Physics – Instrumentation and Detectors
Scientific paper
2009-04-30
A.Lyashenko et. al., J. Appl. Phys. 106 (2009) 044902
Physics
Instrumentation and Detectors
10 pages, 10 figures, for submission to J. Appl. Phys; (2009) accepted
Scientific paper
10.1063/1.3197063
The operation of visible-sensitive gaseous- and, to some extent, vacuum-photomultipliers is critically affected by secondary electrons originating from ion impact on the photocathode. A simple method for indirect measurement of the effective ion-induced secondary-electron emission (IISEE) coefficient from the photocathode into a gas medium, $\gamma_+^{eff}$ was developed. The experimental results with visible-sensitive K-Cs-Sb, Na-K-Sb and Cs-Sb photocathodes, yielded $\gamma_+^{eff}$ - values between 0.02 and 0.03 in Ar/CH$_{4}$ (95/5) at 700 mbar; these are in good agreement with theoretical calculations. The corresponding vacuum IISEE coefficients, $\gamma_+$, were estimated, based on a theoretical model, to be 0.47, 0.49 and 0.47 for K-Cs-Sb, Na-K-Sb and Cs-Sb photocathodes, respectively. The ratio of gas $\gamma_+^{eff}$ and vacuum $\gamma_+$ IISEE coefficients, calculated to be $\sim$0.06, is the fraction of secondary electrons surmounted the backscattering in the gas media.
Breskin Amos
Chechik Rachel
Dias H. V. T. T.
Lyashenko Alexey
No associations
LandOfFree
Ion-induced secondary electron emission from K-Cs-Sb, Na-K-Sb and Cs-Sb photocathodes and its relevance to the operation of gaseous avalanche photomultipliers does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Ion-induced secondary electron emission from K-Cs-Sb, Na-K-Sb and Cs-Sb photocathodes and its relevance to the operation of gaseous avalanche photomultipliers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ion-induced secondary electron emission from K-Cs-Sb, Na-K-Sb and Cs-Sb photocathodes and its relevance to the operation of gaseous avalanche photomultipliers will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-443852