Abstract
Probability generating functions of the number of photoelectrons emitted by a detector during a given interval can often be relatively easily calculated from a physical model of the emissive processes, but inverting them analytically to obtain the distributions of the number of so-called “photocounts” is usually complicated or impossible. Techniques for computing those distributions can be based on numerical evaluation of the inversion integral along a suitably chosen contour passing through a saddlepoint of the integrand and lying as close as possible to a path of steepest descent of that integrand. The method can be extended to include the effects of additive Gaussian noise, intersymbol interference, and postdetector filtering.
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© 1991 Springer-Verlag
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Helstrom, C.W. (1991). Calculating photocount distributions by saddlepoint methods. In: Bendjaballah, C., Hirota, O., Reynaud, S. (eds) Quantum Aspects of Optical Communications. Lecture Notes in Physics, vol 378. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53862-3_179
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DOI: https://doi.org/10.1007/3-540-53862-3_179
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