2020
DOI: 10.1039/d0cp04787b
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Electron spectroscopy and dynamics of HBr around the Br 1s−1 threshold

Abstract: A comprehensive electron spectroscopic study combined with partial electron yield measurements around the Br 1s ionization threshold of HBr at ≅13.482 keV is reported.

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Cited by 6 publications
(5 citation statements)
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“…To calibrate the energies of the incident x-rays precisely, ion yields were recorded across the Br and I Kedges. The 4p 5 configuration of atomic Br results in strong 1s → 4pσ * pre-edge resonances in the Br K -shell x-ray absorption spectra of Br 2 [28], CF 3 Br [29], and HBr [26]. The 4pσ * resonance in the ion yield scan of IBr was recorded at ∼13474 eV, which is 2 eV lower than the resonance energy in CF 3 Br [29] and ∼1 eV higher than the resonance energy in Br 2 [28].…”
Section: B X-ray Energiesmentioning
confidence: 92%
See 1 more Smart Citation
“…To calibrate the energies of the incident x-rays precisely, ion yields were recorded across the Br and I Kedges. The 4p 5 configuration of atomic Br results in strong 1s → 4pσ * pre-edge resonances in the Br K -shell x-ray absorption spectra of Br 2 [28], CF 3 Br [29], and HBr [26]. The 4pσ * resonance in the ion yield scan of IBr was recorded at ∼13474 eV, which is 2 eV lower than the resonance energy in CF 3 Br [29] and ∼1 eV higher than the resonance energy in Br 2 [28].…”
Section: B X-ray Energiesmentioning
confidence: 92%
“…These high-order corrections were included in the same way as our previous calculations on Kr, Xe, and XeF 2 [5]. The calculated Br 1s ionization energy is 1.5 eV lower than the photoelectron measurement on HBr [26] and the calculated I 1s energy is 1.4 eV higher than the measurement on CH 3 I [27]. The 1s ionization energies of IBr were not directly measured in the present work but are expected to be within 1-2 eV of the calculated energies listed in Table I.…”
Section: A Calculated Ionization Energiesmentioning
confidence: 99%
“…In addition to excitation energies, 1s core‐ionization potentials for the molecules of the Tozer‐II test set as well as for the HBr molecule were calculated, resulting in a total of 18 values. Experimental reference values have been taken from the literature (see Table S5 in Supporting Information for details) 87‐96 . In particular, we obtained 1s core ionization potentials as minus the 1s core orbital energies, which have been taken directly from the relativistic ground‐state DFT calculations required to compute the relativistic corrections for the 1s core excitation energies.…”
Section: Computational Detailsmentioning
confidence: 99%
“…S5 in Supporting Information for details). [87][88][89][90][91][92][93][94][95][96] In particular, we obtained 1s core ionization potentials as minus the 1s core orbital energies, which have been taken directly from the relativistic ground-state DFT calculations required to compute the relativistic corrections for the 1s core excitation energies. Accordingly, results…”
Section: Computational Settingsmentioning
confidence: 99%
“…In the last few years also very deep core holes such as the K shells of Br [9], Kr [10], I [11], and Xe [12] became accessible for high-resolution spectroscopy. A recent review with more details on these topics has been published by Piancastelli et al [13].…”
Section: Introductionmentioning
confidence: 99%