4_12
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