Search results for " Direct Dark Matter"

showing 2 items of 2 documents

$^{222}$Rn emanation measurements for the XENON1T experiment

2021

The selection of low-radioactive construction materials is of utmost importance for the success of low-energy rare event search experiments. Besides radioactive contaminants in the bulk, the emanation of radioactive radon atoms from material surfaces attains increasing relevance in the effort to further reduce the background of such experiments. In this work, we present the $^{222}$Rn emanation measurements performed for the XENON1T dark matter experiment. Together with the bulk impurity screening campaign, the results enabled us to select the radio-purest construction materials, targeting a $^{222}$Rn activity concentration of 10 $\mu$Bq/kg in 3.2 t of xenon. The knowledge of the distribut…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Radon emanationFOS: Physical scienceschemistry.chemical_element01 natural sciencesNOHigh Energy Physics - Experimentradon: nuclideHigh Energy Physics - Experiment (hep-ex)XENONXenon222 RnPE2_2PE2_10103 physical sciencesActivity concentration[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)background: radioactivityPhysicsradon: admixture010308 nuclear & particles physicsdetector: surfacescreeningInstrumentation and Detectors (physics.ins-det)chemistryXenon Dark matter 222 Rn radioactivityDark Matter Radon emanation XENON Direct Dark MatterDirect Dark MatterradioactivityAtomic physics
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Search for inelastic scattering of WIMP dark matter in XENON1T

2021

We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off $^{129}$Xe is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV de-excitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.89 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2$\sigma$. A profile-likelihood ratio analysis is used to set upper limits on the cross-section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c${}^2$, with the strongest upper limit of $3.3 \time…

xenon: targetPhotonPhysics::Instrumentation and DetectorsParameter space01 natural sciencesWIMP: dark matterHigh Energy Physics - Experiment; High Energy Physics - Experiment; astro-ph.COHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XENONRecoilWIMPWIMP nucleus: cross section[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matterparameter spaceNuclear ExperimentComputingMilieux_MISCELLANEOUSnucleus: recoilPhysicsDark Matter Inelastic scattering XENON Direct Dark MatterPhysicsphotonAstrophysics::Instrumentation and Methods for AstrophysicsDirect Dark MatterWeakly interacting massive particlesastro-ph.COsignatureAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsInelastic scatteringCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesWIMP: massAstrophysics::Cosmology and Extragalactic AstrophysicsInelastic scatteringNOPE2_2PE2_10103 physical sciencesddc:530010306 general physics010308 nuclear & particles physicsScatteringWIMP nucleus: interactionDarkmatterWIMP: interactionHigh Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics and astroparticle physicsexperimental resultsPhysical Review D. Particles, Fields, Gravitation, and Cosmology
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