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Search for WIMP-¹²⁹Xe inelastic scattering with particle identification in XMASS-I

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arxiv 1809.05358 v2 pith:UGQ7FV7B submitted 2018-09-14 astro-ph.CO hep-exnucl-ex

Search for WIMP-¹²⁹Xe inelastic scattering with particle identification in XMASS-I

classification astro-ph.CO hep-exnucl-ex
keywords inelastictimesbetagammalikelimitsraysscattering
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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A search for Weakly Interacting Massive Particles (WIMPs) was conducted with the single-phase liquid-xenon detector XMASS through inelastic scattering in which $^{129}$Xe nuclei were excited, using an exposure ($\rm 327\; kg \times 800.0 \; days$) 48 times larger than that of our previous study. The inelastic excitation sensitivity was improved by detailed evaluation of background, event classification based on scintillation timing that distinguished $\gamma$-rays and $\beta$-rays, and simultaneous fitting of the energy spectra of $\gamma$-like and $\beta$-like samples. No evidence of a WIMP signal was found. Thus, we set the upper limits of the inelastic channel cross section at 90\% confidence level, for example, $4.1\times 10^{-39} \;{\rm cm^2}$ for a $200\; {\rm GeV}/c^2$ WIMP. This result provides the most stringent limits on the SD WIMP-neutron interaction and is better by a factor of 7.7 at $200\;{\rm GeV}/c^2$ than the existing experimental limit.

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