TY - JOUR
T1 - Experimental and theoretical studies on SiHn2+ dications (n = 1—5)
AU - Koch, Wolfram
AU - Frenking, Gernot
AU - Schwarz, Helmut
AU - Maquin, Francis
AU - Stahl, Daniel
PY - 1986
Y1 - 1986
N2 - Ab initio molecular orbital calculations, executed at the MP4/6-31 G∗∗//6-31 G∗ level, were performed for SiHn2+ dications (n = 1—5). In line with charge-stripping mass spectroscopic experiments both SiH2+ and SiH22+ are stable ions. Depending on the chemical precursor [i.e. Si(CH3)4 or SiH4] either the singlet ground state or the lowest triplet state of SiH+ are involved in the charge-stripping process. Moreover, electron impact ionization of SiH4 directly generates two stable states of SiH2+. For the system SiH2+-SiH22+, however, there is no experimental evidence for the involvement of excited states in the charge-stripping process. SiH32+ is also an experimentally accessible dication; however, the experimentally derived Qmin value and the theoretically predicted vertical ionization energy differ significantly for SiH32+, while they are in good to excellent agreement for SiH2+ and SiH22+, respectively. Owing to the lack of suitable cationic precursors no experimental data are available for SiH42+ and SiH52+. The calculations predict these species to be weakly bound complexes of SiH22+ and atomic and molecular hydrogen respectively.
AB - Ab initio molecular orbital calculations, executed at the MP4/6-31 G∗∗//6-31 G∗ level, were performed for SiHn2+ dications (n = 1—5). In line with charge-stripping mass spectroscopic experiments both SiH2+ and SiH22+ are stable ions. Depending on the chemical precursor [i.e. Si(CH3)4 or SiH4] either the singlet ground state or the lowest triplet state of SiH+ are involved in the charge-stripping process. Moreover, electron impact ionization of SiH4 directly generates two stable states of SiH2+. For the system SiH2+-SiH22+, however, there is no experimental evidence for the involvement of excited states in the charge-stripping process. SiH32+ is also an experimentally accessible dication; however, the experimentally derived Qmin value and the theoretically predicted vertical ionization energy differ significantly for SiH32+, while they are in good to excellent agreement for SiH2+ and SiH22+, respectively. Owing to the lack of suitable cationic precursors no experimental data are available for SiH42+ and SiH52+. The calculations predict these species to be weakly bound complexes of SiH22+ and atomic and molecular hydrogen respectively.
UR - http://www.scopus.com/inward/record.url?scp=37049090980&partnerID=8YFLogxK
U2 - 10.1039/P29860000757
DO - 10.1039/P29860000757
M3 - 文章
AN - SCOPUS:37049090980
SN - 1472-779X
SP - 757
EP - 760
JO - Journal of the Chemical Society, Perkin Transactions 2
JF - Journal of the Chemical Society, Perkin Transactions 2
IS - 5
ER -