Stark broadening in the Sb III spectrum

Djeniže, S.

doi:10.1016/j.physleta.2008.09.029

Cited by 4 publications

(3 citation statements)

References 25 publications

(27 reference statements)

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“…A semi-empirical approach, which uses a set of wave functions obtained from Hartree-Fock relativistic calculations and includes core polarization effects, has been applied to 58 lines of Pb IV (Alonso-Medina Broadening parameters have been obtained experimentally for the following numbers of lines: Bukvić et al 2011), 28 Cd III , Bukvić et al 2009b, 13 Si I, 15 Si II, 28 Si III and 9 Si IV (Bukvić et al 2009a), 29 (Bukvić et al 2008) (Peláez et al 2010b), 38 Xe II (Peláez et al 2009a, Peláez et al 2009b, 10 Xe III (Peláez et al 2009b), 5 Au I and 26 Au II (Djeniže 2009), 9 Sb III (Djeniže 2008), 15 Mn I and 10 Fe I (Zielinska et al 2010), 21 Fe II (Aragón et al 2011) and C I 833.5 nm (Bartecka et al 2011).…”

Section: Isolated Linesmentioning

confidence: 99%

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Division Xii / Commission 14 / Working Group Collision Processes

Peach¹,

Dimitrijević²

2011

Proc. IAU

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Research in atomic and molecular collision processes and spectral line broadening has been very active since our last report, Peach, Dimitrijević & Stancil 2009. Given the large volume of the published literature and the limited space available, we have attempted to identify work most relevant to astrophysics. Since our report can not be comprehensive, additional publications can be found in the databases at the web addresses listed in the final section. Elastic and inelastic collisions among electrons, atoms, ions, and molecules are included and charge transfer can be very important in collisions between heavy particles.

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Section: Isolated Linesmentioning

confidence: 99%

“…and 19(Djurović et al 2011) Ar III, 30 Kr III( Ćirišan et al 2011), 12 Ne II, 8 Kr II and 5 Xe II(Peláez et al 2010b), 38 Xe II(Peláez et al 2009a, Peláez et al 2009b, 10 Xe III(Peláez et al 2009b), 5 Au I and 26 Au II(Djeniže 2009), 9 Sb III(Djeniže 2008), 15 Mn I and 10 Fe I(Zielinska et al 2010), 21 Fe II …”

mentioning

confidence: 99%

Division Xii / Commission 14 / Working Group Collision Processes

Peach¹,

Dimitrijević²

2011

Proc. IAU

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“…Besides the astrophysical importance, antimony is also significant in thin films and nanotechnologies [25][26][27], and as a laser medium [28]. Concerning antimony and its ionization stages, for Stark broadening in literature exist only experimental results for Sb III [29] and theoretical data for Sb II [30].…”

Section: Introductionmentioning

confidence: 99%

Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines

Dimitrijević

Simić

Stamm

et al. 2018

Atoms

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Stark broadening parameters, line width and shift, are needed for investigations, analysis and modelling of astrophysical, laboratory, laser produced and technological plasmas. Especially in astrophysics, due to constantly increasing resolution of satellite borne spectrographs, and large terrestrial telescopes, data on trace elements, which were previously insignificant, now have increasing importance. Using the modified semiempirical method of Dimitrijević and Konjević, here, Stark widths have been calculated for 2 Se IV, 6 Sn IV, 2 Sb IV and 1 Te IV transitions. Results have been compared with existing theoretical data for Sn IV. Obtained results will be implemented in the STARK-B database, which is also a part of Virtual atomic and molecular data center (VAMDC).

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