Search results for "Experiments"

showing 10 items of 435 documents

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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Effect of pH and nitrite concentration on nitrite oxidation rate

2011

The effect of pH and nitrite concentration on the activity of the nitrite oxidizing bacteria (NOB) in an activated sludge reactor has been determined by means of laboratory batch experiments based on respirometric techniques. The bacterial activity was measured at different pH and at different total nitrite concentrations (TNO 2). The experimental results showed that the nitrite oxidation rate (NOR) depends on the TNO 2 concentration independently of the free nitrous acid (FNA) concentration, so FNA cannot be considered as the real substrate for NOB. NOB were strongly affected by low pH values (no activity was detected at pH 6.5) but no inhibition was observed at high pH values (activity wa…

Waste component removalPH rangeUnclassified drugRespirometric techniqueLaboratory methodPHOxidation ratesPH valueNitriteSaturation constantBatch reactorPH effectOxidation kineticsDissociation constantNitrobacterKinetic expressionWaste Disposal FluidInhibition constantschemistry.chemical_compoundBacteriumBioreactorsNitrous acidNitriteBacterial activityReaction kineticsBacteria (microorganisms)Waste Management and DisposalIn Situ Hybridization FluorescenceInhibitionPriority journalFree nitrous acidMicroscopyNitrous acidSewagebiologyFluorescence in situ hybridizationPH effectsGeneral MedicineSaturationRespirometryHydrogen-Ion ConcentrationInorganic acidsNitrite oxidizing bacteriaCalibrationOxidation-ReductionEnvironmental EngineeringInorganic chemistryBioreactorParameterizationBioengineeringActivated sludge reactorsArticleNumerical modelNitrous acid derivativeReaction rateParameter calibrationBatch experimentsNitrite-oxidizing bacteriaOxidationDietary NitrateNitritesTECNOLOGIA DEL MEDIO AMBIENTEExperimental studyBacteriaConcentration (process)Renewable Energy Sustainability and the EnvironmentBacteriologyNitrobacterOxidation reductionNitrogen removalConcentration (composition)biology.organism_classificationInorganic acidsMicrobial activityKineticschemistryActivated sludgeNitrite oxidationHigh pH valueSwitch functionConcentration (parameters)Oxidation processEffect of pHProtein expressionSubstrateControlled studyWaste disposalBioresource Technology
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Enhanced calculation of optimal gradient programs in reversed-phase liquid chromatography

2003

Abstract The resolution of a mixture of 16 β-blockers under gradient elution was optimised using both isocratic and gradient training sets, with a reversed-phase column and acetonitrile–water eluents. Error theory was applied to measure the information extracted from different gradient experimental designs. This allows checking the expected accuracy when gradient predictions exceed the initial solvent concentrations tested in the training set. This work applies the results on modelling found in a previous study [J. Chromatogr. A 1018 (2003) 169] where the performance of several retention models was compared. Enhanced retention predictions were applied to the optimisation of gradient program…

Work (thermodynamics)ChromatographyResolution (mass spectrometry)ChemistryElutionDesign of experimentsOrganic ChemistryAnalytical chemistryGeneral MedicineReversed-phase chromatographyCurvatureBiochemistryHigh-performance liquid chromatographyAnalytical ChemistryChromatography High Pressure LiquidSpectral purityJournal of Chromatography A
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Testing experimental designs in liquid chromatography (I): Development and validation of a method for the comprehensive inspection of experimental de…

2020

The basis of interpretive optimisation in liquid chromatography is the prediction of resolution, from appropriate solute retention models. The reliability of the process depends critically on the quality of the experimental design. This work develops, validates and applies a general methodology aimed to evaluate the quality of any training experimental design, which will be applied in Part II to design optimisation. The methodology is based on the systematic evaluation of the uncertainties associated to the prediction of retention times in comprehensive scans of both isocratic and gradient experimental conditions. It is able to evaluate comprehensively experimental designs of arbitrary comp…

Work (thermodynamics)SulfonamidesChromatographyBasis (linear algebra)ChemistryDesign of experiments010401 analytical chemistryOrganic ChemistryProcess (computing)General Medicine010402 general chemistry01 natural sciencesBiochemistry0104 chemical sciencesAnalytical ChemistrySet (abstract data type)NK modelResearch DesignSolventsLack-of-fit sum of squaresHydrophobic and Hydrophilic InteractionsReliability (statistics)Chromatography LiquidJournal of chromatography. A
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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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Bekämpfung der Alterserscheinungen durch teilweises Zerreissen und Zerdrücken des Hodengewebes: die über 3½ Jahre andauernde Operationswirkung bei Hu…

1933

Teksts vācu valodā, kopsavilkums latviešu valodā.

Zoology experimentalAnimal experimentsDzīvnieku eksperimentiTierversucheZoologie experimentellTierphysiologieDzīvnieku fizioloģija:NATURAL SCIENCES::Biology::Organism biology::Animal physiology [Research Subject Categories]Zooloģija eksperimentālā
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Abnormalities caused by chloroform and ether in the spermatogenesis of mammals [Chloroforma un ētera radītie traucējumi zīdītāju spermatogenezē]

1937

Teksts angļu valodā, kopsavilkums latviešu valodā.

Zoology experimentalAnimal experimentsPeles - eksperimentiDzīvnieku eksperimentiZīdītāju spermatogeneze - eksperimenti:NATURAL SCIENCES::Biology::Organism biology::Morphology [Research Subject Categories]Mammalian spermatogenesis - experimentsZooloģija eksperimentālā
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The effects of unilateral castration on the remaining testicle of the dog [Vienpusējas kastrācijas iespaids uz ķermenī palikušo sēklinieku]

1937

Teksts angļu valodā, kopsavilkums latviešu valodā.

Zoology experimentalDzīvnieku eksperimentiSuņi - eksperimentiDogs - experimentsSuņu anatomija un morfoloģija:NATURAL SCIENCES::Biology::Organism biology::Morphology [Research Subject Categories]Zooloģija eksperimentālāDzīvnieku morfoloģija
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Interconnecteurs métalliques de piles à combustible de type SOFC - Résistance à la corrosion et conductivité électrique à haute température

2009

The need of interconnect to connect individual cells into electrical series in a SOFC stack appears as one of the most important point in fuel cell technology. The main important criteria requires for interconnect is an excellent oxidation resistance in air and in H2/H2O. The goal of this study is to determine the influence on corrosion behaviour of a reactive element oxide coating (La2O3, Y2O3) realized by MOCVD on different metallic alloys like Crofer22APU, Haynes230 and Fe30Cr. The realisation of long ageing (7 700 and 15 400 hours) proved to be insightful. The corrosion kinetic experiments, the oxide scale characterisation and ASR measurements established that the presence of perovskite…

[CHIM.MATE] Chemical Sciences/Material chemistryHigh temperature corrosionMetallic InterconnectsInterconnecteurs métalliques[CHIM.MATE]Chemical Sciences/Material chemistryÉléments réactifsReactive elementsASRVapeur d'eau[ CHIM.MATE ] Chemical Sciences/Material chemistryMOCVDwater vapouCorrosion haute températureMarquage isotopiqueSOFCTwo stage oxidation experiments
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Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory

2013

We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 – 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 – 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Ciencias FísicasAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesultra-high energy cosmic raysCosmic rayAstrophysicsultra high energy cosmic raysAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAugerNUMBERObservatoryCosmic ray experiments0103 physical sciencesultra-high energy cosmic rayUltra-high-energy cosmic ray010303 astronomy & astrophysicsDETECTORLuminosity functionPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)FÍSICA DE PARTÍCULASRange (particle radiation)SPECTRUMCosmologia010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsUltra high energy cosmic raysAstronomíaLUMINOSITY FUNCTIONMagnitude (astronomy)Experimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstronomiaFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical Phenomenacosmic ray experiments; ultra high energy cosmic raysCIENCIAS NATURALES Y EXACTAS
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