1981
DOI: 10.1103/physrevb.24.3537
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Core excitons at the boronKedge in hexagonal BN

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Cited by 52 publications
(26 citation statements)
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“…This identification of a Y 10 -type exciton is consistent with the fact that boron atoms sit only at sites with reflection symmetry about the a-b basal plane, which demands that each final state be an eigenstate of the corresponding reflection parity 22 . For a predominantly Y 10 -type exciton, other possible higher-order Y lm components must possess the same reflection parity.…”
supporting
confidence: 73%
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“…This identification of a Y 10 -type exciton is consistent with the fact that boron atoms sit only at sites with reflection symmetry about the a-b basal plane, which demands that each final state be an eigenstate of the corresponding reflection parity 22 . For a predominantly Y 10 -type exciton, other possible higher-order Y lm components must possess the same reflection parity.…”
supporting
confidence: 73%
“…The anisotropy of the dipole-limit core excitation spectra for q c and q ⊥ c for h-BN is well known from previous EELS 21 , XANES 22,23 , and XRS 24 studies at the q = 0 limit. We extend on this prior work by measuring the q-dependent boron XRS for both q c and q ⊥ c out to q = 9Å −1 , a momentum transfer that is clearly beyond the dipole limit for the B 1s initial state.…”
mentioning
confidence: 55%
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“…[5][6][7][8][9] Despite of many efforts in the past, the electronic properties of hBN remain largely unknown. They have been earlier studied by luminescence, 1,10-17 optical reflectance and absorption, [18][19][20][21] photoconductivity, 22 x-ray emission, [23][24][25] inelastic x-ray scattering, [26][27][28] x-ray absorption, 25,29,30 and electron energy loss [31][32][33] spectroscopy. After all, a large spread of band-gap energies reported in literature, ranging from 3.1 to 7.1 eV, 14 is currently explained by sample quality and related to experimental methods used.…”
Section: Introductionmentioning
confidence: 99%
“…[8][9][10][11][12] However, the influence of the core hole on the spectral shape hampers a straightforward interpretation of the spectra, as was recognized already in the early works. 2,3,9,13 The near-edge absorption fine structure ͑NEXAFS͒ at the B 1s, C 1s, and N 1s thresholds in h-BN and graphite is affected differently by the corresponding core holes, due to the different core-hole screening. Therefore, a correct theoretical description of all XA spectra in h-BN and graphite is difficult from an initial or final-state approach, as well as from a transition state model, because the degree of screening is very different and unknown a priori.…”
mentioning
confidence: 99%