Stark Broadening of the Spectral Lines of Ne v | Zendy

Rafik Hamdi | Zendy; N. Ben Nessib | Zendy; M. S. Dimitrijević | Zendy; S. Sahal–Bréchot | Zendy

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Stark Broadening of the Spectral Lines of Ne v

Author(s) -

Rafik Hamdi,

N. Ben Nessib,

M. S. Dimitrijević,

S. Sahal–Bréchot

Publication year - 2007

Publication title -

the astrophysical journal supplement series

Language(s) - English

Resource type - Journals

eISSN - 1538-4365

pISSN - 0067-0049

DOI - 10.1086/513314

Subject(s) - semiclassical physics , stark effect , atomic physics , superstructure , line (geometry) , ab initio , helium , physics , ionization , electron , spectral line , electron density , proton , plasma , quantum mechanics , quantum , ion , geometry , mathematics , thermodynamics

Using a semiclassical approach, we have calculated ab initio electron-, proton-, and ionized helium-impact line widths and shift for 26 Ne V multiplets. Energy levels and oscillator strengths have been calculated using SUPERSTRUCTURE code. Results have been presented for an electron density of 1017 cm-3 as a function of temperature, and are compared with experimental and other theoretical results.

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