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15 October 2012 Hiding the phase: the filling of the slope discrepancy Hilbert space
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Abstract
Previous theoretical work, to first order, demonstrated that branch points are markers for photons carrying orbital angular momentum (OAM), but gave to indication of the flux associated with a given branch point distribution. In a parallel effort, the OAM flux as a ratio of the total flux is calculated, but that work relies on knowing the non-zero elements in the slope discrepancy Hilbert space. Here, we calculate the “size” of the slope discrepancy Hilbert space for our previously published data.
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Darryl J. Sanchez and Denis W. Oesch "Hiding the phase: the filling of the slope discrepancy Hilbert space", Proc. SPIE 8520, Unconventional Imaging and Wavefront Sensing 2012, 852004 (15 October 2012); https://doi.org/10.1117/12.932282
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