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High-precision electron structure calculation of CaSH molecules and theoretical analysis of its application to laser-cooled target molecules

Feng Zhuo Suo Bing-Bing Han Hui-Xian Li An-Yang

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High-precision electron structure calculation of CaSH molecules and theoretical analysis of its application to laser-cooled target molecules

Feng Zhuo, Suo Bing-Bing, Han Hui-Xian, Li An-Yang
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  • The CaSH molecule is an important target in the field of laser cooling non-linear polyatomic molecules. Successful cooling of such molecules marks a breakthrough of the technical limitations of laser cooling diatomic and linear triatomic molecules. To identify the possible optical cycle in cooling CaSH, precise geometries of the CaSH ground state and the three lowest excited states, along with their excitation energy, are determined by utilizing the EA-EOM-CCSD (electron attachment equation-of-motion coupled cluster singles and doubles) method, in combination with energy extrapolation using cc-pVXZ/cc-pCVXZ (X = T, Q ) serial basis sets. Geometric parameters of the ground state $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} $ are found to be RCaS= 2.564 Å, RSH= 1.357 Å, andCaSH= 91.0°. Additionally, the equilibrium geometries of three excited states are also obtained. The $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ state has a similar equilibrium structure to the ground state, while the $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $ and $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $ states exhibit significant conformer distortions. Specifically, the CaS bond of the $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $ state and $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $ state tend to contract, and the CaSH angel bends by 5° relative to the ground state. The vertical excitation energy from the ground state to $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $, $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ and $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $ are of 1.898, 1.945 and 1.966 eV, respectively, which are in good agreement with the previous experimental results. Moreover, the potential energy surfaces of the four lowest electronic states of CaSH are calculated by EA-EOM-CCSD with 3ζ level of basis sets. The nuclear equations of motion are solved to obtain the vibrational frequencies of the CaS bond stretching and CaSH bending. The vibrational frequencies of the (0,1,0) mode and the CaS stretching frequency of four states are 316 cm–1, 315 cm–1, 331 cm–1 and 325 cm–1, which are in close agreement with the available experimental results. The frequencies of the CaSH bending mode are presented for the first time, with the values of 357 cm–1, 396 cm–1, 384 cm–1, 411 cm–1 for the $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} $, $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $, $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ and $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $ states, respectively. Theoretical calculations give the Frank-Condon factors of 0.9268, 0.9958 and 0.9248 for the $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} ({\mathrm{0,0}},0) $ to $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} ({\mathrm{0,0}},0) $, $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{{{\prime} }{{\prime} }}({\mathrm{0,0}},0) $ and $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} ({\mathrm{0,0}},0) $ transitions. All three excited states are the bright states with considerable oscillator strength relative to the ground state. Based on the Frank-Condon factor and lifetime of excited states, the $ {{\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} ({\mathrm{0,0}},0)\to \tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{{{\prime} }{{\prime} }}({\mathrm{0,0}},0) $ transition is regarded as the main cooling cycle for the CaSH molecule. The corresponding pump light wavelength is 678 nm. By exciting the vibrational excited states (0,1,0) and (0,0,1) of the $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} $ state to $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} ({\mathrm{0,0}},0) $ using lasers at 666 nm and 668 nm, respectively, the optical cooling branch ratio of CaSH is expected to exceed 0.9998.
      Corresponding author: Suo Bing-Bing, bsuo@nwu.edu.cn
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 21873077) and the Natural Science Basic Research Plan in Shaanxi Province of China (Grant No. 2021JM-311).
    [1]

    Balakrishnan N 2016 J. Chem. Phys. 145 150901Google Scholar

    [2]

    Wu Y, Bao W S, Cao S R, et al. 2021 Phys. Rev. Lett. 127 180501Google Scholar

    [3]

    Andreev V, Ang D G, Demille D, Doyle J M, Gabrielse G, Haefner J, Hutzler N R, Lasner Z, Meisenhelder C, O'Leary B R, Panda C D, West A D, West E P, Wu X 2018 Nature 562 355Google Scholar

    [4]

    Baron J, Campbell W C, DeMille D, Doyle J M, Gabrielse G, Gurevich Y V, Hess P W, Hutzler N R, Kirilov E, Kozyryev I, O’Leary B R, Panda C D, Parsons M F, Petrik E S, Spaun B, Vutha A C, West A D 2014 Science 343 269Google Scholar

    [5]

    Barry J F, Mccarron D J, Norrgard E B, Steinecker M H, Demille D 2014 Nature 512 286Google Scholar

    [6]

    Norrgard E B, McCarron D J, Steinecker M H, Tarbutt M R, DeMille D 2016 Phys. Rev. Lett. 116 063004Google Scholar

    [7]

    Truppe S, Williams H J, Fitch N J, Hambach M, Wall T E, Hinds E A, Sauer B E, Tarbutt M R 2017 New J. Phys. 19 022001Google Scholar

    [8]

    Kozyryev I, Baum L, Matsuda K, Augenbraun B L, Anderegg L, Sedlack A P, Doyle J M 2017 Phys. Rev. Lett. 118 173201Google Scholar

    [9]

    Augenbraun B L, Lasner Z D, Frenett A, Sawaoka H, Miller C, Steimle T C, Doyle J M 2020 New J. Phys. 22 022003Google Scholar

    [10]

    Baranov M A 2008 Phys. Rep. 464 71Google Scholar

    [11]

    Ni K K, Ospelkaus S, De Miranda M H, Hg M, Pe'Er A, Neyenhuis B, Zirbel J J, Kotochigova S, Julienne P S, Jin D S, Ye J 2008 Science 322 231Google Scholar

    [12]

    Shuman E S, Barry J F, DeMille D 2010 Nature 467 820Google Scholar

    [13]

    Hummon M T, Yeo M, Stuhl B K, Collopy A L, Xia Y, Ye J 2013 Phys. Rev. Lett. 110 143001Google Scholar

    [14]

    Zhelyazkova V, Cournol A, Wall T E, Matsushima A, Hudson J J, Hinds E, Tarbutt M, Sauer B 2014 Phys. Rev. A 89 053416Google Scholar

    [15]

    Gao Y, Wan M 2017 Phys. Chem. Chem. Phys. 19 5519Google Scholar

    [16]

    陈涛, 颜波 2019 68 043701Google Scholar

    Chen T, Yan B 2019 Acta Phys. Sin. 68 043701Google Scholar

    [17]

    Wells N, Lane I C 2011 Phys. Chem. Chem. Phys. 13 19018Google Scholar

    [18]

    Li D, Fu M, Ma H, Bian W, Du Z, Chen C A 2020 Front. Chem. 8 20

    [19]

    Li D, Cao J, Ma H, Bian W 2022 Phys. Chem. Chem. Phys. 24 10114

    [20]

    Ivanov M V, Bangerter F H, Krylov A I 2019 Phys. Chem. Chem. Phys. 21 19447Google Scholar

    [21]

    Augenbraun B L, Doyle J M, Zelevinsky T, Kozyryev I 2020 Phys. Rev. X 10 031022Google Scholar

    [22]

    Liu L, Yang C L, Sun Z P, Wang M S, Ma X G 2021 Phys. Chem. Chem. Phys. 23 2392Google Scholar

    [23]

    Fernando W T M L, Ram R S, O'Brien L C, Bernath P F 1991 J. Phys. Chem. 95 2665Google Scholar

    [24]

    Jarman C N, Bernath P F 1993 J. Chem. Phys. 98 6697Google Scholar

    [25]

    Ortiz J V 1990 Chem. Phys. Lett. 169 116Google Scholar

    [26]

    Scurlock C T, Henderson T, Bosely S, Jung K Y, Steimle T C 1994 J. Chem. Phys. 100 5481Google Scholar

    [27]

    Taleb-Bendiad A, Scappini F, Amano T, Watson J K 1996 J. Chem. Phys. 104 7431Google Scholar

    [28]

    Sheridan P M, Dick M J, Wang J G, Bernath P F 2007 Mol. Phys. 105 569Google Scholar

    [29]

    Nooijen M, Bartlett R J 1995 J. Chem. Phys. 102 3629Google Scholar

    [30]

    Pritchard B P, Altarawy D, Didier B T, Gibson T D, Windus T L 2019 J. Chem. Inf. Model. 59 4814Google Scholar

    [31]

    Koput J, Peterson K A 2002 J. Chem. Phys. 116 9255Google Scholar

    [32]

    Woon D E, Dunning T H 1995 J. Chem. Phys. 100 4572Google Scholar

    [33]

    Dunning T H 1989 J. Chem. Phys. 90 1007Google Scholar

    [34]

    Müller T, Dallos M, Lischka H, Dubrovay Z, Szalay P G 2001 Theor. Chem. Acc. 105 227Google Scholar

    [35]

    Lanczos C 1950 J. Res. Nat. Bur. Stand. 45 255Google Scholar

    [36]

    Goldfield E M, Gray S K, Harding L B 1993 J. Chem. Phys. 99 5812Google Scholar

    [37]

    Light J C, Carrington Jr T 2000 Adv. Chem. Phys. 114 263Google Scholar

    [38]

    Lill J V, Parker G A, Light J C 1986 J. Chem. Phys. 85 900Google Scholar

    [39]

    Liu W J, Hong Y G, Dai D D, Li L M, Dolg M 1997 Theor. Chem. Acc. 96 75Google Scholar

    [40]

    Zhang Y, Suo B B, Wang Z K, Zhang N, Li Z D, Lei Y B, Zou W L, Gao J, Peng D L, Pu Z C, Sun Q M, Wang F, Ma Y T, Wang X P, Liu W J 2020 J. Chem. Phys. 152 064113Google Scholar

    [41]

    Yang D D, Wang F, Guo J W 2012 Chem. Phys. Lett. 531 236Google Scholar

    [42]

    Tu Z Y, Wang F, Li X Y 2012 J. Chem. Phys. 136 174102Google Scholar

    [43]

    Wang Z F, Hu S, Wang F, Guo J W 2015 J. Chem. Phys. 142 144109Google Scholar

    [44]

    Cao Z L, Li Z D, Wang F, Liu W J 2017 Phys. Chem. Chem. Phys. 19 3713Google Scholar

    [45]

    李永红, 李俊峰, 王连宾, 张敬来 2008 河南大学学报(自然科学版) 38 4

    Li Y H, Li J F, Wang L B, Zhang J L 2008 J. Henan Univ. (Nat. Sci.) 38 4

    [46]

    Baum L, Vilas N B, Hallas C, Augenbraun B L, Raval S, Mitra D, Doyle J M 2020 Phys. Rev. Lett. 124 133201Google Scholar

    [47]

    Kozyryev I, Baum L, Aldridge L, Yu P, Eyler E E, Doyle J M 2018 Phys. Rev. Lett. 120 063205Google Scholar

    [48]

    Franck-Condon factors in the harmonic approximation , Wójcik P, Gozem S, Mozhayskiy V, Krylov A I. http:// iopenshell.usc.edu/downloads [2023-5-3

  • 图 1  CaSH分子前线轨道图 (a) $ 15{{\mathrm{a}}}^{\prime} ; $ (b) $ 16{{\mathrm{a}}}^{\prime} ; $ (c) $ 5{{\mathrm{a}}}^{{{\prime} }{{\prime} }}; $ (d) $ 17{\mathrm{a}}^{{\prime} } $

    Figure 1.  Frontier orbital diagram of the CaSH molecule: (a) $ 15{{\mathrm{a}}}^{\prime} ; $ (b) $ 16{{\mathrm{a}}}^{\prime} ; $ (c) $ 5{{\mathrm{a}}}^{{{\prime} }{{\prime} }}; $ (d) $ 17{\mathrm{a}}^{{\prime} } $ .

    图 2  CaSH激光冷却光学循环示意图, 实线代表激发光, 虚线为自发辐射通道

    Figure 2.  Schematic diagram of optical cycle of laser cooling of CaSH, solid lines represent the excitation light, dash lines are spontaneous emission channels.

    表 1  CaSH分子基态和3个低能级激发态的平衡结构

    Table 1.  Equilibrium structures of the ground state and three low-lying excited states of the CaSH molecule.

    State r0 (Ca-S)/Å r0 (S—H)/Å θ (Ca—S—H)/(°) Method Ref.
    $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} $ 2.557 1.338 91.0 EA-EOM-CCSD This work
    2.614 1.346 100.0 MP2 Calc.[23]
    2.607 1.339 97.1 Calc.[25]
    2.647 1.347 93.1 CCSD(T) Calc.[24]
    2.560 1.346 96.6 Expt.[22]
    2.564 1.357 91.0 Expt.[26]
    $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $ 2.528 1.343 86.0 EA-EOM-CCSD This work
    2.513 1.346 94.6 Expt.[22]
    2.517 1.357 89.1 Expt.[26]
    $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ 2.554 1.338 91.0 EA-EOM-CCSD This work
    2.550 1.357 89.1 Expt.[26]
    $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $ 2.525 1.345 86.0 EA-EOM-CCSD This work
    2.562 1.357 91.0 Expt.[26]
    DownLoad: CSV

    表 2  CaSH 基态到3个低能级激发态激发能的对比

    Table 2.  Comparison of excitation energies from the ground state to three low-lying excited states of the CaSH.

    $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} \to {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $ $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} \to {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} \to {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $
    EA-EOM-CCSD VEE a) 1.945 2.000 2.093
    1.915 1.966 2.016
    1.898 1.945 1.966 Basis set limit
    AEE b) 1.894 1.944 1.961 Basis set limit
    SA-CASSCF VEE 1.884 1.937 2.216
    f c) 0.2628 0.2589 0.1621
    Expt. 1.907 1.966 1.993 Ref. [26]
    1.905 1.960 1.987 Ref. [21]
    Calc. 1.860 1.930 2.110 Ref. [23]
    VEE a) 2.000 2.060 2.330 Ref. [43]
    注: a) 垂直激发能; b)绝热激发能; c) 偶极跃迁振子强度.
    DownLoad: CSV

    表 3  CaSH分子Ca—S键伸缩和CaSH弯曲振动模式的频率(cm–1)a)

    Table 3.  Frequencies of the Ca—S stretching and CaSH bending vibrational modes of the CaSH molecule (cm–1) a).

    $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} $ $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $ $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $
    (0, 1, 0) 316 (326) b) 315 (318) b) 331 (320) b) 326 (312) b)
    (0, 0, 1) 357 396 384 411
    (0, 2, 0) 634 632 661 653
    (0, 1, 1) 681 724 722 742
    (0, 0, 2) 704 785 760 808
    (0, 3, 0) 953 949 990 981
    (0, 2, 1) 1007 1051 1058 1074
    (0, 1, 2) 1034 1122 1102 1145
    (0, 0, 3) 1039 1167 1130 1188
    (0, 4, 0) 1271 1266 1318 1308
    注: a)(0, 1, 0)CaS 伸缩振动模式, (0, 0, 1)CaSH键角弯曲振动模式; b) 括号内值为实验值[23].
    DownLoad: CSV

    表 4  CaSH分子激发态$ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $, $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $和$ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $到基态$ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} $的跃迁FC因子

    Table 4.  The Frank-Condon factor of the excited states $ {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $, $ {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ and $ {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $ transition to ground state $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} $ of the CaSH molecule.

    $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} {\to} {\tilde{{\mathrm{A}}}}^{2}{{\mathrm{A}}}^{\prime} $ $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} {\to} {\tilde{{\mathrm{B}}}}^{2}{{\mathrm{A}}}^{\prime\prime} $ $ {\tilde{{\mathrm{X}}}}^{2}{{\mathrm{A}}}^{\prime} {\to} {\tilde{{\mathrm{C}}}}^{2}{{\mathrm{A}}}^{\prime} $
    (0, 0, 0) →
    (0, 0, 0)
    0.9268 0.9958 0.9248
    (0, 1, 0) →
    (0, 0, 0)
    0.0627 0.0011 0.0626
    (0, 0, 1) →
    (0, 0, 0)
    0.0094 0.0002 0.0114
    (0, 1, 1) →
    (0, 0, 0)
    0.0006 2.4×10–7 0.0008
    (0, 2, 0) →
    (0, 0, 0)
    0.0001 0.0006 2.2×10–5
    (0, 0, 2) →
    (0, 0, 0)
    6.0×10–5 0.0003 5×10–6
    DownLoad: CSV
    Baidu
  • [1]

    Balakrishnan N 2016 J. Chem. Phys. 145 150901Google Scholar

    [2]

    Wu Y, Bao W S, Cao S R, et al. 2021 Phys. Rev. Lett. 127 180501Google Scholar

    [3]

    Andreev V, Ang D G, Demille D, Doyle J M, Gabrielse G, Haefner J, Hutzler N R, Lasner Z, Meisenhelder C, O'Leary B R, Panda C D, West A D, West E P, Wu X 2018 Nature 562 355Google Scholar

    [4]

    Baron J, Campbell W C, DeMille D, Doyle J M, Gabrielse G, Gurevich Y V, Hess P W, Hutzler N R, Kirilov E, Kozyryev I, O’Leary B R, Panda C D, Parsons M F, Petrik E S, Spaun B, Vutha A C, West A D 2014 Science 343 269Google Scholar

    [5]

    Barry J F, Mccarron D J, Norrgard E B, Steinecker M H, Demille D 2014 Nature 512 286Google Scholar

    [6]

    Norrgard E B, McCarron D J, Steinecker M H, Tarbutt M R, DeMille D 2016 Phys. Rev. Lett. 116 063004Google Scholar

    [7]

    Truppe S, Williams H J, Fitch N J, Hambach M, Wall T E, Hinds E A, Sauer B E, Tarbutt M R 2017 New J. Phys. 19 022001Google Scholar

    [8]

    Kozyryev I, Baum L, Matsuda K, Augenbraun B L, Anderegg L, Sedlack A P, Doyle J M 2017 Phys. Rev. Lett. 118 173201Google Scholar

    [9]

    Augenbraun B L, Lasner Z D, Frenett A, Sawaoka H, Miller C, Steimle T C, Doyle J M 2020 New J. Phys. 22 022003Google Scholar

    [10]

    Baranov M A 2008 Phys. Rep. 464 71Google Scholar

    [11]

    Ni K K, Ospelkaus S, De Miranda M H, Hg M, Pe'Er A, Neyenhuis B, Zirbel J J, Kotochigova S, Julienne P S, Jin D S, Ye J 2008 Science 322 231Google Scholar

    [12]

    Shuman E S, Barry J F, DeMille D 2010 Nature 467 820Google Scholar

    [13]

    Hummon M T, Yeo M, Stuhl B K, Collopy A L, Xia Y, Ye J 2013 Phys. Rev. Lett. 110 143001Google Scholar

    [14]

    Zhelyazkova V, Cournol A, Wall T E, Matsushima A, Hudson J J, Hinds E, Tarbutt M, Sauer B 2014 Phys. Rev. A 89 053416Google Scholar

    [15]

    Gao Y, Wan M 2017 Phys. Chem. Chem. Phys. 19 5519Google Scholar

    [16]

    陈涛, 颜波 2019 68 043701Google Scholar

    Chen T, Yan B 2019 Acta Phys. Sin. 68 043701Google Scholar

    [17]

    Wells N, Lane I C 2011 Phys. Chem. Chem. Phys. 13 19018Google Scholar

    [18]

    Li D, Fu M, Ma H, Bian W, Du Z, Chen C A 2020 Front. Chem. 8 20

    [19]

    Li D, Cao J, Ma H, Bian W 2022 Phys. Chem. Chem. Phys. 24 10114

    [20]

    Ivanov M V, Bangerter F H, Krylov A I 2019 Phys. Chem. Chem. Phys. 21 19447Google Scholar

    [21]

    Augenbraun B L, Doyle J M, Zelevinsky T, Kozyryev I 2020 Phys. Rev. X 10 031022Google Scholar

    [22]

    Liu L, Yang C L, Sun Z P, Wang M S, Ma X G 2021 Phys. Chem. Chem. Phys. 23 2392Google Scholar

    [23]

    Fernando W T M L, Ram R S, O'Brien L C, Bernath P F 1991 J. Phys. Chem. 95 2665Google Scholar

    [24]

    Jarman C N, Bernath P F 1993 J. Chem. Phys. 98 6697Google Scholar

    [25]

    Ortiz J V 1990 Chem. Phys. Lett. 169 116Google Scholar

    [26]

    Scurlock C T, Henderson T, Bosely S, Jung K Y, Steimle T C 1994 J. Chem. Phys. 100 5481Google Scholar

    [27]

    Taleb-Bendiad A, Scappini F, Amano T, Watson J K 1996 J. Chem. Phys. 104 7431Google Scholar

    [28]

    Sheridan P M, Dick M J, Wang J G, Bernath P F 2007 Mol. Phys. 105 569Google Scholar

    [29]

    Nooijen M, Bartlett R J 1995 J. Chem. Phys. 102 3629Google Scholar

    [30]

    Pritchard B P, Altarawy D, Didier B T, Gibson T D, Windus T L 2019 J. Chem. Inf. Model. 59 4814Google Scholar

    [31]

    Koput J, Peterson K A 2002 J. Chem. Phys. 116 9255Google Scholar

    [32]

    Woon D E, Dunning T H 1995 J. Chem. Phys. 100 4572Google Scholar

    [33]

    Dunning T H 1989 J. Chem. Phys. 90 1007Google Scholar

    [34]

    Müller T, Dallos M, Lischka H, Dubrovay Z, Szalay P G 2001 Theor. Chem. Acc. 105 227Google Scholar

    [35]

    Lanczos C 1950 J. Res. Nat. Bur. Stand. 45 255Google Scholar

    [36]

    Goldfield E M, Gray S K, Harding L B 1993 J. Chem. Phys. 99 5812Google Scholar

    [37]

    Light J C, Carrington Jr T 2000 Adv. Chem. Phys. 114 263Google Scholar

    [38]

    Lill J V, Parker G A, Light J C 1986 J. Chem. Phys. 85 900Google Scholar

    [39]

    Liu W J, Hong Y G, Dai D D, Li L M, Dolg M 1997 Theor. Chem. Acc. 96 75Google Scholar

    [40]

    Zhang Y, Suo B B, Wang Z K, Zhang N, Li Z D, Lei Y B, Zou W L, Gao J, Peng D L, Pu Z C, Sun Q M, Wang F, Ma Y T, Wang X P, Liu W J 2020 J. Chem. Phys. 152 064113Google Scholar

    [41]

    Yang D D, Wang F, Guo J W 2012 Chem. Phys. Lett. 531 236Google Scholar

    [42]

    Tu Z Y, Wang F, Li X Y 2012 J. Chem. Phys. 136 174102Google Scholar

    [43]

    Wang Z F, Hu S, Wang F, Guo J W 2015 J. Chem. Phys. 142 144109Google Scholar

    [44]

    Cao Z L, Li Z D, Wang F, Liu W J 2017 Phys. Chem. Chem. Phys. 19 3713Google Scholar

    [45]

    李永红, 李俊峰, 王连宾, 张敬来 2008 河南大学学报(自然科学版) 38 4

    Li Y H, Li J F, Wang L B, Zhang J L 2008 J. Henan Univ. (Nat. Sci.) 38 4

    [46]

    Baum L, Vilas N B, Hallas C, Augenbraun B L, Raval S, Mitra D, Doyle J M 2020 Phys. Rev. Lett. 124 133201Google Scholar

    [47]

    Kozyryev I, Baum L, Aldridge L, Yu P, Eyler E E, Doyle J M 2018 Phys. Rev. Lett. 120 063205Google Scholar

    [48]

    Franck-Condon factors in the harmonic approximation , Wójcik P, Gozem S, Mozhayskiy V, Krylov A I. http:// iopenshell.usc.edu/downloads [2023-5-3

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  • supplement 2-20230742Suppl.pdf supplement
Metrics
  • Abstract views:  2207
  • PDF Downloads:  63
  • Cited By: 0
Publishing process
  • Received Date:  07 May 2023
  • Accepted Date:  16 September 2023
  • Available Online:  12 October 2023
  • Published Online:  20 January 2024

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