Optical emission from SiO2-embedded silicon nanocrystals: A high-pressure Raman and photoluminescence study

J. Ibáñez, S. Hernández, J. López-Vidrier, D. Hiller, S. Gutsch, M. Zacharias, A. Segura, J. Valenta, and B. Garrido
Phys. Rev. B 92, 035432 – Published 27 July 2015

Abstract

We investigate the optical properties of high-quality Si nanocrystals (NCs)/SiO2 multilayers under high hydrostatic pressure with Raman scattering and photoluminescence (PL) measurements. The aim of our study is to shed light on the origin of the optical emission of the Si NCs/SiO2. The Si NCs were produced by chemical-vapor deposition of Si-rich oxynitride (SRON)/SiO2 multilayers with 5- and 4-nm SRON layer thicknesses on fused silica substrates and subsequent annealing at 1150 °C, which resulted in the precipitation of Si NCs with an average size of 4.1 and 3.3 nm, respectively. From the pressure dependence of the Raman spectra we extract a phonon pressure coefficient of 8.5±0.3cm1/GPa in both samples, notably higher than that of bulk Si(5.1cm1/GPa). This result is ascribed to a strong pressure amplification effect due to the larger compressibility of the SiO2 matrix. In turn, the PL spectra exhibit two markedly different contributions: a higher-energy band that redshifts with pressure, and a lower-energy band which barely depends on pressure and which can be attributed to defect-related emission. The pressure coefficients of the higher-energy contribution are (27±6) and (35±8)meV/GPa for the Si NCs with a size of 4.1 and 3.3 nm, respectively. These values are sizably higher than those of bulk Si(14meV/GPa). When the pressure amplification effect observed by Raman scattering is incorporated into the analysis of the PL spectra, it can be concluded that the pressure behavior of the high-energy PL band is consistent with that of the indirect transition of Si and, therefore, with the quantum-confined model for the emission of the Si NCs.

  • Figure
  • Figure
  • Figure
  • Figure
  • Figure
  • Received 24 March 2015
  • Revised 30 June 2015

DOI:https://doi.org/10.1103/PhysRevB.92.035432

©2015 American Physical Society

Authors & Affiliations

J. Ibáñez1,*, S. Hernández2, J. López-Vidrier2, D. Hiller3, S. Gutsch3, M. Zacharias3, A. Segura4, J. Valenta5, and B. Garrido2

  • 1Institute of Earth Sciences Jaume Almera, ICTJA-CSIC, Lluís Solé i Sabarís s/n, 08028 Barcelona, Catalonia, Spain
  • 2MIND-IN2UB, Departament d'Electrònica, Universitat de Barcelona, Martí i Franquès 1, 08028 Barcelona, Catalonia, Spain
  • 3IMTEK, Faculty of Engineering, Albert-Ludwigs-University Freiburg, Georges-Köhler-Allee 103, D-79110, Freiburg, Germany
  • 4Departamento de Física Aplicada-ICMUV-MALTA Consolider Team, Universitat de València, 46100 Burjassot, València, Spain
  • 5Faculty of Mathematics and Physics, Charles University, Ke Karlovu 3, 121 16 Prague 2, Czech Republic

  • *Corresponding author: jibanez@ictja.csic.es

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 92, Iss. 3 — 15 July 2015

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review B

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×