Photon Correlation Spectroscopy and Velocimetry 1977
DOI: 10.1007/978-1-4757-1668-9_3
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Statistical Properties of Scattered Radiation

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Cited by 33 publications
(23 citation statements)
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“…(4.3) were reported previously by Bertolotti et al 5 and by Pusey. 6 We also report a generalization in which the negativebinomial distribution is smeared by a noncentral x 2 distribution. This distribution may suitably model the statistics of photodetection for radiation passed through turbulent media, such as the atmosphere.…”
Section: Multiply Stochastic Representations For the Photon-counting mentioning
confidence: 95%
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“…(4.3) were reported previously by Bertolotti et al 5 and by Pusey. 6 We also report a generalization in which the negativebinomial distribution is smeared by a noncentral x 2 distribution. This distribution may suitably model the statistics of photodetection for radiation passed through turbulent media, such as the atmosphere.…”
Section: Multiply Stochastic Representations For the Photon-counting mentioning
confidence: 95%
“…A more general approach, initiated by Pusey, Jakeman, and their colleagues in 1976, made use of the K distribution for problems involving the field and irradiance in scattering, speckle, and the propagation of light through turbulent media. 6 -' 2 The same model was used also to describe non-Rayleigh microwave sea echo. ' 3 -' 5 A number of generalizations of the K distribution, including the I-K distributionl61 7 and the generalized K distribution, 1…”
Section: Introductionmentioning
confidence: 99%
“…For the same reason, we shall just discuss DLS from a system of noninteracting particles, referring to excellent books and reviews [4][5][6][7][8] for a more comprehensive treatment. This short presentation is mostly meant to stress those fundamentals of the technique that are essential to grasp the more recent advancement we shall later discuss.…”
Section: Dls (Intensity-correlation Spectroscopy)mentioning
confidence: 99%
“…In other words, we actually want to avoid using a source with a very long coherence time, for we need t c to be much shorter than the physical fluctuation time of the sample ( Figure 10.1). Quantitatively [7], one finds that the scattered field is not Gaussian, so that, in terms of the full correlation functions g 2 (q,t) 6 ¼ 1 þ |g 1 (q,t)| 2 ; yet, g 2 (t) ¼ 1 þ |g 1 B (q,t)| 2 ; thus, intensity-correlation measurements still yield what is needed. The latter, however, still affect g 1 (t), thus hampering spectroscopic and interferometric measurements.…”
Section: Dls the Ultimate Spectroscopymentioning
confidence: 99%
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