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相关论文: R-matrix inner-shell electron-impact excitation of…

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We present results for the electron-impact excitation of highly-charged sulphur ions (S8+ - S11+) obtained using the intermediate-coupling frame transformation R-matrix approach. A detailed comparison of the target structure has been made…

太阳与恒星天体物理 · 物理学 2015-05-30 G. Y. Liang , N. R. Badnell , G. Zhao , J. Y. Zhong , F. L. Wang

We have carried-out two intermediate coupling frame transformation (ICFT) R-matrix calculations for the electron-impact excitation of C-like Fe $^{20+}$, both of which use the same expansions for their configuration interaction (CI) and…

原子物理 · 物理学 2016-04-12 L Fernandez-Menchero , A S Giunta , G Del Zanna , N R Badnell

Collision strengths for electron-impact of fine-structure level excitation within the ground term of Ne$^{+}$ and Ne$^{2+}$ are calculated using the Breit-Pauli, Intermediate Coupling Frame Transformation, and DARC $R$-matrix methods.…

原子物理 · 物理学 2017-05-31 Qianxia Wang , S. D. Loch , Y. Li , M. S. Pindzola , R. Cumbee , P. Stancil , B. McLaughlin , C. P. Ballance

There are major discrepancies between recent ICFT (Intermediate Coupling Frame Transformation) and DARC (Dirac Atomic R-matrix Code) calculations (Fern\'andez-Menchero et al. 2014, Astron. Astroph. 566 A104, Aggarwal et al. 2016 Mon. Not. R…

原子物理 · 物理学 2017-03-10 L. Fernández-Menchero , O. Zatsarinny , K. Bartschat

A theoretical investigation of photoabsorption and photoionization of Fe^{14+} extending beyond an earlier frame transformation R-matrix implementation is performed using a fully-correlated, Breit-Pauli R-matrix formulation including both…

原子物理 · 物理学 2015-06-04 M. F. Hasoglu , T. W. Gorczyca , M. A. Bautista , Z. Felfli , S. T. Manson

As part of a project to compute improved atomic data for the spectral modeling of iron K lines, we report extensive calculations and comparisons of atomic data for K-vacancy states in Fe XXIV. The data sets include: (i) energy levels, line…

天体物理学 · 物理学 2009-11-07 M. A. Bautista , C. Mendoza , T. R. Kallman , P. Palmeri

Modeling the spectral emission of low-charge iron group ions enables the diagnostic determination of the local physical conditions of many cool plasma environments such as those found in H II regions, planetary nebulae, active galactic…

星系天体物理 · 物理学 2015-06-18 N. R. Badnell , C. P. Ballance

Emission and absorption features from C-like ions serve as temperature and density diagnostics of astrophysical plasmas. $R$-matrix electron-impact excitation data sets for C-like ions in the literature merely cover a few ions, and often…

太阳与恒星天体物理 · 物理学 2020-01-29 Junjie Mao , N. R. Badnell , G. Del Zanna

With construction of ITER progressing and existing tokamaks carrying out ITER-relevant experiments, accurate fundamental and derived atomic data for numerous ionization stages of tungsten (W) is required to assess the potential effect of…

原子物理 · 物理学 2015-08-28 M. M. Bluteau , M. G. O'Mullane , N. R. Badnell

A comprehensive study of relativistic and resonance effects in electron impact excitation of (e+Fe XVII) is carried out using the BPRM method in the relativistic close coupling approximation. Two sets of eigenfunction expansions are…

天体物理学 · 物理学 2009-11-07 Guo-Xin Chen , Anil K. Pradhan , W. Eissner

Fe II emission lines are observed from nearly all classes of astronomical objects over a wide spectral range from the infrared to the ultraviolet. To meaningfully interpret these lines, reliable atomic data are necessary. In work presented…

原子物理 · 物理学 2019-03-12 Yier Wan , C. Favreau , S. D. Loch , B. M. McLaughlin , Yueying Qi , P. C. Stancil

Neutral tungsten is the primary candidate as a wall material in the divertor region of the International Thermonuclear Experimental Reactor (ITER). The efficient operation of ITER depends heavily on precise atomic physics calculations for…

原子物理 · 物理学 2018-05-09 R. T. Smyth , C. P. Ballance , C. A. Ramsbottom , C. A. Johnson , D. A. Ennis , S. D. Loch

Spectral lines from N-like ions can be used to measure the temperature and density of various types of astrophysical plasmas. The atomic databases of astrophysical plasma modelling codes still have room for improvement in their…

太阳与恒星天体物理 · 物理学 2020-11-18 Junjie Mao , N. R. Badnell , G. Del Zanna

Aims. This work reports radiative transition rates and electron impact excitation collision strengths for levels of the 3s23p, 3s3p2, 3s24s, and 3s23d configurations of Siii. Methods. The radiative data were computed using the…

星系天体物理 · 物理学 2015-05-14 M. A. Bautista , P. Quinet , P. Palmeri , N. R. Badnell , J. Dunn , N. Arav

Cross sections are presented for dissociative recombination and electron-impact vibrational excitation of the ArH+ molecular ion at electron energies appropriate for the interstellar environment. The R-matrix method is employed to determine…

星系天体物理 · 物理学 2018-08-21 A. Abdoulanziz , F. Colboc , D. A. Little , Y. Moulane , J. Zs. Mezei , E. Roueff , J. Tennyson , I. F. Schneider , V. Laporta

We present Maxwellian-averaged effective collision strengths for the electron-impact excitation of S III over a wide range of electron temperatures of astrophysical importance, log T(K) = 3.0-6.0. The calculation incorporates 53…

太阳与恒星天体物理 · 物理学 2015-06-16 M. F. R. Grieve , C. A. Ramsbottom , C. E. Hudson , F. P. Keenan

The five J$\Pi$ levels within a $np^2$ or $np^4$ ground state complex provide an excellent testing ground for the comparison of theoretical line ratios with astrophysically observed values, in addition to providing valuable electron…

地球与行星天体物理 · 物理学 2012-04-02 B. M. McLaughlin , Teck-Ghee Lee , J. A. Ludlow , E. Landi , S. D. Loch , M. S. Pindzola , C. P. Ballance

There have been discussions in the recent literature regarding the accuracy of the available electron impact excitation rates (equivalently effective collision strengths $\Upsilon$) for transitions in Be-like ions. In the present paper we…

原子物理 · 物理学 2016-09-07 K. M. Aggarwal , F. P. Keenan , K. D. Lawson

We have measured the resonance strengths and energies for dielectronic recombination (DR) of Fe XX forming Fe XIX via N=2 --> N'=2 (Delta_N=0) core excitations. We have also calculated the DR resonance strengths and energies using…

We report a detailed study of features of electron-impact excitation (EIE) of Ca IV for the first time using the relativistic Breit-Pauli R-Matrix method with a large close coupling wavefunction expansion of 54 fine structure levels…

太阳与恒星天体物理 · 物理学 2023-04-05 Sultana Nahar , Bilal Shafique
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