Search results for "Trap"

showing 10 items of 2144 documents

Time-separated oscillatory fields for high-precision mass measurements on short-lived Al and Ca nuclides

2008

High-precision Penning trap mass measurements on the stable nuclide 27Al as well as on the short-lived radionuclides 26Al and 38,39Ca have been performed by use of radiofrequency excitation with time-separated oscillatory fields, i.e. Ramsey's method, as recently introduced for the excitation of the ion motion in a Penning trap, was applied. A comparison with the conventional method of a single continuous excitation demonstrates its advantage of up to ten times shorter measurements. The new mass values of 26,27Al clarify conflicting data in this specific mass region. In addition, the resulting mass values of the superallowed beta-emitter 38Ca as well as of the groundstate of the beta-emitte…

PhysicsRadionuclide010308 nuclear & particles physicsSpecific massGeneral Physics and AstronomyFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Penning trap01 natural sciencesIonStable nuclide0103 physical sciencesNuclear Physics - ExperimentNuclideAtomic physicsNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentExcitation
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Collisional de-excitation of the metastableD-states of Ba+ by He, Ne, N2 and H2

1989

The rate constants 〈σ · υ〉 for collisional de-excitation of the metastable 5D states of Ba+ ions have been determined in an ion trap experiment. TheD-states are selectively populated by pulsed laser excitation of the 6P1/2 or 6P3/2 state and the decay at different background pressures is monitored by the change in fluorescence intensity of the excited ions. From the pressure dependence of the decay constants we calculate the de-excitation rate constants for different collision partners, averaged over the velocity distribution of the trapped ion cloud. For He, Ne, H2 and N2 we obtain in the c.m. energy range of 0.1–0.5 eV: 〈σ·υ〉 (He)=3.0±0.2·10−13cm3/s, 〈σ·υ〉 (Ne)=5.1±0.4·10−13cm3/s, 〈σ·υ〉 (…

PhysicsRange (particle radiation)NeonReaction rate constantchemistryMetastabilityExcited statechemistry.chemical_elementIon trapAtomic physicsAtomic and Molecular Physics and OpticsExcitationIonZeitschrift f�r Physik D Atoms, Molecules and Clusters
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Model-independent determination of dissociation energies: method and applications

2003

A number of methods are available for the purpose of extracting dissociation energies of polyatomic particles. Many of these techniques relate the rate of disintegration at a known excitation energy to the value of the dissociation energy. However, such a determination is susceptible to systematic uncertainties, mainly due to the unknown thermal properties of the particles and the potential existence of 'dark' channels, such as radiative cooling. These problems can be avoided with a recently developed procedure, which applies energy-dependent reactions of the decay products as an uncalibrated thermometer. Thus, it allows a direct measurement of dissociation energies, without any assumption …

PhysicsReaction rate constantRadiative coolingThermalPolyatomic ionPhysics::Atomic and Molecular ClustersAtomic physicsCondensed Matter PhysicsPenning trapBond-dissociation energyAtomic and Molecular Physics and OpticsDissociation (chemistry)ExcitationJournal of Physics B: Atomic, Molecular and Optical Physics
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Spatial separation of atomic states in a laser-cooled ion crystal

1998

A laser cooled ion crystal containing several hundred Ca+ ions has been stored in a linear Paul trap. Cooling is provided by a red detund laser at the 4S1/2−4P1/2 resonance transition. A second laser serves for repumping of those ions which decay from the excited 4P1/2 level to the metastable 3D3/2 state. The ions can be additionally excited by a third laser to a long lived metastable 3D5/2 energy level which decouples them from the cooling laser radiation. The light pressure acting upon the laser cooled ions pushes them into the direction of the laser beam. The ions in the metastable 3D5/2 state, however, do not experience any light pressure force and diffuse to the crystal side which poin…

PhysicsResolved sideband coolingPhysics::OpticsLaserAtomic and Molecular Physics and OpticsIonlaw.inventionCrystalPhysics::Plasma PhysicslawLaser coolingExcited statePhysics::Atomic PhysicsIon trapAtomic physicsAtomic vapor laser isotope separationPhysical Review A
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Ageing studies of TPB in noble gas detectors for dark matter and neutrinoless ββ decay searches

2017

Noble gases (Xe, Ar, Kr) are very attractive as detector media in Dark Matter search and neutrinoless double-beta decay experiments. However, the detection of their scintillation light (in the VUV spectral region) requires shifting the VUV light to visible light, where standard photosensors are more efficient. Tetraphenyl butadiene (TPB) is widely used as wavelength shifter, absorbing the VUV light and re-emitting in the blue region (~430nm). TPB is an organic molecule that may degrade due to exposure to environmental agents and also to ultraviolet light. In this work, we present TPB ageing studies due to exposure to VUV light, aiming at quantifying the reduction of the absolute fluorescenc…

PhysicsScintillation010308 nuclear & particles physicsPhotodetectorNoble gasTetraphenyl butadieneWavelength shifter01 natural sciences7. Clean energyAtomic and Molecular Physics and OpticsAnalytical Chemistrylaw.inventionchemistry.chemical_compoundchemistry13. Climate actionlaw0103 physical sciencesUltraviolet lightAtomic physics010306 general physicsInstrumentationSpectroscopyVisible spectrumMonochromator
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Action potentials induce biomagnetic fields in Venus flytrap plants

2020

Upon stimulation, plants elicit electrical signals that can travel within a cellular network analogous to the animal nervous system. It is well-known that in the human brain, voltage changes in certain regions result from concerted electrical activity which, in the form of action potentials (APs), travels within nerve-cell arrays. Electrophysiological techniques like electroencephalography, magnetoencephalography, and magnetic resonance imaging are used to record this activity and to diagnose disorders. In the plant kingdom, two types of electrical signals are observed: all-or-nothing APs of similar amplitudes to those seen in humans and animals, and slow-wave potentials of smaller amplitud…

PhysicsSensitive-plantbiologyAtomic Physics (physics.atom-ph)FOS: Physical sciencesPhysics - Applied PhysicsApplied Physics (physics.app-ph)biology.organism_classificationBiomagnetismPhysics - Atomic PhysicsElectrophysiologyBiological Physics (physics.bio-ph)BiophysicsPlant speciesVenus flytrapRepolarizationPhysics - Biological PhysicsIon channel
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gFactor of HydrogenlikeSi13+28

2011

We determined the experimental value of the $g$ factor of the electron bound in hydrogenlike $^{28}\mathrm{Si}^{13+}$ by using a single ion confined in a cylindrical Penning trap. From the ratio of the ion's cyclotron frequency and the induced spin flip frequency, we obtain $g=1.995\text{ }348\text{ }958\text{ }7(5)(3)(8)$. It is in excellent agreement with the state-of-the-art theoretical value of 1.995 348 958 0(17), which includes QED contributions up to the two-loop level of the order of $(Z\ensuremath{\alpha}{)}^{2}$ and $(Z\ensuremath{\alpha}{)}^{4}$ and represents a stringent test of bound-state quantum electrodynamics calculations.

PhysicsSingle ionlawg factorCyclotronGeneral Physics and AstronomyOrder (ring theory)Spin-flipElectronAtomic physicsPenning trapIonlaw.inventionPhysical Review Letters
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First Assignment and Line Strengths of the 4ν4 Band of 12CH4 near 1.9 μm

2001

Abstract The investigation of the methane spectrum in the region 1.6–2 μm has provided the first assignment and analysis of the 4ν 4 band near 1.9 μm. Hamiltonian and dipole moment operators written in tetrahedral formalism and adapted to the extrapolation method have been used to fit the spectra recorded at the Kitt Peak National Observatory/National Solar Observatory. Nearly 190 line positions and 160 measured intensities have been modeled with standard deviations of 0.107 cm −1 and 18.5%, respectively.

PhysicsSolar observatorybusiness.industryExtrapolationAtomic and Molecular Physics and OpticsStandard deviationSpectral lineDipolesymbols.namesakeOpticsObservatoryTetrahedronsymbolsPhysical and Theoretical ChemistryAtomic physicsbusinessHamiltonian (quantum mechanics)SpectroscopyJournal of Molecular Spectroscopy
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A polymer chain trapped between two parallel repulsive walls: A Monte-Carlo test of scaling behavior

1998

An off-lattice bead-spring model of a polymer chain trapped between two parallel walls a distance D apart is studied by Monte-Carlo methods, using chain lengths N in the range $$32 \le N \le 512$$ and distances D from 4 to 32 (in units of the maximum spring extension). The scaling behavior of the coil linear dimensions parallel to the plates and of the force on the walls is studied and discussed with the help of current theoretical predictions. Also the density profiles of the monomers across the slit are obtained and it is shown that the predicted variation with the distance z from a wall, $$\rho (z) \propto {z^{1/\nu }}$$ , is obtained only when one introduces an extrapolation length λ in…

PhysicsSolid-state physicsGaussianMonte Carlo methodExtrapolationSpring (mathematics)LambdaCondensed Matter PhysicsMolecular physicsElectronic Optical and Magnetic Materialssymbols.namesakeChain (algebraic topology)symbolsStatistical physicsScalingThe European Physical Journal B
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GRB 050410 and GRB 050412: are they really dark gamma-ray bursts?

2007

We present a detailed analysis of the prompt and afterglow emission of GRB 050410 and GRB 050412 detected by Swift for which no optical counterpart was observed. The 15-150 keV energy distribution of the GRB 050410 prompt emission shows a peak energy at 53 keV. The XRT light curve of this GRB decays as a power law with a slope of alpha=1.06+/-0.04. The spectrum is well reproduced by an absorbed power law with a spectral index Gamma_x=2.4+/-0.4 and a low energy absorption N_H=4(+3;-2)x10^21 cm^(-2) which is higher than the Galactic value. The 15-150 keV prompt emission in GRB 050412 is modelled with a hard (Gamma=0.7+/-0.2) power law. The XRT light curve follows a broken power law with the f…

PhysicsSpectral indexAstrophysics::High Energy Astrophysical PhenomenaExtrapolationAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curvePower lawAfterglowInterstellar mediumSpace and Planetary ScienceGamma-ray burstAbsorption (electromagnetic radiation)Astrophysics::Galaxy Astrophysics
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