Search results for " Phase"

showing 10 items of 1862 documents

Scattering from concentration fluctuations in polymer blends: A monte carlo investigation

1989

The collective scattering function Scoll( $$\vec q$$ ), which describes light (neutron-, x-ray) scattering under wavevector $$\vec q$$ , is obtained from Monte Carlo simulations for a symmetrical polymer mixture. The polymers are modelled by self-avoiding walks ofN A=NB=N steps on a simple cubic lattice, where a fractionφ V of sites is left vacant, and an attractive energye occurs if two neighboring sites are taken by the same kind of monomer. Spinodal curves are estimated from linear extrapolation of S coll −1 (0) vs.e/k B T, whereT is the temperature. Also the single chain structure factor is obtained and the de Gennes random phase approximation (RPA) can thus be tested. Unexpectedly, str…

PhysicsSpinodalPolymers and PlasticsCondensed matter physicsScatteringMonte Carlo methodExtrapolationNeutron scatteringLight scatteringCondensed Matter::Soft Condensed MatterColloid and Surface ChemistryMaterials ChemistryPhysical and Theoretical ChemistryStructure factorRandom phase approximationColloid & Polymer Science
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Geometric phase in open systems.

2003

We calculate the geometric phase associated to the evolution of a system subjected to decoherence through a quantum-jump approach. The method is general and can be applied to many different physical systems. As examples, two main source of decoherence are considered: dephasing and spontaneous decay. We show that the geometric phase is completely insensitive to the former, i.e. it is independent of the number of jumps determined by the dephasing operator.

PhysicsSpontaneous decaySpontaneous decayDensity matrixQuantum PhysicsQuantum decoherenceMarkovian master equationDephasingOperator (physics)Physical systemGeneral Physics and AstronomyFOS: Physical sciencesCondensed Matter::Mesoscopic Systems and Quantum Hall EffectGeometric phaseBerrys phaseStatistical physicsQuantum Physics (quant-ph)Physical review letters
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Pressure-induced structural phase transitions in materials and earth sciences

2008

Pressure is an important thermodynamic parameter since it allows an increase of matter density by reducing volume. The reduction of volume by applying high pressures leads to an overall decrease of interatomic and intermolecular distances that allows exploring in detail atomic and molecular interactions. Therefore, high-pressure research has improved our fundamental understanding of these interactions in solids, liquids and gasses. The study of the structure of matter under compression is a rapid developing field that is receiving increasing attention especially due to continuous experimental and theoretical developments. In this article, we give a brief description of the experimental and …

PhysicsStructural phaseMolecular interactionsVolume (thermodynamics)Field (physics)Chemical physicsSolid matterTheoretical methodsIntermolecular forceStatistical physicsCondensed Matter PhysicsElectronic Optical and Magnetic Materialsphysica status solidi (b)
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The influence of topological phase transition on the superfluid density of overdoped copper oxides

2017

We show that a topological quantum phase transition, generating flat bands and altering Fermi surface topology, is a primary reason for the exotic behavior of the overdoped high-temperature superconductors represented by $\rm La_{2-x}Sr_xCuO_4$, whose superconductivity features differ from what is described by the classical Bardeen-Cooper-Schrieffer theory [J.I. Bo\^zovi\'c, X. He, J. Wu, and A. T. Bollinger, Nature 536, 309 (2016)]. We demonstrate that 1) at temperature $T=0$, the superfluid density $n_s$ turns out to be considerably smaller than the total electron density; 2) the critical temperature $T_c$ is controlled by $n_s$ rather than by doping, and is a linear function of the $n_s$…

PhysicsSuperconductivityQuantum phase transitionLinear function (calculus)Electron densityStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsCondensed Matter - SuperconductivityFOS: Physical sciencesGeneral Physics and AstronomyFermi surface01 natural sciences010305 fluids & plasmasSuperconductivity (cond-mat.supr-con)SuperfluidityCondensed Matter - Strongly Correlated ElectronsElectrical resistivity and conductivityCondensed Matter::Superconductivity0103 physical sciencesTopological orderCondensed Matter::Strongly Correlated ElectronsPhysical and Theoretical Chemistry010306 general physics
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High Precision Differential Astrometry in Large Angular Separation Pairs of Radiosources

1994

We show preliminary results of three of the four radiosource pairs with angular separations ranging from 0.01° to 6° where we have determined such a separation with a typical fractional precision of 10-8using phase delays corrected for structural and ionospheric contributions. In the radiosource 4C39.25 we measure a motion with respect to an external radiosource which is compatible with previously reported internal superluminal motion.

PhysicsSuperluminal motionTotal electron contentAngular distancePhase (waves)RangingAstrophysicsAstrometryMeasure (mathematics)Group delay and phase delay
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Dust Envelope in Young Supernova Remnants

1974

As stated by Hoyle and Wickramasinghe (1970), hereafter referred to as HW, a significant fraction of the mass ejected by exploding supernovae may condense into solid particles during the expansion phase following explosion. Hence, observable effects on supernova light curves are to be expected.

PhysicsSupernovaCrab NebulaAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Solar and Stellar AstrophysicsAstronomyObservableAstrophysicsExpansion phaseNear-Earth supernovaLight curveEnvelope (waves)Luminosity
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Classical Geometric Phases: Foucault and Euler

2020

In the last chapter we saw how a quantum system can give rise to a Berry phase, by studying the adiabatic round trip of its quantum state on a certain parameter space. Rather than considering what happens to states in Hilbert space, we now turn to classical mechanics, where we are concerned instead with the evolution of the system in configuration space. As a first example, we are interested in the geometric phase of an oscillator that is constrained to a plane that is transported over some surface which moves along a certain path in three-dimensional space. Contrary to determining the Berry phase, there is no adiabatic approximation of the motion along the curve involved. The Foucault phas…

PhysicsSurface (mathematics)Foucault pendulumlaw.inventionAdiabatic theoremsymbols.namesakeClassical mechanicsGeometric phaseQuantum statelawEuler's formulasymbolsConfiguration spaceAdiabatic process
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A geometric analysis of the effects of noise on Berry phase

2007

In this work we describe the effect of classical and quantum noise on the Berry phase. It is not a topical review article but rather an overview of our work in this field aiming at giving a simple pictorial intuition of our results.

PhysicsWork (thermodynamics)Physics and Astronomy (miscellaneous)Geometric analysisField (physics)General MathematicsQuantum noiseQUANTUM COMPUTATIONNoiseGeometric phaseSYSTEMSSimple (abstract algebra)Quantum error correctionQuantum mechanicsgeometric phases open quantum systems quantum information theoryStatistical physics
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Theoretical Tools for the Description of Strong Field Laser-Molecule Interaction

2016

In this chapter, the main theoretical tools used in the work presented in the next two chapters on the laser control of the radiationless decay in pyrazine and of the tunneling dynamics in NHD\(_2\), are introduced.

PhysicsWork (thermodynamics)PyrazineStrong fieldLaserlaw.inventionchemistry.chemical_compoundGeometric phasechemistrylawMoleculeAtomic physicsRabi frequencyQuantum tunnelling
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Stochastic thermodynamics for active matter

2016

The theoretical understanding of active matter, which is driven out of equilibrium by directed motion, is still fragmental and model oriented. Stochastic thermodynamics, on the other hand, is a comprehensive theoretical framework for driven systems that allows to define fluctuating work and heat. We apply these definitions to active matter, assuming that dissipation can be modelled by effective non-conservative forces. We show that, through the work, conjugate extensive and intensive observables can be defined even in non-equilibrium steady states lacking a free energy. As an illustration, we derive the expressions for the pressure and interfacial tension of active Brownian particles. The l…

PhysicsWork (thermodynamics)Statistical Mechanics (cond-mat.stat-mech)FOS: Physical sciencesGeneral Physics and AstronomyThermodynamicsObservableDissipation01 natural sciences010305 fluids & plasmasActive matterSurface tension0103 physical sciencesStable phase010306 general physicsBrownian motionCondensed Matter - Statistical Mechanics
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