Impact of the Fano Factor on Position and Energy Estimation in Scintillation Detectors.

IEEE Trans Nucl Sci

Department of Medical Imaging and College of Optical Sciences, University of Arizona, Tucson, AZ 85225 USA.

Published: February 2015

AI Article Synopsis

  • The Fano factor measures the noise of an integer-valued random variable by comparing its variance to its mean, influencing the performance of scintillation crystals in detecting light.
  • Variations in Fano factors among scintillation crystals range from less noise (sub-Poisson) to more noise (super-Poisson), impacting the quality of spatial and energy resolutions in gamma-camera systems.
  • The study found that while the Fano factor does not affect the spatial resolution when determining the position of gamma-ray photon interactions, a smaller Fano factor leads to improved energy resolution.

Article Abstract

The Fano factor for an integer-valued random variable is defined as the ratio of its variance to its mean. Light from various scintillation crystals have been reported to have Fano factors from sub-Poisson (Fano factor < 1) to super-Poisson (Fano factor > 1). For a given mean, a smaller Fano factor implies a smaller variance and thus less noise. We investigated if lower noise in the scintillation light will result in better spatial and energy resolutions. The impact of Fano factor on the estimation of position of interaction and energy deposited in simple gamma-camera geometries is estimated by two methods - calculating the Cramér-Rao bound and estimating the variance of a maximum likelihood estimator. The methods are consistent with each other and indicate that when estimating the position of interaction and energy deposited by a gamma-ray photon, the Fano factor of a scintillator does not affect the spatial resolution. A smaller Fano factor results in a better energy resolution.

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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC4625574PMC
http://dx.doi.org/10.1109/TNS.2014.2379620DOI Listing

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