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相关论文: Large-scale Breit-Pauli R-matrix calculations for …

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An extensive set of dipole-allowed, intercombination, and forbidden transition probabilities for Fe V is presented. The Breit-Pauli R-matrix (BPRM) method is used to calculate 1.46 x 10^6 oscillator strengths for the allowed and…

天体物理学 · 物理学 2009-10-31 Sultana N. Nahar , Franck Delahaye , Anil K. Pradhan , C. J. Zeippen

The Breit-Pauli R-matrix method developed under the Iron Project has been used to obtain extensive sets of oscillator strengths and transition probabilities for dipole allowed and intercombination fine structure transitions in carbon like…

天体物理学 · 物理学 2009-10-31 Sultana N. Nahar

Ab initio calculations including relativistic effects employing the Breit-Pauli R-matrix (BPRM) method are reported for fine structure energy levels and oscillator strengths upto n = 10 and 0.leq. l .leq.9 for 15 Li-like ions: C IV, N V, O…

天体物理学 · 物理学 2009-11-07 Sultana N. Nahar

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

An extensive set of fine structure levels and corresponding transition probabilities for allowed and forbidden transitions in Fe XVII is presented. A total of 490 bound energy levels of Fe XVII of total angular momenta 0 <= J <= 7 of even…

天体物理学 · 物理学 2011-05-23 Sultana N. Nahar , Werner Eissner , Guo-Xin Chen , Anil K. Pradhan

Improved collisions strengths for the mid-infrared and optical transitions in Ne V are presented. Breit-Pauli R-Matrix calculations for electron impact excitation are carried out with fully resolved near-threshold resonances at very low…

原子物理 · 物理学 2015-06-15 Michael Dance , Ethan Palay , Sultana N. Nahar , Anil K. Pradhan

We have performed large-scale configuration interaction (CI) calculations using CIV3for the lowest (in energy) 155 fine-structure levels of aluminum-like germanium ion. We have calculated the energy levels, lifetimes, oscillator strengths,…

原子物理 · 物理学 2015-08-17 Waleed Othman Younis , Alan Hibbert

We present new calculations for transition probabilities of Fe IV, with much more extensive datasets than heretofore available. The large-scale close coupling R-matrix calculations yield 1,798 LS bound states with n $\leq$ 11 and $l \leq$…

天体物理学 · 物理学 2015-06-24 Sultana N. Nahar , Anil K. Pradhan

Effective collision strengths for forbidden transitions among the 5 energetically lowest finestructure levels of O II are calculated in the Breit-Pauli approximation using the R-matrix method. Results are presented for the electron…

天体物理仪器与方法 · 物理学 2015-05-13 R. Kisielius , P. J. Storey , G. J. Ferland , F. P. Keenan

A comprehensive study of high-accuracy photoionization cross sections is carried out using the relativistic Breit-Pauli R-matrix (BPRM) method for (hnu + Fe XVII --> Fe XVIII + e). Owing to its importance in high-temperature plasmas the…

太阳与恒星天体物理 · 物理学 2015-05-27 Sultana N. Nahar , Anil K. Pradhan , Guo-Xin Chen , Werner Eissner

Aimed at ionization balance and spectral analysis of UV and X-ray sources, we present self-consistent sets of photoionization cross sections, recombination cross sections, and rate coefficients for Li-like O VI and He-like O VII.…

天体物理学 · 物理学 2009-11-07 Sultana N. Nahar , Anil K. Pradhan

Photoionization cross sections and recombination rate coefficients are presented for the L-shell ground state fine structure levels $2s^22p^4 \ ^3P_{2,0,1}$ of Fe~XIX. Several sets of calculations including relativistic effects are carried…

天体物理学 · 物理学 2009-10-31 Hong Lin Zhang , Anil K. Pradhan

To investigate the completeness of coupled channel (CC) Breit-Pauli R-Matrix (BPRM) calculations for opacities, we employ the relativistic distorted wave (RDW) method to complement (``top-up'') and compare the BPRM photoionization cross…

太阳与恒星天体物理 · 物理学 2023-08-30 L. Zhao , S. N. Nahar , W. Eissner , A. K. Pradhan

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

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

Relativistic and channel coupling effects in photoionization and unified electronic recombination of Fe XVII are demonstrated with an extensive 60-level close coupling calculation using the Breit-Pauli R-matrix method. Photoionization and…

天体物理学 · 物理学 2009-11-06 Hong Lin Zhang , Sultana N. Nahar , Anil K. Pradhan

Photoionization and recombination cross sections and rate coefficients are calculated for Li-like Fe XXIV and He-like Fe XXV using the Breit-Pauli R-matrix (BPRM) method. A complete set of total and level-specific parameters is obtained to…

天体物理学 · 物理学 2009-10-31 Sultana N. Nahar , Anil K. Pradhan , Hong Lin Zhang

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

Extensive resonance structures are manifest in R-Matrix (RM) calculations. However, there exist a large number of highly excited electronic configurations that may contribute to background non-resonant bound-free opacity in high-temperature…

太阳与恒星天体物理 · 物理学 2018-01-09 Lianshui Zhao , Werner Eissner , Sultana N. Nahar , Anil K. Pradhan

The primary X-ray diagnostic lines in He-like ions are mainly excited by electron impact from the ground level to the n = 2 levels, but at high temperatures n > 2 levels are also excited. In order to describe the atomic processes more…

天体物理学 · 物理学 2009-11-07 Franck Delahaye , Anil K. Pradhan
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