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Volumn 82, Issue 2, 2010, Pages

How orbital angular momentum affects beam shifts in optical reflection

Author keywords

[No Author keywords available]

Indexed keywords

BEAM SHIFT; DIELECTRIC INTERFACE; GAUSSIAN LIGHT BEAMS; MIXING MATRIX; OPTICAL REFLECTION; ORBITAL ANGULAR MOMENTUM;

EID: 77956328546     PISSN: 10502947     EISSN: 10941622     Source Type: Journal    
DOI: 10.1103/PhysRevA.82.023817     Document Type: Article
Times cited : (195)

References (32)
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    • Here we quantify the GH and IF shifts via the photocurrents Ix/I and Iy/I delivered by the quadrant detector actually used in the experiment, respectively. This furnishes the median of the beam intensity distribution. Conversely, in Ref. [19] the same displacements are quantified via the mean of the intensity distribution. The difference between these two methods leads to both the trivial prefactor Nℓ(experimentally eliminated by a detector calibration procedure) and the terms "2ℓ" (instead of "ℓ") in the mixing matrix (18).
    • Here we quantify the GH and IF shifts via the photocurrents I x / I and I y / I delivered by the quadrant detector actually used in the experiment, respectively. This furnishes the median of the beam intensity distribution. Conversely, in Ref. [19] the same displacements are quantified via the mean of the intensity distribution. The difference between these two methods leads to both the trivial prefactor N ℓ (experimentally eliminated by a detector calibration procedure) and the terms " 2 ℓ " (instead of " ℓ ") in the mixing matrix (18).
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    • °. This was done to reduce the very large intensity contrast occurring during p↔s modulation and thus to minimize a parasitic cross-effect on the displacement as synchronously measured by the quadrant detector.
    • °. This was done to reduce the very large intensity contrast occurring during p ↔ s modulation and thus to minimize a parasitic cross-effect on the displacement as synchronously measured by the quadrant detector.


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