The photoionization of Fe7+ and Fe8+ in the 2p-3d resonance energy region

被引:7
作者
Zeng, JL
Dong, GX
Zhao, G
Yuan, JM
机构
[1] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Chaoyang Dist, Peoples R China
[2] Natl Univ Def Technol, Dept Appl Phys, Changsha 410073, Peoples R China
[3] Natl Nat Sci Fdn China, Dept Math & Phys Sci, Beijing 100085, Peoples R China
关键词
D O I
10.1088/0953-4075/37/12/009
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The photoionization cross sections of the levels belonging to the ground configuration [Ne]3s(2)3p(6)3d of Fe7+ and [Ne]3s(2)3p(6) of Fe8+ have been investigated using the fully relativistic R-matrix method in the 2p-3d excitation region. The detailed resonance structures are described and analysed in some detail with the resonance positions, widths and oscillator strengths being determined. To identify the resonances, the transition energies and oscillator strengths are calculated by the multi-configuration Dirac-Fock method implemented by the GRASP code as well. The cross sections have also been obtained using the non-relativistic R-matrix calculations. The resonances in the relativistic calculation span a much broader energy region than the non-relativistic result. For an iron plasma at a temperature of 20 eV and a density of 0.004 g cm(-3), which is a typical experimental condition recently carried out by Chenais-Popovics et al (2000 Astrophys. J. Suppl. Ser. 127 275), the autoionization widths of the 2p-3d resonances are much larger than the widths caused by the radiative lifetime and electron impact broadening, while the Doppler widths are smaller than but rather close to the autoionization widths.
引用
收藏
页码:2529 / 2542
页数:14
相关论文
共 39 条
[1]  
[Anonymous], THEORY ATOMIC SPECTR
[2]  
[Anonymous], NIST ATOMIC SPECTRA
[3]   SUPER-TRANSITION-ARRAYS - A MODEL FOR THE SPECTRAL-ANALYSIS OF HOT, DENSE-PLASMA [J].
BARSHALOM, A ;
OREG, J ;
GOLDSTEIN, WH ;
SHVARTS, D ;
ZIGLER, A .
PHYSICAL REVIEW A, 1989, 40 (06) :3183-3193
[4]   VARIANCE OF THE DISTRIBUTIONS OF ENERGY-LEVELS AND OF THE TRANSITION ARRAYS IN ATOMIC SPECTRA .3. CASE OF SPIN-ORBIT-SPLIT ARRAYS [J].
BAUCHEARNOULT, C ;
BAUCHE, J ;
KLAPISCH, M .
PHYSICAL REVIEW A, 1985, 31 (04) :2248-2259
[5]   RMATRX1 - BELFAST ATOMIC R-MATRIX CODES [J].
BERRINGTON, KA ;
EISSNER, WB ;
NORRINGTON, PH .
COMPUTER PHYSICS COMMUNICATIONS, 1995, 92 (2-3) :290-420
[6]   ATOMIC DATA FOR OPACITY CALCULATIONS .2. COMPUTATIONAL METHODS [J].
BERRINGTON, KA ;
BURKE, PG ;
BUTLER, K ;
SEATON, MJ ;
STOREY, PJ ;
TAYLOR, KT ;
YAN, Y .
JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 1987, 20 (23) :6379-6397
[7]   Hartree-Fock statistical approach to atoms and photoabsorption in plasmas [J].
Blenski, T ;
Grimaldi, A ;
Perrot, F .
PHYSICAL REVIEW E, 1997, 55 (05) :R4889-R4892
[8]   Multi-wavelength study of the Seyfert 1 galaxy NGC 3783 with XMM-Newton [J].
Blustin, AJ ;
Branduardi-Raymont, G ;
Behar, E ;
Kaastra, JS ;
Kahn, SM ;
Page, MJ ;
Sako, M ;
Steenbrugge, KC .
ASTRONOMY & ASTROPHYSICS, 2002, 392 (02) :453-467
[9]   ELECTRON SCATTERING BY COMPLEX ATOMS [J].
BURKE, PG ;
HIBBERT, A ;
ROBB, WD .
JOURNAL OF PHYSICS PART B ATOMIC AND MOLECULAR PHYSICS, 1971, 4 (02) :153-&
[10]   Photoabsorption in dense plasmas [J].
Blenski, T .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2000, 127 (02) :239-244