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We observe that the pattern of the quenching factors for scintillation light from various ions, recently studied in $CaWO_4$ in connection with dark matter detectors, can be understood as a saturation phenomenon in which the light output is simply proportional to track length, independent of the ion and its energy.
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J. Ninković, Dissertation submitted to the Fakultät für Physik, TUM, Munich, March 2005, and J. Ninković et al. Nuc. Inst. Methods A 564
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See the discussion at the end of the section “quenching factors”in ref gs
Cited in the paper.
We use the program available at www.srim.org
Cited in the paper.
The STAR programs are available at /physics.nist.gov/PhysRefData/Star/Text
Cited in the paper.
In SRIM “straggle” is the square root of the average square fluctuation. Thus in a Gaussian fit ∼ e x p [ − 1 2 ( OPEN l ¯ − l ) σ ) 2 ] \sim exp[-{1\over 2}({{\bar{l}}-l)\over\sigma})^{2}] to the event distribution as a function of l l the light output, “straggle” would be equivalent to σ \sigma
Cited in the paper.
Cited in the paper.
P. Huff, Diplomarbeit
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Later among the works it cites.
Th. Jagemann et al., Astroparticle Phys. 26
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Although it should be noted that V.B. Mikhailik, H. Kraus, S. Henry and A. J. B. Tolhurst, Phys. Rev. B 75
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