Cristin-resultat-ID: 1362671
Sist endret: 20. juni 2016, 18:39
Resultat
Vitenskapelig foredrag
2016

Ellipsometric Study of the Optical Response of ZnS:Cr for PV Applications

Bidragsytere:
  • Thomas Brakstad
  • Benjamin Roaldssønn Hope
  • Mohammadreza Nematollahi
  • Morten Kildemo
  • Niklas J. Podraza
  • Kiran Ghimire
  • mfl.

Presentasjon

Navn på arrangementet: 7th International Conference on Spectroscopic Ellipsometry (ICSE-7)
Dato fra: 6. juni 2016
Dato til: 10. juni 2016

Om resultatet

Vitenskapelig foredrag
Publiseringsår: 2016

Beskrivelse Beskrivelse

Tittel

Ellipsometric Study of the Optical Response of ZnS:Cr for PV Applications

Sammendrag

Cr doped ZnS (ZnS:Cr) has been suggested as an intermediated band material based on density functional theory studies. We have investigated ZnS:Cr as a candidate intermediate band material. The ZnS and ZnS:Cr thin films were deposited by pulsed laser deposition and molecular beam epitaxy on Si and quartz substrates. In this work, we report an elaborate study of the optical properties of the films using spectroscopic ellipsometry (SE). SE data was mainly recorded using a dual rotating compensator spectroscopic ellipsometer (RC2), complemented by data from vacuum ultraviolet extended instrument (VUV-SE). The characteristic features of the ZnS:Cr are a direct band gap (E0) at approximately 3.7 eV, with E1 and E2 critical points around 5.7 and 7 eV. Excitonic effects are in line with the literature and observed to be strong in this material. The sub-band gap absorption appears as a broad feature that increases monotonously with increased doping at a given growth temperature. In this report we discuss three different approaches to extract and analyze the optical properties in terms of the complex dielectric function (ε = ε1 + iε2). First, the optical properties are extracted using parametric dispersion models. In order to correctly fit the highly important sub-band gap absorption features, parametric dispersion models incorporating a band gap are required. As a result, a reasonable robust approach was found to be the use of Tauc Lorentz oscillators to fit the above band features, while the below band gap features were fitted using Lorentzian or Gaussian oscillators. The problem with this approach is that the exact interpretation of the oscillator energies is not trivial. The second approach following Ghimire et al. [3], allow the use of standard oscillators assuming critical point parabolic bands (CPPB) models for the imaginary part of ε modified with a band-gap and an Urbach tail. The real part of ε is then calculated using a numerical Kramers Kronig transformation. Although the latter approach is not rigorously exact, it appears to be a better approach for physical interpretation of the data. Finally, direct inversion was also used to extract ε from the experimental data. The total sub-bandgap absorption is quantified by integration of the imaginary part of ε up to the band-gap. Critical point analysis is applied to the second derivative of numerically inverted ε. Problems in the direct inversion are discussed in terms of uniaxiality of certain columnar films.

Bidragsytere

Thomas Vågenes Brakstad

Bidragsyterens navn vises på dette resultatet som Thomas Brakstad
  • Tilknyttet:
    Forfatter
    ved Institutt for fysikk ved Norges teknisk-naturvitenskapelige universitet

Benjamin Roaldssønn Hope

  • Tilknyttet:
    Forfatter
    ved Institutt for fysikk ved Norges teknisk-naturvitenskapelige universitet

Mohammadreza Nematollahi

  • Tilknyttet:
    Forfatter
    ved Institutt for fysikk ved Norges teknisk-naturvitenskapelige universitet

Morten Kildemo

  • Tilknyttet:
    Forfatter
    ved Institutt for fysikk ved Norges teknisk-naturvitenskapelige universitet

Niklas J. Podraza

  • Tilknyttet:
    Forfatter
    ved University of Toledo
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