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Copyright 2004 by Marcel Dekker, Inc. All Rights Reserved.

Copyright 2004 by Marcel Dekker, Inc. All Rights Reserved.

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To explain these results, the following model for the UCPL that invokessurface states was proposed [51]. The model is based on Fu and Zunger’s [50]calculated energy level structure of InP QDs as a function of QD size,including surface states produced <strong>by</strong> In and P dangling bonds; their resultsare reproduced in Fig. 12a. At QDs sizes above 57 A˚ , the In dangling bond(In-DB) energy level is coincident with the QD conduction-band minimum(CBM); however, below 57 A˚ , the energy separation between the CBM andthe In-DB increases with decreasing size as the conduction-band energymoves up and the In-DP energy remains nearly constant. On the other hand,as seen in Fig. 12a, the P-DB energy level is always above the valence-bandmaximum (VBM) at all QD sizes (0.3 eV for bulk InP), and this separationincreases as the VBM moves down with decreasing QD size.<strong>All</strong> of the UCPL results can be explained within the context of theenergy levels calculated <strong>by</strong> Fu and Zunger [50] and the model is shown in Fig.12b. For upconversion of photon energies above the red-shifted trap emissionenergies, the first step in the process is photoexcitation from the P-DB state tothe conduction band; if the QD size is significantly less than 57 A˚ , the electronin the conduction band then relaxes to the In-DB state, which lies below theconduction band. The second step is excitation of the photogenerated hole inthe P-DB state to the valence band, followed <strong>by</strong> radiative recombination ofthe electrons and holes across the bandgap. For upconversion of the trapemission, the first step is photoexcitation from the P-DB state to the In-DBstate, followed <strong>by</strong> excitation of the P-DB hole to the valence band andradiative recombination from the In-DB state to the VBM.This model also predicts that as the QD size gets smaller, the UCPLdecreases and goes to zero at the QD size (15 A˚ ) where the quantity (P-DBVBM) equals the quantity (CBM In-DB) (i.e., the relaxation energy ofelectrons from the conduction band to the In-DB cancels out the upconversionenergy of the holes from the P-DB to the VBM). The experimental resultsin Ref. 51 are consistent with this prediction. As seen in Fig. 12a, the differencebetween the theoretically calculated P-DB energy and the CBM In-DBenergy as a function of QD size follows the equivalent experimental value ofthe UCPL shift (DE UC ) added to the VBM energy; also, DE UC goes to zero at15 A˚ , as predicted. However, although the experimental results fit the In-DBand P-DB model of Fu and Zunger [50] very well, there is presently noindependent experimental identification of the actual chemical nature of thesurface states in the InP QD samples.In the UCPL model, the energy of upconversion is produced <strong>by</strong>excitation of the In-DP hole to the valence band; this process could be driveneither <strong>by</strong> phonon absorption or <strong>by</strong> absorption of a second photon. The formerprocess is favored for several reasons. (1) The upconversion shows a strongdecrease in intensity with decreasing temperature (while the normal Stokes PLintensity increased with decreasing temperature); a sequential two-photon<strong>Copyright</strong> <strong>2004</strong> <strong>by</strong> <strong>Marcel</strong> <strong>Dekker</strong>, <strong>Inc</strong>. <strong>All</strong> <strong>Rights</strong> <strong>Reserved</strong>.

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