Radiative and Auger transitions of K-shell excited resonance states in boron-like sulfur ion

Sun Yan; Hu Feng; Sang Cui-Cui; Mei Mao-Fei; Liu Dong-Dong; Gou Bing-Cong

doi:10.7498/aps.68.20190481

Abstract

Non-relativistic energy values and wave functions of the K-shell excited resonance states 1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L (L = S, P, D) in boron-like sulfur ion are calculated in the frame of multi-configuration saddle-point variation method. The electron correlation effects are considered by the expansion of configuration wave function. The wave functions are constructed and optimized by the orbital-spin angular momentum partial waves selected based on the rule of configuration interaction. To saturate the wave functional space and to improve the non-relativistic energy, the restricted variational method is used to calculate the restricted variational energy. Then, the mass polarization effect and relativistic correction are calculated by the perturbation theory. The quantum electrodynamics (QED) effect and higher-order relativistic correction are considered by the screened hydrogenic formula. Furthermore, the energy shift originating from the interaction between closed channel and open channel is also calculated. Finally, the accurate relativistic energy levels for these resonance states are obtained by adding the non-relativistic energy and all corrections.Using the optimized wave functions, the line strengths, oscillator strengths, radiative transition rates and transition wavelengths of electric-dipole transitions for the K-shell excited resonance states in boron-like sulfur ion are systematically calculated. In this work, the oscillator strengths and transition rates are given in the length, velocity, and acceleration gauges. The good agreement among the three gauges reflects that the calculated wave functions are reasonably accurate. The calculated radiative transition rates and transition wavelengths are compared with other theoretical data. Good agreement is obtained except the transition: 1s2s(³S)2p³ ²P^o→1s2²s2p^{2 2}D. The deviation between our theoretical result and the MCDF theoretical value is about 46%, which needs further verifying. The Auger rates, Auger branching ratios, and Auger electron energy values of the important decay channels of the K-shell excited states are calculated by the saddle-point complex-rotation method. The calculated Auger rates and Auger electron energy values are also in good agreement with the corresponding reference data. For some K-shell states, the related energy levels and Auger branching ratios are reported for the first time. The present calculations results will provide valuable theoretical data for the calibration of spectral lines and Auger electron spectra in the relevant experiments.

Keywords:

Authors and contacts

1.
School of Mathematic and Physical Science, Xuzhou University of Technology, Xuzhou 221018, China
2.
College of Science, Lanzhou University of Technology, Lanzhou 730050, China
3.
School of Physics, Beijing institute of Technology, Beijing 100081, China

Corresponding author: Sun Yan, suenyangu@163.com

Funds: Project supported by the National Natural Science Foundation of China (Grant Nos. 11604284, 51506184), the Natural Science Foundation of the Jiangsu Higher Education Institutions of China (Grant No. 17KJB140025), and Sun Yan is supported by the Qinlan Project of Jiangsu Province, China.

FullText HTML : translate this paragraph

References

[1]	Altun Z, Yumak A, Badnell N R, Colgan J, Pindzol M S 2004 A&A 420 775
[2]	Rohringer N, Ryan D, London R A, Purvis M, Albert F, Dunn J, Bozek J D, Bostedt C, Graf A, Hill R, Hau-Riege S P, Rocca J J 2012 Nature 481 488 Google Scholar
[3]	Martin A, Nicolas G, Jacques S 2006 Nucl. Phys. A 777 1
[4]	冯雷, 蒋刚 2017 物理学报 66 153201 Google Scholar Feng L, Jiang G 2017 Acta Phys. Sin. 66 153201 Google Scholar
[5]	Rødbro M, Bruch R, Bisgaard P 1979 J. Phys. B: At. Mol. Opt. Phys. 12 2413 Google Scholar
[6]	Schneider D, Bruch R, Butscher W, Schwarz W H E 1981 Phys. Rev. A 24 1223 Google Scholar
[7]	Bruch R, Schneider D, Schwarz W H E, Meinhart M, Johnson B M, Taulbjerg K 1979 Phys. Rev. A 19 587 Google Scholar
[8]	Itoh A, Schneider D, Schneider T, Zouros T J M, Nolte G, Schiwietz G, Zeitz W, Stolterfoht N 1985 Phys. Rev. A 31 684 Google Scholar
[9]	Kádár I, Ricz S, Végh J, Sulik B, Varga D, Berényi D 1990 Phys. Rev. A 41 3518 Google Scholar
[10]	Armour I A, Fawcett B C, Silver J D, Trabert E 1980 J. Phys. B: Atom. Molec. Phys. 13 2701 Google Scholar
[11]	Trabertt E, Fawcett B C 1979 J. Phys. B: Atom. Molec. Phys. 12 L441
[12]	Faenov A Y 1994 Phys. Scr. 49 41 Google Scholar
[13]	Schlachter A S, Sant’Anna M M, Covington A M, Aguilar A, Gharaibeh M F, Emmons E D, Scully S W J, Phaneuf R A, Hinojosa G, Álvarez I, Cisneros C, Müller A, McLaughlin B M 2004 J. Phys. B: At. Mol. Opt. Phys. 37 L103 Google Scholar
[14]	Gharaibeh M F, Hassan N E I, Shorman M M A L, Bizau J M, Cubaynes D, Guilbaud S, Sakho I, Blancard C, McLaughlin B M 2014 J. Phys. B: At. Mol. Opt. Phys. 47 065201 Google Scholar
[15]	Müller A, Borovik A, Buhr T, Hellhund J, Holste K, Kilcoyne A L D, Klumpp S, Martins M, Ricz S, Viefhaus J, Schippers S 2018 Phys. Rev. A 97 013409 Google Scholar
[16]	Müller A, Borovik A, Buhr J T, Hellhund J, Holste K, Kilcoyne A L D, Klumpp S, Martins M, Ricz S, Viefhaus J, Schippers S 2015 Phys. Rev. Lett. 114 013002 Google Scholar
[17]	Chen M H, Crasemann B 1988 At. Data Nucl. Data Tables 38 381 Google Scholar
[18]	Chen M H, Crasemann B 1987 Phys. Rev. A 35 4579 Google Scholar
[19]	Safronova U I, Shlyaptseva A S 1996 Phys. Scr. 54 254 Google Scholar
[20]	Zhou F Y, Ma Y L, Qu Y Z 2016 Phys. Rev. A 93 060501 Google Scholar
[21]	Sakho I, Sow M, Wagué A 2015 Phys. Scr. 90 045401 Google Scholar
[22]	Sun Y, Chen F, Gou B C 2011 J. Chem. Phys. 135 124309 Google Scholar
[23]	Sun Y, Gou B C, Chen C 2013 Phys. Rev. A 87 032509 Google Scholar
[24]	Chung K T 1979 Phys. Rev. A 20 1743 Google Scholar
[25]	Lin B, Berry H G, Shibata T, Livingston A E, Garnir H P, Bastin T, Désesquelles J, Savukov I 2003 J. Phys. B: At. Mol. Opt. Phys. 67 062507 Google Scholar
[26]	Drake G W F 1982 Adv. At. Mol. Phys. 18 399 Google Scholar
[27]	Chung K T, Zhu X W, Wang Z W 1993 Phys. Rev. A 47 1740 Google Scholar
[28]	Drake G W F, Swainson R A 1990 Phys. Rev. A 41 1243 Google Scholar
[29]	Chung K T, Davis B F 1982 Phys. Rev. A 26 3278 Google Scholar
[30]	Davis B F, Chung K T 1984 Phys. Rev. A 29 1878 Google Scholar
[31]	Kramida A, Ralchenko Yu, Reader J, NIST ASD Team 2018 NIST Atomic Spectra Database (ver. 5.6.1) [Online]. Available: https://physics.nist.gov/asd [2019, March 28]. National Institute of Standards and Technology, Gaithersburg, MD. DOI: https://doi.org/10.18434/T4W30F

Cited By

图 1 本文计算的电偶极跃迁振子强度的长度规范值分别与速度规范值及加速度规范值的对比

Figure 1. Comparison diagram of the calculated electrical dipole transition oscillator strength values in length gauge with the velocity gauge and acceleration gauge.

DownLoad: Full-Size Img PowerPoint

图 2 本文计算的长度规范的电偶极辐射跃迁率与MCDF理论计算的跃迁率的对比

Figure 2. Comparison diagram of calculated radiative transition rates in length gauge with the theoretical data from MCDF calculations.

DownLoad: Full-Size Img PowerPoint

表 1 类硼S离子K壳层激发共振态1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L (L = S, P, D)的权重中心能级(单位a.u.), 能量转化关系:1 a.u = 27.21138 eV

Table 1. Center of gravity levels of 1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L (L = S, P, D) of K-shell excited resonance states in boron-like sulfur ion (unit: a.u.). The energy conversion relationship: 1 a.u = 27.21138 eV.

共振态	${E_{{\rm{nonrel}}}}/{\rm{a.u.}}$			${E_{{\rm{total}}}}/{\rm{a.u.}}$	$ - {E_{{\rm{total}}}}/{\rm{eV}}$
共振态	${E_{\rm{b}}} + \Delta {E_{{\rm{RV}}}}$	$\Delta {E_{{\rm{corr}}}}$	$\Delta {E_{\rm{S}}}$	${E_{{\rm{total}}}}/{\rm{a.u.}}$	本文	SCUNC[21]
1s2s²2p^{2 4}P	–229.35389	–0.64011	–0.00245	–229.99645	6258.52
1s2s²2p^{2 2}S	–228.66774	–0.66777	–0.00174	–229.33725	6240.58
1s2s²2p^{2 2}P	–228.81110	–0.66633	–0.00089	–229.47832	6244.42
1s2s²2p^{2 2}D	–228.91613	–0.67942	0.00322	–229.59233	6247.52
1s2s(³S)2p^{3 4}S^o	–227.40768	–0.60823	0.00018	–228.01573	6204.62
1s2s(¹S)2p^{3 4}S^o	–228.21123	–0.62298	0.00151	–228.83270	6226.85
1s2s(³S)2p^{3 4}P^o	–228.00558	–0.62215	0.00106	–228.62667	6221.25
1s2s(³S)2p^{3 4}D^o	–228.30315	–0.62288	–0.00017	–228.92620	6229.40
1s2s(³S)2p^{3 2}S^o	–226.86291	–0.62586	0.00070	–227.48807	6190.26
1s2s(³S)2p^{3 2}P^o	–226.91669	–0.61114	0.00193	–227.52590	6191.29
1s2s(¹S)2p^{3 2}P^o	–227.28245	–0.61646	0.00620	–227.89271	6201.28
1s2s(³S)2p^{3 2}D^o	–227.21472	–0.61330	0.00204	–227.82598	6199.46
1s2s(¹S)2p^{3 2}D^o	–227.56290	–0.62041	0.00280	–228.18051	6209.11
1s2p^{4 4}P	–226.53817	–0.55727	–0.00249	–227.09793	6179.65	6173.07
1s2p^{4 2}S	–225.47488	–0.56220	0.00072	–226.03636	6150.76	6145.67
1s2p^{4 2}P	–225.94003	–0.56493	0.00251	–226.50245	6163.44	6159.02
1s2p^{4 2}D	–226.07283	–0.56074	0.00279	–226.63078	6166.94	6163.51

DownLoad: CSV

表 2 S¹¹⁺离子K壳层激发共振态, S¹¹⁺, S¹²⁺离子低位激发态的精细结构能级($ - E$, 单位eV)

Table 2. Fine-structure energy levels of the K-shell excited resonance states in S¹¹⁺ ion, and low-excited states in S¹¹⁺, S¹²⁺ ion ($ - E$, unit eV).

偶宇称			奇宇称
S¹¹⁺离子K壳层激发态共振态
共振态	本文	文献[19]	共振态	本文	文献[19]
1s2s²2p^{2 4}P_1/2	6259.50	6265.62	1s2s(³S)2p^{3 4}S_3/2	6204.62	6207.16
1s2s²2p^{2 4}P_3/2	6258.83	6264.85	1s2s(¹S)2p^{3 4}S_3/2	6226.85	6229.68
1s2s²2p^{2 4}P_5/2	6257.99	6264.05	1s2s(³S)2p^{3 4}P_1/2	6221.05	6223.62
1s2s²2p^{2 2}S_1/2	6240.58	6243.03	1s2s(³S)2p^{3 4}P_3/2	6221.24	6223.52
1s2s²2p^{2 2}P_1/2	6245.72	6248.94	1s2s(³S)2p^{3 4}P_5/2	6221.32	6223.54
1s2s²2p^{2 2}P_3/2	6243.77	6247.23	1s2s(³S)2p^{3 4}D_1/2	6229.21	6231.96
1s2s²2p^{2 2}D_3/2	6247.38	6251.29	1s2s(³S)2p^{3 4}D_3/2	6229.21	6232.01
1s2s²2p^{2 2}D_5/2	6247.62	6251.38	1s2s(³S)2p^{3 4}D_5/2	6229.30	6232.00
1s2p^{4 4}P_1/2	6178.53	6180.77	1s2s(³S)2p^{3 4}D_7/2	6229.61	6231.85
1s2p^{4 4}P_3/2	6179.12	6181.26	1s2s(³S)2p^{3 2}S_1/2	6190.26	6192.27
1s2p^{4 4}P_5/2	6180.37	6182.44	1s2s(³S)2p^{3 2}P_1/2	6191.17	6193.98
1s2p^{4 2}S_1/2	6150.76	6152.75	1s2s(³S)2p^{3 2}P_3/2	6191.36	6193.65
1s2p^{4 2}P_1/2	6163.28	6165.34	1s2s(¹S)2p^{3 2}P_1/2	6201.72	6204.18
1s2p^{4 2}P_3/2	6163.52	6166.42	1s2s(¹S)2p^{3 2}P_3/2	6201.05	6206.82
1s2p^{4 2}D_3/2	6166.83	6169.56	1s2s(³S)2p^{3 2}D_3/2	6199.29	6199.03
1s2p^{4 2}D_5/2	6167.00	6169.69	1s2s(³S)2p^{3 2}D_5/2	6199.57	6202.14
			1s2s(¹S)2p^{3 2}D_3/2	6209.23	6212.93
			1s2s(¹S)2p^{3 2}D_5/2	6209.03	6212.33
S¹¹⁺离子低位激发态
激发态	本文	NIST[31]	激发态	本文	NIST[31]
1s²2s2p^{2 4}P_1/2	8617.38	8617.29	1s²2s²2p ²P_1/2	8641.58	8641.33
1s²2s2p^{2 4}P_3/2	8616.83	8616.70	1s²2s²2p ²P_3/2	8639.78	8639.70
1s²2s2p^{2 4}P_5/2	8615.98	8615.86	1s²2p^{3 4}S_3/2	8565.71	8565.69
1s²2s2p^{2 2}S_1/2	8586.78	8586.83	1s²2p^{3 2}P_1/2	8545.44	8545.36
1s²2s2p^{2 2}P_1/2	8584.06	8583.71	1s²2p^{3 2}P_3/2	8545.42	8545.14
1s²2s2p^{2 2}P_3/2	8582.99	8582.88	1s²2p^{3 2}D_3/2	8555.97	8555.79
1s²2s2p^{2 2}D_3/2	8598.49	8598.35	1s²2p^{3 2}D_5/2	8555.74	8555.72
1s²2s2p^{2 2}D_5/2	8598.39	8598.31
S¹²⁺离子低位激发态
激发态	本文	NIST[31]	激发态	本文	NIST[31]
1s²2s^{2 1}S₀	8076.99	8076.93	1s²2s2p ¹P₁	8028.74	8028.63
1s²2p^{2 1}S₀	7987.61	7987.44	1s²2s2p ³P₀	8052.36	8052.23
1s²2p^{2 1}D₂	8004.12	8003.85	1s²2s2p ³P₁	8051.81	8051.70
1s²2p^{2 3}P₀	8012.11	8012.06	1s²2s2p ³P₂	8050.64	8050.50
1s²2p^{2 3}P₁	8011.53	8011.37
1s²2p^{2 3}P₂	8010.43	8010.37

DownLoad: CSV

表 3 类硼S离子的K壳层激发共振态1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L(L = S, P, D)的电偶极辐射跃迁线强度S (a.u.)、辐射跃迁率${A_{ik}}$(s^–1) (长度规范${A_{\rm{l}}}$, 速度规范${A_{\rm{v}}}$, 加速度规范${A_{\rm{a}}}$), 跃迁振子强度${f_{ki}}$(长度规范${f_{\rm{l}}}$, 速度规范${f_{\rm{v}}}$, 加速度规范${f_{\rm{a}}}$), 和跃迁波长$\lambda $(Å), 方括号的数代表10的幂次方

Table 3. Line strengths S (a.u.), radiative transition probabilities ${A_{ik}}$ (length gauge ${A_{\rm{l}}}$, velocity gauge${A_{\rm{v}}}$, acceleration gauge ${A_{\rm{a}}}$) (s^–1), transition oscillator strengths ${f_{ki}}$ (length gauge ${f_{\rm{l}}}$, velocity gauge ${f_{\rm{v}}}$, and acceleration gauge ${f_{\rm{a}}}$), and transition wavelengths $\lambda $ (Å) of electric dipole transitions of the K-shell excited resonance states 1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L (L = S, P, D) in boron-like sulfur ion. The numbers in square brackets represent the power of 10.

初态	末态	S/a.u.	${A_{ik}}/{\rm{s}}^{-1}$				${f_{ki}}$			λ/Å
初态	末态	S/a.u.	${A_{\rm{l}}}$	${A_{\rm{v}}}$	${A_{\rm{a}}}$	文献[17]	${f_{\rm{l}}}$	${f_{\rm{v}}}$	${f_{\rm{a}}}$	本文	文献[17]	文献[21]
1s2s²2p^{2 4}P	1s²2p^{3 4}S^o	5.06[–4]	5.48[11]	5.32[11]	5.31[11]	5.09[11]	7.14[–3]	6.94[–3]	6.92[–3]	5.374	5.379
1s2p^{4 4}P	1s²2p^{3 4}S^o	2.14[–2]	2.55[13]	2.65[13]	2.67[13]	2.57[13]	3.12[–1]	3.23 [–1]	3.26[–1]	5.196	5.193	5.203
1s2s²2p^{2 2}S	1s²2s²2p ²P^o	3.81[–3]	2.78[13]	2.82[13]	2.80[13]	2.93[13]	3.72[–2]	3.78[–2]	3.76[–2]	5.166	5.176	5.167
	1s²2p^{3 2}P^o	1.78[–4]	1.15[12]	1.15[12]	1.02[12]	9.87[11]	1.68[–3]	1.67[–3]	1.48[–3]	5.379	5.383
1s2s²2p^{2 2}P	1s²2s²2p ²P^o	3.26[–2]	7.88[13]	7.87[13]	7.84[13]	7.53[13]	3.18[–1]	3.18[–1]	3.17[–1]	5.175	5.176
	1s²2p^{3 2}P^o	1.80[–4]	3.87[11]	3.88[11]	3.99[12]	3.20[11]	1.69[–3]	1.69[–3]	1.74[–3]	5.388	5.392
	1s²2p^{3 2}D^o	6.30[–4]	1.37[12]	1.39[12]	1.40[12]	1.23[12]	3.56[–3]	3.61[–3]	3.64[–3]	5.364	5.368
1s2s²2p^{2 2}D	1s²2s²2p²P^o	1.92[–2]	2.77[13]	2.67[13]	2.64[13]	2.71[13]	1.87[–1]	1.80[–1]	1.78[–1]	5.181	5.183
	1s²2p^{3 2}P^o	1.01[–4]	1.29[11]	1.28[11]	1.45[11]	1.35[11]	9.43[–4]	9.34[–4]	1.06[–3]	5.396	5.401
	1s²2p^{3 2}D^o	3.68[–4]	7.98[11]	8.18[11]	8.25[11]	7.74[11]	3.46[–3]	3.55[–3]	3.59[–3]	5.371	5.375
1s2p^{4 2}S	1s²2p^{3 2}P^o	7.14[–3]	5.17[13]	5.26[13]	5.28[13]	5.13[13]	6.96[–2]	7.08[–2]	7.11[–2]	5.178	5.175	5.191
1s2p^{4 2}P	1s²2p^{3 2}P^o	1.75[–2]	4.17[13]	4.26[13]	4.26[13]	3.97[13]	1.70[–1]	1.74[–1]	1.73[–1]	5.205	5.205	5.217
	1s²2p^{3 2}D^o	2.89[–2]	6.97[13]	6.80[13]	6.71[13]	6.17[13]	1.69[–1]	1.65[–1]	1.63[–1]	5.182	5.182	5.191
1s2p^{4 2}D	1s²2s²2p²P^o	2.58[–4]	4.09[11]	4.42[11]	4.14[11]		2.59[–3]	2.80[–3]	2.62[–3]	5.013
	1s²2p^{3 2}P^o	9.20[–3]	1.30[13]	1.32[13]	1.33[13]	1.32[13]	8.91[–2]	9.04[–2]	9.11[–2]	5.213	5.212	5.220
	1s²2p^{3 2}D^o	2.74[–2]	3.93[13]	4.10[13]	4.13[13]	4.02[13]	1.60[–1]	1.67[–1]	1.68[–1]	5.190	5.189	5.198
1s2s(¹S)2p^{3 4}S^o	1s²2s2p^{2 4}P	3.08[–2]	1.11[14]	1.09[14]	1.09[14]	1.09[14]	1.50[–1]	1.48[–1]	1.47[–1]	5.188	5.189
1s2s(³S)2p^{3 4}S^o	1s²2s2p^{2 4}P	7.57[–4]	2.80[12]	2.90[12]	2.99[12]	2.28[12]	3.72[–3]	3.85[–3]	3.97[–3]	5.141	5.135
1s2s(³S)2p^{3 4}P^o	1s²2s2p^{2 4}P	2.33[–2]	2.81[13]	2.79[13]	2.80[13]	2.67[13]	1.14[–1]	1.13[–1]	1.13 [–1]	5.176	5.174
1s2s(³S)2p^{3 4}D^o	1s²2s2p^{2 4}P	3.89[–2]	2.79[13]	2.78[13]	2.77[13]	2.63[13]	1.89[–1]	1.88[–1]	1.88[–1]	5.194	5.192
1s2s(³S)2p^{3 2}S^o	1s²2s2p^{2 2}P	1.57[–2]	1.13[14]	1.13[14]	1.13[14]	8.54[13]	1.53[–1]	1.52[–1]	1.52[–1]	5.181	5.180
1s2s(¹S)2p^{3 2}P^o	1s²2s2p^{2 2}P	1.05[–3]	2.50[12]	2.78[12]	2.74[12]	2.53[12]	1.02[–2]	1.13[–2]	1.12[–2]	5.205	5.208
	1s²2s2p^{2 2}D	1.71[–2]	4.14[13]	4.17[13]	4.14[13]	3.92[13]	1.00[–1]	1.01[–1]	1.00[–1]	5.172	5.173
1s2s(³S)2p^{3 2}P^o	1s²2s2p^{2 2}S	1.59[–3]	3.85[12]	3.93[12]	3.50[12]	3.55[12]	4.66[–2]	4.76[–2]	4.24[–2]	5.176	5.174
	1s²2s2p^{2 2}P	1.00[–2]	2.42[13]	2.42[13]	2.30[13]	3.01[13]	9.79[–2]	9.79[–2]	9.31[–2]	5.183	5.183
	1s²2s2p^{2 2}D	2.01[–3]	4.95[12]	4.92[12]	5.19[12]	3.38[12]	1.18[–2]	1.19[–2]	1.25[–2]	5.151	5.149
1s2s(¹S)2p^{3 2}D^o	1s²2s2p^{2 2}P	1.85[–3]	2.60[12]	2.64[12]	2.64[12]	2.19[12]	1.79[–2]	1.81[–2]	1.81[–2]	5.222	5.225
	1s²2s2p^{2 2}D	5.21[–2]	7.49[13]	7.54[13]	7.55[13]	7.13[13]	3.04[–1]	3.06[–1]	3.07[–1]	5.189	5.191
1s2s(³S)2p^{3 2}D^o	1s²2s2p^{2 2}P	1.70[–2]	2.43[13]	2.49[13]	2.50[13]	2.40[13]	1.65[–1]	1.69[–1]	1.70[–1]	5.201	5.201
	1s²2s2p^{2 2}D	5.16[–3]	7.51[12]	7.72[12]	7.83[12]	7.84[12]	3.02[–2]	3.11[–2]	3.15[–2]	5.168	5.166

DownLoad: CSV

表 4 类硼S离子K壳层激发态1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L(L = S, P, D)的俄歇跃迁率(s^–1) 和俄歇分支率(BR), 方括号的数表示10的幂次方

Table 4. The Auger rates (s^–1) and branching ratios (BR) of the K-shell excited resonance states 1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L (L=S, P, D) in boron-like sulfur ion. The numbers in square brackets represent the power of 10.

俄歇跃迁通道		俄歇跃迁率/s^–1		BR/%	俄歇跃迁通道		俄歇跃迁率/s^–1		BR(%)
俄歇跃迁通道		本文	文献[17]	BR/%	俄歇跃迁通道		本文	文献[17]	BR(%)
1s2s²2p²	²S →1s²2s^{2 1}S	5.05[13]	8.33[13]	23.3	1s2s(¹S)2p³	²P^o→1s²2s^{2 1}S	6.63[11]	2.33[11]	0.3
	²S →1s²2s2p ¹P^o	6.35[13]	6.02[13]	29.3		²P^o→1s²2s2p ¹P^o	1.18[12]	1.46[13]	0.5
	²S →1s²2s2p ³P^o	1.61[13]	2.06[13]	7.4		²P^o→1s²2s2p ³P^o	1.29[14]	1.22[14]	59.6
	²S →1s²2p^{2 1}S	7.10[13]	7.85[13]	32.8		²P^o→1s²2p^{2 1}S	6.50[12]	5.20[12]	3.0
	²S →1s²2p^{2 1}D	1.53[13]	1.48[13]	7.1		²P^o→1s²2p^{2 1}D	5.25[12]	9.54[12]	2.4
	²P→1s²2s2p ¹P^o	1.82[13]	2.55[13]	14.7		²P^o→1s²2p^{2 3}P	7.40[13]	7.54[13]	34.2
	²P→1s²2s2p ³P^o	1.05[13]	7.34[12]	8.5		²D^o→1s²2s2p ¹P^o	7.30[12]	8.82[12]	2.8
	²P→1s²2p^{2 1}D₂	1.97[10]	7.42[12]	0		²D^o→1s²2s2p ³P^o	1.74[14]	1.74[14]	66.1
	²P→1s²2p^{2 3}P	9.50[13]	8.68[13]	76.8		²D^o→1s²2p^{2 1}D	9.55[12]	1.40[13]	3.6
	²D→1s²2s^{2 1}S	1.24[14]	1.14[14]	40.3		²D^o→1s²2p^{2 3}P	7.25[13]	7.66[13]	27.5
	²D→1s²2s2p ¹P^o	6.80[13]	6.42[13]	22.1		⁴S^o→1s²2p^{2 3}P	3.85[13]	3.88[13]	100
	²D→1s²2s2p ³P^o	1.72[13]	2.26[13]	5.6	1s2s(³S)2p³	²S^o→1s²2p^{2 3}P	6.55[13]	4.35[13]	100
	²D→1s²2p^{2 1}S	3.43[12]	2.82[12]	1.1		²P^o→1s²2s^{2 1}S	4.33[12]	2.67[12]	1.6
	²D→1s²2p^{2 1}D	9.15[13]	9.22[13]	29.8		²P^o→1s²2s2p ¹P^o	1.28[14]	1.18[14]	46.9
	²D→1s²2p^{2 3}P	3.37[12]	4.47[12]	1.1		²P^o→1s²2s2p ³P^o	5.40[12]	7.38[12]	2.0
	⁴P→1s²2s2p ³P^o	1.10[14]	1.18[14]	54.3		²P^o→1s²2p^{2 1}S	4.54[13]	4.68[13]	16.6
	⁴P→1s²2p^{2 3}P	9.25[13]	9.48[13]	45.7		²P^o→1s²2p^{2 1}D	6.40[13]	6.23[13]	23.4
1s2p⁴	²S →1s²2s^{2 1}S	2.75[12]	3.04[11]	0.6		²P^o→1s²2p^{2 3}P	2.58[13]	3.47[13]	9.5
	²S →1s²2s2p ¹P^o	4.15[12]	4.73[12]	1.0		²D^o→1s²2s2p ¹P^o	1.76[14]	1.71[14]	54.5
	²S →1s²2s2p ³P^o	8.57[11]	1.48[12]	0.2		²D^o→1s²2s2p ³P^o	6.85[12]	1.16[13]	2.1
	²S →1s²2p^{2 1}S	2.43[14]	3.66[13]	56.3		²D^o→1s²2p^{2 1}D	1.18[14]	1.19[14]	36.5
	²S →1s²2p^{2 1}D	1.81[14]	1.87[14]	41.9		²D^o→1s²2p^{2 3}P	2.22[13]	1.99[13]	6.9
	²P→1s²2s2p ¹P^o	2.73[11]	5.19[11]	0.1		⁴S^o →1s²2p^{2 3}P	1.92[14]	2.02[14]	100
	²P→1s²2s2p ³P^o	2.38[11]	1.86[11]	0.1		⁴P^o→1s²2s2p³P^o	1.35[14]	1.38[14]	88.9
	²P→1s²2p^{2 1}D₂	6.95[10]	2.06[13]	0		⁴P^o→1s²2p^{2 3}P	1.68[13]	1.45[13]	11.1
	²P→1s²2p^{2 3}P	2.15[14]	1.90[14]	99.8		⁴D^o→1s²2s2p³P^o	1.84[14]	1.84[14]	90.4
	²D→1s²2s^{2 1}S	2.95[12]	7.35[9]	1.0		⁴D^o→1s²2p^{2 3}P	1.96[13]	1.41[13]	9.6
	²D→1s²2s2p ¹P^o	1.35[12]	1.38[12]	0.5
	²D→1s²2s2p ³P^o	2.73[11]	4.54[11]	0.1
	²D→1s²2p^{2 1}S	1.25[13]	4.09[13]	4.2
	²D→1s²2p^{2 1}D	2.68[14]	2.74[14]	90.6
	²D→1s²2p^{2 3}P	1.05[13]	1.26[13]	3.6
	⁴P→1s²2s2p ³P^o	1.96[12]	2.50[12]	0.9
	⁴P→1s²2p^{2 3}P	2.08[14]	2.09[14]	99.1

DownLoad: CSV

表 5 类硼S离子K壳层激发态1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L(L = S, P, D)的俄歇电子能量(单位: eV)

Table 5. The Auger electron energies of the K-shell excited resonance states 1s2s²2p², 1s2s2p³, 1s2p^{4 2, 4}L (L = S, P, D) in boron-like sulfur ion (unit: eV).

跃迁通道		本文	文献[17]	跃迁通道		本文	文献[17]
1s2s²2p^{2 2}S_1/2	1s²2s^{2 1}S₀	1836.41	1837.80	1s2s(³S)2p^{3 2}S_1/2	1s²2p^{2 3}P₀	1821.85	1825.18
	1s²2s2p ¹P₁	1788.16	1787.75		1s²2p^{2 3}P₁	1821.27	1824.50
	1s²2s2p ³P₀	1811.78	1812.97		1s²2p^{2 3}P₂	1820.17	1823.49
	1s²2s2p ³P₁	1811.23	1812.44	1s2s(³S)2p^{3 2}P_1/2	1s²2s^{2 1}S₀	1885.82	1888.35
	1s²2s2p ³P₂	1810.06	1811.23		1s²2s2p ¹P₀	1837.57	1838.30
	1s²2p^{2 1}S₀	1747.03	1746.35		1s²2s2p ³P₁	1861.19	1863.52
	1s²2p^{2 1}D₂	1763.54	1763.33		1s²2s2p ³P₂	1860.64	1862.99
1s2s²2p^{2 2}P_1/2	1s²2s2p ¹P₁	1783.02	1782.25		1s²2s2p ³P₃	1859.47	1861.78
	1s²2s2p ³P₀	1806.64	1807.47		1s²2p^{2 1}S₀	1796.44	1796.90
	1s²2s2p ³P₁	1806.09	1806.94		1s²2p^{2 1}D₂	1812.95	1813.88
	1s²2s2p ³P₂	1804.92	1805.74		1s²2p^{2 3}P₀	1820.94	1823.09
	1s²2p^{2 1}D₂	1758.40	1757.84		1s²2p^{2 3}P₁	1820.36	1822.41
	1s²2p^{2 3}P₀	1766.39	1767.05		1s²2p^{2 3}P₂	1819.26	1821.40
	1s²2p^{2 3}P₁	1765.81	1766.37	1s2s(³S)2p^{3 2}P_3/2	1s²2s^{2 1}S₀	1885.63	1888.87
	1s²2p^{2 3}P₂	1764.71	1765.36		1s²2s2p ¹P₀	1837.38	1838.83
1s2s²2p^{2 2}P_3/2	1s²2s2p ¹P₁	1784.97	1784.03		1s²2s2p ³P₁	1861.00	1864.05
	1s²2s2p ³P₀	1808.59	1809.25		1s²2s2p ³P₂	1860.45	1863.51
	1s²2s2p ³P₁	1808.04	1808.72		1s²2s2p ³P₃	1859.28	1862.31
	1s²2s2p ³P₂	1806.87	1807.52		1s²2p^{2 1}S₀	1796.25	1797.43
	1s²2p^{2 1}D₂	1760.35	1759.62		1s²2p^{2 1}D₂	1812.76	1814.41
	1s²2p^{2 3}P₀	1768.34	1768.83		1s²2p^{2 3}P₀	1820.75	1823.62
	1s²2p^{2 3}P₁	1767.76	1768.15		1s²2p^{2 3}P₁	1820.17	1822.94
	1s²2p^{2 3}P₂	1766.66	1767.14		1s²2p^{2 3}P₂	1819.07	1821.93
1s2s²2p^{2 2}D_3/2	1s²2s^{2 1}S₀	1829.61	1830.38	1s2s(¹S)2p^{3 2}P_1/2	1s²2s^{2 1}S₀	1875.27	1877.33
	1s²2s2p ¹P₁	1781.36	1780.34		1s²2s2p ¹P₀	1827.02	1827.28
	1s²2s2p ³P₀	1804.98	1805.56		1s²2s2p ³P₁	1850.64	1852.50
	1s²2s2p ³P₁	1804.43	1805.02		1s²2s2p ³P₂	1850.09	1851.97
	1s²2s2p ³P₂	1803.26	1803.82		1s²2s2p ³P₃	1848.92	1850.77
	1s²2p^{2 1}S₀	1740.23	1738.94		1s²2p^{2 1}S₀	1785.89	1785.88
	1s²2p^{2 1}D₂	1756.74	1755.92		1s²2p^{2 1}D₂	1802.40	1802.87
	1s²2p^{2 3}P₀	1764.73	1765.13		1s²2p^{2 3}P₀	1810.39	1812.08
	1s²2p^{2 3}P₁	1764.15	1764.45		1s²2p^{2 3}P₁	1809.81	1811.40
	1s²2p^{2 3}P₂	1763.05	1763.44		1s²2p^{2 3}P₂	1808.71	1810.39
1s2s²2p^{2 2}D_5/2	1s²2s^{2 1}S₀	1829.37	1830.33	1s2s(¹S)2p^{3 2}P_3/2	1s²2s^{2 1}S₀	1875.94	1877.26
	1s²2s2p ¹P₁	1781.12	1780.29		1s²2s2p ¹P₀	1827.69	1827.21
	1s²2s2p ³P₀	1804.74	1805.51		1s²2s2p ³P₁	1851.31	1852.43
	1s²2s2p ³P₁	1804.19	1804.97		1s²2s2p ³P₂	1850.76	1851.90
	1s²2s2p ³P₂	1803.02	1803.77		1s²2s2p ³P₃	1849.59	1850.70
	1s²2p^{2 1}S₀	1739.99	1738.89		1s²2p^{2 1}S₀	1786.56	1785.81
	1s²2p^{2 1}D₂	1756.50	1755.87		1s²2p^{2 1}D₂	1803.07	1802.80
	1s²2p^{2 3}P₀	1764.49	1765.08		1s²2p^{2 3}P₀	1811.06	1812.01
	1s²2p^{2 3}P₁	1763.91	1764.40		1s²2p^{2 3}P₁	1810.48	1811.33
	1s²2p^{2 3}P₂	1762.81	1763.39		1s²2p^{2 3}P₂	1809.38	1810.32
1s2p^{4 2}S_1/2	1s²2s^{2 1}S₀	1926.23	1930.57	1s2s(³S)2p^{3 2}D_3/2	1s²2s2p ¹P₀	1829.45	1831.14
	1s²2s2p ¹P₁	1877.98	1880.52		1s²2s2p ³P₀	1853.07	1856.36
	1s²2s2p ³P₀	1901.60	1905.75		1s²2s2p ³P₁	1852.52	1855.83
	1s²2s2p ³P₁	1901.05	1905.21		1s²2s2p ³P₂	1851.35	1854.62
	1s²2s2p ³P₂	1899.88	1904.01		1s²2p^{2 1}D₂	1804.83	1806.72
	1s²2p^{2 1}S₀	1836.85	1839.13		1s²2p^{2 3}P₀	1812.82	1815.93
	1s²2p^{2 1}D₂	1853.36	1856.11		1s²2p^{2 3}P₁	1812.24	1815.25
1s2p^{4 2}P_1/2	1s²2s2p ¹P₁	1865.46	1867.17		1s²2p^{2 3}P₂	1811.14	1814.24
	1s²2s2p ³P₀	1889.08	1892.39	1s2s(³S)2p^{3 2}D_5/2	1s²2s2p ¹P₀	1829.17	1830.60
	1s²2s2p ³P₁	1888.53	1891.86		1s²2s2p ³P₀	1852.79	1855.82
	1s²2s2p ³P₂	1887.36	1890.66		1s²2s2p ³P₁	1852.24	1855.28
	1s²2p^{2 1}D₂	1840.84	1842.76		1s²2s2p ³P₂	1851.07	1854.08
	1s²2p^{2 3}P₀	1848.83	1851.97		1s²2p^{2 1}D₂	1804.55	1806.18
	1s²2p^{2 3}P₁	1848.25	1851.29		1s²2p^{2 3}P₀	1812.54	1815.39
	1s²2p^{2 3}P₂	1847.15	1850.28		1s²2p^{2 3}P₁	1811.96	1814.71
1s2p^{4 2}P_3/2	1s²2s2p ¹P₁	1865.22	1866.27		1s²2p^{2 3}P₂	1810.86	1813.70
	1s²2s2p ³P₀	1888.84	1891.50	1s2s(¹S)2p^{3 2}D_3/2	1s²2s2p ¹P₀	1819.51	1819.23
	1s²2s2p ³P₁	1888.29	1890.96		1s²2s2p ³P₀	1843.13	1844.45
	1s²2s2p ³P₂	1887.12	1889.76		1s²2s2p ³P₁	1842.58	1843.92
	1s²2p^{2 1}D₂	1840.60	1841.86		1s²2s2p ³P₂	1841.41	1842.71
	1s²2p^{2 3}P₀	1848.59	1851.07		1s²2p^{2 1}D₂	1794.89	1794.81
	1s²2p^{2 3}P₁	1848.01	1850.39		1s²2p^{2 3}P₀	1802.88	1804.02
	1s²2p^{2 3}P₂	1846.91	1849.38		1s²2p^{2 3}P₁	1802.30	1803.35
1s2p^{4 2}D_3/2	1s²2s^{2 1}S₀	1910.16	1913.47		1s²2p^{2 3}P₂	1801.20	1802.33
	1s²2s2p ¹P₁	1861.91	1863.42	1s2s(¹S)2p^{3 2}D_5/2	1s²2s2p ¹P₀	1819.71	1819.38
	1s²2s2p ³P₀	1885.53	1888.64		1s²2s2p ³P₀	1843.33	1844.60
	1s²2s2p ³P₁	1884.98	1888.11		1s²2s2p ³P₁	1842.78	1844.07
	1s²2s2p ³P₂	1883.81	1886.91		1s²2s2p ³P₂	1841.61	1842.86
	1s²2p^{2 1}S₀	1820.78	1822.02		1s²2p^{2 1}D₂	1795.09	1794.96
	1s²2p^{2 1}D₂	1837.29	1839.01		1s²2p^{2 3}P₀	1803.08	1804.17
	1s²2p^{2 3}P₀	1845.28	1848.22		1s²2p^{2 3}P₁	1802.50	1803.50
	1s²2p^{2 3}P₁	1844.70	1847.54		1s²2p^{2 3}P₂	1801.40	1802.49
	1s²2p^{2 3}P₂	1843.60	1846.53	1s2s(³S)2p^{3 4}S_3/2	1s²2p^{2 3}P₀	1807.49	1810.50
1s2p^{4 2}D_5/2	1s²2s^{2 1}S₀	1909.99	1913.40		1s²2p^{2 3}P₁	1806.91	1809.82
	1s²2s2p ¹P₁	1861.74	1863.35		1s²2p^{2 3}P₂	1805.81	1808.81
	1s²2s2p ³P₀	1885.36	1888.57	1s2s(¹S)2p^{3 4}S_3/2	1s²2p^{2 3}P₀	1785.26	1785.14
	1s²2s2p ³P₁	1884.81	1888.04		1s²2p^{2 3}P₁	1784.68	1784.46
	1s²2s2p ³P₂	1883.64	1886.84		1s²2p^{2 3}P₂	1783.58	1783.45
	1s²2p^{2 1}S₀	1820.61	1821.95	1s2s(³S)2p^{3 4}P_1/2	1s²2s2p³P₀	1831.31	1832.66
	1s²2p^{2 1}D₂	1837.12	1838.94		1s²2s2p³P₁	1830.76	1832.13
	1s²2p^{2 3}P₀	1845.11	1848.15		1s²2s2p³P₂	1829.59	1830.93
	1s²2p^{2 3}P₁	1844.53	1847.47		1s²2p^{2 3}P₀	1791.06	1792.24
	1s²2p^{2 3}P₂	1843.43	1846.46		1s²2p^{2 3}P₁	1790.48	1791.56
1s2s²2p^{2 4}P_1/2	1s²2s2p³P₀	1792.86	1791.05		1s²2p^{2 3}P₂	1789.38	1790.55
	1s²2s2p³P₁	1792.31	1790.51	1s2s(³S)2p^{3 4}P_3/2	1s²2s2p³P₀	1831.12	1832.56
	1s²2s2p³P₂	1791.14	1789.31		1s²2s2p³P₁	1830.57	1832.03
	1s²2p^{2 3}P₀	1752.61	1750.62		1s²2s2p³P₂	1829.40	1830.83
	1s²2p^{2 3}P₁	1752.03	1749.94		1s²2p^{2 3}P₀	1790.87	1792.14
	1s²2p^{2 3}P₂	1750.93	1748.93		1s²2p^{2 3}P₁	1790.29	1791.46
1s2s²2p^{2 4}P_3/2	1s²2s2p³P₀	1793.53	1791.83		1s²2p^{2 3}P₂	1789.19	1790.45
	1s²2s2p³P₁	1792.98	1791.30	1s2s(³S)2p^{3 4}P_5/2	1s²2s2p³P₀	1831.04	1832.48
	1s²2s2p³P₂	1791.81	1790.09		1s²2s2p³P₁	1830.49	1831.95
	1s²2p^{2 3}P₀	1753.28	1751.40		1s²2s2p³P₂	1829.32	1830.75
	1s²2p^{2 3}P₁	1752.70	1750.72		1s²2p^{2 3}P₀	1790.79	1792.06
	1s²2p^{2 3}P₂	1751.60	1749.71		1s²2p^{2 3}P₁	1790.21	1791.38
1s2s²2p^{2 4}P_5/2	1s²2s2p³P₀	1794.37	1792.66		1s²2p^{2 3}P₂	1789.11	1790.37
	1s²2s2p³P₁	1793.82	1792.13	1s2s(³S)2p^{3 4}D_1/2	1s²2s2p³P₀	1823.15	1824.54
	1s²2s2p³P₂	1792.65	1790.92		1s²2s2p³P₁	1822.60	1824.01
	1s²2p^{2 3}P₀	1754.12	1752.23		1s²2s2p³P₂	1821.43	1822.80
	1s²2p^{2 3}P₁	1753.54	1751.55		1s²2p^{2 3}P₀	1782.90	1784.11
	1s²2p^{2 3}P₂	1752.44	1750.54		1s²2p^{2 3}P₁	1782.32	1783.43
1s2p^{4 4}P_1/2	1s²2s2p³P₀	1873.83	1876.31		1s²2p^{2 3}P₂	1781.22	1782.42
	1s²2s2p³P₁	1873.28	1875.78	1s2s(³S)2p^{3 4}D_3/2	1s²2s2p³P₀	1823.15	1824.49
	1s²2s2p³P₂	1872.11	1874.57		1s²2s2p³P₁	1822.60	1823.96
	1s²2p^{2 3}P₀	1833.58	1835.88		1s²2s2p³P₂	1821.43	1822.75
	1s²2p^{2 3}P₁	1833.00	1835.20		1s²2p^{2 3}P₀	1782.90	1784.06
	1s²2p^{2 3}P₂	1831.90	1834.19		1s²2p^{2 3}P₁	1782.32	1783.39
1s2p^{4 4}P_3/2	1s²2s2p³P₀	1873.24	1875.77		1s²2p^{2 3}P₂	1781.22	1782.38
	1s²2s2p³P₁	1872.69	1875.24	1s2s(³S)2p^{3 4}D_5/2	1s²2s2p³P₀	1823.06	1824.41
	1s²2s2p³P₂	1871.52	1874.03		1s²2s2p³P₁	1822.51	1823.88
	1s²2p^{2 3}P₀	1832.99	1835.34		1s²2s2p³P₂	1821.34	1822.67
	1s²2p^{2 3}P₁	1832.41	1834.66		1s²2p^{2 3}P₀	1782.81	1783.98
	1s²2p^{2 3}P₂	1831.31	1833.65		1s²2p^{2 3}P₁	1782.23	1783.30
1s2p^{4 4}P_5/2	1s²2s2p³P₀	1871.99	1874.50		1s²2p^{2 3}P₂	1781.13	1782.29
	1s²2s2p³P₁	1871.44	1873.96	1s2s(³S)2p^{3 4}D_7/2	1s²2s2p³P₁	1822.20	1823.70
	1s²2s2p³P₂	1870.27	1872.76		1s²2s2p³P₂	1821.03	1822.50
	1s²2p^{2 3}P₀	1831.74	1834.07		1s²2p^{2 3}P₁	1781.92	1783.13
	1s²2p^{2 3}P₁	1831.16	1833.39		1s²2p^{2 3}P₂	1780.82	1782.12
	1s²2p^{2 3}P₂	1830.06	1832.38

DownLoad: CSV

[1]	Altun Z, Yumak A, Badnell N R, Colgan J, Pindzol M S 2004 A&A 420 775
[2]	Rohringer N, Ryan D, London R A, Purvis M, Albert F, Dunn J, Bozek J D, Bostedt C, Graf A, Hill R, Hau-Riege S P, Rocca J J 2012 Nature 481 488 Google Scholar
[3]	Martin A, Nicolas G, Jacques S 2006 Nucl. Phys. A 777 1
[4]	冯雷, 蒋刚 2017 物理学报 66 153201 Google Scholar Feng L, Jiang G 2017 Acta Phys. Sin. 66 153201 Google Scholar
[5]	Rødbro M, Bruch R, Bisgaard P 1979 J. Phys. B: At. Mol. Opt. Phys. 12 2413 Google Scholar
[6]	Schneider D, Bruch R, Butscher W, Schwarz W H E 1981 Phys. Rev. A 24 1223 Google Scholar
[7]	Bruch R, Schneider D, Schwarz W H E, Meinhart M, Johnson B M, Taulbjerg K 1979 Phys. Rev. A 19 587 Google Scholar
[8]	Itoh A, Schneider D, Schneider T, Zouros T J M, Nolte G, Schiwietz G, Zeitz W, Stolterfoht N 1985 Phys. Rev. A 31 684 Google Scholar
[9]	Kádár I, Ricz S, Végh J, Sulik B, Varga D, Berényi D 1990 Phys. Rev. A 41 3518 Google Scholar
[10]	Armour I A, Fawcett B C, Silver J D, Trabert E 1980 J. Phys. B: Atom. Molec. Phys. 13 2701 Google Scholar
[11]	Trabertt E, Fawcett B C 1979 J. Phys. B: Atom. Molec. Phys. 12 L441
[12]	Faenov A Y 1994 Phys. Scr. 49 41 Google Scholar
[13]	Schlachter A S, Sant’Anna M M, Covington A M, Aguilar A, Gharaibeh M F, Emmons E D, Scully S W J, Phaneuf R A, Hinojosa G, Álvarez I, Cisneros C, Müller A, McLaughlin B M 2004 J. Phys. B: At. Mol. Opt. Phys. 37 L103 Google Scholar
[14]	Gharaibeh M F, Hassan N E I, Shorman M M A L, Bizau J M, Cubaynes D, Guilbaud S, Sakho I, Blancard C, McLaughlin B M 2014 J. Phys. B: At. Mol. Opt. Phys. 47 065201 Google Scholar
[15]	Müller A, Borovik A, Buhr T, Hellhund J, Holste K, Kilcoyne A L D, Klumpp S, Martins M, Ricz S, Viefhaus J, Schippers S 2018 Phys. Rev. A 97 013409 Google Scholar
[16]	Müller A, Borovik A, Buhr J T, Hellhund J, Holste K, Kilcoyne A L D, Klumpp S, Martins M, Ricz S, Viefhaus J, Schippers S 2015 Phys. Rev. Lett. 114 013002 Google Scholar
[17]	Chen M H, Crasemann B 1988 At. Data Nucl. Data Tables 38 381 Google Scholar
[18]	Chen M H, Crasemann B 1987 Phys. Rev. A 35 4579 Google Scholar
[19]	Safronova U I, Shlyaptseva A S 1996 Phys. Scr. 54 254 Google Scholar
[20]	Zhou F Y, Ma Y L, Qu Y Z 2016 Phys. Rev. A 93 060501 Google Scholar
[21]	Sakho I, Sow M, Wagué A 2015 Phys. Scr. 90 045401 Google Scholar
[22]	Sun Y, Chen F, Gou B C 2011 J. Chem. Phys. 135 124309 Google Scholar
[23]	Sun Y, Gou B C, Chen C 2013 Phys. Rev. A 87 032509 Google Scholar
[24]	Chung K T 1979 Phys. Rev. A 20 1743 Google Scholar
[25]	Lin B, Berry H G, Shibata T, Livingston A E, Garnir H P, Bastin T, Désesquelles J, Savukov I 2003 J. Phys. B: At. Mol. Opt. Phys. 67 062507 Google Scholar
[26]	Drake G W F 1982 Adv. At. Mol. Phys. 18 399 Google Scholar
[27]	Chung K T, Zhu X W, Wang Z W 1993 Phys. Rev. A 47 1740 Google Scholar
[28]	Drake G W F, Swainson R A 1990 Phys. Rev. A 41 1243 Google Scholar
[29]	Chung K T, Davis B F 1982 Phys. Rev. A 26 3278 Google Scholar
[30]	Davis B F, Chung K T 1984 Phys. Rev. A 29 1878 Google Scholar
[31]	Kramida A, Ralchenko Yu, Reader J, NIST ASD Team 2018 NIST Atomic Spectra Database (ver. 5.6.1) [Online]. Available: https://physics.nist.gov/asd [2019, March 28]. National Institute of Standards and Technology, Gaithersburg, MD. DOI: https://doi.org/10.18434/T4W30F

[1]	Qin Chao-Chao, Cui Ming-Huan, Song Di-Di, He Wei. Ultrafast multiexciton Auger recombination of CdSeS. Acta Physica Sinica, 2019, 68(10): 107801. doi: 10.7498/aps.68.20190291
[2]	Qian Xin-Yu, Sun Yan, Liu Dong-Dong, Hu Feng, Fan Qiu-Bo, Gou Bing-Cong. Energy levels and radiative transitions of the core-excited high-spin states in boron atom (ion). Acta Physica Sinica, 2017, 66(12): 123101. doi: 10.7498/aps.66.123101
[3]	Ma Xiao-Yun, Dong Chen-Zhong, Wu Zhong-Wen, Jiang Jun, Xie Lu-You. Theoretical study on electron-impact excitation processes and the relevant polarization of radiation of 2s1/2—2p3/2 in W65+ through W71+. Acta Physica Sinica, 2012, 61(21): 213401. doi: 10.7498/aps.61.213401
[4]	Sun Wei-Feng, Li Mei-Cheng, Zhao Lian-Cheng. First-principles investigation of carrier Auger lifetime and impact ionization rate in narrow-gap superlattices. Acta Physica Sinica, 2010, 59(8): 5661-5666. doi: 10.7498/aps.59.5661
[5]	Liu Shao-Ding, Cheng Mu-Tian, Zhou Hui-Jun, Li Yao-Yi, Wang Qu-Quan, Xue Qi-Kun. The effect of biexciton, wetting layer leakage and Auger capture on Rabi oscillation damping in quantum dots. Acta Physica Sinica, 2006, 55(5): 2122-2127. doi: 10.7498/aps.55.2122
[6]	Li Jie, Dong Chen-Zhong, Xie Lu-You. Effects of relaxation induced by excitation (or ionization) of inner subshell electrons on the wave functions and transition probabilities. Acta Physica Sinica, 2006, 55(2): 655-660. doi: 10.7498/aps.55.655
[7]	WANG FEI, GOU BING-CONG, HAN LI-HONG. RADIATIVE TRANSITION OF CORE-EXCITED 2smd4De STATES TO THE 2pnd4Do STATES IN LITHIUM. Acta Physica Sinica, 2001, 50(9): 1685-1688. doi: 10.7498/aps.50.1685
[8]	YUAN JIN-SHE, CHEN GUANG-DE, QI MING, LI AI-ZHEN, XU ZHUO. XPS AND AES INVESTIGATION OF GaN FILMS GROWN BY MBE. Acta Physica Sinica, 2001, 50(12): 2429-2433. doi: 10.7498/aps.50.2429
[9]	HAN LI-HONG, GOU BING-CONG, WANG FEI. RELATIVISTIC ENERGIES AND FINE STRUCTURES OF THE EXCITED STATES FOR BERYLLIUM-LIKE BⅡ. Acta Physica Sinica, 2001, 50(9): 1681-1684. doi: 10.7498/aps.50.1681
[10]	HAN LI-HONG, GOU BING-CONG, WANG FEI. RADIATIVE TRANSITION OF TRIPLY EXCITED 2p2np4So STATES TO THE ls2pmp4P STATES IN LITHIUM-LIKE IONS. Acta Physica Sinica, 2000, 49(11): 2139-2145. doi: 10.7498/aps.49.2139
[11]	CHEN WEI-DE, GUI YU-DE. DETERMINATION OF AlxGa1-xAs AUGER SENSITIVITY FACTORS. Acta Physica Sinica, 1994, 43(4): 673-677. doi: 10.7498/aps.43.673
[12]	GOU BING-CONG. RADIATIVE AND AUGER RATES OF HIGH DOUBLY EXCITED INTERSHELL STATES. Acta Physica Sinica, 1993, 42(2): 223-230. doi: 10.7498/aps.42.223
[13]	SHI YI-SHENG, ZHAO TE-XIU, LIU HONG-TU, WANG XIAO-PING. XPS AND AES STUDY FOR Pd/W/Si(lll) BILAYER INTERFACE. Acta Physica Sinica, 1992, 41(11): 1849-1855. doi: 10.7498/aps.41.1849
[14]	ZHAO RU-GUANG, YANG WEI-SHENG. TUNABLE-SAMPLING-DEPTH ELECTRON ENERGY LOSS SPECTROSCOPY AND AUGER ELECTRON SPECTROSC-OPY STUDIES OF Pb/Ni(001) INTERFACE. Acta Physica Sinica, 1992, 41(7): 1125-1131. doi: 10.7498/aps.41.1125
[15]	WEI XING, JIANG WEI-DONG, ZHOU GUO-LIANG, YU MING-REN, WANC XUN. AUGER DEPTH PROFILE ANALYSIS OF GexSi1-x/Si SUPERLATTICE. Acta Physica Sinica, 1991, 40(9): 1514-1519. doi: 10.7498/aps.40.1514
[16]	ZHONG ZHAN-TIAN, WANG DA-WEN, LIAO XIAN-BO, FAN YUE, LI CHENG-FANG, MOU SHAN-MING. XPS AND AES STUDY FOR Au/a-Si:H INTERFACE. Acta Physica Sinica, 1991, 40(2): 275-280. doi: 10.7498/aps.40.275
[17]	YU YUE-HUI, LIN CHENG-LU, ZHANG SHUN-KAI, FANG ZI-ZEI, ZOU SHI-CHANG. AUGER ELECTRON SPECTROSCOPIC STUDIES OF INTERFA CE AND BURIED LAYER OF SOI STRUCTURE FORMED BY ION IMPLANTATION. Acta Physica Sinica, 1989, 38(12): 1996-2002. doi: 10.7498/aps.38.1996
[18]	GUO YUAN-HENG, CHEN LAN-FENG. SURFACE STUDY OF SUPERCONDUCTING Nb-Ge FILM BY AUGER ELECTRON SPECTROSCOPY AND ELECTRON SPECTROSCOPY FOR CHEMICAL ANALYSIS. Acta Physica Sinica, 1988, 37(7): 1196-1102. doi: 10.7498/aps.37.1196
[19]	ZHAO ZHONG-XIN, LI JIA-MING. NON- RELATIVISTIC AND RELATIVISTIC ATOMIC CONFIGURATION INTERACTION THEORY EXCITATION ENERGY AND RADIATIVE TRANSITION PROBABILITY. Acta Physica Sinica, 1985, 34(11): 1469-1478. doi: 10.7498/aps.34.1469
[20]	WU ZI-QIN, DUAN JIAN-ZHONG. THE CALCULATION OF BACKSCATTERING FACTORS IN AUGER ELECTRON SPECTROSCOPY. Acta Physica Sinica, 1984, 33(3): 419-424. doi: 10.7498/aps.33.419

Catalog

Vol. 68, Issue 16 - 2019-08-20

Metrics

Abstract views: 7958
PDF Downloads: 47
Cited By: 0

姓名
邮箱
手机号码
标题
留言内容
验证码

Search

Article

留言板