TY - JOUR
T1 - Temperature dependence of optical centres in ultrapure diamond after 200 keV electron irradiation
AU - Wang, Kaiyue
AU - Guo, Ruiang
AU - Ding, Senchuan
AU - Wang, Hongxing
AU - Tian, Yuming
AU - Wang, Yingmin
N1 - Publisher Copyright:
© 2020 IOP Publishing Ltd.
PY - 2020/1/21
Y1 - 2020/1/21
N2 - In this work, we conduct a temperature-dependent study of optical centres in ultrapure diamond after 200 keV irradiation by photoluminescence spectra, which are performed in a temperature range of 80-200 K. The zero phonon lines (ZPLs) include sizes of 550.3 nm, 593 nm, and 741 nm (GR1 centre). With an increase in measurement temperature, the ZPLs shift to the lower energy side, together with intensity quenching and an increase in the full width at half maximum. These results are noted in models of lattice contraction and electron-phonon coupling, and their inhomogeneous and homogeneous broadening mechanisms are also carefully distinguished by the Voigt function. The 550.3 nm and 593 nm emissions present harder bonds than the GR1 centre, close thermal quenching energies to the interstitial-related defect, a lower thermal softness than that of the ideal diamond, weak phonon bands at each lower energy side, and different broadening mechanisms with the GR1 centre, indicating that the 550.3 nm and 593 nm lines are possibly interstitial-related.
AB - In this work, we conduct a temperature-dependent study of optical centres in ultrapure diamond after 200 keV irradiation by photoluminescence spectra, which are performed in a temperature range of 80-200 K. The zero phonon lines (ZPLs) include sizes of 550.3 nm, 593 nm, and 741 nm (GR1 centre). With an increase in measurement temperature, the ZPLs shift to the lower energy side, together with intensity quenching and an increase in the full width at half maximum. These results are noted in models of lattice contraction and electron-phonon coupling, and their inhomogeneous and homogeneous broadening mechanisms are also carefully distinguished by the Voigt function. The 550.3 nm and 593 nm emissions present harder bonds than the GR1 centre, close thermal quenching energies to the interstitial-related defect, a lower thermal softness than that of the ideal diamond, weak phonon bands at each lower energy side, and different broadening mechanisms with the GR1 centre, indicating that the 550.3 nm and 593 nm lines are possibly interstitial-related.
KW - Diamond
KW - Photoluminescence
KW - Temperature dependence
KW - Zero phonon line
UR - https://www.scopus.com/pages/publications/85079538262
U2 - 10.1088/1361-6463/ab66d9
DO - 10.1088/1361-6463/ab66d9
M3 - 文章
AN - SCOPUS:85079538262
SN - 0022-3727
VL - 53
JO - Journal of Physics D: Applied Physics
JF - Journal of Physics D: Applied Physics
IS - 13
M1 - 135303
ER -