1998
DOI: 10.1016/s0022-0248(98)00194-8
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On the nature of the 3.41 eV luminescence in hexagonal GaN

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Cited by 83 publications
(55 citation statements)
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“…For the FX, we obtained the best fit for E͑0͒ = 3.478 eV, ␣ = 0.80 meV/ K, and ␤ = 800 K. These values are in the range of those reported for c-and a-plane GaN. 18 At low temperature, A excitons are essentially localized on donors but they escape when the temperature is increased above ϳ50 K. In agreement with previous observations in c-plane 19 and a-plane GaN, 20 the BSF energy position follows an "Sshaped" temperature dependence consisting in a small redshift from 8 to 25 K followed by a blueshift that eventually merges with some Varshni curve for temperatures above 75 K.…”
Section: Localization Effectssupporting
confidence: 89%
“…For the FX, we obtained the best fit for E͑0͒ = 3.478 eV, ␣ = 0.80 meV/ K, and ␤ = 800 K. These values are in the range of those reported for c-and a-plane GaN. 18 At low temperature, A excitons are essentially localized on donors but they escape when the temperature is increased above ϳ50 K. In agreement with previous observations in c-plane 19 and a-plane GaN, 20 the BSF energy position follows an "Sshaped" temperature dependence consisting in a small redshift from 8 to 25 K followed by a blueshift that eventually merges with some Varshni curve for temperatures above 75 K.…”
Section: Localization Effectssupporting
confidence: 89%
“…Monoexponential fits to the initial decay of the transients in figure 10 give decay times of 0.4 ns at 3.42 eV, 3.2 ns at 3.33 eV and 15 ns at 3.29 eV. For I 1 BSFs, a number of other groups have measured PL or CL transients [18,25,68,[76][77][78][79]. The reported initial decay times vary over an order of magnitude, ranging from 70 ps [77] up to 780 ps [78].…”
Section: Time-resolved Luminescence Spectroscopymentioning
confidence: 91%
“…This difference was ascribed to a variety of electron-hole overlaps present in the case of electronically coupled bundles of BSFs compared to isolated BSFs. Such a coupling between BSFs, but also a coupling to dopants in their vicinity (see next section) as well as differences in the nonradiative recombination rates depending on the employed growth technique [76] can explain the range of different decay times observed for I 1 BSFs in [25,68,[76][77][78][79].…”
Section: Time-resolved Luminescence Spectroscopymentioning
confidence: 98%
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“…This is because the 3.40 peak can be mixed with the LO phonon replica of the DX peak since the relative contribution of the latter increases with temperature. A model 25 has been proposed for this frequently reported emission 26,27,28 based on recombination of an exciton bound to an I 1 type stacking fault in GaN. In this model, the stacking fault is similar to a cubic quantum well in wurtzite GaN.…”
Section: Low Sheet Carrier Concentrationmentioning
confidence: 99%