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Internally contracted multireference configuration interaction (icMRCI) calculations of the ground state (X 3 R 2 ), the first excited state (a 1 D) as well as the second excited state (b 1 R 1 ) have been performed for a series of halogenated nitrenes NXs (X 5 Cl, Br, and I). Accurate spectroscopic constants of these lowest three electronic states of each NX were obtained in this work using MRCI methods with aug-cc-pVXZ (X 5 T, Q, 5) basis sets and complete basis set (CBS) limit. In addition, various corrections, including the Davidson correction, scalar relativistic effect, corevalence correlation, and spin-orbit coupling effect, have been studied in calculating spectroscopic constants, especially for heavy-atom nitrenes. Comparisons have been made with previous computational and experimental results where available. The icMRCI 1 Q calculations presented in this work provide a comprehensive series of results at a consistent high level of theory for all of the halogenated nitrenes. K E Y W O R D Score-valence correlation, icMRCI1Q, nitrenes, scalar relativistic effect, spectroscopic constants, spin-orbit coupling effect 1 | I N TR ODU C TI ON Halogenated nitrenes NXs (X 5 F, Cl, Br, I) are sextet, neutral, and highly reactive molecular species where the nitrogen atom shows a monovalent nature. Derived from the photochemical process of the halogen azides XN 3 !N 2 1 NX (X 5 F, Cl, Br, I), [1][2][3] the radical NXs play an important photochemical role in the upper atmosphere and interstellar space because of their relatively high contents of the constituent elements in the space. [4,5] Halogenated nitrenes are also expected to be a possible candidate for the application in chemical energy storage sources since there exists two metastable excited states, a 1 D and b 1 R 1 of NXs. [6][7][8] Particularly, the a 1 D state of NF or NCl could be used for pumping the 2 P 1/2 -2 P 3/2 transition of atomic iodine in a successful demonstration of an efficient chemical laser. [9][10][11][12][13] Accurate spectroscopic information about these low-lying electronic states is essential to understand the dynamics and kinetics of chemical processes involving halogenated nitrenes.As analogs to halogenated carbenes, the two unpaired electrons of NX can couple either as a singlet or triplet state very close in energy. Being iso-valent with O 2 , all halogenated nitrenes studied to date have a triplet ground state of X 3 R 2 . The two low-lying excited singlet states, a 1 D and b 1 R 1 , resulting from the same electron configuration (p 4 p* 2 ), could exhibit quite different reactivity comparing to the triplet ground electronic state.The spectroscopy of these low-lying states, the singlet-triplet energy splitting, as well as their reactivity, has been the subject of a myriad of investigations in the literature. [14] The spectroscopic study of NXs could date back to more than 70 years ago when the emission spectrum of NBr (later assigned to the b 1 R 1 -X 3 R 2 transition [15] ) was first observed by Elliott. [16] After that, the stru...
Internally contracted multireference configuration interaction (icMRCI) calculations of the ground state (X 3 R 2 ), the first excited state (a 1 D) as well as the second excited state (b 1 R 1 ) have been performed for a series of halogenated nitrenes NXs (X 5 Cl, Br, and I). Accurate spectroscopic constants of these lowest three electronic states of each NX were obtained in this work using MRCI methods with aug-cc-pVXZ (X 5 T, Q, 5) basis sets and complete basis set (CBS) limit. In addition, various corrections, including the Davidson correction, scalar relativistic effect, corevalence correlation, and spin-orbit coupling effect, have been studied in calculating spectroscopic constants, especially for heavy-atom nitrenes. Comparisons have been made with previous computational and experimental results where available. The icMRCI 1 Q calculations presented in this work provide a comprehensive series of results at a consistent high level of theory for all of the halogenated nitrenes. K E Y W O R D Score-valence correlation, icMRCI1Q, nitrenes, scalar relativistic effect, spectroscopic constants, spin-orbit coupling effect 1 | I N TR ODU C TI ON Halogenated nitrenes NXs (X 5 F, Cl, Br, I) are sextet, neutral, and highly reactive molecular species where the nitrogen atom shows a monovalent nature. Derived from the photochemical process of the halogen azides XN 3 !N 2 1 NX (X 5 F, Cl, Br, I), [1][2][3] the radical NXs play an important photochemical role in the upper atmosphere and interstellar space because of their relatively high contents of the constituent elements in the space. [4,5] Halogenated nitrenes are also expected to be a possible candidate for the application in chemical energy storage sources since there exists two metastable excited states, a 1 D and b 1 R 1 of NXs. [6][7][8] Particularly, the a 1 D state of NF or NCl could be used for pumping the 2 P 1/2 -2 P 3/2 transition of atomic iodine in a successful demonstration of an efficient chemical laser. [9][10][11][12][13] Accurate spectroscopic information about these low-lying electronic states is essential to understand the dynamics and kinetics of chemical processes involving halogenated nitrenes.As analogs to halogenated carbenes, the two unpaired electrons of NX can couple either as a singlet or triplet state very close in energy. Being iso-valent with O 2 , all halogenated nitrenes studied to date have a triplet ground state of X 3 R 2 . The two low-lying excited singlet states, a 1 D and b 1 R 1 , resulting from the same electron configuration (p 4 p* 2 ), could exhibit quite different reactivity comparing to the triplet ground electronic state.The spectroscopy of these low-lying states, the singlet-triplet energy splitting, as well as their reactivity, has been the subject of a myriad of investigations in the literature. [14] The spectroscopic study of NXs could date back to more than 70 years ago when the emission spectrum of NBr (later assigned to the b 1 R 1 -X 3 R 2 transition [15] ) was first observed by Elliott. [16] After that, the stru...
The thermochemistry of halocarbon species containing iodine and bromine is examined through an extensive interplay between new Feller−Peterson− Dixon (FPD) style composite methods and a detailed analysis of all available experimental and theoretical determinations using the thermochemical network that underlies the Active Thermochemical Tables (ATcT). From the computational viewpoint, a slower convergence of the components of composite thermochemistry methods is observed relative to species that solely contain first row elements, leading to a higher computational expense for achieving comparable levels of accuracy. Potential systematic sources of computational uncertainty are investigated, and, not surprisingly, spin-orbit coupling is found to be a critical component, particularly for iodine containing molecular species. The ATcT analysis of available experimental and theoretical determinations indicates that prior theoretical determinations have significantly larger uncertainties than originally reported, particularly in cases where molecular spin-orbit effects were ignored. Accurate and reliable heats of formation are reported for 38 halogen containing systems, based on combining the current computations with previous experimental and theoretical work via the ATcT approach.
We present herein a high-level ab initio study on the mono-iodine substituted carbene, CHI, using internally contracted multireference configuration interaction (icMRCI-F12) with Davidson correction which employs wave functions that explicitly depend on the electron-electron distance. The spin-orbit coupling (SOC) effect was included in our calculations. A total of 20 spin-free states with vertical transition energy up to 7.4 eV, as well as 50 spin-coupled states generated from the spin-free states via the SOC were studied. The results show significant influence of the SOC on the bond angles and the harmonic vibrational frequencies of the bending mode of the ground state (XA') and the lowest triplet state (aA''). Potential energy curves along the bond angle and the bond lengths of the electronic excited states of CHI were investigated. Based on our calculations, photodissociation dynamics in the ultraviolet region was disscussed for the first time, which would pave the way to further experimental investigations of CHI.
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