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A measurement of the time profile of scintillation induced by low energy gamma-rays in liquid xenon with the XMASS-I detector

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arxiv 1604.01503 v3 pith:YKUZGURT submitted 2016-04-06 physics.ins-det astro-ph.COhep-exnucl-ex

classification physics.ins-detastro-ph.COhep-exnucl-ex
keywords decayenergytimedatascintillationconstantinducedliquid
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abstract

We report the measurement of the emission time profile of scintillation from gamma-ray induced events in the XMASS-I 832 kg liquid xenon scintillation detector. Decay time constant was derived from a comparison of scintillation photon timing distributions between the observed data and simulated samples in order to take into account optical processes such as absorption and scattering in liquid xenon. Calibration data of radioactive sources, $^{55}$Fe, $^{241}$Am, and $^{57}$Co were used to obtain the decay time constant. Assuming two decay components, $\tau_1$ and $\tau_2$, the decay time constant $\tau_2$ increased from 27.9 ns to 37.0 ns as the gamma-ray energy increased from 5.9 keV to 122 keV. The accuracy of the measurement was better than 1.5 ns at all energy levels. A fast decay component with $\tau_1 \sim 2$ ns was necessary to reproduce data. Energy dependencies of $\tau_2$ and the fraction of the fast decay component were studied as a function of the kinetic energy of electrons induced by gamma-rays. The obtained data almost reproduced previously reported results and extended them to the lower energy region relevant to direct dark matter searches.

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  1. Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter

    nucl-ex 2025-06 conditional novelty 6.0 of 10

    A new delayed-coincidence tag from 136Cs isomers could let the nEXO detector reject backgrounds down to 10^-9 and measure CNO solar neutrinos, the 7Be neutrino energy, and sub-MeV fermionic dark matter.

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