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CONFINAMIENTO NANOSC´OPICO EN ESTRUCTURAS ... - It works!

CONFINAMIENTO NANOSC´OPICO EN ESTRUCTURAS ... - It works!

CONFINAMIENTO NANOSC´OPICO EN ESTRUCTURAS ... - It works!

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236 Publicaciones(a)(b)ρ (r)ρ (r)ρ v = 0.35 ρ v = 0.59(c)ρ ρ v = 0.90v = 0.93(d)20 30 40 50r (nm)20 30 40 50r (nm)Figure 5: Electron radial density distribution of the exciton ground state in hollow silica nanospheres withdimensions defined by an internal radius R in =20 nm and shell thicknesses (a) d = 4 nm; (b) d = 10 nm; (c) d =20 nm; and (d) d = 28 nm. The meaning of vertical dotted lines and ρ v is the same as in Fig. 3.border profile, R in (d), has an exponential-like decay, the corresponding profile for the electron distributionof the ground state exciton shows a shallow minimum at about d =14 nm. The phase diagramborder profile is now determined by two factors. On the one hand, we have the same single-electronfactors yielding an exponential-like decay profile. As pointed out in the previous subsection and canbe seen in Fig. 4, once a shell thickness of about d = 10 nm is reached, a further increase in d doesnot change the surface trapping radius R in (d). At this point, the many-body electron-hole attractionbecomes relevant. Since the hole distribution is necessarily volumetric, the shorter the shell thickness is,the closer the electron and hole distributions are and the stronger the electron-hole attraction becomes.This many-body effect thus produces an increase in R in (d) vs. d. In other words, the trend of the phasediagram border R in (d) profile is determined by single-particle/many-body effects at short/large d values.As a result, a shallow minimum appears in such a profile at about d = 14 nm. In Fig. 5 we include theelectron density distribution of a set of nanoshells with R in = 20nm and shell thicknesses d =4, 10, 20and 28 nm, in order to compare them to their partners in Fig. 3, which correspond to a single electronin the same nanoshells. As a whole, our results reveal that the presence of a (volume-distributed) holehas little influence on the surface electron state density distribution. This evidences, in turn, that the

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