Search results for "Cooling"

showing 10 items of 470 documents

Transverse laser cooling of a radio-frequency bunched ion beam in the storage ring TSR

1996

Abstract We report on the observation of the indirect transverse laser cooling effect in a radio-frequency bunched beam of 7.3 MeV 9 Be + ions, stored in the Heidelberg Test Storage Ring and subject to direct longitudinal laser cooling. This bunched scheme offers particular advantages for producing ultracold beams with unprecedented phase-space densities.

PhysicsNuclear and High Energy PhysicsResolved sideband coolingIon beamIonTransverse planeLaser coolingPhysics::Accelerator PhysicsPhysics::Atomic PhysicsRadio frequencyAtomic physicsNuclear ExperimentInstrumentationBeam (structure)Storage ring
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3D Gray Radiative Properties of Accretion Shocks in Young Stellar Objects

2013

International audience; We address the problem of the contribution of radiation to the structure and dynamics of accretion shocks on Young Stellar Objects. Solving the 3D RTE (radiative transfer equation) under our "gray LTE approach", i.e., using appropriate mean opacities computed in local thermodynamic equilibrium, we post-process the 3D MHD (magne-tohydrodynamic) structure of an accretion stream impacting the stellar chromosphere. We find a radiation flux of ten orders of magnitude larger than the accreting energy rate, which is due to a large overestimation of the radiative cooling. A gray LTE radiative transfer approximation is therefore not consistent with the given MHD structure of …

PhysicsOpacityRadiative coolingPhysicsQC1-999Young stellar objectAstrophysics[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Accretion (astrophysics)Radiation fluxN/A13. Climate actionRadiative transferAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsChromosphereAstrophysics::Galaxy Astrophysics
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Ballistic phonon transport in dielectric membranes

2006

We have calculated the ballistic phononic heat transport in dielectric membranes as a function of radiator temperature and membrane thickness. The phonon modes of such membranes are known as Lamb-modes from elasticity theory. The striking result is that, for a fixed temperature, the radiated power first decreases with decreasing membrane thickness, but then develops a minimum when the transition to two dimensionality is reached. Further decrease of the membrane thickness in the 2D limit leads to increasing radiated power.

PhysicsPhysics::Biological PhysicsNuclear and High Energy PhysicsCondensed matter physicsPhononMembrane thicknessDielectricEffective radiated powerElasticity (physics)Quantitative Biology::Cell BehaviorQuantitative Biology::Subcellular ProcessesMembraneBallistic conductionRadiator (engine cooling)InstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Continuous Lyman-alpha generation by four-wave mixing in mercury for laser cooling of antihydrogenThis paper was presented at the International Confe…

2011

Cooling antihydrogen atoms is important for future experiments both to test the fundamental CPT symmetry by high resolution laser spectroscopy and also to measure the gravitational acceleration of antimatter. Laser cooling of antihydrogen can be done on the strong 1S–2P transition at the wavelength of Lyman-alpha (121.6 nm). A continuous wave laser at the Lyman-alpha wavelength based on solid-state fundamental lasers is described. By using a two-photon and a near one-photon resonance a scan across the whole phase matching curve of the four-wave mixing process is possible. Furthermore the influence of the beam profile of one fundamental beam on the four-wave mixing process is studied.

PhysicsPhysics::General PhysicsPhysics::OpticsGeneral Physics and AstronomyLaserlaw.inventionWavelengthFour-wave mixinglawAntimatterLaser coolingContinuous wavePhysics::Atomic PhysicsAtomic physicsAntihydrogenMixing (physics)Canadian Journal of Physics
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A novel cooling scheme for antiprotons

2006

We propose a novel technique which uses laser-cooled negative osmium ions for sympathetic cooling of antiprotons. Temperatures down to the sub-millikelvin range might be achievable. These antiprotons could be used to form antihydrogen at ultra-cold temperatures, thus allowing efficient magnetic trapping of antihydrogen for high-resolution laser spectroscopy. Antihydrogen at sub-millikelvin temperatures might also enable first direct measurements of the gravitational acceleration of antimatter. Currently, no other technique exists which allows the cooling of large numbers of antiprotons to temperatures below that of the surrounding trap.

PhysicsPhysics::General PhysicsSympathetic coolingRange (particle radiation)General Physics and AstronomyTrappingGravitational accelerationIonNuclear physicsAntiprotonAntimatterPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsAntihydrogenNew Journal of Physics
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Trapping and sympathetic cooling of single thorium ions for spectroscopy

2018

Precision optical spectroscopy of exotic ions reveals accurate information about nuclear properties such as charge radii and magnetic and quadrupole moments. Thorium ions exhibit unique nuclear properties with high relevance for testing symmetries of nature. We report loading and trapping of single $^{232}$Th$^+$ ions in a linear Paul trap, embedded into and sympathetically cooled by small crystals of trapped $^{40}$Ca$^+$ ions. Trapped Th ions are identified in a non-destructive manner from the voids in the laser-induced Ca fluorescence pattern emitted by the crystal, and alternatively, by means of a time-of-flight signal when extracting ions from the Paul trap and steering them into an ex…

PhysicsQuantum PhysicsSympathetic coolingAtomic Physics (physics.atom-ph)Thoriumchemistry.chemical_elementFOS: Physical sciences01 natural sciencesPhysics - Atomic Physics010305 fluids & plasmasIonCrystalchemistry0103 physical sciencesQuadrupoleQuantum efficiencyIon trapPhysics::Atomic PhysicsAtomic physics010306 general physicsSpectroscopyQuantum Physics (quant-ph)
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Liquid-liquid phase coexistence in gold clusters. 2D or not 2D?

2006

The thermodynamics of gold cluster anions (${\mathrm{Au}}_{N}^{\ensuremath{-}}$, $N=11,\dots{},14$) is investigated using quantum molecular dynamics. Our simulations suggest that ${\mathrm{Au}}_{N}^{\ensuremath{-}}$ may exhibit a novel, freestanding planar liquid phase which dynamically coexists with a normal three-dimensional liquid. Upon cooling with experimentally realizable cooling rates, the entropy-favored three-dimensional liquid clusters often supercool and solidify into the ``wrong'' dimensionality. This indicates that experimental validation of theoretically predicted ${\mathrm{Au}}_{N}^{\ensuremath{-}}$ ground states might be more complicated than hitherto expected.

PhysicsQuantum phase transitionGold clusterliquid-liquid transitionGeneral Physics and AstronomyThermodynamicsExperimental validationMolecular physicsQuantum molecular dynamicsPhysics::Fluid DynamicsPlanarClusterPhase (matter)phase transitions in clusterLiquid liquidSupercoolingspectroscopy and geometrical structure of clusters
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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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An investigation of environmental temperature effects on energy exchange by thermal radiation

2013

The radiative heating or cooling of a body placed in an environment, whose temperature is considered constant is described by Stefan's law. In this paper, an analysis is made of how a time-dependent environmental temperature influences the heating/cooling process. We compare experimental results for a resistor first heated by the Joule effect inside a glass vacuum tube and then cooled under two different conditions: in a bath at a constant temperature and in air. We also discuss a model that describes how the time-dependent tube temperature influences the radiative resistor cooling by identifying the properties of the environment that make the resistor cooling rate linear.

PhysicsRadiative coolingSettore FIS/08 - Didattica E Storia Della FisicaJoule effectVacuum tubeGeneral Physics and AstronomyThermodynamicsMechanicslaw.inventionThermal radiationlawRadiative transferLaboratory procedures Thermal radiation Physics educationTube (fluid conveyance)ResistorConstant (mathematics)American Journal of Physics
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The importance of magnetic-field-oriented thermal conduction in the interaction of SNR shocks with interstellar clouds

2008

We explore the importance of magnetic-field-oriented thermal conduction in the interaction of supernova remnant (SNR) shocks with radiative gas clouds and in determining the mass and energy exchange between the clouds and the hot surrounding medium. We perform 2.5D MHD simulations of a shock impacting on an isolated gas cloud, including anisotropic thermal conduction and radiative cooling; we consider the representative case of a Mach 50 shock impacting on a cloud ten-fold denser than the ambient medium. We consider different configurations of the ambient magnetic field and compare MHD models with or without the thermal conduction. The efficiency of the thermal conduction in the presence of…

PhysicsRadiative coolingsupernovaeAstrophysics (astro-ph)Interstellar cloudFOS: Physical sciencesAstronomy and Astrophysicsheat conductionAstrophysicsMagnetohydrodynamicThermal conductionAstrophysicsComputational physicsMagnetic fieldSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceThermalRadiative transferMagnetohydrodynamicsSupernova remnantAstrophysics::Galaxy Astrophysics
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