Search results for "Xenon"

showing 10 items of 172 documents

Discovery potential of xenon-based neutrinoless double beta decay experiments in light of small angular scale CMB observations

2013

The South Pole Telescope (SPT) has probed an expanded angular range of the CMB temperature power spectrum. Their recent analysis of the latest cosmological data prefers nonzero neutrino masses, with Sigma m(nu) = (0.32 +/- 0.11) eV. This result, if con firmed by the upcoming Planck data, has deep implications on the discovery of the nature of neutrinos. In particular, the values of the effective neutrino mass m(beta beta) involved in neutrinoless double beta decay (beta beta 0 nu) are severely constrained for both the direct and inverse hierarchy, making a discovery much more likely. In this paper, we focus in xenon-based beta beta 0 nu experiments, on the double grounds of their good perfo…

AstrofísicaPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsCosmic microwave backgroundchemistry.chemical_elementdouble beta decayFOS: Physical sciences7. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicssymbols.namesakeHigh Energy Physics - Experiment (hep-ex)XenonHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesPlanck010306 general physicsPhysicsCosmologiaTime projection chamber010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsneutrino masses from cosmologyInstrumentation and Detectors (physics.ins-det)3. Good healthHigh Energy Physics - PhenomenologyMAJORANASouth Pole Telescopechemistry13. Climate actionsymbolsNeutrino
researchProduct

Treatment of scalar-relativistic effects on nuclear magnetic shieldings using a spin-free exact-two-component approach.

2013

A cost-effective treatment of scalar-relativistic effects on nuclear magnetic shieldings based on the spin-free exact-two-component theory in its one-electron variant (SFX2C-1e) is presented. The SFX2C-1e scheme gains its computational efficiency, in comparison to the four-component approach, from a focus on spin-free contributions and from the elimination of the small component. For the calculation of nuclear magnetic shieldings, the separation of spin-free and spin-dependent terms in the parent four-component theory is carried out here for the matrix representation of the Dirac equation in terms of a restricted-magnetically balanced gauge-including atomic orbital basis. The resulting spin…

ChemistryMatrix representationGeneral Physics and Astronomychemistry.chemical_elementIonsymbols.namesakeXenonAtomic orbitalMolybdenum compoundsDirac equationQuantum mechanicssymbolsPhysical and Theoretical ChemistryAtomic physicsHamiltonian (quantum mechanics)Relativistic quantum chemistryThe Journal of chemical physics
researchProduct

Installation of Amine Moieties into a Polycyclic Anodic Product Derived from 2,4-Dimethylphenol

2011

When 2,4-dimethylphenol is anodically treated, a dehydrotetramer with four contiguous stereocentres is readily obtained on a multi-gram scale. The substitution of a 2,4-dimethyl-phenoxy fragment by several amines was demonstrated, and the best results were obtained with primary amines. Optically pure α-chiral aliphatic amines yield diastereomeric mixtures that can be separated in most cases. The basic amine causes a partial hemiketal-opening of the bisbenzofuran moiety leading to an equilibrium within an α,β-unsaturated cyclohexenone. This dynamic behaviour occurs on the time scale of NMR spectroscopy and is also found by X-ray analysis providing a consistent picture.

ChemistryOrganic ChemistryDiastereomerGeneral ChemistryNuclear magnetic resonance spectroscopyCatalysisChiral resolutionchemistry.chemical_compoundCyclohexenoneYield (chemistry)MoietyOrganic chemistryAmine gas treatingAminationChemistry - A European Journal
researchProduct

Formation of HXeO in a xenon matrix: Indirect evidence of production, trapping, and mobility of XeO (1 1Σ+) in solid Xe

2004

IR spectroscopy, laser induced fluorescence (LIF), and thermoluminescence (TL) measurements have been combined to monitor trapping, thermal mobility, and reactions of oxygen atoms in solid xenon. HXeO and O(3) have been used as IR active species that probe the reactions of oxygen atoms. N(2)O and H(2)O have been used as precursors for oxygen atoms by photolysis at 193 nm. Upon annealing of matrices after photolysis, ozone forms at two different temperatures: at 18-24 K from close O ...O(2) pairs and at approximately 27 K due to global mobility of oxygen atoms. HXeO forms at approximately 30 K reliably at higher temperature than ozone. Both LIF and TL show activation of oxygen atoms around 3…

ChemistrySinglet oxygenRadicalPhotodissociationAnalytical chemistryAtomic emission spectroscopyGeneral Physics and Astronomychemistry.chemical_elementInfrared spectroscopychemistry.chemical_compoundXenonIrradiationPhysical and Theoretical ChemistryLaser-induced fluorescenceThe Journal of Chemical Physics
researchProduct

Microstructural evolution of gas hydrates in sedimentary matrices observed with synchrotron X-ray computed tomographic microscopy

2015

The formation process of gas hydrates in sedimentary matrices is of crucial importance for the physical and transport properties of the resulting aggregates. This process has never been observed in situ at submicron resolution. Here we report on synchrotron-based microtomographic studies by which the nucleation and growth processes of gas hydrate were observed at 276 K in various sedimentary matrices such as natural quartz (with and without admixtures of montmorillonite type clay) or glass beads with different surface properties, at varying water saturation. Both juvenile water and metastably gas-enriched water obtained from gas hydrate decomposition was used. Xenon gas was employed to enha…

Clathrate hydrateNucleationMineralogychemistry.chemical_elementMicrostructureMicrometrechemistry.chemical_compoundGeophysicsMontmorilloniteXenonchemistryGeochemistry and PetrologySedimentary rockPhysics::Chemical PhysicsQuartzGeologyGeochemistry, Geophysics, Geosystems
researchProduct

Neutral-Current Neutrino-Nucleus Scattering off Xe Isotopes

2018

Large liquid xenon detectors aiming for dark matter direct detection will soon become viable tools also for investigating neutrino physics. Information on the effects of nuclear structure in neutrino-nucleus scattering can be important in distinguishing neutrino backgrounds in such detectors. We perform calculations for differential and total cross sections of neutral-current neutrino scattering off the most abundant xenon isotopes. The nuclear structure calculations are made in the nuclear shell model for elastic scattering, and also in the quasiparticle random-phase approximation (QRPA) and microscopic quasiparticle phonon model (MQPM) for both elastic and inelastic scattering. Using suit…

Computer Science::Machine LearningNuclear and High Energy PhysicsArticle SubjectNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaDark matterNuclear TheoryFOS: Physical sciencesInelastic scatteringComputer Science::Digital Libraries01 natural sciencesNuclear Theory (nucl-th)Nuclear physicsStatistics::Machine LearningHigh Energy Physics - Phenomenology (hep-ph)neutrino physics0103 physical sciencesIsotopes of xenonsironta010306 general physicsPhysicsElastic scatteringneutrino-nucleus scatteringta114010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyNuclear shell modelneutriinotlcsh:QC1-999High Energy Physics - PhenomenologyComputer Science::Mathematical SoftwareHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsAdvances in High Energy Physics
researchProduct

Dark matter results from 225 live days of XENON100 data

2012

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso (LNGS) for 13 months during 2011 and 2012. XENON100 features an ultra-low electromagnetic background of (5.3 \pm 0.6) \times 10^-3 events (kg day keVee)^-1 in the energy region of interest. A blind analysis of 224.6 live days \times 34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the pre-defined nuclear recoil energy range of 6.6-30.5 keVnr are consistent with the background expectation of (1.0 \pm 0.2) events. A Profile Likelihood analysis using a 6.6-43.3 keVnr energy range sets the most stringent limit o…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsLarge Underground Xenon experimentDark matterFOS: Physical sciencesGeneral Physics and AstronomyWIMP Argon Programme01 natural sciences7. Clean energyParticle detectorHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences[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 physicsLiquid XenonPhysicsRange (particle radiation)010308 nuclear & particles physicsDARK MATTERInstrumentation and Detectors (physics.ins-det)High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]DAMA/NaITPCPandaXDirect search for Dark MatterAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
researchProduct

A low-mass dark matter search using ionization signals in XENON100

2016

We perform a low-mass dark matter search using an exposure of 30\,kg$\times$yr with the XENON100 detector. By dropping the requirement of a scintillation signal and using only the ionization signal to determine the interaction energy, we lowered the energy threshold for detection to 0.7\,keV for nuclear recoils. No dark matter detection can be claimed because a complete background model cannot be constructed without a primary scintillation signal. Instead, we compute an upper limit on the WIMP-nucleon scattering cross section under the assumption that every event passing our selection criteria could be a signal event. Using an energy interval from 0.7\,keV to 9.1\,keV, we derive a limit on …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSignalHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMPIonization0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsPhysicsScintillation010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)Physics and Astronomy (miscellaneous) DARK MATTER XENON TPC WIMPHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Scintillation counterEnergy (signal processing)Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

HP-Xe to go: Storage and Transportation of Hyperpolarized 129-Xe

2016

Abstract Recently the spin–lattice relaxation time T 1 of hyperpolarized (HP)- 129 Xe was significantly improved by using uncoated and Rb-free storage vessels of GE180 glass. For these cells, a simple procedure was established to obtain reproducible wall relaxation times of about 18 h. Then the limiting relaxation mechanism in pure Xe is due to the coupling between the nuclear spins and the angular momentum of the Xe–Xe van-der-Waals-molecules. This mechanism can be significantly reduced by using different buffer gases of which CO 2 was discovered to be the most efficient so far. From these values, it was estimated that for a 1:1 mixture of HP-Xe with CO 2 a longitudinal relaxation time of …

CouplingNuclear and High Energy PhysicsAngular momentumSpinsCondensed matter physicsChemistryRelaxation (NMR)BiophysicsAnalytical chemistrychemistry.chemical_element010402 general chemistryCondensed Matter Physics01 natural sciencesBiochemistry0104 chemical sciencessymbols.namesakeXenon0103 physical sciencessymbolsvan der Waals forceTotal pressure010306 general physicsLongitudinal Relaxation Time
researchProduct

Removing krypton from xenon by cryogenic distillation to the ppq level

2017

The XENON1T experiment aims for the direct detection of dark matter in a detector filled with 3.3 tons of liquid xenon. In order to achieve the desired sensitivity, the background induced by radioactive decays inside the detector has to be sufficiently low. One major contributor is the β-emitter 85Kr which is present in the xenon. For XENON1T a concentration of natural krypton in xenon natKr/Xe<200ppq (parts per quadrillion, 1ppq=10-15mol/mol) is required. In this work, the design, construction and test of a novel cryogenic distillation column using the common McCabe–Thiele approach is described. The system demonstrated a krypton reduction factor of 6.4 · 10 5 with thermodynamic stability a…

CryostatPhysics - Instrumentation and DetectorsXenonPhysics and Astronomy (miscellaneous)WIMPDark matterAnalytical chemistryFOS: Physical scienceschemistry.chemical_elementlcsh:AstrophysicsWeakly Interact Massive ParticleSciences de l'ingénieur01 natural sciences7. Clean energyXenonlcsh:QB460-4660103 physical sciencesDark Matterlcsh:Nuclear and particle physics. Atomic energy. RadioactivitySensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsComputer science information & general worksEngineering (miscellaneous)Liquid XenonComputingMilieux_MISCELLANEOUSPhysicsAir separationPhysique010308 nuclear & particles physicsDistillation ColumnKryptonKryptonOrder (ring theory)Instrumentation and Detectors (physics.ins-det)AstronomiechemistryDirect Searchddc:000lcsh:QC770-798TPCOrder of magnitude
researchProduct