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相关论文: Stark Broadening of the B III 2s-2p Lines

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The Stark widths of the Ne VII 2s3s-2s3p singlet and triplet lines are calculated in the impact approximation using quantum-mechanical Convergent Close-Coupling and Coulomb-Born-Exchange approximations. It is shown that the contribution…

原子物理 · 物理学 2009-10-31 Yuri V. Ralchenko , Hans R. Griem , Igor Bray , Dmitry V. Fursa

Recent experimental and theoretical (both improved semiclassical and fully quantum-mechanical) results for B III and Ne VII delta n = 0 transitions with n = 2 or 3, respectively, are discussed. The probable reasons for disagreements by…

原子物理 · 物理学 2009-10-31 Hans R. Griem , Yuri V. Ralchenko

In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we determined Stark widths and shifts due to electron, proton, and ionized helium impacts, for nine lines (4191.0, 4259.4, 5912.1, 6043.2,…

太阳与恒星天体物理 · 物理学 2018-03-14 Milan S. Dimitrijevic , Andjelka Kovacevic , Zoran Simic , Sylvie Sahal-Brechot

The collisional electron-impact line widths of the 3s-3p transitions in Li-like ions from B III to Ne VIII are calculated with the convergent close-coupling (CCC) method from the atomic collision theory. The elastic and inelastic…

原子物理 · 物理学 2015-06-26 Yu. V. Ralchenko , H. R. Griem , I. Bray

The electron-impact widths for 15 doubly charged Nb ion lines have been theoretically determined by using the modified semiempirical method. Using the obtained results, we considered the influence of the electron-impact mechanism on line…

太阳与恒星天体物理 · 物理学 2015-06-17 Zoran Simić , Milan S. Dimitrijević , Luka Č. Popović

Besides the need of Stark broadening parameters for a number of problems in physics, and plasma technology, in hot star atmospheres the conditions exist where Stark widths are comparable and even larger than the thermal Doppler widths.…

太阳与恒星天体物理 · 物理学 2018-03-14 Z. Simic , M. S. Dimitrijevic , A. B. Kovacevic , S. Sahal-Brechot

Using semiclassical perturbation approach in impact approximation, we have calculated Stark widths for 32 spectral lines of doubly charged argon (Ar III). Oscillator strengths are calculated using Hartree-Fock method with relativistic…

太阳与恒星天体物理 · 物理学 2015-06-17 Rafik Hamdi , Nabil Ben Nessib , Sylvie Sahal-Bréchot , Milan S. Dimitrijević

Stark broadening theory is currently operated for calculating widths and shifts of spectral lines that are needed for spectroscopic diagnostics and modelling in astrophysics, laboratory and technological plasmas. We have calculated a great…

太阳与恒星天体物理 · 物理学 2018-03-14 Sylvie Sahal-Brechot , Milan S. Dimitrijevic , Nebil Ben Nessib

We present in this paper electron impact broadening for six Ar XV lines using our quantum mechanical formalism and the semiclassical perturbation one. Additionally, our calculations of the corresponding atomic structure data (energy levels…

原子物理 · 物理学 2015-06-17 Haykel Elabidi , Sylvie Sahal-Bréchot , Milan S Dimitrijević

We consider the excitation dynamics of the two-photon \sts transition in a beam of atomic hydrogen by 243 nm laser radiation. Specifically, we study the impact of ionization damping on the transition line shape, caused by the possibility of…

Stark effect is observed in many natural and artificial plasmas and is of great importance for diagnostic purposes. Since this effect alters profiles of spectral lines, it should be taken into account when assessing chemical composition of…

太阳与恒星天体物理 · 物理学 2019-07-17 Andrey M. Popov , Nikolay I. Sushkov , Sergey M. Zaytsev , Timur A. Labutin

Radiative atomic data and electron impact excitation cross sections for the $2s-2p$ transitions in O VI for transitions among the fine structure levels belonging to the $1s^{2}nl$ ($2\leq n\leq5$) configurations have been calculated. We…

原子物理 · 物理学 2018-03-14 Haykel Elabidi , Sylvie Sahal-Bréchot , Nébil Ben Nessib

A semi-empirical method is used to characterize the 3s(2)3p(2)-3s3p(3) J=2 transition array in P II. In this method, Slater, spin-orbit, and radial parameters are fitted to experimental energy levels in order to obtain a description of the…

原子物理 · 物理学 2015-05-19 Jeremy Bancroft Brown , Lorenzo J. Curtis , David G. Ellis

We present electron collision strengths and their thermally averaged values for the forbidden lines of the astronomically abundant doubly-ionized oxygen ion, O^{2+}, in an intermediate coupling scheme using the Breit-Pauli relativistic…

原子物理 · 物理学 2014-05-30 P. J. Storey , Taha Sochi , N. R. Badnell

We report measurements of the Stark shifts and Stark widths of sodium spectral lines corresponding to nS-3P and mD-3P transitions. Measurements have been made on AC driven high pressure NaHg and NaCd discharges. Electron density has been…

经典物理 · 物理学 2007-05-23 Z. Miokovic , D. Balkovic , D. Veza

Collisions between electrons and radiating atoms broaden spectral absorption and emission lines in dense plasmas. High densities also introduce screening and pressure ionization effects that distort the wavefunctions of both bound and free…

等离子体物理 · 物理学 2026-02-26 Julian P. Kinney , Stephanie B. Hansen , Thomas A. Gomez , Scott D. Baalrud

We present the most accurate up-to-date theoretical values of the {2p_{1/2}}-{2s} and {2p_{3/2}}-{2s} transition energies and the ground-state hyperfine splitting in ${\rm Sc}^{18+}$. All two- and three-electron contributions to the energy…

Isotope shifts of the 2$p_{3/2}$-2$p_{1/2}$ transition in B-like ions are evaluated for a wide range of the nuclear charge number: Z=8-92. The calculations of the relativistic nuclear recoil and nuclear size effects are performed using a…

We determined relative X-ray photon emission cross sections in Fe XVII ions that were mono-energetically excited in an electron beam ion trap. Line formation for the 3s (3s-2p) and 3d (3d-2p) transitions of interest proceeds through…

Using first-principles calculations, we identify magic wavelengths for the 2s-2p and 2s-3p transitions in lithium. The ns and np atomic levels have the same ac Stark shifts at the corresponding magic wavelength, which facilitates…

原子物理 · 物理学 2015-06-05 M. S. Safronova , U. I. Safronova , Charles W. Clark
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