Observation of OAM sidebands due to optical reflection
W. L\"offler, Andrea Aiello, J. P. Woerdman

TL;DR
This paper studies how the orbital angular momentum of a light beam changes upon reflection, revealing significant OAM sidebands caused by beam spread, supported by a new theoretical model and experimental validation.
Contribution
It introduces a spatial Fresnel coefficient theory to predict OAM sidebands during reflection, validated through experiments.
Findings
OAM sidebands are significant even for modest beam spreads
Theoretical predictions match experimental results
Angular spread influences OAM during reflection
Abstract
We investigate how the orbital angular momentum (OAM) of a paraxial light beam is affected upon reflection at a planar interface. Theoretically, the unavoidable angular spread of the (paraxial) beam leads to OAM sidebands which are found to be already significant for modest beam spread (0.05). In analogy to the polarization Fresnel coefficients we develop a theory based upon spatial Fresnel coefficients; this allows straightforward prediction of the strength of the sidebands. We confirm this by experiment.
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