Search results for "scattering [nucleus nucleus]"

showing 10 items of 161 documents

The πd scattering length from Kα X-rays

1974

Abstract X-rays from the K α transition (2P → 1S) of the π − d mesic atom have been observed. Their energy, 2592.8 −2.0 +1.6 , has been measured by the critical absorber technique, using the M V absorption edge in bismuth. The strong interaction shift in the 1S state is −4.8 eV, corresponding to a scattering length a ( π d) = −(0.052 −0.017 +0.022 ) m π −1 , in agreement with recent calculations. The intensity ratio K α /K total = 0.548 ± 0.015.

Nuclear reactionPhysicsNuclear and High Energy PhysicsAbsorption edgechemistryAtomStrong interactionchemistry.chemical_elementScattering lengthAtomic physicsIntensity ratioSpectral lineBismuthPhysics Letters B
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Time calibration of the ANTARES neutrino telescope

2011

The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of ~1 ns. The methods developed to attain this level of precision are described.

Optical telescopesPhysics - Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectors01 natural sciencesOptimal performanceHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Calibration procedureDimensional arraysAngular resolution[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino energyNEUTRINO TELESCOPE010303 astronomy & astrophysicsPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)Deep seaNeutrino detectorRelative timeCalibrationFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsTime calibrationPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov lightAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesScattering lengthNeutrino TelescopesOptical telescopeNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Tellurium compounds0103 physical sciencesOptical systemsCalibrationAngular resolution14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORCherenkov radiationtime calibration; neutrino telescopes; antaresANTARES010308 nuclear & particles physicsNeutrino interactionsAstronomyElementary particlesAstronomy and AstrophysicsPhotomultipliersFISICA APLICADAHigh Energy Physics::ExperimentUNDERWATER DETECTORNeutrino telescopesSYSTEM
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Structural characterization of a-plane Zn1−xCdxO (0 < x <0.085) thin films grown by metal-organic vapor phase epitaxy.

2006

Zn1−xCdxO(11math0) films have been grown on (01math2) sapphire (r–plane) substrates by metal-organic vapor phase epitaxy. A 800-nm-thick ZnO buffer, deposited prior to the alloy growth, helps to prevent the formation of pure CdO. A maximum uniform Cd incorporation of 8.5 at. % has been determined by Rutherford backscattering spectrometry. Higher Cd contents lead to the coexistence of Zn1−xCdxO alloys of different compositions within the same film. The near band-edge photoluminescence emission shifts gradually to lower energies as Cd is incorporated and reaches 2.93 eV for the highest Cd concentration (8.5 at. %). The lattice deformation, due to Cd incorporation, has been described using a n…

PhotoluminescenceMaterials scienceRutherford backscatteringCadmium compoundsUNESCO::FÍSICAAnalytical chemistrySemiconductor epitaxial layersGeneral Physics and AstronomyII-VI semiconductorsSurface structureChemical vapor depositionRutherford backscattering spectrometryEpitaxyVapour phase epitaxial growthCrystallographyLattice constantZinc compounds ; Cadmium compounds ; II-VI semiconductors ; MOCVD ; Vapour phase epitaxial growth ; Semiconductor epitaxial layers ; Rutherford backscattering ; Photoluminescence ; Surface structure ; Buffer layers:FÍSICA [UNESCO]MOCVDSapphireBuffer layersMetalorganic vapour phase epitaxyZinc compoundsThin filmPhotoluminescence
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Transmission of light in deep sea water at the site of the Antares neutrino telescope

2005

The ANTARES neutrino telescope is a large photomultiplier array designed to detect neutrino-induced upward-going muons by their Cherenkov radiation. Understanding the absorption and scattering of light in the deep Mediterranean is fundamental to optimising the design and performance of the detector. This paper presents measurements of blue and UV light transmission at the ANTARES site taken between 1997 and 2000. The derived values for the scattering length and the angular distribution of particulate scattering were found to be highly correlated, and results are therefore presented in terms of an absorption length lambda_abs and an effective scattering length lambda_sct^eff. The values for …

PhotomultiplierPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsNeutrino telescopeAstrophysicsLambda01 natural sciencesLight scattering[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Sea water properties: absorption and transmission of lightHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAngular resolution07.89.+b 29.40.Ka 42.25.Bs 42.68.Xy 92.10.Bf 92.10.Pt 95.55.Vj010306 general physicsCherenkov radiationPhysicsneutrino telescope undersea Cherenkov detectors sea water properties absorption and transmission of lightUndersea Cherenkov detectors[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsScatteringAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAttenuation lengthSea water properties: absorption and transmission of light.Astronomy and AstrophysicsScattering lengthabsorption and transmission of lightHigh Energy Physics - Phenomenology13. Climate actionFísica nuclearsea water propertiesAstroparticle Physics
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A 1D coupled Schrödinger drift-diffusion model including collisions

2005

We consider a one-dimensional coupled stationary Schroedinger drift-diffusion model for quantum semiconductor device simulations. The device domain is decomposed into a part with large quantum effects (quantum zone) and a part where quantum effects are negligible (classical zone). We give boundary conditions at the classic-quantum interface which are current preserving. Collisions within the quantum zone are introduced via a Pauli master equation. To illustrate the validity we apply the model to three resonant tunneling diodes.

Physics and Astronomy (miscellaneous)Quantum dynamics34L40Pauli master equationinterface conditionsQuantum mechanicsPrincipal quantum numberQuantum operation65Z05quantum-classical couplingAmplitude damping channelscattering states82D37PhysicsNumerical Analysis82C70Applied Mathematics34L30Quantum numberComputer Science Applications34L25Computational MathematicsModeling and SimulationQuantum process78A35Schroedinger equationdrift-diffusionQuantum algorithmQuantum dissipation
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Two-photon exchange corrections to elastic e− -proton scattering: Full dispersive treatment of πN states at low momentum transfers

2017

We evaluate the pion-nucleon intermediate-state contribution to the two-photon exchange (TPE) correction in the elastic electron-nucleon scattering within a dispersive framework. We calculate the contribution from all $\ensuremath{\pi}N$ partial waves using the MAID parametrization. We provide the corresponding TPE correction to the unpolarized $ep$ scattering cross section in the region of low momentum transfer ${Q}^{2}\ensuremath{\lesssim}0.064\text{ }\text{ }{\mathrm{GeV}}^{2}$, where no analytical continuation into the unphysical region of the TPE scattering amplitudes is required. We compare our result in the forward angular region with an alternative TPE calculation, in terms of struc…

Physics010308 nuclear & particles physicsScatteringMomentum transferScattering lengthClassification of discontinuities01 natural sciencesScattering amplitudeMomentumDispersion relation0103 physical sciencesAtomic physics010306 general physicsParametrizationPhysical Review D
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Measurements of Multi-boson production, Trilinear and Quartic Gauge Couplings with the ATLAS detector

2016

The ATLAS collaboration has carried a set of measurements that provide stringent tests of the electroweak sector of Standard Model, specifically on di- and multi-boson production cross sections and on triple and quartic gauge-boson couplings. Such measurements include cross sections for WV (V=W or Z) production in the leptonic or semileptonic channels, the production of a W or Z boson in association with photons, a Z boson in the vector-boson fusion channel and two same-charge W bosons in the vector-boson scattering channel. These measurements are compared to (N)NLO predictions of the Standard Model and provide model-independent constraints on new physics, by setting limits on anomalous gau…

PhysicsCondensed Matter::Quantum GasesParticle physicsPhoton010308 nuclear & particles physicsAtlas detectorPhysics beyond the Standard ModelPhysicsQC1-999Electroweak interactionHigh Energy Physics::Phenomenology7. Clean energy01 natural sciencesNuclear physicsScattering channelQuartic function0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physicsParticle Physics - ExperimentBoson
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Coherence and clock shifts in ultracold fermi gases with resonant interactions.

2007

Using arguments based on sum rules, we derive a general result for the average shifts of rf lines in Fermi gases in terms of interatomic interaction strengths and two-particle correlation functions. We show that near an interaction resonance shifts vary inversely with the atomic scattering length, rather than linearly as in dilute gases, thus accounting for the experimental observation that clock shifts remain finite at Feshbach resonances.

PhysicsCondensed Matter::Quantum GasesStrongly Correlated Electrons (cond-mat.str-el)Condensed Matter - SuperconductivityGeneral Physics and AstronomyResonanceFOS: Physical sciencesScattering lengthSuperconductivity (cond-mat.supr-con)Condensed Matter - Strongly Correlated ElectronsAtomic physicsFermi gasFeshbach resonanceFermi Gamma-ray Space TelescopeCoherence (physics)Physical review letters
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Robust non-Markovianity in ultracold gases

2012

We study the effect of thermal fluctuations on a probe qubit interacting with a Bose-Einstein condensed (BEC) reservoir. The zero-temperature case was studied in [Haikka P et al 2011 Phys. Rev. A 84 031602], where we proposed a method to probe the effects of dimensionality and scattering length of a BEC based on its behavior as an environment. Here we show that the sensitivity of the probe qubit is remarkably robust against thermal noise. We give an intuitive explanation for the thermal resilience, showing that it is due to the unique choice of the probe qubit architecture of our model.

PhysicsCondensed Matter::Quantum GasesWork (thermodynamics)Quantum PhysicsCold Atoms Open Quantum System Markovian Master equations/dk/atira/pure/subjectarea/asjc/3100/3107/dk/atira/pure/subjectarea/asjc/3100/3104Thermal fluctuationsFOS: Physical sciencesScattering lengthPhysics and Astronomy(all)Condensed Matter PhysicsSettore FIS/03 - Fisica Della MateriaAtomic and Molecular Physics and Optics/dk/atira/pure/subjectarea/asjc/3100Quantum Gases (cond-mat.quant-gas)Quantum mechanicsQubitThermalSensitivity (control systems)Condensed Matter - Quantum Gases/dk/atira/pure/subjectarea/asjc/2600/2610Quantum Physics (quant-ph)Mathematical PhysicsCurse of dimensionality
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Resonant hyper-Raman scattering in semiconductors: Excitonic effects

1999

Abstract A theoretical model of resonant hyper-Raman scattering involving two incident photons of frequency ωL is developed. The model is valid for energies 2ℏωL around the absorption edge of the semiconductor, and takes into account Wannier excitons as intermediate states in the scattering process. Both deformation potential and Frohlich interaction are included in the model: It is found that Frohlich-mediated scattering is a dipole-allowed process, in contrast to one-phonon Raman scattering, where the Frohlich mechanism is dipole-forbidden. We have performed numerical calculations of the resonance profile (hyper-Raman cross-section versus 2ℏωL) and applied our model to materials with dipo…

PhysicsCondensed matter physicsPhonon scatteringScatteringScattering lengthMott scatteringInelastic scatteringCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsResonant inelastic X-ray scatteringX-ray Raman scatteringPhysics::Atomic PhysicsScattering theoryElectrical and Electronic EngineeringPhysica B: Condensed Matter
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