Search results for "upper"

showing 10 items of 987 documents

Interdiffusion in blends of polystyrene and polymethylstyrene studied by light scattering after temperature jumps across the phase boundary

1992

Abstract We describe a simple light scattering set-up for measuring interdiffusion coefficients D in polymer blends by generating spinodal decomposition and subsequent dissolution after temperature jumps across the phase boundary. In blends of polystyrene and polymethylstyrene (random copolymer of 60% m-methylstyrene and 40% p-methylstyrene) D values were obtained between 10−11 and 10−15 cm2s−1 at temperatures up to 50 K above the upper critical solution temperature. The results are discussed in relation to tracer diffusion in the same system.

Phase boundaryPolymers and PlasticsChemistrySpinodal decompositionDiffusionOrganic ChemistryThermodynamicsLight scatteringchemistry.chemical_compoundUpper critical solution temperaturePolymer chemistryMaterials ChemistryPolymer blendPolystyreneDissolutionPolymer
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Upper limit on the cosmic-ray photon flux above 1019 eV using the surface detector of the Pierre Auger Observatory

2008

A method is developed to search for air showers initiated by photons using data recorded by the surface detector of the Auger Observatory. The approach is based on observables sensitive to the longitudinal shower development, the signal risetime and the curvature of the shower front. Applying this method to the data, upper limits on the flux of photons of 3.8 x 10-3, 2.5 x 10-3; and 2.2 x 10-3 km-2 sr-1 yr-1 above 1019 eV, 2 x 1019 eV; and 4 x 1019 eV are derived, with corresponding limits on the fraction of photons being 2.0%, 5.1%, and 31% (all limits at 95% c.l.). These photon limits disfavor certain exotic models of sources of cosmic rays. The results also show that the approach adopted…

Photon[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyFluxFOS: Physical sciencesOsservatorio Pierre AugerCosmic rayFotonesAstrophysicsAstrophysics7. Clean energy01 natural sciencesAugerNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)Raggi cosmiciultra high energy photonsCascada atmosféricaObservatory0103 physical sciences010306 general physicsCiencias ExactasPierre Auger ObservatoryPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaAstronomy and AstrophysicsPierre Auger ObservatoryEnergia ultra altaCosmic rayHigh Energy Physics - PhenomenologyPair production13. Climate actionFotoniExperimental High Energy Physicsddc:540flux upper limitNeutrinoSciami atmosferici estesi
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All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

2018

Made available in DSpace on 2018-11-26T17:45:14Z (GMT). No. of bitstreams: 0 Previous issue date: 2018-03-22 Australian Research Council Council of Scientific and Industrial Research of India Department of Science and Technology, India Science AMP; Engineering Research Board (SERB), India Ministry of Human Resource Development, India Spanish Agencia Estatal de Investigacion Vicepresidencia i Conselleria d'Innovacio, Recerca i Turisme Conselleria d'Educacio i Universitat del Govern de les Illes Balears Conselleria d'Educacio, Investigacio, Cultura i Esport de la Generalitat Valenciana National Science Centre of Poland Swiss National Science Foundation (SNSF) Russian Foundation for Basic Rese…

Physics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsLIGO-VirgoMagnetar01 natural sciencesGeneral Relativity and Quantum CosmologyGravitational waves long transients LIGOGravitational wavesGeneral Relativity and Quantum CosmologyUPPER LIMITSSearch algorithmSIGNALS0103 physical sciencesWaveformlong transientsHigh Energy PhysicsLIGO010306 general physicsgravitational wave010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsLIGO-Virgo; gravitational waves; long duration transient[PHYS]Physics [physics]Gravitational wavelong duration transientLIGOgravitational waves; LIGO-Virgo; long duration transient; Physics and Astronomy (miscellaneous)Black holeMODELNeutron starAmplitudegravitational wavesBLACK-HOLEComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRADIATIONNEUTRINOAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Search for Lorentz and CPT violation using sidereal time dependence of neutrino flavor transitions over a short baseline

2017

A class of extensions of the Standard Model allows Lorentz and CPT violations, which can be identified by the observation of sidereal modulations in the neutrino interaction rate. A search for such modulations was performed using the T2K on-axis near detector. Two complementary methods were used in this study, both of which resulted in no evidence of a signal. Limits on associated Lorentz and CPT-violating terms from the Standard Model extension have been derived by taking into account their correlations in this model for the first time. These results imply such symmetry violations are suppressed by a factor of more than 1020 at the GeV scale.

Physics and Astronomy (miscellaneous)CPT symmetryAstrophysicsKAMIOKANDE01 natural scienceshigh energy physicsPhysics Particles & FieldsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Standard-Model Extension[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: interactionPhysicssymmetry: violationPhysicsJ-PARC LabCPT symmetrysuppressionLorentz symmetryviolation: LorentzmodulationSidereal timePhysical Sciencesneutrino: flavorsymbolsNeutrinoupper limitParticle physicsdata analysis method530 PhysicsLorentz transformationFOS: Physical sciencesCPT: violationAstronomy & AstrophysicsStandard Modelsymbols.namesakenear detectorstatistical analysis0103 physical sciences010306 general physicsNeutrino oscillationneutrino oscillationsScience & Technology010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologySymmetry (physics)neutrino/mu: secondary beamcorrelationtime dependenceHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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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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Impulse-based hybrid motion control

2017

The impulse-based discrete feedback control has been proposed in previous work for the second-order motion systems with damping uncertainties. The sate-dependent discrete impulse action takes place at zero crossing of one of both states, either relative position or velocity. In this paper, the proposed control method is extended to a general hybrid motion control form. We are using the paradigm of hybrid system modeling while explicitly specifying the state trajectories each time the continuous system state hits the guards that triggers impulsive control actions. The conditions for a stable convergence to zero equilibrium are derived in relation to the control parameters, while requiring on…

Physics0209 industrial biotechnologyFeedback control020208 electrical & electronic engineeringSystems and Control (eess.SY)02 engineering and technologyImpulse (physics)Motion controlZero crossingUpper and lower bounds020901 industrial engineering & automationControl theoryHybrid systemBounded functionFOS: Electrical engineering electronic engineering information engineering0202 electrical engineering electronic engineering information engineeringComputer Science - Systems and ControlControl parametersIECON 2017 - 43rd Annual Conference of the IEEE Industrial Electronics Society
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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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Structure formation during an early period of matter domination

2014

In this work we show that modifying the thermal history of the Universe by including an early period of matter domination can lead to the formation of astronomical objects. However, the survival of these objects can only be possible if the dominating matter decays to a daughter particle which is not only almost degenerate with the parent particle but also has an open annihilation channel. This requirement translates in an upper bound for the coupling of such a channel and makes the early structure formation viable.

PhysicsAstronomical ObjectsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Structure formation010308 nuclear & particles physicsDegenerate energy levelsFOS: Physical sciencesFísicaAstrophysics16. Peace & justice01 natural sciencesUpper and lower boundsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesParticle010303 astronomy & astrophysicsPeriod (music)Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Electromagnetic form factors and axial charge of the nucleon from Nf = 2 + 1 Wilson fermions

2018

We present an update on our determination of the electromagnetic form factors and axial charge of the nucleon from theNf= 2 + 1 CLS ensembles with increased statistics and an additional finer lattice spacing. We also investigate the impact ofO(a)-improvement of the currents.

PhysicsCLs upper limitsLattice constant010308 nuclear & particles physicsQuantum electrodynamicsPhysicsQC1-9990103 physical sciencesCharge (physics)Fermion010306 general physicsNucleon01 natural sciencesEPJ Web of Conferences
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Universal mechanism of spin relaxation in solids

2005

We consider relaxation of a rigid spin cluster in an elastic medium in the presence of the magnetic field. Universal simple expression for spin-phonon matrix elements due to local rotations of the lattice is derived. The equivalence of the lattice frame and the laboratory frame approaches is established. For spin Hamiltonians with strong uniaxial anisotropy the field dependence of the transition rates due to rotations is analytically calculated and its universality is demonstrated. The role of time reversal symmetry in spin-phonon transitions has been elucidated. The theory provides lower bound on the decoherence of any spin-based solid-state qubit.

PhysicsCondensed Matter - Materials ScienceQuantum decoherenceStatistical Mechanics (cond-mat.stat-mech)Condensed matter physicsSpin polarizationMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesCondensed Matter Physics01 natural sciencesUpper and lower bounds010305 fluids & plasmasElectronic Optical and Magnetic MaterialsUniversality (dynamical systems)Magnetic fieldLattice (order)QubitQuantum mechanics0103 physical sciencesCondensed Matter::Strongly Correlated Electrons010306 general physicsAnisotropyCondensed Matter - Statistical MechanicsPhysical Review B
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