1962
DOI: 10.1021/j100807a035
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ELECTRON IMPACT SPECTROSCOPY OF TETRAMETHYLGERMANIUM, TRIMETHYLSILANE AND DIMETHYLMERCURY1

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Cited by 41 publications
(5 citation statements)
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“…As far as mass 58 amu is concerned, the corresponding electron energy scan is shown in figure 10: two contributions can be observed, one with an appearance energy of 8.3±0.3 eV, which is not present when a shutter prevents the plasma beam from reaching the MS housing, and the other with an appearance energy of 10.2 ± 0.3 eV, whose intensity is not affected by the shutter insertion. According to the literature, the latter can be attributed to the Me 2 Si + originating from the dissociative ionization of Me 3 SiH [61] and Me 2 SiH 2 [62] molecules in the MS. The early appearance energy can be associated with a radical, SiMe 2 , or with the molecule, OSi=CH 2 .…”
Section: Ion-electron Dissociative Recombination Routesmentioning
confidence: 96%
“…As far as mass 58 amu is concerned, the corresponding electron energy scan is shown in figure 10: two contributions can be observed, one with an appearance energy of 8.3±0.3 eV, which is not present when a shutter prevents the plasma beam from reaching the MS housing, and the other with an appearance energy of 10.2 ± 0.3 eV, whose intensity is not affected by the shutter insertion. According to the literature, the latter can be attributed to the Me 2 Si + originating from the dissociative ionization of Me 3 SiH [61] and Me 2 SiH 2 [62] molecules in the MS. The early appearance energy can be associated with a radical, SiMe 2 , or with the molecule, OSi=CH 2 .…”
Section: Ion-electron Dissociative Recombination Routesmentioning
confidence: 96%
“…The possible presence of CH 3 HgCH 3 was ruled out due to the absence of CH 3 Hg 1 cluster. 30 However, the low levels of the mercury preclude unambiguous identification in such a manner. The natural occurrence of CH 3 HgH in the head space of B. juncea appears to be unlikely as it is an intermediate (half-life of approximately 2 h) in the reduction reaction (by means of NaBH 4 ) of alkylmercury species to elemental mercury.…”
Section: Volatile Forms Of Mercury and Seleniummentioning
confidence: 99%
“…Theory predicts that silyl cations are stable, even more so than analogous carbocations, because of the larger size, polarizability, and electropositivity of silicon (2). Moreover, such species have been studied thoroughly in the gas phase (3), and recent studies have provided evidence for their existence as reactive intermediates (4). Many reports of direct observation of stable, long-lived silyl cations in condensed phase have been flawed (5) and continue to be controversial (6)(7)(8).…”
mentioning
confidence: 99%