1984
DOI: 10.1016/0009-2614(84)85332-4
|View full text |Cite
|
Sign up to set email alerts
|

The x-ray emission spectrum of gaseous ethene

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

1
6
0

Year Published

1986
1986
2022
2022

Publication Types

Select...
6
1

Relationship

0
7

Authors

Journals

citations
Cited by 8 publications
(7 citation statements)
references
References 12 publications
1
6
0
Order By: Relevance
“…The series of lower energy emission lines were then attributed to transitions from the HOMO − 1 to HOMO − 4 to the same 1s energy level, with an energy progression that was approximately consistent with the valence energy level spacing reported by ultraviolet photoelectron spectroscopy [68]. The DFT-ROCIS calculations in this work (figure 4(a)) suggest that while the initial state for the four highest energy (Brammer, 1984) with NXES spectra upon 312.0 eV excitation of ethylene [44]. The literature data has been shifted to match the energy calibration in this work.…”
Section: Non-resonant X-ray Emissionsupporting
confidence: 82%
See 3 more Smart Citations
“…The series of lower energy emission lines were then attributed to transitions from the HOMO − 1 to HOMO − 4 to the same 1s energy level, with an energy progression that was approximately consistent with the valence energy level spacing reported by ultraviolet photoelectron spectroscopy [68]. The DFT-ROCIS calculations in this work (figure 4(a)) suggest that while the initial state for the four highest energy (Brammer, 1984) with NXES spectra upon 312.0 eV excitation of ethylene [44]. The literature data has been shifted to match the energy calibration in this work.…”
Section: Non-resonant X-ray Emissionsupporting
confidence: 82%
“…For ethylene, the symmetries of the four highest energy occupied orbitals are as follows: (2b 2u ) 2 (3a g ) 2 (1b 3g ) 2 (1b 3u ) 2 (see figure S1). In the previous EI study [44], the highest energy intense emission band was assigned to emission from the HOMO (1b 3u ) 2 to a hole formed in the 1s orbital following EI ionization. The series of lower energy emission lines were then attributed to transitions from the HOMO − 1 to HOMO − 4 to the same 1s energy level, with an energy progression that was approximately consistent with the valence energy level spacing reported by ultraviolet photoelectron spectroscopy [68].…”
Section: Non-resonant X-ray Emissionmentioning
confidence: 93%
See 2 more Smart Citations
“…This seems also to hold for core-electron spectroscopies for which, in addition to shake-up, [9][10][11] one can find experimental and theoretical work for near-edge x-ray-absorption fine-structure spectra ͑NEXAFS͒, 5,12,13 x-ray emission, [14][15][16][17] and photoelectron shifts. 18,19 The x-ray photoelectron shake-up spectra have been presented in high resolution for the three first members of the polyene seriesethylene, butadiene, and hexatriene-in Refs.…”
Section: Shake-up Spectra Of Short Polyenesmentioning
confidence: 98%