Search results for "IONIZATION"

showing 10 items of 1255 documents

Resonant scattering in macromolecular structure research. Applications in molecular biology and material science

1983

Abstract This report concerns the X-ray resonance scattering work carried out using the instrument X15 which receives synchrotron radiation from the storage ring DORIS. X15 covers a wavelength range from 0.6 to 3.3 A. It therefore accesses resonance scattering at the K-absorption edges of the elements with Z = 20 (Ca) to Z = 42 (Mo) and at the L 3 -absorption edges from Z = 50 (Sn) to all heavier atoms. The instrument consists of a double monochromator with a vertical offset of the beam by 1.22 m and a camera of 10 m length. A multiwire proportional chamber (from A. Gabriel) at the end of the evacuated beam line detects the scattered X-ray photons on its area 200 mm × 200 mm. The distances …

PhysicsExtended X-ray absorption fine structureAbsorption spectroscopyScatteringMolecular physicsXANESIonInorganic ChemistryExcited stateMaterials ChemistryRadius of gyrationPhysical chemistryPhysical and Theoretical ChemistryIonization energyInorganica Chimica Acta
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Beta Decay of Molecular Tritium

2020

The beta decay of tritium in the form of molecular TT is the basis of sensitive experiments to measure neutrino mass. The final-state electronic, vibrational, and rotational excitations modify the beta spectrum significantly, and are obtained from theory. We report measurements of the branching ratios to specific ionization states for the isotopolog HT. Two earlier, concordant measurements gave branching ratios of HT to the bound HHe$^+$ ion of 89.5% and 93.2%, in sharp disagreement with the theoretical prediction of 55-57%, raising concerns about the theory's reliability in neutrino mass experiments. Our result, 56.5(6)%, is compatible with the theoretical expectation and disagrees strongl…

PhysicsFOS: Physical sciencesGeneral Physics and AstronomyBranching (polymer chemistry)01 natural sciencesBeta decayIonIonization0103 physical sciencesTritiumNuclear Experiment (nucl-ex)Atomic physicsNeutrino010306 general physicsNuclear ExperimentPhysical Review Letters
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Configuration-interaction calculations of jellium clusters by the nuclear shell model

1994

Configuration-interaction (CI) calculations are performed on Na clusters of up to 20 atoms within the spherical jellium model, with particular attention paid to the magic clusters with N=2, 8, and 20. The interacting valence electrons are assumed to move in the Coulomb field of the jellium core. The numerical work is carried out by the nuclear-structure code oxbash modified to handle LS coupling. The many-particle bases are constructed of harmonic-oscillator single-particle states extending over 11 major shells and, alternatively, of single-particle states generated by the local-spin-density approximation (LSDA). The calculated quantities include ground- and excited state energies, ionizati…

PhysicsField (physics)Excited stateIonizationJelliumPhysics::Atomic and Molecular ClustersQuasiparticleNuclear shell modelConfiguration interactionAtomic physicsValence electronPhysical Review B
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X‐Ray Spectroscopy of the Unsteady Quiescent Corona of AD Leonis withChandra

2004

We present the analysis and interpretation of an observation of the flare star AD Leo (dM3e) with Chandra/LETG. The high resolution X-ray spectrum allowed us to infer the plasma emission measure distribution (EMD) vs. temperature, and the abundances of individual elements in the corona of this magnetically-active star, during a typical state characterized by significant variability but no large flaring event. We have also measured plasma densities at various temperatures using spectroscopic diagnostics provided by He-like triplets and Fe XXI lines. We show that the present EMD is similar to those previously obtained from EUVE spectra during quiescent and flaring states, confirming the long-…

PhysicsFilling factorAstrophysics::High Energy Astrophysical PhenomenaMetallicityAstrophysics (astro-ph)Flare starFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaAstrophysicsCoronaSpectral lineStarsSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsIonization energyThe Astrophysical Journal
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Finite difference time domain simulation of soil ionization in grounding systems under lightning surge conditions

2004

This paper proposes a Maxwell’s equations finite difference time domain (FDTD) approach for electromagnetic transients in ground electrodes in order to take into account the non linear effects due to soil ionization. A time variable soil resistivity method is used in order to simulate the soil breakdown, without the formulation of an initial hypothesis about the geometrical shape of the ionized zone around the electrodes. The model has been validated by comparing the computed results with available data found in technical literature referred to concentrated earths. Some application examples referred to complex grounding systems are reported to show the computational capability of the propos…

PhysicsFinite difference electromagnetic transient grounding systemsGroundSoil resistivityFinite differenceFinite-difference time-domain methodSoil ionizationOcean EngineeringMechanicsPhysics::Classical PhysicsNon-linear effectsSettore MAT/08 - Analisi NumericaSettore ING-IND/31 - ElettrotecnicaIonizationLightning surgesSimulation
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Stability of a Tensioned Axially Moving Plate Subjected to Cross-Direction Potential Flow

2015

We analyze the stability of an axially moving Kirchhoff plate, subjected to an axial potential flow perpendicular to the direction of motion. The dimensionality of the problem is reduced by considering a cross-directional cross-section of the plate, approximating the axial response with the solution of the corresponding problem of a moving plate in vacuum. The flow component is handled via a Green’s function solution. The stability of the cross-section is investigated via the classical Euler type static linear stability analysis method. The resulting eigenvalue problem is solved numerically using Hermite type finite elements. As a result, the critical velocity and the corresponding eigenfun…

PhysicsFlow (mathematics)BucklingAntisymmetric relationPotential flowMechanicsEigenfunctionCritical ionization velocityAxial symmetryFinite element method
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AC-Stark shift and photoionization of Rydberg atoms in an optical dipole trap

2010

We have measured the AC-Stark shift of the $14D_{5/2}$ Rydberg state of rubidium 87 in an optical dipole trap formed by a focussed CO$_2$-laser. We find good quantitative agreement with the model of a free electron experiencing a ponderomotive potential in the light field. In order to reproduce the observed spectra we take into account the broadening of the Rydberg state due to photoionization. The extracted cross-section is compatible with previous measurements on neighboring Rydberg states.

PhysicsFree electron modelAtomic Physics (physics.atom-ph)General Physics and AstronomyFOS: Physical sciencesPhotoionizationSpectral linePhysics - Atomic Physicssymbols.namesakeDipoleStark effectRydberg atomsymbolsRydberg formulaPhysics::Atomic PhysicsRydberg stateAtomic physics
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Radiative recombination in a strong laser field: low-frequency approximation

2005

A theoretical treatment of the laser-assisted radiative recombination (LARR) is presented in which the low-frequency (LF) assumption is exploited. The merit of the proposed LF approximation is twofold. First, the LF approximation considerably simplifies the calculations of the transition rates, whereas the results obtained within this approximation are only slightly different from those obtained without resorting to it. Second, the LF approximation gives more insight into the physical picture of the process, which may be viewed as a two-step process. In the first step, the free electron propagates toward the ion, and its motion is described classically with motion changes ascribed mainly to…

PhysicsFree electron modelStatistical and Nonlinear PhysicsObservableOptical fieldMaxwell–Boltzmann distributionAtomic and Molecular Physics and OpticsComputational physicssymbols.namesakeDistribution functionIonizationElectric fieldsymbolsHigh harmonic generationAtomic physicsJournal of the Optical Society of America B
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GW quasiparticle energies of atoms in strong magnetic fields

2019

Quasiparticle energies of the atoms H–Ne have been computed in the GW approximation in the presence of strong magnetic fields with field strengths varying from 0 to 0.25 atomic units (0.25 B 0 =0.25 ℏe −1 a −2 0 ≈58 763 0.25 B0=0.25 ℏe−1a0−2≈58 763 T). The GW quasiparticle energies are compared with equation-of-motion ionization-potential (EOM-IP) coupled-cluster singles-and-doubles (CCSD) calculations of the first ionization energies. The best results are obtained with the evGW@PBE0 method, which agrees with the EOM-IP-CCSD model to within about 0.20 eV. Ionization potentials have been calculated for all atoms in the series, representing the first systematic study of ionization potentials …

PhysicsGW approximation010304 chemical physicsField (physics)General Physics and AstronomyField strengthElectron010402 general chemistry01 natural sciences7. Clean energy0104 chemical sciencesMagnetic fieldIonization0103 physical sciencesPhysics::Atomic and Molecular ClustersQuasiparticlePhysics::Atomic PhysicsPhysical and Theoretical ChemistryAtomic physicsIonization energyThe Journal of Chemical Physics
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Rydberg Series Excitation of a Single Trapped Ca+40 Ion for Precision Measurements and Principal Quantum Number Scalings

2021

A complete set of spectroscopic data is indispensable when using Rydberg states of trapped ions for quantum information processing. We carried out Rydberg series spectroscopy for $n{S}_{1/2}$ states with $38\ensuremath{\le}n\ensuremath{\le}65$ and for $n{D}_{5/2}$ states with $37\ensuremath{\le}n\ensuremath{\le}50$ on a single trapped $^{40}{\mathrm{Ca}}^{+}$ ion. We determined the ionization energy of 2 870 575.582(15) GHz, 60 times more accurately as compared to the accepted value and contradicting it by 7.5 standard deviations. We confirm quantum defect values of ${\ensuremath{\delta}}_{{S}_{1/2}}=1.802\text{ }995(5)$ and ${\ensuremath{\delta}}_{{D}_{5/2}}=0.626\text{ }888(9)$ for $n{S}_…

PhysicsGeneral Physics and Astronomy01 natural sciences010305 fluids & plasmasIonsymbols.namesakeQuantum defectIonization0103 physical sciencesPrincipal quantum numberRydberg formulasymbolsPhysics::Atomic PhysicsAtomic physicsIonization energy010306 general physicsSpectroscopyExcitationPhysical Review Letters
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