Search results for "XENON"

showing 10 items of 172 documents

Status of new 18 GHz ECRIS HIISI

2018

A new 18 GHz ECR ion source HIISI is under commissioning at the Accelerator Laboratory at the University of Jyvaskyla (JYFL). The main purpose of HIISI is to produce high-energy beam cocktails, e.g. Xe44+, for radiation effects testing of electronics with the K130 cyclotron. The initial commissioning results in 18+14 GHz operation with oxygen, argon and xenon are reported. The beam currents are compared to those produced by reference ion sources (JYFL 14 GHz ECRIS, GTS and SuSI). At the moment (October 2017) 560 µA of O6+ and 310 µA of Ar13+, for example, have been reached with HIISI at 2.3 kW total power.A new 18 GHz ECR ion source HIISI is under commissioning at the Accelerator Laboratory…

University of JyväskyläMaterials scienceCyclotrontutkimuslaitteetchemistry.chemical_elementRadiation01 natural sciences7. Clean energy010305 fluids & plasmasIonlaw.inventionNuclear physicsXenonHIISIlaw0103 physical sciencesheavy ion ion source injector010302 applied physicsArgonta114syklotronitIon sourcechemistrysäteilyfysiikkaMoment (physics)ionsaccelerator laboratoryBeam (structure)
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Electronic spectroscopy of I2–Xe complexes in solid Krypton

2012

In the present work, we have studied ion-pair states of matrix-isolated I(2) with vacuum-UV absorption and UV-vis-NIR emission, where the matrix environment is systematically changed by mixing Kr with Xe, from pure Kr to a more polarizable Xe host. Particular emphasis is put on low doping levels of Xe that yield a binary complex I(2)-Xe, as verified by coherent anti-Stokes Raman scattering (CARS) measurements. Associated with interaction of I(2) with Xe we can observe strong new absorption in vacuum-UV, redshifted 2400 cm(-1) from the X → D transition of I(2). Observed redshift can be explained by symmetry breaking of ion-pair states within the I(2)-Xe complex. Systematic Xe doping of Kr ma…

Valence (chemistry)KryptonDopingGeneral Physics and Astronomychemistry.chemical_elementElectron spectroscopysymbols.namesakeXenonchemistryPolarizabilitysymbolsPhysical and Theoretical ChemistryAtomic physicsta116Electron scatteringRaman scatteringThe Journal of Chemical Physics
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Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector

2017

International audience; We report on weakly interacting massive particles (WIMPs) search results in the XENON100 detector using a nonrelativistic effective field theory approach. The data from science run II (34  kg×224.6 live days) were reanalyzed, with an increased recoil energy interval compared to previous analyses, ranging from (6.6–240)  keVnr. The data are found to be compatible with the background-only hypothesis. We present 90% confidence level exclusion limits on the coupling constants of WIMP-nucleon effective operators using a binned profile likelihood method. We also consider the case of inelastic WIMP scattering, where incident WIMPs may up-scatter to a higher mass state, and …

WIMP nucleon: scatteringParticle physicsdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsWIMP[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matterchemistry.chemical_elementFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesNuclear physicsXENONXenonWIMPstatistical analysis0103 physical sciencesEffective field theoryDark Matter010306 general physicsS030UDMnucleus: recoilPhysicsCoupling constanteffective field theory: nonrelativistic010308 nuclear & particles physicsScatteringDetectorAstrophysics::Instrumentation and Methods for Astrophysicsdark matter: detectorchemistryWeakly interacting massive particlesDirect SearchHigh Energy Physics::ExperimentTPC[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]recoil: energyAstrophysics - Cosmology and Nongalactic Astrophysics
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Projected WIMP sensitivity of the XENONnT dark matter experiment

2020

XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 ± 0.6 (keV t y)-1 and (2.2± 0.5)× 10−3 (keV t y)-1, respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage…

WIMP nucleon: scatteringdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsHadronDark matterFOS: Physical sciencesElementary particledark matter: direct detection01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentNONuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONPE2_2WIMPPE2_1electron: recoil0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPE2_4Dark matter experimentComputingMilieux_MISCELLANEOUSactivity reportnucleus: recoilPhysicsxenon: liquid010308 nuclear & particles physicsbackgroundAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Dark matter experiments dark matter simulationssensitivityBaryonDark matter experimentsDark matter simulationsWeakly interacting massive particlesDark matter experiments; Dark matter simulationsNucleon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Encapsulation of Xenon by a Self-Assembled Fe4L6 Metallosupramolecular Cage

2015

We report (129)Xe NMR experiments showing that a Fe4L6 metallosupramolecular cage can encapsulate xenon in water with a binding constant of 16 M(-1). The observations pave the way for exploiting metallosupramolecular cages as economical means to extract rare gases as well as (129)Xe NMR-based bio-, pH, and temperature sensors. Xe in the Fe4L6 cage has an unusual chemical shift downfield from free Xe in water. The exchange rate between the encapsulated and free Xe was determined to be about 10 Hz, potentially allowing signal amplification via chemical exchange saturation transfer. Computational treatment showed that dynamical effects of Xe motion as well as relativistic effects have signific…

Xenon010405 organic chemistryChemistryChemical exchangechemistry.chemical_elementGeneral Chemistry010402 general chemistry01 natural sciencesBiochemistryBinding constantCatalysis0104 chemical sciencesSelf assembledColloid and Surface ChemistryXenon13. Climate actionComputational chemistrySaturation transferChemical physicsmetallosupramolecular cagesmolecular encapsulationCageRelativistic quantum chemistrySignal amplificationta116Journal of the American Chemical Society
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Analytical measurements of fission products during a severe nuclear accident

2018

The Fukushima accident emphasized the fact that ways to monitor in real time the evolution of a nuclear reactor during a severe accident remain to be developed. No fission products were monitored during twelve days; only dose rates were measured, which is not sufficient to carry out an online diagnosis of the event. The first measurements were announced with little reliability for low volatile fission products. In order to improve the safety of nuclear plants and minimize the industrial, ecological and health consequences of a severe accident, it is necessary to develop new reliable measurement systems, operating at the earliest and closest to the emission source of fission products. Throug…

Xenon010504 meteorology & atmospheric sciencesQC1-999Nuclear engineeringFission productsNuclear plant01 natural sciences7. Clean energyRutheniumsevere accidentlaw.inventionlaw0103 physical sciencesfission productsrutheniumSevere accidentkrypton0105 earth and related environmental sciencesFission products010304 chemical physicsHealth consequencesiodinePhysicsKryptonGénéralitésNuclear reactorMolecular spectroscopyxenonAccident managementNuclear reactor coreContainment13. Climate actionmolecular spectroscopyEnvironmental scienceDose rateIodineEPJ Web of Conferences
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Online 222 Rn removal by cryogenic distillation in the XENON100 experiment

2017

We describe the purification of xenon from traces of the radioactive noble gas radon using a cryogenic distillation column. The distillation column was integrated into the gas purification loop of the XENON100 detector for online radon removal. This enabled us to significantly reduce the constant 222 Rn background originating from radon emanation. After inserting an auxiliary 222 Rn emanation source in the gas loop, we determined a radon reduction factor of R>27 (95% C.L.) for the distillation column by monitoring the 222 Rn activity concentration inside the XENON100 detector.

XenonPhysics and Astronomy (miscellaneous)WimpDirect SearchDark MatterTPCEngineering (miscellaneous)European Physical Journal C
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First Dark Matter Search Results from the XENON1T Experiment

2017

We report the first dark matter search results from XENON1T, a ∼2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042±12)-kg fiducial mass and in the [5,40] keVnr energy range of interest for weakly interacting massive particle (WIMP) dark matter searches, the electronic recoil background was (1.93±0.25)×10-4 events/(kg×day×keVee), the lowest ever achieved in such a dark matter detector. A profile likelihood analysis shows that the data are consisten…

Xenon[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Massive particleGeneral Physics and Astronomy01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)RecoilXenonWIMPS046DM2[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]PhysicsRange (particle radiation)Time projection chamberDetectorHigh Energy Physics - Phenomenologydark matter: scatteringTPCAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPDark matterFOS: Physical scienceschemistry.chemical_elementWIMP: massS030DI2Nuclear physicsPhysics and Astronomy (all)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesrecoil[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physique010308 nuclear & particles physicsbackgrounddark matter: detectorAstronomieGran SassochemistryDirect Searchtime projection chamber: xenoninterpretation of experiments: XENON[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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On-Line Measurement of Gaseous Iodine Species During a PWR Severe Accident

2015

International audience; Iodine is a highly radio-toxic element, due to its affinity to the thyroid, and represents the major part of the radioactivity released during a nuclear accident. In the context of nuclear safety and radio-protection, we are interested in identifying the iodine gaseous species which are released, in the nuclear power plants, under molecular (I$_2$) and organic (CH$_3$I) forms. Therefore, we are working on providing a spectroscopic database for both species. While the infrared spectrum of the ν6 band of methyl iodide was previously studied, only 4000 lines were assigned. We present the rovibrational analysis of a high quality experimental spectrum, of this band, recor…

[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th]Fission productsRadionuclide[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]business.industry[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear engineeringchemistry.chemical_elementInternational Nuclear Event ScaleNuclear power[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Iodinecomplex mixtures7. Clean energyAerosolXenonchemistryCaesiumEnvironmental sciencebusiness
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Hyperfine structure of some near-infrared Xe I and Xe II lines

2011

International audience; This work reports on the experimental determination of the hyperfine splitting of the Xe I lines at 828.01 nm and 834.68 nm and the Xe II line at 834.72 nm. Measurements were performed by means of Doppler-free saturation spectroscopy in a low-pressure radio-frequency discharge. The absolute wavelength of all hyperfine components is obtained by way of a high-precision wavemeter backed-up with the absorption spectrum of the NO 2 molecule. We provide an accurate estimate of hyperfine constants for the lower level of the Xe II transition at 834.72 nm. The two Xe I transition outcomes of our experimental study are compared with data available in the literature.

[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Absorption spectroscopyNear-infrared spectroscopychemistry.chemical_element01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasAnalytical ChemistryWavelengthXenonchemistry[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]0103 physical sciencesAtomic physics010306 general physicsSpectroscopyInstrumentationSaturation (magnetic)Hyperfine structureSpectroscopyLine (formation)
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