Quenching factor measurements of sodium nuclear recoils in NaI:Tl determined by spectrum fitting
L. J. Bignell, I. Mahmood, F. Nuti, G. J. Lane, A. Akber, E. Barberio,, T. Baroncelli, B. Coombes, W. Dix, J. T. H. Dowie, T. Eriksen, M. S. M., Gerathy, T. J. Gray, B. P. McCormick, A. J. Mitchell, M. S. Rahman, F., Scutti, N. J. Spinks, A. E. Stuchbery, H. Timmers, P. Urquijo

TL;DR
This paper measures sodium nuclear recoil quenching factors in NaI:Tl crystals using spectrum fitting, providing data crucial for dark matter detection experiments and introducing a new analysis method for future research.
Contribution
It introduces a spectrum-fitting methodology to accurately determine quenching factors in NaI:Tl crystals for nuclear recoils.
Findings
Quenching factors measured between 36 and 401 keV.
Results agree with recent neutron source measurements.
Method applicable to SABRE experiment crystals.
Abstract
We have performed measurements of sodium nuclear recoils in NaI:Tl crystals, following scattering by neutrons produced in a Li(p,n)Be reaction. Understanding the light output from such recoils, which is reduced relative to electrons of equivalent energy by the quenching factor, is critical to interpret dark matter experiments that search for nuclear scattering interactions. We have developed a spectrum-fitting methodology to extract the quenching factor from our measurements, and report quenching factors for nuclear recoil energies between 36 and 401 keV. Our results agree with other recent quenching factor measurements that use quasi-monoenergetic neutron sources. The new method will be applied in the future to the NaI:Tl crystals used in the SABRE experiment.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Quantum, superfluid, helium dynamics · Atomic and Subatomic Physics Research
