Search results for "Dark matter experiment"

showing 9 items of 39 documents

Applicability of a simple model for computing diffuse solar radiation to locations of the European, African, Asian and North American areas

1992

Abstract It is tested if the correlation type D = K(s/S)−0.25 (sin hn)1.55, 0.2 ⩽ s/S ⩽ 0.9 previously proposed by Coppolino for Italian locations using K = 7.0, allows a reliable estimation of the monthly mean daily diffuse solar radiation D (MJ m−2 day−1), from only the monthly mean daily relative sunshine s/S and the noon altitude of the sun on the 15th of the month hn (degrees) at locations of the European, African, Asian and North American areas. The test is performed at 14 stations in the above areas displaced at various latitudes L, elevations above sea level E and geographical situations, using K = 7.0 for the stations where 0.48 ⩽ (s/S)m, ⩽ 0.63, K = 8.5 for those where 0.40 ⩽ (s/S…

SIMPLE (dark matter experiment)AltitudeGeographyMeteorologyRenewable Energy Sustainability and the EnvironmentNoonAtmospheric sciencesSea levelLatitudeRenewable Energy
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A simple analysis of the HA centre destruction temperatures for doped alkali halides

1998

Abstract A simple relation for the destruction temperatures Td of the HA centres (H centres trapped by an impurity cation) as a function of the difference in the radii for a host cation and impurity in alkali halide crystals is presented and theoretically justified. This relation allows to predict Td for H centres trapped by other monovalent cation impurities.

SIMPLE (dark matter experiment)ChemistryDopingInorganic chemistryHalideGeneral ChemistryCondensed Matter PhysicsAlkali metalCondensed Matter::Materials ScienceImpurityCondensed Matter::SuperconductivityPhysics::Atomic and Molecular ClustersMaterials ChemistryPhysical chemistryPhysics::Atomic PhysicsPhysics::Chemical PhysicsSolid State Communications
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A very simple model for computing global solar radiation

1990

Abstract In this paper a very simple model for predicting the daily global solar radiation at any Italian location using as input of a few extensively measured meterological parameters is proposed. In fact the daily radiation G (MJ m−2) is here correlated only with the sunshine duration s (h) and the noon altitude of the sun on the 15th of the month h n (degrees) by the following equation: G= Ks 0.5 (sin h n ) 1.15 where only one value of the factor K is used. The validity of this formula is verified fixing K = 7.8 and using the data from 34 Italian stations displaced at various latitudes, altitudes or geographical situations (inland or coastal site). The test results show that the deviatio…

SIMPLE (dark matter experiment)Global solar radiationAltitudeMeteorologySunshine durationGeneral EngineeringMicroclimateNoonMaximum errorMathematicsLatitudeSolar & Wind Technology
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Simple, Fast, Bright, and Stable Light Sources

2012

In this work we show that solution-processed light-emitting electrochemical cells (LECs) based on only an ionic iridium complex and a small amount of ionic liquid exhibit exceptionally good performances when applying a pulsed current: sub-second turn-on times and almost constant high luminances (>600 cd m(-2) ) and power efficiencies over the first 600 h. This demonstrates the potential of LECs for applications in solid-state signage and lighting.

SIMPLE (dark matter experiment)Materials scienceLightbusiness.industryMechanical EngineeringAnalytical chemistryTin Compoundschemistry.chemical_elementIonic bondingElectrochemical TechniquesEquipment DesignThiophenesIridiumElectrochemical cellchemistry.chemical_compoundchemistryCoordination ComplexesMechanics of MaterialsIonic liquidPolystyrenesOptoelectronicsGeneral Materials ScienceGlassIridiumbusinessAdvanced Materials
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The relaxation dynamics of a simple glass former confined in a pore

2000

We use molecular dynamics computer simulations to investigate the relaxation dynamics of a binary Lennard-Jones liquid confined in a narrow pore. We find that the average dynamics is strongly influenced by the confinement in that time correlation functions are much more stretched than in the bulk. By investigating the dynamics of the particles as a function of their distance from the wall, we can show that this stretching is due to a strong dependence of the relaxation time on this distance, i.e. that the dynamics is spatially very heterogeneous. In particular we find that the typical relaxation time of the particles close to the wall is orders of magnitude larger than the one of particles …

SIMPLE (dark matter experiment)Materials scienceStatistical Mechanics (cond-mat.stat-mech)Relaxation (NMR)Dynamics (mechanics)General Physics and AstronomyFOS: Physical sciencesFunction (mathematics)Disordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksTime correlationMolecular dynamicsOrders of magnitude (time)Chemical physicsCondensed Matter - Statistical Mechanics
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A simple low-cost highly reproducible method of fabricating optical fiber tips for a photon scanning tunneling microscope

1996

SIMPLE (dark matter experiment)Optical fiberMaterials scienceMicroscopePhotonbusiness.industryCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectrochemical scanning tunneling microscopeElectronic Optical and Magnetic Materialslaw.inventionScanning probe microscopyOpticslawElectrical and Electronic EngineeringScanning tunneling microscopebusinessMicrowave and Optical Technology Letters
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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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Physics reach of the XENON1T dark matter experiment.

2016

The XENON1T experiment is currently in the commissioning phase at the Laboratori Nazionali del Gran Sasso, Italy. In this article we study the experiment's expected sensitivity to the spin-independent WIMP-nucleon interaction cross section, based on Monte Carlo predictions of the electronic and nuclear recoil backgrounds. The total electronic recoil background in $1$ tonne fiducial volume and ($1$, $12$) keV electronic recoil equivalent energy region, before applying any selection to discriminate between electronic and nuclear recoils, is $(1.80 \pm 0.15) \cdot 10^{-4}$ ($\rm{kg} \cdot day \cdot keV)^{-1}$, mainly due to the decay of $^{222}\rm{Rn}$ daughters inside the xenon target. The nu…

dark matter simulationsPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsdark matter experimentFOS: Physical scienceschemistry.chemical_elementCosmic ray7. Clean energy01 natural sciencesdark matter simulationNuclear physicsRecoilXenonIonization0103 physical sciencesNeutronNuclear Experiment010306 general physicsPhysicsMuon010308 nuclear & particles physicsdark matter experimentsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)dark matter experiments; dark matter simulationschemistryNeutrinoNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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A new simple chromo-fluorogenic probe for NO2 detection in air.

2015

[EN] A new chromo-fluorogenic probe, consisting of a biphenyl derivative containing both a silylbenzyl ether and a N,N-dimethylamino group, for NO2 detection in the gas phase has been developed. A clear colour change from colourless to yellow together with an emission quenching was observed when the probe reacted with NO2. A limit of detection to the naked eye of about 0.1 ppm was determined and the system was successfully applied to the detection of NO2 in realistic atmospheric conditions.

inorganic chemicalsGas phase reactionsAnalytical chemistryEtherPhotochemistryNO2Nitric Oxidecomplex mixturesCatalysisGas phasechemistry.chemical_compoundQUIMICA ORGANICAChromogenic detectionFluorescent DyesDetection limitBiphenylEmission quenchingSIMPLE (dark matter experiment)Molecular StructureSensorsAirOrganic ChemistryQUIMICA INORGANICAGeneral Chemistryrespiratory systemchemistryChromogenic CompoundsNaked eyeDerivative (chemistry)Chemistry (Weinheim an der Bergstrasse, Germany)
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