Search results for "53"

showing 10 items of 2908 documents

Linear and nonlinear spin dynamics in multi-domain magnetoelastic antiferromagnets

2021

Antiferromagnets have recently surged as the prominent material platform for the next generation spintronics devices. Despite the remarkable abundance of antiferromagnets and the variety of their spin textures in nature, they share a widely common, if not ubiquitous, feature. Magnetoelasticity, which is expressed as strictions of different origin, relativistic and/or exchange, significantly contributes to the magnetic anisotropy of antiferromagnets. Crucially, a general theoretical framework able to address the role of domain walls on the spin dynamics in antiferromagnets in the presence of magnetoelasticity is lacking. Here we tackle this problem developing a very general macroscopic pheno…

PhysicsAcoustics and UltrasonicsSpin dynamicsSpintronicsCondensed Matter PhysicsSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsDomain (software engineering)Nonlinear systemMagnetic anisotropytheory antiferromagnets spin dynamics nonlinear phenomenaPhenomenological modelAntiferromagnetismCondensed Matter::Strongly Correlated Electronsddc:530Statistical physicsSpin-½
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Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array

2002

The Antarctic Muon and Neutrino Detector Array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 10^6 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05*10^9 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulat…

PhysicsAntarctic Muon And Neutrino Detector ArrayNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysicsSolar neutrino problemAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Neutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentddc:530Astrophysics::Earth and Planetary AstrophysicsNeutrinoNeutrino astronomyNeutrino oscillation
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Polarization analysis of $\bar{p}$ produced in pA collisions

2019

A quite simple procedure for the generation of a polarized antiproton beam could be worked out if antiprotons are produced with some polarization. In order to investigate this possibility measurements of the polarization of produced antiprotons have been started at a CERN/PS test beam. The polarization will be determined from the asymmetry of the elastic antiproton scattering at a liquid hydrogen target in the CNI region for which the analyzing power is well known. The data are under analysis and an additional measurement is done in 2018. Details on the experiment and the ongoing data analysis will be given.

PhysicsAntiparticle010308 nuclear & particles physicsPhysicsQC1-999Polarization (waves)01 natural sciences7. Clean energyNuclear physicsAntiproton beamAntiproton0103 physical sciencesPhysics::Accelerator Physicsddc:530High Energy Physics::ExperimentPhysics::Atomic Physics010306 general physicsAntihydrogenNuclear Experiment
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Status of the analysis for the search of polarization in the antiproton production process

2016

The P-349 experiment aims to test whether for antiprotons the production process itself can be a source of polarization in view of the preparation of a polarized antiproton beam. In this article we present the details of performed measurements and report on the status of the ongoing analysis.

PhysicsAntiparticle010308 nuclear & particles physicsPhysicsQC1-999Polarization (waves)01 natural sciencesEngineering physicsNuclear physicsSubatomär fysikAntiproton beamAntiprotonAntimatter0103 physical sciencesSubatomic PhysicsPhysics::Accelerator PhysicsNuclear Physics - Experimentddc:530010306 general physicsEPJ Web of Conferences
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Effect of low mass dark matter particles on the Sun

2010

We study the effect of dark matter (DM) particles in the Sun, focusing in particular on the possible reduction of the solar neutrinos flux due to the energy carried away by DM particles from the innermost regions of the Sun, and to the consequent reduction of the temperature of the solar core. We find that in the very low-mass range between 4 and 10 GeV, recently advocated to explain the findings of the DAMA and CoGent experiments, the effects on neutrino fluxes are detectable only for DM models with very small, or vanishing, self-annihilation cross section, such as the so-called asymmetric DM models, and we study the combination of DM masses and Spin Dependent cross sections which can be e…

PhysicsAstrophysics and AstronomyNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Solar energetic particles010308 nuclear & particles physics530 PhysicsSolar neutrinoDark matterFOS: Physical sciencesAstrophysics01 natural sciencesMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Solar coreConvection zone10231 Institute for Computational Science0103 physical sciencesNeutrino3106 Nuclear and High Energy Physics3101 Physics and Astronomy (miscellaneous)010303 astronomy & astrophysicsLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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Drude weight increase by orbital and repulsive interactions in fermionic ladders

2019

In strictly one-dimensional systems, repulsive interactions tend to reduce particle mobility on a lattice. Therefore, the Drude weight, controlling the divergence at zero-frequency of optical conductivities in perfect conductors, is lower than in non-interacting cases. We show that this is not the case when extending to quasi one-dimensional ladder systems. Relying on bosonization, perturbative and matrix product states (MPS) calculations, we show that nearest-neighbor interactions and magnetic fluxes provide a bias between back- and forward-scattering processes, leading to linear corrections to the Drude weight in the interaction strength. As a consequence, Drude weights counter-intuitivel…

PhysicsBosonizationCondensed Matter::Quantum GasesCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Interaction strengthFOS: Physical sciencesddc:500.201 natural sciencesMatrix multiplication010305 fluids & plasmasCondensed Matter - Strongly Correlated ElectronsUltracold atomQuantum Gases (cond-mat.quant-gas)Lattice (order)0103 physical sciencesParticleddc:530Edge states010306 general physicsCondensed Matter - Quantum Gases
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Precision Measurement of the Branching Fractions of η′ Decays

2019

PubMed ID: 31050481

PhysicsBranching fractionElectron–positron annihilationComputerSystemsOrganization_COMPUTER-COMMUNICATIONNETWORKSGeneral Physics and AstronomyBranching (polymer chemistry)01 natural sciencesHigh Energy Physics - Experiment; High Energy Physics - ExperimentNOHigh Energy Physics - ExperimentCrystallographyComputingMilieux_MANAGEMENTOFCOMPUTINGANDINFORMATIONSYSTEMSComputingMethodologies_PATTERNRECOGNITION0103 physical sciencesddc:530InformationSystems_MISCELLANEOUS010306 general physicsPhysical Review Letters
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Observation of the Leptonic Decay $D^+ → τ^+ ν_τ$

2019

Physical review letters 123(21), 211802 (2019). doi:10.1103/PhysRevLett.123.211802

PhysicsCabibbo–Kobayashi–Maskawa matrixElectron–positron annihilationGeneral Physics and Astronomy530High Energy Physics - Experiment; High Energy Physics - Experiment01 natural sciencesHigh Energy Physics - ExperimentNOCrystallography0103 physical sciencesMatrix elementddc:530Exponential decay010306 general physicsLepton
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Frequency-modulated atomic force microscopy operation by imaging at the frequency shift minimum: the dip-df mode.

2014

In frequency modulated non-contact atomic force microscopy, the change of the cantilever frequency (Delta f) is used as the input signal for the topography feedback loop. Around the Delta f(z) minimum, however, stable feedback operation is challenging using a standard proportional-integral-derivative (PID) feedback design due to the change of sign in the slope. When operated under liquid conditions, it is furthermore difficult to address the attractive interaction regime due to its often moderate peakedness. Additionally, the Delta f signal level changes severely with time in this environment due to drift of the cantilever frequency f(0) and, thus, requires constant adjustment. Here, we pre…

PhysicsCantileverbusiness.industrySurface PropertiesPID controllerAbsolute valueDerivativeFeedback loopModels TheoreticalMicroscopy Atomic Force530SignalCalcium CarbonateSetpointOpticsbusinessConstant (mathematics)InstrumentationThe Review of scientific instruments
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Molecular parity nonconservation in nuclear spin couplings

2017

The weak interaction does not conserve parity, which is apparent in many nuclear and atomic phenomena. However, thus far, parity nonconservation has not been observed in molecules. Here we consider nuclear-spin-dependent parity nonconserving contributions to the molecular Hamiltonian. These contributions give rise to a parity nonconserving indirect nuclear spin-spin coupling which can be distinguished from parity conserving interactions in molecules of appropriate symmetry, including diatomic molecules. We estimate the magnitude of the coupling, taking into account relativistic corrections. Finally, we propose and simulate an experiment to detect the parity nonconserving coupling using liqu…

PhysicsChemical Physics (physics.chem-ph)Antisymmetric relationAtomic Physics (physics.atom-ph)FOS: Physical sciencesParity (physics)010402 general chemistry01 natural sciences5300104 chemical sciencesPhysics - Atomic PhysicsQuantum mechanicsPhysics - Chemical Physics0103 physical sciencesddc:530Physics::Atomic Physics010306 general physics
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