A novel algorithm for solving the true coincident counting issues in Monte Carlo simulations for radiation

Fada Guan1, Jesse M Johns, Latha Vasudevan

  • 1*The University of Texas MD Anderson Cancer Center, Department of Radiation Physics, Houston, TX, 77030; †Texas A&M University, Department of Nuclear Engineering, College Station, TX, 77843; ‡Texas A&M University, Environmental Health and Safety, College Station, TX, 77843; §Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Department of Nuclear Safety and Engineering, Shanghai, China, 201800; **Nanjing University of Aeronautics and Astronautics, Department of Nuclear Science and Engineering, Nanjing, Jiangsu, China, 210016.

Health Physics
|April 24, 2015
PubMed
Summary

A new algorithm improves radiation detection efficiency by accounting for coincident counts, crucial for accurate source quantification in spectroscopy. This method enhances Monte Carlo simulations for complex radiation fields.

Related Concept Videos

¹³C NMR: ¹H–¹³C Decoupling01:04

¹³C NMR: ¹H–¹³C Decoupling

The probability of having two carbon-13 atoms next to each other is negligible because of the low natural abundance of carbon-13. Consequently, peak splitting due to carbon-carbon spin-spin coupling is not observed in spectra. However, protons up to three sigma bonds away split the carbon signal according to the n+1 rule, resulting in complicated spectra.
A broadband decoupling technique is used to simplify these complex, sometimes overlapping, signals. Broadband decoupling relies on a...
2.1K
Atomic Absorption Spectroscopy: Radiation and Light Sources01:13

Atomic Absorption Spectroscopy: Radiation and Light Sources

Atomic absorption spectroscopy (AAS) relies on the Beer-Lambert law, which requires that the radiation source emits a narrow range of wavelengths to match the absorption characteristics of the analyte atom. The primary criteria for choosing an appropriate radiation source in AAS is to provide a precise and intense emission at specific wavelengths that will allow accurate detection of the analyte.
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...
1.7K
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
771
Atomic Absorption Spectroscopy: Interference01:25

Atomic Absorption Spectroscopy: Interference

Interference leads to systematic error in atomic absorption (AA) measurements by enhancing or diminishing the analytical signal or the background. These interferences can be grouped into three main categories: spectral interference, chemical interference, and physical interference.
Spectral interference occurs when signals from other elements or molecules overlap with the analyte signal, falsely elevating or masking the analyte's absorbance. This interference can be corrected using Zeeman,...
2.4K