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arxiv: 1805.12562 · v2 · pith:VKRBMTSDnew · submitted 2018-05-31 · 🌌 astro-ph.CO · astro-ph.IM· hep-ex· hep-ph· physics.ins-det

Dark Matter Search Results from a One TonnetimesYear Exposure of XENON1T

classification 🌌 astro-ph.CO astro-ph.IMhep-exhep-phphysics.ins-det
keywords mathrmtimesxenon1tbackgroundenergyexposuresearchtextrm
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We report on a search for Weakly Interacting Massive Particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of $(1.30 \pm 0.01)$ t, resulting in a 1.0 t$\times$yr exposure. The energy region of interest, [1.4, 10.6] $\mathrm{keV_{ee}}$ ([4.9, 40.9] $\mathrm{keV_{nr}}$), exhibits an ultra-low electron recoil background rate of $(82\substack{+5 \\ -3}\textrm{ (sys)}\pm3\textrm{ (stat)})$ events/$(\mathrm{t}\times\mathrm{yr}\times\mathrm{keV_{ee}})$. No significant excess over background is found and a profile likelihood analysis parameterized in spatial and energy dimensions excludes new parameter space for the WIMP-nucleon spin-independent elastic scatter cross-section for WIMP masses above 6 GeV/c${}^2$, with a minimum of $4.1\times10^{-47}$ cm$^2$ at 30 GeV/c${}^2$ and 90% confidence level.

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