## X-ray emission spectra of S Kb, S and O Ka for sulfur dioxide were calculated by the discrete variational Xa L 2, 3 (DV-Xa) method. The absolute energies of the peaks in the theoretical spectra agree with the experimental values within an error of 3% . The relative energies and intensities of p
Calculation of B K–V x-ray emission spectra of boron nitrides
✍ Scribed by Takahiro Kaneyoshi; Hidenori Kohzuki; Yasuji Muramatsu; Yoshiyuki Kowada; Jun Kawai; Muneyuki Motoyama
- Publisher
- John Wiley and Sons
- Year
- 1999
- Tongue
- English
- Weight
- 148 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0049-8246
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✦ Synopsis
The DV-Xa molecular orbital (MO) calculation method was applied to the B K-V x-ray emission spectra of hexagonal (h-), cubic (c-) and wurtzite (w -) type boron nitrides (BN). The calculated B 2p density of states (DOS) was in good agreement with the B K-V x-ray emission. The main peaks and low-energy satellite peaks in the B K-V x-ray emission spectra are due to the B 2p and the B 2p hybridized with N 2s, respectively. The high-energy satellite peak in the B K-V x-ray emission spectra clearly corresponds to the p * sub-band of the B 2p DOS in h-BN. However, the high-energy satellite peak observed in w -BN is not in agreement with the B 2p DOS. It is considered that the high-energy satellite peaks are due to less than four-coordinated B atoms such as have dangling bonds and defects in w -BN. In the B K-V x-ray emission spectra of h-BN, the synthesizing p and s sub-bands of B 2p DOS could explain the polarized emission spectra very well.
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