2015
DOI: 10.1016/j.jms.2014.11.004
|View full text |Cite
|
Sign up to set email alerts
|

Fourier-transform microwave spectroscopy of an alkyl substituted Criegee intermediate anti-CH3CHOO

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

1
41
1

Year Published

2015
2015
2021
2021

Publication Types

Select...
6
1
1

Relationship

1
7

Authors

Journals

citations
Cited by 39 publications
(44 citation statements)
references
References 41 publications
1
41
1
Order By: Relevance
“…As shown in previous studies of alkyl-substituted Criegee intermediates, such as CH 3 CHOO, 14,39 C 2 H 5 CHOO 25 and (CH 3 ) 2 CHCHOO 26 the syn conformers are predicted to be the preferred configurations. This major stability can be ascribed to the attractive interaction between the terminal oxygen atom and the protons of the closer carbon atom of the alkyl moiety.…”
Section: Discussionsupporting
confidence: 53%
“…As shown in previous studies of alkyl-substituted Criegee intermediates, such as CH 3 CHOO, 14,39 C 2 H 5 CHOO 25 and (CH 3 ) 2 CHCHOO 26 the syn conformers are predicted to be the preferred configurations. This major stability can be ascribed to the attractive interaction between the terminal oxygen atom and the protons of the closer carbon atom of the alkyl moiety.…”
Section: Discussionsupporting
confidence: 53%
“…48 Nakajima and Endo detected also the microwave spectra of alkyl-substituted Criegee intermediate syn-CH 3 CHOO 27 and anti-CH 3 CHOO. 29 The observed pure rotational transitions show a small splitting corresponding to the A/E components due to the threefold methyl internal rotation (torsion). The structure and rotational parameters were evaluated, and the barrier heights, V 3 = 837.1 and 399.1 cm .…”
Section: Larger Criegee Intermediatesmentioning
confidence: 98%
“…After the discovery of this source of CH 2 OO, many researchers utilized this scheme to produce CH 2 OO and reported ultraviolet (UV) depletion, 18 UV absorption, 19,20 infrared (IR) absorption, 21 microwave, 22,23 and submillimeter-wave 24 spectra. Spectra of slightly larger Criegee intermediates such as acetaldehyde oxide (CH 3 CHOO), 15,[25][26][27][28][29][30][31][32] acetone oxide [(CH 3 ) 2 COO], 16,33 and propionaldehyde oxide (C 2 H 5 CHOO) 10 are also reported. Figure 1 shows the structures of CH 2 OO, syn-CH 3 CHOO, and anti-CH 3 CHOO.…”
Section: Spectroscopy Of Criegee Intermediatesmentioning
confidence: 99%
See 1 more Smart Citation
“…After this pioneering work, the same method has been applied for generation of other CIs, like CH 3 CHOO (Taatjes et al, 2013), (CH 3 ) 2 COO (Liu et al, 2014a) and methyl vinyl ketone oxide (MVKO) (Barber et al, 2018), methacrolein oxide (MACRO) (Vansco et al, 2019), etc. These CIs have been identified with various detection methods, like photoionization mass spectrometry (Taatjes et al, 2013), infrared action (Liu et al, 2014b) and absorption Lin et al, 2015) spectroscopy, UV-visible spectroscopy (Beames et al, 2013;Sheps, 2013;Liu et al, 2014a;Ting et al, 2014;Smith et al, 40 2014;Chang et al, 2016), microwave spectroscopy (McCarthy et al, 2013;Nakajima et al, 2015), etc. In addition, utilizing the direct detection of CIs, a number of kinetic investigations of CI reactions, e.g., with SO 2 (Huang et al, 2015), water vapor (Chao et al, 2015), alcohols (Chao et al, 2019), thiols (Li et al, 2019), amines (Chhantyal-Pun et al, 2019), carbonyl molecules (Taatjes et al, 2012), and organic (Welz et al, 2014) and inorganic (Foreman et al, 2016) acids, etc., have been reported (Lee, 2015;Osborn and Taatjes, 2015;Lin and Chao, 2017;Khan et al, 2018).…”
Section: Ch I → Ch I I ( R 1 )mentioning
confidence: 99%