|
|
Oscillator strength study of the excitations of valence-shell of C2H2 by high-resolution inelastic x-ray scattering |
Qiang Sun(孙强)1, Ya-Wei Liu(刘亚伟)2, Yuan-Chen Xu(徐远琛)1, Li-Han Wang(王礼涵)1, Tian-Jun Li(李天钧)1, Shu-Xing Wang(汪书兴)1, Ke Yang(杨科)3,†, and Lin-Fan Zhu(朱林繁)1,‡ |
1 Hefei National Research Center for Physical Sciences at Microscale and Department of Modern Physics, University of Science and Technology of China, Hefei 230026, China; 2 Anhui Province Key Laboratory of Medical Physics and Technology, Institute of Health and Medical Technology, Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230026, China; 3 Shanghai Advanced Research Institute, Chinese Academy of Sciences, Shanghai 201204, China |
|
|
Abstract The oscillator strengths of the valence-shell excitations of C2H2 are extremely important for testing theoretical models and studying interstellar gases. In this study, the high-resolution inelastic x-ray scattering (IXS) method is adopted to determine the generalized oscillator strengths (GOSs) of the valence-shell excitations of C2H2 at a photon energy of 10 keV. The GOSs are extrapolated to their zero limit to obtain the corresponding optical oscillator strengths (OOSs). Through taking a completely different experimental method of the IXS, the present results offer the high energy limit for electron collision to satisfy the first Born approximation (FBA) and cross-check the previous experimental and theoretical results independently. The comparisons indicate that an electron collision energy of 1500 eV is not enough for C2H2 to satisfy the FBA for the large squared momentum transfer, and the line saturation effect limits the accuracy of the OOSs measured by the photoabsorption method.
|
Received: 22 October 2021
Revised: 30 November 2021
Accepted manuscript online:
|
PACS:
|
34.80.Gs
|
(Molecular excitation and ionization)
|
|
61.05.cf
|
(X-ray scattering (including small-angle scattering))
|
|
95.30.Ky
|
(Atomic and molecular data, spectra, and spectralparameters (opacities, rotation constants, line identification, oscillator strengths, gf values, transition probabilities, etc.))
|
|
Fund: Project supported by the Strategic Priority Research Program of the Chinese Academy of Science (Grant No.XDB34000000),the National Natural Science Foundation of China (Grant Nos.U1932207 and 12104437),and the National Key Research and Development Program of China (Grant No.2017YFA0402300).The support from the Heavy Ion Research Facility in Lanzhou (HIRFL) is also acknowledged.The IXS experiment was performed at the BL12XU of SPring-8 with the approval of Japan Synchrotron Radiation Research Institute (Proposal No.2019A4275) and "National" Synchrotron Radiation Research Center,Taiwan,China (Proposal No.2019-2-089-1). |
Corresponding Authors:
Ke Yang,E-mail:yangke@zjlab.org.cn;Lin-Fan Zhu,E-mail:lfzhu@ustc.edu.cn
E-mail: yangke@zjlab.org.cn;lfzhu@ustc.edu.cn
|
About author: 2021-12-11 |
Cite this article:
Qiang Sun(孙强), Ya-Wei Liu(刘亚伟), Yuan-Chen Xu(徐远琛), Li-Han Wang(王礼涵), Tian-Jun Li(李天钧), Shu-Xing Wang(汪书兴), Ke Yang(杨科), and Lin-Fan Zhu(朱林繁) Oscillator strength study of the excitations of valence-shell of C2H2 by high-resolution inelastic x-ray scattering 2022 Chin. Phys. B 31 053401
|
[1] Prasad S S and Huntress W T 1980 Astrophys. J. Suppl. Ser. 43 1 [2] Ridgway S T, Hall D N B, Kleinmann S G, Weinberger D A and Wojslaw R S 1976 Nature 264 345 [3] Jorgensen U G and Johnson H R 1991 Astron. Astrophys. 244 462 [4] Mitchell G F, Prasad S S and Huntress W T 1981 Astrophys. J. 244 1087 [5] Shemansky D E, Stewart A F, West R A, Esposito L W, Hallett J T and Liu X M 2005 Science 308 978 [6] Price W C 1935 Phys. Rev. 47 444 [7] Liu Y W, Xu L Q, Chen T, Qi D G, Xiong T and Zhu L F 2018 Astrophys. J. Suppl. Ser. 234 10 [8] Smith P L, Yoshino K, Parkinson W H, Ito K and Stark G 1991 J. Geophys. Res. Planets 96 17529 [9] Wu C Y R, Chen F Z and Judge D L 2001 J. Geophys. Res. Planets 106 7629 [10] Cheng B M, Chen H F, Lu H C, Chen H K, Alam M S, Chou S L and Lin M Y 2011 Astrophys. J. Suppl. Ser. 196 3 [11] Suto M and Lee L C 1984 J. Chem. Phys. 80 4824 [12] Gedanken A and Schnepp O 1976 Chem. Phys. Lett. 37 373 [13] Moe G and Duncan A B F 1952 J. Am. Chem. Soc. 74 3136 [14] Chan W F, Cooper G and Brion C E 1991 Phys. Rev. A 44 186 [15] Xu L Q, Liu Y W, Kang X, Ni D D, Yang K, Hiraoka N, Tsuei K D and Zhu L F 2015 Sci. Rep. 5 18350 [16] Wang S X and Zhu L F 2020 Matter Radiat. Extremes 5 054201 [17] Cooper G, Burton G R and Brion C E 1995 J. Electron Spectrosc. Relat. Phenom. 73 139 [18] Xu L Q, Liu Y W, Xu X, Ni D D, Yang K and Zhu L F 2017 Eur. Phys. J. D 71 183 [19] Xiong T, Xu Y C, Yang K, Hiraoka N and Zhu L F 2019 Astrophys. J. 885 163 [20] Jensen J O, Adams G F and Chabalowski C F 1990 Chem. Phys. Lett. 172 379 [21] Demoulin D and Jungen M 1974 Theoret. Chim. Acta 34 1 [22] Xie B P, Zhu L F, Yang K, Zhou B, Hiraoka N, Cai Y Q, Yao Y, Wu C Q, Wang E L and Feng D L 2010 Phys. Rev. A 44 032501 [23] Zhu L F, Wang L S, Xie B P, Yang K, Hiraoka N, Cai Y Q and Feng D L 2011 J. Phys. B: At. Mol. Opt. Phys. 44 025203 [24] Platzman P M and Tzoar N 1965 Phys. Rev. 139 A410 [25] Eisenberger P and Platzman P M 1970 Phys. Rev. A 2 415 [26] Kang X, Yang K, Liu Y W, Xu W Q, Hiraoka N, Tsuei K D, Zhang P F and Zhu L F 2012 Phys. Rev. A 86 022509 [27] Zhu L F, Xu W Q, Yang K, Jiang Z, Kang X, Xie B P, Feng D L, Hiraoka N and Tsuei K D 2012 Phys. Rev. A 85 030501 [28] Bethe H 1930 Ann. Phys. 397 325 [29] Bethe H 1932 Z. Phys. 76 293 [30] Inokuti M 1971 Rev. Mod. Phys. 43 297 [31] Lassettre E N 1965 J. Chem. Phys. 43 4479 |
No Suggested Reading articles found! |
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
Cited |
|
|
|
|
Altmetric
|
blogs
Facebook pages
Wikipedia page
Google+ users
|
Online attention
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
View more on Altmetrics
|
|
|