Published November 1, 2012 | Version v1
Journal article

Effects of hydrostatic pressure on ionized donor bound exciton states in strained wurtzite GaN/AlxGa1-xN cylindrical quantum dots

  • 1. College of Physics and Electromechanical Engineering, Sanming University, Sanming 365004 (China)

Description

Based on the effective-mass approximation and variational procedure, ionized donor bound exciton (D+, X) states confined in strained wurtzite (WZ) GaN/AlxGa1-xN cylindrical (disk-like) quantum dots (QDs) with finite-height potential barriers are investigated, with considering the influences of the built-in electric field (BEF), the biaxial strain dependence of material parameters and the applied hydrostatic pressure. The Schrödinger equation via the proper choice of the donor bound exciton trial wave function is solved. The behaviors of the binding energy of (D+, X) and the optical transition associated with (D+, X) are examined at different pressures for different QD sizes and donor positions. In our calculations, the effective masses of electron and hole, dielectric constants, phonon frequencies, energy gaps, and piezoelectric polarizations are taken into account as functions of biaxial strain and hydrostatic pressure. Our results show that the hydrostatic pressure, the QD size and the donor position have a remarkable influence on (D+, X) states. The hydrostatic pressure generally increases the binding energy of (D+, X). However, the binding energy tends to decrease for the QDs with large height and lower Al composition (x<0.3) if the donor is located at z0≤0. The optical transition energy has a blue-shift (red-shift) if the hydrostatic pressure (QD height) increases. For the QDs with small height and low Al composition, the hydrostatic pressure dependence of the optical transition energy is more obvious. Furthermore, the relationship between the radiative decay time and hydrostatic pressure (QD height) is also investigated. It is found that the radiative decay time increases with pressure and the increment tendency is more prominent for the QDs with large height. The radiative decay time increases exponentially reaching microsecond order with increasing QD height. The physical reason has been analyzed in depth.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physb.2012.06.042

Additional details

Identifiers

DOI
10.1016/j.physb.2012.06.042;
PII
S0921-4526(12)00670-9;

Publishing Information

Journal Title
Physica. B, Condensed Matter
Journal Volume
407
Journal Issue
21
Journal Page Range
p. 4160-4167
ISSN
0921-4526
CODEN
PHYBE3

Optional Information

Copyright
Copyright (c) 2012 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.