Effects of hydrostatic pressure on ionized donor bound exciton states in strained wurtzite GaN/AlxGa1-xN cylindrical quantum dots
Creators
- 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.2012.06.042Additional 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
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44041530
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S77: NANOSCIENCE AND NANOTECHNOLOGY;
- Descriptors DEI
- BINDING ENERGY; DEUTERIUM IONS; EFFECTIVE MASS; ENERGY GAP; GALLIUM NITRIDES; PERMITTIVITY; PIEZOELECTRICITY; POLARIZATION; PRESSURE DEPENDENCE; QUANTUM DOTS; RADIATIVE DECAY; RED SHIFT; SCHROEDINGER EQUATION; STRAINS; WAVE FUNCTIONS
- Descriptors DEC
- CHARGED PARTICLES; DECAY; DIELECTRIC PROPERTIES; DIFFERENTIAL EQUATIONS; ELECTRICAL PROPERTIES; ELECTRICITY; ENERGY; EQUATIONS; FUNCTIONS; GALLIUM COMPOUNDS; IONS; MASS; NANOSTRUCTURES; NITRIDES; NITROGEN COMPOUNDS; PARTIAL DIFFERENTIAL EQUATIONS; PARTICLE DECAY; PHYSICAL PROPERTIES; PNICTIDES; WAVE EQUATIONS
Optional Information
- Copyright
- Copyright (c) 2012 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.