6533b854fe1ef96bd12af373

RESEARCH PRODUCT

Dark Matter Search Results from a One Ton-Year Exposure of XENON1T

Xenon CollaborationE. AprileJ. AalbersF. AgostiniM. AlfonsiL. AlthueserF. AmaroM. AnthonyF. ArneodoL. BaudisB. BauermeisterM. BenabderrahmaneT. BergerP. BreurA. BrownA. BrownE. BrownS. BruennerG. BrunoR BudnikC. CapelliJ. CardosoD. CichonD. CoderreA. ColijnJ. ConradJ. CussonneauM. DecowskiP. De PerioP. Di GangiA. Di GiovanniS. DiglioA. ElykovG. EurinJ. FeiA. FerellaA. FieguthW. FulgioneA. RossoM. GallowayF. GaoM. GarbiniC. GeisL. GrandiZ. GreeneH. QiuC. HasterokE. HogenbirkJ. HowlettR. ItayF. JoergB. KaminskyS. KazamaA. KishG. KoltmanH. LandsmanR. LangL. LevinsonQ. LinS. LindemannM. LindnerF. LombardiJ. LopesJ. MahlstedtA. ManfrediniT. Marrodán UndagoitiaJ. MasbouD. MassonM. MessinaK. MicheneauK. MillerA. MolinarioK. MoråM. MurraJ. NaganomaK. NiU. OberlackB. PelssersF. PiastraJ. PienaarV. PizzellaG. PlanteR. PodviianiukN. PrielD. GarcíaL. RauchS. ReichardC. ReuterB. RiedelA. RizzoA. RocchettiN. RuppJ. SantosG. SartorelliM. ScheibelhutS. SchindlerJ. SchreinerD. SchulteM. SchumannL. LavinaM. SelviP. ShaginE. ShockleyM. SilvaH. SimgenD. ThersF. ToschiG. TrincheroC. TunnellN. UpoleM. VargasO. WackH. WangZ. WangY. WeiC. WeinheimerC. WittwegJ. WulfJ. YeY. ZhangT. Zhu

subject

Dark matterGeneral Physics and Astronomychemistry.chemical_elementS030DI5WIMP: massElectronParameter spacedark matter: direct detectionGravitation and AstrophysicsS030DI101 natural sciencesS030DI3S030DI2Nuclear physicsXenonRecoilWIMPelectron: recoil0103 physical sciencesS046DM2[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsnumerical calculationsDark Matter WIMP TPC XENON Direct searchPhysicsxenon: liquidTime projection chamber010308 nuclear & particles physicsbackgrounddark matter: massGran SassoWIMP nucleonchemistryWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]time projection chamber: xenon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]

description

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.

10.1103/physrevlett.121.111302https://hdl.handle.net/21.11116/0000-0003-350D-421.11116/0000-0003-350F-2