Kα1,2 x-ray linewidths, asymmetry indices, and [K M] shake probabilities in elements Ca to Ge and comparison with theory for Ca, Ti, and Ge

被引:28
作者
Ito, Y. [1 ]
Tochio, T. [2 ]
Ohashi, H. [3 ]
Yamashita, M. [4 ]
Fukushima, S. [5 ]
Polasik, M. [6 ]
Slabkowska, K. [6 ]
Syrocki, L. [7 ]
Szymanska, E. [6 ]
Rzadkiewicz, J. [8 ]
Indelicato, P. [9 ]
Marques, J. P. [10 ,11 ]
Martins, M. C. [11 ]
Santos, J. P. [11 ]
Parente, F. [10 ,11 ]
机构
[1] Kyoto Univ, ICR, Uji, Kyoto 6110011, Japan
[2] Kobe Univ, Fac Sci, 1-1 Rokkodai, Kobe, Hyogo 6578501, Japan
[3] Accuray Japan KK, Chiyoda Ku, 2-2-1 Ootemachi, Tokyo 1000004, Japan
[4] HIT, Suma Ku, 3-1-12 Yukihira, Kobe, Hyogo 6540037, Japan
[5] NIMS, 1-2-1 Sengen, Tsukuba, Ibaraki 3050047, Japan
[6] Nicolaus Copernicus Univ Torun, Fac Chem, Gagarina 7, PL-87100 Torun, Poland
[7] Nicolaus Copernicus Univ Torun, Fac Phys Astron & Informat, Grudziadzka 5, PL-87100 Torun, Poland
[8] Natl Ctr Nucl Studies, PL-01497 Warsaw, Poland
[9] ENS PSL Res Univ, UPMC Sorbonne Univ, CNRS, Coll France,Lab Kastler Brossel, Case 74,4 Pl Jussieu, F-75005 Paris, France
[10] Univ Lisbon, Fac Ciencias, BioISIBiosyst & Integrat Sci Inst, C8, P-1749016 Lisbon, Portugal
[11] Univ Nova Lisboa, Fac Ciencias & Tecnol, Dept Fis, Lab Instrumentacao Engn Biomed & Fis Radiacao LIB, P-2892516 Monte De Caparica, Caparica, Portugal
关键词
MULTICONFIGURATION-DIRAC-FOCK; IONIZED HEAVY-ATOMS; ELECTRON SELF-ENERGY; STRONG COULOMB FIELD; EMISSION-SPECTRA; TRANSITION ENERGIES; FLUORESCENCE YIELDS; NATURAL WIDTHS; INNER-SHELL; ALPHA;
D O I
10.1103/PhysRevA.94.042506
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We have investigated systematically the K alpha x-ray spectra in elements from Ca to Ge within Berger's twoLorentzian functions model, using a high-resolution antiparallel double-crystal x-ray spectrometer, in order to obtain in detail the physical meaning of the asymmetry in the spectral profiles. The overall tendency of the corrected full width at half maximum of the K alpha(1) and K alpha(2) lines as a function of Z, as well as the linewidths, are in good agreement with the data reported in the literature. It is found, from both the experiments and calculation, that satellite lines arising from shake-off appear between the K alpha(1) and K alpha(2) lines. The asymmetry index of Ka1 in 3d elements from Sc to Zn is ascribed to the existence of a 3d spectator hole. Moreover, the observed Sc Ka1 line shows a symmetric profile unlike the Ti K alpha(1) line profile, this discrepancy being explained by the existence of satellite lines on both sides of the Sc profile. Our experimental results yielded around 25% probability for the probability of shake processes creating a second hole in the 3p or 3d subshells in Sc and around 18% probability for creating a second hole the in the 3p in Ca. For the latter process our calculated value, using multiconfiguration Dirac-Fock wave functions and the sudden approximation yielded a 10% probability.
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页数:11
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