1980
DOI: 10.1103/physrevb.22.4900
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Low-temperature fluorescence in sapphire

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Cited by 63 publications
(39 citation statements)
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“…The absence of polarization or a weak polarization of the optical absorption (OA) of the F-center at 6.05 eV [2,3] and a considerable anisotropy [1,2] of its luminescence at 3 eV confirms the supposition [2], which is based on a long-time decay of the luminescence, about the triplet-singlet origin of the radiative transition. Some experimental facts, which are related to the luminescence near 3 eV, have not been explained so far.…”
Section: Introductionmentioning
confidence: 69%
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“…The absence of polarization or a weak polarization of the optical absorption (OA) of the F-center at 6.05 eV [2,3] and a considerable anisotropy [1,2] of its luminescence at 3 eV confirms the supposition [2], which is based on a long-time decay of the luminescence, about the triplet-singlet origin of the radiative transition. Some experimental facts, which are related to the luminescence near 3 eV, have not been explained so far.…”
Section: Introductionmentioning
confidence: 69%
“…The position of the maximum at 5.7 eV depends on the temperature and at T = 80 K it is displaced to 5.8-5.9 eV. (2), and luminescence excitation (3) at E em = 3 eV; b -time-resolved spectra (1, 2 − δt 1 = 1.2 ns, ∆t 1 = 5.9 ns; 3 − δt 2 = 23 ns, ∆t 2 = 111 ns) of luminescence excitation with E em = 3 eV at E ⊥C 3 (1,3) or E || C 3 (2,3) Figure 1b presents time-resolved excitation spectra at T = 295 K for two orientations of the sample relative to the SR electric field vector E (E⊥C 3 and E||C 3 ). The fast component (curve 1) at E⊥C 3 replicates the stationary excitation spectrum and includes bands with E ex1 = 5.7 eV, E ex2 = 6 eV and E ex3 = 6.3 eV.…”
Section: Resultsmentioning
confidence: 99%
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“…Vinceller et al [46] because the F band is known to show photocurrents down to 10 K [2,47]. The emission at 3.0 eV (420 nm) is generated by the transition from the 3 P excited state to the 1 S ground state [2,4,48].…”
Section: Interpretation Of Spectral Features: General Observationsmentioning
confidence: 99%