Search results for "Measurement"

showing 10 items of 2918 documents

Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data

2017

A search for the solar neutrino effective magnetic moment has been performed using data from 1291.5 days exposure during the second phase of the Borexino experiment. No significant deviations from the expected shape of the electron recoil spectrum from solar neutrinos have been found, and a new upper limit on the effective neutrino magnetic moment of $\mu_{\nu}^{eff}$ $<$ 2.8$\cdot$10$^{-11}$ $\mu_{B}$ at 90\% c.l. has been set using constraints on the sum of the solar neutrino fluxes implied by the radiochemical gallium experiments.Using the limit for the effective neutrino moment, new limits for the magnetic moments of the neutrino flavor states, and for the elements of the neutrino magne…

Physics and Astronomy (miscellaneous)neutrino: solarPhysics::Instrumentation and DetectorsSolar neutrino01 natural sciencesHigh Energy Physics - ExperimentNeutrino detectorHigh Energy Physics - Experiment (hep-ex)SPIN ROTATIONHigh Energy Physics - Phenomenology (hep-ph)electron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar AstrophysicsBorexinoS066MGMgalliumPhysicsMagnetic momentneutrino: magnetic momentHigh Energy Physics - Phenomenologyneutrino: momentNeutrino detectorneutrino: flavorneutrino: MajoranaMeasurements of neutrino speedBorexinoNeutrinoupper limitParticle physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSolar neutrinoDECAYSMagnetic momentNuclear physicsstatistical analysis[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesddc:530010306 general physicsNeutrino oscillationDETECTORELECTROMAGNETIC PROPERTIES010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemMAJORANA NEUTRINOS[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]electron: energy spectrum[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentexperimental resultsPhysical Review D
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Hybrid particle-continuum simulations coupling Brownian dynamics and local dynamic density functional theory

2017

We present a multiscale hybrid particle-field scheme for the simulation of relaxation and diffusion behavior of soft condensed matter systems. It combines particle-based Brownian dynamics and field-based local dynamics in an adaptive sense such that particles can switch their level of resolution on the fly. The switching of resolution is controlled by a tuning function which can be chosen at will according to the geometry of the system. As an application, the hybrid scheme is used to study the kinetics of interfacial broadening of a polymer blend, and is validated by comparing the results to the predictions from pure Brownian dynamics and pure local dynamics calculations.

Physics010304 chemical physicsContinuum (measurement)On the flyKineticsFOS: Physical sciencesGeneral ChemistryCondensed Matter - Soft Condensed MatterCondensed Matter PhysicsDynamic density01 natural sciences0103 physical sciencesBrownian dynamicsSoft Condensed Matter (cond-mat.soft)Polymer blendStatistical physics010306 general physicsFunctional theorySoft Matter
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Perspective: Polarizable continuum models for quantum-mechanical descriptions

2016

Polarizable continuum solvation models are nowadays the most popular approach to describe solvent effects in the context of quantum mechanical calculations. Unexpectedly, despite their widespread use in all branches of quantum chemistry and beyond, important aspects of both their theoretical formulation and numerical implementation are still not completely understood. In particular, in this perspective we focus on the numerical issues of their implementation when applied to large systems and on the theoretical framework needed to treat time dependent problems and excited states or to deal with electronic correlation. Possible extensions beyond a purely electrostatic model and generalization…

Physics010304 chemical physicsElectronic correlationContinuum (measurement)Implicit solvationSolvationGeneral Physics and Astronomy010402 general chemistry01 natural sciences0104 chemical sciencesPolarizability0103 physical sciencesStatistical physicsPhysical and Theoretical ChemistryQuantumElectrostatic model
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Contrail Formation: Analysis of Sublimation Mechanisms

2018

We study losses of ice crystals in a persistent, soot-rich contra i l in the wake behind a medium-sized aircraft at cru i se. Constrain i n g a model covering ice nucleation, growth, and subl i m a t i o n phases with a n aircraft data set, we track the subl i m a t i o n history over two minutes of cont r a i l age and rela t e ice crystal numbers to the number of soot particles emitted by th e aircraft engines.

Physics010504 meteorology & atmospheric sciencesIce crystalscontrailsAtmosphärische SpurenstoffeCloud physicsThermodynamics010502 geochemistry & geophysics01 natural sciencesGeophysicsIce nucleusprocess modelingGeneral Earth and Planetary SciencesSublimation (phase transition)microphysicsWolkenphysikSoot particlesaircraft measurements0105 earth and related environmental sciencesGeophysical Research Letters
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Dynamics of correlations due to a phase noisy laser

2012

We analyze the dynamics of various kinds of correlations present between two initially entangled independent qubits, each one subject to a local phase noisy laser. We give explicit expressions of the relevant quantifiers of correlations for the general case of single-qubit unital evolution, which includes the case of a phase noisy laser. Although the light field is treated as classical, we find that this model can describe revivals of quantum correlations. Two different dynamical regimes of decay of correlations occur, a Markovian one (exponential decay) and a non-Markovian one (oscillatory decay with revivals) depending on the values of system parameters. In particular, in the non-Markovia…

Physics03.67.Mn Entanglement measures witnesses and other characterizationQuantum discordQuantum PhysicsPhase (waves)Markov processFOS: Physical sciencesQuantum entanglement03.65.Ud Entanglement and quantum nonlocality (e.g. EPR paradox Bell's inequalities GHZ states etc.)Condensed Matter PhysicsAtomic and Molecular Physics and OpticsSettore FIS/03 - Fisica Della Materiasymbols.namesake02.50.Ga Markov processeQubit42.50.Dv Quantum state engineering and measurementsymbolsStatistical physicsExponential decayQuantum Physics (quant-ph)QuantumMathematical PhysicsLight field03.67.Lx Quantum computation architectures and implementations03.65.Ud Entanglement and quantum nonlocality (e.g. EPR paradox Bell's inequalities GHZ states etc.); 42.50.Dv Quantum state engineering and measurements; 03.67.Mn Entanglement measures witnesses and other characterizations; 02.50.Ga Markov processes; 03.67.Lx Quantum computation architectures and implementations
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Does GRS 1915+105 exhibit "canonical" black-hole states?

2003

We have analysed RXTE data of the superluminal source GRS 1915+105 in order to investigate if, despite its extreme variability, it also exhibits the canonical source states that characterise other black-hole candidates. The phenomenology of GRS 1915+105 has been described in terms of three states (named A, B and C) based on their hardness ratios and position in the colour-colour diagram. We have investigated the connection between these states and the canonical behaviour and found that the shape of the power spectral continuum and the values of the best-fit model parameters to the noise components in all three states indicate that the source shows properties similar to the canonical very hi…

PhysicsAccretionSuperluminal motionContinuum (measurement)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)BinariesFOS: Physical sciencesAstronomy and AstrophysicsModel parametersAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Individual StarsSpace and Planetary ScienceX-raysGRS 1915+105UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAccretion discIndividual Stars ; GRS 1915+105 ; Binaries ; X-rays ; Accretion ; Accretion disc:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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On Anomaly-Free Dark Matter Models

2019

We investigate the predictions of anomaly-free dark matter models for direct and indirect detection experiments. We focus on gauge theories where the existence of a fermionic dark matter candidate is predicted by anomaly cancellation, its mass is defined by the new symmetry breaking scale, and its stability is guaranteed by a remnant symmetry after the breaking of the gauge symmetry. We find an upper bound on the symmetry breaking scale by applying the relic density and perturbative constraints. The anomaly-free property of the theories allows us to perform a full study of the gamma lines from dark matter annihilation. We investigate the correlation between predictions for final-state radia…

PhysicsAnnihilationContinuum (measurement)Dark matterFOS: Physical sciencesRadiationUpper and lower boundsHigh Energy Physics - ExperimentTheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Gauge theorySymmetry breakingGauge symmetry
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Observation of high-energy neutrinos using Cerenkov detectors embedded deep in Antarctic ice.

2001

Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate enormous amounts of matter, and therefore have the potential to directly convey astrophysical information from the edge of the Universe and from deep inside the most cataclysmic high-energy regions. The neutrino's great penetrating power, however, also makes this particle difficult to detect. Underground detectors have observed low-energy neutrinos from the Sun and a nearby supernova2, as well as neutrinos generated in the Earth's atmosphere. But the very low fluxes of high-energy neutrinos from cosmic sources can be observed only by mu…

PhysicsAntarctic Muon And Neutrino Detector ArrayMultidisciplinaryPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoAstronomyAstrophysicsSolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyNature
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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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Attractive ion-ion correlation forces and the dielectric approximation.

2016

We analyze the classical problem of the interaction between two charged surfaces separated by a solution containing neutralizing counter-ions. The focus is on obtaining a description where the solvent is treated explicitly rather than through a dielectric approximation as is conventionally done. We summarize the results of three papers where we have used a Stockmayer fluid model in Monte Carlo simulations. It is shown that the attractive ion-ion correlation mechanism is also operating when the solvent is described explicitly. There appears an oscillatory component to the force, but when this is accounted for, there is a semi-quantitative agreement between the continuum model and the model w…

PhysicsAqueous solutionContinuum (measurement)Monte Carlo method02 engineering and technologySurfaces and InterfacesDielectric010402 general chemistry021001 nanoscience & nanotechnology01 natural sciencesDouble layer forces0104 chemical sciencesIonSolventColloid and Surface ChemistrySolvent modelsStatistical physicsPhysical and Theoretical Chemistry0210 nano-technologyAdvances in colloid and interface science
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