Theoretical study of transition spectra of TiO molecule
被引:1
|
作者:
Cheng, Junxia
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h-index: 0
机构:
Xian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R ChinaXian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R China
Cheng, Junxia
[1
]
Zhang, Hong
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机构:
Sichuan Univ, Coll Phys, Chengdu 610065, Peoples R ChinaXian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R China
Zhang, Hong
[2
]
Cheng, Xinlu
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机构:
Sichuan Univ, Minist Educ, Key Lab High Energy Dens Phys & Technol, Chengdu 610065, Peoples R ChinaXian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R China
Cheng, Xinlu
[3
]
Wang, Jia
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机构:
Xian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R ChinaXian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R China
Wang, Jia
[1
]
Wu, Shenjiang
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h-index: 0
机构:
Xian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R ChinaXian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R China
Wu, Shenjiang
[1
]
机构:
[1] Xian Technol Univ, Sch Photoelect Engn, Xian 710021, Peoples R China
[2] Sichuan Univ, Coll Phys, Chengdu 610065, Peoples R China
[3] Sichuan Univ, Minist Educ, Key Lab High Energy Dens Phys & Technol, Chengdu 610065, Peoples R China
Ab initio;
TiO molecule;
Excited state;
Transition dipole moments;
Spectroscopy;
BAND OSCILLATOR-STRENGTHS;
DELTA-SYSTEM;
BASIS-SETS;
HOT;
SPECTROSCOPY;
ATMOSPHERES;
STATES;
(1)PI;
D O I:
10.1016/j.jms.2020.111325
中图分类号:
O64 [物理化学(理论化学)、化学物理学];
O56 [分子物理学、原子物理学];
学科分类号:
070203 ;
070304 ;
081704 ;
1406 ;
摘要:
The transitional characters for eight transition systems of TiO were investigated by using the ab initio calculation. Highly accurate MRCI + Q approach was used to investigate the potential energy curves (PECs) and transition dipole moment curves (TDMCs) with 4221 levels that results are consisted with experimental determinations. Moreover, combining the values of PECs with TDMCs, the Einstein A coefficients, transitional lifetimes, ro-vibrational intensities, absorption oscillator strengths, and frequency-integrated cross sections are calculated including transition bands v' = 0-6 <- v '' = 0-6. For application in the atmospheres, the absolute intensities and line-shapes of allowed transition systems at different temperature were studied to satisfy some astrophysical applications. The results are also potentially useful for important Astrophysics Data System (ADS) and databases such as HITEMP, NIST. Since the results from many laboratory techniques and our calculations now agree, analyses of TiO based on absorption from allowed transitions are no longer hindered by present determinations. (C) 2020 Elsevier Inc. All rights reserved.