Search results for "Physical Sciences"

showing 10 items of 20240 documents

On the convergence of zero-point vibrational corrections to nuclear shieldings and shielding anisotropies towards the complete basis set limit in wat…

2016

The method and basis set dependence of zero-point vibrational corrections (ZPVCs) to nuclear magnetic resonance shielding constants and anisotropies has been investigated using water as a test system. A systematic comparison has been made using the Hartree–Fock, second-order Møller–Plesset perturbation theory (MP2), coupled cluster singles and doubles (CCSD), coupled cluster singles and doubles with perturbative triples corrections (CCSD(T)) and Kohn–Sham density functional theory with the B3LYP exchange-correlation functional methods in combination with the second-order vibrational perturbation theory (VPT2) approach for the vibrational corrections. As basis sets, the correlation consisten…

waterBiophysicsZero-point energyzero-point vibrational correctionMonotonic function010402 general chemistry01 natural sciencesQuantum mechanics0103 physical sciencesPhysics::Atomic and Molecular ClustersCCSD(T)Limit (mathematics)complete basis set limitPhysics::Chemical PhysicsPhysical and Theoretical ChemistryMolecular BiologyBasis setPhysics010304 chemical physicsBasis (linear algebra)Condensed Matter PhysicsNMR shielding constant0104 chemical sciencesCoupled clusterDensity functional theoryPerturbation theory (quantum mechanics)Molecular Physics
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Few-body insights of multiquark exotic hadrons

2018

In this contribution we discuss the adequate treatment of the $4-$ and $5-$body dynamics within a constituent quark framework. We stress that the variational and Born-Oppenheimer approximations give energies rather close to the exact ones, while the diquark approximation might be rather misleading. Hall-Post inequalities provide very useful lower bounds that exclude possible stable states for some mass ratios and color wave functions.

wave functionhadron: exoticBorn–Oppenheimer approximationConstituent quarkFOS: Physical sciences01 natural sciencesStability (probability)symbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)multiquarkquark: constituent0103 physical sciences010306 general physicsWave functionBorn-Oppenheimer approximationStable statePhysics010308 nuclear & particles physicsExotic hadronMass ratiostabilityDiquarkHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]symbolsapproximation: diquarkmass ratio
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Effect of Boron Doping on the Wear Behavior of the Growth and Nucleation Surfaces of Micro- and Nanocrystalline Diamond Films

2016

B-doped diamond has become the ultimate material for applications in the field of microelectromechanical systems (MEMS), which require both highly wear resistant and electrically conductive diamond films and microstructures. Despite the extensive research of the tribological properties of undoped diamond, to date there is very limited knowledge of the wear properties of highly B-doped diamond. Therefore, in this work a comprehensive investigation of the wear behavior of highly B-doped diamond is presented. Reciprocating sliding tests are performed on micro- and nanocrystalline diamond (MCD, NCD) films with varying B-doping levels and thicknesses. We demonstrate a linear dependency of the we…

wearMaterials sciencereciprocating slidingMaterial properties of diamondta221diamond filmsNucleation02 engineering and technologyengineering.material01 natural sciencesnucleation surfaceChemical-mechanical planarization0103 physical sciencesboron dopingGeneral Materials Scienceta116Elastic modulus010302 applied physicsta114MetallurgyDiamondTribology021001 nanoscience & nanotechnologyMicrostructureCarbon filmengineeringplanarization0210 nano-technologyACS Applied Materials & Interfaces
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Kinetics of phase separation in thin films: Lattice versus continuum models for solid binary mixtures

2008

A description of phase separation kinetics for solid binary (A,B) mixtures in thin film geometry based on the Kawasaki spin-exchange kinetic Ising model is presented in a discrete lattice molecular field formulation. It is shown that the model describes the interplay of wetting layer formation and lateral phase separation, which leads to a characteristic domain size $\ell(t)$ in the directions parallel to the confining walls that grows according to the Lifshitz-Slyozov $t^{1/3}$ law with time $t$ after the quench. Near the critical point of the model, the description is shown to be equivalent to the standard treatments based on Ginzburg-Landau models. Unlike the latter, the present treatmen…

wettingMaterials scienceStatistical Mechanics (cond-mat.stat-mech)Condensed matter physicscritical pointsGinzburg-Landau theoryTime evolutionFOS: Physical sciencesBinary numberfree energyLattice constantthin filmsCritical point (thermodynamics)Lattice (order)Ising modelWettingphase separationThin filmCondensed Matter - Statistical MechanicsWetting layerPhysical Review E
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Deformation Quantization in White Noise Analysis

2007

We define and present an example of a deformation quantization product on a Hida space of test functions endowed with a Wick product.

white noise analysisMoyal productQuantization (signal processing)lcsh:MathematicsMathematics::Number TheoryMathematical analysisFOS: Physical sciencesWhite noiseMathematical Physics (math-ph)lcsh:QA1-939Mathematics - Quantum AlgebraFOS: MathematicsMoyal productQuantum Algebra (math.QA)Geometry and TopologyWick productAnalysisMathematical PhysicsMathematicsMathematical physics
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The Large Observatory For x-ray Timing

2014

The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final down-selection for a launch slot in 2022-2024. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument, LOFT will study the behaviour of matter under extreme conditions, such as the strong gravitational field in the innermost regions of accretion flows close to black holes and neutron stars, and the supra-nuclear densities in the interior of neutron stars. The science payload is based on a Large Area Detector (LAD, 10 m 2 effective area, 2-30 keV, 240 eV spectral resolution, 1 deg collimated field of view) and a WideFi…

x-ray and γ-ray instrumentationcompact objects; microchannel plates; X-ray detectors; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringVisionX-ray timingObservatoriesField of view01 natural sciences7. Clean energyneutron starsObservatory010303 astronomy & astrophysicsPhysicsEquipment and servicesApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsSteradian[ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Computer Science Applications1707 Computer Vision and Pattern RecognitionX-ray detectorsCondensed Matter Physicscompact objectsX-ray spectroscopyAstrophysics - Instrumentation and Methods for AstrophysicsX-ray detector[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cosmic VisionSpectral resolutionmicrochannel platesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesNOmicrochannel platecompact objects; microchannel plates; X-ray detectors; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic EngineeringSettore FIS/05 - Astronomia e AstrofisicaX-rayscompact object0103 physical sciencesElectronicOptical and Magnetic MaterialsElectrical and Electronic EngineeringSpectral resolutionInstrumentation and Methods for Astrophysics (astro-ph.IM)dense hadronic matterSensors010308 nuclear & particles physicsX-ray imagingAstronomyAccretion (astrophysics)[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutron star13. Climate actionx-ray and γ-ray instrumentation; neutron stars; dense hadronic matter[ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Gamma-ray burstastro-ph.IM
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Online ^{222}Rn removal by cryogenic distillation in the XENON100 experiment

2017

International audience; 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.

xenon: liquidradon: admixturePhysics - Instrumentation and DetectorsPhysicsFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)XENONmonitoringefficiencycryogenicsgasddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]background: radioactivity[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
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The XENON1T Dark Matter Experiment

2017

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2 t liquid xenon inventory, 2.0 t constitute the active target of the dual-phase time projection chamber. The scintillation and ionization signals from particle interactions are detected with low-background photomultipliers. This article describes the XENON1T instrument and its subsystems as well as strategies to achieve an unprecedented low background level. First results on the detector response and the performance of the subsystems are also presented. © 2017, The Author(s).

xenon: targetPhotomultiplierCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)WIMP[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matterchemistry.chemical_elementFOS: Physical scienceslcsh:Astrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONXenonbackground: lowWIMP[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Ionization0103 physical scienceslcsh:QB460-466[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)Instrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]AstrophysiquePhysicsScintillationxenon: liquidTime projection chamberphotomultiplier010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)dark matter: detectortime projection chamberchemistrylcsh:QC770-798TPCAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]performanceAstrophysics - Cosmology and Nongalactic AstrophysicsEuropean Physical Journal C
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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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Search for Light Dark Matter Interactions Enhanced by the Migdal Effect or Bremsstrahlung in XENON1T.

2019

Direct dark matter detection experiments based on a liquid xenon target are leading the search for dark matter particles with masses above ∼5 GeV/c2, but have limited sensitivity to lighter masses because of the small momentum transfer in dark matter-nucleus elastic scattering. However, there is an irreducible contribution from inelastic processes accompanying the elastic scattering, which leads to the excitation and ionization of the recoiling atom (the Migdal effect) or the emission of a bremsstrahlung photon. In this Letter, we report on a probe of low-mass dark matter with masses down to about 85 MeV/c2 by looking for electronic recoils induced by the Migdal effect and bremsstrahlung us…

xenon: targetPhysics - Instrumentation and Detectorsdark matter: interactionelastic scatteringGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonIonizationexcited state[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentLight dark matterElastic scatteringPhysicsxenon: liquidatommomentum transferMomentum transferBremsstrahlungInstrumentation and Detectors (physics.ins-det)photon: bremsstrahlungS030DN5Weakly interacting massive particlesExcited stateAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterLight Dark Matter Direct search Liquid Xenon TPCFOS: Physical sciencesS030DI5chemistry.chemical_elementNuclear physicsParticle dark matterrecoilionization0103 physical sciencesDark matter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsscintillation counterS030DP5010308 nuclear & particles physicsdown: masssensitivityDark matter Particle dark matter Weakly interacting massive particles* Automatic Keywords *chemistryElementary Particles and Fieldsbremsstrahlung: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physical review letters
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