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The 18 -S states correlated to the lowest dissociation (Si(3Pg)+S(3Pg)) limit are computed with high-level multireference configuration interaction (MRCI(SD)) approach through utilizing all-electron aug-cc-pwCVQZ-DK basis set. The scalar relativistic effect and the core-valence correlation effect of Si (2s22p6) and S (2s22p6) are taken into account. On the basis of calculated potential energy curves, the spectroscopic constants of the bound states are fitted, including equilibrium distance Re, adiabatic transition energies Te, harmonic vibrational frequencies e, anharmonic terms exe, and rotational constant Be. The electronic configurations at different bond lengths are given. The electronic dipole moments of 18 -S states are calculated, illuminating the influence of electronic configuration variation on electronic dipole moment. With the help of nonvanishing spin-orbit matrix elements including b3 and A1 as a function of the internuclear distance, the nearby state perturbations to b3 and A1 are discussed in detail. Finally, the transition dipole moments and Franck-Condon factors of A1X1+ and E1+X1+ transitions are obtained, and radiative lifetimes of five lowest vibrational levels of the two singlet excited states are evaluated.
[1] Yan B, Pan S F, Wang Z G, Yu J H 2006 Acta Phys. Sin. 55 1736 (in Chinese)[闫冰, 潘守甫, 王志刚, 于俊华 2006 55 1736]
[2] Yan B, Pan S F 2008 Chin. Phys. B 17 1501
[3] Yan B, Zhang Y J 2013 Chin. Phys. B 22 023103
[4] Gao X Y, You K, Zhang X M, Liu Y L, Liu Y F 2013 Acta Phys. Sin. 62 233302 (in Chinese)[高雪艳, 尤凯, 张晓美, 刘彦磊, 刘玉芳 2013 62 233302]
[5] Glassgold A E 1996 Annu. Rev. Astron. Astrophys. 34 241
[6] Ziurys L M 2006 Proc. Natl. Acad. Sci. 103 12274
[7] Woodall J, Agúndez M, Markwick-Kemper A J, Millar T J 2007 Astron. Astrophys. 466 1197
[8] Barrow R F, Jevons W 1938 Proc. R. Soc. A: Math. Phys. Eng. Sci. 169 45
[9] Robinson S J Q, Barrow R F 1954 Proc. Phys. Soc. Sect. A 67 95
[10] Nilheden G 1956 Ark. Fys. 10 19
[11] Bredohl H, Cornet R, Dubois I, Wilderia D 1975 J. Phys. B At. Mol. Phys. 8 259
[12] Katti P H, Korwar V M 1975 Acta Phys. Acad. Sci. Hung. 39 145
[13] Linton C 1980 J. Mol. Spectrosc. 80 279
[14] Harris S M, Gottscho R A, Field R W, Barrow R F 1982 J. Mol. Spectrosc. 91 35
[15] Sanz M E, McCarthy M C, Thaddeus P 2003 J. Chem. Phys. 119 11715
[16] Mller H S P, McCarthy M C, Bizzocchi L, Gupta H, Esser S, Lichau H, Caris M, Lewen F, Hahn J, Degli Esposti C, Schlemmer S, Thaddeus P 2007 Phys. Chem. Chem. Phys. 9 1579
[17] Li S, Moncrieff D, Zhao J, Brown F B 1988 Chem. Phys. Lett. 151 403
[18] Chattopadhyaya S, Chattopadhyay A, Das K K 2002 J. Phys. Chem. A 106 833
[19] Coriani S, Marchesan D, Gauss J, Hättig C, Helgaker T, J ørgensen P 2005 J. Chem. Phys. 123 184107
[20] Li C, Deng L, Zhang Y, Wu L, Yang X, Chen Y 2011 J. Phys. Chem. A 115 2978
[21] Li R, Wei C L, Sun Q X, Sun E P, Xu H F, Yan B 2013 J. Phys. Chem. A 117 2373
[22] Werner H J, Knowles P J, Knizia G, Manby F R, Schtz M, Celani P, Korona T, Lindh R, Mitrushenkov A, Rauhut G, Shamasundar K R, Adler T B, Amos R D, Bernhardsson A, Berning A, Cooper D L, Deegan M J O, Dobbyn A J, Eckert F, Goll E, Hampel C, Hesselmann A, Hetzer G, Hrenar T, Jansen G, Köppl C, Liu Y, Lloyd A W, Mata R A, May A J, McNicholas S J, Meyer W, Mura M E, Nicklass A, Neill D P, Palmieri P, Peng D, Pflger K, Pitzer R, Reiher M, Shiozaki T, Stoll H, Stone A J, Tarroni R, Thorsteinsson T, Wang M 2010 MOLPRO: a package of ab initio programs
[23] Woon D E, Dunning T H 1993 J. Chem. Phys. 98 1358
[24] Werner H J, Knowles P J 1985 J. Chem. Phys. 82 5053
[25] Knowles P J, Werner H J 1985 Chem. Phys. Lett. 115 259
[26] Werner H J, Knowles P J 1988 J. Chem. Phys. 89 5803
[27] Knowles P J, Werner H J 1988 Chem. Phys. Lett. 145 514
[28] Langhoff S R, Davidson E R 1974 Int. J. Quantum Chem. 8 61
[29] Douglas M, Kroll N M 1974 Ann. Phys. 82 89
[30] Hess B A 1986 Phys. Rev. A 33 3742
[31] Berning A, Schweizer M, Werner H J, Knowles P J, Palmieri P 2000 Mol. Phys. 98 1823
[32] Le Roy R J 2002 LEVEL 7.5: a Computer Program for Solving the Radial Schröinger Equation for Bound and Quasibound Levels (University of Waterloo, Chemical Physics Research Report CP-655)
[33] Huber K P, Herzberg G 1979 Molecular Spectra and Molecular Structure IV: Constants of Diatomic Molecules (New York: Van Nostrand Reinhold) pp608-609
[34] Green G J, Gole J L 1980 Chem. Phys. 46 67
[35] Murty A N, Curl Jr. R F 1969 J. Mol. Spectrosc. 30 102
[36] Sunanda K, Gopal S, Shetty B J, Lakshminarayana G 1989 J. Quant. Spectrosc. Radiat. Transf. 42 631
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[1] Yan B, Pan S F, Wang Z G, Yu J H 2006 Acta Phys. Sin. 55 1736 (in Chinese)[闫冰, 潘守甫, 王志刚, 于俊华 2006 55 1736]
[2] Yan B, Pan S F 2008 Chin. Phys. B 17 1501
[3] Yan B, Zhang Y J 2013 Chin. Phys. B 22 023103
[4] Gao X Y, You K, Zhang X M, Liu Y L, Liu Y F 2013 Acta Phys. Sin. 62 233302 (in Chinese)[高雪艳, 尤凯, 张晓美, 刘彦磊, 刘玉芳 2013 62 233302]
[5] Glassgold A E 1996 Annu. Rev. Astron. Astrophys. 34 241
[6] Ziurys L M 2006 Proc. Natl. Acad. Sci. 103 12274
[7] Woodall J, Agúndez M, Markwick-Kemper A J, Millar T J 2007 Astron. Astrophys. 466 1197
[8] Barrow R F, Jevons W 1938 Proc. R. Soc. A: Math. Phys. Eng. Sci. 169 45
[9] Robinson S J Q, Barrow R F 1954 Proc. Phys. Soc. Sect. A 67 95
[10] Nilheden G 1956 Ark. Fys. 10 19
[11] Bredohl H, Cornet R, Dubois I, Wilderia D 1975 J. Phys. B At. Mol. Phys. 8 259
[12] Katti P H, Korwar V M 1975 Acta Phys. Acad. Sci. Hung. 39 145
[13] Linton C 1980 J. Mol. Spectrosc. 80 279
[14] Harris S M, Gottscho R A, Field R W, Barrow R F 1982 J. Mol. Spectrosc. 91 35
[15] Sanz M E, McCarthy M C, Thaddeus P 2003 J. Chem. Phys. 119 11715
[16] Mller H S P, McCarthy M C, Bizzocchi L, Gupta H, Esser S, Lichau H, Caris M, Lewen F, Hahn J, Degli Esposti C, Schlemmer S, Thaddeus P 2007 Phys. Chem. Chem. Phys. 9 1579
[17] Li S, Moncrieff D, Zhao J, Brown F B 1988 Chem. Phys. Lett. 151 403
[18] Chattopadhyaya S, Chattopadhyay A, Das K K 2002 J. Phys. Chem. A 106 833
[19] Coriani S, Marchesan D, Gauss J, Hättig C, Helgaker T, J ørgensen P 2005 J. Chem. Phys. 123 184107
[20] Li C, Deng L, Zhang Y, Wu L, Yang X, Chen Y 2011 J. Phys. Chem. A 115 2978
[21] Li R, Wei C L, Sun Q X, Sun E P, Xu H F, Yan B 2013 J. Phys. Chem. A 117 2373
[22] Werner H J, Knowles P J, Knizia G, Manby F R, Schtz M, Celani P, Korona T, Lindh R, Mitrushenkov A, Rauhut G, Shamasundar K R, Adler T B, Amos R D, Bernhardsson A, Berning A, Cooper D L, Deegan M J O, Dobbyn A J, Eckert F, Goll E, Hampel C, Hesselmann A, Hetzer G, Hrenar T, Jansen G, Köppl C, Liu Y, Lloyd A W, Mata R A, May A J, McNicholas S J, Meyer W, Mura M E, Nicklass A, Neill D P, Palmieri P, Peng D, Pflger K, Pitzer R, Reiher M, Shiozaki T, Stoll H, Stone A J, Tarroni R, Thorsteinsson T, Wang M 2010 MOLPRO: a package of ab initio programs
[23] Woon D E, Dunning T H 1993 J. Chem. Phys. 98 1358
[24] Werner H J, Knowles P J 1985 J. Chem. Phys. 82 5053
[25] Knowles P J, Werner H J 1985 Chem. Phys. Lett. 115 259
[26] Werner H J, Knowles P J 1988 J. Chem. Phys. 89 5803
[27] Knowles P J, Werner H J 1988 Chem. Phys. Lett. 145 514
[28] Langhoff S R, Davidson E R 1974 Int. J. Quantum Chem. 8 61
[29] Douglas M, Kroll N M 1974 Ann. Phys. 82 89
[30] Hess B A 1986 Phys. Rev. A 33 3742
[31] Berning A, Schweizer M, Werner H J, Knowles P J, Palmieri P 2000 Mol. Phys. 98 1823
[32] Le Roy R J 2002 LEVEL 7.5: a Computer Program for Solving the Radial Schröinger Equation for Bound and Quasibound Levels (University of Waterloo, Chemical Physics Research Report CP-655)
[33] Huber K P, Herzberg G 1979 Molecular Spectra and Molecular Structure IV: Constants of Diatomic Molecules (New York: Van Nostrand Reinhold) pp608-609
[34] Green G J, Gole J L 1980 Chem. Phys. 46 67
[35] Murty A N, Curl Jr. R F 1969 J. Mol. Spectrosc. 30 102
[36] Sunanda K, Gopal S, Shetty B J, Lakshminarayana G 1989 J. Quant. Spectrosc. Radiat. Transf. 42 631
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