Study of the effect of changing the microstructure of titania layers on composite solar cell performance

Xie Z, Henry BM, Kirov KR, Smith HE, Barkhouse A, Grovenor CRM, Assender HE, Briggs GAD, Webster GR, Burn PL, Kano M, Tsukahara Y

This paper reports a study of the microstructures of titania thin films fabricated by two methods; doctor blade casting and glancing angle deposition (GLAD). The microstructures were characterised by a broad range of techniques, including SEM, HRTEM, and XRD. Porous films with a three-dimensional network of interconnected TiO2 particles were obtained using the doctor blade technique. GLAD was used to fabricate well-defined columnar structures. The power efficiency of composite solar cells (CSCs) based on doctor-bladed titanium dioxide and a spin coat MEH-PPV layer is reproducibly greater than 0.5% at 800 W/m(2), using a solar simulator and 420 rim UV blocking filter, with typical values J(sc) = 14.3 A/m(2), V-oc=0.79 V and FF=36%. This performance is significantly better than that reported for similar devices by other groups [1,2]. Under the same illumination conditions, preliminary results for CSCs based on GLAD titanium dioxide gave at best efficiencies of only 0.08%, with J(sc)=2.4 A/m(2), V-oc=0.61 V and FF=43%. We discuss how the morphology, crystal structure and optical absorption properties of the two types of TiO2 affect the overall device performance. (c) 2005 Elsevier B.V. All rights reserved.

Keywords:

THIN-FILMS

,

TIME

,

TiO2

,

solar cells

,

TIO2 FILMS

,

glancing angle deposition