| Literature DB >> 28892396 |
S Assali1, J Lähnemann2, T T T Vu1, K D Jöns3, L Gagliano1, M A Verheijen1,4, N Akopian1,3, E P A M Bakkers1,3, J E M Haverkort1.
Abstract
One of the major challenges in the growth of quantum well and quantum dot heterostructures is the realization of atomically sharp interfaces. Nanowires provide a new opportunity to engineer the band structure as they facilitate the controlled switching of the crystal structure between the zinc-blende (ZB) and wurtzite (WZ) phases. Such a crystal phase switching results in the formation of crystal phase quantum wells (CPQWs) and quantum dots (CPQDs). For GaP CPQWs, the inherent electric fields due to the discontinuity of the spontaneous polarization at the WZ/ZB junctions lead to the confinement of both types of charge carriers at the opposite interfaces of the WZ/ZB/WZ structure. This confinement leads to a novel type of transition across a ZB flat plate barrier. Here, we show digital tuning of the visible emission of WZ/ZB/WZ CPQWs in a GaP nanowire by changing the thickness of the ZB barrier. The energy spacing between the sharp emission lines is uniform and is defined by the addition of single ZB monolayers. The controlled growth of identical quantum wells with atomically flat interfaces at predefined positions featuring digitally tunable discrete emission energies may provide a new route to further advance entangled photons in solid state quantum systems.Entities:
Keywords: Semiconductor nanowire; crystal phase quantum well; gallium phosphide; photoluminescence; spontaneous polarization
Year: 2017 PMID: 28892396 PMCID: PMC5642001 DOI: 10.1021/acs.nanolett.7b02489
Source DB: PubMed Journal: Nano Lett ISSN: 1530-6984 Impact factor: 11.189
Figure 1(a) Plot of the spontaneous polarization fields in III–V semiconductors. The dark blue areas are the values predicted from DFT, while the dark red areas are the values determined from experimental measurements. (b) Calculated band diagram for a CPQW in GaP with 5 ZB MLs using 1D Schrödinger–Poisson simulations. The dashed lines indicate the normalized wave functions for electrons (dark blue) and holes (dark red). Curves are shifted to allow easier comparison. (c) Enlarged view of panel b showing a capacitor-like charge configuration where the sheet of polarization charges and the related QCSE are sketched. (d) Digital tuning of the CPQW transition energy for increasing ZB thicknesses of 5, 6, and 7 MLs. By adding (removing) one monolayer, the resulting transition will be decreased (increased) by an amount of Δ.
Figure 2(a) TEM image of a WZ GaP nanowire with 100 nm diameter and multiple CPQWs of different ZB lengths separated by 200 nm long WZ segments. (b,c) HRTEM images of CPQWs with ZB segments of 12 MLs (b) and 33 MLs (c) in length.
Figure 3(a) PL spectra acquired for different CPQWs and compared with the emission from WZ GaP. (b) Enlarged view of a CPQW peak with a fwhm of ∼320 μeV. Inset: polarization-dependent PL measurement on a single NW with CPQWs. (c) Statistical analysis of the emission energy of hundreds of nanowires with CPQWs. Fifteen Gaussian peaks are used for fitting, with additional peaks at 2.170 and 2.244 eV, with low statistical count being visible. A bin size of 0.5 meV is used for the histogram. Inset: width σG of the different Gaussian histogram peaks as a function of the ZB thickness. (d) Emission energy as a function of the number of ZB MLs (red spheres). The low statistical count peaks at 2.170 and 2.244 eV are indicated with hollow grey spheres. The 1D Poisson simulations using the WZ band gap of 2.19 eV (dashed dark green line) and γ-line bound exciton level at 2.25 eV (blue dashed line) are shown.
Figure 4(a) PL spectra from two different QWs with a difference in thickness of 1 ZB ML. (b) Integrated PL intensity as a function of the excitation power density for the peaks in panel a. Inset: peak energy as a function of the excitation power density. (c) Time-resolved PL measurements on a CPQW peak at 2.221 eV compared with the time decay for the γ-exciton line. (d) Integrated PL intensity as a function of the reciprocal temperature for a CPQW at 2.220 eV. The fit is performed considering one active nonradiative recombination channel. Inset: PL spectra for increasing temperature.