Search results for "spheres"

showing 10 items of 329 documents

The heavenly spheres regained

1993

PhysicsHistory and Philosophy of ScienceGeneral MathematicsCelestial spheresAncient historyThe Mathematical Intelligencer
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London equation of state for a quantum-hard-sphere system

1994

The London analytical interpolation equation between zero and packing densities for the ground-state energy of a many-boson hard-sphere system is corrected for the reduced mass of a pair of particles in a ``sphere-of-influence'' picture. It is thus brought into good agreement with computer simulations and with experimental results extrapolated out to close packing.

PhysicsLondon equationsClassical mechanicsZero (complex analysis)Close-packing of equal spheresState (functional analysis)Reduced massGround stateQuantumInterpolationPhysical Review B
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MAGNETIC INTERACTIONS OF CHAINS FORMED BY FERROMAGNETIC SPHERES

2002

General properties of sphere-chain and chain-chain structures are analysed for homogeneously magnetized spheres. For field aligned structures the local maximum of the magnetic force is observed at H0/MS ≈ 0.5. The magnetic saturation effects are accounted by the Frölich-Kennelly law. Outlines of the approximate methodology of multi-chain interaction are given together with the test results.

PhysicsMaterials scienceCondensed matter physicsFerromagnetismField (physics)Statistical and Nonlinear PhysicsSPHERESCondensed Matter PhysicsMagnetic fieldInternational Journal of Modern Physics B
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Electrophoretic mobility of charged spheres

2008

The electrophoretic mobility μ of charged 0.3 µm Polystyrene spheres suspended in water was measured over a wide range of salt concentrations c and packing fractions Φ. To observe isolated spheres at packing fractions Φ ≤ 2 × 10−7 a newly developed optical tweezing electrophoresis (OTE) apparatus was used. At deionised conditions μ=2.5 × 10−8 m2V−1s−1, it decreases further upon increasing the salt concentration c. Measurements at larger Φ generally show much larger μ and a qualitatively different dependence on c. At no added salt μ increases in the unordered state but a saturation at μ=6.8 × 10−8 m2V−1s−1 is observed, as the system develops fluid order. The fluid-crystal phase transition is…

PhysicsMean squared displacementElectrokinetic phenomenaPhase transitionRange (particle radiation)ElectrophoresisAnalytical chemistrySPHERESConductivitySaturation (chemistry)
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Suspensions of rod-like colloids and a depleting agent under confinement

2008

We present a computer simulation study of suspensions of rod-like colloids and a depletant in confinement to a slit-pore. Mixtures of hard spherocylinders and ideal spheres were studied by means of Monte Carlo simulations in the grand canonical ensemble. By use of finite size scaling analysis we determined the critical behaviour. In order to overcome large barriers in the free energy we applied the successive umbrella sampling method (Virnau and Muller 2004 J. Chem. Phys. 120 10925). We find that, under confinement, the critical point of gas–liquid demixing shifts to higher concentrations of rods and smaller concentrations of spheres due to the formation of an orientationally ordered surfac…

PhysicsMonte Carlo methodThermodynamicsCondensed Matter PhysicsRodCondensed Matter::Soft Condensed MatterGrand canonical ensembleChemical physicsCritical point (thermodynamics)General Materials ScienceSPHERESWettingUmbrella samplingScalingJournal of Physics: Condensed Matter
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Fluids in extreme confinement.

2012

For extremely confined fluids with two-dimensional density $n$ in slit geometry of accessible width $L$, we prove that in the limit $L\to 0$ the lateral and transversal degrees of freedom decouple, and the latter become ideal-gas-like. For small wall separation the transverse degrees of freedom can be integrated out and renormalize the interaction potential. We identify $n L^2 $ as hidden smallness parameter of the confinement problem and evaluate the effective two-body potential analytically, which allows calculating the leading correction to the free energy exactly. Explicitly, we map a fluid of hard spheres in extreme confinement onto a 2d-fluid of disks with an effective hard-core diame…

PhysicsPhase transitionStatistical Mechanics (cond-mat.stat-mech)Degrees of freedom (physics and chemistry)General Physics and AstronomyFOS: Physical sciencesHard spheresCondensed Matter - Soft Condensed MatterTransverse planeBoundary layerClassical mechanicsTransition pointTransversal (combinatorics)Soft Condensed Matter (cond-mat.soft)Limit (mathematics)Condensed Matter - Statistical MechanicsPhysical review letters
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Generalized Bloch spheres form-qubit states

2006

m-Qubit states are imbedded in $\mathfrak{Cl}_{2^m}$ Clifford algebras. Their probability spectra then depend on $O(2m)$ or $O(2m+1)$ invariants. Parameter domains for $O(2m(+1))-$ vector and tensor configurations, generalizing the notion of a Bloch sphere, are derived.

PhysicsQuantum PhysicsBloch sphereClifford algebraFOS: Physical sciencesGeneral Physics and AstronomyStatistical and Nonlinear PhysicsSpectral lineComputer Science::Emerging TechnologiesQubitSPHERESTensorQuantum Physics (quant-ph)Mathematical PhysicsMathematical physicsJournal of Physics A: Mathematical and General
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Experimental Evidence for a Structural-Dynamical Transition in Trajectory Space.

2016

Among the key insights into the glass transition has been the identification of a non-equilibrium phase transition in trajectory space which reveals phase coexistence between the normal supercooled liquid (active phase) and a glassy state (inactive phase). Here we present evidence that such a transition occurs in experiment. In colloidal hard spheres we find a non-Gaussian distribution of trajectories leaning towards those rich in locally favoured structures (LFS), associated with the emergence of slow dynamics. This we interpret as evidence for an non-equilibrium transition to an inactive LFS-rich phase. Reweighting trajectories reveals a first-order phase transition in trajectory space be…

PhysicsQuantum phase transitionPhase transitionFOS: Physical sciencesGeneral Physics and Astronomy02 engineering and technologyHard spheresCondensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnologySpace (mathematics)01 natural sciencesCondensed Matter::Soft Condensed MatterClassical mechanicsPhase (matter)0103 physical sciencesTrajectorySoft Condensed Matter (cond-mat.soft)Statistical physics010306 general physics0210 nano-technologySupercoolingGlass transitionPhysical review letters
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Numerical study on the limit of quasi-static approximation for plasmonic nanosphere

2019

Plasmonic nanospheres are often employed as resonant substrates in many nanophotonic applications, like in enhanced spectroscopy, near-field microscopy, photovoltaics, and sensing. Accurate calculation and tuning of optical responses of such nanospheres are essential to achieve optimal performance. Mie theory is widely used to calculate optical properties of spherical particles. Although, an approximated version of Mie approach, the quasi-static approximation (QSA) can also be used to determine the very same properties of those spheres with a lot simpler formulations. In this work, we report our numerical study on the limit and accuracy of QSA with respect to the rigorous Mie approach. We c…

PhysicsScatteringMie scatteringNanophotonicsPhysics::Opticsoptiset ominaisuudetResonance (particle physics)Computational physicstiiviin aineen fysiikkaplasmonitError functionQuasistatic approximationcondensed matter physicsSPHERESnanohiukkasetPlasmon
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The Sun as a benchmark of flaring activity in stellar coronae

2009

The solar corona is a template to study and understand stellar activity. However the solar corona differs from that of active stars: the Sun has lower X‐ray luminosity, and on average cooler plasma temperatures. Active stellar coronae have a hot peak in their emission measure distribution, EM (T), at 8–20 MK, while the non‐flaring solar corona has a peak at 1–2 MK. In the solar corona significant amounts of plasma at temperature ∼10 MK are observed only during flares.To investigate what is the time‐averaged effect of solar flares we measure the disk‐integrated time‐averaged emission measure, EMF (T), of an unbiased sample of solar flares. To this aim we analyze uninterrupted GOES/XRS light …

PhysicsSolar flareStar formationopacity and line formationAstronomyStellar atmospheresAstrophysicsCoronal loopCoronal radiative lossesCoronalaw.inventionSolar cycleNanoflaresSettore FIS/05 - Astronomia E Astrofisicaradiative transferlawCoronal mass ejectionX-ray emission spectra and fluorescence gamma-rayFlareAIP Conference Proceedings
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